SCIENTIFIC ABSTRACT LEVIN, B.YU. - LEVIN, D.I.

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• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R000929520008-6
• Release Decision: RIF
• Original Classification: S
• Document Page Count: 100
• Document Creation Date: November 2, 2016
• Document Release Date: August 23, 2000
• Sequence Number: 8
• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT

Problems in Cosmogony SOV/1415
TABLE OF CONTENTS:
ARTICLES
Magnitakly, V.A. On the Origin and Evolution of Continents
and Oceans 5
Baranov,, V*I~ Latest Data in Determining the Earth's
Absolute Age 39
,Levin Be Yup History of the Moon's Rotation and the
geld-;gical Properties of Its Material 56
Safronov, V. S. On the Growth of Terrestrial Planets
Alfven,, He On the Origin of the Solar System Ti
Kipper, A. Ya. and V. Me Tiyt. Disintegration Processes
In Light Quanta and Their SigniEioance in the Physics
of Gaseous Nebulae 98
Sobolev, V.V. Physics of Planetary Nebulae 112
Gurzadyan, GeAe Dynamics of Planetary Nebulae 15T
Minin, I~N~ Light Pressure and the Dynamics of Planetary
Nebulae 211
Card T/9

Problems in Cosmogony SOV/1415
Agekyan, T*A* Interaction of Stars with Diffuae Matter 221
Kaplan* So A* Magnetic Gas Dynamics and Problems of
Cosmogony 2-,18
Parkhomenko, P.G. On the Preservation of Continuance
in the Formation of Elements 265
Parkhomenko., P,G, Determining the Location of an "Equi-
ponderant" Thermonuclear Medium 269
Pikellner, S*Bo On the Theories of the "Equiponderant"
Origin of Elements 273
Naan, G*Io The State of Cosmology Today 277
REPORTS
Kukarkinp BoV. Conference on Variable Stars Sponsored
by the Hungarian Academy of Sciences and Hold in
Budapest on August 23-28, 1956 333
Terletskiy, Yao P. Symposium on Problems In Electro-
magnetic Phenomena in Cosmic Phy sios 334
Kholopov,, P*No Conference on Non-Fixed Stars 338
Voronteov-Vollyaminov,, B.Ao Conference on the Physics
of Planetary Nebulae 354
Card 8/9

Problems in Cosmogony SOV/W5
Ruskolo Ye, Lo Conferenoe of the Committee on Cosmogony
Devoted to Examining the Possibilities of the De-
velopment of Extragalaotic Astronomy and Cosmogony 359
Taitsin, F*Aq The Sixth Coamogohic&l Coftference 361
AVAILABLBi Library of Congross
MM/91,
4-1 59
Card 9/9

AUTHOR: Krinov, Ye. L. 7-1-11/12
TITLE: Chronicle: Internutional Conference on Interplanetary Matter
(Khronika: Mezhdunarodnaya Konferentsiya po =enhplanetnoy
materii)
PERIODICAL: Geokhimiya, 1958, Ur 1, pp. 96-96 (USSR)
ABSTRACT: The International Congress on Interplanetary Matter took place
at Jena, German Democratic Republic from October 7 to October
12, 1957- It was organized by the German Academy of Sciences.
About 100 representatives of 11 countries took part in it.
The Soviet Union was represented by Ye. L. Krinovt Scientific
Secretary of the Comittee for Meteorite Science of the Aft
USSR, by the Scientific Aosistant of this comittee L. G.
Kvaoha, and by V. S. Safronov, Scientific Anuistant of the
Institute for Geophysice of the Ali USSR.
The Soviet delegation gave ton of the thirty reports heard
there:
V. G. Fesenkov, Member of the All USSR: The Vorthern Zodiacal
Light
V. G. Fesenkov, Uember of the AN USSR: The Pressure Wave at
Card 1/3 the Fall of the Tungusska Meteor in l9oS

Chronicle: International Conference on Interplanetary Matter 7-1-11/12
Ye. L. Krinov: The Mechanism of the Destruction of Meteoric
Bodies in the Atmosphere, and Their Original
Forms
L. G. Kvasha: Certuin Types of Stone Meteors
B. Yu. Levin: On the Uistory of the Investigation of the
Variation of Meteorite Frequency
B. Yu._Le-In" The Origin of Meteors and Comets
y
Member of the AN USSR, 1. K. Zadorozhnyy and
K. P. Florenskiy: The Contents of Inert Gases in the Sikhote-
Alin Iron Meteor (published in CC, 1957, no. 6)
N. N. Pariyakiy and L. M. Gindilis: Investigation of the
Luminiscence of the Green Band 5577 in the
Night Sky in the Counter-Glow Region
(Idaledovaniye evecheniya zelenoy linii 5577
nochnogo neba v oblasti protivosiyaniya)
I. S. Shklovskiy: The State of Ionization of Interplanetary
Gas and Its Significance for Certain Geophysical
Problems
The conference decided to publish all reports in special
editions of the following periodicals:
Card 2/3 Astronomical reports in; "Die Sterne";

Chronicle: International Conference on Interplanetary Matter 7-1-11/12
Reports on the material consistency of meteoritea in:
%lemie der Erde".
AVAILABLE: Library of Congress
1. Reports-BibliograptW 2, USSR
Card 3/3

LF-70, -RIYU,
Tenth International Astronomical Congress In August 1958, in
Hoscowo Part 2: Symposium on the origin of the Earth and planete,
Gookhimiia no.7:691-692 158. (HIRA 12:2)
(Earth--Congresses)

[F,VINj B. YU.
"The History of the Motion of the Mo(~n and abutit Gc(,lrjwl(,aL Prol)ertler,
of Its Material."
"Remate of the nemetical Investigatim of the Tbermal Ristory of awe an&
the Moon." B. Yu. TATIns Wyeftj 8, V. azA Banbashor, X. P.
Report promoted at the r1enary Wet1% of the Co=dttee of Plawtary P*aicg,
comen or wtrmmrs, martkov.. 23-22 may 1955.
Not. Ak Nauk SM., 19A, no. 8v P- U3-114)

UMN# B*Yuel OWHIMBUT, G,L.
.
Origin of motoorite, choadris, Metooritika no-16130-36 138,
(Meteorites) (MIRA 11:8)

PHASE I BOOK MWITATION 6UV/4538
Levin,, Boris Yullyevich
Proiskhozhdealye zemli I placet (Origin of the Earth and Planets) 3d ed., eni.
Moscow Fizmatgiz, 1959. 82 p. (Series: Populyarnyye lektsJi po astroncmii,
vYF- 3~ 20,000 copies printed.
Ed.: L.V. Samsonenko; Tech. Ed., Ye.A. Yermakova.
PTIRP(SE, The booklet is Intended for the general reader interested In astroncmy.
This lopular science booklet presents basic data on the structure of the
solar system and discusses various theories on the origin of the Earth and plan-
The theories of O.Yu. Shmidt on the formation of the circumsolar gas-dust
~-loul and the origin of planets is expounded in some detail. The compatibility
b4!tveen Shmidt's theory on the origin of the earth and A.I. Oparim's theory an
the origin of life on the earth is shown. No personalities are mentioned. There
am 3 references, all Soviet.
TABLE OF CONTEM:
InVi6d6tion
C64Y& 1/ 2
3

gk
all a
do v

Uff IN, B. Tu.
History of studying variations in meteor numbers, Biul.lonopo
konst. I meteor. AN SSSR no.4:3-8 159. KRA 13:4)
1. Institut fisiki Zemli in. O.Yu.Shmidta AN SSSR.
(Meteors)

3(l) SOV/26-59-10-4/51
AUTHOR: Levin, B.Yu., Doctor of Physical and Mathematical
Sciences
TITLE: The Development of Planetary Cosmogony
PERIODICAL: Priroda, 1959, Nr 10, pp 19-26 (USSR)
ABSTRACT: Cosmogony is no longer limited to the problem of the
origin of our planetary system. Cosmogony today em-
braces the subject of the origin of giant stellar ga-
laxies, planetary systems in general and, finally,
the origin of atoms of various chemical elements which
constitute the universe. All contemporary scientists
are of the opinion that planets were formed of a
gaseous dusty and perisolar cloud. However, they dif-
fer upon the origin of this cloud. Only American
astronomcr G.P. Kuiper and Soviet Academician V.G.
Fesenkov suppose a decay of the protoplanetary cloud
into giant protoplanets. Kuiper Wio has brought the
basic ideas of German physicist C.F. von Weizsgcker
Card 1/3 into the form of a self-consistent theory, thinks that
L",

The Development of Planetary Cosmogony SOV/26-59-10-4/51
the formation of protoplanets took place in darkness.
WeizsUcker's hypotheses were supported by Soviet
Academician O.Yu. Shmidt (deceased) who stated that
the planets were formed of numerous bodies rotating
around the sun. Later on it was found out by Soviet
scientists L.E. Gurevich and A.I. Lebedinskiy that the
bodies were formed of a gaseous and dusty cloud near
the sun. Similar to both Soviet scientists, American
physicist and chemist H. Urey also starts from the che-
mical composition of planets. The author also men-
tions the now theory as propagated by British scien-
tists T. Gold and F. Hoyle, the so-called steady-state
cosmology which assumes that progressive dispersal of
galaxies does not lead to rarefaction of the space
of the universe since their place is taken by younger
galaxies. Goldschmidt's statement that stony meteo-
rites probably are an analogous material of the sili-
cate crust was later confirmed by Soviet geochemist
A.P. Vinogradov experimentally. Some years ago, the
theory of a step-by-step formation of crust was sug-
Card 2/3 gested by V.A. Magnitskiy (USSR) and J. T. Wilson

29662
$116 61/000/005/019/049
0 A005Y,130
AUTHORS Levin# B*Yuo
TITUlt The distribution of true radiants of meteoric bodies with a
nass up to a definite limit
PERIODICAL# Reforativnyy shurnal, Geofiziks., no. 5, 1961, 7, abstract 5 0
49s (V obvi Issledo-ionoefery i aeteorov, no. 2. Moscow,
All SSSR, 1960t 54-60)
TEXTs In an such as the concept of spatial density of meteoric
bodies asks* sense only when the bodies are understood to have a mass up
to a definite limit, the author emphasizes the necessity of taking into
account the physical factor (in addition to the kinematic factor) when
determining the said density from radar and visual observations. He shows
that the number of particles with direct motion is greater by a hundred
times than those with inverse notion. The distribution of the true ra-
diants of seteorio bodies has only one "label', which is very stretched out
in the direction of the antapex, where the density of true radiants ex-
Card 1/2

LEVIN, D. Yu.
Concerning the Th anal History f the I-Soon.
report presented at the International Symposium on the moon, held at the
Pulkovo Observatoryp Leningrad.. USSR, 6-8 Dee 19W.

