5930 lines
169 KiB
Plaintext
5930 lines
169 KiB
Plaintext
UC-NRLF
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REESE LIBRARY
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UNIVERSITY OF CALIFORNIA.
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Co
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^Accession No .
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o o 5 9 . Class No .
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SCIENTIFIC MEMOIRS
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EDITED BY
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J. S. AMES, PH.D.
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PROFESSOR OF PHYSICS IN JOHNS HOPKINS UNIVERSITY
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X.
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THE WAVE-THEORY OF LIGHT
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THE
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WAVE THEORY OF LIGHT
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MEMOIRS BY HUYGENS, YOUNG AND FRESNEL
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EDITED BY
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HENRY CREW, Pn.D. \N
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PROFKSSOR OK PHYSICS, NORTHWESTERN UNIVERSITY
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NEW YORK : CINCINNATI .: CHICAGO
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AMERICAN BOOK COMPANY
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to *i<&
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COPYRIGHT, 1900, HY
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AMERICAN BOOK COMPANY
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Crew, Light.
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W. P. I
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PKEFACE
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THANKS to the labors of Kirchhoff, Kelvin, Huxley, and
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others, there is now a widespread opinion that any physical
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phenomenon
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" is explained" only
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when some
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one
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has
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devised a
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dynamical model which will duplicate the phenomenon. The
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completeness of the explanation is to be measured by the com-
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pleteness with which the model will duplicate the phenomenon.
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Thus, for instance, a refraction model which, like that of
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Airy, describes only the path of the refracted ray when the
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incident ray is given, does not in any true sense explain how
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the refracted ray comes to take one path rather than another.
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Such a model illustrates Suell's law, but does not explain the
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phenomenon.
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If, however, we take a large and shallow tank of water, the
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floor of the tank being partly covered with a false bottom, so
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as to give two, and only two, different depths of water, we shall
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find that the speed of the waves in the deeper portion of the
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tank bears to the speed in the shallower portion a constant
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ratio ;
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hence,
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in
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passing
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from
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one
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depth
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to
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the
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other,
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these
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waves are refracted according to the sine law.
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Such a model may be said to be a " partial explanation" of
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refraction in so far as it refers the phenomenon to change of
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speed which accompanies change of medium. It represents,
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however, only the kinematics of refraction.
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If, now, we could go one step further, and make a model in
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which the wave -producing forces were duplicated in other
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words, if we could make a model of the medium and of the
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disturbing forces we should have a fairly complete "expla-
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nation" of refraction ; in fact, the dynamics of refraction would
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be understood. This would imply not only that we knew the
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substance disturbed, but also that we were acquainted with
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the laws according to which it is disturbed.
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83059
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PREFACE
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A theory of light may be considered either from a kinemat-
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ical or from a dynamical point of view. To assume, on exper-
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imental grounds, that a ray of light has a certain speed in one
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medium and a different speed in a different medium, and that it consists in a particular kind of motion, and thence to infer
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the laws of refraction, rectilinear propagation, and diffraction, is to construct a kinematical theory of light. But to assume a certain structure for the luminous body and for the medium, and thence to derive the motions and the different speeds assumed in the kinematical case, is to offer a dynamical ex-
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planation of light.
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The wave-theory of light is used, nearly always, in the former and narrower sense to mean the kinematical explanation of
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light; it leaves entirely to one side the dynamical questions hinted at above. It assumes, not without strong experimental evidence, the existence of waves travelling with different speeds in different media, and proposes to explain the cardinal phe-
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nomena of optics. To illustrate its limitations, we may cite the instance of the
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ordinary and extraordinary ray in crystals. How it happens
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that there are two rays is a problem in the dynamics of light ; but, assuming these two rays, their subsequent behavior, their inability to interfere, etc., must be accounted for in a general way, at least by the kinematical theory of light.
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It is in this narrow sense that the wave-theory of light is employed in the memoirs translated in this volume.
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The first clear and unmistakable suggestion that light consists in a vibratory motion appears to be due to that brilliant but unfortunate genius, Robert Hooke (1635-1703), who, in
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his Micrograpliia (London, 1665), describes the three characteristic features of the motion which he believes to constitute
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light.
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Since it has not been deemed advisable to reprint Hooke's paper in this volume, it may not be out of place here to quote what few paragraphs are necessary fairly to present his point of view. This will, perhaps, be accomplished by the follow-
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ing selections :
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' ' It would be somewhat too long a work for this place Zetetically to examine, and positively to prove, what particular kind of motion it is that must be the efficient of Light; for though it be a motion, yet 'tis not every motion that produces
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vi
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PREFACE
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it, since we find there are many bodies very violently mov'd,
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which
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yet
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afford
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not
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such
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an
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effect ;
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and
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there
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are
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other
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bodies,
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which to our senses, seem not mov'd so much, which yet shine.
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Thus Water and quick-silver, and most other liquors heated, shine not; and several hard bodies, as Iron, Silver, Brass, Cop-
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per, Wood, &c., though very often struck with a hammer, shine not presently, though they will all of them grow exceeding
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hot; whereas rotten Wood, rotten Fish, Sea Water, Gloworms, &G. have nothing of tangible heat in them, and yet (where
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there is no stronger light to affect the Sensory) they shine some of them so Vividly, that one may make a shift to read by them.
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"It would be too long, I say, here to insert the discursive
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progress by which I inquir'd after the proprieties of the motion of Light, and therefore I shall only add the result.
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"And, First, I found it ought to be exceeding quick, such as those motions of fermentation and putrefaction, whereby, certainly, the parts are exceeding nimbly and violently mov'd; and that, because we find those motions are able more mi-
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nutely to shatter and divide the body, then the most violent heats or menstruums we yet know. And that fire is nothing else but such a dissolution of the Burning body, made by the most universal menstruum of all sulphureous bodies, namely, the Air, we shall in an other place of this Tractate endeavour
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to make probable. And that, in all extremely hot shining
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bodies, there is a very quick motion that causes Light, as well
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as a more robust that causes Heat, may be argued from the
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celerity wherewith the bodyes are dissolv'd.
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"Next, it must be a Vibrative motion. And for this the
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newly mentioned Diamond affords us a good argument; since
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if the motion of the parts did not return, the Diamond must
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after many rubbings
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decay and be
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wasted ;
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but we
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have
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no
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reason to suspect the latter, especially if we consider the ex-
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ceeding difficulty that is found in cutting or wearing away a
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Diamond. And a Circular motion of the parts is much more
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improbable, since, if that were granted, and they be suppos'd irregular and Angular parts, I see not how the parts of the Diamond should hold so firmly together, or remain in the same
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sensible dimensions, which yet they do. Next, if they be Glob-
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ular, and mov'd only with a turbinated motion, I know not any
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cause that can impress that motion upon the pellucid medium,
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which yet is done. Thirdly, any other irregular motion of the
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vii
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PREFACE
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parts one amongst another, must necessarily make the body of a fluid consistence, from which- it is far enough. It must
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therefore be a Vibrating motion.
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" And Thirdly, That is a very short vibrating motion, I think the instances drawn from the shining of Diamonds will also make probable. For a Diamond being the hardest body we yet know in the World, and consequently the least apt to yield or
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bend, must consequently also have its vibrations exceeding
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short.
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"And these, I think, are the three principal proprieties of
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a motion, requisite to produce the effect call'd Light in the
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Object." [Micrographia, pp. 54-56.]
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The total absence of experimental evidence from the above statement of the case stands in such marked contrast with the
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method of modern physics as initiated by Galileo, that we cannot for a moment reckon Hooke among the founders of the
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wave-theory. So important, on the contrary, have been the contributions
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of Huygens, Newton, Young, and Fresnel, that each has in turn been considered the founder of the modern science of
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optics. What justification there is for each of these views will
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be clearer from a brief consideration of optical theory before and after it had been modified by the work of each of these four men.
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Two questions naturally arise in the consideration of any theory, viz., (1) What phenomena does it explain? and (2) How does it explain them ? The answers which have been
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given to these two questions at various periods in the develop-
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ment of the wave-theory may be outlined as follows: At the time when Huygens and Newton began their work
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on light, the following phenomena were demanding explana-
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tion :
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1. The existence of rays and shadows, known from the ear-
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liest times.
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2. The phenomenon of reflection, known from the earliest
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times.
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3. The phenomenon of refraction, as described by Snell's law. 4. The rainbow and the production of color by the prism. 5. The colors of thin plates Newton's rings.
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6. Diffraction bands outside the geometrical shadow, de-
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scribed by Grimaldi, 1665.
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PREFACE
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To these might be added the two following phenomena which
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were discovered before the final publication of Newton's Opticks (1704) or Huygens's Traite dela Lumiere (1690).
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7. The polarization of light by crystals (Bartholinus, 1670). 8. The finite speed of light (Romer, 1675). Of these eight cardinal facts, the second, the third, and the eighth,, were explained by Huygens on the assumption (a) That a luminous disturbance consists of a wave-motion
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in the ether.
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(b) That this wave-disturbance travels with a uniform finite
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speed through the ether in any homogeneous medium.
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(c) That in different media it travels with speeds which are
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related inversely as the refractive indices of those media.
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But the wave-disturbance as pictured by Huygens was a
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single longitudinal pulse, or blow, imparted to an elastic fluid.
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Since he did not have in mind either a train of waves or trans-
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verse
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waves, or
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the
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idea
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of
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"
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phase,"
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or
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waves
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of
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different
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lengths, it is evident that he was unable to explain any of the
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remaining five facts.
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Turning now to that portion of the work of Newton which contributed to the wave-theory, we find that the fourth phenomenon prismatic colors was explained by him in 1666, when
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he demonstrated that a single ray of white light contains all the colors of the spectrum, and that color is not produced at the surface of the prism, as had been hitherto supposed. This
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discovery made possible, for the first time, the correct explana-
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tion of the rainbow.
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In Newton's ingenious, though, as we now know, incorrect explanation of the fifth phenomenon colors of thin plates we meet the earliest measurement of the wave-length of light,
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viz., the distance traversed by a ray of light during the inter-
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val between two successive "fits" of the same kind. We meet
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here, also, the first evidence that, in these fits, or, as we now say, waves, there is a regular periodicity. From this point on we must consider light as travelling not only in waves, but in
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trains of waves.
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At the close of the period of Huygens and Newton, we have then the following facts still demanding explanation :
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1. The existence of rays and shadows. 5. The colors of thin plates. .6. The existence of diffraction fringes.
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PREFACE
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7. The polarization of light by crystals. To these must now be added
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9. The phenomenon of stellar aberration, discovered by Brad-
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ley in 1727.
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Considering next the work of Young, we find that he first
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suggested the correct explanation for the colors of thin plates,
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having shown by experiment that two rays of light can interfere to produce alternately bright and dark bands. From this experiment and the dark centre in Newton's rings, he concludes that light consists of series of waves which, like other wave - motions, change phase by 180 on reflection from a denser medium.
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Young, at this period (1802-3), was still laboring under the
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impression that light-waves were longitudinal and were propa-
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gated in a fluid
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medium ;
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fortunately, neither of these assump-
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tions affects the validity of his reasoning concerning the colors
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of thin plates.
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When Fresnel began his optical studies (1814) the following
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facts, viz., (1) existence of rays, (6) diffraction fringes, (7)
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polarization, and (9) aberration, were still to be accounted for
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on the wave-theory. By the union of Huygens's principle with
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the principle of interference, Fresnel gave the first satisfac-
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tory explanation of the rectilinear propagation of light, and
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of the existence of diffraction fringes outside the geometrical
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shadow.
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FresneFs tematically
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memoir, in which these set forth, and which was
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discoveries
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" crowned"
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are most sysby the French
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Academy in 1819, is translated in the following pages. For
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the purpose of offering an elementary geometrical explanation
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of rays and diffraction bands, Fresnel invented the idea of
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dividing the wave-front into a certain series of zones, which in
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nearly
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all
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text - books
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are
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wrongly
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referred
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to
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as
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" Huygens's
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Zones." That this is not only unfair, but also misleading, has
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been pointed out by Professor Schuster. Phil. Mag. vol. xxxi.,
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p. 77 (1891). The first mention of these Fresnel Zones, as
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they should be called, will be found on p. Ill of the present
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volume.
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It was in order to explain the phenomenon of polarization
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that Fresnel introduced the idea of transverse vibrations in the
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ether. The boldness of this now universally accepted hypothesis, which was then practically equivalent to supposing the
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PREFACE
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ether an elastic solid, can be fully appreciated only after one has carefully studied the views of Fresnel's contemporaries.
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The evidence for the transversality of light vibrations rests .pon the inability of two oppositely polarized rays to interfere. The memoir of Arago and Fresnel upon this subject is trans-
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lated in the present volume.
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Of the nine phenomena which we have more or less arbi-
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trarily selected as the principal facts of optics, all, save only the last aberration had received a fairly complete explana-
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tion at the close of the labors of Young and Fresnel. This
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discovery of Bradley's, which he so easily disposed of on the
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corpuscular theory, has received many explanations in terms of the wave -theory; but none of these can be considered as thoroughly satisfactory. Young imagines the ether to pass through ordinary matter "as freely, perhaps, as the wind passes through a grove of trees." On this view, however, it is difficult to see how the speed of light in glass, say, should differ from its speed in a vacuum, or how the aberration constant can remain unchanged when the tube of the telescope
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is filled with water, as in Airy's experiment. Proc. Roy. Soc., vol. xx., p. 35 (1872).
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For it will be remembered that the aberration constant is
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vl V radians, where
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#=speed of earth in its orbit, and F^speed of light between the objective and eye-piece of
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telescope employed. Fresnel, accordingly, modified Young's hypothesis by assuming that, in their motion through space, refracting bodies carry
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with them only so much ether as is required to increase the
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density of free ether from unity to p, where p at any point in
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the medium is defined by the following equation:
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H being the refractive index at the same point in the body. This is really equivalent to saying that et the luminiferous
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ether is entirely unaffected by the motion of the matter which
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it permeates." [Amer. Jour. Sci., vol. cxxxi., p. 386.] And
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that this is the fact of nature is exactly the conclusion at which Fizeau and Michelson and Morley arrive from their experi-
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ments upon the effect of motion of the medium upon the speed
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of light. LOG dt., p. 377.
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xi
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PREFACE
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When, however, Michelsou and Morley attempt to detect this relative motion of the earth and the ether as the earth
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proceeds in its orbital motion, they do not succeed in certainly finding that there is any [Phil. Mag., December, 1887]; and they accordingly conclude that this relative motion is "quite small enough to refute FresnePs explanation of aberration."
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Of the two experimental facts just cited, one apparently confirms FresnePs view, and makes possible an explanation of aberration in terms of the wave-theory; while the other leads us to think that the ether moves with the refracting medium, in which case the wave-theory appears incompetent to explain
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stellar aberration.
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It was in the year 1850 that Fizeau and Foucault measured directly the speed of light in air and in water, and found the ratio of these speeds numerically equal to the ratio of their refractive indices. This experiment has sometimes been called the experimentum crucis of the wave-theory; but with scant justice we venture to think, inasmuch as no great doctrine in physics can be said to rest upon any single fact, though mod-
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ification may be demanded by a single fact.
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We have now followed, in merest outline, the general ex-
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planations which Huygens, Newton, Young, and Fresnel have offered for all, save one, of this group of nine cardinal facts. It is needless to remind the reader that this enumeration forms
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but a small fraction of the phenomena which optical science has brought to light within the last two centuries, or, indeed, since the labors of these four men were ended.
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No outline of the wave-theory would be complete without
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mention of the important addition which was made to it in .the year 1849 by Sir George Stokes. For he it was who first completely justified Huygens's principle by showing that if the primary wave be resolved as proposed by Huygens, no "back wave" will be produced provided we adopt the proper law of disturbance for the secondary wave. The discovery of this law was announced in his memoir on the Dynamical Theory of Diffraction. [Trans. Oamb. Phil. Soc.,vo\. ix., p. 1; Math.
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andPhys. Papers, vol. ii., p. 243.] Mathematically speaking, this contribution amounts to the introduction of the factor
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1 -f- cos into the equation [Eq. 46, loc. cU.~\, which describes the disturbance in a secondary wave proceeding from an element of the primary wave.
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xii
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PRE F AC K
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While, as has been said above, the following memoirs concern themselves only with the kinematics of light-waves and not at all with the question of what is vibrating, it may not
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be out of place to indicate that principally during the last half of the present century at least four more cardinal facts have
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presented themselves and demanded explanation. 10. The speed of light in free space is numerically equal
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to the ratio of the electrostatic and electromagnetic units of
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quantity. 11. In refracting media, the speed of light varies inversely
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as the square root of the product of the electric and magnetic
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inductivities.
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12-. " Most transparent solid bodies are good insulators, and
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all good conductors are very opaque." MAXWELL, Treatise, vol.
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ii.,art. 799.
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13. The plane of polarization is rotated in a magnetic field.
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(Faraday.) It was to
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"
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explain"
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these
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additional
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phenomena
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that
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Max-
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well proposed, in 1865, to modify the wave-theory of light by
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replacing the mechanical shear of the ether by an electric dis-
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placement. How thoroughly justified Maxwell was in this
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move has been amply proved mathematically by the analogy
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of his equations with those of the elastic solid theory, and
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experimentally by Hertz (1888).
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Within the last decade the wave -theory has shown itself
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capable of explaining an entirely new group of phenomena,
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viz., the color photography discovered by Lippmann. Wiener
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has shown that we have here merely two rays of light the
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direct and reflected travelling in opposite directions and inter-
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fering to produce stationary light waves.
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The flexibility of the wave - theory has still more recently
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been exemplified by the beautiful discovery of Zeeman; and
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Larmor and Preston have shown that by assuming a particular
|
|
|
|
kind of electrical displacement, viz., an orbital motion of an
|
|
|
|
ion, the wave-theory is competent to predict not only the trip-
|
|
|
|
lets and even the sextet, but also the polarization produced by
|
|
|
|
placing the source of radiation in a magnetic field. Phil Mag.,
|
|
|
|
February, 1899.
|
|
|
|
Striking as the resemblance appears between the kinematics
|
|
|
|
of wave-motion considered in this volume and the phenomena
|
|
|
|
of optics, it must never be forgotten that in all probability the
|
|
|
|
PREFACE
|
|
vibrating atom is a structure whose motion is vastly complicated as compared with the few simple motions which the' experiments of Huygens, Newton, Young, Fresnel, Maxwell, and Michelson have assigned to it.
|
|
H. 0. EVANSTON, 111., November, 1899.
|
|
xiv
|
|
|
|
GENEBAL CONTENTS
|
|
|
|
PAGE
|
|
|
|
Preface
|
|
|
|
v
|
|
|
|
Treatise on Light. By Christiaan Huygens. (First three chapters).. . 1
|
|
|
|
Biographical Sketch of Huygens
|
|
|
|
42
|
|
|
|
On the Theory of Light and Colors. By Dr. Thomas Young
|
|
|
|
45
|
|
|
|
An Account of Some Cases of the Production of Colors not Hitherto
|
|
|
|
Described. By Dr. Thomas Young
|
|
|
|
62
|
|
|
|
Experiments and Calculations relative to Physical Optics. By Dr.
|
|
|
|
Thomas Young
|
|
|
|
68
|
|
|
|
Biographical Sketch of Young
|
|
|
|
77
|
|
|
|
Memoir on the Diffraction of Light, crowned by the [French] Acad-
|
|
|
|
emy of Sciences. By A. J. Fresnel
|
|
|
|
79
|
|
|
|
On the Action of Rays of Polarized Light upon Each Other. By
|
|
|
|
Arago and Fresnel
|
|
|
|
145
|
|
|
|
Biographical Sketch of Fresnel
|
|
|
|
156
|
|
|
|
Bibliography
|
|
|
|
161
|
|
|
|
Index
|
|
|
|
165
|
|
|
|
xv
|
|
|
|
TBEATISE ON LIGHT
|
|
CONTAINING
|
|
THE EXPLANATION OF REFLECTION AND OF REFRACTION AND ESPECIALLY OF THE REMARKABLE REFRACTION WHICH
|
|
OCCURS IN ICELAND SPAR
|
|
BY
|
|
CHRISTIAAN HUYGENS
|
|
(Leyden, 1690)
|
|
|
|
CONTENTS
|
|
|
|
rAGE
|
|
|
|
Preface
|
|
|
|
3
|
|
|
|
Table of Contents
|
|
|
|
7
|
|
|
|
The Rectilinear Propagation of Rays and some General Considerations
|
|
|
|
concerning the Nature of Light
|
|
|
|
9
|
|
|
|
Explanation of the Laws of Reflection
|
|
|
|
25
|
|
|
|
Explanation of the Laws of Refraction
|
|
|
|
30
|
|
|
|
TREATISE ON LIGHT
|
|
BY
|
|
CHRISTIAAN HUYGENS
|
|
|
|
PKEFACE
|
|
|
|
THIS treatise was written during my stay in Paris twelve
|
|
years ago, and in the year 1678 was presented to the Eoyal Academy of Sciences, to which the king had. been pleased to call me. Several of this body who are still living, especially those who have devoted themselves to the study of mathematics, will remember having been at the meeting at which I present-
|
|
ed the paper; of these I recall only those distinguished gentle-
|
|
men Messrs. Cassini, Homer, and De la Hire. Although since
|
|
then I have corrected and changed several passages, the copies which I had made at that time will show that I have added noth-
|
|
|
|
ing except some conjectures concerning the structure of Iceland spar and an additional remark concerning refraction in rockcrystal. I mention these details to show how long I have been
|
|
thinking about these matters which I am only just now publish-
|
|
ing, and not at all to detract from the merit of those who, with-
|
|
out having seen what I have written, may have investigated
|
|
similar subjects : as, indeed, happened in the case of two distinguished mathematicians., Newton and Leibnitz, regarding
|
|
|
|
the question of the proper figure for a converging lens, one
|
|
|
|
surface being given.
|
|
|
|
It may be asked why I have so long delayed the publication of this work. The reason is that I wrote it rather carelessly in
|
|
|
|
French, expecting to translate it into Latin, and, in the mean-
|
|
|
|
time, to give the subject still further attention.
|
|
3
|
|
|
|
Later I
|
|
|
|
PREFACE
|
|
|
|
thought of publishing this volume together with another on
|
|
|
|
dioptrics in which I discuss the theory of the telescope and the
|
|
|
|
phenomena associated with it. But soon the subject was no longer new and was therefore less interesting. Accordingly I kept putting off the work from time to time, and now I do
|
|
|
|
not know when I shall be able to finish it, for my time is large-
|
|
|
|
ly occupied either by business or by some new investigation.
|
|
|
|
In view of these facts I have thought wise to publish this
|
|
|
|
manuscript in its present state rather than to wait longer and run the risk of its being lost.
|
|
|
|
One finds in this subject a kind of demonstration which does
|
|
|
|
not carry with it so high a degree of certainty as that employed
|
|
|
|
in geometry ; and which differs distinctly from the method
|
|
|
|
employed by geometers in that they prove their propositions
|
|
|
|
by well-established and incontrovertible principles, while here
|
|
|
|
principles are tested by the inferences which are derivable
|
|
|
|
from them. The nature of the subject permits of no other
|
|
|
|
treatment. It is possible, however, in this way to establish a
|
|
|
|
probability which is little short of certainty. This is the case
|
|
|
|
when the consequences of the assumed principles are in perfect
|
|
|
|
accord with the observed phenomena, and especially when
|
|
|
|
these verifications are numerous ; but above all when one
|
|
|
|
employs the hypothesis to predict new phenomena and finds
|
|
|
|
his expectations realized.
