SCIENTIFIC ABSTRACT LEBEDINSKIY, A.I. - LEBEDINSKIY, P.V.

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• Collection: Scientific Abstracts
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• Document Creation Date: January 3, 2017
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• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT

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LE;1ZD1NSK1Y$ A- I- ,,Isations Of '-"' C,,)iejds Part I,"
A i - 'Mie . . C. items.
and Lclbedil - 13ibliOV,-
,-2E - ~" ~-', 10 3
Gurevich) L* 1949, Issu" 2 p. 97-
p,stxon- zhurn2LI) 7_1urnal I rykh Statey i1o. 17., 194))-
soz U-3736, 21 may 53, (LetOP's on of cepheidsp also kno',M
gives a brief introducti part 11 will
articles Dhenomenone
First Of two I who have studied this I art I. pA 42/49T4
as Pulsating 9tars- L-Ists people e of the Statements made in P
present mathematical Proofs Of som
1,7P1EE;Ii-i.-.KIY, A. T.
M 17 0 T,"-, 7
-USSR/Physics - Astronomy Nov/Ded '50
"The Formation of the Planets," L. E. Gurevich " A. I.
Lebed-inskiy, Leningrad State U imeni Zhdanov
"Iz Ak Nauk SSSR, Ser Fiz" Vol XIV, No 6, 13P 765-803
Tnree reports delivered at meeting of the Depart of
Physicomath Sci, Acad Sci USSR, 21 - 23 Ain 50 in
Riga: "I. Gravitational Condensation," n1-1. Lav -
Governing Distances of Planets and Their Rotation,"
and "III. Structure of the Primordial Cloud and Sep-
aration of the Planets Into the Inferior and Superior
Planets."
170T97

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MOW-
-A
4A 7:,i
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--,'BI I Y-
USSR/Astronomy Planets 21 Oct- 50
"Law Governing Planets' Distances and Rotation,"
L. E. Gurevich, A. I. Lebedinskiy, Leningrad State
U imeni Zhdanov.
"Dok AX Nauk SSSR" Vol LXXIV, no 6, pp loft-io&
Derives general "Bode" formula for distance of nth
planet to the Sun, which involves av eccentricity e:1
F 1 + e - n
n I -+-~5eft(l 4 2e)
Submitted 25 Jul 50 by Acad 0. Yu. Shmidt.
"b
172T2

LEDED:ENSKIY., A. 1.
UUSH/Ast.ron
nOM7 - cosmogony
*Wthest. Concerning the Formati Ju.,
A. I- Lebedinskiy; Leningrad
Zhdanov Stateon of Stars'"
U imeni A. A.
:'IDOk Ak Nauk sSSR,, VO_, I.
,Da,
X, 170
PP 41-44
sesp, ho
thesis On Je
ans' inequa
-M T where li-ty
is the gravit
,,A gas cons?; P ationa.1
Condense they may sep in-tmol Ve'ght- If big masses
fying Jeans, inequal.,ty 0 smaller ones., each B,tl,
limit Of max . Author attempts to find
"'"B condensing into a 'tar.
',tively assumes max mass of hYdrla,n star equaa to
00 GO-lar masses. Ile tenta_
SbmIdt. Submitted 3 May 5.1 by .4cad 0. Yu.
~_IIJI Aad O~T.Yu-
2.1

USSR/Astronomy - Mass of Stars, Maximim 21 Jul 51

"The Greatest Possible Masses of Solitary Stars
and the Formation of Red Systems," A. 1.
Lebedinskiy, LerAngrad State U imeni Zhdanov
'Tok Ak Nauk SSSRII Vol LXXIX, No 3, PP 415-418
Discusses the problem concerning the evolution of a
cloud of diffuse matter Vhich is slowly and
gradually being converted into a star. Also dis-
cusses the causes of the instability of super-
massive stars and some incorrect assumptioas of
2ml
Eddington. Gives criteria and inequalities
governing upper limits of mass, density, radius,
etc., Submitted by Acad 0. Yu. Shmidt 2 Jun 51-
21M

CA
USSR/Astronomy - Nova Mar/Air 52
tiVelocities of the Envelopes Burled Out by Novae,"
A.I. Lebedinskiy, Leningrad State U imeni Zhdanov
"Astron Zhur" Vol XXI , No 2, PP 135-143

Examines qualitatively the process of a peri-
pheral explosion due to a flare of a iSova, by
-proceeding from dnalogy with the well-studied
processes of ordinary ex~,?losions. Schezati-
cally represents the distribution of pressure
In the star. During a f lare in a nova a sud-
den release of energy occurs in it s depths;
the transfer of this energy from bowls to surf ace
of star is effected by wave condensation in the
space of. several tens of minutes, the vave,in
passing from bigh to low densities being acceler-
ated to finally reach high vel4cities. Submitted
22 Jun 51.

USSR/Astronomy - Cosmogony 21 Apr 52
"The Forming of Sturs at the Present Time, " L.' E.
GurevichY A. I. Lebedinskiy, Leningrad State Peda-
gogical Inst imeni A. I. Gertsen
"Dok Ak Nauk SSSR" Vol LMIII, No 6, PP 813-816
State that star forming cannot be an act that oc-
curs once but rather represents a multiple pro-
longed repeating process which is connected with
the evolution of the Galaxy. The authors I theory
of star formation in the process of gravitational
condensation leads to the conclusion that stars
that are forming must rotate with a speed close to
limit of centrifugal stability and the conversion
223T58
of a forming star into a normal slowly ro-
tating star requires the loss of mass. Sub-
mitted by Acad 0. Yu. Shmidt 5 Mar 52.
223T58
PCII
PI

and GITXEYT
j.: TH A"
V.

LISSR/Astronomy - Gravitational Condensation 1 May 52
"Gravitational Condensation of Stellar Gas and For-
mation of Stellar Clouds," A. I. Lebedinskiy,
Leniugrad State Pedagogic Inst imeni A. 1. Gertsen
"Dok Ak Nauk SSSR" Vol LXXXIV, No 1, PP 33-36
Considers the case of condensation of a stellar gas
in a planar-parallel layer, which may be considered
external parts of our Galaxy, where the Sun is
located. A considerable part of stars in the Gal-
SXy is united in various stellar systems: spheri-
cal and open clusters and stellar clouds. The ques-
tion arises% Are all stellar systems made up of
stars possessing a common origin, or can stars wilh
224T65
Deg energy join into systems7 In latter case
arises the problem of gravitational instability
and stellar dispersion. Submitted by Acad O.Yu.
Shm-idt 12 Mar 52.

224T65

LMIMITSKIY, A. I.
USSR/Astronony Diffused Nebulae 11 MY 52
"Dyramics of Diffused Nebulae," A. I. Lebedin-
skiy, Leningrad State Pedagogical Inst imeni
Gertsen
"Dok Ak Nauk SSSR" Vol 84, No 2, pp 249-252
Analyzes peculiarities of distribution of dif-
fused matter spread over a space of hundreds
of Darsecs. Refers to his previous works (Cf.
"Dok Alk Nauk SSW' Vol 84, No 1, 1952 and Vol
79, No 3, 415, 1951) and concludes that dif-
fused matter may be distributed only in irreg-
ular form. Received 3 Mar 52.
231T61

USSR/Astronomy - Stellar Associations 21 May 52
"Stellar Associations," A. I. Lebedinskiy; Leningrad
..,tate Pedagogic Inst imeni A. I. Gertsen
"Dok Al~ Wauk SSSR" Vol IMIV, No 3, pp 467-470
The hypothesis that hot giants are stws that have
captured diffused matter (Lebedinskiy, "Dok Ak Nauk
SSSR" Vol L)OIIX, No 1, 1951; Lebedinskiy and L. E.
Gurevich, "Dok Ak Nauk. SSSR" Vol LMIII, No 6, 1952)
gives the possibility of constructing a rational clas-
sification of open clusters and galactic subsystems
and explaining the peculiarities of assocns of hot
stars Shows that the evolution of clusters proceeds

225T36
dir..--_z-tion 4-3-2 according to W. Becker's lumi-
in the
.
nation-spectrum diagram for the main types of open

'lusters enumerated from 1 to 4 (Sterne und Stern-
c
systeme, Dresden und Leipzig, 1950, p 154). Submitted
by Acad 0. Yu. Shmidt 5 Mar 52.