MSE I BOOK MLOITATION SOV/4290
BOV/37-S-38
Akjademlya nauk SSSR. Kcmitet po, meteoritam
Mateoritika; sbornik statey, vyp. 18 (Meteoritic's, Collection of Articles, No. 18)
Moscow, AN SSSR, 1960. 1,200 copies printed.
Ed.* V.0. Fesenkovq Academician; Deputy Reap. Ed.: Ye.L. Krinov; Ed. of Publishing
House: I.Ye. Rakhlin; Tech. Ed.: A.P. Guseva.
PUFdM: This publi'cation is intended for astrophysiciStO, astronomerejand geolo-
gists, particularly those interested in the study of meteorites.
COVERAGE: This collection of 26 articles on problems in meteoritics includes the
Transactions of the Eighth Meteoritic Conference which took place in Moecow,
June 3'- 5# 1958. An Introductory article reviews recent progress in the field,
particularly in the matter of determining the age of meteorites. Individual
articles discuss the fall., physical and chemical properties, and age or meteor-
ites*. The danger presented by meteors to artificial earth satellites in dis-
cussed. V.G. Fesenkov describes the theory and adduces ccmputations for
Card 1/5

Meteoritics; Collection of Articles, NO. 18 SOV/4290
determining the distribution of ozone in the atmosphere during lunar eclipses.
Refe"noss accompexq individual articles.
TABIZ OF C I
TRANUMONS OF ZIE HIaM XLVEORMC COVERUCE
tesukorp V,G.., Academician. Major Recent Achievements in Meteoritics
Xr:Lnov,, Te.L. Results of the Study of Tungusskiy Meteorite rall
(Synopsis of the Report) 17
Stanyukovichp K*P. Effects of the Fall of IAm Meteorites
(Synopsis of the Report) 19
Levin,_B,_'rq. Artificial Earth Satellites and Keteoric Bodies 20
Aaloe,, A. 11metza.Craters in the Estonian SSR 26
Bonev, No (Soft&, Bulgaria), The Origin of Asteroids and Meteorites 32
C ard 2/5

Meteoritics; Collection of Articles, no. !8 SOV/4290
Starik, I.Ye-, E.V. Sobotorich,, and M.M. Sbats. Determination of the
Age of Meteorites by the Lead-Isotopic Method 88
Vinogradov, A.P., Academician, I.K. Zadorozhnyy, and K.G. Knorre.
on Argon tu Mfteorites', * 92
Gerling, E.K., and L.K. Levskly. Products of Cosmic Radiation in the
Sikhote-Alinskiy Meteorite 100
0
Pokrzywnickip Jerzy (Warsaw, Poland). Meteorite Zab ritea 1o6
Bgatov, V.I., and Yu.A. Chernyayev. The Meteoric Dust in Schlich
Sampled 111
Yudin, I.A. Finds of Meteoric Dust in the Area of the Kunashak Stone
Meteorite Sh&er 113
Ovchinnikova,, T.N. Educational Exposition ou Meteoritics in the Muse=
of Earth Sciences at Moscow State University 119
Card 4/5

4
EM, 0'*
Meteo.ritics; Collection of Articles,, No. 18 SOV/4290
ARTICLES
Fesenkov, V.G., Academician. On the Theory of lAmar Eclipses 125
Krinov, Ye.L. Some Considerations on the Collection of Meteoric Substance
in Polar Regions 136
Zadorozhnyy, I.K6 Mass-Spectral Determination of Inert Gases in Iron 141
Pencher,, N.P., Poncheva, Ye.N.1 &n& Bonchev, P.R., (Sofia, Bulgaria)
On the Chemical Composition of the Gunoshnik Meteorite (Bulgaria) 144
Win., I.A. Minerdographic Investigation of the nikollskoye, Stone Meteorite 147
Kolcmenskiy,,V.D. Results of the Roentgananetric Investigation of the
Nikollskoye Stone Meteorite 155
AVAILABLE: Library of Congress
Curd 5/5 JA/ dvv/g"

1"1N, B. .YU. H&YWVA, S. V. 0. Schmidt last. of Physics of the Earth,14oscov.
A
"On The 7hermal History Of The Moon."
paper presented at TAU Symposium on the Moon, Leningrad, ussR, 6-8 Dec. 60.
Calculations of the heating of the initially cold Moon by radiogenic heat have sho
that Moonts interiors =at have been completely or partly melted in 0.5 - 1-5 x 1T
years after its formation., the time interval depending on the assumed content of
radioactive elements. If the melting was complete, the solid external layer should
break amd sink down. In the case of partial melting the Impacts of great
"planetesimals" were needed for lava flows.

s/o4g/60/000/02/007/022
9131/9459
AUTHORS: -Levin, U.Yu. and Mayeva, S.V.
TITLE: On the Thermal History of the Earth -v
PERIODICALsIzvestiya Akademii nauk SSSR, Seriya geofizicheskaya,
1960, Nr 2, pp 243-252 (USSR)
ABSTRACTI Thermal calculations of the originally cold Earth are
given. Models of the Earth were considered which had
different radioactive elements, specific heat of the core
and thermal radiation. The formation of the crust in
assumed to have been a lengthy process lasting 3 x 109 years.
The calculated effect of the thermal radiation, together
with the thermal flow was found to agree with observational
data in the case of smaller content of the radioactive
elements. A comparison of the theoretical results for
both the continental and oceanic regions of the crust
showed that the difference between their thermal flows is
smaller than that relating to the thickness of the crust.
This difference Is caused by the flow being affected not
only by the crust itself but also by deeper layers. This
fact explains why the thermal flows of oceans differ from
Card 1/2 those of continents. The results of investigations are /

89064
9/5%60~007/000/002/007
311 0 (/,o q to , //0 B123 20
AUTHOR: I-L-0-vt-nj -B-Yu-
TITLE: Distance@ and masses of planets
PERIODICAL., Yopromy kosmogonii, V. 7, 1960, 55-58
TEXT: A very important problem of planetary cosmogony in discussed here.
Various processes taking place in the protoplanstary cloud are dealt.vith
in connection with mutual distances and masses of the planets. The author
wanted to find a oorrelation between th;;;)t;o quantities. 0. Yu. Shmidt
hold (Dokl. AN 85SHt Vol. 52t p. 6731 1 hat when two evolving planet
come too close to each other# they will enter Into some sort of competitl
which will establish the distance between their orbits# He further hold
that every planet has a sharply defined space of its own from which it draw
matter during its evolutiong and that mass is uniformly distributed. He
used a straightforward formula to represent the distances of terrestrial
and even more distant planets. L. E. Gurevich and A. I. Lebedinakiy stated
in 1950 that the planets must have formed from the protoplanetary dust
cloud around the Sun. At first, they traveled nearly on a orbit, in the
Card 1/3

S75A5Y5) 60/007/000/002/007
B
Distances and masses of planets B123 B201
plans of the disk from which they had originated, and later entered oth or
orbits, This process is very complicated, and only a few laws have been
found for it. The planets caused an extremely violent disturbance in the
deneer parts of the dust system. The larger planets acquired matter from
larger zones. This is the reason why these planets arranged themselves at
greater distances from one another than the terrestrial ones. This also
explains the correlation between masses and distances to which Kuiper
referred in connection with both plaAets and moons. Since evolving planets
were the largest bodies of their respective regions, they caused a great
disturbance in the motion of other bodies. Masses decrease from Jupiter to
Neptunal these planets have about the largest mass a planet can possibly
acquire by absorption of other bodies. Their mass depends only slightly on
the original amount of solid matter present in the region. V. S. Safronov
has found that the mass of solid bodies and particles distributed in the
zones of Uranus and Neptune corresponds to their present masses; the plarets
needed a time of 1011-1012 years for their evolution. Oort's planetary
cloud was formed by particles hurled onto a parabolic orbit. Kuiper men-
tioned a number of facts which, in his opinion, are indicative of the
existence of massive protoplansts at an early period. Some of these facts
Card 2/3

