1349 lines
64 KiB
Plaintext
1349 lines
64 KiB
Plaintext
Title: SCIENTIFIC ABSTRACT PYASKOVSKAYA-FESENKOVA, YE. V. -
|
||
Subject: SCIENTIFIC ABSTRACT PYASKOVSKAYA-FESENKOVA, YE. V. -
|
||
Keywords: ~
|
||
3c!-,tt--~riar
|
||
1 Ja n 53
|
||
I "So-le ProT:ia!-ties- of Atmosrheric I-Idicatz-1-c-2z of Lirrhtu Sca I Ye.v.
|
||
|
||
|
||
|
||
|
||
|
||
|
||
|
||
|
||
Name: PYASKOVSKAYA-FESENKOVA, Y
|
||
|
||
307
|
||
PHASE I BOOK MWITATION
|
||
Pyaskovskaya-Fesenkova, Ye. V.
|
||
Issledovaniye rasseyaniya avets v zesnoy stmosfere (Investigation of Light Scatter-
|
||
ing In the Earth's Atmosphere) Moscav, Izd-vo AN SSSR, 1957. 21T p. 2,500,
|
||
copies printed.
|
||
Sponsoring Agency: Akademlya nauk'SOM.
|
||
Resp. Ed.: Fesenkov, V. G.; Ed. of Publishing House- Yefigemovs Yu. I.-
|
||
Tech. Ed.: Klseleva, A. A.,
|
||
PURPOSE- The book presents advances made In the study of light scattering In
|
||
terrestrial atmosphere and is directed to.the specialist in the field.
|
||
COVERAGE: This book in a theoretical study of the optics of terrestrial atmosphere
|
||
and is supplemented vith observations of the brightness of the daylight
|
||
sky conditioned by molecular and sex4mol scattering of light. A now
|
||
method is proposed for the derivation of the scattering Indicatrix from
|
||
the calculation of multiple light scattering in the atmosphere.
|
||
Card 1/4
|
||
|
||
Investigation of Light Scattering in the Earth's Atmosphere 307
|
||
V. G. Fesenkov's criterion of stability of the optical rties of atmosphere
|
||
is refined and expanded. The author discusses his proposed methods for
|
||
determining the atmospheric transparency coefficient and the brightness of the
|
||
daylight sky. Observations of sky brightness vere performed by: N. N. Kalitin,
|
||
G. A. Tikhov, V. G. Fesenkov (Astrophysical Observatory at XUchino
|
||
"Astrofizicheskaya. observatoriya v Kuehino pod Moskyoy"); V. A. Krat (Tashkent);
|
||
V. V. Sobolev and Ye. H. Yustova (Yelabuga); V. N. Yamalayto" (Tashicent);
|
||
G. Sh. Livehits (Alm-AU); Ye. V. Pyukovikaya-Yesenkova; L. V. Fesenkava;
|
||
A. P. 1(utyreva; T. P. Toropova; V. M. Kazachevskiy; P. N. Boyko; and
|
||
N. I. Oychlinnikova. The author made visual-photometry observations at different
|
||
places varying in elevation (h): Gudauta, Caucasian shore of the Black Sea
|
||
(h = 3m.); a state faru near Pugachersk (h = 100m.); Orlinaya gors at
|
||
Vla(Uvostok (h = 144m.); sanatorium "Tzkor" near Moscow (hw 150A.); village
|
||
of Bogorodsoye near Ivanovo (h = 150A.); Saq-lshik-Ortau Desert, Southern
|
||
Pribalkhash (h = Won.); 51khote-Alin' (b 6oon.); Almia-Ata Observatory
|
||
(h = 1450m.); shore of lasyk-Null Lake (h 1600m.); Kislovodsk Astronomical
|
||
Station of the GM AN SSSR (h = 2130m.), and Kumbell Mountain near Almis,-Ata
|
||
(h = 3140m.). Other personalities mentioned: G. Sh. Lifshits, K. N. Shistovskiy,
|
||
Kh. A. Abishev, X. P. Pervertyn, V. B. Nikonar, V. G. K"trov, Ye. S. Kuznetsov,
|
||
and V. V. Ovehinakiy. There are 106 figures, 65 tables, and 104 references,
|
||
77 of vhich are Soviet, 9 USA, 2 British, and 1 Polish.
|
||
C ar& 2/4
|
||
|
||
Investigation of Light Scattering in the Earth's Atmosphere 307
|
||
TABU OF
|
||
CONEM: Introduction3
|
||
Ch. 1. Fundamental Concepts and Definitions7
|
||
1. Weakening of light Intbe GtmO~Pb8rO7
|
||
2. Scattering of.ligbt in the atmospbere32
|
||
Ch. 2. Apparatus and Methodology of Observations16
|
||
1. Daylight-sky photometer16
|
||
2. Aureole photometer19
|
||
3- Determination of effective Va. length$24
|
||
4. Accuracy of measurements28
|
||
Ch. 3. BrIghtness.of the Blue Daylight Sky33
|
||
1. Formula for.the brightness of the blue sky with
|
||
consideration of first order scattering =A certain
|
||
deductions fran this formils.33
|
||
Card 3/4
|
||
|
||
Investigation of Light Scattering in the Earth's Atmosphere 307
|
||
2. Observed brightness of the blue dayllght sky41
|
||
3. Formula for sky brightness vith consideration of multiple
|
||
light scattering and collation of the formila with
|
||
observational data91
|
||
''Ch. 4. Indiestrix of Light Scattering in the Atmosphere
|
||
Ch. 5. calculation of Multiple Ll&t Scattering166
|
||
ch. 6. criterion for the Stability of Optical Properties of the
|
||
Atmosphere185
|
||
Ch. 7- Methods for Deter-in' the AtuDsoeric Cleamss Coefflelent
|
||
from the Blue-sky Brightness200
|
||
conclusion215
|
||
Bibliogm]phy217
|
||
AVAnABW: Library,of Congms
|
||
Card 4/4
|
||
|
||
AUTHOR: Kirillov, F.A. 49-12-15/16
|
||
TITLE: Dissertations Defended in the Scientific Council of the
|
||
Institute of Physics of the Earth, Institute of Physics of the
|
||
AtmosDhere and Institute of Applied Geophysics Ac Sc USSR during
|
||
t9e First Semester of 195T (Dissertatsii, zashchiZch;nn~e v uchenom
|
||
sovete iastituta fiziki zemli, instituta fiziki atmosfery i
|
||
instituta prikladnoy geofiziki AN SSSR za pervoye polugodiye 1957)
|
||
PERIODICAL: Izvestiya Akademii Nauk SSSR, Seriya Geofizicheska a,
|
||
195?, No.12t PP. 1532 - 1536 (USSR~
|
||
ABSTRACT: 'Ye.S. Borisevich - Magneto-electric Oscillogra
|
||
erimen-t-a-l-G-e-o-pffy--sl-c-a=nvestigations (Magnitoelektricheskiye
|
||
ostsillografy dlya.eksperimentallnykh geofizicheskikh i.2-,sledovaniy)
|
||
Doctor dissertation. Opponents: Corresponding Memberof the Ac.Sc.
|
||
USSRI.M.A..Sadovskiy, Doctor of Physico-Mathematical Sciences,
|
||
D.P,Kirnos, Doctor of Technical Sciences, G.L. Shnirman.May 10,195?.
|
||
In the dissertation, the design was briefly reviewed of 16 various
|
||
models of oscillographs for experimental, geophysical investigations
|
||
which were developed by the author or under his direction. Some of
|
||
these are series-manufactures and apply also in other branches of
|
||
science and engineering. Particular attention is devoted to the
|
||
design of the individual assemblies of the oscillographs. Standard
|
||
assemblies include typer 6 galvanometers, mounted into blocks
|
||
Card
|
||
V21 with permanent magnets, galvanometer illumination time markers,
|
||
|
||
49-12-15/16
|
||
Dissertations Defended in the Scientific Council of the Institute of
|
||
of the Earth, Institute of Physics of the Atmosphere and
|
||
Institute of Applied Geophysics.Ac.Se. USSR during the First
|
||
Sek#Wt~~r-of 1957.
|
||
compact gear boxes with swivel-mounted sectors, spring-powered
|
||
engines, speed regulators. All the oscillographs developed by
|
||
the Institute of Physics of the Earth, which is pioneering in this
|
||
field in the Soviet Union, can.be sub-divided into the following
|
||
three groups: oscillographs for recording short-duration processes
|
||
with high speeds of the film; oscillographs for recording long-
|
||
duration of occasional processes at relatively low speeds of the
|
||
filih~ strip; universal oscillographs for recording various proces-
|
||
ses within a wide range of speeds of the film strip. Oscillographs
|
||
intended for recording long-duration and occasional phenomena
|
||
(earthquakes) and designed for recording with a speed of 0.1 to
|
||
2 cm/sec for moving the film; spring-operated mechanisms proved
|
||
advantageous in this case and therefore it was necessary to develop
|
||
special speed-regulators. The presence of spring-operated
|
||
mechanisms and galvanometers grouped into a block with a common
|
||
Card permanent magnet enabled reducing parasitic influences on the
|
||
2/21 metering circuit and also reducing to a
|
||
|
||
49-12-15/16
|
||
Dissertations Defended in the Scientific Council of the Institute of
|
||
Physics of the 'Earth, Institute of Physics of the Atmosphere and
|
||
Instituteof Applied Geop hysicsAc.Sc. USSR during the First
|
||
Semesterof 1957.
|
||
minimum the power consumption of the oscillographwhich is
|
||
particularly important in regions with difficult access.
