SCIENTIFIC ABSTRACT GRIGORYAN, L.A. - GRIGORYAN, N.A.

• Document Type: CREST
• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R000516730007-2
• Release Decision: RIF
• Original Classification: S
• Document Page Count: 100
• Document Creation Date: January 3, 2017
• Document Release Date: July 27, 2000
• Sequence Number: 7
• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT

GINZBURG, V.L.
0000~
Conveyer belt with n zipper fastener (from "Gummi u.Aabest,"
10 no.2 1956). KFrach.1 rez. 16 no.5:39-4o my $57. (MIRA 10:7)
(Belts and beltinp)

GINZBURG, V.L.; ROTLEDER, V.M.
Reviev of foreign patents of tyke ORS" tires. Kauch.i rez.
22 no.2;36-38 F 163. (MIRA 16:2)
1. Nauchno-isaledovateliskiy institut shinnoy promyshlemosti.
(Tires, Rubber-Patents)

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W. M. Stemberg

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Category: USSR/Analytical Chemistry - General Questions. G-1
Abs Jour: Referat Zhur-Khimiya, No 9, 1957, 30945
Author , Ginzburg V. L., Alekseyenko Ye. F., Belokrinitskaya Ye. Ye.,
--V_ff.-u-sHRIn-K-T-.-N., Ineshins. F. M.
Inst : not given
Title : Accuracy of Photographic Methods of Spectral Analysis
Orig Pub: Zavod. laboratoriya, 1956, 22, No 11, 1331-1333
Abstract: A comparison was made of the accuracy of anstlyses of fused nickel,
copper regulus, fused cobalt and cathodic nickel, according to
calibration graphs in & 3, lg C coordinates, and in accordance
with the solid graph method, Determinations were made of Cu, Fe,
Au, Pt, Pd, Ni, Si, Mn, Pb, Sb, Bi, Sn, Co, at concentrations from
several thousandth to decimal fractions of one percent, with spec-
trum excitation in are discharge of direct and alternating current,
and photographic recording on plates of type I, II and III. In
most instances no substantial differences were found In the =gni-
tude of errors with different calibration graphs.
Card 1/1 -18-
USSR/Optics - Optical Methods of Analysis. Instruments. K-7
Abs Jour : Referat Zhur - Fizika, No 3) 1957) 7962
Author : VitushKina, I.N., GinA3pre, V.L.
Inst : Norillsk Mining and Metallurgical Combine, USSR.
Title : Spectral Analysis of Nickel in Low-Voltage Spark Using
Cast Electrodes.
Orig Fubq ; Zavod. laboratoriya, 1956, 22, No 4, 436-44o
Abstract : In the determination of copper and iron admixtures in
pure nickel, the spectrum is excited by a DG-1 genera-
tor, operating in the spark mode (current 2 2-5 amp).
The analytic pairs of lines are Cu 3273-96 Ni
3286-95 A end Fe 2599.40/57 -- N 2551.01 A. The inter-
val of the determined concentrations of copper and
iron is 0.01 -_ 0.5%.
The mean arithmetic error of the determination ranges
from 5 to 9%.
Card 1/1 - 105 -

AUTHORS: Nedler, V.V. , Gimburg, V.L. 32-24-4-64/6,7
TITLE: The Third Conference of Spectroscopy Analysts of Nonferrous
Metallurgy (Tratlye soveshohaniye spektroskopistov-analitikov
tsvetnoy metallurgii)
PERIODICAL- Zavodskaya Laboratoriya, 1958, Vol. 24, Nr 4, PP. 507-508 (USSR)
ABSTRACT: The abo-v-3 mentioned conference took place at Moscow from November
`5 to November 20, '1957; it was called by the Soientifio-Technical
~ccn-ety of Nonferrms ile-tall-urgy, and was attended by 255 re-
presentati7es of 175 orgarJ-zations. The contributions made by
I.E. Britske (Gintsvetmet, Moscow) and N.S. Poluektova. (Ukrgiredmet,
Odessa) dealt vd.th T;.es+,ions of flame photometry. The report ae-
livered by L.I. Kononenko dealt with the method of determining
zirconium, hafnium, molybdenia and vanadium. An interesting con-
tribution was made by Ya.D. Raykhbaum, Ye.S.Kostyukova, and
V.D. Malvkh. (Irgir-admet, Irkutsk) under the title "On some Causes
of the Influence Exercizied by Chemical Composition on the Results
of Ore Analyses". A detailed r
cowjort by N.A. Makulova.
(Giprotsvetmetcbrabotka, Moe dealt with investigations of the
Cara 1/3 rale governing the tx-arLgition of --,est mateeial to the emission