|
|
|
|
If in the following treatise all these evidences of probability
|
|
|
|
are present, as, it seems to me, they are, the correctness of my
|
|
|
|
conclusions will
|
|
|
|
be confirmed ;
|
|
|
|
and, indeed,
|
|
|
|
it is scarcely pos-
|
|
|
|
sible that these matters differ very widely from the picture
|
|
|
|
which I have drawn of them. I venture to hope that those who enjoy finding out causes and who appreciate the wonders
|
|
|
|
of light will be interested in these various speculations arid in
|
|
the new explanation of that remarkable property upon which the structure of the human eye depends and upon which are
|
|
|
|
based those instruments which so powerfully aid the eye. I
|
|
|
|
trust also there will be some who, -from such beginnings, will
|
|
|
|
push these investigations far in advance of what I have been
|
|
|
|
able
|
|
|
|
to
|
|
|
|
do ;
|
|
|
|
for
|
|
|
|
the
|
|
|
|
subject
|
|
|
|
is
|
|
|
|
not
|
|
|
|
one
|
|
|
|
which
|
|
|
|
is
|
|
|
|
easily
|
|
|
|
exhausted.
|
|
|
|
This will be evident especially from those parts of the subject
|
|
|
|
which I have indicated as too difficult for solution; and still
|
|
|
|
more evident from those matters upon which I have not
|
|
|
|
touched at all, such as the various kinds of luminous bodies
|
|
|
|
4
|
|
|
|
PREFACE
|
|
and the whole question of color, which no one can yet boast of having explained.
|
|
Finally, there is much more to be learned by investigation
|
|
concerning the nature of light than I have yet discovered ; and I shall be greatly indebted to those who, in the future, shall
|
|
furnish what is needed to complete my imperfect knowledge.
|
|
THE HAGUE, 8th of January, 1690.
|
|
|
|
TABLE OF CONTENTS
|
|
|
|
CHAPTER I
|
|
|
|
ON THE RECTILINEAR PROPAGATION OF RAYS
|
|
|
|
PAGE
|
|
|
|
Light is produced by a certain motion
|
|
|
|
10
|
|
|
|
Particles do not pass from the luminous object to the eye
|
|
|
|
10
|
|
|
|
Light is propagated radially very much after the manner of Sound ... 11
|
|
|
|
[As to] whether Light requires time for its propagation
|
|
|
|
11
|
|
|
|
An experiment which apparently shows that its transmission is in-
|
|
|
|
stantaneous
|
|
|
|
11
|
|
|
|
An experiment which shows that it requires time
|
|
|
|
13
|
|
|
|
Comparison of the Speeds of Light and Sound
|
|
|
|
15
|
|
|
|
How the propagation of Light differs from that of Sound
|
|
|
|
15
|
|
|
|
They are not each transmitted by the same medium.
|
|
|
|
15
|
|
|
|
The propagation of Sound
|
|
|
|
16
|
|
|
|
The propagation of Light
|
|
|
|
17
|
|
|
|
Details concerning the propagation of Light
|
|
|
|
19
|
|
|
|
Why rays travel only in straight lines
|
|
|
|
22
|
|
|
|
How rays coming from different directions cross each other without
|
|
|
|
interference
|
|
|
|
23
|
|
|
|
CHAPTER II
|
|
|
|
ON REFLECTION
|
|
|
|
Proof that the angles of incidence and reflection are equal to each
|
|
|
|
other
|
|
|
|
25
|
|
|
|
Why the incident and reflected rays lie in one and the same plane
|
|
|
|
perpendicular to the reflecting surface
|
|
|
|
27
|
|
|
|
Equality between the angles of incidence and reflection does not de-
|
|
|
|
mand that the reflecting surface be perfectly plane
|
|
|
|
28
|
|
|
|
CHAPTER III ON REFRACTION
|
|
|
|
Bodies may be transparent without any matter passing through them 30
|
|
|
|
Proof that the ether can penetrate transparent bodies
|
|
|
|
31
|
|
|
|
How the ether renders bodies transparent by passing through them. . 32
|
|
|
|
Bodies, even the most solid ones, have a very porous structure
|
|
|
|
32
|
|
|
|
7
|
|
|
|
TABLE OF CONTENTS
|
|
|
|
PAGJ?
|
|
|
|
The speed of light is less in water and in glass than in air
|
|
|
|
32
|
|
|
|
A third hypothesis for the explanation of transparency and of the
|
|
|
|
retardation which light undergoes in bodies
|
|
|
|
33
|
|
|
|
Concerning a possible cause of opacity
|
|
|
|
34
|
|
|
|
Proof that refraction follows the Law of Sines
|
|
|
|
34
|
|
|
|
Why the incident and the refracted rays are each capable of produc-
|
|
|
|
ing the other
|
|
|
|
35
|
|
|
|
Why reflection inside a triangular glass prism suddenly increases
|
|
|
|
when the light is no longer able to emerge
|
|
|
|
38
|
|
|
|
Bodies in which refraction is greatest are also those in which reflec-
|
|
|
|
tion is strongest
|
|
|
|
40
|
|
|
|
Demonstration of a theorem due to Fermat . .
|
|
|
|
40
|
|
|
|
CHAPTER IV
|
|
ON ATMOSPHERIC REFRACTION
|
|
[Not translated.]
|
|
CHAPTER V ON THE PECULIAR REFRACTION OF ICELAND SPAR
|
|
[Not translated.]
|
|
CHAPTER VI ON FIGURES OF TRANSPARENT BODIES ADAPTED FOR REFRAC-
|
|
TION AND REFLECTION
|
|
[Not translated.] 8
|
|
|
|
CHAPTER I
|
|
ON THE RECTILINEAR PROPAGATION OF RAYS
|
|
DEMONSTRATIONS in optics, as in every science where geometry is applied to matter, are based upon experimental facts; as,
|
|
for instance, that light travels in straight lines, that the angles
|
|
of incidence and reflection are equal, and that rays of light are refracted according to the law of sines. For this last fact is
|
|
now as widely known and as certainly known as either of the
|
|
preceding.
|
|
Most writers upon optical subjects have been satisfied to assume these facts. But others, of a more investigating turn of mind, have tried to find the origin and the cause of these facts, considering them in themselves interesting natural phe-
|
|
nomena. And although they have advanced some ingenious
|
|
ideas, these are not such that the more intelligent readers do not still want further explanation in order to be thoroughly
|
|
satisfied.
|
|
Accordingly, I here submit some considerations on this subject with the hope of elucidating, as best I may, this department of natural science, which not undeservedly has gained the reputation of being exceedingly difficult. I feel myself especially indebted to those who first began to make clear these deeply obscure matters, and to lead us to hope that they were
|
|
capable of simple explanations. But, on the other hand, I have been astonished to find these
|
|
same writers accepting arguments which are far from evi-
|
|
dent as if they were conclusive and demonstrative. No one
|
|
has yet given even a probable explanation of the fundamental
|
|
and remarkable phenomena of light, viz*, why it travels in straight lines and how rays coining from an infinitude of dif-
|
|
ferent directions cross one another without disturbing one an-
|
|
other.
|
|
I shall attempt, in this volume, to present in accordance with
|
|
9
|
|
|
|
M KM 01 US ON
|
|
the principles of modern philosophy, some clearer ;i,nd more probable reasons, first, for the rectilinear propagation of light, and, secondly, for its reflection when it meets .other bodies. Later 1 shall explain the phenomenon of rays which art! said to undergo refraction in passing through transparent, bodies of dilTerenl, kinds. Here 1 shall treat, also of refraction efl'i-ets due
|
|
to the. varying density of the earth's atmosphere. Afterwards I shall examine the causes of that peculiar refraction occur-
|
|
ring in a certain crystal which comes from Iceland. And last I y,
|
|
I shall consider the dill'crenl, shapes required in transparent and in rellecting bodies to converge! rays upon a single point or to deflect them in various ways. Hero we shall see with what ease are determined, by our new theory, not only the ellipses, hyperbolas, and Other Curves which M. Descartes has so ingeniously devised for this purpose, but also the curve which one surface of a lens must, have when the other surface is given, as
|
|
spherical, plane, or of any figure whatever.
|
|
We cannot, help believing that light, consists in the motion
|
|
of a certain material. lA>r when we consider its production we find that here on the earth it is generally produced by fire and llame which, beyond doubt, contain bodies in a state of rapid motion, since they are able to dissolve and melt numerous other more solid bodies. And if we consider its effects, we see
|
|
that when light is converged, as, for instance, by concave mirrors, it is able to produce combustion just as fire does ; i.e., it.
|
|
is able to tear bodies apart ; a property that surely indicates motion, at least in the true philosophy whore one believes all
|
|
natural phenomena to be mechanical effects. And, in my opin-
|
|
ion, we must admit this, or else give up all hope of ever under-
|
|
standing anything in physics. Since, according to this philosophy, it is considered certain
|
|
thai, the sensation of sight is caused only by the impulse of some form of matter upon tin* nerves at the base of the eye, we have here still another reason for thinking that light consists in a motion of the matter situated between us and the lumi-
|
|
nous body.
|
|
When we consider, further, the very great speed with which light is propagated in all directions, and the fact that when rays come from different directions, even those directly op-
|
|
posite, they cross without disturbing each other, it must be
|
|
evident that we do not see luminous objects by means of matter
|
|
10
|
|
|
|
TIIH \\AYK-TIIKOHY OF LIGHT
|
|
|
|
translated from the <>l)jcct to us, as a shot or MM arrow travels
|
|
|
|
through the air. For certainly this would be in contradiction
|
|
|
|
to the two properties of light which wo have just mentioned,
|
|
and especially to the hitter. Light is then propagated in some other manner, an understanding of which we may obtain from our knowledge of the manner in which sound travels through the air.
|
|
|
|
\\ < know that through the medium of the air, an invisible
|
|
|
|
and impalpable body, sound is propagated in all directions, from the point where it is produced, by means of a motion which is communicated successively from one part of the air to another ; and since this motion travels with the same speed in all directions, it must, form spherical surfaces which contin-
|
|
ually enlarge until linally they strike our ear. Now there can
|
|
|
|
be no doubt that, light also comes from the luminous body to us by means of some motion impressed upon the matter which
|
|
lies in the intervening space; for we have already seen that
|
|
|
|
this cannot occur through the translation of matter from out-
|
|
|
|
point to the other.
|
|
|
|
If. in addition, light requires time for its passage a point
|
|
we shall presently consider it will then follow that this motion
|
|
|
|
is impressed upon the matter gradually, and hence is propagated, as that of sound, by surfaces and spherical waves. I
|
|
|
|
call these 'irdrrti because of their resemblance to those 'which
|
|
|
|
are formed when one throws a pebble into water and which
|
|
|
|
represent gradual propagation in circles, although produced by a different cause and confined <<> ;t plane surface.
|
|
|
|
As
|
|
|
|
to
|
|
|
|
the
|
|
|
|
nest ion
|
|
')
|
|
|
|
of
|
|
|
|
light
|
|
|
|
requiring
|
|
|
|
time for
|
|
|
|
its
|
|
|
|
propaga-
|
|
|
|
tion, let us consider first whether there is any experimental
|
|
|
|
evidence to the contrary.
|
|
|
|
What we can do here on the earth with sources of light placed
|
|
|
|
at great, distanc.es (alt hough showing that light does not occupy
|
|
|
|
:i sensible time in passing over these distances) may be objected to on the ground that these distances are still too srnaM, and
|
|
|
|
thai, therefore, we can conclude only that the propagation of
|
|
light is exceedingly rapid. M. Descartes thought it instanta-
|
|
neous, and based his opinion upon much better evidence, fur-
|
|
|
|
nished by the eclipse of the moon. Nevertheless, as I shall
|
|
|
|
show, even this evidence is not conclusive. I shall state the
|
|
|
|
matter in a manner slightly different from his in order that we may more easily arrive at all the consequences.
|
|
|
|
11
|
|
|
|
MEMOIRS ON
|
|
|
|
A BD Let
|
|
|
|
be
|
|
|
|
the
|
|
|
|
position
|
|
|
|
of
|
|
|
|
the
|
|
|
|
sun ;
|
|
|
|
a part of the orbit or
|
|
|
|
ABC annual
|
|
|
|
path
|
|
|
|
of the
|
|
|
|
earth ;
|
|
|
|
a straight line intersecting in
|
|
|
|
C the orbit of the moon, which is represented by the circle CD.
|
|
|
|
If, now, light requires time say one hour to trav-
|
|
|
|
erse the space be-
|
|
tween the earth
|
|
|
|
and the moon, it follows that when
|
|
|
|
the earth has
|
|
|
|
reached the point
|
|
|
|
fig j
|
|
|
|
B, its shadow, or the interruption
|
|
|
|
of light, will not yet have reached the point C, and will not
|
|
|
|
reach it until one hour later. Counting from the time when
|
|
|
|
the earth occupies the position B, it will be one hour later that
|
|
|
|
the moon arrives at the point C
|
|
|
|
and
|
|
|
|
is there obscured ;
|
|
|
|
but this
|
|
|
|
eclipse or interruption of light will not be visible at the earth until the end of still another hour. Let us suppose that during
|
|
|
|
these two hours the earth has moved to the position E. From this point the moon will appear to be eclipsed at C, a position
|
|
|
|
which it occupied one hour before, while the sun will be seen
|
|
|
|
at A. -For I assume with Copernicus that the sun is fixed and,
|
|
|
|
since light travels in straight lines, must always be seen in its
|
|
|
|
true position. But it is a matter of universal observation, we are told, that the eclipsed moon appears in that part of the
|
|
|
|
ecliptic directly opposite
|
|
|
|
the sun ;
|
|
|
|
while
|
|
|
|
according to our view
|
|
|
|
its position ought to be behind this by the angle GEC, the
|
|
supplement of the angle AEC. But this is contrary to the fact,
|
|
for the angle GEC will be quite easily observed, amounting to about 33. Now according to our computation, which will be
|
|
|
|
found in the memoir on the causes of the phenomena of Sat-
|
|
|
|
urn,- the distance, BA, between the earth and the sun is about
|
|
|
|
12,000 times the diameter of the earth, and consequently 400
|
|
|
|
times the distance of the moon, which is 30 diameters. The
|
|
|
|
ECB angle
|
|
|
|
will, therefore, be almost 400 times as great as
|
|
|
|
BAE, which is 5', viz., the angular distance traversed by the
|
|
|
|
earth in its orbit during an interval of two hours. Thus the
|
|
angle BCE amounts to almost 33, and likewise the angle
|
|
|
|
CEG, which is 5' greater.
|
|
|
|
12
|
|
|
|
f^"
|
|
|
|
^^ THE
|
|
|
|
WAVE-THEORY
|
|
|
|
OF
|
|
|
|
(
|
|
LI'GHT
|
|
|
|
But it must be noted that in this argument the speed of light is assumed to be such that the time required for it to pass from here to the moon is one hour. If, however, we suppose that it
|
|
requires only a minute of time, then evidently the angle CEG
|
|
will amount to only 33' ; and if it requires only ten seconds of time, this angle will amount to less than 6'. But so small a
|
|
quantity is not easily observed in a lunar eclipse, and conse-
|
|
quently it is not allowable to infer the instantaneous propaga-
|
|
|
|
tion of light.
|
|
It is somewhat unusual, we must 'confess, to assume a speed one hundred thousand times as great as that of sound, which,
|
|
according to my observations, travels about 180 toises [1151
|
|
feet] in a second, or during a pulse-beat; but this supposition appears by no means impossible, for it is not a question of carrying a body with such speed, but of a motion passing successively from one point to another.
|
|
I do not therefore, in thinking of these matters, hesitate to
|
|
|
|
suppose that the propagation of light occupies time, for on this view all the phenomena can be explained, while on the contrary view none of them can be explained. Indeed, it seems to
|
|
me, and to many others also, that M. Descartes, whose object has been to discuss all physical subjects in a clear way, and who
|
|
has certainly succeeded better than any one, before him, has written nothing on light and its properties which is not either
|
|
full of difficulty or even inconceivable. But this idea which I have advanced only as a hypothesis has
|
|
recently been almost established as a fact by the ingenious method of Komer, whose work I propose here to describe, expecting that he himself will later give a complete confirmation
|
|
of this view.
|
|
|
|
His method, like the one we have just discussed, is astro-
|
|
|
|
nomical. He proves not only that light requires time for its
|
|
|
|
propagation, but shows also how much time it requires and that
|
|
|
|
its speed must be at least six times greater than the estimate
|
|
|
|
which I have just given.
|
|
|
|
For this demonstration, he uses the eclipses of the small plan-
|
|
|
|
ets which revolve about Jupiter, and which very often pass
|
|
|
|
A into its shadow. His reasoning is as follows : Let
|
|
|
|
denote
|
|
|
|
the sun; BODE, the annual orbit of the earth; F, Jupiter;
|
|
|
|
and GN, the orbit of the innermost satellite, for this one, on
|
|
|
|
account of its short period, is better adapted to this investi-
|
|
|
|
13
|
|
|
|
MEMOIRS ON
|
|
|
|
Cation than is either of the other three. Let G represent the
|
|
|
|
H point of the satellite's entrance into, and
|
|
|
|
the point of its
|
|
|
|
emergence from, Jupiter's shadow.
|
|
|
|
Let us suppose that an emergence of this
|
|
|
|
satellite has been observed while the earth
|
|
|
|
occupies the position B, at some time before
|
|
|
|
the last quarter. If the earth remained in
|
|
|
|
this position, 42J hours would elapse before the next emergence would occur. For this
|
|
|
|
is the time required for the satellite to make one revolution in its orbit and return to op-
|
|
position with the sun. If, for instance, the
|
|
earth remained at the point B during 30 rev-
|
|
olutions, then, after an interval of 30 times
|
|
|
|
42-J hours, the satellite would again be observed to emerge. But if meanwhile the earth has moved to a point 0, more distant from Jupiter, it is evident that, provided light requires time for its propagation, the
|
|
|
|
emergence of the little planet will be recorded later at than it would have been at B.
|
|
|
|
For it will be necessary to add to this in-
|
|
|
|
terval, 30 times 42 \ hours, the time occupied by ligh't in passing
|
|
|
|
CH over a distance MC, the difference of the distances
|
|
|
|
and BH.
|
|
|
|
In like manner, in the other quarter, while the earth travels
|
|
|
|
D from
|
|
|
|
to E, approaching Jupiter, the eclipses will occur
|
|
|
|
earlier when the earth is at E than if it had remained at D.
|
|
|
|
Now by means of a large number of these eclipse observations,
|
|
covering a period of ten years, it is shown that these inequalities are very considerable, amounting to as much as ten minutes or more; whence it is concluded that, for traversing the whole diameter of the earth's orbit KL, twice the distance from
|
|
|
|
here to the sun, light requires about 22 minutes.
|
|
The motion of Jupiter in its orbit, while the earth passes
|
|
from B to C or from D to E, has been taken into account in
|
|
|
|
the computation, where it is also shown that these inequalities cannot be due either to an irregularity in the motion of the
|
|
|
|
satellite or to its eccentricity.
|
|
If we consider the enormous size of this diameter, KL,
|
|
|
|
which I have found to be about 24 thousand times that of the
|
|
|
|
earth, we get some idea of the extraordinary speed of light.
|
|
14
|
|
|
|
THE WAVE-THEORY OF LIGHT
|
|
|
|
KL Even if we Suppose that
|
|
|
|
were only 22 thousand diameters
|
|
|
|
of the earth, a speed covering this distance in 22 minutes would
|
|
|
|
be equivalent to the rate of one thousand diameters per minute,
|
|
|
|
i.e., 16f diameters a second (or a pulse-beat), which makes more
|
|
|
|
than eleven hundred times one hundred thousand toises [212,222
|
|
|
|
kilometres], since one terrestrial diameter contains 2865 leagues,
|
|
|
|
of which there are 5 to the degree, and since, according to the
|
|
|
|
exact determination made by Mr. Picard in 1669 under orders
|
|
|
|
from the king, each league contains 2282 toises.
|
|
|
|
But, as I have said above, sound travels at the rate of only
|
|
|
|
180 toises [350 metres] per second. Accordingly, the speed of
|
|
|
|
light is more than 600,000 times as great as that of sound,
|
|
|
|
which, however, is a very different thing from being instanta-
|
|
|
|
neous, the difference being exactly that between a finite quantity
|
|
|
|
and infinity. The idea that luminous disturbances are handed
|
|
|
|
on from point to point in a gradual manner being thus con-
|
|
|
|
firmed, it follows, as I have already said, that light is propa-
|
|
|
|
gated by spherical waves, as is the case with sound.
|
|
|
|
But if they resemble each other in this, respect, they differ in
|
|
|
|
several others viz., in the original production of the motion
|
|
|
|
which causes them, in the medium through which they travel, and in the manner in which they are transmitted in this
|
|
|
|
medium.
|
|
|
|
Sound, we know, is produced by the rapid disturbance of some body (either as a whole or in part) ; this disturbance setting in motion the contiguous air. But luminous disturbances must
|
|
arise at each point of the luminous object, else all the different parts of this object would not be visible. This fact will be more evident in what follows.
|
|
|
|
In my opinion, this motion of luminous bodies cannot be bet-
|
|
ter explained than by supposing that those which are fluid, such as a flame, and apparently the sun and stars, are composed
|
|
of particles that float about in a much more subtle medium, which sets them in rapid motion, causing them to strike against the still smaller particles of the surrounding ether. But in the case of luminous solids, such as red-hot metal or carbon, we
|
|
may suppose this motion to be caused by the violent disturb-
|
|
ance of the particles of the metal or of the wood, those which lie on the surface exciting the ether. Thus the motion which produces light must also be more sudden and more rapid than that which causes sound, since we do not observe that sonorous
|
|
|
|
15
|
|
|
|
MEMOIRS ON
|
|
|
|
disturbances give rise to light any more than that the motion
|
|
|
|
of the hand through the air gives rise to sound.
|
|
|
|
The question next arises as to the nature of the medium in
|
|
|
|
which is propagated this motion produced by luminous bodies.
|
|
|
|
I
|
|
|
|
have
|
|
|
|
called
|
|
|
|
it
|
|
|
|
ether ;
|
|
|
|
but
|
|
|
|
it
|
|
|
|
is
|
|
|
|
evidently
|
|
|
|
something
|
|
|
|
different
|
|
|
|
from the medium through which sound travels. For this lat-
|
|
|
|
ter is simply the air which we feel and breathe, and which,
|
|
|
|
when removed from any region, leaves behind the luminiferous
|
|
|
|
medium. This fact is shown by enclosing a sounding body in a
|
|
|
|
glass vessel and removing the atmosphere by means of the air-
|
|
|
|
pump which Mr. Boyle has devised, and with which he has per-
|
|
|
|
formed so many beautiful experiments. But in trying this it
|
|
|
|
is well to place the sounding body on cotton or feathers in such
|
|
|
|
a way that it cannot communicate its vibrations either to the
|
|
|
|
glass receiver or to the air-pump, a point which has hitherto
|
|
|
|
been neglected. Then, when all the air has been removed, one
|
|
|
|
hears no sound from the metal even when it is struck.
|
|
|
|
From this we infer not only that our atmosphere, which is unable to penetrate glass, is the medium through which sound
|
|
travels, but also that it is different from that which carries
|
|
|
|
luminous disturbances for when the vessel is exhausted of ;
|
|
|
|
air, light traverses it as freely as before.
|
|
This last point is demonstrated even more clearly by the celebrated experiment of Torricelli. That part of the glass tube which the mercury does not fill contains a high vacuum, but transmits light the same as when filled with air. This shows that there is within the tube some form of matter which
|
|
|
|
is different from air, and which penetrates either glass or mercury, or both, although both the glass and the mercury are im-
|
|
pervious to air. And if the same experiment is repeated, ex-
|
|
cept that a little water be placed on top of the mercury, it becomes equally evident that the form of matter in question passes either through the glass or through the water or through
|
|
|
|
both.