|
||
Universal, portable oscillographs represent the widest group
|
||
amongst oscillographs produced in the Institute;: they are
|
||
small and light and therefore convenient for expeditions; they
|
||
are suitable not only for recording geophysical, but any other
|
||
phenomena which can be.transformed into an electric current or,
|
||
voltage. The oscillographs rkO&-14 M, MG-12 M and iIC05-9 are
|
||
among the best produced in the Soviet Union as well as in other
|
||
countries. The developed, fundamental, typical assemblies and
|
||
unification of the main circuits enabled rationalising the
|
||
designof the oscillographs and also simplifying and covering
|
||
the cost of the development and manufacture of new mo*ls adapted
|
||
for given conditions. First, the author tonsiders the method
|
||
of calculation of the basic elements of the oscillographs which
|
||
he has developed; all the calculations were tested by practical
|
||
experience and are effe4c~tdd by formulae which are convenient
|
||
or practical use. ror simplifying the calculations, nomograms,
|
||
Card3/2f
|
||
|
||
49-12-15/16
|
||
Dissertations Defended in the Scientific uouncil of the Institute of
|
||
Physics.of the Earth, Institute of Physics of the Atmosphere and
|
||
Institute of j[pplied Geophysics..Ac.Sc. USSR during the First
|
||
Seme.ster of 1957.
|
||
data tables and examples are included. A fundamentally-new
|
||
metering system was created; a high-frequency, frame galvan-
|
||
ometer with a ",continuous extension (pull)" and a method of
|
||
calculation is presentedfcr the type of galvanometer, giving
|
||
results of experimental investigations which indicate the possi-
|
||
bility of achieving a sensitivity,exceeding that of loops. The
|
||
conditions of optimum electro-magnetic and liquid damping of
|
||
frame galvanometers were investigated. The calculation is
|
||
presented of the kinematics of oscillographs and of film adaptors
|
||
and the phenomenon of shock was considered when switching on
|
||
film adaptors designed for high speeds. Formulae are derived
|
||
which permit calculation of the impact force and of the time
|
||
necessary for reaching a given speed. A new type of simple,
|
||
compact and reliable gear box was developed and the method of
|
||
its calculation evolved. Other mechanisms were also considered,
|
||
,intended for stepped and stepless speed changes and used for
|
||
oscillographs. A method of calculation is proposed of spring-
|
||
Gard4/21operated mechanisms for 0scillographs aiming at achieving maximuv
|
||
|
||
49-12-15/16
|
||
Dissertations Defended in the Scientific Council of the 1nstitute of
|
||
Physics of the Earth, Institute of Physics of the Atmosphere and
|
||
Institute of Applied Geophysics..Ac.Sc. USSR during the First
|
||
Semester of 1957.
|
||
useful work from the energy stored in the springs. The problem
|
||
is considered of ensuring uniform movement of the film strip
|
||
and various designs were developed of speed regulators with
|
||
low-rated r.p.m. which are capable of.taking up a considerable
|
||
excess moment generated by the springs. A method of calcul-
|
||
ation is presented of a radial-action, centrifugal regulator.
|
||
All the.described oscillographs were used in geophysical
|
||
investigations, i.e. in studying the physics of earthquakes
|
||
by systematic,recording of weak, local tremors, development of
|
||
a new method of deep seismic-sounding of the Earth's crust,
|
||
study of the vibrations of soils and of.buildings caused by
|
||
explosions and earthquakes, development of new, progressive
|
||
methods of seismic and electro-magnetic prospectingof minerals
|
||
study of atmospheric phenomena, etc. The oscillographs
|
||
developed by the author are widely used, not only for geo-
|
||
physical investigations, but also in scientific establishments
|
||
and undertakings of various ministries and the manufacture of
|
||
,.rd0ke5e instruments does not satisfy requirements.
|
||
|
||
49-12-15/16
|
||
Dissertations Defended in the Scientific Council of the Institute of
|
||
Physics of the Earth, Institute of Physics of the Atmosphere and
|
||
Institute of Applied GeophysicsAc.Sc. USSR during the First
|
||
Semester of 1957.
|
||
Ye.V. Pyaskovskaya-Fesenkova - Investigation of the Scatterina
|
||
re (Issiedovanlye rasseyan-lya
|
||
sveta v zemnoy atmosfere) - Doctor dissertation. Opponents:
|
||
Doctor of Physico-Mathematical Sciences Ye.S. Kuznetsov,
|
||
Doctor of Physico-Mathematical Sciences S.M. Polozkov, Doctor
|
||
of Physico-Mathematical Sciences G.B. Rozenberg, Doctor of
|
||
Physico-Mathematical Sciences I.S. Shklovskiy. March 23, 1957.
|
||
The dissertation represents the result of many years of study
|
||
of the clear, daytime sky.- The observations were carried out
|
||
in twelve locations at various altitudes above the sea,
|
||
various climatic, meteorological and synoptic conditions. The
|
||
observations were carried out mainly during high-transparency
|
||
of the atmosphere in the visual raiEp of the spectrum in the
|
||
absence of asnow cover. In the investigations 'two instru-
|
||
ments,designed by V.G. Fesenkov were used; one of these was a
|
||
visual photometer of the daytime sky intended for measuring
|
||
the brightness of the firmament; the other was a photo-
|
||
Uard6/21 electric halo photometer for determining the brightness from
|
||
|
||
49-12-15/16
|
||
Dissertations Defended in the Scientific Council of the Institute of
|
||
Physics of the Earth, Institute of Physics of the Atmosphere and
|
||
Institute of Applied GeophysicsAc-Sc. USSR during the First
|
||
Semester of 1957.
|
||
near-sun halo and also from the sun on a surface perpendiciilar
|
||
to these rays. The dissertation contains a certain formula
|
||
of the brightness of the sky,taking into consideration only
|
||
the brightness of the first order and derived on the assumption
|
||
of a,"flat" Earth ahd giving some conclusions derived on the
|
||
basis of this formula. For a certain coefficient, of trans-
|
||
parency of the atmosphere, the brightness of the sky at any
|
||
point is represented by derivation of two functions of which
|
||
one is the function of the diffubian of light and the other is a
|
||
function of the zenith distances of.the.sun and of the observed
|
||
point of the sky. Og changing of the zenith distances of the
|
||
sun z from 90 to 0 , the brightness of the sky on the
|
||
almucantar of the sun increases firstj reaching a maximum for
|
||
a certain value of z and then decreases. A method is also
|
||
proposed of determining the brightness of the clear daylight
|
||
sky at any point based on measuring the brightness along the
|
||
almucantar of the sun and of 5-6 points of the firmament located
|
||
at various zenith'.distances. This method permits determination
|
||
Card7/21
|
||
|
||
49-12-15/16
|
||
Dissertations Defended in The Scientific Council of the Institute of
|
||
Physics of the Earth, Institute of Physics of the Atmosphere and
|
||
Institute of Applied Geophysics,Ac.Sc. USSR during the First
|
||
Semester of 1957,
|
||
of the brightness at any other point from the observed bright-
|
||
ness of the sky. The'method consists essentially af excluding
|
||
from -the observed brightnesses local indicatrices of ft (WTus]Dn
|
||
and introducing another one which relates to the-spot where
|
||
it is desired to determine the brightness of the sky; for
|
||
this purpose, it is necessary to measure.at that point the
|
||
brightness of the sky along the almutantar of the sun. A
|
||
necessary condition thereby is 'that the transparency coeffic-
|
||
ients of the atmosphere be equ. 1 in both points. The theoret-
|
||
a i
|
||
ical brightness was also considered, taking into.consideration
|
||
the multiple scattering of light in the case of a spherical
|
||
indicatrix of scattering and a comparison is made of this
|
||
brightness with the one observed at an angular distance of the
|
||
sun of 57 - 60 For solving the integral equation of the
|
||
theory of the diffusion of light, the approximate method of
|
||
Ye-S. Kuznetsov was used which proved sufficiently accurate.
|
||
Diffusi'on indicatrices are given in the dissertation which
|
||
Oard8/23wer-e obtained from observations of the brightness of the sky.
|
||
|
||
49-12-15/16
|
||
Dissertations Defended in the Scientific (;ouncil of the Institute of
|
||
Physics of the Earth, Institute of Physics of the Atmosphere and
|
||
Institute of Applied Geophysics.,Ac.Sc. USSR during the First
|
||
Semester of 1957.
|
||
calculated for the entire height of the atmosphere. Itis
|
||
.shown that there is no w4ll-deflned relation between the coeff-
|
||
icient of scattering iL for small scattering angles j& and
|
||
the coefficient of transparency or, respectively,-the optical
|
||
thickness of the atmosphere. Such a well-deCined dependence
|
||
does exist for diffusion angles oapproaching 60u. Thus, the
|
||
diffusion of light near -4 = 60 does not-depend on the prop-
|
||
erties of the d if fus ion particles. It is shown that the
|
||
diffusion of light ih the Earth's atmosphere cannot be attrib-
|
||
uted to a medium particle with some definite effective radius.
|
||
The effective radius of the diffusion particle changes with
|
||
the difftLsion angle. The dependence of the diffusion of light
|
||
in the gar~hls atmosphere on the wavelength for the visual part
|
||
of the spectrum can be expressed by the relation A = c%-n I
|
||
representing a generalisation of the known&VIdgh formula where
|
||
.n ), 0 and independent of the wavelength for all angular
|
||
distances of the,,sun, provided the.dust content of the atmosphere,
|
||
is not high. If that is not the case, this relation is dis-
|
||
(;ard9/21 turbed and becomes somewhat complicated for small angular
|
||
|
||
49-12-15/16
|
||
Dissertations Defended in the Scientific Council of the Institute of
|
||
Physics of the.Earth, Institute of Physics of the Atmosphere and
|
||
Institute of Applied GeophysicsjAc.Sc. USSR during the First
|
||
Semester of 1957.