Distances and manses of planets
8W64
8/555/60/007/000/002/007
B123/B201
have been explained from an opposed viewpointg by the assumption of a plane-
tary accumulation* .(Among these facts are the chemical composition, the law
of planetary distances# regular and irregular satellites# mad the existence
of asteroids). A decrease of the mass of protojupiter is, however, required
in Rabe's calculations to explain inclination and eccentricity of the orbit
of Mercury# The author notes that if matter is hurled out to more distant
regions from the region of formation of planetary giants# this must neces-
sarily lead to a decrease in mass. There are I table and 6 references:
4 Soviet-bloc and i non-Bovist-bloo.
ASSOCIATION: Institut fisiki Zemli im. 0. Yu. Shmidta Akademii nauk SSSR
(institute of Physics of the Earth imeni 0. Yuo Shmidt,
Academy of Sciences USSR)
Card 3/3

855ho
S/026/60/000/009/005/010
(1PS'71 /vop/ 2.~ A166/AO29
AUMORs lAffin, B.tL,_
TITLEt The Origin of Comets
PERIODICALt Priroda, 1960, No. 9, PP. 10 - 13
TMM The author discusses various theories on the origin of comets.
Oort2a theory is that the solar system in surrounded by a cloud of comets, or
rather comet nuclei, which serves as a source for the replenishment of all ob-
servable comets. Replenishment is needed because the comets tend gradually to
disintegrate In their approaches to the nun. Academician O.Yu. Shmidtla cosma-
genic theory given a simple explanation of the formation of comet nuclei and
their involvement in 0ort's comet cloud. The cloud originated as follows: due
to friction against the gases and Intercollisions among themselves, the particles
settled to the central plane of the cloud, forming an Increasingly packed disc.
Because of the disc's opacity, only its narrow Inter zone was heated by the sun,
while the vast outer part remained cold, In the inner zone the solid particles
consisted only of fusible non-volatile substances, while In the outer part al-
most all the gases in the cloud condensed onto such particles (with the exception
Card 1/3

85540
The Origin of Comets
S/026/60/000/009/005/010
A166/AO29
of inert gases and, possibly, also hydrogen). Because of gravitational instabi-
lity, the disc split up into a myltituds of "clots" which then turned Into bodies
of asteroid dimensions. Collisions between these bodies led to their amalgama-
tion, and sometimes to their disintegration, in which case the fragments were
again drawn into the amalgamation process. _Amalgamation processes predominated
and led to the formation of today's ejAE94"from the matter of the intermediate
bodies. The differences in the chemical composition of the particles In the
packed disc were perpetuAted in the form of two groups of planets-, planets of
the Earth type and the giant planets. The Intermediate bodies and their fragmen 4:'S
In the Slant planet zone must have consisted of mixtures of fusible Wticles and
various "ices", i.e., the same composition is is assumed for the comet rpiclel In
Whipple's ice model. The orbital divergence mechanism which led to Jupiterle
ejection of part of its asteroids into the comet cloud oust have been effective
for the whole giant planet zone and therefore Jupitez, Saturn, Uranus and Nep-
turie-must all have participated in the formation of the comet cloud. In the
giant planertal case the escape speed at the surface of the planet was many tIme2
greater than the difference between the parabolic wid the circular speeds at a
corresponding distance from the sun, while In the case of the earth they were
Card 2/3

LF,VIN, B.Yu.
Artificial earth satellites and moteors. Mateoritika no.18:
20-25 16o. (MIRA 13:5)
(Artificial satellites) (Moteors)

JMOLOPOV, P.N., kand.fiziko-matematicbeakikh nauk; LITIN, S.Tu.;
103TTLEY, X.T.
In the Astronomy Council# Yeat.0 SSSR 30 no.9 99-102 3 160,
(Astronomy) (MIRA 13:9)
" '114
7 .-. III L.

81
8/020 60/TI1353/01/12/070
V.
B014)BO1I
AUTHORS: Levin, B. Tust MayeYar S. V.
1000~~ \1
TITLE., Some Calculations of the Thermal History of the Moon
PERIODICAL: Doklady Akadsmii nauk SSSRI 1960p Vol. 133# No. 1,
pp. 44-47
TEXT: By the calculations under review the authors try to explain the
development of the Moon with the accumulation of cold bodies. The beat
balance of the Moon Is assumed to be determined by its radioactive sle-
monts. In accordance with Vo S. Safronov, the Moon is assumed to have
original;d 0.23*10 9 years ago, and at its surface) temperature is assumed
to be 0 at all times. In the selection of the content of radioactive
elements the authors bass on analyses ofAsteorityA made by A. P. Vino-
gradov and others. The heat conductivity Is assumed to be
X = 1.2,10-2 Cal/omesso.gradg and the heat capacity to be 0.2 cal/g.grad.
Calculations made under thee* assumptions and discussed here were carried
out with the bydrointogrator devised by V. S. LuklyAnoy at the
Card 1/4

81
Some Calculations of the Thermal History 3/02 60 133/01/12/070
of the moon B014Y3011
Teentrallnyy nauchno-isoledovat*lfekiy institut stroitalletva Mintranostroy
(Central Scientific Research Institute for Construction of the Mintranestroy).
OZoulations or the initial heating of the Noon are ti-e-a-i-ea xirst. For "a;'~"~
density of 3-3 9/cm3 t4s authors obtain a temperature in the center of
the Moon, which in 190 C higher than the surface temperature, The beginning
of the melting process in the center is approximately obtained at the
time t - 0-5o109 (with an age of 0.23-109 years being assumed for the 9
Moon) for a variant of the content of radioactive elements and t - 0.7 .10
for another variant. In a detailed discussion of the processes which
axose in the melting of the Moon it in shown that a thin solid shell,
which is denser than the underlying malt, could not exist. MorsoYst,
the transition from the heating and melting of the Moon to its cooling
and solidification was accompanied by a reduction of radioactive elements.
This reduction was caused by the natural decay and by the surface losses
of the Moon. In a calculation of the cooling process of the Moon it is
shown that about 3 - 3.5 billion years after the Moon began to cool, the
original temperature distribution made itself manifest. Xoreover, the
temperature depends on the distribution of radioactive elements and on
1411
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Some Calculations of the Thermal History 4620/60IR9/01/12/070
of the Ifoon B014/BO11
heat conductivity. The model of the Moon for which the cooling was
calculated Is shown. This model features an iron core (r - 685 km) and
a shell. The content of radioactive elements In taken from analyses of
iron meteorites according to A. Go Starkova (Ref. 2). The authors con-
olude from the results obtained that the shell has today a thickness
of 500 - 700 ka.-that the layer underneath is not completely molten, and
that the iron core has melted to at most 15%. It is finally stated that
the temperature distribution today Is primarily dependent on the content
of radioactive elements, and that the shell is at least 500 - 700 km thick.
There are I figure and 6 references: 5 Soviet and I American.
ASSOCIATION: Inatitut fisiki Zemli im. 0. Yu. Shmidta Akademii nauk SSSR
(Institute for the Physics of the Earth imeni 0. Yu. Shmidt
of the Academy of Sciences,_02R3
PRESENTED: March 12, 1960, by V. A* Ambartoumyan, Academician
Card 3/4

Some Calculations of the Thermal History
of the Moon
SUBMITTED: March 2, 1960
81 15
S/020/60M3/01/12/070
B014/BO11
~r
Card 4/4

8/169 63/000/002/002/127
D263YD307
4UTHOR I z _r_S1zkL1
ILE:*
TIT ''13r'eakdown of meteoric bod
Us and meteoric assessments
of atmospherio,density
PERIODICALs Referativnyy zhurnal, Geofizikaj no. 2, 1963, 15, ab-
stract 2A85 (Byul. Komie. po kometam i meteoram Astron;
..soveta AN SSSRO 1961, no.. 6, 3-10 (summary in Eng.))
TEXT: Processes of meteor breakdown play an important part in the
observed meteoric phenomenag since they considerably increase the
.A meteor's glow. The author considers four main processes of diainte-4:
gration: breakdown of the*meteor into a few 'permanent' parts; pro
'lire breakdown) i.e. breakdown into parts which split up fur-
gross
ther; sizh~ltaneoua separation of fines from the main body of the
~meteor; and quasi-continuoue separation of fines from the main bo-
dy. It is p inted out that,-in practice, cases intermediate botween!
0
the above 4 main types will be observed. It is shown that calcula-
ition og.ths'breakdown index XO introduced by Yakkiat is only effec-1
lAard -1/3,:

S/169
/63/000/002/002/127
Breakd.own~ of meteoric ... _D263/10307
-tive when the breakdown is of'the -!pro-gressivel.t.Ype, for luminous
~Imeteoritee X P 0, for weak ones X = 0.35. The proble! of meteor
density-io discussed, in connection with Whipple's views, who consi-
these densities to be low# It,is shown that it is still uncer-
2 g/cm3; in
."'JI-tain just how reliable are densities such as 5 x 10-
.-~_!_._eyery,case.these densities were invalid for small granules making
up the main,part of large 'friable' meteors.-Assumption of low
:,'densities leads in consequence.to more precise definition of con-
itemporary views on the structure of the ice cores of comets. In t e
:artiole,.the author shows that in calculating the atmospheric den-
raity from meteor data it is c6ilvenient to use L. A. Katasev's for-
mula
1/3
My co'
8 z .0
dWdt