The T!jrd Conf erence of Speoiroz copy Analp- ta 32-24-4-64/67
of Nonferrous Metallurgy
clozO. A.A.Frishberg ancl V.V. Nedler (Nigrizolato, Moscow) spoke
albout problems of the pbysical-chemical th,-.ory in connection with
chemical reaotions during the forwation of -vola-cile compounis in
the elaotrio arc. V.L. GInzib-arg (Worlllsl-Ay CoDJ)ALve) ga-re a re,
pore or tne devel 'upment of a ruethod of deteradning the temperat-,;re
Intensity of ellectrole~. The following contribuUone dealing with
special methods of spectral arz-lysis duser-ie mentiouing: The re-
orti by D.M. Shimrts,, L.N. Kapor,9kiy and V.V. Portnova
Gipronikel' , Leningrad) ani I.S. Nilo-,u (Sev~.-ronAel' Monchtgonk)
r
which deal vrith th6 amlysis of zinc, thallium wxd antimoU; the
rdport5 by S.M. Solod;y-,-viik (Gire3yret, Moscow, ) anA others. or. the
analysia of zil-,'.con, 4ill.con diox-Me and siliclo aelli -the; reporth
by V.P. Khrfpiy and 0,11. Gusev or. the increa:3tj oe .3ensltiviiy in
determinatiorn of microadmiuture.9 in sil-.Y-er, the ccmtributions
made by N.A. SinIkov and D.Y. Liv3hits (Norl!13?k Combfne) deal
with the analysis of solutiorz containing platinum metals. The re-
port delivered by V.0. Khandros and L.N.Filimonov (Giprotsvet-
metobrabotka) deals vnlth the problems of the application of quanto-
meters. A.G. Kres-L'yoninov, Yu.I. Stakheyev anvi Ya.D.Raykhbaum
Carl 2/3 (Irgiredmet) were the first to use photoelec+rla apparvatw? for thj

The Third Conference of Spectroscopy Analysts 32-24-44b/6-~,
of Non:ferrous Metallurgy
direct am2,vais of ores for lith-4,un. The contribution made by
V.V.Nedler domalt with attempts made at using the horizontal
el~cteio are, stabilized by an air current. The reeporis con-
cerning standaris pt;:blishea by the institutes Gintsvetmetp
Giprots7etmetobrabotla, VIM (all at Moscow) , TsNIIolovo
(NovoEPA.rsk) , Irgiredmet (Irlaitsk) , Gipronikell (Leningrad)
VNIItsvetmet (Ust' -Y.Ammogorsk) , Ukrgiredmet (Odessa) confirm
the work performed by these -institutes during recent years. The
necP,3.iIiy of centmlizing the pullishing of standa-Ms was
stressed, and the industrial production of high-quality spectral'
cvArbcvxr3 cAnd an increased dist,~ibution of ordinary spectral
carbonz, mw urgently deman3ed.
1. 14etall-drgy--USSR 2. Spectroscopy--USSR
Car-I 313

r- s a a 1~
TO P
fill V I
go
All

L. (i.100cm)
113pectral Method of Analyisis of Technical Teilurilim in Ubble Metals.11
paper submitted to the Fifth Conference on the Analysis of Nobel Metals.,
Novosibirsk, 20-23 September 1960
So: Zhurnal analiticheskoy khimii, Vol XVI, No 1, 1961, page 119