|
||
distances to the sun (the halo surrounding the sun); the
|
||
number n, is dependent on the wavelength and in some parts of
|
||
the spectrum may become negative. This explains thevarious
|
||
colour shadings of the halo surrounding the sun. A method is
|
||
proposed of determining the indicatrix of the atmosphere which
|
||
is not affected by the influence of the multiple diffusion of
|
||
light. This method permits obtaining the indicatrix solely from
|
||
the observed data andconsists in determining by two differing
|
||
methods the optical thickness of the atmosphere. One method
|
||
gives optical thickness 1-1 on the basi's of measurement of the
|
||
direct solar radiation and is therefore not dependent on the
|
||
multiple diffu sion of light. In the other method, the optical
|
||
thickness is determined by measuring the brightness of the sky
|
||
and, consequently, is influenced by the multiple diffusion..
|
||
The difference between these gives an increase in the optical
|
||
thickness of the atmosphere which depends on the multiple
|
||
d4f f usio n of light, i. e. of the d iff u s ion in all directions
|
||
(;ardlO/21:)f,the light flux caused by diffusion of higher orders relative
|
||
|
||
49-12-15/16
|
||
Dissertations Defended in the Scientific Council of the Institute of
|
||
~Physics of the Earth, Institute of Physics of the Atmosphere and
|
||
Institute of Applied Geophysics,Ac-Sc. USSR during the Pirst
|
||
Semester of 1957.
|
||
to the incident light flux. The author gives the formula of the
|
||
brightness of the sky, taking into consideration the multiple
|
||
diffusion and also the light reflected from the underlying
|
||
surface. The problem of stability of optical properties of the
|
||
atmosphere was -considered and existing stability criteria were
|
||
supplemented and improved by the author. It is shown, too, that
|
||
the ratio of the brightness of the sky at any point of the
|
||
almucantar of the sun to the illumination from the sun.also
|
||
gives a linear dependence on the atmosphere mass and consequently
|
||
can serve as a criterion of stability of the optical properties
|
||
of the atmosphere. rinally, methods are.described of determin-
|
||
ation of coefficients of transparency of the atmosphere from the
|
||
brightness of a clear sky, namely: a method based on the
|
||
instant of maximum brightness of the halo surrounding the sun;
|
||
a method based on the indicatrix of d if f us ion of light in the
|
||
atmosphere; a method of determining the coefficient of trans-
|
||
parency on the basis of empirical formulae.
|
||
uard 11/21
|
||
|
||
49-12-15/16
|
||
Dissertations Defended in the Scientific Council of the Institute of
|
||
Physics of the Earth, Institute of Physics of the Atmosphere and
|
||
Institute of Applied Geophysics, Ac. Sc. USSR during the First
|
||
Semester of 1957.
|
||
V.A.~Romanyuk Determination of the Gravity Forces on the Sea
|
||
by the Pendulum Method (Opredelenlye tyazhesti na more may-a=tn k-
|
||
ovym sposobom) Can ate dissertation. Opponents: Doctor
|
||
of Physico-Mathematical Sciences I.D. Zhongolovich, Doctor of
|
||
Physico-Mathematical Sciences V.V. Fedynskiy, Candidate of
|
||
Physico-Mathematical Sciences N.N. Pariyskiy. May 31, 1957.
|
||
The author attempted to make a more exact analysis of the move-
|
||
ment.of a pendulum on a mobile support with the aim of deriving
|
||
more accurate formulae and developing methods for the calculation
|
||
of the action of acceleration and inclination of the base of the
|
||
pendulum. The calculation of this action Is precisely the most
|
||
important and least clear problem in the theory of the measure-
|
||
ment of gravity forces on sea.
|
||
The author obtained a formula for the correctiQn of the inclina-
|
||
tion and acceleration of the support in the observed value of,
|
||
gravity force which is valid for accelerations below 50 91.
|
||
Card The main terms of this re2ation correspond to the corrections
|
||
12/21 of Brown, but there is some divergence in the terms
|
||
|
||
49-12-1-5/16
|
||
Dissertations Defended in the Scientific Council of the Institute of
|
||
-Physics of the Earth, Institute of Physics of the Atmosphere and
|
||
Institute of Applied GeophysicsAc.Sc. USSR during the First
|
||
Semester of 1957.
|
||
which depend on the periods of oscillations of the pendulum and
|
||
the accelerations.. In many cases, these terms can be dis-
|
||
regarded. The problem was formulated and solved of determining
|
||
the accelerations and the inclinations of the mounting by means
|
||
of inclination-meters and accelero-meters. Attention is drawn
|
||
to theerroneous nature of the view relating to the compensation
|
||
of the term '2 during the observation time (!9 - vertical
|
||
0 0
|
||
acceleration component of the mounting in an absolute system of
|
||
co-ordinates). Under certain unfavourable ponditions, partic-
|
||
ularly during observations in submarines, z 0 can be consider-
|
||
ably larger than the value of other correction factors of the
|
||
second order. For reducing the influence of the term YO
|
||
the author proposed to' Inc r e as e the number of measurements
|
||
at various sections of the film.during determination of the
|
||
average period of the pendulum; for this purpose, it is necessary
|
||
tocarry out recordings at the beginning and at the end of
|
||
Cardl3/2 :P bservations at high-speed of movement of thefilm for durations
|
||
|
||
49-12-15/16
|
||
Dissertations Defended in the Scientific Council of the Institute of
|
||
.Physics of the Earth, Institute of Physics of the Atmosphere and
|
||
Institute of Applied GeoPhYsics,Ac-Sc. during the First
|
||
Semester of 1957.
|
||
of 4 6 minutes. The advantage was emphasised of constructing
|
||
pendulum instruments in a cardan suspension with a minimum
|
||
natural frequency. It is not advisable to apply a damping
|
||
device of the cardan suspension,.which is linked with the ship.
|
||
Methods were developed and investigated of evaluating the
|
||
recordings of inclination-meters and accelero-mters for obtain-
|
||
ing correction for the inclination and the acceleration and
|
||
appropriate calculations were made based on materials collected
|
||
by marine gravimetric expeditions. It is concluded that it is
|
||
in principle possible to effect pendulum measurements on surface
|
||
ships provided that the acceleration of the ship is below 20 gl;
|
||
at larger accelerations, considerable difficulties occur
|
||
associated with the determination of the accelerationsand
|
||
inclinations.
|
||
Oard 14/21
|
||
|
||
49-12-15/16
|
||
Dissertations Defended in -the Scientific Council of the Institute of
|
||
Physics of the Earth),InsLitute of Physics of the Atmosphere and
|
||
Institute of Applied Geophysics, Ac.Sc. USSR during the First
|
||
Semester of 1957.
|
||
I.I. Rokityanskiy Induced Polarisation in Ion-conductinv,
|
||
Rocks (Vyzvannaya po-lyarizatsiya,icnoprovodyashchikh porod)
|
||
--Ua-- Opponents: Doctor of Geol.-Min.
|
||
ndidate dissertation.
|
||
Sciences V.N. Dakhov, Doctor of Phys.-Math. Sciences A.G.Tarkhov,
|
||
Candidate of Phys.-Math. Sciences D.A. Fridrikhsberg. May 17,
|
||
1957.
|
||
The author investigated under induced polarisation the Dhysico-
|
||
chemical phenomena taking place in rocks and other non-uniformly,
|
||
conducting bodies under the effect of an electric current. These
|
||
phenomena lead to the generation of secondary e.m.f. which
|
||
exist for some time, even after the primary current is switched
|
||
off. Study of the nature of the induced polarisation of ion-
|
||
conducting rocks is of great importance in elucidating the
|
||
prospecting possibilities of this method, both in field prv-
|
||
ecting, particularly coring d1also for stud the properties
|
||
of transient regions betviee,~'Tleiquid (water) L so id dielectric,
|
||
i.e. inelucidating one of the difficult problems of the physics
|
||
(;ardl5/ZLcf surfaces. The author has studied the influence on induced
|
||
|
||
49-12-15/16
|
||
Dissertations Defended in the Scientific Council of the Institute of
|
||
Physics of the Earth, Institute of Physics of the Atmosphere and
|
||
Institute of Applied Geophysics,Ac-Sc. USSR during the First Semester
|
||
of.~1957-
|
||
polarisation of a number of factors: the chemical composition
|
||
of the pore moisture, the 4-potential, the structure of the
|
||
specimen and its uniformity. The experiments were effected in~
|
||
quartz sand which was boiled several times in hydrochloric and
|
||
nitric acids and then washed in distilled water until the
|
||
resistance of the pore solution did not reach the resistance of
|
||
the distilled water (2 500 Qm)- It was found that the chemical
|
||
composition.of the pore moisture influenced the induced polaris-
|
||
ation only through the specific resistance and the Z -potential.
|
||
For an equal specific resistance of the specimens, the induced
|
||
polarisation will be the larger, the larger the negative
|
||
otential. In the case of a constant ;-potential, the
|
||
n uced polarisation is proportional to the specific resistance
|
||
of the specimen, but the speed of the drop does not depend on
|
||
the specific resistance. In moisture-saturated sands with a
|
||
re-charged, twin electric layer, the induced polarisation
|
||
approaches zero and does not depend on the 4-potentilal. However,
|
||
cardl6/21in specimens which were not moisture-saturated, but did have a
|
||
|
||
49-12-15/16
|
||
Dissertations Defended in the Scientific Council of the Institute of
|
||
Physics of the Earth, Institute of Physics of the Atmosphere and
|
||
Institute of Applied GeophysicsAc.Sc. USSR during the.First
|
||
%mester of 1957.