225T36

bs
4A
MMI~
LEBET)INMY9 A. I.
PA 245T31
USSR/Geophysics Northern Lights 11 0,:t 52
"Radiant and Arc Forms of Northern Lights," A. I. Lebe-
dinskiy, Leningrad State Pedagogical Inst imeni Gertsen
"Dok Ak Nauk SSSR" Vol 86) No 5~, PP 913-916
Assumes that northern lights are produced in the upper
atmosphere, which consists of plasma. Radiative
auroras are generated by electron impact and are strong
in luminosity, while arc-shaped lights are duc to ex-
citation by ions and are weak in visibility, Submitted
~by Acad 0. Yu. Shmidt 11 Aug 52..
245T31

523.2
of do Put
011 llw.otlgla
7~7 t JI"if. Au"'.
A
arch~ on the birth 0114
~2=41 "5), let Me!
of dcCIdC, lia",
last
A MY10w 0 led out during
,t,m carr onic. theory -Of 0' Y'-
low is
diva Mier 011~ the planetary C
Igg-Ific P
he SUD
Idt (1944) in tured by t
Schrre, a &rnic gas and dull caP tcniwc.~
through an C,
the latter's T.Issap which have;
-arlous thco"'s Potbols:
dollbil- or ScbnWt's hyl
,,,fd nebula
_q dvT5-past-150 YC", Ithe - solar',
thr fmiln ;~iih ear
..can alone explain ed Incomp"arl
em now obse" , * . . f the theory Is &I
Llistil..'Clion 01 by t
work, Ark, sessimrit Of the- Part P ~y tic into
d. 'Otitauvo U ,gy of the dual
qui . of the kincil' "I
version , 't emission into.1pa
t, and t6 subsequel R, BA"EA;
hca
r
_!!'-!7-7!77777_7

LIDEDRiSM, A- I
MR/Astronomy - Interstellar Dust 21 Sep 53
IlDust-and Gas in Interstellar Space.fi~~A.I. Lebedin-
skiy,_--Leningrad State Pedagog Inst im Gertsen
DAN SSSR, Vol 92, No 3, PP 507-510
Analyzes adsorption of H atoms to a dust particle
with successive formation of H~mol, followed by
release of a certain amt of energy, which, he as-
sumes, propagates as a wave with velocity of sound.
Derives corresponding eqs and tabulates energies
and temps of formation of various mols. Presented
by Acad O.Yu. Shmidt 15 Jul 53.
268T72

-- - ill ~-. , - #,P ... - .-
~. - -,; - - - , ~ 41"J~,,--i . 1~;L: - - . W,-, . . ~ ~!
, *~ .. - -.;t -~.v-.: 4 , i~, - ~~ .. f.. ~~ ! . . ., 1.
'A , - ~ I
LLBEDINSKIIS AoI*
RT-952 (DYnamics'Of cliffup-se nebulae) Dinnmika diffuznykh tumannostei.
DOKLADY AKADENII NAUK SSSR, 92(5): 911-924v 1953.

LER&DINSKIT, A.L.
-en~
, W-Vmef, - r, wt --; K'.
Hypothesis of star formation. Vop.koem. 2:5-149 154. (Mim 8:5)
(stars)

GURSVICH,L.E.; LBEEDIIISKIY,A.I.
On the CaUBes of stellar flares. Dokl. Ali SSSR 103 no.4:569-572 Ag'55.
(Stars, New) (MLRA 8:11)

LEBEDINSKIY, A.I.; KHOROSHEVA, O.V.
Motion of stars in associations. Astron.zhur-33 no.1:54-61
.Ta,-F 156. NLRA 9:6)
1.Moskovakiy gosudarstvenny7 universitet imeni, H.V.Lomononova.
(stars)

;.7- - I . - .
SHMIDT, Otto Tullyevich, akademik4!EF.U9I&*-AaJ., otvetBtvenW
redaktor; KOZLOVSXAYA, S.V.'. redaktor izdatellatva; RTLIKA, Yu.V.
tekhnicheskiy redaktor I
[Your lectures on a theory of the origin of the earth] Ghetyre
lekstsit. o teorii proiakhozdeniia zemli. Izd. 3-e, dop. [Moskva]
Izd-vo Akad.nauk SSSR. 1957. 138 P. (MTRA 10:9)
(Cosmogony)

Name LEBEDINSKIY, A.
Title : Professor
Remarks: Professor A. Lebedinskiy has written an article,
"Triumph of the Human Mind", in connection with the
October 4, 1957 launching of Sputnik No. 1, which
demonstrates considerable knowledge of upper-stratosphe-
ric phenomena.
Source : N: Promyshlenno-Ekonomi4cheskaya Gazeta, No. 120,
6 October 1957, P-1, c-7

moxv, Serge' Ivanovich; FUSHMNq. ITik,)IV Taoil lyovicb.-;.,T_XM SKIY , A. .,
7 Aj- - - -
prof., doktor kiz.-mi. um*, otvatetven'W red.; SAMPON=Ot* L.V.;
.. red. lzdvva; FqMOTAt TsFo, tekhn, red,
[wortkem lightS3 Poliarny'* slUmlia. Zarisovki p~llarnykh siianii
G~H. Gamon-Gamana. Moekva, lzd-vo Almil. nauk SSSR* 1958. 111 ir.
(Aurorae) (KM& 11:9)

MIDT, Otto Yullyevich, akademik Ldecaasedj; KUROSH, A.G., d:)ktor fiz.-matem.
nauk, otv.red.toma; GRIGORIYEV, A.A., akademik, red.; DE-1012, B.N.,
red.; KAT-ASHNIKOV, A.G., doktor fiz.-matem.nauk, red.; KOZLOVSKAYA,
S.V.. red.;.14~ ~IY _AI doktor fiz.-matem.nauk, red.*- LEVIN,
B.Tu., doktor fiz.-matem.nauk, red.; MALITSEV. A.I., red.: LILIMI,
G.F.. doktor fiz.-matem.nauk, red.; SHEVELEV, M.I., gsneral-layte-
nant, red.; PCLENOVA, T.F,,, tekhn.red.
(Selected works; mathematical Izbrannye trudy; matematika. Moskva,
Izd-vo Akad.nauk SSSR, 1959. 315 P. (MIRA 12:2)
1. Chlen-korrespondent AN SSSR (for Delone, Malltsev).
(Groups, Theory of)

KOGAN, Ya.y',., red.-sostavitel'; ALSLESAITI)ROV, akademik, otv.red.; KALASHNIKOV,
A.G., doktor fiz.-mat.naulc, red.; GRIGOR'YJ3V, A.A., akademik, red.;
IBLOYA, B.N., red.; KOZLOVSKAYA, S.V., red.; KUROSH, A.G., doktor
fiz.-mat.nauk, red.; jpp~ll S'K'IY A. I. doktor fiz.-mat.nauk., red.;
LWIN, B.Yu., doktor fiz.-mat.nauk, red'.-~,'MALITSEV, A.I.. skademik.
zed.; KHILIMI, G.F., doktor fiz.-mat.nauk, red.; SIOVELEW, M.I., geroy
S.)vetekogo Soyuza, red.; FROKOFIYEVA, N.B., red.izd-va; POLENOVA. T.P.,
tekhn.red.
[Ctto IUl1evich Shmidt; his life and works. A collection devoted to a
hero of the Soviet Union, Academician Otto IU11'evich Shmidt, 1891-19561
Otto IUllevich Shmidt; zhizn' i deiatellnost'. Sbornik, posviashchennyi
geroiu Sovetskoj~q Soiuza akademiku Otto IUVevichii Shmidtu, 1891-1956.
Moskva, 1959. 469 p. (MIRA 12:12)
1. Ikodemiya nank SSSR. 2. Chlen-1--orres-pondent All SSSR (for Delone).
(Shmidt, Otto IUllevich, 1891-1956)

LEBMINSKY, A. 1.
"The composition of terrestrial corpuscular radioaction and possil-le
mechanisms of its originif
Lebedinsky, A. 'I., S. N. Vernov, A. E. Chudakov, I. P. Ivanenko
Investigations conducted during the flights of the Soviet earth satellites and
the cosmic rocket have yielded the following data on the composition of "terrestrial
corpuscular radiation", that is, particles revolving about the earth:
1. In the outbr zone (1), the overwhelming majority of particles are electrons
of energy 26 tO 100 kev. If we represent the energy spectrum of these electrons in
the region of maximum radiation in the form: N ( E) l/E , then 5. Extrapola
of such a soft spectrum into the region of lower energies shows that at F--5 to lo
kev, the total density of electron energy would exceed the energy density of the
map-natie fiald H2 /8- . For this reason, the electron spe-otrum in the region of
law energies (several kilovalts) should either have a maximum or at least should
be small at least in this region. The number of electrons of relatively high energies
5 X 106 ev) is negligibly small as compared w-ith the number of electrons in the
20-100 Kev range. The overall energy released in the crystal of the scintillation
counter from photons due to the bremsstr2hlung of electrons is from, two to three
orders of magnitude in excess of the energy released by all hi h energy particles
that produce an energy release In the crystal of over 4.5 x lOg ev per particle.
The total energy of all electrons in the outwe zone is approximately equal to the
energy rel~9sed in aurorae during somewhat over one week.
report presented at the International Cosmic Ray conference, Moscow, 6-11 July 1959

21(8)
AUTHORS: Vernov, S. N,, Corresponding Member, SOY/20-124-5-17/62
AS USSR, Grigorov, N. L,2 Ivanenko, I. P., Lebedinskiy,
A. I., Ylurzin, V. S.., Chudakovq A. Ye.
TITLE: A Possible Mechanism of the Production of "Terrestrial
Corpuscular Radiation" Under the Action of Cosmic Rays
(Vozmozhnyy mekhanizm sozdaniya 11zemnogo korpuskulyarnogo
izlucheniyall pod deystviyem kosmicheskikh luchey)
PERIODICAL: Doklady Akademii nauk SSSR, 1959, Vol 124, Fr 5,
pp 1022-1025 (USSR)
ABSTRACT: By "terrestrial corpuscular radiation" the authors mean
the fluxes of particles moving in the terrestrial magnetic
field along closed orbits. According to the authors~
opinion, the following radiation production mechanism
deserves the most attention: Under the action of cosmic
radiation, the earth, like any othercelestial body,
becomes a neutron source. The neutrons traverse the
magnetic field without being disturbed as uncharged
particles and attain great distances from the earth.
The charged particles originating from neutron decay move
in the magnetic field along the lines of force. The particle
Card 1/4 in the course of time reaches the region of high geomagnetic