.,_GINZBURG, V,L.; ROGOVER, GvB,
Regularities in the distribution of nonferrous
the predominatit ore minerals and silicates of
Sov. geol. 3 no;3:48-60 Mr 160.
'l. Hinieteretva geologli i okhranv nedr SSSR.
(Nori'llsk region--Metals)
and noble metals in
the Norillsk deposit.
(MIRA 13:11)

S/032/60/026/05/18/o63
BO1O/BOO5
AUTHORS: Ginzburg, V. L., Glukhovetskaya, N. P.
TITLE: Determination of Silicon and Other Impurities in Selenium
PERIODICAL: Zavodskaya laboratoriya, 1960, Vol. 26, No- 5, PP. 559-561
TEXT: N. N. Danilova and L. A. Lerner collaborated in the experimental
part of the present investigation, A spectrum analysis for determining
impurities in selenium was worked out. The calibration samples used were
produced by fusing together Si and Be; less Si was used than corresponds
to the stoichiometric ratio in the compound SiSe2. Thus, it was possible
to obtain a chemically stable mixture of Sise and Be. Br increasing the
2
addition of Se, a series of calibration samples was produced up to a
Si content of 2-10-4%. silicon was determined.ace3rding to the following
spectral lines; Si 2516.12A (from 1,jo-4 to 3 10- % of Si), Si 2881.58A
(from 2-10-4 to 2-10-2~ of Si), Si 2514.33A (from 1-1o-3 to 5-10-2% of Sj)~
Si 2435-16A (from 1-10-2 to 3-10-1% of Si). The calibration samples for
determining the other impurities in selenium were also prepared by fusing
together the initial alloy with pure selenium. The initial alloy was
Card 1/2

Determination of Silicon and Other S/032/60/026/05/18/o63
Impurities in Selenium B010/B005
produced at the institut "Gintavetmet" ("Gintevetmet" Institute), and
contained 1% each of Cu, Pb, Mg, Al, Ag, As, Fe, Sb. Ni, Bi, Te, as well
as the selenideB of Cd, 11g, Sn, Cu, Ni, and/or their melts with selenium
The samples, as well as the calibration samples, were granulated and
fused into the crater of the carbon electrode (Fig. 2). There are 2
figures and 4 non-Soviet references.
ASSOCIATION: Institut obshchey i neorganicheskoy khimii im. N. S.
Kurnakova Akademii nauk SSSR (Institute of General and
Inorganic Chemistu imeni N. S. Rurnakov of the Academy
of Sciences, USSR
Card 2/2

SVESHNIKOVA, V.N.; GINZBURG, V.L.
Study of the ternary system consisting of cerium phosphate
phosphoric acid - water at 700C. Zhur.neorg.khim. 7 no.5:
1169-1173 My 162. (KRA 15:7)
(Cerium phosphate) (Phosphoric acid)

GINZBURG, V.L.; GLUKHOVETSKAYA, N.P.
Spectral line intensity as a function of the effective ionization
potential of an electric are. Opt. i spaktr. 12 no.3:344-349
Mr 162. (MIRA 15:3)
(Spectrum analysis) (Electric are) (Plasma (Ionized gases))

~N~BURG, V. L.; GLUENVIMKAYA, N. P.
Note on 0. P Semenova and N. 1. Levehenko's article n)ependence
of the effe;". ionization potential on the concentration of
readily ionizable impurities in an are discharge." t. i "ktr.
13 no.6:831-882 D 162. (MIRA 1~
(Electric discharges) (Ionization)

S/075/62/017/009/005/006
E071/E436
AUTHORS: Ginzburg,,V.L., lukhovetskaya, N.P., Danilova, N.N.*
-~,TITLE: A spectrochemical method for the determination of
.impurities in selenium
PERIODICAL: Zhurnal analiticheskoy khimii,*Y,17, no.9, 1962,
1096-11Q0
TEXT: A method of determination of small amounts of impurities by
their preliminary concentrationand subsequent-spectral analysis
is proposed. The concentration is carried out by distilling a
of selenium placed on a*powdered carbon support at 315% in
a stream of nitrogen oxides. Selenium distils off in the form
Of Se02 while impurities remain in the carbon powder which is then
To increase
submitte.d to spectral analysis on carbon electrodes.
the sensitivity of the determination of impurities in carbon powder,
sodium chloride (0.6*,,'G*) or potassium chloride (0-350 are added to
the concentrates. The degree of recovery :of various elements in
the concentrates was tested. According to-the degree of recovery
:the elements were divided into three groups:,-'I) 70 to 8051o', Au, Mg,
Sn,' Sb, Bl, Te, Al, Cu, AS; '2) 40 to 500' Cd, As, Fe, Pbs Ti, Mn;
Card 1/2