|
||
re-charged, twin,.electric layer, the induced polarisation
|
||
increases sharply with increasing 4-potential. On reducing
|
||
the humidity, the induced polarisation increases proportionally
|
||
with the.sDecific resistance of the specimen, but for low
|
||
humidity contents, this increase slows down, the induced
|
||
polarisation passes through a maximun and then decreases,
|
||
although the specific resistance of the specimen continues to
|
||
increase. The author has proved the existence of a certain
|
||
dependence of the induced polarisation on the degree of dis-
|
||
persion and thereby he indicated the possibility of applying
|
||
the method of.induced polarisation for.coring oil deposits
|
||
for the purpose of determining the permeabilityand the speci-
|
||
fic conductivity of rocks. He also obtained the relation
|
||
between the speed of fall of,the induced polarisation and the
|
||
degree of dispersion. leor sands, the speed of fall is the
|
||
higher the finer the sand. This result seems to favour the
|
||
view that when passing anelectric current through the specimen,
|
||
uardl?/21 each sand grain is similar to an electric dipole and the drop
|
||
|
||
49-12-15/16
|
||
Dissertations Defended in the Scientific Council of the InscUtute of
|
||
Physics of the Earth, Institute of Physics of the Atmosphere and
|
||
Institute of Applied Geophysics, Ac.Sc. USSR during the leirst
|
||
Semester of 1957.
|
||
in the induced polarisation represents the total field of
|
||
the discharge of these dipoles. The fundamental relations
|
||
of induced polarisation of ion-conducting rocks were clari-
|
||
fied, starting off by taking into consideration the forces
|
||
acting on the charges of the difffidm part of the twin,
|
||
electric layer. In the equilibrium state (in the absence of
|
||
current flow), the only force maintaining the charges of the
|
||
diffusion layer around the surface is the electro-static
|
||
attraction from the charges of the fixed layer; therefore,
|
||
the surface density of,the charges of the diffusion layer at
|
||
each point of the surface equals the density of the charges
|
||
of the fixed layer. It can be assumed that on applying an
|
||
external electric field, the surface density of the charges
|
||
does not change in the fixed layer (or changes much less than
|
||
in the diffusion layer).
|
||
uard 18/21
|
||
|
||
49-12-15/16
|
||
Dissertations Defended in the Scientific Council of the Institute of
|
||
Physics of the Earth, Institute of Physics of the Atmosphere and
|
||
Institute of Applied Geophysica,Ac.Sc. USSR during the First
|
||
Semester in 1957.
|
||
N.I. Parkhomenko Piezo7electric Effect of Rocks (Plezoelek-
|
||
tricheskiy effekt gornykh porod) Candidate dissertatLon.
|
||
Opponents: Doctor of Physico-Mathematical Sciences V.F.
|
||
Bonchkovskiy, Candidate of Physico-Mathematical Sciences I.S.
|
||
Zholudev, Candidate of Technical Sciences B.A. Bazhenov.
|
||
July 21, 195?.
|
||
For many centuries, the descriptions of earthquakes mentioned
|
||
the light effects~but the-phys'ical-nature of.-the latter
|
||
was no t kn o w n.~ With the &ivelbpment of investigations
|
||
in electricity and improved instrumentation, the electrical
|
||
character of these phenomena was estabiished. Only individual
|
||
statements of hypothetic character exist on the sources of
|
||
the changes of the electrical field of the Earth. In view of
|
||
the importance of this problem of a possible relation between
|
||
the electro-magnetic and the seismic fields, the author studied
|
||
the electrical effects in rocks subjected to mechanical forces.
|
||
By means of a dynamic method, a piezo-electric effect was
|
||
observed in rocks (granite, gneiss, ciuartzites, etc.) containing
|
||
uardlq/;~yartz grains which are orientated in a specific way. In the
|
||
|
||
49-12-15/16
|
||
Dissertations Defended in the Scientific Council of the Institute of
|
||
Physics of the Earth, Institute of Physics of the Atmosphere and
|
||
Institute of Applied Geophysics,Ac.Se. USSR during the First
|
||
Semester of 1957.
|
||
absence of orientation of the quartz grains, no piezo-electric
|
||
effect was observed. Under laboratory conditions, the exis- . ~
|
||
tence of the E effect discovered by A.G. Ivanovwas confirmed
|
||
and '.also its relation to the presence of a liquid phase
|
||
in rocks., On the basis of investigation of ideal piezo-
|
||
electric textures of quartz in accordance with the theory of
|
||
A.V. Shubnikov, it was found that from a single modification
|
||
of quartz, it is possible to form piezo-electric textures of
|
||
the first kind, type W and oo-.2 and of two shapes of
|
||
quartz, it is possible to form a texture of the type DO.M.
|
||
The possibility was elucidated of ordinating quartz-containing
|
||
rocks to piezo-electric textures of the type Do.m and also
|
||
to the symmetry class 3:2.A 'technique was developed of the
|
||
qualitative measurement of the piezo-electric moduli of rocks
|
||
in the case of longitudinal and transverse effeclB,by the
|
||
static method applying an electrometer. It ism5hown that in
|
||
rock specimens of volumes of the order of 10 c , the piezo-
|
||
(;ard20/2l electric effect can be observed owing to the non-compensated
|
||
--:7- 7 7 7 7~
|
||
I TI TT
|
||
|
||
49-12-15/16
|
||
Dissertations Defended in the Scientific Council of the Institute of
|
||
Phjsics of the Earth, Institute of Physics of the Atmosphere and
|
||
Institute of Applied GeophysicsAc.Sc. USSR during the First
|
||
'S emester of 1957.
|
||
effect of the individual quartz grains. On the basis of
|
||
experimental data, the coefficient of orientation of the quartz
|
||
grains was calculated with some degree of approximation in
|
||
various rocks by means of the formula of Zheludev. Model tests
|
||
on granite blocks enabled establishment (in addition to an
|
||
elastic wave) of two types of electro-magnetic oscillations.
|
||
Oscillations of one type precede the arrival of the elastic
|
||
wave and coincide with the incident of emission, oscillations
|
||
of the other type a:be r-ecorded at about the same time as
|
||
the elastic,wave. The os Icillations of the first type-are
|
||
caused by the piezo effect of the granite block near the
|
||
emmitter of the ultra-sound., whilst oscillations of the second
|
||
type are caused by the piezo-electric effect of the,%me granite
|
||
near to the receiver. The results of these experiments can be
|
||
applied in studying the physics of earthquakes and also for
|
||
developing new methods of electric prospecting.
|
||
AVAILABLE: Library of Congress.
|
||
Card 21/21
|
||
|
||
5(7),24(4)
|
||
AUTHOR:Pyaskovskaya-Fesenkova, Ye. V. SOV/20-123-2-161/50
|
||
TITLE-On Some Optical Pr-ope-rr ~s ~tmo
|
||
sphere of the Lybian
|
||
-
|
||
Desert (0 nekotorykh opticheskikh svoys4.vakh atmosfery
|
||
pustyni)
|
||
PERIODICAL%Doklady Akademii nauk SSSRp '1958, Vol 123, Nr,2, pp 269-271
|
||
(USSR)
|
||
ABSTRACT;The authoress And her collaborat6rs carried out investigations
|
||
in Egypt (October-November 1957) in connection with the prog-
|
||
ram of the International Geophysical Year. The exgedition work-
|
||
ed in the Libyan desert south of Assuan ( (f = 23 59', ,
|
||
X = 320521) in-a distance of I km from the river Nile and
|
||
about 200 km west of' the Red S%E;. The following was found: The
|
||
optical properties of the atmosphere are very constant in the
|
||
forenoon and afternoon hours. Nevertheless, this constancy was
|
||
disturbed for several hours at about noon, after which the
|
||
atmosphere becamemore transparent than in the forenoon, a
|
||
phenomenon that is only very rarely observed in the USSR. The
|
||
aureole of,the sun was weaker in the afternoon than in the
|
||
forenoon. The atmosphere at the place where observations were
|
||
'
|
||
Card 1/5carried out was very
|
||
homogeneous in optical respect on cloud-
|
||
|
||
0n Some Optical Properies of the Altmosphere of the SOV/20-123-2-16,150
|
||
Lybian Desert
|
||
less days. A schematical drawing shows 2 scattering indicat-
|
||
rices which were determined on October 25 on the basis of
|
||
observations of.the brightness of the sky along the entire
|
||
almucantar of the sun with a zenith distance of z = 740. These
|
||
two indicatrices hardly differ at all from ench other. There
|
||
was no fine atmospheric dust, there was little moisture, and
|
||
it was probably for this reason that a green shine became
|
||
noticeable nearly every evening before sunset. The increase of
|
||
transparency in the afternoon influenced the polarization
|
||
properties of the atmosphere. The degree of polarization of the
|
||
sky by day is always less high in the afternoon than in the
|
||
forenoon. The authoress determined the direction and the
|
||
amount of polarization by Aeans of a visual photometer des-
|
||
L
|
||
cribed in one of her earlier papers (Ref 2). The degree of
|
||
polarization.attains very high values; it is higher in the
|
||
afternoon than in the forenoon, and immediately after sunset
|
||
it roseto 60 %.A diagram shows the course of the degree of
|
||
polarization in the almucantar of the sun at an angular dis-
|
||
tance of 900 to the sun, as a function of the atmosDheric
|
||
Card 2/3 mass m in the direction towards the sun. This curve describes
|
||
|
||
On Some ODtical Properties of the Atmosphere of the SOV/20-123-2-16/50
|
||
Lybian Desert
|
||
the observations made on November 16 from z 6702t in the
|
||
morning to 87034' in the evening. When the light is scattered
|
||
in the first order, the direction of the oscillation plane
|
||
must be vertical to the plane of vision. In tho forenoon of
|
||
November 16, the transpark~ncy couff tcient amounted to p - 0.85,
|
||
and the difference between the measured and the theoretical
|
||
plane of oscillation remained constant (-20). In the after-
|
||
noon (p = 0.69) these two planes were in agreement. There are
|
||
4 figu-i-t~~s and 4 referen,--es, 3 of whii-,h are Soviet.