A Possible Mechanism of the Production of "Terrestrial SOV/20-124-5-17/62
Corpuscular Radiation" Under the Action of Cosmic LIFys
latitudes, where fieldstrength increases considerably
with increasing latitude. In this region the velocity
vector of the particle will, as the particle approaahes
the earth, turn so lone with respect to the vector H,
until at the latitude X max the angle between the
-4
velocity of the particle and the vector H becomes equal
to 90c). At this point the particle returns and begins
to move in the rear direction along the same magnetic
line of force. If conditions are favourable, the decay
products of the neutrons may perform 10 a and more
oscillations between the northern and the southern
turning points Therefore, the intensity of the flux of
these particles increases by the same amount. Experimental
data indicate the existence of such a radiation. The
present paper carries out a closer investigation in order
to find out by what factors the intensity of these rays
is determined. Calculation is followed step by step. The
Card 2/4 authors calculate the intensity of the "terrestrial

A Possible Mechanism of the Production of "Terrestrial SOV/20-124-5-17/62
Corpuscular Radiation" Under the Action of Cosmic Rays
corpuscular radiation" for various heights and latitudes;
the results obtained by these calculations are shown by
a diagram. They lead to the following conclusions:
Although the number of neutrons decaying in the earth is
very small, they may cause intensive cosmic radiation. The
experimentally determined intensity is by -.100 times
lower near the equator than calculated intensity, According
to experimental data there is no terrestrial corpuscular
radiation in geomagnetic latitudes above 400g but in the
pre5ent paper j(X . 4,o) ,j(, - 00) is obtained,, This
means non-agreement by moTe than 105 times the amount. In
order to reestablish agreement with the experiment, it is
useful to assume an additional flux of particles from
"magnetic traps", which are particularly strong in large
latitudes., This may be due to the existence of electric
fields. This assumption also appears to be confirmed by
the data concerning the considerable increase of
perturbations of the terz~?strial magnetic field with
increasing latitude, With increasing latitude, the
interdictions imposed upon energy by Stoermer's theory
Card 3/4 are being disobeyed to an ever-increasing extent, The

A Possible Mechanism of the Production of "Terrestrial SOV/20-124-5-17/62
Corpuscular Radiation" Under the Action of Cosmic Rays
mechanism discussed in the present paper mustapply
also in the neighborhood of astrophysical objects having
a magnetic field. Therefore, the investigation of this
radiation in the neighborhood of planets may be a means
of observing weak magnetic fields. The authors thank
D, V. Skobelltsyn for his advice and M, S. Rabinovich
for discussions. There are 2 figures and 7 Soviet references.
ASSOCIATION: Moskolrskiy gosudarstverinyy universitet im. M. V.
Lomonosova (Moscovi State University imeni Ia. V.
Lomonosov)
SUBMITTED: November 21, 1958
Card 4/4

SMULT, Otto Yallyevich [deceased];-LEMIIISKIY, A.I., doktor fiz.-mtem.
nauk, otv.red.toma; LEVIN, B.Yu., dok-to-r-Yf-z-';:-matem.nsuk, otv.red.
toma-, YLHILIMI, G.F., doktor fiz,-matem,na&.j otvtred.toma;
KAUMUKOV, A.G., doktor fiz.-matem.nauk, red.; GRIGORtYET, A.A..
almdemik, red.; DELONE, B.N., red.; KOZLOVSKAYA, S.Y., red.;
KUROSH, A.G., doktor fiz.-matem.nauk, red.; MALITSEV, A.I., akademik,
rod.; SIL:,j'VbLL'V, 14.1., goneral-loytenant, Goroy Sovetakogo Soyuza,
red.; NOVICHKOVA, II.D., tekhn.red.; KASHINA, P.S., teklui.red.
[Selected works: geophysics and cosmogony] Izbrannye trudy; geo-
fizika i koamogoniia. Moskva, Izd-vo Akad.nauk SSSR, 196o. 2o9 p.
(miRA 14:1)
(Cosmogony) (Geophysics)
(Schraidt, Otto Nllevich. 1891-1956)

SHMIDT, Otto Yullyevich, akademik (deceased, 1891-19561; GRIGOROYEV,
A.A.. akndeaik, otv.red.toms; SHEYELEV, M.I., gone ral-leytenant,
Geroy Sovetskogo Sovuze, otv.red.toms; DELOUS, B.H., red.;
YAT,A IKOV,.A.G., doktor fiz.-matem.nauk, red.; KOZWVSKAYA,
S.Y., red.; KUROSH, -A.G., doktor fis.-matem.nauk, red.;
I.M., INSKIY, A.L., doktor fiz.-matem.nBuk, red.; LEVIN, B.Yu..
dokt-o-r-Yrz-.-m-a`E-e-M.nauk. red.; MALITSEV, A.I., akademik, red.;
KHILIMI, G.F., doktor fiz.-matem.nauk, red.; MEYEROVIGH, O.V.,
red.izd-va; KASHINA, P.S., tekhn.red.
(Selected geographical works] Izbrannye trudy; geograficheskie
raboty. Ko5kvn, Izd-vo Akad.nDuk SSSR, 1960. 212 p.
(MIRA 13:11)
1. Chlen-korrespondent AN SSBR (for Delone).
(Schmidt, Otto IU11,3vich, 1891-1956)
(Arctic regions)

23236 /61/000/006/018/044
S/0,35
A opi 1 Al. 5 1
AUMORS: Vernov, 3,N., Chudakov, A.Ye., Lebedinskiy, A.!., Ivanenko, !.P.
TITU: Composition of terre-strial corpuscular radiation and possible mechan-
isms of itS origination
PERIODICAL: Referativnyy zhurnal. Astronomiya i Geodeziya, no.6 , 1961, 33, ab-
stract, 6A287 ("Tr. Mezhdunar. konferentsii po kosmich. lucham, 1959,
v. 3", Mcscow, AN SSSR, 196o, 54_,:~8)
TEXT: Assuming tha-., -rhe ou-er radiation bell. consis7s of electrons with
E)/ -_ ~;- - I
energy spectrum N (~;, -_ E , he value ofT was determined to be/-_/~-- for ener-
gies from 20 to 100 kev. Extraprlatlon of this spectrum to the region of lower
energies (3 - 10 kev) would result ir -density of energy of particles which would
exceed the density of energy of the constraining magnetic field. Therefore, either
the spectrum of low-energy elec;zr~~ns mus-r- have a maxirwim or p shouid be small. A
weakening of the Ear-.hls magnet_1,:, field was observed in the seat of a maximum f4j_
led trap. A fraction of aurcra:F, can be explained by leakage cc particles Irrom the
outer belt into the atmosphere. The soarce of replenishment of' the outer zone is
solar corpusoular fl-uxes. At their motion, recombination is possible which gives
Card 112

23936
S/035/61/000/006/018/044
Composition of terresTrial corp--is-~ular radiation ... A001/A101
rise to neutral atoms. A~-,oms ionized atout or within the radiation belt give rise
to electrons capz-Lired by -he mag-~-etic field in the outer z.:,ne. The inner radiatli3n
belt is restricted by +hE~ force linzws starting from the Earth's surface at lati-
tudes 300-400. It Is fil-'e'-' 3 dec~ay of neutrons formed in the Earth?s at.,Tc-
sphere by cosmic rays. A-, life ---ime of protons in the belt being-.01071 -=ec, the
neutron mechanism is for fili-ing up the inner zo--l .i-p intens-'+.v ob-
served. A share fa-11 off of -4nt=nE-!-..F in- the belt at thA- geomagnetic la-,:-,'.ide Yjo
can be explained by -hree mec-Jhanls:-~s- a.) non-conser-wation cf magnetic moment ~,f
particles, b) effec-, of' magnetic dis-,urt-ances, c) drift of low-energy particl-
from the Earth as a result of beirg affe,~'~ed by ring currents presumed to exis'~ in
the ionosphere.
V. Temnyy
r
LAbstracter's note; Complete -7~ranalationl
Card 2/2

8"63
8/555/60/007/000/001/007
B12313201
AUTHOR: Lebedinskiye A. I.-
TITLE: Hydrogen content in large planets
PERIODICAL: Voprosy kosmogonii, v. 7, 196o, 50-54
TEXT: An attempt has been made by the author to explain the fact that the
chemical composition of giant planets differs from that of other planets.
For his purposes, the author assumed heating of the outer part of the proto-
planetary cloud to have been caused,by the motion of solid components. A
hypothesis put forth by him in 1950 explains why there.is an excess of
hydrogen in planets starting from Jupiter# and lack of it from Mercury to
Mars. According to this hypothesis, the protoplanetary cloud was composed
of hydrogen and, possiblyp helium. Other elements were contained as small
admixtures, Before thi6 cloud was subjected to a high pressure, hydrogen
and all its.volatile compounds were in the gaseous phase. As condensation
rose, dust began to concentrate in the equatorial plane, and formed a com-
pact ring, like Saturn's, around the Sun. Because the Sun did not heat
through to,the outer zones of the ring, the light gases condensed on the
Card 0

Hydrogen content in....
89063
8/555j6O/OO7/000/001/007
B123/B201
dust. The heated part gave rise to the planets of the terrestrial group on
:the basis of sparingly fusible materials (rocks, metals) with moderate
masses. The planets of the Jupiter group were formed from light matter
adding to the dust. The various chemical compositions of the Jupiter group
~planets can only be explained by considering the energy equilibrium of dust
at the periphery, where solar radiation was practically inexistent, and
stellar radiation could not heat the dust to more than 30K- Under these
conditions, friction was-apt to be the main source of thermal energy. The
,author has shown in two previous papers that the evolution of a dust system
and that of a system of solid..47Wies exclude each other. The later paper
has been published in the present periodical, Vol. 2, P- 5, 1954. When a
flat disk, similar to a Saturn ring, arises# and the solid bodies act upon
one another by gravitation, their volume is increased as the result of
collisions of bodies of the subsystem. The equatorial diameter of the dust
system is reduced by a decrease of the moment of momentum. The author
considers the case where solid bodies and dust particles coexist in the sub-
system. The energy of solid bodies is reduced by the friction on dust; it
radiates into space as thermal energy. When bodies with comparable mass
collide they are crushed in most oases# since, as a rule, their relative
Card 2/3.