S/075/62/017/009/005/oo6
A spectrochemical method E071/E436
io
'3) 20% Cr and Ni. For the elements of the*3rd group, the method
cannot be used. There are 4 figures and I table.
ASSOCIATION: Institut obahchey i neorganicheakoy khiml'i im.
N.S.Kurnakova AN SSSR Moskva (Institute of General
and Inor8anic.Chemistry imeni N..S.Kurnakov.AS USSR,
Moscow)
SUBMITTED: November 20, 1961
Card 2/2

S/032/62/028/006/012/025
B101/B138
AUTHORSs Ginzburg, V. L., Glukhovetskaya, N. P., and Lerner, L. A.
TITLEi Increasing the sensitivity of the spectral determination of
impurities in selenium
PERIODICALs Zavodskaya laboratoriya, v. 28, no. 6p 1962, 682 - 684
T---'XT; By adding NaCl (ionization potential V 5-1 ev), the V of
i off
the arc plasma may be controlled in such a way that the sensitivity of the
impurity determination is increased considerably. Calibration curves AS
against log C were plotted for selenium samples with impurity standards in
the presence of carbon powder containing various NaCl additions in the
counterelectrode. The dependence of the intensity of the spectral lines
on V was determined. V - 8 ev, achieved by carbon powder
i eff i eff 0 7
with 1-j.' Ila (- 2.5% NaCl), was the optimum. The sensitivity increase
results from the ratio AC - C without NaCl A NaCl' For the elements -
investigated, the following 6C values were founds Te 0.46; Hg 0.201 As
0.50; Cd 0-30; Mg 5.0; Ni 2.2; Al 5-5; Au 5.0; Pb 4-0; Bi 2-5; CU 5.01 Ti 5-01
Card 1/2

Increasing the sensitivity ...
S10321621028100610121025
B101/B138
Sb 1.0. Tne brightness of the Cd, 11g, Te, and As lines is not increased
when reducing the selenium arc temperature because of the high ionization
potential of these elements (V,,)~8.6 ev). There are 2 figures and I table*..
ASSOCIATIONt Institut obahchey i neorganicheskoy khimii im. N. S. Kurnakova
Akademii nauk SSSR (institute of General and Inorganic
Chemistry imeni N. S. Kurnakov of the Academy of Sciences
USSR)
Card 2/2

GI�&%ghIOV"L ; GLUKHOVETSfAYA M.P.; LERNER, L.A.
- ..1 1 .~ '4
Fluorination of samplea in epectr~l analysis. Zav. lab. 29
no.6:684-685 163. (MIRA 16:6)
1. Institut obahchey i neorganicheskoy khimii imeni N.S.
Kurnakcrwa AN SSSR.
(Spectrum analysis) (Fluorination)

GIN7BURG? V.L.j LIVSHITS, D.M.; SATARINA G.I.
Determination of silver, gold, jalladluin, platinum, and rhodlum by
atomic absorption flame spectrophotometry. Zhur.anal.khim. 19 no.9:
1089-1093 164. (MIRA 17: 10)
1. Kona truktorskafe by-uro IIISvetmelavtcmatikall I TSentrallnyy
nauchno-issledovateliskiy gornorazvedochnyy instituil, Moskva.

cl-~Nll'l Bl"RIG ; v0,*-*ER'l;Oy,
y
Gravithtional colipp6c of' ii marmet,;--; -,,hl,-. vl-,".qp~ -' I-f~or.
fiz. 47 no.3-1030-1040 S~ 164. / - , -. . -
t -Izt 1 1 ~ -,
1. Fizicheskly instit-ut imen! -,A~be~ipva AN

GIMBURGY~ V.I,.; RETAYEVSKIY, L.P.
Optical -propertiea of polyvalent irateala and electron interaction.
Dokl. All SSSR 163 no.6zl352-1355 Ag 165o
(MIRA IM)
1. Fizicheskiy institut imo P,NeLebadeva AN SSSR i Institut
fiziches'kikh problem AN SSSR. 2.. Chlen-korrespondent AN SSSR (for
Ginzburg).