|
||
PRESENTED. July 121, 1958, by,V. G. Fesenkov, Academician
|
||
SUBMITTED: July 12, 1958
|
||
Card 3/3
|
||
|
||
3(7)
|
||
AUTHOR:Pyaskovskaya-Fesenkova, Ye. V& SOV/20-123-6-14/50
|
||
TITLE:On the Scattering and Polarization of Light in the Atmosphere
|
||
Under the Conditions of the Libian Desert (0 rasseyanii i -
|
||
polyarizatsii sveta,v atmoefere v usloviyakh W1viyskoy pustyni)
|
||
PERIODICAL:Doklady Akademii nauk SSSR, 195811,1'91.12,3j~.'Alr 6, pp 1006-1009
|
||
(USSR)
|
||
ABSTRACT:The authoress investigated the luminosity and the polarization
|
||
of the daylight sky in October-November 1557 in the Lybian
|
||
Desert 20 km south of Assouan 230591 32052,
|
||
h - 200m) by means of a visual photometer provided with a yellow
|
||
Schott (Shot) filter and with a Polaroid. The degree and the
|
||
angle of polarization were determir,,_~d according to the method
|
||
of V. 0. Posenkov, according to which the luminosity of the
|
||
investigated point of the sky is measured through a Polaroid at
|
||
3 positions B1, B 2 9 B3 at various angular'distances 4 from the
|
||
sun in the solar almucantarat. (These points on the sky and the
|
||
sun have the same distance from the zenith). The angular
|
||
distances between the positions B,, B 21 and B3 amount to 600
|
||
Card 1/3Moreover, the authoress measured the luminosity of a plane
|
||
|
||
On the Scattering and Polarization of Light SOV/20-123-6-14/50
|
||
in the Atmosphere Under the Conditions of the Lybian Desert
|
||
perpendicular to the sunbeam. From these.data, the degree of
|
||
polarization, the orientation of the plane of the light
|
||
vibrations, the tolal luminosity Be and the scattering
|
||
indicatrix could be determined. Moreover, the scattering
|
||
.indicatrix could be divided into 2 components. One of them is
|
||
,the indicatrix of the scattering in natural beams, the other one$
|
||
in polarized beams. Moreover, the total scattering indicatrix
|
||
was subdivided into.2 other components: one of them corresponds
|
||
to molecular scattering, the other to aerosol scattering.
|
||
Finally, the authoress tried to separate out the degree of
|
||
polarization caused by aerosols and to subdivide the aerosol
|
||
indicatrix into 2 indicatrices which correspond to natural and
|
||
to polarized beams. A diagram shows the distribution of the
|
||
polarization degree P along the almucIntarat of the sun. The
|
||
,maximum polarization degree was at - - 900 and was equal to
|
||
74%. The second diagram gives the orientation of the plane of
|
||
the light-vibrations with respect to the corresponding vertical.
|
||
as a function of the angular distance 4( from the sun. The third
|
||
diagram'shows the total indicatrix in polar coord-4nates.---
|
||
A formula is then given for the intensity of the polarized light.
|
||
Card 2/3
|
||
|
||
On the Scattering and Polarization of Light SOV/20-123-6-14/50
|
||
|
||
23933
|
||
'S/U35/61/000/006/015/044
|
||
AGOI/AlOl
|
||
AIJ'. Pyaskovskaya-Fesenkova, Ye.V.
|
||
T11ME: Some data on.sky polarization in southern Egypt
|
||
PERIODICAL. Referativnyy zhurnal. Astronomiya I Geodeziya, no. 6, 1961, 26-27,
|
||
abstract 6A231 ("TZV. Astrofiz. In-ta AN KazSSq', 1959, v. 8, 82-
|
||
97, Engl. summary)
|
||
MT- The author 6scribes the results of observations on atmospheric op-
|
||
,ties In southern Egypt, c-onducted by an expedition of the Academy of Sciences,
|
||
USSR, in the fall 1957. A visual photometer of daily sky (for measuring the brW_
|
||
ness and polarization of -.he sky) and a photoelectric photometer (for observations
|
||
of circ-umsolar aureole and ccnllrol of stability of the atmosphere optical proper-
|
||
ties) were used. It was found out --.hat in the region investigated a good stabill-
|
||
ty was obi~erved before and after noon, which was disturbed only about ncon (fol-
|
||
lowed by aureole decreaea). In the USSR usually the aureole grows after noon.
|
||
Almost every evening a green ray was ot.served. Polariza-lion degree after noon in-
|
||
creased. The V.G, Fesenkcv metticid (Astron. zh., 1935, v. 12, no. 4), which con-
|
||
=Is~. - L
|
||
's In measuring the brigh*.ness of a given sky point at three polaroid positions,
|
||
Card 1/2
|
||
|
||
2-VA5/,,~: 1/000/006,/015/044
|
||
Some data on Zky pcIariza-_I3n in so~~-hern Egyp-I .4001./AlO'L
|
||
was employed for determinin ,gdegree and angle of polarization. These measurements
|
||
werle pF-rf'criPed in almucan-.ar of the Sun and in zenith. ITe observed pciarizat-ion,
|
||
angle tLne of light, oscillations) was oom-
|
||
6 ob.- (between the vertical and the pI
|
||
pared wl th that caicalated theoretically ( ~ th) fz~r f I rst-order ecattering. At
|
||
high transparency the d_'fferenc-e -_-e-~ween them amounted t_o 1--20. 'Ln four Zaae ut
|
||
o
|
||
of 5, polarization fraximum in _almucan~ar of the. Sun was at scattering angle =60,
|
||
i.e., the plane of light oscillations in -Zhe real atmc-sphere ccinl,ides with the
|
||
similar plane at firs!--order s:!at-tering (if transparency is sufficiently high) in
|
||
proximity of this angle. The author presents components of the summary s0attering
|
||
indica-Irix in na-,.urai light t'and in polarized light #', determined from ob-serva.-
|
||
tions in almucantar of the S-LL-. Cc-mponent /11 varies frcm day to day mcre thanlu
|
||
An' attempt is made --- ZIngle out polarization depe-1:4-ent on aerosol componen-~ from
|
||
-the observed (ZLI V
|
||
immar-j) polarization.
|
||
G, Livshits
|
||
[Abstracter's notlet Complete translation]
|
||
Card 2/2
|
||
|
||
"'~335/61/000/006/0 14/044
|
||
A001/AIOI
|
||
AUM Pyaskov~kaya_Fesenkova, Ye.V.
|
||
"TITLE: Certaln relations in the phenomenon of sky polarization
|
||
PERIODICAL: Referativnyy zhurnal. Astr.onomiya i Geodeziya, no. 6, 1961, 26, ab-
|
||
stract 6A230 ("Izv. Astrofiz. in-ta AN Ka7..9.c;R" 196o, v. io, 64-7o,
|
||
Engl. summary)
|
||
TEXT:- The author describes the results of observations of brightness a-id
|
||
polarJzation of -uhe,ciear sky along the almucantar of the Sun at its different
|
||
heights in the region of the Mount-ainnus Observatory of the AstrophysicbL1 Insti-
|
||
tue, AS KazSSR. The photometer was described by the author earlier (RZhAstr, 1960,
|
||
no. 5, 4036). Polarization was determined by the V.G. Fesenkov method (measuring
|
||
sky brightness at -..hree pcsitions of 'the polaroid (see RZhAstr, 1959, no. 5, 3556).
|
||
Observations, which were conducted on sky points over mountains and lowlands, have
|
||
shown that polarization degree was almost the same at equal angular distances to
|
||
the Sun. Polarization degree P at different scattering angles turned out often to
|
||
be proportional to "RayleigirP polarization degree- P = kPR- This relation holds
|
||
sometimes also at poor transparency. On the other hand, deviations from the Ray-
|
||
Card 112
|
||
|
||
23?/19-35/61/000/006/014/044
|
||
Certain relations AGOI/A101
|
||
letgh law may often happen to be very significant. Observations permitted the
|
||
singling out of summary, indicatrix indicatrix in natural rays IA'(?) and
|
||
in polarized rays ~1" (,?j;) (j.~ is scattering angle). A comparison of observational
|
||
data in different aces clarified the problem of relation between 1A )and ~L9at
|
||
different atmospheric transparency p. It has been found out that /~1(900) and Ik
|
||
(900) var-y linearly with p and, consequently, the change of a scattered flux in
|
||
natural light is greater than in a polarized one. This is connected with a lesser
|
||
light polarization on aerosols (in comparison with molecular polarization).
|
||
G. Livshits
|
||
[Abstracter',s note. Complete translation]
|
||
|
||
J. 4000 68983
|
||
AUTHOR: pyaskov#~~' ak'A S/020/40/131/02/022/071
|
||
BO13/BO11 .
|
||
Data
|
||
the Polarization of Light
|
||
~v
|
||
on
|
||
by the Atmosphere
|
||
TITLE: Some
|
||
PERIODICAL: Doklady Akademii nauk SSSR9 1960y Vol 131v Mr 2, pp 297-299 (USSR),
|
||
ABSTRACT:
|
||
1/3
|
||
The author reports on observations made concerning the brightness
|
||
and polarization of the olearsky along the alnuosatar of the am
|
||
on the mountain observatory of the Astrofixicheekly institut
|
||
AN Kax It (institute of Astrophysics of th AS of the lasekbakaya
|
||
SSR) in the surroundings of Alas, At& 00450 M) in August, 19549
|
||
in the Aksengerskiy sovkhoz in the surroundings of Alas, At&
|
||
h-500 in June - July, 1957# and in the Lybian Desert (ant)
|
||
~h-,200 :~ in October - Novenber, 1957- Observations more &ad* by
|
||
means of a visual photometer with a yellow Schott filter. Polariza-
|
||
tion was determined according to Y.G. Fesonkov's procedure. The
|
||
brightness of the celestial point under investigation was seasur*d
|
||
by a polaroid with three different positions. Polarization degree
|
||
and direction of the polarization plans can be deterain9d in a
|
||
similar w4X. The d9gres of polarization was determined by the forauls.