PHASE I BOOK E(PLOITATION SOV/5704
Levin, Boris Yul'yevIch, Doctor of Physics and Mathematics.
ty, -Ates) 2d
Meteorl rev . ed,,,,Moscow, Izd-vo "Znanlye,
1961. 43 P. (Series; Voeab'y'uznoye obahchestvo po rasprostranenlyu
politicheskikh i nAuchnykh znaniy. Serlya tX, 1961: Fizika I
khimiya, no. 12) 26,000 copies printed.
Ed.: I. B. Faynboym; Tech. Ed.: I. T. Rakitin.
PURPOSE: This booklet is intended for the general reader inter-
ested in meteorites.
COVERAGE: This is a popular discussion of meteorites. The author
traces the history of the scientific study of meteorites, and
describes the characteristics and properties of meteorites as
well as the physical phenomena accompanying their flight and
fall, origin, and age. Several outstanding meteorites such as
the Tungus, Sikhote-Alinl,.and Goba, and the larger meteor
craters, such as the Arizona crater, are described. V. I. Vernadskiy,
Card 1/3

Meteorites
SOV/5704
A. Ye, Fersman, A. N. Zavaritskiy, and,L. A. Kuli)c are mentioned
as the outstanding authorities on meteorites. There are 8 refer-
ences, all Soviet.
TABIZ OF CONTMS:
Beginning of the Scientific Study of Meteorites 3
Fall of Meteorites
Orbits of Meteorites
5
9
Pbysical Prooesses During the Flight of a Meteorite Through the
Atmosphere 12
Meteoritic Craters on the Surface of the Earth 15
Card 2/3

IZVIN 0 B. Tu.
Planetary perturbations and the origination of plane meteor swarms.
Biul.Kom.po komet.i meteor. All SSSR no.5:3-6 161.
(MMA 14: 6)
1. Inatitut f--~ziki Zemli imeni 0. Tu. Shmidta AN SSSR.
(Meteors)

?1741
3, 15'rd 13 S/025/61/000/006/003/007
40 9;7
., 9) D244/D305
AUTHORS: .--Ley-Ln,_ B. Yu.,_, Doctor of Physico-Mathematical Sciences,
and R-u-sW =je. L., Candidate of,Physico-Mathematical
Sciences
TITIZ: Stranger-from space
.2t
PERIODICAL: Wauka i.zhiznl no.
- on the,hypothesis of N. Bonev
6, 1961, 9
TEM. In.the third-Assue-of-I '1Nauka.,i.zhizn111,for 1961 there
was a short.accouni of a hypothesis.by astronomer.N. Bonev on
the origin.of-the-moon.. The authors.state.that this hypothesis
is.groundless. N. Bonev suggests,that initially.the moon was not
an,earth-satellite but-an.independent.planet-which.was.braked by
powerful.volcanic.eruptions.-on.passing..the earth.and then went
into orbit around it. it,is.supposed tbat.these eruptions acted
on the moon like the.motor of a braking.!.rocket. For the braking
effect to.be adequate, N. Bonev has to assume that these volcanic
eruptions.were.so strong,that the moon.lost much of its original
mass. The-possibility.of.a planet having great internal energy
Card 1/3

21741
S/025/61/000/006/003/007
D244/D305
Stranger from space
is strengthened.by reference to.the hypothetical-planet Phayton,
x4hose,explooion.is-alleged to have-given birth to.asteroids and
meteorites. One of the main reasons, however,.for the rejection
of.this particular,hypothesia.by astronomers is the fact that
thpy,have-failed to.find.the..source-of energy for such an explo-
sion.- In order to leave the moon, matter must have flown out of
the volcanoes.at a colossal speed (3 - 5 km/sec). One has to
completely exclude the possibility,of there existing in the moon
at that time,sufficient reserves.of energy for.the ejection of
most.of..its original mass. In.order to obtain a reaction effect
while ejecting-matter.to.one side, the volcanoes must have been
operating.not over.the.whole lunar surface.but only in a compara-
tively small area. The.authors-point-out that in Bonev's diagram
the explosion-is depicted.in.a direction.which.is the reverse of
that necessary,for capture by the earth. Turthermore, such a
volcanic "rocket-brake" would have been applied just when it was
Card 2/3

,, - ,
I
4aMMt=-LIv~-Dr. )
"The Modern Form of the Meteoritic Hypothesis of Lunar Belief Formation"
report presented at the 13th Intl. Astronautical Federation Congress (FAI)
Varnaj Bulgaria) 23-29 Sep 1962

IZMj Boris Yu.
"Piresent day form of the 'Meteorite' hypothesis of the lwiar relief
formation"
report to be submitted for the 13th Intl. Astronautical Congress, I",
Varna, Bulgaria) 23-29 Sep 1962.

S/555/62/008/000/002/003
1023/1242
AUTHORS: Levin, B. Yu., and Ruskolq Yet L.
TITLE: Review o' present data on the moon
SOURCE: Akademiya nauk SSSR. Voprosy. Xo9mogonii. v.8.
Moscow, 1962, 109-144
TEXT: The present review is based on Soviet and Western
sources and covers the period up to 1962.. The following topics
are discussed: 1) orbital motion, rntation, and libration;
2) atmosphere; 3) photometric data, 4) radio location data;
5) surface temperature; 6) structure of the surface layer (micro-
~elief); 7) surface relief; 8) origin, internal structuret and
thermal-history. There are 2 tables and 117 references.
Card 1/1

S/()30/62/OOO/O11/uO4/005
D21e/D308
AUTHORSt Levin, B.Yu., Doctor of Physical and
--?Z~ematical Scienceaq and Rudich,Ye.M.
TITLEs The fourth conference on astrogeology
PEHIODICALi Akademiya nauk SSSR. Vestnik. no. 11, 1962,
131 - 134
TEXTs The conference took place on May 7 - 12 in
Leningrad. The present authors report that some of the papers
read at the conference, and indeed "astro.geology" itself as
defined by the participants in this conference, must be treated
with some reservation, since there is some doubt as to their
scientific validity. Among the papers read at the conference
were the followings P.S. Voronov "Main contemporary problems
in astrogeology" Mi. Katterfelldt "Astrogeology, its contentl
probleme and place in the scienceell B.L. Lichkov, "Interaction
between the earth's shells and the conditions of Its rotation
as the cause of all the geological phenomena on the planet"
Card 1/3

5/030/62/000/011/004/005
The fourth conference D218/D308
B.h. Lichkov and I.I. Shafranovskly, "The universal importance of
some angular quantities characteristic for the earth" G.N. Katter-
fel'Id, "Fregeological era in the history of the earth and its effect
on the evolution of the geoid" P.S. Voronov, "On the rotational
causes of tangential stresses in the lithoaphere and some of their
geostructural consequences." M.V. Stovae, "The effect of external
factors on the seismicity of the earth." A.V. Shnitnikov, "Tidal
force as a factor in landscape dynamics." Papers vere also read
by F.P. Krendelev, I.G. Klushin, A.A. Xhlobustov, R.I. Burtman,
V.S. Vasillyev, A.V. Volin, V.S. Voropinov, A.V. Dolitskiy, 0.1.
Islamov and G.G. Tamrazyan, but the present authors find them-
selves unable to take them seriously. The remaining papers weret
G.G. Khizanishvili and M.V. Klenova, "The origin of submarine
terraces in the light of the rotational dynamics of the earth."
V.A. Buning "Hecent problems in gravitation In the light of classi-
cal physics." B.V. Timofeyev, "On the discovery of organic resi-
dues in stony meteoriteaft. G.U. Lindberg, "On geocratic oscil-
lations in the ocean level.,, V.A. Zubakov, "Absolute dating of
glaciation in the last 70,000 years." V.V. Kochegurt "Paleomagnotic
Card 2/3

B/030/62/000/Oil/004/005
The fourth conference D218/D308
studies of busalts In the :joviet Far East." V.S. Lebodov, "For-
mation of chemical elements In meteoriten under the action of
cosmic rays." V.F. Derpgollts, "The 1hydrochlorospherel as a
planetary zource of all natural water in the outer shells of the
earth." V.I. Vullfson# "Free oxygen in the earth's crust." The
resolution of the conference noted that the conclusions reached
in many of the papers were not sufficiently well argumentedq but
nevertheless, it was recommended that the proceedings of the con-
fer,ence should be published. The present authors are highly scepti-
cal about the entire venture.
Card 313

S/556/62/000/030/001/005
D218/D308
AUTHOR: Aevin B. _ Yu.
TITLE., The present form of meteor hypothesis rlo"garding the
formation of the lunar relief
SOURCE: Vsesoyuznoye astronomo - geodezicheskoyi obshchestvo.
Byulleten'.. no. 30 (37). Moscow, 1962, 6-19
TEXT: This is a review paper showing the present state of the the-
ory according to which lunar craters were produced by meteors. The
following problems are discueseds 1) Is there an agreement between
the history of bombardment of the lunar surfacp And the thermal '
history of the lunar interior? 2) Why are there so few meteor cra-
ters on the earth? 3) Is a random distribution of craters to be
expected? 4) Is there a superposition of large craters on small
ones? 5) Is there an agreement between the distribution of crater
& and planetesimal sizes? 6) Do the craters and maria form a single
sequence? 7) Does SchrUter's rule hold? 8) Are lhe~e currently ac-
tive valcanoes on the moon? 9) Are there apertures in the central
ca. Card 1/2