|
|
|
|
As to the different modes of transmission of Sound and light,
|
|
it is easy to understand what happens in the case of sound when one recalls that air can be compressed and reduced to
|
|
a much smaller volume than it ordinarily occupies, and that
|
|
just in proportion as its volume is diminished it tends to regain its original size. This property, taken in conjunction with its penetrability, which it retains in spite of compression,
|
|
16
|
|
|
|
THE WAVE-THEORY OF LIGHT
|
|
|
|
appears to show that it is composed of small particles which
|
|
|
|
float about, in rapid motion, in an ether composed of still finer
|
|
|
|
particles. Sound, then, is propagated by the effort of these
|
|
air particles to escape when at any point in the path of the wave
|
|
|
|
they are more compressed than at some other point.
|
|
|
|
But the enormous speed of light, together with its other
|
|
|
|
properties, hardly allows us to believe that it is propagated in
|
|
the same way. Accordingly, I propose to explain the manner
|
|
|
|
in which I think it must occur. It will be necessary first, how-
|
|
|
|
ever, to describe that property of hard bodies in virtue of which
|
|
|
|
they transmit motion from one to another.
|
|
|
|
If one takes a large number of spheres of equal size, made of
|
|
|
|
any hard material, and arranges them in contact in a straight
|
|
|
|
line, he will find that, on allowing a sphere of the same size to
|
|
|
|
roll against one end of the line, the motion is transmitted in an
|
|
|
|
instant to the other end of the line* The last sphere in the
|
|
|
|
row flies off while the intermediate ones are apparently undis-
|
|
|
|
turbed ;
|
|
|
|
the
|
|
|
|
sphere
|
|
|
|
which
|
|
|
|
originally produced
|
|
|
|
the
|
|
|
|
disturbance
|
|
|
|
also remains at rest. Here we have a motion which is trans-
|
|
|
|
mitted with high speed, which varies directly as the hardness
|
|
of the spheres. Nevertheless, it is certain that this motion is not instantane-
|
|
|
|
ous, but is gradual, requiring time. For if the motion, or, if you please, the tendency to motion, did not pass successively from one sphere to another, they would all be affected at the same instant, and would all move forward together. So far from this being the case, it is the last one only which leaves the row, and it acquires the speed of the sphere which gave the blow. Besides this experiment there are others which show that all bodies, even those which are considered hardest, such as tempered steel, glass, and agate, are really elastic, and bend to some extent whether they are made into rods, spheres, or bodies
|
|
|
|
of any other shape; that is, they yield slightly at the point
|
|
|
|
where they are struck, and immediately regain their original
|
|
|
|
figure. For I have found that in allowing a glass or agate
|
|
|
|
sphere to strike upon a large, thick, flat piece of the same ma-
|
|
|
|
terial, whose surface has been dulled by the breath, the point
|
|
|
|
of contact is marked by a circular disk which varies in size
|
|
|
|
directly as the strength of the blow. This shows that during
|
|
|
|
the encounter these materials yield and then fly back, a proc-
|
|
|
|
ess which must require time.
|
|
|
|
B
|
|
|
|
17
|
|
|
|
MEMOIRS ON
|
|
Now to apply this kind of motion to the explanation of
|
|
light, nothing prevents our imagining the particles of the ether as endowed with a hardness almost perfect and with an elasticity as great as we please. It is not necessary here to discuss the cause either of this hardness or of this elasticity, for such a consideration would lead us too far from the subject. I will, however, remark in passing that these ether particles, in spite of their small size, are in turn composed of parts, and that their elasticity consists in a very rapid motion of a subtle material
|
|
which traverses them in all directions and compels them to assume a structure which offers an easy and open passage to this fluid. This accords with the theory of M. Descartes, except that I do not agree with him in assigning to the pores the form of hollow circular canals. So far from there being any-
|
|
thing absurd or impossible in all this, it is quite credible that nature employs an infinite series of different-sized molecules, endowed with different velocities, to produce her marvellous
|
|
effects.
|
|
But although we do not understand the cause of elasticity? we cannot fail to observe that most bodies possess this property : it is not unnatural, therefore, to suppose that it is a char-
|
|
acteristic also of the small, invisible' particles of the ether. If,
|
|
indeed, one looks for some other mode of accounting for the
|
|
gradual propagation of light, he will have difficulty in finding one better adapted than elasticity to explain the fact of uniform
|
|
speed. And this appears to be necessary; for if the motion slowed
|
|
up as it became distributed through a larger mass of matter, and receded farther from the source of light, then its high speed would be lost at great distances. But we suppose the
|
|
elasticity to be a property of the ether so that its particles regain their shape with equal rapidity whether they are struck with a hard or a gentle blow; and thus the rate at which the
|
|
light moves remains the same [at all distances from the source]. Nor is it necessary that the ether particles should be arranged
|
|
in straight lines, as was the ease with our row of spheres. The most irregular configuration, provided the particles are in con-
|
|
tact with each other, will not prevent their transmitting the motion and handing it on to the regions in front. It is to be
|
|
noted that we have here a law of motion which governs this kind of propagation, and which is verified by experiment, viz., when a sphere such as A, touching several other smaller ones,
|
|
18
|
|
|
|
THE WAVE-THEORY OF LIGHT
|
|
|
|
CCC, is struck by another sphere, B, in such a way as to make an impression upon each of its neighbors, it transfers its motion to them and remains at rest, as does also the sphere B. Now, without supposing that ether particles are
|
|
spherical (for I do not see that this is necessary), we can nevertheless understand that this
|
|
Jaw of impulses plays a part in the propagation of the motion.
|
|
|
|
Equality of size would appear to be a more necessary assumption, since otherwise we should expect the motion to be reflected on passing from a smaller to a larger particle, following the laws of percussion which I published some
|
|
|
|
Fig. 3
|
|
|
|
years ago. Yet, as will appear later, this equal-
|
|
ity is necessary not so much to make the propagation of light possible as to make it easy and intense. Nor does it appear improbable that the ether particles were made equal for a pur-
|
|
pose so important as the transmission of light. This may be
|
|
true, at least, in the vast region lying beyond our atmosphere and serving only to transmit the light of the sun and the
|
|
stars.
|
|
|
|
I have now shown how we may consider light as propagated, in time, by spherical waves, arid how it is possible that the speed of propagation should be as great as that demanded by
|
|
experiment and by astronomical observation. It must, however, be added that although the ether particles are supposed
|
|
to be in continual motion (and there is much evidence for this
|
|
view), the gradual transmission of the waves
|
|
is not thus interfered with. For it does not
|
|
|
|
consist in a translation of these particles, but merely in a small vibration, which they are
|
|
|
|
compelled to transmit to their neighbors in spite of their proper motion and their change
|
|
of relative position.
|
|
But we must consider, in greater detail, the origin of these waves and the manner of their propagation from one point to another. And, first, it follows from what has already been said concerning the production of light that each point of a luminous body, such as the sun, a candle, or a piece of burning car-
|
|
19
|
|
|
|
MEMOIRS ON
|
|
|
|
bon, gives rise to its own waves, and is the centre of these waves. Thus if A, B, and C represent different points in a
|
|
candle flame, concentric circles described about each of these
|
|
points will represent the waves to which they give rise. And
|
|
the same is true for all the points on the surface and within the flame. But since the disturbances at the centre of these
|
|
|
|
waves do not follow each other in regular succession, we need
|
|
not imagine the waves to follow one another at equal intervals; and if, in the figure, these waves are equally spaced, it is rather
|
|
to indicate the progress which one and the same wave has made
|
|
|
|
during equal intervals of time than to represent several waves having their origin at the same point.*
|
|
Nor does this enormous number of waves, crossing one another without confusion and without disturbing one another, appear unreasonable, for it is well known that one and the same particle of matter is able to transmit several waves coming from different, and even opposite, directions. And this is true not only in the case where the displacements follow one
|
|
|
|
another in succession, but also where they are simultaneous. This is because the motion is propagated gradually. It is shown by the row of hard and equal spheres above mentioned.
|
|
A If we allow two equal spheres, and D, to strike against the
|
|
opposite sides of this row at the same instant, they will be observed to rebound each with the same speed that it had before
|
|
|
|
collision, while all the other spheres remain at rest, although
|
|
|
|
the motion has twice traversed the entire row. [This evidently
|
|
|
|
A D implies that the spheres
|
|
|
|
and have equal speeds justi before
|
|
|
|
OOO00OO
|
|
|
|
collision.] If these two oppositely directed motions happen to meet at the middle sphere, B, or at any other sphere, say 0, it will yield and spring back from both sides, thus transmitting both motions at the same instant.
|
|
* [From this paragraph it would appear that Huygens had no conception of trains of light-waves. The experimental evidence for thinking that light-
|
|
waves travel in trains seems first to have been furnished by Young. See pp. 60, 61 below. If, however, one prefers to interpret the colored rings of Newton
|
|
in terms of the wave-theory, this experimental evidence may be ascribed to
|
|
Newton.'] 30
|
|
|
|
THE WAVE-THEORY OF LIGHT
|
|
|
|
Bnt what is strangest and most astonishing of all is that waves produced by displacements and particles so minute should spread to distances so immense, as, for instance, from the sun or from
|
|
|
|
the stars to the earth. For the intensity of these waves must diminish in proportion to their distance from the origin until finally each individual wave is of itself unable to produce the sensation of light. Our astonishment, however, diminishes when we consider that in the great distance which separates us from the luminous body there is an infinitude of waves which, although coming from different parts of the [luminous] body, are practically compounded into a single wave which thus acquires sufficient intensity to affect our senses. Thus the infinitely great number of waves which at any one instant leave a fixed star, as large possibly as our sun, unite to form what
|
|
is equivalent to one single wave* of intensity sufficient to affect
|
|
the eye. Not only so, but each luminous point may send us
|
|
thousands of waves in the shortest imaginable time, on account of r! e rapidity of the blows with which the particles of the
|
|
luminous body strike the ether at these points. The effect of the waves would thus be rendered still more sensible.
|
|
|
|
In considering the propagation of waves, we must remember that each particle of the medium through which the wave spreads doe not communicate its motion only to that neighbor which lies in the straight line drawn from the luminous point, but shares it with all the particles which touch it and resist its motion. Each particle is thus to be considered as the centre
|
|
of a wave. Thus if DCF is a wave whose centre and origin
|
|
is the luminous point A, a parti-
|
|
cle at B, inside the sphere DCF, will give rise to its own individual
|
|
[secondary] wave, KCL, which will
|
|
touch the wave DCF in the point
|
|
C, at the same instant in which the
|
|
|
|
principal wave, originating at A,
|
|
|
|
reaches the position DCF. And it
|
|
|
|
is clear that there will be only one D
|
|
point of the wave KCL which will
|
|
|
|
touch the wave DCF, viz., the point
|
|
A which lies in the straight line from
|
|
|
|
Fig. 6
|
|
|
|
drawn through B. In like manner, each of the other particles,
|
|
|
|
bbbb, etc., lying within the sphere DCF, gives rise to its
|
|
|
|
21
|
|
|
|
MEMOIRS ON
|
|
|
|
own wave. The intensity of each of these waves may, however, be infinitesimal compared with that of DCF, which is
|
|
the resultant of all those parts of the other waves which are at
|
|
a maximum distance from the centre A.
|
|
We see, moreover, that the wave DCF is determined by the
|
|
extreme limit to which the motion has travelled from the point
|
|
A within a certain interval of time. For there is no motion
|
|
|
|
beyond this wave, whatever may have been produced inside by
|
|
those parts of the secondary waves which do not touch the
|
|
sphere DCF. Let no one think this discussion mere hair-
|
|
|
|
splitting. For, as the sequel will show, this principle, so far from being an ultra-refinement, is the chief element in the ex-
|
|
|
|
planation of all the properties of light, including the phe-
|
|
nomena of reflection and refraction. This is exactly the point which seems to have escaped the attention of those who first
|
|
took up the study of light-waves, among whom are Mr. Hooke,
|
|
in his Miorographia, and Father Pardies, who had undertaken to explain reflection and refraction on the wave -theory, as I know from his having shown me a part of a memoir which he was unable to finish before his death. But the most important fundamental idea, which consists in the principle I have just stated, is wanting in his demonstrations. On other points also his view is different from mine, as will some day appear in case
|
|
his writings have been preserved.
|
|
Passing now to the properties of light, we observe first that
|
|
each part of the wave is propagated in such a way that its extremities lie always between the same straight lines drawn from the lumi-
|
|
nous point. For instance, that part of the wave
|
|
BGr, whose centre is the luminous
|
|
|
|
point A, develops into the arc CE,
|
|
ABO limited by the straight lines,
|
|
and AGE. For although the sec-
|
|
|
|
ondary waves produced by the par-
|
|
CAE ticles lying within the space
|
|
|
|
Rff.fi
|
|
|
|
may spread to the region outside,
|
|
nevertheless they do not combine at
|
|
|
|
the same instant to produce one single wave limiting the
|
|
motion and lying in the circumference CE which is their common tangent. This explains the fact that light, pro-
|
|
22
|
|
|
|
THE WAVE-THEORY OF LIGHT
|
|
|
|
vided its rays are not reflected or refracted, always travels in straight lines, so that no body is illuminated by it unless the straight -line path from the source to this body is unob-
|
|
|
|
structed.
|
|
|
|
Let us, for instance, consider the aperture BG- as limited by
|
|
|
|
the
|
|
|
|
opaque
|
|
|
|
bodies
|
|
|
|
BH,
|
|
|
|
GI ;
|
|
|
|
then, as
|
|
|
|
we
|
|
|
|
have
|
|
|
|
just
|
|
|
|
indicated,
|
|
|
|
the light- waves will always be limited by the straight lines
|
|
|
|
AC, AE. The secondary waves which spread into the region
|
|
|
|
ACE outside of
|
|
|
|
have not sufficient intensity to produce the
|
|
|
|
sensation of light.
|
|
|
|
Now, however small we may make the opening BG, the cir-
|
|
|
|
cumstances which compel the light to travel in straight lines
|
|
|
|
still remain the same ;
|
|
|
|
for
|
|
|
|
this
|
|
|
|
aperture
|
|
|
|
is
|
|
|
|
always
|
|
|
|
sufficiently
|
|
|
|
large to contain a great number of these exceedingly minute
|
|
|
|
ether particles. It is thus evident that each particular part of
|
|
|
|
any wave can advance only along the straight line drawn to it
|
|
from the luminous point. And this justifies us in considering
|
|
|
|
rays of light as straight lines.
|
|
From what has been said concerning the small intensity of
|
|
the secondary waves, it would appear not to be necessary that all the ether particles be equal, although such an equality would favor the propagation of the motion. The effect of inequality would be to make a particle, in colliding with a
|
|
larger one, use up a part of its momentum in an effort to recover. The secondary waves thus sent backward towards
|
|
the luminous point would be unable to produce the sensation of light, and would not result in a primary wave similar to CE.
|
|
|
|
Another and more remarkable property of light is that when rays come from different, or even opposite, directions each produces its effect without disturbance from the other. Thus several observers are able, all at the same time, to
|
|
look at different objects through one single opening ; and two individuals can look into each other's eyes at the same
|
|
|
|
instant.
|
|
|
|
If we now recall our explanation of the action of light and of
|
|
waves crossing without destroying or interrupting each other, these effects which we have just described are readily understood, though they are not so easily explained from Descartes' point of view, viz., that light consists in a continuous [hydrostatic] pressure which produces only a tendency to motion.
|
|
23
|
|
|
|
MEMOIRS ON THE WAVE-THEORY OF LIGHT
|
|
For such a pressure cannot, at the same instant, affect bodies from two opposite sides unless these bodies have some tendency to approach each other. It is, therefore, impossible to understand how two persons can look each other in the eye or how one torch can illuminate another.
|
|
24
|
|
|
|
CHAPTER II ON REFLECTION
|
|
|
|
HAVING explained the effects produced by light-waves in a
|
|
homogeneous medium, we shall next consider what happens when they impinge upon other bodies. First of all we shall see how reflection is explained by these same waves and how
|
|
the equality of angles follows as a consequence.
|
|
Let AB represent a plane
|
|
polished surface of some
|
|
metal, glass, or other sub-
|
|
stance, which, for the present, we shall consider as
|
|
|
|
perfectly smooth (concerning irregularities which are unavoidable we shall
|
|
|
|
have something to say at the close of this demon-
|
|
|
|
stration) ; and let the line
|
|
AC, inclined to AB, represent a part of a light-wave whose centre is so far away that this
|
|
part AC may be considered as a straight line. It may be men-
|
|
tioned here, once for all, that we shall limit our consideration
|
|
|
|
to a single plane, viz., the plane of the figure, which passes
|
|
|
|
through the centre of the spherical wave and cuts the plane
|
|
AB at right angles.
|
|
|
|
The region immediately about C on the wave AC will, after
|
|
|
|
a certain interval of time, reach the point B in the plane AB,
|
|
|
|
travelling along the straight line CB, which we may think of
|
|
|
|
as drawn from the source of light and hence drawn perpen-
|
|
dicular to AC. Now in this same interval of time the ^egion A about on the same wave is unable to transmit its entire
|
|
|
|
AB motion beyond the plane
|
|
|
|
; it must, therefore, continue its
|
|
|
|
25
|
|
|
|
MEMOIRS ON
|
|
|
|
motion on this side of the plane to a distance equal to CB,
|
|
|
|
sending out a secondary spherical wave in the manner described
|
|
|
|
above. This secondary wave is here represented by the circle
|
|
|
|
A AN SNR, drawn with its centre at and with its radius
|
|
|
|
equal
|
|
|
|
to CB.
|
|
|
|
H So, also, if we consider in turn the remaining parts of the
|
|
|
|
wave AC, it will be seen that they not only reach the surface
|
|
|
|
AB HK along the straight lines
|
|
|
|
parallel to CB, but they will
|
|
|
|
produce, at the centres K, their own spherical waves in the
|
|
|
|
transparent medium. These secondary waves are here repre-
|
|
|
|
KM sented by circles whose radii are equal to
|
|
|
|
that is, equal
|
|
|
|
HK to the prolongations of
|
|
|
|
BG to the straight line
|
|
|
|
which
|
|
|
|
is drawn parallel to AC. But, as is easily seen, all these cir-
|
|
|
|
cles have a common tangent in the straight line BN, viz., the same line which passes through B and is tangent to
|
|
the first circle having A as centre and AN, equal to BC, as
|
|
|
|
radius.
|
|
|
|
BN This line
|
|
|
|
(lying between B and the point N, the foot of
|
|
|
|
the perpendicular let fall from A) is the envelope of all these
|
|
|
|
circles, and marks the limit of the motion produced by the
|
|
|
|
reflection of the wave AC. It is here that the motion is more
|
|
|
|
intense than at any other
|
|
|
|
point, because, as has been
|
|
|
|
BN explained,
|
|
|
|
is the new
|
|
|
|
position which the wave
|
|
AC has assumed at the in-
|
|
|
|
stant when the point C has reached B. For there is
|
|
|
|
no other line which, like
|
|
BN, is a common tangent
|
|
to these circles, unless it
|
|
|
|
be BG, on the other side of the plane AB. And BGr
|
|
|
|
Fig. 7
|
|
|
|
will represent the trans-
|
|
mitted wave onlv in case
|
|
|
|
the motion occurs in a medium which is homogeneous with
|
|
|
|
that above the plane. If, however, one wishes to see just how
|
|
|
|
the wave AC has gradually passed into the wave BN, he has
|
|
|
|
KO only to use the same figure and draw the straight lines
|
|
|
|
KL parallel to BN, and the straight lines
|
|
|
|
parallel to AC. It is
|
|
|
|
thus seen that the wave AC, from being a straight line, passes
|
|
|
|
26
|
|
|
|
THE WAVE-THEORY OF LIGH
|
|
|
|
successively into all the broken lines OKL, and reassumes the
|
|
|
|
form of a single straight line NB.
|
|
|
|
It is now evident that the angle of reflection is equal to the
|
|
|
|
BNA ABC angle of incidence. For the right-angled triangles
|
|
|
|
and
|
|
|
|
have the side AB in common, and the side OB equal to the side
|
|
|
|
NA, whence it follows that the angles opposite these sides are
|
|
equal, and hence also the angles CBA and NAB. But .CB,
|
|
|
|
perpendicular to CA, is the direction of the incident ray, while AN, perpendicular to the wave BN, has the direction of the
|
|
|
|
reflected ray. These rays are, therefore, equally inclined to the plane AB.
|
|
BN Against this demonstration it may he urged that while
|
|
is the common tangent of the circular waves in the plane of
|
|
|
|
this figure, the fact is that these waves are really spherical and
|
|
have an infinitely great number of similar tangents, viz., all
|
|
straight lines drawn through the point B and lying in the sur-
|
|
|
|
face of a cone generated by the revolution of a straight line
|
|
|
|
BN BA about
|
|
|
|
as axis. It remains to be shown, therefore, that
|
|
|
|
this objection presents no difficulty ; and, incidentally, we shall see that the incident and reflected rays each lie in one plane
|
|
|
|
perpendicular to the reflecting plane.
|
|
|
|
I remark, then, that the wave AC, so long as it is considered
|
|
|
|
merely a line, can produce no light. For a ray of light, however slender, must have a finite thickness in order to be visible.
|
|
|
|
In order, therefore, to represent a wave whose path is along
|
|
|
|
AC this ray, it is necessary to replace the straight line
|
|
|
|
by a
|
|
|
|
HC plane area, as, for instance, by the circle
|
|
|
|
in the following
|
|
|
|
figure, where the luminous point is supposed to be infinitely
|
|
distant. From the preceding proof it is easily seen that each
|
|
|
|
element of area on the wave HC, having reached the plane AB,
|
|
|
|
will
|
|
|
|
there
|
|
|
|
give
|
|
|
|
rise
|
|
|
|
to
|
|
|
|
its
|
|
|
|
own
|
|
|
|
secondary
|
|
|
|
wave ;
|
|
|
|
and
|
|
|
|
when C
|
|
|
|
reaches the point B, these will all have a common tangent
|
|
|
|
BN plane, viz.. the circle
|
|
|
|
equal to CH. This circle will be cut
|
|
|
|
through the centre and at right angles by the same plane which
|
|
|
|
CH thus cuts the circle
|
|
|
|
and the ellipse AB.
|
|
|
|
It is thus seen that the spherical secondary waves can have
|
|
no common tangent plane other than BN. In this plane will
|
|
|
|
be located more of the reflected motion than in any other, and it will therefore receive the light transmitted from the wave CH.
|
|
|
|
I have noted in the preceding explanation that the motion of
|
|
A the wave incident at is not transmitted beyond the plane AB,
|
|
|
|
27
|
|
|
|
MEMOIRS ON
|
|
at least not entirely. And here it is necessary to remark that, although the motion of. the ether may be partly communicated
|
|
to the reflecting body, this cannot in the slightest alter the speed of the propagation of the waves, which determines the angle of reflection. For, in any one medium, a slight disturbance produces waves which travel with the same speed as those
|
|
Fig. 8
|
|
due to a very great disturbance, a consequence of that property of elastic bodies concerning which we have spoken above, viz., the time occupied in recovery is the same whether the compression be large or small. In every case of reflection of light from the surface of any substance whatever the angles of incidence and reflection are therefore equal, even though the body be of such a nature as to absorb a part of the motion delivered .by the incident wave. And, indeed, experiment shows
|
|
that among polished bodies there is no exception to this law
|
|
of reflection.