|
||
2 -B2)+B2(B2-B )+B (B _D
|
||
01 (B1 Bj + B2 + B 3 3 3 17- . where Dj,B2PB3 denote the
|
||
brightness.of the celestial point observed with the three above-
|
||
|
||
68983
|
||
Some Data on the Folarization of Light by the S/020/60/131/02/022/071
|
||
Atmosphere B013/9011
|
||
mentioned positions. On certain days, the influence exerted by
|
||
aerosols in a real atmosphere manifesto itself only by a certain
|
||
decrease of the polarization degr
|
||
n 2
|
||
PR ("'C) + 0082Ah
|
||
namely, in the same ratio for all scattering angles2p.. gone*, P(-I,&)
|
||
kPR(i4 holds for these days, with k denoting the maximum pol&rix&-
|
||
tion degree in the almucanter of the sun (for~A - 900). Such a
|
||
proportionality does not depend on the ataospheric transparency. the
|
||
last-montioned equation is satisfied well with bad t=ansparency, and
|
||
poorly in the case of good transparency. Examples are offered. On
|
||
the basis of observations.of the sky brightness along the almucantar
|
||
of the sun with the three above-mentioned positions of the polarold
|
||
it was possible to determine the scattered light flux #(%,I,) for,
|
||
different scattering anglea -LA and to subdivide it into two parts,
|
||
namely, into natural rays 41(vFs) and into polarized rays A4 of (iA)
|
||
The ratio between these two scattered fluxes changes with a change
|
||
in the atmospheric visibility. IAI(900) risen more quickly with
|
||
increasing atmospheric dullness than P"(900 Aorosole.perhaps
|
||
polarize the light to a lesser degree than molecules. 7or this reason,
|
||
Card 2/3 the scattered flux in the case of an increased quantity of aerosols
|
||
|
||
68983
|
||
Some Data on the Polarization of Light by~the 8/020/60/131/02/022/071
|
||
Atmosphere B013/Boll
|
||
Is likely to grow more slowly in polarized rays than in natural
|
||
rays. and #"(i)k) are likely to depend linearly on the
|
||
M1 - - - - - - -A 04 4 4-U1- --A X
|
||
|
||
84686
|
||
S/020/60/134/004/010/023
|
||
VI., 01P 3~v M69) BOI19/BO67
|
||
AUTHOR: Fygskovska a-Fesenkova. V. U
|
||
TITLE: Determination of the Transmission Coefficient of the
|
||
Atmosphere From the Polarization of the Sky light \0V
|
||
PERIODICAL: -Doklady Akademii nauk SSSR, 1960, Vol...134,,No. 4,
|
||
pp. 812 - 815
|
||
TEXT: From 1956 to 1957 the author studied the sky brightness by means
|
||
of a polaroid and aphotometer on a mountain observatory '(1450 m above
|
||
sea level)) in the Aksengerskiy sovkhoz (kksengir (?) sovkhoz) near
|
||
Alma-Ata and also in the Liviyskaya pustina Yegipetskogo rayon. They also
|
||
measured solar radiation and the brightness of thelv8alix-corona. These
|
||
measurements were made at the~mountain observatory by N. I. Ovchinnikova,
|
||
in the Aksengerskiy sovnarkhoz by PZ.
|
||
_~Jio~koq and in the Liviyskaya
|
||
pustina by V. M. Kazachevski and P. N. Boyko. The observations were made
|
||
by means of photometers with yellow Schott glass filter. The effective
|
||
wavelength in the system glass yellow screen was calculated from formula
|
||
Card 1/4
|
||
|
||
Determination of the Transmission Coefficient S/020/60/134/004/010/023
|
||
of the Atmosphere From the Polarization of B019/BO67
|
||
the Sky Light
|
||
E;~p d%
|
||
0 OD
|
||
EXpj&~L d%
|
||
,,E denotes the energy,distribution in the spectrum of the light source,
|
||
p' the transparency of the filter, F. the spectral sensitivity of the
|
||
0 0
|
||
glass-Absolutely black bodies with temperatures of T = 20,000 K, 4,000 K
|
||
and the sun (t - 6,OOOOK) were studied. Results: Ao . 560 m~Lat 20,OOOOK,
|
||
Ao - 565 m/L at 6,OOOOK, and ;Lo - 56a T at 4,OOOOK. For a light source
|
||
of E const, X0 was found to be 567. The effective wavelength in Ithe
|
||
system selenium photocell yellow screen was calculated from formula
|
||
Card 2/ 4
|
||
|
||
84686
|
||
Determination of the Transmission Coefficient S/020/60/134/004/010/023
|
||
of the Atmosphere From the Polarization of the B019/BO67
|
||
Sky Light
|
||
00
|
||
m
|
||
E p d?,
|
||
(2)
|
||
0 CD
|
||
pie M
|
||
E d%
|
||
0
|
||
Here, E is the energy distribution in the solar spectrum at the
|
||
atmosphere boundary, t thespectral sensitivity,of the photocell, p. the
|
||
spectral transmission coefficient, and m the atmospheric mass in the
|
||
direction of the sun. For m 1, %0 was found to be 577, and for M = 5.6,
|
||
10' was found to be 582. The degree of polarization was calculated from
|
||
formula P = 2YB
|
||
1 'B 1-B 2) + B2(B2B 3) + B3(B3-B /(B 1+B 2+B 3) (3). B i are
|
||
the three brightnesses of the sky measured by V. G. Fesenkov's method by
|
||
means of the polaroid. The transparency coefficients were.measured by
|
||
three different methodsi 1) from solar radiation according to Buger,
|
||
2) from measurements of the sky brightness at an angular distance of 600
|
||
Card 3/4
|
||
jj
|
||
|
||
Determination of the Transmission Coefficient 5/020/60/134/004/010/023
|
||
of the Atmosphere From the Polarization of the B019/BO67
|
||
Sky Light
|
||
from the sun, and by a method suggested by the author with the aid of
|
||
formula p = 0.973 - 9,80B(~SOOVE m (4); 3) from measurements of the solar
|
||
m
|
||
corona at the moment of its maximum brightness, by the aid of formula:
|
||
logp - -M/m max (5), In Fig 1 F f(p) is graphically r Iepresented
|
||
according to measuremews at the three localities mentioned initially with
|
||
0 1 0 0
|
||
s
|
||
,attering angles of 40 j 60 , and.90 i
|
||
e, The author points to the nonl near
|
||
character of this dependence which is not locally dependent within the
|
||
maas-arement error. Furthermore, P = f(T) is graphically represented (Fig.2)
|
||
where x denotes the optical path of the atmosphere. The relation
|
||
lnT = 0.035 - %344P (6) is given for this case, For T = O~05 the author
|
||
cal,3ulated a polarization at 900 of 100%, at 600 of 60%, and at 40' of
|
||
26% with a transparency coefficient of 0.954 By taking account of an
|
||
effective wavelength in the system glass - screen of 564 ~v4 the author
|
||
obtains a 83% polarization at a scattering angle Of 90 0 at sea level, and
|
||
anF37% polarization at the mountain observatory, There are 2 figures and
|
||
Soviet reference,
|
||
PRESENTED: May 3, !960; by V, G. Fesenkov, Academician
|
||
SUBMITTED:
|
||
27, 1960
|
||
April
|
||
Card 4/4
|
||
|
||
PYASKOVSKAYA-FESENKOVA, V. (Alma-ata)
|
||
"Some results of investigation about atmospheris scattering and
|
||
polarization of the day skylight."
|
||
Report submitted in connection with the Symposium on Radiation,
|
||
Vienna, Austria 14-19 Aug 1961.
|
||
|
||
S/169/62/000/003/047/098
|
||
AUTI-10R: ~Pyaskovskaya-Fesenkova, Ye. V.
|
||
TITLE: Day-time sky polarization (Theses)
|
||
PERIODICAL: Re_-~'erativnyy zhurnal, Geofizika, no. 37 1962, 2061 ab-
|
||
stract 3B212,.(V sb.,Akt-inometriya i atmoofern. optika,
|
||
L., Gidormeteoizdatu, 1961, 103-104)
|
||
TEXT: The results of sky brightness observations, carried ou, in
|
||
the Libyan desert, in southern Egypt, and atla mountain observato-
|
||
ry.near Alma-Ata, are analysed.N. G. Fesenkov's method was used
|
||
in determining Ithe degree of sky-dispersed light polarization 'and
|
||
the orientation. oli" the plane.of the electrical vector's variations.
|
||
An attempt was made to distinguish from 'the summary radiation, ob-
|
||
served alon- the sun's almacantar, the radiation that depends on.
|
||
the presence of aerosols in the azmosphere. The mazeimum of the aero-
|
||
sol component of the polarization ban be observed-at an angular
|
||
distance of 110 - 1200 from the sun and amounts to 40%. /-Abstrac-
|
||
ter's note: 03mplete translation.7
|
||
Card 1/1
|
||
|
||
9/169/62/000/003/061/098
|
||
D228/D301
|
||
AUTHOR: Pyaskovskaya-Fesenkova
|
||
Y e
|
||
TITLE: Methods of determining the coefficient of atmospheric
|
||
transparency from the sky brightness (Theses)
|
||
PERIODICAL: 'Referativnyy zhurnal, Geofizika, no. 3, 1962, 28, ab-
|
||
stract 3B232 (V sb. Aktinometriya i atmosfern. optika,
|
||
L., Gidrometeoizdat, 1961, 144)
|
||
TEXT: Three methods of determining thecoefficient of transparen-,
|
||
cy are suggested: 1) From the moment of onset of the brig4tness
|
||
maximum of the circumsolar halo, since in this case there is 4 very
|
||
simDle relationship; 2) from the indicatrix of dispersion wh6n true
|
||
absorption is absent; and 3) from empirical formulas, derived on
|
||
the basis of much observational material,*/-Abstracter'.9 note: Com-r
|
||
plete translation.-7
|
||
Card
|
||
|
||
S/035/61/000/012/008?u4 I
|
||
A0OI/AIOI
|
||
ALWORS~ Pjaskovskaya-Fesenkova-Ye.V., Boyko, P.N., Belyak, G,M, Boykc.