89063
.8/555J60/007/000/001/007
Hydrogen content in ... B123/B201
velocity is not less than several km/sec. The thus resulting small bodies
go to augment the bigger bodies with which they collide, and the planetary
bodies are formed on the expense of dust of the subsystem. Eventually# the
disperse matter gets together to form the2planets. The heat set free in
the process varies from 0.1 to 100 erg/am sea, depending on the distance
from the Sun# and corresponds to a dust temperature of 5-300K. The process
of planet formation takes place in two stages. In the first one, the solid
component accumulates, and as the next stage, the chemical composition
undergoes a change, once the planet has grown sufficiently massive. The
gas density passed through a maximum at some distance from the Sunj this
explains the maximum in the Jupiter - Saturn zone. Moreover, a monotonic
dependence of the density on the orbital radius is observed with the
Jupiter satellites. It is concluded that the planetary satellites as well
must have formed under the same law. There are I table and 2 Soviet-bloc
references.
ASSOCIATION: Moskovskiy gosudarstvennyy universitet im. M , V. Lomonosova
(Moscow State University imeni M. V. Lomonosov)
Card 3/3

L'i; , 1: ~': , -:' '--' 77;'f
I - .-:I ' , ': .
A,
1 t,. .
- J- -I - . - 1 .1 ;.: ~ , - j . -,'I,
"The Study of the Planet.,.-iry DiqtribiitL,)n of Aurorae,"
Report presented at the Intl. Conference on Cosmic F-ays and
!earth Storms, Yi.voto, Japan, 4-15 Sept. 1.91')l.

SWIDT, Otto Yullyevich (deceased]$ akademik,- LEVIN, B.Yu., doktor
fiz.-mat. nauk, otv. red.; LEBEDINSKIY, A.I., doktor fiz.-
d.; KOZt9V-SrX-A--,*~-.V.----d--Y
mat. nauk, otv. re , re . zd-va;
POIYAKOVAI T.V., tekbn. red.
[Origin of the earth and planets]Proizkhozhdonie zemli i
planet. Mosk-,al Izd-vo Akad. nauk SM, 1962. 129 p.
(MM 15 . 11)
(Solar system) (Nebular bypothenis)

)/62/r-,- U3 '607/010
ALITFOR6: LeVleClf~5ki*, A. 1. $ and Salova, G. 1.
T! TLE : ar,~unt of free water on Mars
PSiZIO;)1OAL. Astronomicheskiy zhurnal, V.39, no,3, 1962, 494-505
TEXT: ~n a previous paper it was shoim that a considerable
amount of water may exist on Mars in the form of ice carried down
to the surface by dust and screened by it. This idea was later
developed by V.D. Davydov. In the present paper the authors
consider the amount of water present on Mars in free state; i.e.
in the atmosphere or the polar caps. The amount of water is
determined by estimating the upper limit of the amount of ice
crystals in the Martian atmosphere from its turbidity, and the
rate of evaporation of ice from the polar caps. Elementary
calculations indicate that the thicknes~s "Layer of snow or
cloud at the polar caps is 0.01 g/cm2 and total amount
of water in free state'on Mars is 2 x 1015 g. is pointed out
that the calculations of Vaucc-Aeurs are subjec;t to
errors.- The former assumed that a con.-,ic:erable part of the solar
radiation absorbed by'snow i-, u4ed ii-i evaporating it, whereas the
Card 1/2

The amount of free w`ater on Mars S/033/62/039/003/001/010
E032/E114
present results indicate that the snow surface re-emits
practically all the incident solar radiati-,~n and only a small
fraction of it i_-, u.-~ed ii. ev-,~oratiori. ;.. the other
hand ignored the i-il.artant item --- z1-::-- :-;td,- 'T:!-or. balance
equation; namel-, t`ie cm.,15zion of the surface. !'he present low
result for the thickness of the layer of snow, ur more accurately
hoar frost or ia in agreement with the results obtained
by A. Dollfus.
There are 3 and 4 tables.
ASSOCIATION: i-;c--':)vskiy gosudarstvennyy universitet im.
,M.V, iomonosova (Moscow State Unl-~rsity imeni
M.V. Lomonosov)
SUBMITTED: June 1, 1961.
~i-d 2/2

LEBEDINSKIY, A. I.
"Planetary Distribution of Aurorae."
report presented at the 13th Gen Assembly, IUGG, Berkeley, Calif, 19-31 Aug 63-

BAGARYATSKIY, B.A.; FELIDSHTEYN, doktor
fiz.-matem. nauk, otv. red.; MILYUTINA, Ye.N., red.
[Collection of articles) Sbornik statei. 14oskva, Pauka.
No.12. 1965. 56 p. (MIRA 18:4)
1. Akademiya nauk SSSR. Mezhduvedomstvennyy geofizicheskiy
komitet. IV razdel programmy MGG. Polyarnyyo siyaniya.

L 2476-66 jss- W/Tsw Mw
JACCESSIONRR: , AP*5025243 UR/0026/65/ooo/ooq/pouMc~
1AUTHOR: Kel~ I" iProfessor) -, Khodar~qK,"i'fu
Zsh,,M. V.'(Academician);
1K. -(Engineer); Masevich, A, G- sciences)
results of an important experiment (Preliminary evaluation of Zond-3
TITLE: Fir t
moon photosl
SOURCE: Priroda, no., 1965 II_IV
TOPIC TAGS: mo-Qn, Zmd_~', lunar topography, selenology, moon far side, lunar probe,'
lunar surface, selenograpby
;ABSTRACT: A preliminary,evaluation is given of the photographs of the far side of
Ahe moon obtained by
I ~ Zqp4~::3~,,_ The following observations are based on statements made
Jby 9.-V. Ke -s-h, A-.--I-. Lebedinskiy, Yu. K. Khodarev, and A. G. Masevich at a press
1conference held on 23 August 1965. Spectra of the lunar surface -;iere photographed
.1in the 3500-2500-R wavelength range and spectrophotometry was carried out in the
lultraviolet rangd from 2700 to 1900'k and in the infrared from 4 to 3 microns. The.
iprobe employed a specially devised small-size'.phototelevision system that ensured:
I
;protection of the film against cosmic radiation. The camera had an objective with a
i
.;focal length of lo6.4 mm and a relative aperture of.1:8. Special film 25 = ih width-
land exposute.,times of 1/100 And 1/300 see were used. -'The photographs were ex-
1 Card
OWN
I I _1 I IN M

L 2476-66
CES,91011 NR: AP5025243
amined at the Shternberg State Astronomical Institute under the direction of Yu. N.
Lipskiy. They showed few extended dark depressions of the far side. The northern
part of the moon facing the earth consists mostly-of seas, while the far side is
almost completely covered by a gigantic continent. So-called talassoids, extensive
depressions whose floor is covered by craters, appeared on the far side. These for-j
mations are similar in size to the seas on the near side, but differ in coloration.
A high degree of crater concentration is evident on the far side. The photographs
:also confirm the asymmetry of the moon relative to a plane dividing the near and
.far sides. It is concluded that, in general, the far side has fewer seas an d is
brighter and more mountainous than the near side. (DM
ASSOCIATION: none
SUBMITTED- ENCL: 00 SUB CODE: AA
NOIREF SOV." 000 OTHER: 000. ATD PRESS: A
BVK

-NtM44, -~.;M ~ R
L" 2962-66 FSS-2/D[TM/FS(v)-3/EWA(d) TT/GB/GVI
1ACCESSION NR: AT5023566 UR/0000/65/000/000/0065/0077
!AUTHOR: T! M P ov ~0 P-O-V, B Ve
-Lebedinskiy, A. I.,; qlqyatpj~iy,_ D. _N
~4 4
Yomichev, s er.,
I 5<
':rITIE: Infrared spectrophotometry of the Earth's thermd.,AdiationV)
SOURCE:1'11\~V na a k4~nferentqiya zk iAheqkqM.pXp-ptran scow
__f L
__pp
1965. Is- oamicheskogo prostranstva (Space research); trudy konferentsii.!
sledovaniya k
Moscow, lid-~vo Nauka, 1965, 65-77
iTOPIC TAGS: spectrophotometer, IR spectrum, instrumentation satellite, thermal
.radiation, atmospheric radiation, radiation intensity, radiation spectometer/Cosmos
i
45 satellite
!ABSTRACT: Results and equipment used in an experimental study of the energy distri- !
bution of the Earth's thermal radiiltion.are reported. A diffraction scanning qPVr,=-L-
itrophotometer,,mounted on Cosmos-45~rccmprised the basic equipment. The spectrophotom-
eter was esig-ned to measure thermal radiation in two bands, 7-20 P and 14-38 P.
he spectral resolution for the first band ranged from 1.4 V for the 7-p wavelength;---
Ito 1.1 tj for the 18-p wavelength. For the second band, the range was from 2.8 It for
Card