|
|
"We must emphasize the fact that in our demonstration there is no need that the reflecting surface be considered a perfectly smooth plane, as has been assumed by all those who have attempted to explain the phenomena of reflection. All that is called for is a degree of smoothness such as would be produced by the particles of the reflecting medium being placed one near another. These particles are much larger than those of the ether, as will be shown later when we come to treat of the transparency and opacity of bodies. Since, now, the surface consists thus of particles assembled together, the ether particles being above and smaller, it is evident that one cannot demonstrate the equality of the angles of incidence and reflection from the time-worn analogy with that which happens when
|
|
28
|
|
|
|
THE WAVE-THEORY OF LIGHT
|
|
a ball is thrown against a wall. By our method, on the other
|
|
hand, the fact is explained without difficulty. Take particles of mercury, for instance, for they are so
|
|
small that we must think of the least visible portion of surface as containing millions, arranged like the grains in a heap of
|
|
sand which one has smoothed out as much as possible; this
|
|
surface for our purpose is equal to polished glass. And, though such a surface may be always rough compared with ether particles, it is evident that the centres of all the secondary waves of reflection which we have described above lie practically in one plane. Accordingly, a single tangent comes as near touch-
|
|
ing them all as is necessary for the production of light. And
|
|
this is all that is required in our demonstration to explain the equality of angles without allowing the rest of the motion, reflected in various directions, to produce any disturbing elfect.
|
|
|
|
CHAPTER III
|
|
OK REFRACTION
|
|
|
|
IK the same manner that reflection has been explained by
|
|
|
|
light-waves reflected at the surface of polished bodies, we pro-
|
|
|
|
pose now to explain transparency and the phenomena of refrac-
|
|
|
|
tion by means of waves propagated into and through transpar-
|
|
|
|
ent bodies, whether solids, such as glass, or liquids, such as
|
|
|
|
water and oils. But, lest the passage of waves into these
|
|
|
|
bodies appear an unwarranted assumption, I will first show that
|
|
|
|
this is possible in more ways than one.
|
|
|
|
Let us imagine that the ether does penetrate any transparent
|
|
|
|
body, its particles will still be able to transmit the motion of
|
|
|
|
the waves just as do those of the ether, supposing them each to
|
|
|
|
be elastic. And this we can easily believe to be the case with
|
|
|
|
water and other transparent liquids, since they are composed
|
|
|
|
of discrete particles. But it may appear more difficult in the
|
|
|
|
case of glass and other bodies that are transparent and hard,
|
|
|
|
because their solidity would hardly allow that they should take
|
|
|
|
up any motion except that of their mass as a whole. This,
|
|
|
|
however, is not necessary, since this solidity is not what it ap-
|
|
|
|
pears to us to be, for it is more probable that these bodies are
|
|
|
|
composed of particles which are placed near one another and
|
|
|
|
bound together by an external pressure due to some other kind
|
|
|
|
of matter and by irregularity of their own configurations. For
|
|
|
|
their looseness of structure is seen in the facility with which
|
|
|
|
they are penetrated by the medium of magnetic vortices and
|
|
|
|
those which cause gravitation. One cannot go further than to
|
|
|
|
say that these bodies have a structure similar to that of a sponge,
|
|
|
|
or of light bread, because heat will melt them and change the
|
|
|
|
We relative positions of their particles.
|
|
|
|
infer, then, as has
|
|
|
|
been indicated above, that they are assemblages of particles
|
|
|
|
touching one another but not forming a continuous' solid.
|
|
|
|
This being the case, the motion which these particles receive
|
|
|
|
30
|
|
|
|
MEMOIRS ON THE WAVE-THEORY OF LIGHT
|
|
in the transmission of light is simply communicated from one to another, while the particles themselves remain tethered in their own positions and do not become disarranged among themselves. It is easily possible for this to occur without in any way affecting the solidity of the structure as seen by us.
|
|
By the external pressure of which I have spoken is not to be
|
|
understood that of -'the air, which would be quite insufficient, but that of another and more subtle medium, whose pressure is exhibited by an experiment which I chanced upon a long while ago, namely, that water from which the air has been removed remains suspended in a glass tube open at the lower end, even
|
|
though the air may have been exhausted from a vessel enclosing
|
|
this tube.
|
|
We may thus explain transparency without assuming that
|
|
bodies are penetrated by the luminiferous ether or that they
|
|
contain pores through which the ether can pass. The fact, however, is not only that this medium penetrates ordinary
|
|
bodies, but that it does so with the utmost ease, as indeed has
|
|
already been shown by the experiment of Torricelli which we
|
|
have cited above. When the mercury or the water leaves the
|
|
upper part of the glass tube, the ether appears at once to take its place and transmit light. But following is still another argument for thinking that bodies, not only those which are transparent, but others also, are easily penetrable.
|
|
When light traverses a hollow glass sphere which is com-
|
|
pletely closed, it is evident that the sphere is filled with ether,
|
|
just as is the space outside the sphere. And this ether, as we
|
|
have shown above, consists of particles lying in close contact with each other. If, now, it were enclosed in the sphere in such a way that it could not escape through the pores of the glass, it would be compelled to partake of any motion which one might impress upon the sphere ; ^consequently nearly the same force would be required to impress a given speed upon this sphere, lying upon a horizontal plane, as if it were filled with water, or possibly mercury. For the resistance which a body offers to any velocity one may wish to impart to it varies directly as the quantity of matter which the body contains and which is compelled to acquire velocity. But the fact is that the sphere resists the motion only in proportion to the amount of glass in it. Whence it follows that the ether within is not
|
|
enclosed, but flows through the glass with perfect freedom.
|
|
31
|
|
|
|
MEMOIRS ON
|
|
|
|
Later we shall show, by this same process, that penetrability
|
|
|
|
may be inferred for opaque bodies also.
|
|
A second and more probable explanation of transparency
|
|
|
|
is to say that the light-waves continue on in the ether which
|
|
|
|
always fills the interstices, or pores, of transparent bodies.
|
|
|
|
For since it passes continuously and with ease, it follows that
|
|
|
|
these pores are always full. Indeed, it may be shown that these
|
|
|
|
interstices occupy more space than the particles which make
|
|
|
|
up the body.
|
|
Now if it be true, as we have said, that the force required
|
|
|
|
to impart a given horizontal velocity to a body is proportional
|
|
|
|
to the mass of the body, and if this force be also proportional
|
|
to the weight of the body, as we know by experiment that it
|
|
|
|
is,
|
|
|
|
then
|
|
|
|
the
|
|
|
|
mass
|
|
|
|
of any body
|
|
|
|
must
|
|
|
|
be
|
|
^also
|
|
|
|
proportional
|
|
|
|
to
|
|
|
|
its weight. Now we know that water weighs only -fa part as
|
|
|
|
much as an equal volume of mercury, therefore the substance
|
|
|
|
of the water occupies only -fa part of the space that encloses
|
|
|
|
its mass. Indeed, it must occupy even a smaller fraction than
|
|
|
|
this, "because mercury is not so heavy as gold, and gold is a
|
|
substance which is not very dense, since the medium of mag-
|
|
|
|
netic vortices and that which causes gravitation penetrate it
|
|
|
|
with the utmost ease.
|
|
|
|
But it may be objected that if water be a substance of such
|
|
small density, and if its particles occupy so small a portion of
|
|
its apparent volume, it is very remarkable that it should offer such stubborn resistance to compression ; for it has not been condensed by any force hitherto employed, and remains perfectly liquid while under pressure.
|
|
This is, indeed, no small difficulty. But it may nevertheless
|
|
be explained by supposing that the very violent and rapid
|
|
motion of the subtle medium which keeps water liquid also
|
|
sets in motion the particles of which it is composed, and maintains this liquid state in spite of any pressure which has hitherto
|
|
been applied. If, now, the structure of transparent bodies be as loose as we
|
|
have indicated, we may easily imagine waves penetrating the ether which fills the interstices between the particles. Not
|
|
only so, but we can easily believe that the speed of these waves inside the body must be a little less on account of the small detours necessitated by these same particles. I propose to show
|
|
that in this varying velocity of light lies the cause of refraction.
|
|
32
|
|
|
|
THE WAVE-THEORY OF LIGHT
|
|
|
|
I will first indicate a third and last method by which we may
|
|
|
|
explain transparency, namely, by supposing that the motion of
|
|
|
|
the light-waves is transmitted equally well by the ether particles
|
|
|
|
which fill the interstices of the body, and by the particles which
|
|
|
|
compose the body, the motion being handed on from one to the
|
|
|
|
A other.
|
|
|
|
little later we shall see how beautifully this hypothesis
|
|
|
|
explains the double'refraction of certain transparent substances.
|
|
Should one object that the particles of ether are much smaller
|
|
|
|
than those of the transparent body, since the former pass
|
|
|
|
through the intervals between the latter, and that consequent-
|
|
|
|
ly they would be able to communicate only a small portion of
|
|
|
|
their momentum, we may reply that the particles of the body
|
|
|
|
are composed of other still smaller particles, and that it is these
|
|
secondary particles that take up the momentum from those of
|
|
|
|
the ether.
|
|
|
|
Moreover, if the particles- of the transparent body are slight-
|
|
ly less elastic than are the ether particles, which we may
|
|
|
|
reasonably suppose, it would still follow that the speed of
|
|
|
|
the light waves is less inside the body than outside in the
|
|
|
|
ether.
|
|
|
|
We have here, what appears to me, the manner in which
|
|
|
|
light-waves are probably transmitted by transparent bodies. But there still remains the consideration of opaque bodies and
|
|
|
|
the difference between these and transparent bodies, a question all the more interesting in view of the ease with which ether
|
|
|
|
penetrates all bodies, a fact to which attention has already been directed, and which might lead one to think that all bodies
|
|
|
|
should be transparent. For considering the hollow sphere, by which I have shown the open structure of glass and the ease
|
|
|
|
with which ether passes through it, one would naturally infer the same penetrability as a property of metals and all other
|
|
|
|
substances. Imagine the sphere to be of silver; it would then
|
|
|
|
certainly contain luminiferous ether, because this substance,
|
|
|
|
as well as air, would be present in it when the opening in the sphere was closed up. But when closed and placed upon a horizontal plane it would resist motion only in proportion to the amount of silver in it, showing as above that the enclosed
|
|
|
|
ether does not acquire the motion of the sphere. Silver, there-
|
|
|
|
fore, like glass, is easily penetrated by ether. In between the"
|
|
|
|
particles of silver and of all other opaque bodies this substance
|
|
|
|
is distributed continuously and abundantly ; and, since it can
|
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|
|
c
|
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|
|
33
|
|
|
|
MEMOIRS ON
|
|
|
|
transmit light, we are led to expect that these bodies should be
|
|
|
|
as transparent as glass, which, however, is not the fact.
|
|
|
|
How, then, shall we explain their opacity? Are their con-
|
|
|
|
stituent particles soft and built up of still smaller particles, and thus able to change shape when they are struck by ether
|
|
particles ? Do they thus damp out the motion and stop the
|
|
|
|
propagation of the light-waves ? This seems hardly possible ;
|
|
for if the particles of a metal were soft, how could polished silver and mercury reflect light so well ? What seems to me
|
|
|
|
more probable is that metallic bodies, which are almost the
|
|
|
|
only ones that are really opaque, have interspersed among their
|
|
|
|
hard particles some which are soft, the former producing reflec-
|
|
|
|
tion, the latter destroying transparency ; while, on the other
|
|
|
|
hand, transparent bodies are made up of only hard and elastic
|
|
|
|
particles, which, together with the ether, propagate light- waves
|
|
|
|
in the manner already indicated.
|
|
We pass now to the explanation of refraction, assuming, as
|
|
|
|
above, that light-waves pass through transparent substances
|
|
|
|
arid in them undergo diminution of speed.
|
|
|
|
The fundamental phenomenon in refraction is the follow-
|
|
|
|
ing, viz., when any ray of light, AB, travelling in air, strikes
|
|
|
|
obliquely upon the polished surface of a transparent body, PGy
|
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|
|
it undergoes a sudden change of direction at the point of inci-
|
|
|
|
dence,
|
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|
|
B ;
|
|
|
|
and
|
|
|
|
this change occurs in such
|
|
|
|
a way that the angle
|
|
|
|
CBE, which the ray makes with the normal to the surface, is less than the angle ABD, which the ray in air made with the same normal. To determine the numerical value of these
|
|
|
|
angles, describe about the point B a circle cutting the rays AB, BC. Then the perpendiculars, AD, CE,
|
|
|
|
let fall from these points of intersection
|
|
|
|
upon the normal, DE, viz., the sines of
|
|
|
|
the angles ABD, CBE, bear to one an-
|
|
|
|
other a certain ratio which, for any
|
|
|
|
one transparent body, is constant for
|
|
|
|
all directions of the incident ray. For
|
|
|
|
glass this ratio is almost exactly f,
|
|
|
|
while for water it is very nearly f , thus
|
|
|
|
varying from one transparent body to
|
|
|
|
another.
|
|
|
|
Another property, not unlike the preceding, is that the refractions of rays entering and of rays emerging from a transpar-
|
|
34
|
|
|
|
THE WAVE-THEORY OF LIGHT
|
|
|
|
ent body are reciprocal. That is to say, if an incident ray, AB,
|
|
|
|
be refracted by a transparent body into the ray BO, so also will
|
|
|
|
a ray, CB, in the interior of the body be refracted, on emer-
|
|
|
|
gence, into the ray BA.
|
|
|
|
In order to explain these phenomena on our theory, let the
|
|
|
|
AB straight line
|
|
|
|
Fig. 10, represent the plane surface bounding a
|
|
|
|
transparentbodyextendingin
|
|
a direction between C and N.
|
|
|
|
By the use of the word plane we do not mean to
|
|
|
|
imply a perfectly smooth sur-
|
|
|
|
face, but merely such a one
|
|
|
|
as was employed in treating
|
|
|
|
of reflection, and for the
|
|
|
|
same reason. Let the line
|
|
|
|
M
|
|
|
|
AC represent a part of a
|
|
|
|
light- wave whose source is
|
|
|
|
so distant that this part may
|
|
|
|
be treated as a straight line.
|
|
|
|
The region 0, on the wave
|
|
|
|
Fig. 10
|
|
|
|
AC, will, after a certain in-
|
|
|
|
terval of time, arrive at the plane AB, along the straight line
|
|
|
|
CB, which we must think of #s drawn /from the source of
|
|
|
|
AC light, and which will, therefore, intersect
|
|
|
|
at right angles.
|
|
|
|
A But during this same interval of time the region about would
|
|
|
|
have arrived at G, along the straight line AG, equal and parallel
|
|
to CB, and, indeed, the whole of the wave AC would have
|
|
|
|
reached the position GB, provided the transparent body were capable of transmitting waves as rapidly as the ether. But
|
|
suppose that the rate of transmission is less rapid, say one-third
|
|
A less. Then the motion from the point will extend into the
|
|
transparent body to a distance which is only two-thirds of CB, while producing its secondary spherical wave as described above. This wave is represented by the circle SNR, whose cen-
|
|
A tre is at and whose radius is equal to f CB. If we consider,
|
|
H in like manner, the other points of the wave AC, it will be
|
|
seen that, during the same time which C employs in going to B, these points will not only have reached the surface AB, along the straight lines HK, parallel to CB, but they will have start-
|
|
ed secondary waves into the transparent body from the points
|
|
K as centres. These secondary waves are represented by cir-
|
|
35
|
|
|
|
MEMOIRS ON
|
|
|
|
KM HK cles whose radii are respectively equal to f of the distances
|
|
|
|
that is, f of the prolongations of
|
|
|
|
to the straight line
|
|
|
|
BG. If the two transparent media had the same ability to
|
|
|
|
transmit light, these radii would equal the whole lengths of
|
|
|
|
the various lines KM.
|
|
|
|
But all these circles have a common tangent in the line BN,
|
|
|
|
viz., the same line which we drew from the point B tangent to
|
|
|
|
SNR the circle
|
|
|
|
first considered. For it is easy to see that all
|
|
|
|
the other circles from B up to the point of contact, N, touch,
|
|
|
|
N in the same manner, the line BN, where
|
|
|
|
is also the foot of
|
|
|
|
the perpendicular let fall from A upon BN.
|
|
|
|
BN We may, therefore, say that
|
|
|
|
is made up of small arcs of
|
|
|
|
these circles, and that it marks the limits which the motion
|
|
from the wave AC has reached in the transparent medium, and
|
|
the region where this motion is much greater than anywhere
|
|
|
|
else. And, furthermore, that this line, as already indicated, is
|
|
the position assumed by the wave AC at the instant when the
|
|
|
|
region C has reached the point B. For there is no other line
|
|
|
|
below the plane AB, which, like BN, is a common tangent to
|
|
|
|
all these secondary waves.
|
|
|
|
Accordingly, if one wishes to discover through what in-
|
|
|
|
termediate steps the wave AC reached the position BN, he has
|
|
|
|
KO only to draw, in the same figure, the straight lines
|
|
|
|
KL parallel to BN, and all the lines
|
|
|
|
parallel to ,AC. He will
|
|
|
|
CA thus see that the wave
|
|
|
|
passes from a straight line into the
|
|
|
|
successive broken lines LKO, reassuming the form of a straight line in the position BN. From what has preceded this will be
|
|
|
|
so evident as to need no further explanation.
|
|
|
|
If, now, using the same
|
|
|
|
C
|
|
|
|
figure, we draw EAF nor-
|
|
|
|
mal to the plane AB at the
|
|
|
|
point A, and draw DA at
|
|
|
|
right angles to the wave AC,
|
|
|
|
the incident ray of light will
|
|
|
|
then be represented by DA;
|
|
|
|
and AN, which is drawn per-
|
|
|
|
pendicular to BN, will be
|
|
|
|
the refracted ray; for these
|
|
|
|
rays are merely the straight
|
|
|
|
ffiff- 10
|
|
|
|
lines along which the parts of the waves travel.
|
|
|
|
36
|
|
|
|
THE WAVE-THEORY OF LIGHT
|
|
|
|
From the foregoing it is easy to deduce the principal law of
|
|
|
|
DAE refraction, viz., that the sine of the angle
|
|
|
|
always bears a
|
|
|
|
constant ratio of the sine of the angle NAF, whatever may be
|
|
|
|
the direction of the incident ray, and that the ratio is the
|
|
|
|
same as that which the speed of the waves in the medium on
|
|
|
|
AE the side
|
|
|
|
bears to their speed on the side AF.
|
|
|
|
AB For if we consider
|
|
|
|
as the radius of a circle, the sine
|
|
|
|
ABN of the angle BAG is BC, and the sine of the angle
|
|
|
|
_is
|
|
|
|
AN.
|
|
|
|
DAE But the angles BAG and
|
|
|
|
are equal; for each is
|
|
|
|
the complement of CAE.
|
|
|
|
ABN And the angle
|
|
|
|
is equal to
|
|
|
|
NAF, since each is the complement of BAN". Hence the sine
|
|
|
|
NAF DAE of the angle
|
|
|
|
is to the sine
|
|
|
|
as BC is to AN. But
|
|
|
|
AN the ratio of BO to
|
|
|
|
is the same as that of the speeds of
|
|
|
|
AE light in the media on the side towards
|
|
|
|
and the side tow-
|
|
|
|
DAE ards AF, respectively ; hence, also, the sine of the angle
|
|
|
|
NAF bears to the sine of the angle
|
|
|
|
the same ratio as these two
|
|
|
|
speeds of light.
|
|
In order to follow the refracted ray when the light-waves en-
|
|
ter a body which transmits them .more rapidly than the body from which they emerge (say in the ratio of 3 to 2), it is necessary only to repeat the same construction and the same demonstration which we have just been
|
|
|
|
using, substituting, however,
|
|
f in place of f . And we find,
|
|
by the same logical process,
|
|
employing this other figure, that when the region of
|
|
the wave AO reaches the
|
|
|
|
point B of the surface AB, the whole wave AC will have
|
|
|
|
advanced to the position BN,
|
|
|
|
such that the ratio of BC, per-
|
|
|
|
pendicular to AC, is to AN,
|
|
|
|
perpendicular to BN, as 2 is to 3. The same ratio will
|
|
|
|
Fig. 11
|
|
|
|
EAD also hold between the sine of the angle
|
|
|
|
and the sine of
|
|
|
|
the angle FAN.
|
|
|
|
The reciprocal relations between the refractions of a ray
|
|
|
|
on entering and on emerging from one and the same me-
|
|
|
|
NA dium is thus made evident. If the ray
|
|
|
|
is incident upon
|
|
|
|
the exterior surface AB, and is refracted into AD, then
|
|
|
|
37
|
|
|
|
MEMOIRS ON
|
|
|
|
DA the ray
|
|
|
|
on emerging from the medium will be refracted
|
|
|
|
into AN".
|
|
|
|
We are now able to explain a remarkable phenomenon which
|
|
|
|
DA occurs in this refraction. When the incident ray
|
|
|
|
exceeds
|
|
|
|
a certain inclination it loses its ability to pass into the other
|
|
|
|
DAQ medium. Because if the angle
|
|
|
|
OBA or
|
|
|
|
is such that, in
|
|
|
|
the triangle AOB, OB is equal to or greater than f of AB, then
|
|
|
|
AN, being equal to or greater than AB, can no longer form one
|
|
|
|
BN side of the triangle ANB. ' Therefore the wave
|
|
|
|
does not
|
|
|
|
AN exist, and consequently there can be no line
|
|
|
|
drawn at right
|
|
|
|
DA angles to it. And thus the incident ray
|
|
|
|
cannot penetrate
|
|
|
|
the surface AB.
|
|
|
|
When the wave-speeds are in the ratio of % to 3, as in the
|
|
|
|
case of glass and air, which we have considered, the angle
|
|
|
|
DAQ DA must exceed 48 11' if the ray
|
|
|
|
is to emerge. And
|
|
|
|
when the ratio of speeds is that of 3 to 4, as is almost exactly
|
|
|
|
DAQ the case in water and air, this angle
|
|
|
|
must be greater than
|
|
|
|
41 24'. And this agrees perfectly with experiment.
|
|
|
|
But one may here ask why no light penetrates the surface,
|
|
since the encounter of the wave AC against the surface AB
|
|
must produce some motion in the medium on the other side. The answer is simple, if we recall what has already been said. For although an infinite number of secondary waves may be started into the medium on the other side of AB, these waves
|
|
|
|
at no time have a common tangent* line, either straight or
|
|
curved. There is thus no line which marks the limit to which
|
|
|
|
the wave AC has been transmitted beyond the plane, AB, nor is
|
|
|
|
there any line in which the motion has been sufficiently con-
|
|
|
|
centrated to produce light.
|
|
In the following manner one may easily recognize the fact
|
|
that, when OB is greater than f AB, the waves beyond the
|
|
K plane AB have no common tangent. About the centres
|
|
describe circles having radii respectively equal to f LB. These
|
|
circles will enclose one another and will each pass beyond the
|
|
|
|
point B.
|
|
|
|
DAQ It is to be noted that just as soon as the angle
|
|
|
|
becomes
|
|
|
|
DA too small to allow the refracted ray
|
|
|
|
to pass into, the other
|
|
|
|
AB medium, the internal reflection which occurs at the surface
|
|
|
|
increases rapidly in brilliancy, as may be easily shown by means
|
|
|
|
of a triangular prism. In terms of our theory, we may thus
|
|
|
|
DAQ explain this phenomenon : While the angle
|
|
|
|
is still large
|
|
|
|
38
|
|
|
|
THE WAVE-THEORY OF LIGHT
|
|
|
|
DA enough for the ray
|
|
|
|
to be transmitted, it is evident that the
|
|
|
|
light from the wave-front AC will be concentrated into a much
|
|
|
|
shorter line when it reaches the position BN. It will be seen
|
|
|
|
BN also that the wave-front
|
|
|
|
grows shorter in proportion as the
|
|
|
|
DAQ angle CBA or
|
|
|
|
becomes smaller, until finally, when the
|
|
|
|
BN limit indicated above is reached,
|
|
|
|
is reduced to a point.