|
||
T i Some data on attenuation and dispersion of light at varlous alti-
|
||
tudes above sea level
|
||
FERIODICAL: Referativnyy zhurnal, Astronomiya i Geodezlya, no, 12Y 19161, A3,
|
||
abstract 12A285 ("*Lzv. Astrofiz, in-ta AN.KazSSIV, 1961, v, 11,
|
||
78 88, Engl, summary)
|
||
TEXT- Brightness of daily sky on the Sun's almucantar was measured simu 'L-
|
||
~aneously at two points e = -
|
||
57 and'60c at the Mountain - Observatory of the A:~
|
||
ohysical lnitiWte, AS KazSSR, and on the Kumbel' mountain. A visual photometer
|
||
and a pho"oelectrical photometer, with selenium photoelement were used. Trans-
|
||
parency coefftelents P), optical thicknesses of atmosphere ( T') and .9cattering
|
||
IndIcat.nices i),(~) were-determined from the measurement data, it. is noted tha,,
|
||
tran-sparency coefficients over the lowland and mountains differ only slightly-
|
||
Linke~s turbidity factor increases in afte~rnoon hours in comparison with mornine,
|
||
f~ard lf-~
|
||
|
||
|
||
B/913162/003/000/002/033,.-
|
||
1)405/D301
|
||
|
||
~AUTHORs
|
||
.yaskovskaya-Fesenkovas Ye. V.,
|
||
P
|
||
TITLESDevelopment of atmoopheric optics in Kazakhstan.'
|
||
SOURCESAkademiyal:nauk Kazakfiskoy SSR. Aotrofizicheskiy.
|
||
instituta'";Trudy. v.
|
||
~'3, 1962,.Rasseyani e i poly-
|
||
ariiatsiyal.:sveta v. zemnoy atmosfere; 'materialy
|
||
Sovesfichaniya.po rasseya:idyu i polyarizatsii
|
||
oveta :v atmosfere. 14.- 25
|
||
|
||
TEXT:The,study of..atmospherio optics in Kazakhstan
|
||
|
||
was initiated-from-
|
||
in September I e
|
||
90, when eight exp ditions,
|
||
various partsof the USSR arrived there to study the total- solar:'-
|
||
~eclipse. Soonafterwards iVwas~deoided by,the Council of Ministers
|
||
of the USSR (at the initiative~.of V.G. Fesenkov:) to-create' the
|
||
Institute.of Astrono and...`Ffi~,sica at the Kazakh Branch of the'4
|
||
MY
|
||
-:~The' ar y
|
||
Academy of Sciences USSR. e 1 days of the~Institute coincided'
|
||
with the difficult.stage of the-Second-World War, so that great,
|
||
obstacles wereencountered. in instrument construction. blany,instrument
|
||
Gard 1
|
||
|
||
|
||
|
||
|
||
i19131621003160010021033
|
||
Development of atmospheric optics,,.. D40VD301.
|
||
were constructed by the scientists themselves,' in particular V,G,
|
||
Feserikov; among these were an.
|
||
instrument for laboratory deter-
|
||
mination of the scattering~function in turb:~d wedia,and an instru-
|
||
ment for the determination'bf-,th6 absolute albedo of reflecting
|
||
stirfaces. In 1950 the Inatituteof Astronomy and Physics was.divided
|
||
into two: the Astrophy'sical:~.Institute and. the Physicotechnical
|
||
Institute; in addition an'independent Section for Astrobotany was
|
||
,created. The Astrophysical Institute moved.to the Kamensk'Plateau
|
||
a
|
||
V rious expeditions were'organized, mainly inside Kazakhat n; among
|
||
a
|
||
themt to the Kumbeli.Mountain'-( 200 m) and the G eat Alma_ e
|
||
3 r Ata Lak
|
||
the Sary-Ishik-Otrau deseri:1(near the Balkhash~Sea)lleto., Other.'
|
||
,expeditions led to the Sikhote-Alin'sk Mountain Range in the Par East,,
|
||
and to the Black-Sea',(Gudaut).'Durin the-International.Geophysical.'
|
||
9 171
|
||
Year 1957t an expedition was,sent.to Egypt.where it worked in the
|
||
desert South of the town of Assuan-The. research'of the Atmospheric- M..i:
|
||
Optics Section was mainly'.'concerned with,the scattering capacity' 1
|
||
of the atmosphere, the extinction of. light by,the.atmosphere, solar'
|
||
halos, the-energy distribution,in the spectrum of the diurnal sky
|
||
In recent years, the polarization of light of the: diurnal sky Va
|
||
Card 2/4
|
||
|
||
S/913/62/003/000/002/033
|
||
Development of atmospheric optice., D405/D301
|
||
investigated, as Weil as-'the scattering of light in'the bottom
|
||
layer of the atmosphere. 'Por~this purpose three new instruments
|
||
io
|
||
were construoteds - aspeot -electropolarlmeter with automatic
|
||
recording of spectra, a diurnal-sky electropolarimeter using a'
|
||
photomultiplierf and a' two-channel polarimet6r which'enables to
|
||
directly determine the irst parameters of Sto
|
||
.3;f kes (intensityt,
|
||
difference betweenintensities at two.mutually perpendicular"..
|
||
directions, and the.*Angle of the polarization plane. The polari-
|
||
in the lower-atmosphere was studied~by a specially-designed
|
||
photoelectric photometer.;-Rere,are some of.tfie results,of nearly,
|
||
20 years of research in atmospheric optics: The solar. halo
|
||
attains its highest brightness when the direct solar radiation.i,
|
||
is attenuated by-a factore (the bass of natural logarithms) in"
|
||
.-A the direction of.the line,of sight. The sky brightnees-with,respeot''-,l
|
||
to the solar illumination does not depend, atan angular distance
|
||
of 570 from the Sun,'on.the form-.of the scattering funotio * "The i
|
||
n.
|
||
nature of the latter is the same irrespective of climatic- and
|
||
meteorologic conditions' Among -thetheoretical studies are V.G.
|
||
Fesenkov's theory.of vertical visibility, etc., andthe new method-:"-'.'-
|
||
Card 3/4
|
||
Ix,
|
||
|
||
|
||
|
||
s/gi3/62/003/060/003/033
|
||
Some data on sky brightness D405/D301
|
||
homogen eous in the hIorizonta 1 direction. The directional scattering
|
||
coefficients were determine d~by a,well-known formula of sky bright~.
|
||
ness in which multiple scattering,,is neglected. From figures plotting.i
|
||
the coefficient ~L as a function of atmospheric mass, the following
|
||
conclusions were obtaineds 'At constant angular distance from the
|
||
Sun the.directional scattering coefficient,IA decreases when the.
|
||
Sun approaches the horizon (the zen .ith distance.of the point under~
|
||
consideration remaining fixed); it~remainsconstant for the solar,
|
||
almacantar; it decreases',,~when the Sun,apprbaches the horizoni for
|
||
points which are on an,almacantar-that,is higher than the solar
|
||
almacantar and which move'.together with the latter so that z-~-'const
|
||
(z denoting the zenith distance of the:Sun, and 5 the zenith distance
|
||
of the point under consideration); it increases, when the Sun
|
||
approaches the horizon, for points which are on an almacantar lower
|
||
than the solar and move--together with latter as above..These results.
|
||
are discussed in relation to'suoh-factors as'theldecreasing,atmos-
|
||
pheric density with altitude' multiple',scattering, ground reflection,
|
||
etc. It is noted that the'dbservations.of light polarization conf
|
||
the above results. There"are 3 fi res.
|
||
9U
|
||
Card 2/2
|
||
0
|
||
|
||
|
||
|
||
913/62/003/000/013/033.-
|
||
9
|
||
05/1)301
|
||
AUTHOR: Pyaskovskaya-Pesenkova, Ye. V.
|
||
TITLE%~ On the sky-brightn6so layer
|
||
'Akademiya nauk Kazakhskoy SSRi Astrofizicheeki
|
||
SOURCE:
|
||
institut. Trudy., v.,3,:1962. Rasssyaniye i
|
||
polyarizatsiya sveta v zemnoy,"atmoofere;
|
||
m6terialy Soveshchaniya po rasseyaniyu i poly-
|
||
arizatsii eveta vatmosfer6. 83 88
|
||
|
||
TEXTt The'height'h of*the effective-brightness,layer
|
||
0I-,
|
||
.
|
||
-integrals,of the brightness hi
|
||
|
||
is defin B
|
||
ed by a formula involving
|
||
Thereby it is assumed that.*the atmosphere consiBts,of thin plan46-
|
||
-:
|
||
parallel homogeneous layers, that the density. and optical:. thiokn6ss.~""~':.!:
|
||
l
|
||
of the atmosphere.decreas*e.exponentially, and that multiple s
|
||
catter
|
||
ing and light reflection f.rom.th e ground are absent* After evaluat-*!-I
|
||
I-.-';
|
||
ing the integrals, the'author illustrates the method'of calculation.