5/030/62/000/002/001/009
B105/B110
AUTHORi Levin, B. Yu., Doctor of Physics and Mathematics
TITLEt Origin of the earth and problems of its structure an4 compo-
sition
PIRIODICALt Akademiya nauk SSSR. Vestnik,/,no. 2, 1962, 9 - 16
TEXT: The author discusses the processes of the formation of the earth on
the basis of the hypotheses of 0. Yu. Shmidt (formation of the planets
from an originally cold protoplanetaric cloud) and the hypothesis of Ram-
ss~y. He mentions the approximately equal composition of Venus, Earth.
MArs, and the moon, the composition of the meteorites (P. N. Chirvinskij.
(1919) is mentioned), the heating of the formed bode by radioactivity, thf,,
problems of the formation of the terrestrial crust reference to geologi-
cal and seismological results) the tides of the solid terrestrial mass,
the deformation of the spheroid of the earth, and the participation of th.,
comets in the formation of the terrestrial hydrosphere and atmosphere. .".*.
the Institut fiziki Zemli im. 0. Yu. Shmidta (Institute of Physics of tht~
Earth im, 0. Yu. Shmidt) the phase transitions for magnesium were theoret4
Card 112

3/030/62/000/002/001/008
Origin of the earth ... B105/B110
cally caloulated and experimen95 were made with impact compression of du
nits. At a pressure of 1.4-10 atm no phase transition was observed A
present three main directions can be distinguished in the re3enrch wrlrk
on planetary cosmogeny: (1) study of the physicochemical development -,f
the planetary matter; (2) study of the accumulation process of the pLani-ta.-
(3) comparative study of the planets of the terrestrial group and of the
moon. The development of the theory of the origin of the earth is one of
the most promising methods for solving geophysical problems,
Card 212

AUTHOR:
TITLE:
VERIODICAL:
S/169/62/000/012/002/095
D228/D307
Levin, D.Yu.
-Origin of the earth
day of Q.Yu. Shmidt)
ber 21, 1961)
(70th anniversary of the birth-
0%uthor's paper read on Novem-
Referativnyy zhurnal, Geofizika, no. 12, 1962, 4-5,
abstract 12A10 (Byul. Mosk. o-va ispyt. prirody, Utd.
geol., 37, no. 2, 1962, 159-160).
TEXT: At present the best developed theory for the origin
of the earth in the one worked out by ,caderucian G.Yu. Shmidt and
his colleagues. The formation of the Vlanct occurred as a result
of the evolution of a protoplanetary cloud of gas and dust that
once surrounded the sun. In the first stage the dust component
accumulated into a flat disk, which then broke up into numerous
condensations that afterwards served as the nuclei of planets.
According to O.Yu. Shmidt's theory the earth can-be considered as
a primarily cold body, -md the present hot state of its interior
Card 1/2

UVIN. Bayu.
----- -
Constitution of icy cometary nuclei, Astronabure 39 no,4:70-765
J1-Ag 162. (MA 15:7)
1, Institut fiziki Zemli imeni O.Yu.Shmidta AN SSSR.
(comets)

JaVIN, B-7u., doktor fiz.-matem.nauk; RUDICH,, Ye.M.
Fourth conference on astrogeology. Vest. AH SSSR 32
no.llsl3l-134 N 162. (MIRA 15:11)
(Earth)

WIN Blyu.
0-1
Structure of icy cowboy nuclei. Astron. tair no.229:8-10
-To 062, iMMA 16t6)
1. Itistitut fisiki Zemli in. O.Yu. ShaUta AN SSSR.
(Cmets)
t

LEVIN, B.Yu.
Origin of comtso Vopskosm. 9:215-231 163. (MIRA 17:5)

LMNS B.YU.
Moons
Report submitted at the X111th International 6ongress on Astronautics in Varnav
Balgaria
P* Tomas molodeshis 13.9 19639 pp.24-25

LEVIN, B,Yu4; SAFRONGV# V.S&
Comments on D.D. Ivanenko and H.U. Sagitov's article 00n the
hypothesis or the expansion of the earths" Vest, Mosk. un.
,Seri 3t Fiz., astron. 18 no.4t"5 JI-Ag 163. (KMA 16t8)
1. Institut fisiki Zemli AN SSSR imeni O.Yu. Shmidta.
(Cosmology)

or
3/033/63/040/002/014/021
___ZOOI/8120
AUTHORs &,2vi is B.Xu a'
..~'TITLZs On the fragmentation of meteoric bodies
PERIODICALt.Astronomichookiy thurnall v9401 no*29 1963, 304-311
TEXT s': Observational evidence accumulated in past years has
shown that fragmentation in on* of the main processes determining
the course of meteor phenomena. The purpose of the present paper
in to take into account the fragmentation process in deriving the.
formulas for maximum stellar magnitudes of meteors. The data
publishod'by G#S. Hawkins and R.D* Southward (Smiths. Contrib.
'Astrophys*1 veg, lqsS_,~349).contain the range-of variations of
stellar magnitudes from the appearance and disappearance points or
..meteors to the maximum. The analysis of their photometric data for
36o meteors' taken with super-Schmidt cametas, has shown that the
observed lengths of meteor path& are shorter.than the theoretical*
~This discrepancy can be naturally explained by assuming
fragmentation of meteoric bodies rather than by adopting a
different luminosity coefficient, am is done in an ad hoe
hypothesis-by Ro Ananthakrishnan (Maturej Y,187, 196o. 673; v.190s'
1/3,
d

S/033/63/040/002/014/021
On the., fragmentation of meteoric ZOOI/E120
1961, 896), The effect of fragmentation'is manifested in an
increase of -the maximum brightness which is inversely proportional
to the path length. In stallar magnitudes this looks an followz3
m m0 + 2s5 19 f
-where f L/td* i1o the ratio of path lengths* The author
introduces a parameter F9 characterizing the fragmentation
process which does not differo according to observational data,
from the f-values. Using'data on the masses of meteors, supplied
-.by Hawkins and Southward, the author reduced the values of
maximum absiolute photographic site llat. magnitudes mM to the mass
value 'equal to g, and the, values of, thus obtained
correlated with F by the relations
+1.6o + 2*5 Ig F
which in analogous to formula (3). This relation shows good
agreement-, with,ex'erimental datao -Xt-is concluded from this that
p
~fragmentation proceeds.so intensely in 90% of meteor bodies that
Card 2/3
V
--I tP M.

S/033/63/040/002/014/021
On theIfragmentation of m6te~oric 9001/9120
there is a noticeable shortening of path lengths of meteors.
observations also indicate that the distribution of meteors over
fragmentation.paremeter F depends on their masses. It follows
hencet that the determination of the exponent a in the law of
mass distribution 6f*meteorie bodies leads to false resultal if them
effect of fragmentation is.not taken into account. Therefore* all
prevlou estimmatlons of a, based on the luminosity function of
and on radar observations, should be reconsidered.
There -are 3--figures#
ASSOCIATIONs.Xnatitut fiziki Zemli. im.'O.Yu. Shmidta Akademii nauk
SSSR
.-(Inztitute.of Physics of the Earth imeni 0&YuqSchmidt9!
AS ~USSR)
SUBMITTEDt-.'. )jarch 24s,'1962
Cayd ~3/3

LEVINg B*Yuo
Nature of the moon's surface layer, Astron.zhur, , .1,0 no.6:
1071-1(Y75 11-D '63* (MIRA I,: IT
1. Inatitut fizikl Zemli AN SSSR.

MIN Boris Yullyevich.- !IAKHLII;, I.Ye. p red.
7
[Origin of the Earth and planets] Prolsktozhdenie Ze=.Ii i
planet. lzd.4.p dop. Voskvaj Izd-vo "Nauka," 1964. 113 p.
(Populiarnye lektsii po astronomil, no.3) (EIRA 17:9)
I . I -~ 77~~

LEVINt MUG
Some actual problems of meteoritics. Yeteoritika no.24t
16-21 164. (MIRA 170)

LVVIIJ, 13.Yu.; MAYEVA, "'.V.
Anower to MoOrnataskaltils lettlr. kstron.Aur. 41
998 S-0 164. lmli~A P. 10)

LEVINY B.Yu., doktor fit.-matemat. nauk
Moon from a close range. Pr1roda 53 no.lOtll5-ll8 164.
(WFA 17silli
1. Institut fisiki Zemli Im. O.Yu. Shmidta AN SSSR, Moskva.

i 7~
'I-. IN" - - - - - -
EwT(j)/Ewa(v)/EW-4/KV,(t)/&A(d) OW
L 62697-65
jACCESSION MR: AP5013401 UR/0053/65/086/001/r)041/0069
523-51
~AUTHORs ving.B. Yu.
iTITLE: The origin of Mteorites
SOURCE: Uopekhi fizicheskikh nauk, v. 86, no. 1, 1965, 41-69
TOPIC TAGS: meteorite, meteorite compooltion, meteorite origin,
,~,,asteroid, solar system, cosmogony
ABSTRACT: This is a-review article reporting on the changes that
have occurred in
-the a6ientific explanations of the origin and nature
.,..,Of meteorites during the last decades, making use of recent Informa-
:-'Ition on the abundance of elements and their Isotopic ratios from the
,point of view of nuclear physics. The various hypotheses advanced
,.Jconcerning the nature of meteorites are outlined and the experimental,
Innel nnr-_n^&r.n1os%1' nuielanna in fKa-in j~~M iWT-.6a, V144gWrl'trA
Koft"~~~Ttte--~miri--points---Of~-view--of!-~-Urey-and-Ringwood-o- --Anders-i
Wood,--Marlon --and -the author of the paper are described In detail. The
rd