L 112,~po-.66, m1r!wA (h) Gi
ACC NRt 6 -00'26 8" SOURCE CODE: UR/0033/651042f=71129111'
AUTHOR: Ginzbur , V. L.
ice
ORG: Institute of Phraics of the Academy of-Sctencesj8SSR (Fiticheskiy inatitut
im. Lebedeva Akadeniii nauk SSSR)
TITLE: Cosmic rays and plasma phenomena in the Galaxy and the Metagalaxy
SOURCE: Astronomicheakiy zhurnal, v. 42, no. 6, 1965, 1129-1134
TOPIC TAGS: cosmic ray, metagalaXy, opave, magnetic field,
galaxy, p14*-.vta, adiabatic invariant,W AAA~ f rZt4A---
ABSTRACT: It hp been generally held that in metagalactic space no anisotropy
of cosmic raysil6an exist because the magnetic field of this space is unable to
od;-et the anisotropic pressure of cosmic rays. This, however, has not been borne
out by calculations. The problem of anisotropy of cosmic rays and the transition
space between a galaxy and the Metagalaxy is considered to be unsolved. V. L.
Ginzburg hypothesized that the unsolved problems of cosmic rays are associated with
plasma effects Irr space, especially with cluster and other instabilities in rarif ied
plasm . The transition of the magnetic field from galaxy to metagalactic space
occurs smoothly without hindrances. I:h moving under such conditions, anisotropic.
cosmic rays preserve the adiabatic invariant and form cluotere in the Metagalaxy'
The clusters move along magnetic force lines and become unstable, generating their
own waves. Instability of the cluster causes turbulent motion in the plasma and
Card 1/2 "Jur"
Z-1

L n250-66
~iC-C NR, AP6002686
isotropic motion of the cluster. A transition region is formed in -Aich the magnetic'
field becomes turbulent and the movement of cosmic rays Isotropic. In thii way
a solution is''found for the unsolved problems of cosmic rays in metagalactic
intermediati space. 10rig. art, hast 8 formulas, (EGI
SUB CODE: 03/ 61IBM DATE: 29Apr65/ ORIG REFs 0181 OTH REPI 006/ ATV PRESS;

L 15889-66 c) JD
ACC NR: AT6002491 SOURCE CODE: UR/0000/65/000/000/0001/0009
AUTHOR: Ginz burg, V. L lHotulevich, G. P.; Pitayevskiy, L. P.
ORG: Physics Institute im. P. N. Lebedev (Fizicheak;,y institut)
TITLE: Optical properties of polyvalent metals and interelectronic interaction
SOURCE: AN SSSR. Fiziche:skiy institut. Doklady, 1965. Opticheskiye svoystva
polivalentnykh metallov i inezhduelektronnoye vzaimdeystviye, 1-9
TOPIC TAGS: electron, gold, aluminum, tin, lead, electron interaction, metal
crystal, permitt ivIty, absorption band
I
ABSTRACT: In polyvalent matals (J Sn, Pb), on the one hand, the approximation
of weakly bound electrons is adeifu-ate;_`but7`on the other hand, the concentration
of optical electrons Nopt is much lower than that of valence electrons, Nval (by
definition, N t figures I the expression for the permittivity LC 4f.4 43opt
for optical i0r9quencies v 11!ying outside the absorption band). This F3w-z
difference can be explained by the Influence of interelectronic Interaction, since
in the theory of the Fermi liquid for cryst! ine metals Hopt A Nval. -At the @=e
time, for liquid metals, tits equality Hopt 21 Nval should take placeg and this Is
indeed observed in practice.-.-Authors are grateful to M. Ya. Azbell and D.-Pays fo
Car"/.2