1 2962-M
SION NR: AT5023566
the 14-11 wavelength'to 2.1 p for the 36-p wavelength. The instantaneous field of
.vision of the optical system was 1*46' x 2*20', encompassing a radiating-surface area
f 7.5 x 10 km at the average altitude of 250 km. The instrument was.capable of
field of vision scanning within �8030'. Spectral intensity measurements-were carried
!out at X= 9.5 � 0.6')j for the first band and X = 18.5 + 1.35 V for the second. Semi.-
1conductor 'bolometers with a sensitive area of 1 mm2 were employed as radiation sen- !
:sors. Radiation detected by the. bolometers was converted into electrical signals with
;a frequency of 27 cps. The signals were amplified and converted into d-c voltages
!Proportional to the radiation flux. To measure cloud cover below the satellite, a
,'Photometer operating at 6000-8000 A with a resolution of about 30 km was used. From
the data obtained during the flight of Cosmos 45,the following.conclusions concerning
,the intensity of the Earth's thermal radiation were drawn: 1) The intensity at the
!minimum of the absorption band near 15 )j is almost constant. 2) A close correlation
between the intensities at the other wavel6ngths- was noted. This provides evidence P
ithat the effective radiation levels differ but slightly for various regions of the !'
!spectrum within 8-35 p. 3) The lower layers of the troposphere are the basic source
_,of the thermal radiation leaving the Earth's atmosphere. 4) There is a strong vari,
able intensity of the ozone band with its center at 9.6 U.' Orig.'art. has: 14 fig-~
:uresi [GS]
'ASS
OCIATION: none
1. Card 21P. -

L-10587m& ; FBD/EWT(1)
SOURCE CODE.--UR/dM/65/603)
AUTHORS: Vakhnin, V. X.; Lebedinskiy, A. I.
.ORG: none
9 t2
_Ye _nu 13 A'
TITLEs On the nature of radio noise radiation~irom the surface of V
SOURCE: Kosmicheskiye issledovaniya, v. 3, no. 6, 1965, 917-926
TOPIC TAGS: Venus planet, cosmic radiation$ cosmic radiation ener6y, gas discharget
radio astronomy
ABSTRACT: The increased level of radiowave radiation from Venus (600--700K) may be
explained as "quiescent" or "glow" discharges in the upper atmosphere, creating a gain
in radiated noise 200--300K above normal thermal radiation. Two hypotheses are
advanced in explanation of the phenomenon: 1) the radiation comes from the surface of
the planet which is heated by means of the "hotbed" effect in the atmosphere (see C.
Sagan, Science, 133# No- 34569 1961), and 2) the radiation is created by the motion of
ticles in heated and extremely rarefied layers of the Venuslan ionospheie
a:artrop. cit. and D._E. Jones. "Planet", Space Science 5, No. 2,
1961). A
review of some of the literature pertaining to the study of the same problem is given*
The authors present and discuss some of the data obtained during the operation of the
Mariner-2 satellite. It is felt that the Mariner data are insufficient in detail.
-Several'reasons are given in demonstrating that neither the hotbed nor the ionosphere
Card 1/2 UDCt 523-42t523-164

L 10587-66
ACC NR: AP6000308
hypothesis is completely aound on a theoretical basis. It is proposed that solar.
energy is.transformed into radio noise by two means: ordinary bot body radiation and
glow discharge radiation. The solar heat energy goes through a sequence of atmos-
pheric flow energy, atmospheric electrical ourrentsp and finally gaseous discharge
radio noise. The surface temperature of Venusand the temperature characteristic of
the radio noise are related in-context with the.authbrat hypothesis. Supporting data
on observed gas discharges from experimenti-are given.,.Orig. art. has: 3 figures and
10 equations
SUB COES 0 DATEs 26Feb65/ ORIG REFs 007/, MH MW: 010
C rd 2

7 7
?
-~M_2 F&cJ;~2M4T(1)/'~FS(v)-3/FCC/EWA(d)4 TT/GS/GW
963
.,,,GM8rC4 --'AT5023567 UR/WW/65/WO/J)d0 88
A
vileVe4bikiyo 'A. I'.' Kras-nopq ~skiy,* V. A.-..Kuzneteov, A. P4.,.;A-ozenai'~;*.V.-, A
-3 d, ultr
-imd, ultr
-7"iii~Jou aterrestrial atmospheric radiation, ba the V18i la-
TI.
3,kiationd' 7
-~'~~Msbyuzhava oiife~ieiiisi7a-:12~Lfli:tlw~k6ii~dcbeTskogo-BroEa;t&tan,-tya,-- Moscow
1 5
saledovanlya koamichaskogo prostranstva (Space research); truuy_b a
i;:,~-.,- qq C lrd-VO-Nauka, 196% 77-88
TOPIC TiGS.* at IR radiation, Wxadlatlou,
mospheric radiation, visible radiation
instrum,entatIon satellite, satellite data*anq1ysis,.radiation measiurement, airg
Cos mbs 45 savillIte
ABSTRACT: Heasurements of airglow and scattered solar UV radia'tion were made by"
)Cosmos-45 in 1964. Scattered UV radiation was measured.by a UV spectropbotom~mweter
I(range, 2Z50-3100.1,1; resolution,',15 A; field of vision, 20 km in width) operating
only on'the day-side of the Earth. Airglow was measured by a colorimeter (field of
r switching
vision, 120 km In width) operating only an the night side. Fo tfiellinst
ments I :and- fixing * on-. the,,underlyIng- -surface,.-;' A- s'einsor -wbich' 'tEeasured:.~-_ i~-
ti .0,6 0 85--u,'was
1.1lumina an at used.;-...The colorimeter, carried -four
Ii ,ht_.'.filters on coiMion_-.,:AXis-"-.M6unted, a disk. One filter
along,-.
7-
Card

VL 2.963--U)
ACCESSION NR: AT5023567
;screened out 'UV radiation; its long-wave boundar~i was near 6000 '1 11% c
2500 to 4000
second was used to investigate wavelengths ~at I and two varrow-band fil-
ters with passbands of 100 ~ filtered emission at 5577 A and 3914 X, reSDectlyely.
P IR spectrophotometer recorded thermal radiation concurrently with the operation
of the other two instruments. A correlation was found to exist between readings of
the UV and IR spectrophotometers in the 9.65-11 ozone band. A correlation of inter.,3i-
,ties was also disclosed near the long-wave boundary of the UV spectrum at A > 300-0 A
land in the readings of the illumination sensor. These readings depended strongly on
:cloudiness because the albedo of clouds in the red zone is substantially arenter than
.the albedo of the Earth's surface and of the clear atmosphere. The correlation con-
,Eirms that at A > 3000 A, the noticeable part of atmospheric radiationis due to.tropo-
.spheric dispersion and reflection occurring below the basic mass of the ozone layer.
,Conclusions were also reached on local, diurnal, and latitudinal variations of air-
low. A difficulty'arose in the evaluation because of the dependence of the readings
.9
on cloud cover. In.making the measurements in space, it was necessary to include re-
flections of airglow from the atmosphere and glow of astronomical origin in addition
,to airglow itself. Consequently, results varied with atmospheric conditions by as
much as a factorof two, with the minimum occurring during cloudless weather and the
maximum during total.cloudiness. The correlation'of readings of one light filter
:X5577 X) with 'the others indicated that the share'of illmtintation from the start; and
2/3

77
2963-66-
ACCESSION NR: AT5023567
light was relatively small. A comparison of these readings (averaged) with
;the results of ground observations at 3200-4000 A lead to the conclusion that night
0-3000 X is small and at 3200-4000 X does not exceed star glow
:sky radiation at 250
and zodiacal light., Measurements at 1700-2500 X indicated that no night sky radia-
tion exists in this region. Thus, results of measurements over the eqtire wavelength
.!range (1700-4000. X) confirmed the absence in the night sky of high-energy excitatio.a
~Iprocesses.' Orig. art. has., 7.figures. [JPI
IPSOCIATION: none
SUBMITTED: 02Sep65 ENCL: 00 SUB CODE: F-1. 5 11 A
0 REF SOV: 004 OTHER:~ 008 ATD PRESS,
cc '313

L 23449-~-66 FSS-?ZEVIT(l) TrZGw-
ACC NR. AP6011690 SOURCE CODE: UR/0203/66/006/002/0185/0189
311
AUT110R: Krasnopollskiy, V. A.; Kuznetsov, A. P.; Lebedinskiy, A. I.
ORG: Moscow State University, Institute of Nuclear Physi.cs (Moskovskiy gosudarstven-
nyy universitet Institut y,adernoy fiziki)
TITLE: Measurew-nts of the ultraviolet spectrum of the earth made by the satellite
"Kosmos-65"
SOURCE: Geomagnetizm i aeronomiya, v. 6, no. 2, 1966, 185-189
TOPIC TAGS: solar ultraviolet radiation, ultraviolet spectrophotometer, diffractiona
monochromator, ozone concentration, spectral brightness, radiation intensity
ABSTRACT: Solar ultraviolet radiation"'ieflected from the terrestrial atmosphere was
measured with an ultraviolet spectrophotometewunted on the artificial satellite
"Kosmos-65 - " The spectrophotometer used was a.double dif fractional monochromator
operating in the spectral range of 2250-3070 A. 2500 spectra were obtained during
the flights. Spectra were recorded on motion-picture films. The distribution of
energy in the violet spectrum changes with the zenithal distance of the run and the
geographical latitude. Local peculiarities caused by the ozone concentration appear.
Longer waves in the ultraviolet range penetrate deeper into the atmosphere and in-
crease the albedo intensity. Two kinds of spectra were obtained on cloudless days
Card
523~72:629.192.2