|
|
|
|
That is to say, when the region about C, on the wave AC,
|
|
reaches B, the wave BN", which is the wave AC after trans-
|
|
|
|
mission, is entirely compressed into this same point B ; and, in
|
|
|
|
H K like manner, when the region about has reached the point
|
|
|
|
AH the part
|
|
|
|
is completely reduced to this same point K. It
|
|
|
|
follows, therefore, that in proportion as the direction of propa-
|
|
gation of the wave AC happens to coincide with the surface AB,
|
|
|
|
so will be the quantity of motion along this surface.
|
|
Now this motion must necessarily spread into the transparent
|
|
|
|
body and also greatly reinforce the secondary waves which pro-
|
|
|
|
duce internal reflection at the face AB, according to the laws
|
|
|
|
of this reflection explained above.
|
|
|
|
And since a small diminution in the angle of incidence is
|
|
|
|
BN sufficient to reduce the wave -front
|
|
|
|
from a fairly large
|
|
|
|
quantity to zero (for if this angle in the case of glass be
|
|
|
|
BAN 49 11', the angle
|
|
|
|
amounts to as much as 11 21'; but if
|
|
|
|
DAQ this same angle
|
|
|
|
be diminished by one degree only, the
|
|
|
|
angle BAN becomes zero and the wave-front BN is reduced to
|
|
|
|
a point), it follows that the internal reflection occurs suddenly,
|
|
|
|
passing from comparative darkness to brilliancy at the instant when the angle of incidence assumes a value which no longer
|
|
|
|
permits refraction.
|
|
|
|
Now as to ordinary external reflection, i. e., reflection which
|
|
|
|
DAQ occurs when the angle of incidence
|
|
|
|
is still large enough
|
|
|
|
to allow the refracted ray to pass through the face AB, this
|
|
|
|
reflection must be from the particles which bound the trans-
|
|
|
|
parent body on the outside, apparently from particles of air
|
|
|
|
and from others which are mixed with, but are larger than, the
|
|
|
|
ether particles.
|
|
On the other hand, external reflection from bodies is pro-
|
|
|
|
duced by the particles which compose these bodies, and which
|
|
|
|
are larger than those of the ether, since the ether flows through
|
|
|
|
the interstices of the body.
|
|
|
|
It must be confessed that we here find difficulty in explain-
|
|
|
|
ing the experimental fact that internal reflection occurs even
|
|
|
|
39
|
|
|
|
MEMOIRS ON
|
|
|
|
where the particles of air can cut no figure, as, for instance, in vessels and tubes from which the air has been exhausted.
|
|
|
|
Experiment shows further that these two reflections are of
|
|
|
|
almost equal intensity, and that in various transparent bodies
|
|
|
|
this intensity increases directly as the refractive index. Thus
|
|
|
|
we see that reflection from glass is stronger than that from
|
|
|
|
water, while in turn that from diamond is stronger than that
|
|
|
|
from glass.
|
|
|
|
I shall conclude this theory of refraction by demonstrating a
|
|
|
|
remarkable proposition depending upon it, namely, that when
|
|
|
|
a ray of light passes from one point to another, the two points
|
|
|
|
lying in different media, refraction at the bounding surface
|
|
|
|
occurs in such a way as to make the time required the least
|
|
|
|
possible ; and exactly the same thing occurs in reflection at a
|
|
|
|
plane surface. M. Fermat discovered this property of refrac-
|
|
|
|
tion, believing with us and in opposition to M. Descartes that
|
|
|
|
light travels more slowly through glass than through air.
|
|
|
|
But, besides this, he assumed what we have just proved from
|
|
|
|
the fact that the velocities in the two media are different, viz.,
|
|
|
|
that
|
|
|
|
the ratio
|
|
|
|
of
|
|
|
|
the
|
|
|
|
sines is
|
|
|
|
a
|
|
|
|
constant ;
|
|
|
|
or,
|
|
|
|
what
|
|
|
|
amounts
|
|
|
|
to
|
|
|
|
the same thing, he assumed, besides the different velocities,
|
|
|
|
that
|
|
|
|
the
|
|
|
|
time
|
|
|
|
employed
|
|
|
|
was
|
|
|
|
a
|
|
|
|
minimum ;
|
|
|
|
and from this he
|
|
|
|
derived the constancy of the sine ratio.
|
|
|
|
His* demonstration, which may be found in his works and in
|
|
|
|
the correspondence of M. Descartes, is very long. It is for this
|
|
|
|
reason that I here offer a simpler and easier one.
|
|
|
|
KF A Let
|
|
|
|
represent a plane surface ; imagine the point in
|
|
|
|
the medium through which the light travels more rapidly, say
|
|
|
|
air ;
|
|
|
|
the
|
|
|
|
point C lies
|
|
|
|
in
|
|
|
|
anoth-
|
|
|
|
er, say water, in which the speed
|
|
|
|
of light is less. Let us sup-
|
|
|
|
pose that a ray passes from A,
|
|
|
|
through B, to 0, suffering re-
|
|
|
|
fraction at B, according to the
|
|
|
|
law above demonstrated ;
|
|
|
|
or,
|
|
|
|
what is the same thing, having
|
|
|
|
drawn PBQ perpendicular to
|
|
|
|
the surface, the sine of the
|
|
|
|
ABP angle
|
|
|
|
is to the sine of the
|
|
|
|
angle CBQ in the same ratio as
|
|
|
|
the speed of light in the medium
|
|
|
|
40
|
|
|
|
THE WAVE-THEORY OF LIGHT
|
|
|
|
A containing is to the speed in the medium containing C. It
|
|
|
|
remains to show that the time required for the light to traverse
|
|
AB and BC taken together is the least possible. Let us assume
|
|
|
|
that the light takes some other path, say AF, FC, where F, the
|
|
|
|
point at which refraction occurs, is more distant than B from A.
|
|
|
|
Draw
|
|
|
|
AO
|
|
|
|
perpendicular
|
|
|
|
to
|
|
|
|
AB,
|
|
|
|
and
|
|
|
|
FO
|
|
|
|
BA parallel to
|
|
|
|
;
|
|
|
|
BH
|
|
|
|
perpendicular to FO, and FG perpendicular to BC. Since, now,
|
|
|
|
the angle HBF is equal to PBA, and the angle BFG is equal to
|
|
|
|
HBF QBC, it follows that the sine of the angle
|
|
|
|
will bear to the
|
|
|
|
sine of BFG the same ratio as the speed of light in the medium
|
|
|
|
A bears to the speed in the medium 0. But if we consider BF
|
|
|
|
the radius of a circle, then sines are represented by the lines
|
|
|
|
HF, BG.
|
|
|
|
BG Accordingly, the lines HF,
|
|
|
|
are in the ratio of
|
|
|
|
these speeds. If, therefore, we imagine OF to be the incident
|
|
H ray, the time of passage from to F will be the same as the
|
|
|
|
time of passage from B to G in the medium C.
|
|
|
|
But the time from A to B is equal to the time from to H.
|
|
|
|
A Hence the time from to F is the same as the time from to
|
|
|
|
G, via B. Again, the time along FC is greater than the time
|
|
|
|
along
|
|
|
|
GC ;
|
|
|
|
and
|
|
|
|
hence
|
|
|
|
the
|
|
|
|
time
|
|
|
|
along
|
|
|
|
the
|
|
|
|
route
|
|
|
|
OFC
|
|
|
|
is greater
|
|
|
|
than that along the path ABC. But AF is greater than OF;
|
|
|
|
AFC hence, a fortiorij the time along
|
|
|
|
is greater than that
|
|
|
|
along ABC.
|
|
|
|
Let us now assume that the ray passes from A to C by the
|
|
|
|
A route AK, KC, the point of refraction, K, being nearer to
|
|
|
|
CN than is B. Draw
|
|
|
|
perpendicular to
|
|
|
|
BC ;
|
|
|
|
KN" parallel
|
|
|
|
to BC ;
|
|
|
|
BM KN perpendicular to
|
|
|
|
KL and
|
|
;
|
|
|
|
perpendicular to BA.
|
|
|
|
KM Here BL and
|
|
|
|
BKL represent the sines of the angles
|
|
|
|
and
|
|
|
|
KBM that is, the angles PBA and QBC ; and hence they are
|
|
|
|
A in the same ratio as the speeds of light in the media and C
|
|
|
|
respectively. The time, therefore, from L to B is equal to the
|
|
K M time from to ; and, since the time from B to C is equal to M the time from to N, the time by the path LBC is the same K as the time via KMN. But the time from A to is greater
|
|
|
|
A than the time from to L, and, therefore, the time by the
|
|
|
|
AKN route
|
|
|
|
is greater than the route ABC.
|
|
|
|
KC Not only so, but since
|
|
|
|
is greater than KN, the time by
|
|
|
|
AKC the path
|
|
|
|
will be so much the greater than by the path
|
|
|
|
ABC. Hence follows that which was to be proved, namely,
|
|
|
|
ABC that the time along the path
|
|
|
|
is the least possible.
|
|
|
|
41
|
|
|
|
MEMOIRS ON
|
|
|
|
BIOGRAPHICAL SKETCH
|
|
|
|
WHILE there are no sharp lines in nature, there is a very
|
|
true sense in which the year 1642, marking the death of
|
|
|
|
Galileo and the birth of Newton, serves as a line of demar-
|
|
|
|
cation between the foundation and the superstructure of mod-
|
|
|
|
ern physics.
|
|
|
|
Galileo, by his careful study of gravitation, by his clear grasp
|
|
|
|
of force as determining acceleration, by his careful search after
|
|
|
|
causes and their respective effects, by his profound faith in experiment, had more than cleared the ground for the builders of modern physics. The rapid rise of this structure at the hands of Newton and his brilliant contemporaries, Boyle,
|
|
Leibnitz, Bonier, Du Fay, Bradley, and Hooke, marks a dis-
|
|
tinctly modern era compared with that of Galileo.
|
|
|
|
The work of Christiaan Huygens, the "Dutch Archimedes,"
|
|
|
|
occupies, as regards both time and character, a position inter-
|
|
|
|
mediate between these two periods. He was born at The
|
|
|
|
A Hague in 1629, and died there in 1695.
|
|
|
|
splendid ancestry,
|
|
|
|
three years of university training at Leyden and Breda, much
|
|
|
|
travel, and a rare group of associates, combined to give him
|
|
|
|
an education which left little to be desired. Most of his life
|
|
|
|
was spent in Holland, but for the fifteen years following 1666 he lived and worked in Paris, where he was the guest of Louis
|
|
XIV. and the then recently founded French Academy of Sciences. This was for him a happy period of great activity, and
|
|
it was only in anticipation of the revocation of the Edict of
|
|
Nantes, in 1685, that he returned to his own country, where in private retirement and study he spent most of his remain-
|
|
|
|
ing years. His intellectual achievements fall into three not very dis-
|
|
|
|
tinct departments of science namely, mathematics, physics, and physical astronomy. In mathematics, his chief accom-
|
|
|
|
plishments refer to
|
|
(a) The quadrature of conies. (#) The theory of probabilities.
|
|
A (c) discussion of the evolutes and involutes of curves and
|
|
the introduction of the idea of the envelope of a moving
|
|
|
|
straight line. 42
|
|
|
|
THE WAVE-THEORY OF LIGHT
|
|
In physics he gave
|
|
(a) A general solution of the problem of the Compound Pen-
|
|
dulum, and in the demonstration enunciated the very general principle that in any mechanical system acting under gravity the centre of gravity can never rise to a point higher than that from which it fell a principle which we now recognize as a special case of the law that the potential energy of any mechanical system tends to a minimum. (b) The invention of the pendulum clock and its application to the measurement of gravity at various points on the
|
|
earth's surface.
|
|
(c) An accurate description of the behavior of bodies in
|
|
collision.
|
|
(d) The laws governing centrifugal forces. (e) The undulatory theory of light arid its application to
|
|
the explanation of reflection, ordinary refraction, and double refraction.
|
|
Among his contributions to physical astronomy are
|
|
(a) The construction of the first powerful telescope of the
|
|
refracting kind.
|
|
(b) The discovery of the rings of Saturn and its sixth
|
|
satellite.
|
|
(c) Improvements in the methods of grinding lenses and the addition of a tube to the object-glass and another to
|
|
the eye-piece of the aerial telescope. All his mechanical inventions are characterized by practica-
|
|
bility, and all his intellectual work by clearness and elegance. Those who wish a more detailed account of his activity will
|
|
find it in the superb edition of his works* recently published by the Societe Hollandaise des Sciences, while that delightful sketch of his life and work given 'by Dr. Bosschaf should be read by every one.
|
|
* (Euvres Computes de Christiaan Huygens (La Haye : Martin us Nijhoff, 1888 to 19).
|
|
f Bosscha : Christiaan Huygens, Rede am 200sten Ged^chtnistage seines
|
|
Lebensende. Ubersetzt von Engelmann. (Eugelmann : Leipzig, 1895),
|
|
pp. 77. 43
|
|
LIBRA >*-' ov
|
|
Oc
|
|
|
|
ON THE THEORY OF LIGHT AND
|
|
COLOES
|
|
From the Philosophical Transactions for 1802, p. 12.
|
|
AN ACCOUNT OF SOME CASES OF THE
|
|
PRODUCTION OF COLORS NOT HITHERTO DESCRIBED
|
|
From the Philosophical Transactions for 1802. p. 387.
|
|
EXPERIMENTS AND CALCULATIONS
|
|
RELATIVE TO PHYSICAL OPTICS
|
|
From the Philosophical Transactions for 1804.
|
|
.BY
|
|
THOMAS YOUNG.
|
|
These three papers are reprinted in Young's Miscellaneous Works, vol. i., and also in his Lectures on Natural Philosophy and Mechanical Arts.
|
|
45
|
|
|
|
CONTENTS
|
|
|
|
PAGE
|
|
|
|
General Statement of Wave - Theory, including the Principle of Inter-
|
|
|
|
ference
|
|
|
|
47
|
|
|
|
Diffraction in che Shadow of a Narrow Obstacle
|
|
|
|
,
|
|
|
|
62
|
|
|
|
Observations on the Interference Bands in the Shadow of a Narrow
|
|
|
|
Obstacle. . .
|
|
|
|
68
|
|
|
|
46
|
|
|
|
ON THE THEORY OF LIGHT AND
|
|
COLORS*
|
|
A BAKERIAN LECTURE
|
|
Read November 12, 1801.
|
|
|
|
ALTHOUGH the invention of plausible hypotheses, indepen-
|
|
|
|
dent of any connection with experimental observations, can be of
|
|
|
|
very little use in the promotion of natural knowledge, yet the discovery of simple and uniform principles, by .which a great
|
|
|
|
number of apparently heterogeneous phenomena are reduced to coherent and universal laws, must ever be allowed to be of
|
|
|
|
considerable importance towards the improvement of the hu-
|
|
man intellect.
|
|
|
|
The object of the present dissertation is not so much to pro-
|
|
|
|
pose any opinions which are absolutely new, as to refer some
|
|
|
|
theories, which have been already advanced, to their original
|
|
inventors, to support them by additional evidence, and to apply them to a great number of diversified facts, which have hitherto been buried in obscurity. Nor is it absolutely necessary in this instance to produce a single new experiment ; for of experiments there is already an ample store, which are so much
|
|
|
|
the more unexceptionable as they must have been conducted
|
|
|
|
without the least partiality for the system by which they will be explained ; yet some facts, hitherto unobserved, will be brought forward, in order to show the perfect agreement of
|
|
|
|
that system with the multifarious phenomena of nature.
|
|
|
|
The
|
|
|
|
optical
|
|
|
|
observations
|
|
|
|
of Newton are yet
|
|
|
|
unrivalled ;
|
|
|
|
and,
|
|
|
|
excepting some casual inaccuracies, they only rise in our estimation as we compare them with later attempts to improve on
|
|
|
|
* From the Philosophical Transactions for 1802, p. 12
|
|
47
|
|
|
|
MEMOIRS ON
|
|
|
|
A them.
|
|
|
|
further consideration of the colors of thin plates, as
|
|
|
|
they are described in the second book of Newton's Optics, has
|
|
|
|
converted that prepossession which I before entertained for the
|
|
|
|
undulatory system of light into a very strong conviction of its
|
|
|
|
truth and sufficiency, a conviction which has been since most
|
|
|
|
strikingly confirmed by an analysis of the colors of striated
|
|
|
|
substances. The phenomena of thin plates are indeed so sin-
|
|
|
|
gular that their general complexion is not without great diffi-
|
|
|
|
culty reconcilable to any theory, however complicated, that
|
|
|
|
has
|
|
|
|
hitherto
|
|
|
|
been
|
|
|
|
applied
|
|
|
|
to
|
|
|
|
them ;
|
|
|
|
and
|
|
|
|
some
|
|
|
|
of
|
|
|
|
the
|
|
|
|
principal
|
|
|
|
circumstances have never been explained by the most gratui-
|
|
|
|
tous assumptions; but it will appear that the minutest particu-
|
|
|
|
lars of these phenomena are not only perfectly consistent with
|
|
|
|
the theory which will now be detailed, but that they are all the
|
|
|
|
necessary consequences of that theory, without any auxiliary suppositions ; and this by inferences so simple that they become particular corollaries, which scarcely require a distinct
|
|
|
|
enumeration.
|
|
|
|
A more extensive examination of Newton's various writings
|
|
|
|
has shown me that he was in reality the first that suggested
|
|
|
|
such a theory
|
|
|
|
as
|
|
|
|
I
|
|
|
|
shall
|
|
|
|
endeavor
|
|
|
|
to
|
|
|
|
maintain ;
|
|
|
|
that
|
|
|
|
his
|
|
|
|
own
|
|
|
|
opinions varied less from this theory than is now almost univer-
|
|
|
|
sally supposed ; and that a variety of arguments have been ad-
|
|
|
|
vanced, as if to confute him, which may be found nearly in a
|
|
|
|
similar
|
|
|
|
form
|
|
|
|
in his
|
|
|
|
own
|
|
|
|
works ;
|
|
|
|
and
|
|
|
|
this
|
|
|
|
by
|
|
|
|
no
|
|
|
|
less
|
|
|
|
a
|
|
|
|
math-
|
|
|
|
ematician than Leonard Euler, whose system of light, as
|
|
|
|
far as it is worthy of notice, either was, or might have been,
|
|
|
|
wholly borrowed from Newton, Hooke, Hnygens, and Male-
|
|
|
|
branche.
|
|
|
|
Those who are attached, as they may be with the greatest justice, to every doctrine which is stamped with the Newtonian
|
|
approbation, will probably be disposed to bestow on these con-
|
|
siderations so much the more of their attention, as they appear to coincide more nearly with Newton's own opinions. For
|
|
this reason, after having briefly stated each particular po-
|
|
sition of my theory, I shall collect, from Newton's various
|
|
writings, such passages as seem to be the most favorable to its admission; and although I shall quote some papers which may
|
|
be thought to have been partly retracted at the publication of the Optics, yet I shall borrow nothing from them that can be
|
|
supposed to militate against his rnaturer judgment.
|
|
48
|
|
|
|
THE WAVE-THEORY OF LIGHT
|
|
|
|
HYPOTHESIS I
|
|
|
|
A luminiferous ether pervades the universe, rare and elastic
|
|
in a high degree.
|
|
|
|
PASSAGES FROM KEWTOtf
|
|
|
|
"The hypothesis
|
|
his own/' that is,
|
|
|
|
certainly has Dr. Hooke's,
|
|
|
|
a
|
|
"
|
|
|
|
much greater affinity with
|
|
hypothesis than he seems
|
|
|
|
to be aware of; the vibrations of the ether being as useful and
|
|
|
|
necessary in this as in his." Phil. Trans., vol. vii., p. 5087.
|
|
|
|
Abr., vol. i., p. 145. Nov., 1672.
|
|
" To proceed to the hypothesis : first, it is to be supposed therein that there is an ethereal medium, much of the same
|
|
|
|
constitution with air, but far rarer, subtler, and more strongly
|
|
|
|
elastic. It is not to be supposed that this medium is one uni-
|
|
|
|
form matter, but compounded, partly of the main phlegmatic
|
|
|
|
body of ether, partly of other various ethereal spirits, much after the manner that air is compounded of the phlegmatic
|
|
|
|
body of air, intermixed with various vapors and exhalations :
|
|
|
|
for the electric and magnetic effluvia and gravitating princi-
|
|
|
|
ple seem to argue such variety." BIRCH, Hist, of R. 8., vol.
|
|
|
|
iii., p. 249, Dec., 1675.
|
|
" Is not the heat (of the warm room) conveyed through the vacuum by the vibrations of a much subtler medium than air ? And is not this medium the same with that medium by
|
|
which light is refracted and reflected, and by whose vibrations
|
|
light communicates heat to bodies, and is put into fits of easy
|
|
reflection and easy transmission ? And do not the vibrations of this medium in hot bodies contribute to the intenseness and
|
|
|
|
duration of their heat ? And do not hot bodies communicate
|
|
|
|
their heat to contiguous cold ones by the vibrations of this me-
|
|
|
|
dium propagated from them into the cold ones ? And is not this
|
|
|
|
medium exceedingly more rare and subtle than the air, and ex-
|
|
|
|
ceedingly more elastic and active ? And doth it not readily pervade all bodies ? And is it not, by its elastic force, expanded
|
|
|
|
through all the heavens ? May not planets and comets, and
|
|
|
|
all the gross bodies, perform their motions in this ethereal me-
|
|
|
|
dium ? And may not its resistance be so small as to be incon-
|
|
|
|
siderable ? For instance, if this ether (for so I will call it)
|
|
|
|
should be supposed 700,000 times more elastic than our air,
|
|
|
|
and above 700,000 times more rare, its resistance would be
|
|
|
|
D
|
|
|
|
49
|
|
|
|
MEMOIRS ON
|
|
|
|
about 600,000,000 times less than that of water. And so small a resistance would scarce make any sensible alteration in the
|
|
motions of the planets in ten thousand years. If any one
|
|
would ask how a medium can be so rare, let him tell me how
|
|
an electric body can by friction emit an exhalation so rare and
|
|
subtle, and yet so potent? And how the effluvia of a mag-
|
|
net can pass through a plate of glass without resistance, and yet turn a magnetic needle beyond the glass ?" Optics, Qu. 18, 22.
|
|
HYPOTHESIS II
|
|
|
|
Undulations are excited in this ether 'whenever a body becomes luminous.
|
|
|
|
Scholium. I use the word undulation in preference to vibration, because vibration is generally understood as implying a motion which is continued alternately backward and for-
|
|
ward by a combination of the momentum of the body with an
|
|
accelerating force, and which is naturally more or less permanent; but an undulation is supposed to consist in vibratory motion transmitted successively through different parts of a medium without any tendency in each particle to continue its motion, except in consequence of the transmission of succeeding undulations from a distinct vibrating body; as in the air the vibrations of a chord produce the undulations constituting
|
|
sound.