|
||
by a numerical example. On the basis of this:example the following
|
||
conclusions are obtaineds., 1).For celestial-points of-fixed zenith
|
||
|
||
Card
|
||
1/2
|
||
|
||
|
||
|
||
S/913/62/903/000/021/033
|
||
Atmospheric polarization 405/D30V
|
||
~Thereby the effects of.multiple scattering, of ground
|
||
and those due to th presence of aerosols, are,taken into..account-
|
||
it is assumed that the multiple-s"cattering intensity is not -depen-.::
|
||
dent on azimuth. The method was verified theoretically;,it was
|
||
shown that, under certain conditions, the method involves a
|
||
n error
|
||
of a few percent only..In~order to separate the integral and aerosol,,~-i~%,
|
||
scattering functions' into polarized and non-polarized light com-
|
||
ponents, the duthor,neglected,the'polarizati6n,of the multiply~
|
||
scattered light. The reasons for such'an assumption are set forth~'.
|
||
From.the curves representing'the degree of.polarizatlon as a func-w
|
||
tion of the scattering angleit is evident that, for a trans
|
||
parency
|
||
coefficient of 0.88, the effect., of multiple *scattering -is negligibly
|
||
small; on the other hand,.-for a-.transparency coefficient of 0.80~,-
|
||
neglect.the multipl scattering. The:a
|
||
it is no longer possible, to,.: e eroa---
|
||
a -~'just as~ the integral. o es. h
|
||
sol.degree of polar.iz tionj~' ne,'..increas wit
|
||
a tmo sphe ri c trans parency; 'f or. a - . trans parency oo ef f i ci ent. of . 0. 68 the
|
||
degree of polarization of,.light'icattered by aerosols.--was found.. to.';~.be -f!
|
||
36%, and.for-a transparency.,ooefficient..of 0. 60: it, was 29%.' There
|
||
s,and 1 table.
|
||
are 6 figure
|
||
Card 2/2
|
||
|
||
|
||
|
||
|
||
ACC NR: AR6035286 SOURCE CODE: UR/0269/66/000/009/0027/0027
|
||
AUTHOR: Pyaskovs kaya- Fes enkova, Ye. V.
|
||
TITLE: Atmospheric polarization of light with dri and wet aerosols
|
||
SOURCE: Ref. zh. Astronomiya, Abs. 9.51.245
|
||
REF SOURCE: Tr. As.trofiz. in-ta. AN KazSSR. v. 7, 1966, 79-84
|
||
TOPIC TAGS: atmospheric optics, optics, light polarization, aerosol, light
|
||
scattering
|
||
ABSTRACT: Data are presented on the polarization of light, scattered in the day-
|
||
time at differenct points in the sky in various localities principally along the solar
|
||
almucantar. The observations showed, that at the same atmospheric optical thick-
|
||
ness, the degree of polarization (P) is approximately 10% less when dry aeIrosols
|
||
predominate over moist ones. If multiple scattering is assumed to be nonpolarized
|
||
and independent of the azimuth, then the computer degree of aerosol component
|
||
(P.) polarization is independent of atmospheric transparency. The mean value of
|
||
Pa in a location with predominantly moist aerosols was found to be greater (50.3%)
|
||
r.,d 1/ 2 UDC: 525.7
|
||
|
||
WCC-NG---
|
||
AR6035286
|
||
than with predominately dry aerosols (28.5%). In computing P a, molecular
|
||
anisotropy was not taken into account. which reduces the values obtained by
|
||
2-3%. It is assumed that the differences observed in the degree of polarization
|
||
are explained by the difference In the polarization proportion of dry and moist
|
||
aerosols. [Translation of abstract) (SPI
|
||
.SUB CODE: 03
|
||
|
||
|
||
|
||
|
||
|
||
0 a 0 0 0 a
|
||
is 16 IF J7 n J4
|
||
AI R_j_j Is is -Y m so is v u 14 is 1. 1: a J. c 41 At &I CEO
|
||
f 1, 0 p a _J~I~AA_M j_', ~ I, e, 4 6 - _ 't~ _ & , 0
|
||
If 'o. C.D(.5
|
||
I..~Ctm
|
||
TM PrOW16 of crww ov Pedolov (U. S. S R-) 36.
|
||
116-107(1931).-P. ckm t1w knostion ambi an nwks in the Dnicprr Rivemr.
|
||
00 ir Analywo ad saw MMPJM AM SJWM. Mb*Wbq thilit 11111BUY tJ Ok-111 00111,lin 161 it. whkb,
|
||
spimmustly I the dark mokir. Tlw wminsweve amstitticuls founal in t1w cervatem
|
||
a AM PJ11(j. JIML111111 WSICC, IN Wkkb OW MIND MIJ Ft SFV in 11W hilng 4 b"fINNIIAM ashesna
|
||
Vat d6mmy of awls cruou in any tergiist cues. thwer-
|
||
luce. twl 1w taken as am bodimmum CIO a ebeorii type of chumter. I I Joffe
|
||
all
|
||
~40 0
|
||
06
|
||
As 5 a - I I, A of TALLVRfK4L LITERSTWE CL41WOCATPCO CV
|
||
u A .1 N is is, *A
|
||
ooe 60 o" S" o" 0"o o'0 Go 0 o" 0 1is* 00 0 0 0 0
|
||
0 0 0 0 0.0 0 0 0 0 0 0 0 0 0, 0 00 00 00 0 0 0 c 0 0 0
|
||
|
||
rTASKCVSKIY, ~,. V.
|
||
|
||
PYASKOVSKIY. B. V.
|
||
|
||
What Is Loess? Materialy po Inzh. geologil, No 3, 1953, 56-68
|
||
The aughor analyzes the ideas of L. S. Berg, who explained the origin
|
||
of loess from the viewpoint of soil-formation processes and refuted the
|
||
aeolian theory. In theformation of loess two stages are distinguished:
|
||
accumulation of fine earth (the matrix of loess), and its process of loess
|
||
form1nF. The author's orinion is that loess is formed under the humus layer
|
||
of steppe soils and Is P. conT&ent part of their profile and that loess is
|
||
a Ilime melkozem Z fine earth_/ of dust-like mechanical comrosition possessing
|
||
a number of characteristic signs. (RZhGeol, 1, 1954)
|
||
SO: W-31128), 11 Jan 55
|
||
|
||
USSR/Goology - Dosert soils
|
||
Card 1/11 Pub. 86 25/35,
|
||
AuthorsPyaskovskiy., B. V.
|
||
TitleDid a desert exist, in southern Ukrainia during the Pliocene 1.e h?'
|
||
POP
|
||
Periodical.I Priroda 44/2.- 115 U6,,, Feb.I: 1 .955
|
||
AbstractI A studyis made' 'of:the.loese-soll in,the southern part Of the
|
||
Ukraine, In 1914 this
|
||
scientis,t,,I* Levinskiy.,Idiscovered
|
||
.
|
||
ed'rock covered by: a~
|
||
beneath a thick layer of clay rounde'd-off brick-r
|
||
l
|
||
black shiny coating., which could be attributed.t6 I'desert,burno
|
||
This is,found at..Kherson and near Odessa.: Against the desert-
|
||
theory are the findings of,other scientists attributing the
|
||
formations described to other causes, thus leaving the question
|
||
in doubt. Two USSR references (1914 1931). Illustration.
|
||
InatitutionState Scientific Research Institute of Rock Chemical Materials
|
||
Submitted
|
||
|
||
|
||
|
||
|
||
SfMMp A.N.; ~IYASMVSKIYI B.V. [Pliaskovslkyi) B.V.]
|
||
|
||
|
||
(HDtts V.)
|
||
|
||
PYASKOVSKIY. B.V. [Piaskovelkyi, B.V.j
|
||
|
||
(Relativity 0Physic~)) (Slace and time)
|
||
|
||
|
||
|
||
|
||
|
||
KOROSTELEVAj, 0.1.; PYASKOVSKIY, S.V.; BYCHKOVA, G.I... red.
|
||
[Annotated bib2iography of the literaiure on machine ac-
|
||
|
||
|
||
|
||
|
||
|
||
- .
|
||
|
||
0 0 0
|
||
JV if )j H 14 L, AS 11 40 4) Aj 1)
|
||
A -j-A-1 14 M EV
|
||
A
|
||
ft, 1.0 C'0(01
|
||
00
|
||
00
|
||
of &
|
||
-00
|
||
00 -00
|
||
of -00
|
||
00 .00
|
||
.00
|
||
..S.-Olim Uitim 18 go 4 331)-N(1VWM1.T- .600
|
||
of mqo. OW zz;;; ;~ the wask.way ti.
|
||
a bd few. diffww "Wholism, As pop we U d,
|
||
00 .3 , chow of ansit"Y. dxw OW AAM bmths. -W
|
||
InfraredwWostitive Pkin we dhmmmd.
|
||
06 F. H. Rathmann
|
||
00 ILO 0
|
||
so a &POO
|
||
*OR
|
||
5.
|
||
'00
|
||
t:oo
|
||
'00
|
||
LITINATUSE CLASUPOCOTPOW boo
|
||
5 L A M41ALLUOrKAL
|
||
via., 42.111v
|
||
141041 -&- QML viiw *'..c
|
||
- q I it 1 -- _0 -3 F 111AL %*ado mawous"a 11,9911,
|
||
it p ft to go d a a If a 19 a tt it a "a n I im doe
|
||
0 0 *see o 0 0 :i0 0 o 0 o 0 q 0 o 0 o 0 o * 0 o o o M
|
||
eOo::!:::::::::::00*0e0G 00000060090900099041/
|
||
|
||
|
||
|
||
Producer: iText<78> 5.5.5 <20>2000-2014 iText Group NV (AGPL-version)
|
||
CreationDate: Fri Dec 30 23:48:16 2016
|
||
ModDate: Fri Dec 30 23:48:16 2016
|
||
Tagged: no
|
||
Form: none
|
||
Pages: 100
|
||
Encrypted: no
|
||
Page size: 612 x 792 pts (letter) (rotated 0 degrees)
|
||
File size: 4221333 bytes
|
||
Optimized: no
|
||
PDF version: 1.4
|