L 15889-M
ACC NR: AT6002491
a discussion of.the problems touched ispon in the present note. Orig art. has:
2 tables and 5 formulas.
none
SUB CODE., 07,v20 SUBM DIOTE: ORIC REF 1 013 M REF. 004
Card 2/ 2
7, -V 1
. . . . . . . . . . . .
NOW T
ANN() WMM

GIMMURCY, V.L.
Cosmic rays and plasma phenomena in the ralaxy ar;cl meLagalcocy.
Astron. zhur. 42 no.6:112?-1134 Y-D 165. (L%mv~ 19. 11)
1. Fizichesidy instituL ha. Lebacleva '~?! SSSII. Submitted Al)!--,! -19,
1965.

259-30-66 7-w7(,-n);~. LJP(c)
ACC NR, Ap6ol6663 R.-M--,--C- O-D~ T- K160573 510 M70- W, 6.'df
AUTHOR: Ginzburg, It. L.; qyrovatskiy, S. I
ORGI none
TITIB: Cosmic magneitobremsstrahlung (synchrotron) radiation
SOURCE: Uspekhi fizicheskikh nauk, v. 87,,no. 1, 1965, 65-M
TOPIC TAGSs bremastrahlung, cosmic radiation, partiole.aoceleration, relativistic
particle
e
ABSTRAC Magne-tWbremigstrahlung theory Is reviewed and Itdiol
;in raalodstronomy and astrophysics is described. All of the
tneoessary details are ISIven for the application of the theory to
iastrophysical problems. Magnetobremestrahlung Is rather wide-
ispread In spaoet cosmic radio-radiatlon In most cases has magne-
tobremostrahlung charaoteristics. This holds for the overall
galactic radio-radiation, as well as for that from supernova,
ordinary and radio ghlaxies, etc. liagnetobremsatrablung is highly'
,important In the atudy'of the origin of cosmic rays and gamma- ozd,
ix-ray astronomy# The nature of electromagnetic radiation from
laooelerabing nortrolativistio and super-relativistio partioles-la,
~disouseed, and formulae are derived for Individual electrons,
IThis Is, compared with magnotobromootrahlung from groups of eleo-;:"
Card 1/2 UDC: 323.165

-L 2593o-66
ACC NRt AJP601666~-)
i~rons g and the .1,5tokes parameters are defined. The Influence of
cosmic plasma ort the propagation and radiation of electromagnetic
Yaves Is considered. It Is pointed out that magnetobremastrahlung
.1radiation can be reabsorbed by relativistic particles, and the
Absorption coefficient to calculated, Certain applications f, "J
,'wAgnetobremestrahlung.are diacussed in relation to cosmic plasma--~,..,
:and magnetic Inatabilitlese_The more,--imuortant formulau are.,
1summarize x1thout pr;Lqti,-' Origo art* hast 8 figures, 4 formilas-,'-and
table's ,TM
R V
SUB CODFt 20, EIUEM DAIISt none~ /,.'ORIG REFt 042 OTH REFI 027
Card 2/2
17

L 25773-66 - EWTQ) ON
ACC7i~R, AP6016379 SOURCE CODE: UR/0048/65/029/010/1825/182911
AUTHOR: Ginzburg, 11. L.; GzernoZ, L, M.; Syrovatskiy, S. I.
ORG: Physics-Institute im. P. N. Lebedey, AN SSSR (Fizicheskiy institut AN SSSR)
TITLE'. Relativit5tic, electrons in the M82 galaxy- eR~
SOURCE: AN SSSR. :Ezvestiya. Seriya fizicheskaya, v. 29, no. 10, 1965, 182~-1829
TOPIC TAGS: gala_xy,, relativistic electron.. hot star, Compton effect, bremstrahlung,,
pi meson, nebula/MV galaxy
,ABSTRACT: 'The gaiaxY M82 (aiso' called NdC 3034 and 3C 231). whloh-~
'is part or'the UIrsus Major group, Is of special Interest, since
'its relatively close position makes possible a comparatively de-
.tailed study of thd nonsteady-etate (explosion) stage of galactic
.development. It belonge In a special subclass of Irregular galaxot,
:les Whose members are characterized by an anomalously red lightq
thigh luminoeit Iy co-nelderable quantities of dusty matter with
',floooular' structure, and the absence of high-luminoolty hot
.In this connection, the authors present formulas for calculating'...,.:
ithe energies and energy losses of the relativistic electrons In,. '.t.
,this galaxy - partioularly.with respect to the total energy of,~
the. light-emi-ttl~ng.-re,,lat,ivlotio -electronaj the-energy losses
ICar 1/2'