|
|
PASSAGES FROM NEWT02ST
|
|
|
|
" Were I to assume an hypothesis, it should be this, if pro-
|
|
|
|
pounded more generally, so as not to determine what light is
|
|
|
|
further than that it is something or other capable of e-xciting
|
|
|
|
vibrations in the ether ;
|
|
|
|
for
|
|
|
|
thus
|
|
|
|
it will
|
|
|
|
become so general
|
|
|
|
and
|
|
|
|
comprehensive of other hypotheses as to leave little room for
|
|
|
|
new ones to be invented." BIRCH, Hist, of R. S., vol. iii., p.
|
|
|
|
249. Dec., 1675.
|
|
" In the second place, it is to be supposed that the ether is a
|
|
|
|
vibrating medium like air, only the vibrations far more swift
|
|
|
|
and
|
|
|
|
minute ;
|
|
|
|
those
|
|
|
|
of
|
|
|
|
air,
|
|
|
|
made
|
|
|
|
by
|
|
|
|
a
|
|
|
|
man's
|
|
|
|
ordinary
|
|
|
|
voice,
|
|
|
|
succeeding one another at more than half a foot or a foot dis-
|
|
|
|
tance, but those of ether at a less distance than the hundred-
|
|
thousandth part of an inch. And as in air the vibrations are
|
|
|
|
50
|
|
|
|
THE WAVE-THEORY OF LI
|
|
some larger than others, but yet all equally swift (for in a ring of bells the sound of every tone is heard at two or three miles distance in the same order that the bells are struck), so, I suppose, the ethereal vibrations differ in bigness, but not in swiftness. Kow, these vibrations, besides their use in reflection and
|
|
refraction, may be supposed the chief means by which the parts
|
|
of fermenting or putrefying substances, fluid liquors, or melted, burning, or other hot bodies, continue in motion." BIRCH, Hist, of R. S., vol. iii., p. 251, Dec., 1675.
|
|
"When a ray of light falls upon the surface of any pellucid body, and is there refracted or reflected, may not waves of
|
|
vibrations, or tremors, be thereby excited in the refracting or
|
|
reflecting medium ? And are not these vibrations propagated from the point of incidence to great distances ? And do they
|
|
not overtake the rays of light, and by overtaking them successively, do not they put them into the fits of easy reflection and easy transmission described above ?" Optics, Qu. 17.
|
|
"Light is in fits of easy reflection and easy transmission
|
|
before its incidence on transparent bodies. And probably it is
|
|
put into such fits at its first emission from luminous bodies, and continues in them during all its progress/' Optics, Book ii.,
|
|
part iii., prop. 13.
|
|
HYPOTHESIS III
|
|
The sensation of different colors depends on the different frequency of vibrations excited by light in the retina.
|
|
PASSAGES FROM NEWTON
|
|
"The objector's hypothesis, as to the fundamental part of it,
|
|
is not against me. That fundamental supposition is, that the parts of bodies, when briskly agitated, do excite vibrations in the ether, which are propagated every way from those bodies in straight lines, and cause a sensation of light by beating and dashing against the bottom of the eye, something after the manner that vibrations in the air cause a sensation of sound
|
|
by beating against the organs of hearing. Now, the most free and natural application of this hypothesis to the solution of phenomena I take to be this that the agitated parts of bodies, according to their several sizes, figures, and motions, do excite
|
|
vibrations in the ether of various depths or bignesses, which,
|
|
51
|
|
|
|
MEMOIRS ON
|
|
|
|
being promiscuously propagated through that medium to our
|
|
|
|
eyes, effect in us a sensation of light of a white color; but if
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|
|
|
by any means those of unequal bignesses be separated from one
|
|
|
|
another, the largest beget a sensation of a red color; the least,
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|
|
|
or shortest, of a deep violet, and the intermediate ones of inter-
|
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|
|
mediate
|
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|
colors ;
|
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|
much
|
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|
|
after
|
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|
|
the
|
|
|
|
manner
|
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|
|
that
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|
|
|
bodies,
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|
|
according
|
|
|
|
to their several sizes, shapes, and motions, excite vibrations in
|
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|
|
the air of various bignesses, which, according to those bignesses,
|
|
make several tones in sound : that the largest vibrations are
|
|
|
|
best able to overcome the resistance of a refracting superficies,
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|
|
and
|
|
|
|
so break
|
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|
|
through
|
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|
it
|
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|
with
|
|
|
|
least
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|
|
refraction ;
|
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|
|
whence
|
|
|
|
the vi-
|
|
|
|
brations of several bignesses that is, the rays of several colors,
|
|
|
|
which are blended together in light must be parted from one
|
|
|
|
another by refraction, and so cause the phenomena of prisms
|
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|
|
and
|
|
|
|
other
|
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|
|
refracting
|
|
|
|
substances ;
|
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|
|
and
|
|
|
|
that it depends on the
|
|
|
|
thickness of a thin transparent plate or bubble whether a vi-
|
|
|
|
bration shall be reflected at its further superficies or transmit-
|
|
|
|
ted ;
|
|
|
|
so
|
|
|
|
that,
|
|
|
|
according
|
|
|
|
to
|
|
|
|
the
|
|
|
|
number of
|
|
|
|
vibrations
|
|
|
|
interced-
|
|
|
|
ing the two superficies, they may be reflected or transmitted for many successive thicknesses. And since the vibrations which
|
|
|
|
make blue and violet are supposed shorter than those which
|
|
|
|
make red and yellow, they must be reflected at a less thickness
|
|
|
|
of the plate, which is sufficient to explicate all the ordinary
|
|
|
|
phenomena of those plates or bubbles, and also of all natural
|
|
|
|
bodies, whose parts are like so many fragments of such plates.
|
|
|
|
These seem to be the most plain, genuine, and necessary con-
|
|
|
|
ditions of this hypothesis; and they agree so justly with my
|
|
|
|
theory that if the animadversor think fit to apply them, he
|
|
|
|
need
|
|
|
|
not,
|
|
|
|
on
|
|
|
|
that
|
|
|
|
account,
|
|
|
|
apprehend
|
|
|
|
a
|
|
|
|
divorce
|
|
|
|
from
|
|
|
|
it ;
|
|
|
|
but
|
|
|
|
yet, how he will defend it from other difficulties I know not."-
|
|
|
|
Phil Trans., vol. vii., p. 5088. Abr., vol. i., p. 145. Nov., 1672.
|
|
"To explain colors, I suppose that as bodies of various
|
|
|
|
sizes, densities, or sensations do by percussion or other action
|
|
|
|
excite sounds of various tones, and consequently vibrations in
|
|
|
|
the air of different bigness, so the rays of light, by impinging
|
|
|
|
on the stiff refracting superficies, excite vibrations in the
|
|
|
|
ether of various bigness, the biggest, strongest, or most po-
|
|
|
|
tent rays, the largest
|
|
|
|
vibrations ;
|
|
|
|
and
|
|
|
|
others
|
|
|
|
shorter, according
|
|
|
|
to their bigness, strength, or power : and therefore the ends of
|
|
|
|
the capillamenta of the optic nerve, which pave or face the retina, being such refracting superficies, when the rays impinge
|
|
|
|
52
|
|
|
|
THE WAVE-THEORY OF LIGHT
|
|
|
|
upon them, they must there excite these vibrations, which vi-
|
|
|
|
brations (like those of sound in a trunk or trumpet) will run
|
|
|
|
along the aqueous pores or crystalline pith of the capillamenta,
|
|
|
|
through
|
|
|
|
the
|
|
|
|
optic
|
|
|
|
nerves, into
|
|
|
|
the
|
|
|
|
sensorium ;
|
|
|
|
and
|
|
|
|
there, I
|
|
|
|
suppose, affect the sense with various colors, according to their
|
|
|
|
bigness
|
|
|
|
and
|
|
|
|
mixture ;
|
|
|
|
the
|
|
|
|
biggest
|
|
|
|
with
|
|
|
|
the
|
|
|
|
strongest colors,
|
|
|
|
reds and yellows ; the least with the weakest
|
|
|
|
blues and violets ;
|
|
|
|
the middle with green, and a confusion of all with white
|
|
much after the manner that, in the sense of hearing, nature
|
|
|
|
makes use of aerial vibrations of several bignesses to generate
|
|
|
|
sounds of divers tones, for the analogy of nature is to be ob-
|
|
|
|
served." BIRCH, Hist, of R. 8., vol. iii., p. 262, Dec., 1675.
|
|
|
|
' ' Considering the lastingness of the motions excited in the bot-
|
|
tom of the eye by light, are they not of a vibrating nature ? Do
|
|
|
|
not the most refrangible rays excite the shortest vibrations, the
|
|
|
|
least refrangible the largest ? May not the harmony and dis-
|
|
|
|
cord of colors arise from the proportions of the vibrations
|
|
|
|
propagated through the fibres of the optic nerve into the brain,
|
|
|
|
as the harmony and discord of sounds arise from the propor-
|
|
|
|
tions of the vibrations of the air ?" Optics, Qu. 16, 13, 14.
|
|
|
|
[Scholium omitted.]
|
|
|
|
HYPOTHESIS IV
|
|
|
|
All material bodies have an attraction for the ethereal medium, by means of which it is accumulated within their substance, and for a small distance around them, in a state of greater
|
|
density but not of greater elasticity.
|
|
|
|
It has been shown that the three former hypotheses, which
|
|
|
|
may be called essential, are literally parts of the more compli-
|
|
|
|
cated Newtonian system. This fourth hypothesis differs per-
|
|
|
|
haps, in some degree from any that have been proposed by
|
|
|
|
former authors, and is diametrically opposite to that of New-
|
|
|
|
ton ;
|
|
|
|
but
|
|
|
|
both
|
|
|
|
being
|
|
|
|
in
|
|
|
|
themselves
|
|
|
|
equally
|
|
|
|
probable, the op-
|
|
|
|
position is merely accidental, and it is only to be inquired
|
|
|
|
which is the best capable of explaining the phenomena. Other
|
|
|
|
suppositions might perhaps be substituted for this, and there-
|
|
|
|
fore I do not consider it as fundamental, yet it appears to be
|
|
|
|
the simplest and best of any that have occurred to me.
|
|
|
|
53
|
|
|
|
OK THli
|
|
UNIVERSIT
|
|
|
|
MEMOIRS ON
|
|
PROPOSITION I
|
|
All impulses are propagated in a homogeneous elastic medium with an equable velocity.
|
|
Every experiment relative to sound coincides with the observation already quoted from Newton, that all undulations are propagated through the air with equal velocity ; and this is further confirmed by calculations. (LAGRANGE, Misc. Taur.,
|
|
vol. i., p. 91. Also, -much more concisely, in my syllabus of
|
|
a course of lectures on Natural and Experimental Philosophy, about to be published. Art. 289.) If the impulse be so great as materially to disturb the density of the medium, it will be no longer homogeneous; but, as far as concerns our
|
|
senses, the quantity of motion may be considered as infinitely
|
|
small. It is surprising that Euler, although aware of the matter of fact, should still have maintained that the more frequent undulations are more rapidly propagated. (Tlieor. mus. and Conject. phys.} It is possible that the actual velocity of the
|
|
particles of the luminiferous ether may bear a much less pro-
|
|
portion to the velocity of the undulations than in sound, for
|
|
light maybe excited by the motion of a body moving at the rate
|
|
of only one mile in the time that light moves a hundred millions. Scholium 1. It has been demonstrated that in different me-
|
|
diums the velocity varies in the snbduplicate ratio of the force directly and of the density inversely. (Misc. Taur., vol. L, p. 91. Young's Syllabus. Art. 294.)
|
|
Scholium 2. It is obvious, from the phenomena of elastic bodies and of sounds, that the undulations may cross each other without interruption ; but there is no necessity that the
|
|
various colors of white light should intermix their undulations, for, supposing the vibrations of the retina to continue but a five-hundredth of a second after their excitement, a mill-
|
|
ion undulations of each of a million colors may arrive in dis-
|
|
tinct succession within this interval of time, and produce the same sensible effect as if all the colors arrived precisely at the same instant.
|
|
PROPOSITION II
|
|
An undulation conceived to originate from the vibration of a
|
|
single particle must expand through a homogeneous medium
|
|
54
|
|
|
|
THE WAVE-THEORY OF LIGHT
|
|
|
|
in a spherical form, but with different quantities of motion in different parts.
|
|
|
|
For, since every impulse, considered as positive or negative,
|
|
|
|
is propagated with a constant velocity, each part of the undula-
|
|
|
|
tion must in equal times have passed through equal distances
|
|
|
|
from the vibrating-point. And, supposing the vibrating particle,
|
|
|
|
in the course of its motion, to proceed forward to a small dis-
|
|
|
|
tance in a given direction, the principal strength of the undula-
|
|
|
|
tion will naturally be
|
|
|
|
straight
|
|
|
|
before it ;
|
|
|
|
behind
|
|
|
|
it the motion
|
|
|
|
will be equal in a contrary direction ; and at right angles to
|
|
|
|
the line of vibration the undulation will be evanescent.
|
|
|
|
Now, in order that such an undulation may continue its
|
|
|
|
progress to any considerable distance, there must be in each
|
|
|
|
part of it a tendency to preserve its own motion in a right line
|
|
|
|
from
|
|
|
|
the
|
|
|
|
centre ;
|
|
|
|
for
|
|
|
|
if
|
|
|
|
the
|
|
|
|
excess
|
|
|
|
of
|
|
|
|
force
|
|
|
|
at
|
|
|
|
any part
|
|
|
|
were
|
|
|
|
communicated to the neighboring particles, there can be no
|
|
|
|
reason why it should not very soon be equalized throughout,
|
|
|
|
or, in other words, become wholly extinct, since the motions in
|
|
|
|
contrary directions would naturally destroy each other. The
|
|
|
|
origin of sound from the vibration of a chord is evidently of
|
|
|
|
this nature ;
|
|
|
|
on the contrary, in a circular wave
|
|
|
|
of water every
|
|
|
|
part is at the same instant either elevated or depressed. It may be difficult to show mathematically the mode in which this in-
|
|
|
|
equality of force is preserved, but the inference from the mat-
|
|
|
|
ter of fact
|
|
|
|
appears to be
|
|
|
|
unavoidable ;
|
|
|
|
and
|
|
|
|
while the science
|
|
|
|
of
|
|
|
|
hydrodynamics is so imperfect that we cannot even solve the
|
|
|
|
simple problem of the time required to empty a vessel by ;i
|
|
|
|
given aperture, it cannot be expected that we should be able
|
|
|
|
to account perfectly for so complicated a series of phenomena
|
|
|
|
as those of elastic fluids. The theory of Huygens, indeed, ex-
|
|
|
|
plains the circumstance in a manner tolerably satisfactory. He supposes every particle of the medium to propagate a distinct
|
|
|
|
undulation in all directions, and that the general effect is only
|
|
|
|
perceptible where a portion of each undulation conspires in
|
|
|
|
direction at the same instant ;
|
|
|
|
and it is easy to
|
|
|
|
show that
|
|
|
|
sucli
|
|
|
|
a general undulation would in all cases proceed rectilinearly,
|
|
|
|
with proportionate force ; but, upon this supposition, it seems
|
|
|
|
to follow that a greater quantity of force must be lost by the
|
|
|
|
divergence of the partial undulations than appears to be con-
|
|
|
|
sistent with the propagation of the effect to any considerable
|
|
|
|
55
|
|
|
|
MEMOIRS ON
|
|
|
|
distance ;
|
|
|
|
yet it
|
|
|
|
is
|
|
|
|
obvious
|
|
|
|
that
|
|
|
|
some
|
|
|
|
such
|
|
|
|
limitation
|
|
|
|
of the
|
|
|
|
motion must naturally be expected to take place, for if the in-
|
|
|
|
tensity of the motion of any particular part, instead of co^itinu-
|
|
|
|
ing to be propagated straight forward, were supposed to affect
|
|
|
|
the intensity of a neighboring part of the undulation, an im-
|
|
|
|
pulse must then have travelled from an internal to an external circle in an oblique direction, in the same time as in the direc-
|
|
|
|
tion of the radius, and consequently with a greater velocity,
|
|
|
|
against the first proposition. In the case of water the velocity is by no means so rigidly limited as in that of an elastic medium.
|
|
|
|
Yet it is not necessary to suppose, nor is it indeed probable, that
|
|
|
|
there is absolutely not the least lateral communication of the
|
|
|
|
force of the undulation, but that, in highly elastic mediums,
|
|
|
|
this communication is almost insensible. In the air, if a chord
|
|
|
|
be perfectly insulated so as to propagate exactly such vibra-
|
|
tions as have been described, they will, in fact, be much less
|
|
|
|
forcible than if the chord be placed in the neighborhood of a
|
|
|
|
sounding-board, and probably in some measure because of this
|
|
|
|
lateral communication of motions of an opposite tendency.
|
|
And the different intensity of different parts of the same circular undulation may be observed by holding a common tun-
|
|
|
|
ing-fork at arm's-length, while sounding, and turning it, from
|
|
|
|
a plane directed to the ear, into a position perpendicular to
|
|
|
|
that plane.
|
|
|
|
PROPOSITION III
|
|
A portion of a spherical undulation, admitted through an
|
|
aperture into a quiescent medium, toill proceed to be further propagated rectilinearly in concentric superficies, terminated laterally by weak and irregular portions of newly diverging
|
|
undulations.
|
|
|
|
At the instant of admission the circumference of each of
|
|
|
|
the undulations may be supposed to generate a partial undula-
|
|
|
|
tion, filling up the nascent angle between the radii and the sur-
|
|
|
|
face
|
|
|
|
terminating
|
|
|
|
the medium ;
|
|
|
|
but
|
|
|
|
no
|
|
|
|
sensible addition
|
|
|
|
will
|
|
|
|
be
|
|
|
|
made to its strength by a divergence of motion from any other
|
|
|
|
parts of the undulation, for want of a coincidence in time, as
|
|
|
|
has already been explained with respect to the various force of
|
|
|
|
a spherical undulation. If, indeed, the aperture bear but a small
|
|
|
|
proportion to the breadth of an undulation, the newly gener-
|
|
|
|
56
|
|
|
|
THE WAVE-THEORY OF LIGHT
|
|
|
|
ated undulation may nearly absorb the whole force of the por-
|
|
|
|
tion admitted ;
|
|
|
|
and
|
|
|
|
this
|
|
|
|
is
|
|
|
|
the
|
|
|
|
case
|
|
|
|
considered
|
|
|
|
by Newton
|
|
|
|
in
|
|
|
|
the Principia. But no experiment can be made under these
|
|
|
|
circumstanced with light, on account of the minuteness of its
|
|
|
|
undulations and the interference of inflection; and yet some
|
|
|
|
faint radiations do actually diverge beyond any probable lim-
|
|
|
|
its of inflection, rendering the margin of the aperture distinctly
|
|
|
|
visible in all directions. These are attributed by Newton to
|
|
|
|
some unknown cause, distinct from inflection (Optics, Book
|
|
|
|
iii., obs. 5)/and they fully answer the description of this
|
|
|
|
proposition.
|
|
|
|
Let the concentric lines in Fig. 13 represent the con-
|
|
|
|
temporaneous situation of similar parts of a number of succes-
|
|
|
|
sive undulations diverging from the point A; they will also
|
|
|
|
represent the successive situations of each individual undula-
|
|
|
|
tion: let the force of each undulation be represented by the
|
|
|
|
ABO breadth of the line, and let the cone of light
|
|
|
|
be admitted
|
|
|
|
through the aperture BO; then the principal undulations will proceed in a rectilinear direction towards GrH, and the faint
|
|
radiations on each side will diverge from B
|
|
|
|
and as centres, without receiving any ad-
|
|
|
|
ditional force from any intermediate point
|
|
D of the undulation, on account of the in-
|
|
|
|
DE equality of the lines
|
|
|
|
and DF. But if
|
|
|
|
we allow some little lateral divergence from
|
|
|
|
the extremities of the undulations, it must
|
|
|
|
diminish their force, without adding materi-
|
|
|
|
ally to that of the dissipated light ; and their -
|
|
|
|
termination, instead of the right line BG,
|
|
|
|
will assume the form OH, since the loss of
|
|
|
|
force must be more considerable near to
|
|
|
|
than at greater distances. This line corre-
|
|
|
|
sponds with the boundary of the shadow
|
|
|
|
in
|
|
|
|
Newton's first
|
|
|
|
observation,
|
|
|
|
Fig.
|
|
|
|
13 ;
|
|
|
|
and
|
|
|
|
it is much more probable that such a dissi-
|
|
|
|
pation of light was the cause of the increase
|
|
|
|
of the shadow in that observation than that
|
|
|
|
it was owing to the action of the inflecting
|
|
|
|
atmosphere, which must have extended a
|
|
|
|
thirtieth of an inch each way in order to pro-
|
|
|
|
duce it ;
|
|
|
|
especially when it
|
|
|
|
is
|
|
|
|
considered
|
|
|
|
that
|
|
|
|
57
|
|
|
|
Fig. 13
|
|
|
|
MEMOIRS ON
|
|
|
|
the shadow was not diminished by surrounding the hair with a denser medium than air, which must in all probability have weakened and contracted its inflecting atmosphere. In other
|
|
|
|
circumstances the lateral divergence might appear to increase, instead of diminishing, the breadth of the beam.
|
|
As the subject of this proposition has always been esteemed the most difficult part of the undulatory system, it will be proper to examine here the objections which Newton has
|
|
|
|
grounded upon it.
|
|
''To me the fundamental supposition itself seems impossi-
|
|
ble namely, that the waves or vibrations of any fluid can, like
|
|
the rays of light, be propagated in straight lines, without a continual and very extravagant spreading and bending every way into the quiescent medium, where they are terminated by it. I mistake if there be not both experiment and demonstra-
|
|
|
|
tion to the contrary." Phil. Trans., vol. vii., p. 5089. Abr., vol. L, p. 146. Nov. 1672.
|
|
" Motus omnis per flu id urn. propagatus divergit a recto
|
|
|
|
tramite in spatia immota.",
|
|
"Quoniam medium ibi," in the middle of an undulation admitted, " densius est, quam in spatiis hinc inde, dilatabit sese
|
|
|
|
tarn versus spatia utrinque sita, quam versus pulsum rariora
|
|
|
|
intervalla ;
|
|
|
|
eoque
|
|
|
|
pacto
|
|
|
|
pulsns eadem fere celeritate sese in
|
|
|
|
medii partes
|
|
|
|
quiescentes
|
|
|
|
hinc
|
|
|
|
inde
|
|
|
|
relaxare
|
|
|
|
debent ;
|
|
|
|
ideoqne
|
|
|
|
spatium totum occupabunt Hoc experimur in sonis." Prin-
|
|
|
|
cip., lib. ii., prop. 42.
|
|
"Are not all hypotheses erroneous in which light is sup-
|
|
posed to consist in pression or motion propagated through a
|
|
fluid medium ? If it consisted in pression or motion, propa-
|
|
gated either in an instant, or in time, it would bend into the shadow. For pression or motion cannot be propagated in a fluid in right lines beyond an obstacle which stops part of the motion, but will bend and spread every way into the quiescent
|
|
medium which lies beyond the obstacle. The waves on the
|
|
|
|
surface of stagnating water passing by the sides of a broad obstacle which stops part of them, bend afterwards, and dilate themselves gradually into the quiet water behind the obstacle. The waves, pulses, or vibrations of the air, wherein sounds
|
|
consist, bend manifestly, though not so much as the waves of water. For a bell or a cannon may be heard beyond a hill
|
|
which intercepts the sight of the sounding body ; and sounds
|
|
58
|
|
|
|
THE WAVE-THEORY OF LIGHT
|
|
|
|
are propagated as readily through crooked pipes as straight
|
|
|
|
ones. Bat light is never known to follow crooked passages
|
|
|
|
nor to bend into the shadow. For the fixed stars, by the inter-
|
|
|
|
position of any of the planets, cease to be seen. And so do
|
|
|
|
the parts of the sun by the interposition of the moon, Mer-
|
|
|
|
cury, or Venus. The rays which pass very near to the edges
|
|
|
|
of any body are bent a little by the action of the body ; but
|
|
|
|
this bending is not towards but from the shadow, and is per-
|
|
|
|
formed only in the passage of the ray by the body, and at a
|
|
|
|
very small distance from it. So soon as the ray is past the
|
|
|
|
body it goes right on." Optics, Qu. 28.