L 62697 -65
-ACCESSION NRt A9501340I
toed tioh'- hbadii*s --are.,1-tntroduction-6--2-Mateorites and asteroids.
ele-ationg 4. Cosmogonical considerations. 5.
Atmospheric a Some
p~opertles of meteorited. 6. Hypotheses of the 'fire liquid' origin
of meteorites. 7. Hypotheses of primordial nature of chondruleB.
8. Hypothesis of urtmolten parent bodies. 9. Some conclusions. Orig.
art. has: 9 figures
ASSOCIATIM None
su~TTED: 00 ENCL., 00 SUB CODE: ES, AA
NR RMF SOV,. 029 OTHERt 105
Card 2/2
N

L 42-11 EWT (I I WVMAX - - - -
ACC_NF,__D6019674 SMCZ COMBI UR/0033/66/04 21
AUTHOR i Levin. D. Yu.
CHM Institute of 0oophysics, Acad!ff. of Sciences.SSSR (In-t fisiki Zemlig Akademii
nauk SM)
TITLEs The structure of the soon V/
SOURCEi Astronomichaskiy shurnalp ve 43v no* 3P 1966,,6o6-621
TOPIC TAGSt moong lunar surfaceg lunar atmosphere
ABSTRACTs This report was presented at the Conference on the Moon and Planetep
sponsored by the California Institute of Technology and the :at Propulsion Laboratory
in P"Mensp September 1965. It reviews three theories an the origin of the soon and
Gerstenkorn's theory of the tidal evolution of the earth-moon, system. The author
favors the idea of the common formation of the earth and soon about 5 billion years
ago# which is compatible with the Schmidt-Ruskol th M of lunar origin. Three basic
stages of lunar bombardment are described as follow:t 1) the period of the final stage
of the mom's accumulation; 2) the period of the radial expansion of the lunar orbit
,wheii collisions occurred at a speed of 2-4 ka/seoi 3) the subsequent period when
bodies in solar orbit collided at 10-15 lm/eeo. Various factors and theories for
determining the therml proportion of the soon are presented. The author supports
Xeyeva's work showing that the moon has a semi-molten interior and solid exterior
COM 4 /0 nw-2 r.9%_,A

L 42314-66
ACC NRs AP6019674
(see Table
-Table
10 40 to 40
A 1. *700 1 500 Wo 430
Mean content of radioactive elements in moon as a whole:
uranium- ns10-8 C/gI thorium-- 4n-le g1g; potassium--
8.1074 gle. Data for n - 2 are reduced. Content of
radioactive elements in interior of moon after their
differentiations uranium- N-10-8 g/g; thorium- 4%'16-8
g1g; potassium- 2-5- 1074 g/g. F, - absorption coefficient.
Thermal stresses and meteorite collisions are cited as possible causes of lunar
seismic activitys Theories on the shape of the moon and the density distribution
along its radius are discussed. The existence on the moon of metallic iron, bydrous
silicatest and volatile substances is uncertain. The author agrees with the majority
of experts that the moon does not have and never has had any appreciable atmosphere.
Orige art, h"I 3 tablesp 2 graphop and 6 formu.1".
SUB 009R 1 3% am DATS I I W=661 CRIG RIFt 030/ OM RM 051
L Serd 212 ei J

ACC NRs AP6018932
AUTIIOR:jAvin, B. Yu.; Simonenko, A. N.
SOUILCE CODE: UR/0203/GG/00G/003/0G08/0G091
ORG: Institute of Earth Physics im. 0. Yu. Schmidt, AN SSSR (Institut fiziki Zemli AN SSSR).
TITLE: The disintegration of moteorto'bodies in the Earth's atmosphere
SOURCE: Gcomagnetlzrn I acronomiya, v. G, no. 3, 19G6, 608-609
TOPIC TAGS: meteor, meteor observation, atmosphere
ABSTRACT: Zhe authors dispute the contention of Ye. N. Kramer (Geornagn. I acronomiya,
1965, 5, No. 2, 27G) that the conclusions of the micrometeorito theory are applicable to the
movement of particles which have separated from a larger meteor body. Disintegration of
the meteor body Is shown to lead to an increase of a, and, consequently, to a reduction of the
residual mass. Thus, contrary to Kramer's opinion, disintegration not only does not reduce
the emission of the meteor, but rather Increases It (negligibly, since the residual masses are
small). Complete light energy emitted by the meteor Is proportional to the initial mass of the
meteor body, with disintegration leading only to a redistribution of the emitted energy along
t;ie path, without changing the sun light energy, since the proportionality between the mass
Card 1/2 UDC: 523. 6

1. L.-MNI B. YU. : CEU:.R.'A, 11. M.
2. !JjSli (600)
4. Wool-ttork
7. Work methods of progrezjive woodworkir Dolzl.,..~nko. Der. i
prom. 1 no. 3. 1952.
9. Monthly List of tussian AccesAon jLibrar-y of Congres:s, -Earch 1153- Uncla:;Gilfied.

AID P - 5390
Subject t USSR/Engineering
Card 1/1 Pub. 103 - 20/28
Author : Levin, B. Yu.
Title : Device for planing spiral grooves of rectangular profile
Periodical s Stan. i instra, 9, 349 S 1956
Abstract i The author briefly describes an attachment which facilitates
planing a shaft vith 24 spiral grooves of 622.5mm pitch. The
origina-.or is the Presnenskiy (Presnya, Moscow) Machibe-Building
Plant* One drawing.
Institution s As above
Submitted t No date

L 23368-6
J1)/j0AT/WH
AcussioN NR: AR5oOO739 S/O?-77/64/000/,309/0020/0020
SOURCEt Ref. zh. MashinostroitelOnr e material7*p konstruktsii i
raaohot dotaley mashin, Gidroprivod, Rd, Yy*pq# Abse 9*48*121
AUTHOR: SmirnovP__F,,,Fq Gurevich, L. F.; SleRanova. T.-M,-
Be Z, L-0 44 ft!~
TITLEt 0 ""perties of a now expeMnental variant of alloy
VX4 with improv strength
Jb
GI7173D SOURCE: Sb,, tr, Vaes, n,-i, In-t tvordy*IM Url"RYA no- 5,
19649 14-28
TOPIC TAGS -cutting tool, tungsten carbide,, carhide tool/
X
alloy VK48 alloy VK
7-ji
___TRANSLATIOKt__Rqsults of laboratory and plant tests of the cutting
Iproperties-of a.now inditistrial Variant of alloy VH4,, produced as a
result of the use of tungsiten carbide with a higher oarbidizing
tomporaturep are presented, The outting proportion were tested by
comparison with standard t7pes of alloys M and Me On the basis
Card 1/2

L 233"
ACCOSSION NRI AR5000739
of the tests# experimental alloy is rooo=ended for Introduation
in the operation of rouah turning of angina pistons,
SUB CODE: HK ENCL: 00
Card
-T"~Rjylra -P

RYZHAVBXIY, I.M.: SH3PEZA, H,D.; UTS, ?.A., nsuchuyy red.; LLYLY
nauchuyy red.1 YWIMO. Y.Hoo usuchrq7 red*; S12OWS", 0,
red.-, MBOV. N.B.. takha.red.
CUse of hard alloys and cermets; a collection of articles]
0 primeneuit tvardykh splavoy i minerelokeramiki; abornik statet.
Moskva. 1957. 87 P. (MIRA l116)
lo Mosoowe TSentrallnyy institut informateii tevetnor inetallurgii.
(Alloys) (Cermeta)

23MRA, TS.O.. inshener; DIAGOXAIZZHDIN. Y.Te.. Inzhener; BOGUSIAVSKIY,
P.Te., kandIdat tekhnicheakikh nauk; VORONKOV, I.M., professor.
GITINA, L.Ta., Inzhener; GROMAN, F.B., Inzhener; GOROKHOV, N.Y.,
doktor tekhnichesklkh nauk (deceased]; tENISTUIC, I.N., kandidat
tekhnicheskikh nauk; DOVZHIK. S.A., kandidat takhnicheakikh nauk-
DMLISKIT, M.P., professor, doktor khimicheskikh nauk [deceasedi;
DYXHOVICHM, A.I.. professor: ZHITIOV, D.G., professor, doktor
takhaicheskikh nauk; KOZLOVSKIT, N.S., Inzhener; 1AMIN, Yu.M..
doktor tekhnicheskikh nauk: 1XVINSON, L#B., professor, doktor tokhni-
cheskikh nauk [deceased); 1XVIN, B.Z., in2hener: LIFKAN, V.F., inzhe-
nor; XARTTROV, M.V.. kandiU-T-TAhfilchesklkh nauk: MOLEVA, T.I.,
Inshener; NOVIXOT, Y.S., kandidat takhnicheskikh nauk; OSETSKIT. V.M.,
kandidat tokhnicheakikh nauk; OMOUMOV, G.A.; POIICKARZNKO, Yu.F.,
kandidat tekhnicheskikh nauk: RANOVSKIT, V.S., kandidat tekhnicheskikh
nauk; RXGIRZR, Z.L., inzhener; SOKOIDY, A.N., inzhener; SOSUNOV, G.I..
kandidat tekhnichaskikh nauk; STEPANOV, V.N., professor; SHIMAKRANOV,
X.H., kandidat tekhnicheskikh nauk; BLIKIND, I.A., inthener-, TANUSHE-
VICH, L.V., kandidat tekhnicheskikh nauk; BOKSHITSKIY. Ta.M.. Inzhe-
ner, redaktor; BULATOV, S.B., inzhener, redaktor; GASHVISKIT, A.G.,
Inzhener, redaktor; GRIGROIYEV, V.S., inzhener, redaktor; YNGURNOV,
G.P., kandidat tekhnicheskikh nauk, redaktor; ZHARKOV, D.V., dotsent,
redaktor; ZAKRAROV, Tu.G., kandidat tekhnichookikh nauk, reduktor;
NAMINSKIT, T.S., kandidat tekhnicheskikh nauk, redaktor; KOKARKOV,
T9.7., professor, redaktor; KOSTTLEV. B.H., inzbener, redaktor;
POVAROV. L.5., kandidat tekhnichesklkh nauk, redaktor; ULINICH, P.R.,
redaktor; XWRIKIYAN, S.Kh., oivetstvenny7 redaktor; GIADILIN, L.V.,
redaktor, (Continued on next card)