ACC NRi APOW79
to the Compton el7footo and the energy losses due to magnetic
bremostrahlung. It Is shown that the total flux of Compton rays'
,from M82 equals the Compton losses. An evaluation of the brems-
strahlung flux of r.-rays due to the decay of 0-mesons and brems-;
Istrabluns is prenented. The magnetic X-ray bremastrahlung of M82
lis evaluated on the aaeumption that,the optical spectral Index of
iM82As close to I;he optloal Index K * 1 6 5 !pr the Crab NebUlaq which.,
jis eorreot_only up to the f requenoy Yo '1010 cpsAi Or-ig. dit. hiff!
12 f omulae. (JMS.1
SUB GODEts. 03, 20, SUBM DATE: none. ORIG R ff: ON RE, F: .012
Card 2/2

E?IT(],)/FCC GH
ACC NR1 AP60231,30. SOURCE CODE: UR/0053/66/O88/OQ3/W5/O5C4
AUTHOR:'~'dj'
MlLmArp V.,L.: Syrovatakin S. 1.
..'ORG Fhysica Inatitute.*im. P, No Lebedev, AN SSSR (Fizicheskiy inatitut AN SSSR)
Tl=i' 'Origin of comic rays
SOUR=:, t1spekhi f1sicheskikh nauk, v. 88, no. 3, 1966, 485-504
j-
-
dko Wer comic' ray# simpernova, astronomic conference, galaxy, electron spectrm
T
'ABSTRACTi.-- It in argued that cosmic rays cannot be of metagalactic origin and that
plasma effects are of fundamental importance to the further development of the
-.-astrophysics of comic rays; this also pertains to the quasars. According to the
hors, the principal sources of cosmic rays in the Galaxy are the bursts of
agt
and possibly also explosions of the galactic nucleus. Emphasis is placed
on the role of instability in the formation of the boundary of the galactic halo
and in the isotropicization of the cosmic rays emerging from the Galaxy into the
Metagalazy., Allowance is made for the now knowledge that has been gained following
the.Jaipur Conference on.Coandc Rays in 1963. The Ninth International Conference
on Cosmic_Rays hold in London (September 1965) is critically evaluated; at this
-oo,
confoonce.no new In fe in favor of the.theory of the metagalaciie origin of galactic,
~cosmic rap - unless the highest energies are concerned - were presented. It is
shown'that;studies of the.electron spectrum provide a means of verifying the
ICaM -1/21 UDCt 623.165

L ~ 31467,46
ACC - Mks,: AP6023130
hypothesis that a large part of cosmic rays (or more exactly,, their electron
component) ia generated during powrerful explosions of the galactic nucleus.
Any proofs refuting this hypothesis would serve as a strong argumnt in favor
of the local metagalactic theory of the origin of comic rays,, but no such
proofs have yet been presented; nevertheless,, this theory merits further
di,eausei6n. Orig. art. has: 5 formulas. [JPRS1
SUB C0194 03 SUEN DATEs none ORIG REF: 032 OTH REN 027
6rd 2/i