|
|
Now the proposition quoted from the Principia does not di-
|
|
|
|
rectly contradict this proposition ; for it does not assert that
|
|
|
|
such
|
|
|
|
a motion
|
|
|
|
must diverge
|
|
|
|
equally in
|
|
|
|
all
|
|
|
|
directions ;
|
|
|
|
neither
|
|
|
|
can it with truth be maintained that the parts of an elastic
|
|
|
|
medium communicating any motion must propagate that mo-
|
|
|
|
tion equally in all directions. All that can be inferred by rea-
|
|
|
|
soning is that the marginal parts of the undulation must be
|
|
|
|
somewhat weakened and that there must be a faint divergence
|
|
|
|
in
|
|
|
|
every
|
|
|
|
direction ;
|
|
|
|
but
|
|
|
|
whether
|
|
|
|
either
|
|
|
|
of these
|
|
|
|
effects
|
|
|
|
might
|
|
|
|
be of sufficient magnitude to be sensible could not have been
|
|
|
|
inferred from argument, if the affirmative had not been ren-
|
|
|
|
dered probable by experiment.
|
|
|
|
As to the analogy with other fluids, the most natural infer-
|
|
|
|
ence from it is this : "The waves of the air, wherein sounds
|
|
|
|
consist, bend manifestly, though not so much as the waves of
|
|
|
|
water "; water being an inelastic and air a moderately elastic
|
|
|
|
medium ;
|
|
|
|
but
|
|
|
|
ether
|
|
|
|
being
|
|
|
|
most
|
|
|
|
highly elastic,
|
|
|
|
its
|
|
|
|
waves
|
|
|
|
bend
|
|
|
|
very far less than those of the air, and therefore almost imper-
|
|
|
|
ceptibly. Sounds are propagated through crooked passages,
|
|
|
|
because their sides are capable of reflecting sound, just as light
|
|
|
|
would be propagated through a bent tube, if perfectly polished
|
|
|
|
within.
|
|
|
|
The light of a star is by far too weak to produce, by its faint
|
|
|
|
divergence, any visible illumination of the margin of a planet
|
|
|
|
eclipsing
|
|
|
|
it ;
|
|
|
|
and
|
|
|
|
the
|
|
|
|
interception
|
|
|
|
of
|
|
|
|
the
|
|
|
|
sun's
|
|
|
|
light
|
|
|
|
by
|
|
|
|
the
|
|
|
|
moon is as foreign to the question as the statement of inflec-
|
|
|
|
tion is inaccurate.
|
|
|
|
To the argument adduced by Huygens in favor of the rectilinear propagation of undulations Newton has made no reply; perhaps because of his own misconception of the nature of the
|
|
59
|
|
|
|
MEMOIRS ON
|
|
|
|
motions of elastic mediums, as dependent on a peculiar law of vibration, which has been corrected by later mathematicians.
|
|
On the whole, it is presumed that this proposition may be
|
|
safely admitted as perfectly consistent with analogy and with
|
|
experiment.
|
|
|
|
PROPOSITION IV
|
|
When an undulation arrives at a surface which is the limit of mediums of different densities, a partial reflection takes
|
|
place proportionate in force to the difference of the densities.
|
|
|
|
This may be illustrated, if not demonstrated, by the analogy
|
|
of elastic bodies of different sizes. " If a smaller elastic body
|
|
strikes against a larger one, it is well known that the smaller is
|
|
|
|
reflected more or less powerfully, according to the difference of
|
|
|
|
their magnitudes : thus, there is always a reflection when the
|
|
|
|
rays
|
|
|
|
of
|
|
|
|
light pass
|
|
|
|
from a
|
|
|
|
rarer
|
|
|
|
to
|
|
|
|
a
|
|
|
|
denser
|
|
|
|
stratum
|
|
|
|
of
|
|
|
|
ether ;
|
|
|
|
and frequently an echo when a sound strikes against a cloud.
|
|
|
|
A greater body striking a smaller one propels it, without losing
|
|
|
|
all its motion : thus, the particles of a denser stratum of ether
|
|
|
|
do not impart the whole of their motion to a rarer, but, in their
|
|
|
|
effort to proceed, they are recalled by the attraction of the
|
|
|
|
refracting
|
|
|
|
substance
|
|
|
|
with
|
|
|
|
equal
|
|
|
|
force ;
|
|
|
|
and
|
|
|
|
thus a reflection is
|
|
|
|
always secondarily produced when the rays of light pass from
|
|
|
|
a denser to a rarer stratum." But it is not absolutely necessary to suppose an attraction in the latter case, since the effort
|
|
|
|
to proceed would be propagated backward without it, and the
|
|
|
|
undulation would be reversed, a rarefaction returning in place
|
|
|
|
of a condensation ;
|
|
|
|
and
|
|
|
|
this
|
|
|
|
will
|
|
|
|
perhaps
|
|
|
|
be
|
|
|
|
found
|
|
|
|
most
|
|
|
|
con-
|
|
|
|
sistent with the phenomena.
|
|
|
|
[Propositions F., VI., and VII. omitted.]
|
|
|
|
PROPOSITION VIII
|
|
When two undulations, from different origins, coincide
|
|
either perfectly or very nearly in direction, their joint effect is a combination of the motions belonging to each.
|
|
|
|
Since every particle of the medium is affected by each undu-
|
|
lation, wherever the directions coincide, the undulations can
|
|
proceed no otherwise than by uniting their motions, so that
|
|
the joint motion may be the sum or difference of the separate
|
|
60
|
|
|
|
THE WAVE-THEORY OF LIGHT
|
|
motions, accordingly as similar or dissimilar parts of the undu-
|
|
lations are coincident.
|
|
I have, on a former occasion,, insisted at large on the application of this principle to harmonics ; and it will appear to be of still more extensive utility in explaining the phenomena of
|
|
colors. The undulations which are now to be compared are those of equal frequency. When the two series coincide ex-
|
|
actly in point of time, it is obvious that the united velocity of
|
|
the particular motions must be greatest, and, in effect at least, double the separate velocities ; and also that it must be smallest,
|
|
and, if the undulations are of equal strength, totally destroyed
|
|
when the time of the greatest direct motion belonging to one undulation coincides with that of the greatest retrograde motion
|
|
of the other. In intermediate states the joint undulation will be of intermediate strength ; but by what laws this intermediate strength must vary cannot be determined without further data.
|
|
It is well known that a similar cause produces in sound that
|
|
effect which is called a beat ; two series of undulations of nearly equal magnitude co-operating and destroying each other alternately, as they coincide more or less perfectly in the times of performing their respective motions.
|
|
[Proposition IX. and five corollaries to Proposition VIII.
|
|
are here omitted.] 61
|
|
|
|
AN ACCOUNT OF SOME CASES OF THE
|
|
PRODUCTION OF COLORS NOT HITHERTO DESCRIBED*
|
|
READ JULY 1, 1802
|
|
WHATEVER opinion maybe entertained of the theory o
|
|
and colors which I have lately had the honor of submitting to the Royal Society, it must at any rate be allowed that it has given birth to the discovery of a simple and general law capable of explaining a number of the phenomena of colored light, which, without this law, would remain insulated and unintelligible. The law is, that " wherever two portions of the same light arrive at the eye by different routes, either exactly or very nearly in the same direction, the light becomes most intense when the difference of the routes is any multiple of a certain length, and least intense in the intermediate state of the interfering portions ; and this length is different for
|
|
light of different colors."
|
|
I have already shown in detail the sufficiency of this law for explaining all the phenomena described in the second and third books of Newton's Optics, as well as some others not mentioned by Newton. But it is still more satisfactory to observe its conformity to other facts, which constitute new and distinct classes of phenomena, and which could scarcely have agreed so well with any anterior law, if that law had been erroneous or imaginary : these are the colors of fibres and the colors of mixed plates.
|
|
As I was observing the appearance of the fine parallel lines' of light which are seen upon the margin of an object held near
|
|
*From the Philosophical Transactions for 1802, p. 387.
|
|
|
|
ERSITY
|
|
MEMOIRS OK THE WAVE-THEORY OF LIGHT
|
|
|
|
the eye, so as to intercept the greater part of the light of a
|
|
distant luminous object, and which are produced by the fringes caused by the inflection of light already known, I observed
|
|
|
|
that they were sometimes accompanied by colored fringes,
|
|
much broader and more distinct and I soon found that ;
|
|
|
|
these broader fringes were occasioned by the accidental inter-
|
|
|
|
position of a hair. . In order to make them more distinct, I
|
|
|
|
employed a horse-hair, but they were then no longer visible.
|
|
|
|
r \\
|
|
|
|
ith
|
|
|
|
a
|
|
|
|
fibre of
|
|
|
|
wool,
|
|
|
|
on
|
|
|
|
the
|
|
|
|
contrary,
|
|
|
|
they
|
|
|
|
became
|
|
|
|
very large
|
|
|
|
ard conspicuous; and, with a single silk -worm's thread,
|
|
|
|
their magnitude was so much increased that two or three of
|
|
|
|
them seemed to occupy the whole field of view. They appeared to extend on each side of the candle, in the same order
|
|
|
|
as the colors of thin plates seen by transmitted light. It oc-
|
|
curred to me that their cause must be sought in the interfer-
|
|
|
|
ence of two portions of light, one reflected from the fibre, the other bending round its opposite side, and at last coinciding
|
|
|
|
nearly in direction with the former portion ; that, accordingly, as both portions deviated more from a rectilinear direction, the difference of the length of their paths would become gradual-
|
|
|
|
ly greater and greater, and would consequently produce the
|
|
|
|
appearances
|
|
|
|
of
|
|
|
|
color
|
|
|
|
usual
|
|
|
|
in
|
|
|
|
such
|
|
|
|
cases ;
|
|
|
|
that
|
|
|
|
supposing
|
|
|
|
them to be inflected at right angles, the difference would
|
|
|
|
amount nearly to the diameter of the fibre, and that this dif-
|
|
|
|
ference must consequently be smaller as the fibre became
|
|
|
|
smaller ;
|
|
|
|
and, the
|
|
|
|
number
|
|
|
|
of fringes
|
|
|
|
in a right angle
|
|
|
|
becoming
|
|
|
|
smaller, that their angular distances would consequently be-
|
|
|
|
come greater, and the whole appearance would be dilated. It
|
|
|
|
was easy to calculate that for the light least inflected the
|
|
|
|
difference of the paths would be to the diameter of the fibre
|
|
|
|
very nearly as the deviation of the ray at any point from the rectilinear direction to its distance from the fibre.
|
|
|
|
I therefore made a rectangular hole in a card, and bent its
|
|
|
|
ends so as
|
|
|
|
to support
|
|
|
|
a
|
|
|
|
hair parallel
|
|
|
|
to
|
|
|
|
the
|
|
|
|
sides of the
|
|
|
|
hole ;
|
|
|
|
then, upon applying the eye near the hole, the hair, of course, appeared dilated by indistinct vision into a surface, of which
|
|
|
|
the breadth was determined by the distance of the hair and
|
|
|
|
the magnitude of the hole, independently of the temporary
|
|
aperture of the pupil. When the hair approached so near to
|
|
the direction of the margin of a candle that the inflected light was sufficiently copious to produce a sensible effect, the fringes
|
|
63
|
|
|
|
M E M O I R S ON
|
|
|
|
began to appear ; and it was easy to estimate the proportion
|
|
|
|
of their breadth to the apparent breadth of the hair across the
|
|
|
|
image of which they extended. I found that six of the bright-
|
|
|
|
est red fringes, nearly at equal distances, occupied the whole
|
|
|
|
of that image. The breadth of the aperture was T{Hb-> and its
|
|
|
|
distance from the hair -f$ of an inch ; the diameter of the hair
|
|
|
|
was
|
|
|
|
less
|
|
|
|
than
|
|
|
|
of
|
|
|
|
-g-J-g-
|
|
|
|
an
|
|
|
|
inch ;
|
|
|
|
as
|
|
|
|
nearly
|
|
|
|
as
|
|
|
|
I
|
|
|
|
could
|
|
|
|
ascertain
|
|
|
|
it was ^. Hence, we have y-j-J^ for the deviation of the
|
|
|
|
^ ^ first red fringe at the distance
|
|
|
|
and as
|
|
;
|
|
|
|
T^-Q :
|
|
|
|
::
|
|
|
|
-g-g-g-
|
|
|
|
rro O-OTT* or OTST f r tne difference of the routes of the rea
|
|
|
|
light where it was most intense. The measure deduced from
|
|
|
|
Newton's experiments is 36 | 00 . I thought this coincidence,
|
|
|
|
with only an error of one-ninth of so minute a quantity, suffi-
|
|
|
|
ciently perfect to warrant completely the explanation of the
|
|
|
|
phenomenon, and even to render a repetition of the experi-
|
|
|
|
ment unnecessary ; for there are several circumstances whicft
|
|
|
|
make it difficult to calculate much more precisely what ought
|
|
|
|
to be the result of the measurement.
|
|
|
|
When- a number of fibres of the same kind for instance, a
|
|
|
|
uniform lock of wool are held near to the eye, we see an ap-
|
|
|
|
pearance
|
|
|
|
of
|
|
|
|
halos
|
|
|
|
surrounding
|
|
|
|
a
|
|
|
|
distant
|
|
|
|
candle ;
|
|
|
|
but
|
|
|
|
their
|
|
|
|
brilliancy, and even their existence, depends on the uniformity
|
|
|
|
of the
|
|
|
|
dimensions
|
|
|
|
of
|
|
|
|
the
|
|
|
|
fibres ;
|
|
|
|
and
|
|
|
|
they
|
|
|
|
are
|
|
|
|
larger
|
|
|
|
as
|
|
|
|
the
|
|
|
|
fibres are smaller. It is obvious that they are the immediate
|
|
|
|
consequences of the coincidence of a number of fringes of the
|
|
|
|
same size, which, as the fibres are arranged in all imaginable
|
|
|
|
directions, must necessarily surround the luminous object at
|
|
|
|
equal distances on all sides, and constitute circular fringes.
|
|
|
|
There can be little doubt that the colored atmospherical
|
|
|
|
halos are of the
|
|
|
|
same kind ;
|
|
|
|
their
|
|
|
|
appearance
|
|
|
|
must
|
|
|
|
depend on
|
|
|
|
the existence of a number of particles of water of equal dimen-
|
|
|
|
sions, and in a proper position with respect to the luminary
|
|
|
|
and to the eye. As there is no natural limit to the magnitude
|
|
|
|
of the spherules of water, we may expect these halos to vary
|
|
|
|
without limit in their diameters, and accordingly Mr. Jordan
|
|
|
|
has observed that their dimensions are exceedingly various,
|
|
|
|
and has remarked that they frequently change during the time
|
|
|
|
of observation.
|
|
|
|
I first noticed the colors of mixed plates in looking at a candle through two pieces of plate-glass with a little moisture between them. I observed an appearance of fringes resembling
|
|
|
|
64:
|
|
|
|
THE WAVE-THEORY OF LIGHT
|
|
|
|
the common colors of thin plates ; and, upon looking for the
|
|
|
|
fringes by reflection, I found that these new fringes were
|
|
|
|
always in the same direction as the other fringes, but many
|
|
|
|
times larger. By examining the glasses with a magnifier, I
|
|
|
|
perceived that wherever these fringes were visible the moist-
|
|
|
|
ure was intermixed with portions of air, producing an appear-
|
|
|
|
ance similar to dew. I then supposed that the origin of the
|
|
|
|
colors
|
|
|
|
was
|
|
|
|
the
|
|
|
|
same
|
|
|
|
as
|
|
|
|
that
|
|
|
|
of
|
|
|
|
the
|
|
|
|
colors
|
|
|
|
of
|
|
|
|
halos ;
|
|
|
|
but, on
|
|
|
|
a more minute examination, I found that the magnitude of the
|
|
|
|
portions of air and water was by no means uniform, and that
|
|
|
|
the explanation was, therefore, inadmissible. It was, however,
|
|
|
|
easy to find two portions of light sufficient for the production
|
|
|
|
of these fringes ; for the light transmitted through the water,
|
|
|
|
moving in it with a velocity different from that of the light
|
|
|
|
passing through the interstices filled only with air, the two
|
|
|
|
portions would interfere with each other and produce effects of color according to the general law. The ratio of the
|
|
|
|
velocities
|
|
|
|
in
|
|
|
|
water
|
|
|
|
and
|
|
|
|
in
|
|
|
|
air
|
|
|
|
is
|
|
|
|
that of
|
|
|
|
3
|
|
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|
to
|
|
|
|
4 ;
|
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|
|
the
|
|
|
|
fringes
|
|
|
|
ought, therefore, to appear where the thickness is six times as
|
|
|
|
great as that which corresponds to the same color in the com-
|
|
mon case of thin plates ; and, upon making the experiment
|
|
|
|
with a plane glass and a lens slightly convex, I found the sixtli
|
|
|
|
dark circle actually of the same diameter as the first in the
|
|
|
|
new fringes. The colors are also very easily produced when
|
|
|
|
butter or tallow is substituted for water; and the rings then
|
|
|
|
become smaller, on account of the greater refractive density
|
|
|
|
of
|
|
|
|
the
|
|
|
|
oils ;
|
|
|
|
but when water is
|
|
|
|
added,
|
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|
|
so
|
|
|
|
as
|
|
|
|
to
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|
|
|
fill
|
|
|
|
up
|
|
|
|
the
|
|
|
|
in-
|
|
|
|
terstices of the oil, the rings are very much enlarged ; for here
|
|
|
|
the difference only of the velocities in water and in oil is to
|
|
|
|
be considered, and this is much smaller than the difference
|
|
|
|
between air and water. All these circumstances are sufficient
|
|
|
|
to satisfy us with respect to the truth of the explanation ; and
|
|
|
|
it is still more confirmed by the effect of inclining the plates
|
|
|
|
to the direction of the light; for then, instead of dilating, like
|
|
|
|
the colors of thin plates, these rings contract: and this is the
|
|
|
|
obvious consequence of an increase of the length of the paths
|
|
|
|
of light, which now traverse both mediums obliquely ; and the
|
|
|
|
effect is everywhere the same as that of a thicker plate.
|
|
|
|
It must, however, be observed that the colors are not pro-
|
|
|
|
duced in the whole light that is transmitted through the
|
|
|
|
mediums : a small portion only of each pencil, passing through
|
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|
|
E
|
|
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|
65
|
|
|
|
MEMOIRS ON
|
|
|
|
the water contiguous to the edges of the particle, is sufficient-
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|
|
|
ly coincident with the light transmitted by the neighboring
|
|
|
|
portions
|
|
|
|
of
|
|
|
|
air
|
|
|
|
to
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|
|
|
produce
|
|
|
|
the
|
|
|
|
necessary
|
|
|
|
interference ;
|
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|
|
and
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|
|
it
|
|
|
|
is easy to show that, on account of the natural concavity of the
|
|
|
|
surface of each portion of the fluid adhering to the two pieces
|
|
|
|
of glass, a considerable portion of the light which is beginning
|
|
|
|
to pass through the water will be dissipated laterally by re-
|
|
flection at its entrance, and that much of the light passing
|
|
|
|
through the air will be scattered by refraction at the second
|
|
surface. For these reasons the fringes are seen when the
|
|
|
|
plates are not directly interposed between the eye and the
|
|
luminous object; and on account of the absence of foreign light, even more distinctly than when they are in the same
|
|
right line with that object. And if we remove the plates to a
|
|
|
|
considerable distance out of this line, the rings are still visible
|
|
|
|
and
|
|
|
|
become
|
|
|
|
larger
|
|
|
|
than
|
|
|
|
before ;
|
|
|
|
for here
|
|
|
|
the
|
|
|
|
actual
|
|
|
|
route
|
|
|
|
of
|
|
|
|
the light passing through the air is longer than that of the
|
|
|
|
light passing more obliquely through the water, and the differ-
|
|
|
|
ence in the times of passage is lessened.
|
|
|
|
It is however, im?<
|
|
|
|
possible to be quite confident with respect to the causes of
|
|
|
|
these minute variations, without some means of ascertaining
|
|
|
|
accurately the forms of the dissipating surfaces.
|
|
|
|
In applying the general law of interference to these colors, as well as to those of thin plates already known, I must confess that it is impossible to avoid another supposition, which is
|
|
|
|
a part of the undulatory theory that is, that the velocity of
|
|
|
|
light
|
|
|
|
is
|
|
|
|
the
|
|
|
|
greater
|
|
|
|
the
|
|
|
|
rarer
|
|
|
|
the
|
|
|
|
medium ;
|
|
|
|
and
|
|
|
|
that
|
|
|
|
there
|
|
|
|
is
|
|
|
|
also a condition annexed to the explanation of the colors of thin plates which involves another part of the same theory that is, that where one of the portions of light has been reflected at the surface of a rarer medium, it must be supposed
|
|
|
|
to be retarded one-half of the appropriate interval for instance, in the central black spot of a soap-bubble, where the
|
|
|
|
actual lengths of the paths very nearly coincide, but the effect is the same as if one of the portions had been so retarded as to
|
|
destroy the other. From considering the nature of this cir-
|
|
cumstance,- I ventured to predict that if the two reflections
|
|
|
|
were of the same kind, made at the surfaces of a thin plate of a density intermediate between the densities of the mediums
|
|
|
|
containing it, the effect would be reversed, and the central
|
|
|
|
spot,
|
|
|
|
instead
|
|
|
|
of
|
|
|
|
black,
|
|
|
|
would
|
|
|
|
become
|
|
|
|
white ;
|
|
|
|
and
|
|
|
|
I
|
|
|
|
have
|
|
|
|
now
|
|
|
|
66
|
|
|
|
THE WAVE-THEORY OF LIGHT
|
|
the pleasure of stating that I have fully verified this prediction by interposing a drop of oil of sassafras between a prism of fiint-glass and a lens of crown-glass ; the central spot seen by reflected light was white and surrounded by a dark ring. It was, however, necessary to use some force in order to produce a contact sufficiently intimate ; and the white spot differed, even at last, in the same degree from perfect whiteness as the black spot usually does from perfect blackness.
|
|
[Three pages of speculation concerning dispersion are here
|
|
omitted.] 67
|
|
|
|
EXPEEIMENTS AND CALCULATIONS REL-
|
|
ATIVE TO PHYSICAL OPTICS*
|
|
A BAKEKIAN LECTUEE
|
|
Read Noveniber 24, 1803
|
|
I. EXPERIMENTAL DEMONSTRATION OF THE GENERAL LAW OF THE INTERFERENCE OF LIGHT.
|
|
IN making some experiments on the fringes of colors accompanying shadows, I have found so simple and so demonstrative a proof of the general law of the interference of two portions of light, which I have already endeavored to estab-
|
|
lish, that I think it right to lay before the Royal Society a
|
|
short statement of the facts which appear to me so decisive. The proposition on which I mean to insist at present is simply
|
|
this that fringes of colors are produced by the interference of two portions of light ; and I think it will not be defied by the most prejudiced that the assertion is proved by the ex-
|
|
periments I am about to relate, which may be repeated with
|
|
great ease whenever the sun shines, and without any other apparatus than is at hand to every one.