L 23449-66
AP6011690
in the equatorial zone: the typical spectrum and the spectrum of maximum intensity.
Tile first consi sts of the usual-spectra of tropical zones and the second seldom
occurs. The intensity of radiation reflected by the atmosphere depends upon the
quantity of ozone in a vertical column of the atmosphere. Spectra of the terrestrial
atmosphere and the sun obtained under the same solution conditions have great
structural similarity. Tile decrease in intensity in the atmospheric spectrum
occurring with decrease in wavelengLh is greater than in the solar spectrum. Ilie
authors thank Yu. V. Yaremenko, V. Ii for their great help with
this experiment. Orig. 'art. has: 4 figures, 1 table, and I formula. [EG]
SUB CODE: 04/ SUBM DATE: 24Nov65/ ORIG REF: 003/ OTH REF: 0091 ATD PRESS:
Card 2/21~w

C NR-. A26019461 SOURCE CODE: UR/0384/66/000/001/0079/0081
AUTHOR: Vcll--hnin, V. M. (Candidate of physico-mathematical sciences); Lebedinskiv.
A. I. (?Mle.-sor)
ORG:
TITLE: Fzdio noise and the temperature on Venus
SOURCE: Z-2:.ilya i vselennaya, no. 1, 1966, 79-81
TOPIC T.%GS: radio noise, Venus probe, space temperature, glow discharge, rarefied gas
ABSTR:,;-":! "he use of radio signals emitted by Venus to study its surface temperature
is discul-,t,-~~---~,, A theore-tical explanation of Venus' apparently high temperature surface
the "hot house effect", the ionospheric hypothesis and the contradiction
of th~:- c-.otbesis by the peculiarities of radio signals emitted from Venus) is prese
ed. t..--.;,ctric glow discharge in rarefied gases in relation to the very slow speed
with t-he planet Venus rotates around its axis and the possible existence of hi'ah!
velocl`,- ---obal breezes which do not create disturbances are considered. It is propos-
ed th~--L atmospheric current going through the upper layers of the atmosphere of the
plane-, creates a continuous glow discharge resulting in powerful radio noise and!
a low ~,ee of luminescence. The proposed explanation is substantiated by experiment-~
al data and can be explained theoretically. If this interpretation is correct, then
Card 1/2

ACC N,'.; AP6019461
the surface temperature of Venus would be between 50-600C. Orig. art. has: 3 figuresiI
Z
SUB CODE: 0417/ SUBM DATE: none
2/2

L 45257-66 "E'-iT(l)/EEC(k)-2/FCC JY.T/T]'/DD
Vg-
IACC i~ 7
AP6020934 SOURCE, CODE- UR/0029/66/000/006/0008/0011
AUTHOR: Lidov, M. L., (Doctor of Physical and Mathematical Sciences);
Leb E!
L.,_ (Doctor of Physical and Mathematical Sciences, Professor);
Vernov, S. N., (Corresponding Member of the Academy of Sciences SSSR)
ORG: none
TITLE: The battle for the Moon continues
SOU,RCE: Tekhnika-molodezhi, no. 6, 1966, 8-11
TOPIC TAGS: moon, space, lunar surface, lunar radiation, lunar landing
/Geiger counter, Luna 9, Luna 10
i ABSTRACT- The interviewer revic~vs briefly the history of lunar research,
presents a table of chronology and facts and rt~pf!ats questions and answers.
Dr. M. L. Lidov stated that one of the prob,(2nis solved by Luna 9 and Luna 10
was that of landing at the mosi favorable tinic, ~. e. , lunar daybreak. Another
problem was the selection of the most "economical" trajectory along which to send
the heaviest apparatus. He stressed the importance of human initiative ir, the
Card -1/2

L 45257-66
FACC-MR--.A1k020934
guidance and control of space vehicles and this spoke of a third major problem
involving slowing down the space station. Tile braking process was controlled from
Earth and was started 2 1/2 hr before the actual landing. The flight problems
faced by Luna 9 and Luna 10 were similar enough but owing to a correction, Luna 10
i moved to a flight trajectory along which it approached the Moon to within a mintrnuni
distance of 1000 kin. Dr. A. 1. Lebedinskiy discussed the special features of the
i lunar landscape as transmitted on television, explained the structure of the space
station and its operation when taking pictures, also the topography of the moon.'
The objectives of Luna 10 were research on lunar space and lunar radiation.
Academician S. N. Vernov, a specialist in cosmic rays, stated that tile Geiger
counter installed on Luna 9 recorded protons, electrons, and gamma-quanta with I
a strength sufficient to penetrate the hermetically sealed space station. Lunar
radiation was found to be 10 times stronaer than that of tile Earth; it was found to
be harmless to astronauts clad in space suits. Orig. art. has: 5 figures and
I table. [GC]
SUB CODEL 14, 03, 18, 22/ SUBM DATE: none/
I" /, /
Card 2/2 "',-J\

ACC NR. AP7000546 SOURCE CODE: UR/0293/66/004/006/0838/0841
AUTROR, j&hcdinskiy,,A& le; Lozhnikov, A. A.; Tulupov, V. 1.
011c: none
TITLE: Neasurements of lunar radiation flux in the infrared and visible
regions of the spectrum by the Luna-10 satellite
SOURCE: Nosmicheskiyo Issledovaniya, v. 4, no. 6, 1966, 838-841
TONC TAGS: lunar radiation, lunar satelliEe. lunar'surface / Luna-10 lunar
satellite
ABSTRACT:
The lunar radiation flux in the infrared (IR) and visible spectral
bands was measured by the Luna-10 satellite from a lunar orbit. The
results have not yet been fully analyzed, and the data presented by the
authors are only preliminary.
Radiation in the two spectral bands was of different origin. The
visible band was used to measure radiation caused by heat from the
Sun being reflected by the Moon's surface; the IR band measured the
Moon - radiated heat which was emitted by the Moon's surface, the
temperature of which varies from -150 to +1200C. Infrared and
visible radiation coming directly from the Sun also contributed to the
total measured in both bands.
Card 1/6 UDC:

ACC NR.- AP7000546
A detector carrying two sensors (15 x 30-mm thin plates) mounted
outside the Luna-10 body were utilized to separate different heat ra-
.diation contributions (see I~ig. 1). The detector action was based on
the variable resistance principle (i. e. , changes in heat radiation varied
.the detector resistance). Detector resistance was measured by a cir-
cuit (such as a resistance bridge) and the results of these measurements
were telemetered back to Earth. One of the sensors was covered with
enamel, which absorbed 85-95% of the incident IR radiation and
reflected 70-751o of the radiation in the visible band, The other
sensor was covered with thin gold foil, which reflected 97-9916 of
the IR radiation and passed most of the visible radiation. Data taken
simultaneously from both sensors will be used to isolate that portion
of the total heat radiation which was contributed by the Moon. The
satellite was rotating around its own axis with a period which was
shorter than the detectors' thermal time constants, and the readings
therefore represent the average values of thermal radiation. The
sensors were sampled simultaneously every two minutes.
Card 2/6

ACC NR, AP7000546
Fig. 1. Thermal radiation detector
1 - Heat insulator; 2 sensors;
3 - clamping ring; 4 stand*
Temperatures measured by the sensors (A, with enameA! cover;
B, Aith gold foil cover) during the 8th, 31st, and 49th measurement
sessions are given in Fig. 2. In the 8th session the satellite crossed
Card 3/ 6

ACC NR: A?7000546
from the dark to the sunlit portion of the Moon. During the 49th session,
a crossing from the light to the dark portion was made. In the 31st
measurement session the satellite was on the sunlit side of the Moon.
-The time marks in Fig. 2 indicate Moscow time. As expected, the
,teiTiperatures on the light side of the Moon are higher than on the dark
.side. During crossings the sensors registered corresponding changes
in temperature after a time delay associated with their thermal inertia.
The influence of thermal detector inerti 'a was investigated by
taking temperature measurements at different instants during a single
session. The instants at which Ithese measurements were taken varied
from session to session. These readings are plotted and compared in,
the figure,. illustrating the effect of thermal time delay on.the sensor
-output.
-From 2-3 May through i3 May the temperatures of both sensors
.declined noticeably. The A-sensor temperature decreased by 22'C
and that of the B-sensor, by 50*C. After 13 May the temperatures
again began to rise. The speculation that this phenomenon is associated
with the changing orientation of the satellite with respect to the Sun is
-confirmed by the fact that the B:-Bensor, the more sensitive of the two
to the Sun's rays, was affected more than the A-sensor.
Cord 416

~i" 'TRMllWqw'
ACC NRt j%P7000546'
To
S.a sessionSIr

* "
JO
20 83 77 74 72 72 V, degme
108 101
8
to
~ Soo 014 h"(m
500
7,5
5O
J5#
J
20,J91" h M t
0
-10

40
.id 49.d SWSJM U-5.7
50
I1
1

q
0
10
card 5/6
j0
is 10 10 . . . . . . . . V, degree
10 ;Z
.10 KA4
7 Iiso ~007- 't
to..4
-10
4 Ii a N

=_77-
ACC NRi AP7000546
Fig. 2. Detector readings during sessions 8, 31, and 49
1 - B-sensor; 2 - A-sensor; y - angle between a line ex-
tending from the Moon's center to the Sun and a line
between the Moon's center and the Luna-10;.h-satellite height.
The authors state that.analypis. and evaluation of the. results will.
b.e published in-the future. The authors thank A. D. Levchenko and V. V.
Vernigor for assis6-qnce in the carrying out of the experiments. Orig. art. has:
5 figures. , OB: ve 39 no* i
.7
suB CODEs 22,03 / SUBM DATEt 22Aug66
Card 6/6