EMYLINA, TS.O. -- (continued) Card 2.
RUFFS IT, X.Y., redaktor: TMPIGCRZV, A.M., glavny7 redaktor;
BARABANOVO T*A.q redaktor; BARANOV, A.I., redaktor; BUCFDM7, V.K.,
redaktor; GRAYOV, L.Ta.i redaktor- DOMIN, A*T., redaktor; ZADIYID-
KO, A.N., redaktor; ZASYADIKO, A.Y., redaktor; KRASIIIKOVSKIT, G.V.
redaktor; LIRTOV, N.A., redaktor; DISHIN. G.L., redaktor; MAIVIOV-
SKIY, G.I., redaktor; MELINIKOV, II.T., redaktor: OMIA. D.G.,
redaktor; OSTROVSKIT. S,B.j redaktor; POKROVSKIT, redaktor;
POLSTTAHOY, G.R., redaktor; SKOCHINSKIT, A.A., redaktor-, SOUIRP
S.D., redaktor; SPIVAKOVSKIT, A.O., redaktor, STAIICHNIIKO, I.K.,
redaktor; SUDOPIATOV, A.P.. redaktor; TOPCHIYZV. A.Y.. redaktor;
TROTANSKIY, S.V.. redaktor; SHNVYAKOV, L.D.. redaktor; BYKHOV-
SKATA, S.H., redaktor lzdatelletva; ZAZULISKATA, V.F., tekhnichs-
skiy redaktor; MOZOROVSKATA, V.L., tekhnicheskiy redaktor.
(Mining; an encuclopedic handbook] Gornoe delo; entsiklopedicheskii
spravochnik. Glay.red. A.M. Terpigorev. Chleny glav.red. F.A. Bara-
banov i dr Moskva, Oos.nauchno-tekhn,isd-vo lit-ry po ugollnoi
promysh). ;o1.1. (General engineering) Obahchie inzhenernve
evedeniia. Redkollegiia toma S.Kh.Kloriklian i dr. 1957. 760 p.
(Mining engineering) (MLRA 10:10)

ANDR&Sv N.R.; LEVIN, H-Z-, red.1 xovALEVsKry, M.A., red. izd-va,-
OBUKHOVSKAYAp G:P., tekhn. red.
[Hard alloys are tool materials] Tvardys splavy - instrumental#-
nyi material. Moskva, Ketallurgizdat, 1963. 31 p. (MIRA 16:6)
(Cerudc metals) (Metal cutting tools)
(Mining machinery)

L 145,6-&6~ - JUIP(9)/Vr(m)/tPF(n)~2/VWA(d)/VR/k%P(t)/WP(b) Ped/Pei-Wfu-4
IJP(c) Y.JW1JD1M11.TG1ATACA
ACCESSION NRt AR5004790 S/0137/64/000/olo/IOBO/1081---7
ISOURM Refs sh, Metallurglyap Abe, 101575
qS
AUTHOR: Smirnova P, F.; Gurevioh, L, P,j Stepanovas To Me;
:Levin# B, Zo
ITITig-i-cgutt properties of a now experimental variant of alloy
,.-,VK4 with inareased strength
Xrm BOURCM Bb, tro 1~!es, nq-it in-t tverdykh splavoyo no* 5#
A964P 14-28
-TOPIC TAGS: tun 6' alloy# oobal~oontaining alloys tungsten
Zaten bas
~Parbldea cutting tool# oarbidizi~ ~oy VK4
WA
"TRANSLATION: Results of laboratory and produotion tests of the
cutting properties or a now industrial variant of alloy VK4# obtained:
'by uao of tungsten oarbIde with an Increased oarbidizing tomperaturej
are described, Cutting propo
i ,dies wore tested by oomparison with
~standard alloys VK4 and M#j On the basis of test results# experl-
imental alloy VA to rooommended for Introduotion In the rough
Card 1/2

L 32456-65
AOCESSION KRI AR5064790
ma0hiiiing of angino pistone, No Saznova,
SUB CODHI MM ENCLI 00

BILIBIS. Iq_IXVIllj_D..- SOROCHKIN. Tu.
RAlulto of testing the PAZ-652 iotorbus. Ayt. trsaso. 36 no. 6:16-
39 Jo f58. (Notorbusee-Testing) (MIRA U .-.7)

.LVIN D
Possibilities to reduce marketing expenses. Fin. 888121 uo.8j74-75
Ag '60. (XIIIA 1318)
1. Wonomist goodokhodov Derpohokogo rayfinotdola.
(Derpohi District-Cooperative societies)

KO. G.1. [Dotsenko. R.I.]: TOYT, S.K., lmnd.sellskokhos.nauk;
OZIMOT, T.I.,,'k9nd.ssl'skokhos.nsuk; TMONOT, H.I., kend.
sel'skokhox.nauks TAXAL L 6 nauchnyy sotrudnik; TISHMSKAU,
T.G. ETyshnevs'ka. T.H.), ;;;;hW sotrudnikt KRAM, T.I.,
nsuohnyy notradnik; TAXOTMO, M,S" nauchnyy actrudnik;
q6VA-D.Aw, agronom; GALAT, D.P. [Hoist, B.7 "]0 sootakhnik;
rMOTSKIT, 0. K. EPetrovalkyi, O.M.19 red.; LIMANOTA, X.I.,
tokhn,redo
EXanagement system on a collective form; the Dzerzhinskii
Artel, Swq Province] Systems vadenlia hospodarstva u kolhospi;
artill imeni Dsershyns'koho Bamalkol oblasti. Kharkiv, Kharkivalke
knyzhkove vyd-voo 1960. 77 P. (MIRA 14:4)
1e Nachaltnik kolkhoss imeni Dzershinskogo, Sumakogo rayons,
9=skoy oblasti (for Dotnanko).
(Samy Frovinoe-Ferm management)

BARKASH, Vadim Hikolayevich; _nXYMERG. Tls-
dimir ZinOT'YOTICh;'NOTIKOY, M.P.. ksnd.tekhn.naukq reteenzent;
KORUKOY, T.S., prof., doktor takhn.nauk, red.; SMOLOVA. G.Y.,
tekhn.red.; ILIKIND. Y.D., takhn.red.
[portable tools for assembling and finishing operations] Ruehnye
=shiny d1la montashnykh I otdolochnykh rabot. Moskva. Goo.
nauchno-takhn.isd-vo mashinostrolt.lit-ry, 1960. 264 p.
(MIRA 13:4)
(Building--Tools and implements)

,IZVIN D skonoudet
They have relaxed their attention toward taxes. Fin. SWR 22
zo.4s4g-49 Ap 161. (MIRA 14:4)
L Dbrgachevskiy rayfinotdol Kharlkovokoy oblasti.
(Dergachi Distriot-Income tax)

WaAhmistry opalescence of glass
cam JA Pub. 40 -5-27
Author*' I tavlav~D. I.; Zhdamvp S. U.1 and PorejvAoshites, Te. A,
Otruaturs of sodius borosilicate glass in connection with the opalescence
phenomenon, Part 1. Study of the opalescence of glass
-15y. AN MM. Otd. khim. nauk 19 31-39, Jan-Feb 1955
Ab straot.I The origin of opalescence In sodLva borosilloate glass to disousWe A
study of relay diffusion In the glass 9stablishO in close connection betr-
wean the diffusion intensity mid the structure of the "a. rare* tupftv-
ature &ones characteristic for opalescence intensity changes are listed.,
The connection between the ability of oodIvis borosilicate &Us$ to opalescov
and thisir ability to tom porous glass (during 113dviation) Is OplaIVAC
Yourtesn refsrenooss 10 USM# 3 USA and I Gelmn (1939-1953)-, QMPMO
UsMs, last, of Chen. of Silicates
bildtted 1pril 2-P 1954

7 -
USSR/Chem1cal Technology. Chemical Products and Their Application Silicates
Glass. Ceramics. Binderso 1-9
Abst Jcurral: Referat Zhur - Kh1miya, No 2. 1957., 5171
Author: 14vin, D. 1.
Institution: Academy of Sciences WSR
Title., Raleigh Scattering in Glasses and Glass Structure
Original
Publlcatlon: Sb. Stroyenlye stekla, M.-L., AN SSSRI 19551 198-201
Abstract: Investigation of the scattering In a series of optical glasses.
Fr= the results thus obtained the author dravo the conclusion that
Raleigh scattering is due to heterogeneity of glans structure per Be.
lt vas found that at temperaturea above the temperature of industrial
annealing., where a rapid relaxation of stresses can be expected,. the
Intensity of scattering of flints is not reduced) but somewhat in-
creased. Optical heterogeneity is caused by structural heterogenei-
ties, which are of the order of hundreds of angstrom units.
Card 1/1