|
|
Experiment 1. I made a small hole in a window-shutter, and covered it with a piece of thick paper, which I perforated with a fine needle. For greater convenience of observation I placed
|
|
a small looking-glass without the window-shutter, in such a position as to reflect the sun's light in a direction nearly horizontal upon the opposite wall, and to cause the cone of diverging light to pass over a table on which were several little screens of card-paper. I brought into the sunbeam a slip of
|
|
*From the Philosophical Transactions for 1804.
|
|
|
|
MEMOIRS ON THE WAVE-THEORY OF LIGHT
|
|
|
|
card about one-thirtieth of an inch in breadth, and observed
|
|
|
|
its shadow, either on the wall or on other cards held at differ-
|
|
|
|
ent distances. Besides the fringes of color on each side of
|
|
|
|
the shadow, the shadow itself was divided by similar parallel
|
|
fringes of smaller dimensions, differing in number according
|
|
to the distance at which the shadow was observed, but leaving
|
|
the middle of the-' shadow always white. Now these fringes
|
|
|
|
were the joint effects of the portions of light passing on each
|
|
|
|
side of the slip of card, and inflected, or rather diffracted, into
|
|
|
|
the shadow ;
|
|
|
|
for
|
|
|
|
a
|
|
|
|
little screen being
|
|
|
|
placed
|
|
|
|
a few inches
|
|
|
|
from the card so as to receive either edge of the shadow on
|
|
|
|
its margin, all the fringes which had before been observed in
|
|
|
|
the shadow on the wall immediately disappeared, although the
|
|
|
|
light inflected on the other side was allowed to retain its course,
|
|
|
|
and although this light must have undergone any modification
|
|
|
|
that the proximity of the other edge of the slip of card might
|
|
have been capable of occasioning. When the interposed screen
|
|
was more remote from the narrow card, it was necessary to plunge it more deeply into the shadow, in order to extinguish
|
|
|
|
the parallel lines ; for here the light diffracted from the edge of the object had entered farther into the shadow in its way towards the fringes. Nor was it for want of a sufficient in-
|
|
|
|
tensity of light that one of the two portions was incapable of
|
|
|
|
producing the
|
|
|
|
fringes
|
|
|
|
alone ;
|
|
|
|
for
|
|
|
|
when they were
|
|
|
|
both
|
|
|
|
unin-
|
|
|
|
terrupted, the lines appeared, even if the intensity was reduced
|
|
|
|
to one- tenth or one-twentieth.
|
|
|
|
Experiment 2. The crested fringes described by the ingenious
|
|
|
|
and accurate Grimaldi afford an elegant variation of the pre-
|
|
ceding experiment and an interesting example of a calcula-
|
|
tion grounded on it. When a shadow is formed by an object
|
|
|
|
which has a rectangular termination besides the usual external
|
|
|
|
fringes there are two or three alternations of colors, beginning from the line which bisects the angle, disposed on each side of it in curves, which are convex towards the bisecting line, and which converge in some degree towards it as they become more remote from the angular point. These fringes are also the joint effect of the light which is inflected directly towards the shadow from each of the two outlines of the object ; for if a screen be placed within a few inches of the object, so as to receive only one of the edges of the shadow, the whole of the fringes disappear ; if, on the contrary, the rectangular point
|
|
|
|
MEM OIKS ON
|
|
|
|
of the screen be opposed to the point of the shadow so as barely to receive the angle of the shadow on its extremity, the fringes will remain undisturbed.
|
|
|
|
II. COMPARISON OF MEASURES DEDUCED FROM VARIOUS EX-
|
|
PERIMENTS.
|
|
|
|
If we now proceed to examine the dimensions of the fringes under different circumstances, we may calculate the differences
|
|
|
|
of the lengths of the paths described by the portions of light which have thus been proved to be concerned in producing
|
|
those fringes ; and we shall find that where the lengths are
|
|
|
|
equal
|
|
|
|
the
|
|
|
|
light always
|
|
|
|
remains white ;
|
|
|
|
but
|
|
|
|
that where
|
|
|
|
either
|
|
|
|
the brightest light or the light of any given color disappears and reappears a first, a second, or a third time, the differences
|
|
|
|
of the lengths of the paths of the two portions are in arithmet-
|
|
|
|
ical progression, as nearly as we, can expect experiments of this
|
|
|
|
kind to agree with each other. I shall compare, in this point of view, the measures deduced from several experiments of
|
|
Newton and from some of my own.
|
|
|
|
In the eighth and ninth observations of the third book of
|
|
|
|
Newton's Optics some experiments are related which, together
|
|
|
|
with the third observation, will furnish us with the data neces-
|
|
sary for the calculation. Two knives were placed, with their
|
|
edges meeting at a very acute angle, in a beam of the sun's light, admitted through a small aperture, and the point of concourse of the two first dark lines bordering the shadows of the re-
|
|
|
|
spective knives was observed at various distances. The results
|
|
|
|
of six observations are expressed in the first three lines of the
|
|
first table. On the supposition that the dark line is produced
|
|
by the first interference of the light reflected from the edges of
|
|
|
|
the knives, with the light passing in a straight line between
|
|
them, we may assign, by calculating the difference of the two
|
|
|
|
paths, the interval for the first disappearance of the brightest
|
|
light, as it is expressed in the fourth line. The second table
|
|
contains the results of a similar calculation from Newton's ob-
|
|
|
|
servations
|
|
|
|
on the
|
|
|
|
shadow
|
|
|
|
of
|
|
|
|
a
|
|
|
|
hair ;
|
|
|
|
and
|
|
|
|
the
|
|
|
|
third,
|
|
|
|
from
|
|
|
|
some
|
|
|
|
experiments of
|
|
|
|
my own of the
|
|
|
|
same
|
|
|
|
nature ;
|
|
|
|
the
|
|
|
|
second
|
|
|
|
bright
|
|
|
|
line being supposed to correspond to a double interval, the sec-
|
|
ond dark line to a triple interval, and the succeeding lines to depend on a continuation of the progression. The unit of all
|
|
|
|
,the tables is an inch.
|
|
|
|
70
|
|
|
|
THE WAVE-THEORY OF LIGHT
|
|
|
|
TABLE I. Observation 9. N.
|
|
|
|
Distance of the knives from the aperture
|
|
|
|
101
|
|
|
|
Distance of the
|
|
|
|
paper from the knives
|
|
Distance b e -
|
|
|
|
1
|
|
|
|
^
|
|
|
|
&t
|
|
|
|
32
|
|
|
|
96
|
|
|
|
131
|
|
|
|
tween the
|
|
|
|
edges of the knives o p-
|
|
posite to the
|
|
point of concourse
|
|
|
|
012
|
|
|
|
.020
|
|
|
|
.034
|
|
|
|
.057
|
|
|
|
.081
|
|
|
|
.087
|
|
|
|
Interval of dis-
|
|
|
|
appearance
|
|
|
|
0000122 .0000155 .0000182 .0000167 .0000166 .0000166
|
|
|
|
TABLE II. Observation 3. N.
|
|
|
|
Breadth of the hair
|
|
|
|
Distance of the hair from the aperture Distances of the scale from the aperture (Breadths of the shadow Breadth between ihe second pair of bright lines
|
|
Interval of disappearance, or half the difference of the
|
|
|
|
paths
|
|
|
|
Breadth between the third pair of bright lines
|
|
|
|
. ..
|
|
|
|
Interval of disappearance, one-fourth of the difference..
|
|
|
|
^
|
|
|
|
144
|
|
|
|
150
|
|
|
|
252
|
|
|
|
^
|
|
|
|
)
|
|
|
|
4
|
|
|
|
-g?
|
|
|
|
TT
|
|
|
|
0000151 .0000173
|
|
|
|
^
|
|
|
|
3
|
|
T
|
|
|
|
.0000130 .0000143
|
|
|
|
TABLE III. Experiment 3.
|
|
Breadth of the object Distance of the object from the aperture Distance of the wall from the aperture Distance of the second pair of dark lines from each other Interval of disappearance, one-third of the difference
|
|
|
|
434 125 250 1.167 0000149
|
|
|
|
Experiment 4.
|
|
|
|
Breadth of the wire
|
|
|
|
083
|
|
|
|
Distance of the wire from the aperture
|
|
|
|
32
|
|
|
|
Distance of the wall from the aperture
|
|
|
|
250
|
|
|
|
(Breadth of the shadow, by three
|
|
|
|
measurements
|
|
|
|
815.
|
|
|
|
.826, or
|
|
|
|
.827 ;
|
|
|
|
mean,
|
|
|
|
.823)
|
|
|
|
Distance of the first pair of dark lines 1.165, 1.170, or 1.160; mean, 1.165
|
|
|
|
Interval of disappearance ..........
|
|
|
|
0000194
|
|
|
|
Distance of the second pair of dark
|
|
|
|
lines
|
|
|
|
1.402. 1.395, or 1.400; mean. 1.399
|
|
|
|
Interval of disappearance Distance of the third pair of dark
|
|
|
|
0000137
|
|
|
|
lines. ,
|
|
Interval of disappearance
|
|
|
|
1.594,
|
|
|
|
1.580,
|
|
|
|
or
|
|
|
|
1.585 ;
|
|
|
|
mean,
|
|
|
|
1.586
|
|
|
|
0000128
|
|
|
|
71
|
|
|
|
MEMOIRS ON
|
|
|
|
It appears, from five of the six observations of the first
|
|
|
|
table, in which the distance of the shadow was varied from
|
|
|
|
about 3 inches to 11 feet, and the breadth of the fringes was
|
|
|
|
increased in the ratio of 7 to 1, that the difference of the
|
|
|
|
routes constituting the interval of disappearance varied but
|
|
|
|
one-eleven tli at most and that in three out of the five it ;
|
|
|
|
agreed with the mean, either exactly or within y^- part.
|
|
|
|
Hence we are warranted in inferring that the interval appro-
|
|
|
|
priate to the extinction of the brightest light is either accu-
|
|
|
|
rately or very nearly constant.
|
|
|
|
But it may be inferred from a comparison of all the other
|
|
|
|
observations that when the obliquity of the reflection is very
|
|
|
|
great some circumstance takes place which causes the inter-
|
|
|
|
val thus calculated to be somewhat greater ; thus, in the elev-
|
|
|
|
enth line of the third table it comes out one-sixth greater than
|
|
the mean of the five already mentioned. On the other hand,
|
|
|
|
the mean of two of Newton's experiments and one of mine is
|
|
|
|
a result about one-fourth less than the former. With respect
|
|
|
|
to the nature of this circumstance I cannot at present form a
|
|
|
|
decided opinion ; but I conjecture that it is a deviation of
|
|
|
|
some of the light concerned, from the rectilinear direction as-
|
|
|
|
signed to it, arising either from its natural diffraction, by which
|
|
|
|
the magnitude of the shadow is also enlarged, or from some
|
|
|
|
other unknown cause. If we imagined the shadow of the
|
|
|
|
wire and the fringes nearest it to be so contracted that the
|
|
|
|
motion of the light bounding the shadow might be rectilinear,
|
|
|
|
we should thus make a sufficient compensation for this devia-
|
|
|
|
tion ;
|
|
|
|
but
|
|
|
|
it is
|
|
|
|
difficult to
|
|
|
|
point
|
|
|
|
out what
|
|
|
|
precise track
|
|
|
|
of
|
|
|
|
the
|
|
|
|
light would cause it to require this correction. The mean of the three experiments which appear to have been
|
|
|
|
least affected by this unknown deviation gives .0000127 for the
|
|
|
|
interval appropriate to the disappearance of the brightest
|
|
|
|
light ; and. it may be inferred that if they had been wholly ex-
|
|
|
|
empted from its effects the measure would have been some-
|
|
what smaller. Now the analogous interval, deduced from the
|
|
|
|
experiments of Newton on this plate, is .0000112, which is
|
|
|
|
about one-eighth less than the former result ; and this appears
|
|
|
|
to be a coincidence fully sufficient to authorize us to attribute
|
|
|
|
these two classes of phenomena to the same cause. It is very
|
|
|
|
easily shown, with respect to the colors of thin plates, that
|
|
|
|
each kind of light disappears and reappears where the differ-
|
|
|
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72
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THE WAVE-THEORY OF LIGHT
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ences of the routes of two of its portions are in arithmetical
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progression*} and we have seen that the same law may be in general inferred from the phenomena of diffracted light, even
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independently of the analogy.
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The distribution of the colors is also so similar in both cases
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as to point immediately to a similarity in the causes. In the
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thirteenth observation of the second part of the first book
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Newton relates that the interval of the glasses where the rings
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appeared in red light was to the interval where they appeared in
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violet light as
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14 to
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9 ;
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and,
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in
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the
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eleventh
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observation
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of the
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third book, that the distances between the fringes, under the
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same circumstances, were the twenty-second and the twenty-sev-
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enth of an inch. Hence, deducting the breadth of the hair and
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taking the squares, in order to find the relation of the difference
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of the routes, we have the proportion of 14 to 9, which scarcely
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differs from the proportion observed in the colors of the thin
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plate.
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We may readily determine from this general principle the
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form
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of
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the
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crested fringes
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of
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Grimaldi,
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already
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described }
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for
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it will appear that, under the circumstances of the experiment
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related, the points in which the differences of the lengths of
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the paths described by the two portions of light are equal to
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a constant quantity, and in which, therefore, the same kinds
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of light ought to appear or disappear, are always found in
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equilateral hyperbolas, of which the axes coincide with the
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outlines of the shadow, and the asymptotes nearly with the
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diagonal line. Such, therefore, must be the direction of the
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fringes ; and this conclusion agrees perfectly with the observa-
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tion. But it must be remarked that the parts near the out-
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lines of the shadow are so much shaded off as to render the
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character of the curve somewhat less decidedly marked where it approaches to its axis. These fringes have a slight resemblance to the hyperbolic fringes observed by Newton ; but the
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analogy is only distant.
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[///. Application to the Supernumerary Rainbows, omitted.]
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IV. ARGUMENTATIVE INFERENCE RESPECTING THE NATURE
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OF LIGHT.
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The experiment of Grimaldi on the crested fringes within
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the shadow, together with several others of his observations
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73
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MEMOIRS ON
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equally important, has been left unnoticed by Newton. Those
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who are attached to the Newtonian theory of light, or to the
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hypothesis of modern opticians founded on views still less
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enlarged, would do well to endeavor to imagine anything like
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an explanation of these experiments derived from their own
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doctrines ;
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and if they fail in
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the
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attempt, to
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refrain
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at
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least
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from idle declamation against a system which is founded on
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the accuracy of its application to all these facts, and to a thou-
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sand others of a similar nature.
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From the experiments and calculation which have been premised, we may be allowed to infer that homogeneous light
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at certain equal distances in the direction of its motion is pos-
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sessed of opposite qualities capable of neutralizing or destroy-
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ing each other, and of extinguishing the light where they happen to be united; that these qualities succeed each other
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alternately in successive concentric superficies, at distances
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which are constant for the same light passing through the
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same medium. From the agreement of the measures, and from the similarity of the phenomena, we may conclude that these
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intervals are the same as are concerned in the production of the
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colors of thin plates ; but these are shown, by the experi-
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ments of Newton, to be the smaller the denser the medium;
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and since it may be presumed that their number must neces-
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sarily remain unaltered in a given quantity of light, it follows, of course, that light moves more slowly in a denser than in a rarer medium'; and this being granted, it must be allowed that
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refraction is not the effect of an attractive force directed to a
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denser medium. The advocates for the projectile hypothesis
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of light must consider which link in this chain of reasoning they may judge to be the most feeble, for hitherto I have advanced in this paper no general hypothesis whatever. But since we know that sound diverges in concentric superficies,
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and that musical sounds consist of opposite qualities, capable of neutralizing each other, and succeeding at certain equal
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intervals, which are different according to the difference of the note, we are fully authorized to conclude that there must be some strong resemblance between the nature of sound and
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that of light. I have not, in the course of these investigations, found any
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reason to suppose the presence of such an inflecting medium
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in the neighborhood of dense substances as I was formerly
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74
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THE WAVE-T11EOKY OF LIGHT
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inclined
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to attribute to them ;
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and,
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upon considering the
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phe-
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nomena of the aberration of the stars, I am disposed to believe
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that the luminiferous ether pervades the substance of all ma-
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terial bodies, with little or no resistance, as freely, perhaps, as
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the wind passes through a grove of trees.
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The observations on the effects of diffraction and inter-
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ference may, perhaps, sometimes be applied to a practical pur-
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pose in making us cautious in our conclusions respecting the
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appearances of minute bodies viewed in a microscope. The
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shadow of a fibre, however opaque, placed in a pencil of light
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admitted through a small aperture, is always somewhat less dark
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A in the middle of its breadth than in the parts on each side.
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similar effect may also take place, in some degree, with respect
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to the image on the retina, and impress the sense with an idea
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of a transparency which
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has
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no
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real
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existence ;
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and if a
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small
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portion of light be really transmitted through the substance,
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this may again be destroyed by its interference with the dif-
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fracted light, and produce an appearance of partial opacity,
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instead of uniform semi-transparency. Thus a central dark spot
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and a light spot, surrounded by a darker circle, may respec-
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tively be produced in the images of a semi-transparent and
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an opaque corpuscle, and impress us with an idea of a com-
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plication of structure which does not exist. In order to detect
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the fallacy, we make two or three fibres cross each other, and
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view a number of globules contiguous to each other; or we
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may obtain a still more effectual remedy by changing the mag-
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nifying power; and then, if the appearance remain constant in
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kind and in degree, we may be assured that it truly represents
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the nature of the substance to be examined. It is natural to
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inquire whether or not the figures of the globules of blood
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delineated by Mr. Hewson in the Phil. Trans., vol. Ixiii., for
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1773, might not in some measure have been influenced by a
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deception
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of
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this
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kind ;
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but,
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as
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far
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as
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I have
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hitherto
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been
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able
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to examine the globules with a lens of one-fiftieth of an inch
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focus, I have found them nearly such as Mr. Hewson has de-
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scribed them.
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[ V. Remarks on the Colors of Natural Bodies, omitted.]
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VI. EXPERIMENT ON THE DARK RAYS OF RITTER
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Experiment 6. The existence of solar rays accompanying light, more refrangible than the violet rays and cognizable by
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75
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MEMOIRS ON
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their chemical effects,
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was first ascertained by Mr.
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Bitter ;
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but
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Dr. Wollaston made the same experiments a very short time
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afterwards without having been informed of what had been
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done on the Continent. These rays appear to extend beyond
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the violet rays of the prismatic spectrum, through a space
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nearly equal to that which is occupied by the violet. In order
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to complete the comparison of their properties with those of
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visible light, I was desirous of examining the effect of their re-
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flection from a thin plate of air, capable of producing the well-
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known rings of colors. For this purpose I formed an image
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of the rings, by means of the solar microscope, with the appa-
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ratus which I have described in the Journals of the Royal
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Institution, and I threw this image on paper dipped in a solu-
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tion of nitrate of silver, placed at the distance of about nine
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inches from the microscope. In the course of an hour portions
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of three dark rings were very distinctly visible, much smaller
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than the brightest rings of the colored image, and coinciding
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very nearly in their dimensions with the rings of violet light
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that appeared upon the interposition of violet glass. I thought
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the dark rings were a little smaller than the violet rings, but
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the difference was not sufficiently great to be accurately ascer-
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tained ;
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it might
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be
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as
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much
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as fa or fa of
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the
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diameters,
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but
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not greater. It is the less surprising that the difference should
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be so small, as the dimensions of the colored rings do not by
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any means vary at the violet end of the spectrum so rapidly as
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at the red end. For performing this experiment with very
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great accuracy a heliostat would be necessary, since the motion
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of the sun causes a slight change in the place of the image ;
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and leather impregnated with the muriate of silver would
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indicate the effect with greater delicacy. The experiment,
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however, in its present state, is sufficient to complete the anal-
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ogy of the invisible with the visible rays, and to show that they
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are equally liable to the general law which is the principal sub-
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ject of this paper. If we had thermometers sufficiently delicate,
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it is probable that we might acquire, by similar means, infor-
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mation still more interesting with respect to the rays of invis-
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ible
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heat
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discovered
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by Dr.
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Herschel ;
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but
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at
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present
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there is
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great reason to doubt of the practicability of such an experi-
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ment.
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76
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THE WAVE-THEORY OF LIGHT
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BIOGRAPHICAL SKETCH
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THOMAS YOUNG was born at Milverton. England, in 1773,
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and died at London in 1829. His education, in respect to the amount of ground it co.vered, is quite as remarkable as his later scientific work. As a lad he showed marked proficiency in
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linguistic studies, acquired great mechanical skill, distin-
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guished himself in drawing, music, and athletics. As a young man he pursued his university studies at London, Edinburgh, Gb'ttingeu, and Cambridge.
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The following programme of his daily work at Gottingen in the autumn of 1795 characterizes at once the lad, the youth, and the mature man:
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" At 8, I attend Spittler's course on the History of the Principal States of Europe, exclusive of Germany.
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" At 9, Arnemann on Materia Medica. "At 10, Richter on Acute Diseases. " At 11, twice a week, private lessons from Blessman, the academical
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dancing-master.
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"At 12, I dine at Ruhlander's table d'hote. "At 1, twice a week, lessons on the clavichord from Forkel; and twice a week at home, from Fiorillo on Drawing. " At 2, Lichtenberg on Physics. "At 3, I ride in the academical manege, under the instruction of Ayrer,
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four times a week. " At 4, Stromeyer on Diseases. *' At 5, Blumenbach on Natural History.
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"At 6, twice Blessman with other pupils, and twice Forkel."
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He was born of a well-to-do Quaker family; he inherited
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ample money ; he had all that travel, leisure, and good society could do for a man. Only in one particular does his education appear to have been defective viz., in the absence of any training in advanced dynamics or in higher mathematical
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analysis.
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In 1800 he completed his medical studies at Cambridge, and settled as a practising physician in London. In the year following he was appointed to the professorship of natural philosophy in the then newly founded Royal Institution, a position from which he resigned at the end of two years in order to devote himself more completely to the practice of medicine. It was during his occupancy of this chair that he published the
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77
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MEMOIRS ON THE WAVE-THEORY OF LIGHT
|
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three papers reprinted in this volume, the first of which is possibly the most important of his contributions to physics. It was during this period also that he wrote his Lectures on Natural Philosophy, which must always be reckoned as a potent factor in the spread of sound physical science in the nineteenth century, while its bibliography of more than four hundred quarto pages is to-day valuable as well as classic.
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But nothing short of a catalogue of his papers can give one an adequate idea of the varied activity of this man during the remaining quarter-century of his life. His contributions cover
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fields as diverse as the physiology of the human eye, hydro-
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dynamics, music, paleography, atmospheric refraction, theory of tides, tables of mortality, theory of structures. His explanation of color-vision as due to the presence of three sets of
|
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nerve fibres in the retina, which, when excited, give respectively sensations of red, green, and violet, has been adopted and modified by Helmholtz, and is to-day perhaps the most widely accepted of the various theories on this subject.
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After all, it rnnst^ be confessed, even by his most ardent admirers, that Young's style is, in general, far from clear. Whether this is in any way connected with his lack of mathematical training, or whether it is due to the fact that his own clear intuitions bridged most of the gaps in his written work,
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it is difficult to say ; but in any event many of his papers are obscure, and few of them are read. The reader who desires a
|
|
full biography will find it in Dr. Peacock's Life of Young (London, 1855). This biographer also edited his Miscellaneous Works, 3 vols. (London, 1855). All his papers, however, which
|
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are of especial interest to the student of physics are contained in the lectures on Natural Philosophy (London, 1807).
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78
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