GALOYMN, M.Ya.; LEMINSKIYO A.P.1- ZELENSKAYA, R.G.
-U-ww~- .
Knock testing of automobile engines. Trudy lab.dvig. no.1:61-87
'55. (Automobiles--Mugines) . (MMA 9-,.g)

ARONOV, D.M.0 kandidat tekhnicheskikh nauk; LEBEDINSKIY, A.P.
Technical and economic effectivaness of raising the octane
number of atitomobile gasoline. Avt. i trakt.prom.no.10:5-11
0 156, Owu 10: 1)
1. Ilauchno-issledovatel'ski7 avtomotorny7 institut.
(Gasoline)

LUHV, I.S.; INBEDINSKIY, A.P.; SENUOV. V.M.
k & W ~ -. - ~, ~_
Portable cathode ray oscillograph for the photorecording of
deformations and VibratIons. Pribor'ostroanie no.10:18-20 0
.156. (ML 9:12)
(Cathode ray oscillograph) (strain gauges)

26(l.4) PHASE I BOOK ML431TATION SOV/2396
Akademlya nauk SSSR. Laboratoriya dvigateley
Teorlys, konstrukr%IXa, ranchet I lopytaniya dvigateley vn
nego agoraniya (Theory, Construction, Deaign.and Teetutre"i
In.
Internal Combustion Engines) Moscow, Izd-vo AN SSSR, 1957.
209 p. (Scrieas Itat Trudy, v~P. 3) Errata alip inserted.
4,000 copies printed.
9d. or Publishing Houses V. M. Klennikov. Tech. Ed.s A. 4.
Paylovokiy, Editorial Boards M. D. Apanhev, Doctor or Tech-
missal Sciences, K. 0. Yevgrafov, V. A. Lurlye, Candidate of
Tectusical Sciencesp and Yu. B. Svirldovs Candidate of Tech-
nical Sciences.
PURPOSEi This book Is intended for technical personnel working
with internal combustion engines.
COVERAOE: This collection or scientific pApers deals with inter.
nal combustion engines. The book Is divided into three parts.
The first part deals with gas turbines, the second with recip.
roosting Internal combustion engines, and the third with
Oda and equipment for Investigations. No personalltioa art
n-tioned. _R6.rerences follow each article.
;
PART III. )MIMODS AND EQUIPMENT FOR INVESTIOATION
J
Labedinakl thods of Road-testing Automobile Engines 1917
Txi' =-Yawlen-~41b"eB a method or road testing In which braking
of the automobile tested is accomplished by a towing automobile.
According to the author, this method makes It P0361.blo to regu-
late the braking Intensity In a wide range or speLds and load,
It is also recommended as an effective method for replacing
stand tests :in many cases.
AVAILABLE: Library of Congress
00/ib
Card 6/6 10-30-59

ARONOV,D.M., kandidat tekhnicheskikh nauk; LRBEDINSKIY, A.P. *; GALIPERIN, M.Ya.
Nonuniform performance of engine cylinders and gasoline octane
requirements. Avt.i trakt.prom. no.4:3-8 Ap '57. (MLRA 10:5)
l.Nauchno-issledovatellskiy avtomotornyy institut i Institut
mashinovedeniya AN SSSR.
(Antomobiles--Engines--Cylinders)
(Gasoline--Antiknock and antiknock mixtures)

KONEV, Boris Fedorovich; ARONOV, David Hatveyevich; EMOV. Boris Aiekse-
yevich; 1HBZDMMY, Aleksandr Favlovich; HILOV, N.A., inzh.,
retsenzent; TEGORKINA, L.I., red.; HAMMS011, V.A., red.; TIKHA~
NOV, A.Ya., tekhn.red.; UVAROVA, A.F.. tekhn.red. -A -
(Automobile carburetor engines; characteristics and methods for
their determination] Avtomobillnve karbiuratornye dvigateli;
kharaktoristiki i metody ikh opredeleniia. Moskva, Gos.nauchno-
tekhn.izd-vo mashinoctroit.lit-ry, 1960. 229 p. (MIRA 13:4)
(Automobiles--Nnginee)

LEBEDINSKIY, A.P.; GZRSHMAN, I.I., kand.tekhn.nauk
Automobile engines using various fuels. A-7t.prom. rx.4:IB-23 160.
(MIA 13:6)
1. Gosuaarstvewwy soyuznyy ordena Trudovogo Krasnogo Znameni nauchno-
iseledovatel'skly avtomobilInyy I avtomotornyy institut,.-
(Automobiles-19ngines)

LEBEDINSKIY, A. P.
Effect of antiknock qualities of fuel on the power and economic
indices of engines. Art. prom. 29 no.5:5-10 My 163.
(MIRA 16:4)
1. Gosudaretvennyy soyuznyy ordena Trudovogo KrAsnogo Znameni
nauchno-iseledovatellskiy av-tomobillnyy i avtomotornyy institut.
(Motor fuels) (Motor vehicleA-Engines)

. . . . . .. . . . . . . .z 'I'd `1 j 1. L
L. T. Imd U-YEV, 7h. F.
I I -
.. .. p
LEBSID!3MI--~~, ~-
"The Effect of ~hy3ical ~-Xfort on the j),trk-Adap tat*.. on of ti e &jell, Fiziolog.
Zhurnal SSSR, Vol. 16, 5th Ed., 193'-).

- ....- ......I
LEB~DIIII,'3i'r 1.1 Ij
- -. -f. A. V. p DIC".FE,~OV, 3. M. and TU' T3AH-V, Zn. 1.
IlThe Effect of deflex Excitations (Clold) on the Ligh~ Sensibility of the Dark-
Adapted Eye", Fiziolog. Zhurnal JSSR, Vol. 17, 1st. ed., 1934.

LEBEDlN3,K_-,1, A. V.
"New Investigations of the Problem of Interaction Between the Center and the Per-
iphery of the aetina - Report at the jonference of the V.I.E.M.", 1937.

A
f

ft a 23 26 27 21 29
o
it it 11 4 11 As 17
A
v
~ 13 As
x It 11 IS V

AL
s
L _u
,
- P_ L .d

1.0 'sho If. "I,
Is,
PROCCISE1 A-D PIPCOINT)l
KU, A. V.
Action of procaine an the effect produced on the pu
il
p
Is
If 11i t1lbbit IsT atimutation of the trigerninal nerve.
/imilits and A. V. f.clociliaskil. J. Phy%ja. -00
32, Kl-.S(l94n)fjn-Ruvqsn),-Jn eipi,. slah r.sbbst,.
h
7
l

I
, 1
rct orof stimulatiott of the ilith pair of the iligloliti.11 ee

nvr~vc its Smolfucing contmetillit of the pui)il is cmairiml. ~90
This effect persists whets atropine. curatc, nicotisie.

't-livilaline or "Witille are admillisirml rithcr infratc. "0o
nou'lV or directly tioder tile caiijillictiv.1 rill .01111lis-
i lee
trutw
l (of ptocitille (1) 1111&1 tile CtW1111111(tiva di'milied

tho- traimuiviiism o(excitation to the contra,tilu t:lcim-til, .1
-
thc
u
i1
Jn thi
w
I
l Is

: .
s
p
p
ay
comp
efel)
prct-ritts (fie dc%-clop.
tile
lot of the
ff
t
f
i
l
0 cc
e
o
ant
l
ronsic excitatioll of [lie affer.-Ill
nerve. Thi,; action of I tlcvclt)lis along ollith di%turtwil
roo

o 0 of other elsCitalf"ll, afolig "111'r illll,rfVjll,,Il
C:60

00 of file colitritclile drillorists, dml sh ... Nilig
th
t thk
i
t
a
act
on of I cattlaot be selective. After admini- oo
station of 1. the effect of acety1cholitit: oil tile pugoil is CIO*
jacativ rvilm-M S. C.0ttlich
too
too
AIS' 0

ILA
A It OtTALLURGOCAL LIMAJURE CLASSWICATIC10i
SIVIIISIV4
loollaiij *41 Oar IIIIIIII GIN amv M
I --- 1" -1 a rw a U

U U AT 00 Ali, t
IT IT a I? at a fit It W is it 09 KLG
10
a 00 0 0 0 9 00 0 00 0 00 4 06 a 00 00 0 0 00 09 0 0 0 0
of
siii, -db ! a al V 9 0 go
. a a 0 a * 0 0 0 * 0 0 * 0 0 0 000 0 4

LEBEDINSKIY, A.V., professor, doktor meditsinskikh nauk.
Analysis of functional states of the cerebral cortex in
penetrating cranial wounds. Trudy Gos.inst.po izuch.mozga*
15:140-145 147. MLRA 7:2)
(Cerebral cortex) (Skull--Wounds and injuries)
*VIorks of the State Inst. for Brain Study

LEDEDINSKIY) Andrey Vladimiro-Ach (Dr.), and MIKIMISON, M. I-
11 ;, s undcr ti;e
Reselient-Viscous Properties of the Skeletal muscle and its thane
Influence of Sjppathetic Enervation." Zef. Zhur., Vol 33, No 4., 1947, P 5%.
-paculty of il~ljsiology, Military Mled Acaa-i-m';-niKirov.
SO: U-4396