-v
Structure *I "diurn borasiticate glasses In fit reliflon to
enon of opalescence. Ill. Comparison of 1hu
11nnrestiptlomi on sodium boroallicato ;tsms and
=
on products obtained from Went by lesching. It. A.
S. 11. Zhitusay, and 11, 1. I-gritt. hull,
&W. Sri, U.S.S.R, Div. Chom.1ri-M3,
frousLitiou).-Na barvallicate gla%,m were leached with
IfClwAa. I till L41 SiOl *6 It 14mi arto lilm-w i~e I(xind itt k-wh
gulsed. The inuth(j%6 4 luvt~tiptlou were b ah-wxptioft,
ck-ciron mkimvtse. end by litw-angle Waltag CA I-My's.
The etih of tlic&t strue(ures were filled with a sccuthlary
4.-omponcat coutg. BA, Si()~. And NaO. 71tese micro
two-plisse" ilritemi provklal the source td light scattering
and OPalCk'tftCC. 013S~", 73% SiO%, becume ck-Ar when,
heated to MAO while office tksom. &M SiO., twarne
Clear at M- -OD'. ULtvs with low-,%Os conttut. 33%
t1s" stnnfy gtwilre prMucts. Of D
-7
-M-77

---I- -ft'
Category : USSR/Optics - optic-la wija
Abs Jour :Ref 2bur - Fizlkao So 1, 1957, Ifo ~_92p_
K-3
Author Zhdanov, S.P., Froray-Fzshits, Te.A., levin. D.j.
last Inst. of Chemistry of Sil_4cates, Acsd. W ScitV:CeG W&F, IkqA4496-d
Title On the Structure.- of &xiium Borosilicate Glaze t_- 0:,nr_ecti'.m with the Opalescence
Phenomezen. Rep,,-rt J2. Jawatigatica of the F_-,pe-ltes cf Porcus Glaza
Crig Pub :Izv. AN MR, Otd. kh1m. nauk, 3955, No 2, 197-207
Abstract :Three intependent metsiods -- aAsorpticr, electrrn micr,:sc,:py, and X-ray
scattering at 2ov angles -- ve-re wited to investigate the zty-=U're tit porous
glaas to establish tbp-- comect!-.ia betv--gT. the degree of :)PsLlescerci- of sodium
borovilicate glass proceaaa4 by the acid methM It -~m-s that
porvus g1wa In a cambLtation- of tvo structures a deep-..- btructcoxe of the
silica skeleton and &! fiaer structure of Geconds-ry f,rmerl by the
highly dispersed silicic acid inside the ducts of the skeletm.. The diameter
of the ducts (cells) of the siLica, skeleton of porous glass zbtained from opal-
escent glass may reach 1000 A and more, while the diameters of the ducts of
the skeleton of porous glass obtained from ncm-opalescent ktraasparent) origi-
nal glass doea uot excee4 80-160 A. The differences in tLe structure cf pcrous
glasses, obtained from cpaleaceat and non-opalescent widlum borosillcate glass)
is due to the differences In the structure of the latter (fcr Report #1 see
Ref. Zhur. Fiz.. 1956j 20889).
Card : 1/1

PORAT-ICOHM,Ye.A.; ZHDANOF,S.P.; LITIN.D.J.
Structure of sodium boroallicate glass and opalescence. Report
no.3. Comparison of results of research on sodium borosilicate
klasses and of porous products of their leaching. lzvJI SSSR-
Otd.khIm.nauk no.3:Y)5-02 vq-Je '55. (KrAA 8:9)
1. Institut khtall. allikatow Akademil -k S6SR.
(Glass sanufacture-Chosistry)

FORAY-KOSMTS, Te.A.; LIVIN. D.L: AND YEV, N.S.
Structure of sodium borosilicate glasses in connection with opales-
cence. Part 4. Relation of the structure of sodium borosilicate
glasses to prolonged heating at a constant temperature. Z%v.AN SSSR.
Otd.khim.nauk no.3:287-293 Mr 156. (KM 9:8)
1. Institut khimli silikatov AkMemii nauk SM.
(Olass manufaoturs--Chomistry)

I C. ty I IV 3. 1. 1 1
I- IL-
I I' I

SOV/81-59-12-43034
Translation froms Referativnyy zhurnal. Khimiya,.1959, Nr 12, P 308 (USSR)
AUTHORSs Levin, D.I., Basin, Ye.V.
TITLEs A Sonio Method for Determining the Elasticity Module of Ceramic
Materials in the Plastic Btate
PERIODICALs Tr. Goo. n.-i. keram. in-tat 1958, Nr 1, pp 92-97
ABSTRACTs A dynamic method has been described for determining the elasticity
module, based_,on the measurement of the frequencies of the,natural
oacillationstof the tested sample. The determination of-the reson-
&nos frequi-ney of the sample is carried out on an installation con-
sisting of a "ZG-10" generator of audio frequency oscillations, an
exciter of mechanical oscillations* a receiver of mechanical osoil-
lations, an "EO-7" oscillographp ;L a test panel,*on whi'ch the ex-
citer, the receiver and the supports of the sample are mounted. A
diagram of the installation, the compositions of the porcelain mas-
aso and the curves of the dependence of the elasticity module on
the humidity are given.
Card 1/1 G. Gerashchenko

150)
aUTHORt Yustova, YO.N. SOV172-58-12-23123
TITM Conference on Problems of Measuring the 11hiteness of Products
(Boveshchaniye po voprosam izmereniya belizAy izdeliy)
PERIODICILs Steklo i keremika, 1956, Nr 12, PP 48-48 (USSR)
ABSTRACT3 In the current year, the Vaesoyuznyy nauchno-isoledovatellakiy
14 inatitut metrologii imani. Mendeleyeva (111-Union Scientific He-
search Institute of Metrology imani Xendeleyev)j with the partici-
pation of representatives of interested organizations, held an
extended session of the Postoyannaya komissiya pri VNIIHe (Permanent
commission at the VNIIM#)j which dealt with problems of the white-
ness measurement. The following reports and informations were givens
Ye.1- Yustove. on. mathods, of whiteness measurement.
D.1. Shklovsx,on an-al*ctronlo.color-oomparator and its application
in the- daterm'"Atim ~ot whiteness.
V.S. Khazanoy on the photometer IT-2 and its application in the
measurement of whiteness,
D.I. lovin.reported,on the determination of an expedient measuring
method Tf --- iorcelain whiteness.
M.M. Gurevich spoke on the atage of the problem of whiteness measure-
Card 1/2 ment.

Conference on Problems of Measuring the Whiteness of Products SOV172-58-12-23123
As a resuLt of the conference it was stated that it is necessary to
use either the colorimetric or the apso tropho tome tric method, accord-
ing-to the purpose for which the whiteness is measured. It was re-
garded as necessary to organize the series production of the photo-
meter FT-2, the colorimeter KNO, the spherical photometer IV-58, and
the photo~electric comparator GOI. The work done by the All-Union
Scientific Research Institute of Metrology, the Veesoyuznyy nauchno-
iereledovatellakiy avototekhnichaskiy institut (All-Union Scientific
Photological Research Institute), the Gosudarstyennyy nauchno-issledo-
vatel'skiy keramicheakiy institut (State Scientific Ceramic Research
Institute), the Nauchno-iseledovatellskiy institut khlopchatobumazhnqy
promyshlennosti (Scientific Research Institute of Cotton Industry)
was appreciated, and its continuation wa a recommeqded. The desire
was expressed to create in the VNIIK~ a center wh ch should be
equipped with the most up-to-date apparatus for measuring the white-
ness in order to help industrial organizations.
Card 2/2 uscomm-Dc-6o.515

BASINO Ye,V.1 LEVIN. Do-J.-
Investigating the relatiern of the elasticity
porcelain bodies to temperature. Trudy GIKI
modulus of
no.lz68-U 160.
(MIRA 16:1)
(Ceramics) (Elasticity)

MOM
BASIN, Ye.V.; LEVIN, D.I.-
Effect of quartz an the dependence of the uodulus of elastielty
of ceramic materials on the temperature. Zhur. Prikl. khim. 34
no.51ll57-1158 W 161. (MIRA 16:8)
(Ceranic matoriale)

BERMAN) A.S.; MELINIKOVA, I.G.; LEVIN, D.I. kand. fiz.-mat.nauk.,
0 - .
nauchmyy red.; FETRRIKO., ". -,-Fe-a-.1zd-va; CHERKASSKAYA, F.T..,
tekbn. red.
[Structure and frost resistance of wall materials] Struktura i
wrozootolkosti stenovykh materlalov. Leningrad,, Goestroiizdatt
1962. 164 p. (Vallo) (Building materials) (HIM l5s6)

kand. fiz.-matex. naukl NIKULINA, L.N., kand. pol.-
is nauk
Ilse of a microscope vith a heating device for studying feldspars.
Stak, i ker. 20 no.6:30-32 Je 163. (MIRA l6t6)
1. GosudarstvenrW nauohno-isaledow tallskiy keramichaskiy
institut,
FaIdaw-Testing)
Microecopy-Teehnique)
~