(90
LEBEDINSKIY, Andrey Vlidimirovichy, -and SAVVIi.', N.
IlOn Relations of 'ympathetic Enervation to the Reaction of Contractinr Foruations
onEfferent -nfluences of Various ;-vpss." Zef. Zh-kr., V,-)133, llo 6, 190, p 7L-9.
Chair of Physiolowl, Military '~ed Acad M. 'Korov.
SC-. U-4396

V.
USSR/Kedicine-Publications NOV 49
Yedicins-Ir'ater Supply
41few Books" p
"Gig i San" No U
Lists new books, giviag authors,, publishing dates and prices. Includes Vd. Kozhim's
0
T;Tmter Supply" and A. G. Ginstainskiy and A. V. Lebedinskiy's "Fundainentals of Hman and
Animl Physiolool."
?A 49/49T?7

VM/Yedicima Optics NOV/Dee -48
---Eye, Adaptation-of
."Contempory Representations of the Mechanism of
;Optical Adaptation to D&rkness,!Z A. V.
-4 Lebedinskly, Leningrad, 22 ppI
f"Uspekhi Sov--em.Biol7 Vol XXVi, 116-3 (6)
~'Theory that toculsx adaptation is a process of
~increase in the sensitivity to light which occurs
In weak illumination remains valid,'but Importa Int
'details have I~een addedand whole.,process of adapta-
tion bas been ezwmined fici various N eypoints.
CW=jnk&-=s and amoqws author., a, experimiiis 'and
Condlusions of many otb~er aut~,Oris.
3/5OT55~

MM-,,'DTNVTY~ A. V.
Assoc. Men-ber, U5971 Academ,,;, of ~.eilical -`:?cience.
III.P. Ravlo-tr on the Tronhic Role of the Nervous
System." Izvestia, 1949, Lecture
j
Current Digest of the Soviet Press, Vol. 1 No. 36, 191,9, page 55, (Tn 4MLibrary)

LEBEDINSKIY,, A. V.
33468. K Stoletiyu So Dnya Rozhdeniya I. P, Pavlova. Voprosy Neyrokhirurgii,.)
1949, No. 5l c. 12-16, c. Portr.
SO. Letopial Zhurnaltnykh Statey., Vol. 45, Moskvap 1949

USSRtNedicine - Intestines, Physiology Jan 49
Medicine - Intestines, Sensitivity
"Problem of the Sensitivity of the Internal Organs" A. I. Bronshteyn, A. V.
Lebedinskiy, V. M. Simenko, Chair of Physiol, Chair of Faculty I-lurg, Mil Med Acad
imeni 3. M. Kirov, 12 pp
341
"Fiz:64 Zhur. a56W1 Vol XXXV, No 1
Conducted tests on four animals with abnormally small intestines to determine degree
of expansion before pain became noticeable. Determined that the animal sensory reactions
could be observed not only when intestine was moved, but also when an electric charge
acted on interior walls of the intestine. Charge produces reactions by : (1) stimu-
lating peristalsis of the intestine (direct current), and (2) irritation of the
sensory nerve in the caecum. (pulsed current).
PA 47/49T62

~ e b (:1 (~ ( vil k IV) /-) ~ t -
DYMSHITS, L.A.; LIBEDINSKIT, A.Y.; PITM, I.A.; SHULITS, V.A.
Application of electroratinography in glaucoma. Vapr. klin. eksper,
oft., Moskva no. 1:30r4l 1952. (OLML 22:4)
1. Leningrad.

1. LEBEDINSKIY, A. V.; MQ77MIJUMT, ~* - s.
2. -
4. FlectroDhysiology
.*I,
7. 1. P. Pavlov on the work of V. Yu. Chagovets. Fiz-. 3hur. 39, No. 2, 1953.
9. Monthl List of Russian Accessions, Library of Congress, April -1953, Uncl.

IEBEDINSK31, AN.
I
e
rii;fRiuence of ionizing radiation on the anlrol organism; as
revealed by studies df Soviet investigators]' 0 vIiianii ioni-
ziruiushchego izlucheniia na organizm zhivotnogo; po danmym
rabot sovetskikh issledovateldi* Moskval 1955. 35 p. (MIU 14:6)
(RuicioN-pusioLoGicAL xmcT)

F 13 9b I 05/f I Y, AV
Radiatsionnaya Meditsina (Radiation Medicine), edited by A. V.
'Lebedinskiy, Moscow, Medgiz, 1955, 278 PP (from Sovyetsko~e_
Meditsinskoye Referativnoye Obozreniye: Vnutrenniye Bolezni,
No 24, 195b, p 96
The book is a handbook on the physics and the biological action of
radioactive radiation, and consists of eight chapters covering the fol-
lowing material: physics and dosimetry of penetrating radiation, basic
laws of radiation injury, pathologic physiology of radiation injuries of
various systems of the organism, toxicology of radioactive substances,
clinical aspects and therapy, radiation burns, clinicolaboratory methods
.of diagnosing radiation sickness, and pathologic anatomy of radiation in~
juries.
The-book is intended for physicians and students. (U)

USSR/Hunan and Aninal Physiology (Normal and Pathological) T
Effects of Physical Factors. Ionizing Euissions.
Abs Jour: Ref Zhur-Diol., 1,10 17) 1958Y 80118.
Autbor Lebedinshiy, AN.
Inst
Title On the Difluence of Ionizing Radiation on the Organs
of an Animl (According to Data of the Work of Soviet
Investigators).
Orig Pub: V.sb.: Deystviye oblucheniya na organism. M., Izd-vo
All SSSR, 1955, 43-77.
Abstract: Review. Probleus are discriminated on the influence
of ionizing radiation on the functional condition of
the CNS, the morphological changes of the nerve cells,
skeletal macles and skin coverings, on the change of
reflex and conditioned reflex reaction, the condition
Card .01/2
114

USSR/Humn and Animal Physiology (Norma-I and Pathological). T
.v Effects of Physical Factors. Ionizing Emissions.
Il I - ~'13 Jour: Rof Zhixr-Diol-, NO 17, 1958, 80118.
of the interoreceptors, as well as on the nucleic
acid metabolism chwves in the b1cod picture mid
the blood-forrAna organs and the permeability of
the blood-brain barrier. Dib- 76 titles.
Card : 2/2

EXCERPTA MEDICA Sec.22 -V01.20112 Ophthallrr.Llogy Ded 56
180L LEMEDINSKY A. V. and PEYMEV 1. A. Dept. of Physiol., Milit. Med. Acad.,
LeMn-ir-07vRolar izat ion phenomena in the retina of the
eye (Russian text) f'R0BL.FIZI0L.0PT.(htoscow) 1955, II(I.07-It2l
Tables 2 Illus. 3
The experiments were performed on enucleated eyes of tile spring frog. The eve
was ptit on a small gauze pad, moistened with Ringer's sulution and plact-d in .1
smill dark chamber. One chlorinated silver electrode was connected to tile Inar-
gin of the cornea, the other to the back-pole of the eye near the outlet of the optic
nerve. The currents in the retina were registered by the loop oscilloyraph. The
indifferent polarizing electrode was connected to the gauze pad, the active polar-
izing electrode was placed on the surface of the eve bulb between the electrodes
connected to the oscillograph. The strength of tile polarizing current was 20-100
;An. The electroretinogram taken during the illumination of the eye had been re-
gistered before the switching on of the polarizing current, during its action and
after the switching off. The following results were obtained: during the passing
of the direct current and polarization by the anode a distinct lowering of all tile
3 peaks, W, 'B' and 'C', was observed; the lowering was, to a certain extent,
proportional to the strength of the polarizing current. By polarization with the
cathode a marked heightening of all the peaks was noticed. particularly of th~
peak W. After the switching off of the polarizing current, while polarizing with
i the anode, a distinct increase of the waves was noticed, while, when using the
cathode as polarizing electrode, a distinct decrease was noticed after switching
off. The changes in the ERG. induced by the polarizing current, vanished only
3 min. after the switching off. The authors regard the results obtained as proof
of the fact that the waves 'B' andC' of the ERG are the electrical expression of
the activity of the ganglionic cells of the retina. The changes.observed in the ERG
during the polari"flon of the retina aret considert4 to be chanires in the functional
state of the nerve cells.
Tron - Leningrad (XII. 2)

LEB-DiINSKIY, A. V.
IlEffects of Ionizing iadiation of the Nervous System of Animals," Meditsinskiy
iagotnik, Vol. lF, N-0. 66, 1955.
Z-Comment: This paper was presented by the author at the Geneva Conference on the
Peaceful uses of Atomic inergyj-
Translation W-31506, Oct 1955.

USSR/General Division Congresses. Sessions. Conferences. A-4
Abs Jour : Ref Zhur Biologiya, No 1, 1957, 88 K.
Author : AN. Lebedinskly, Editor.
Inst
Title : Theses of the Plenary Reports Read at the All-Union
Conference on Medical Radiology, Moscow, 1956.
Orig Pub : M., Medgis, 1956, 31 pp.
Abst No abs`tract.
Card 1/1

/I _z- "j,
KROTKOV, F.G.,redaktor IGILATIYEV, A.I.,
redaktor; LANDAU, S.P.iAda~ IMANOVA, T.M.,redaktor;
BELICHIKOVA, Yu.S.,tekhnichaskiy redaktor
(Abstracts of reports at the conference on late sequelae of
affections caused by ioaizin&r6diation] Referaty dokladov na
konferentsii po otdalenriym poiledetviiam porazhenii,
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'(RADIATIOR-PHYSIOLOGICAL EFFECT)