;_i. Lobed(w A.'! ji.:,~,.ILWL Ai'l
'Uhe rwllo
o~f Genel-al anki Appli-A, IIiy.Jc:,, April I)ij))
v- 69, no. 511'~)-5'
Cw;-.)j.c radlo ourco, L;alw~j, x ray cmj..-;tAon, 7 ray ar.LronorV
i a roview
article by 1-ccc,-It ob~;crvation 01, powerful x-ray
i . T."; deals 'aith the hit;bory of .:-ray oh-'Cc ithc olbzscl-,ra-
1*:.(')'m lie slin in IS)48 an(" 1"; Lh tht: obt!iincd In x-ray
and of the mietag-al"Ictic rq!ion~- Of Crj--..,;-I-c
li~;tr_-d --nd th-jir lumino.-~itiics given. 'Aic n:,.ture of the co~;.:iic x. rc;dla-
cII;;cw;,-.cd wrid the most important proccs:-,c:; which can Give ii_-e to rays are
*bcd (bre;iis-strahlung, characteristic radiation due to atomic 16-1-an . itu ions, cynchro-
tron ra(Iliation, Conipt-c.-. radiantion). Estimates of the relative c ont ribut, ions of the
c-'Ifferent neclianisms arc! given. lurther prospects and the required apparatus are
6.I.;cu:;scd in Uie concluc;ion. Orig. art. has: 2 figures and 5 formulas.
suit CODE: SUBM DATT: 00/ ORIG REP: OID/ GTH REEF- 024
Cord
Vl'
UDC: 523-85

G IM MG ) v 1 1-1 4
"On the Exclusion of the LongitWinal. ~hp-netlc Fleld from the flamiltoll Rinction,"
Zhur. Eksper. i Teoret. Fiz., 9, No.8, 1939
Ontics Lab. and Sci. Res. Inst. of Physics, Moscow 'Aftte 11.

GIKBUIIG~ V. L.
"On Quantum -Electrodynamics. I," Dold. Ml SISSR, 23, No.8, 1939.
"On Quantum Ilectrodynamics. IP, Dokl. AN SSSRI 23, No.9, 1939

Gillis-BURC) V. L I
1939.
"So= Contribution to Quantum Electrorlynamics. III," Dokl. P~N SSSR, 24, No.2,
Sci. Res. Inst. Physics, Moscow State U.

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GINSBURG) V. L,
"Wave Equation for a Particle with a Spin 1/2 and with Two Values of the Rest
Yass) H Zhur. EksDer. i Teoret. Fiz., 12, No.10, 1942
"On the Theorf of a Particle with a W"pin 3/2," ibid.
Physics Inst. im. Lebedev, AS USSR

a 11'If 00 IJ "k -L. '1A., Ad
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J-P I I- P,
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00 DZl.39C*U 550.30 : 551.594.6
09 On the ,*ra=Cnj)t1c effects influencing the radio-&-aye propaeation
00 in the atr-092haxe. W. Aaad. SOL. URSS, 35. 9, pp,,
09 r 270-M, 190 - The earth's anCmatic field elven rise to a double
go r retnation and rotation of he plans of polarization of radio ways* in
00 a the attiosphers. In evaluating these wreffectse it is ordinarily suff-
00 0; icient to calculate the change In refr. Index of the modlum contalning
00 j!
fr" eloctrons, which It brouebt about by the raignetic field. The paper
00 considers process" of a paramognstlo nature, dapen4lng -ori a cunst.
0 0 Me"tic =ment of the atoms and nolocules of gases in the atmosphere,
Considarati.
00 ons relating to the electronic Btayes of nolecul", atwa
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effect can be ernluntod. The influence or the paruringuetic procesees
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NU in how IL
-L.J;~ifiksbwl (J. PAYSICS. '00
U-S.S.R., 1943. 7.303-MOI.-The propext of He are explaincti
b= Is= &V no as thi COodrUntion of a Bose gas.
T rattu
of i
scaitcred to incident light is given. above
V x_ Iby the clanka jimeaule, for o"ADAry liquids. Fur fie 11 1 c
h
voloci y (a) of sound Waves Is givvn by a quadratic in ml, one
velocity Corresponds to tb* " M09OW " and UM to 1114 " &VIOMAJOUR " 1
souad. Three waveo we copsidwad. For orthowy liquids the
scathered light is a triplet. bet lot He It the ceatts.1 component,
Correa bled
doub PoIstlinbe to the " anomallown " waves, is dou . 7he inner
let a 0th too vrask and too close to be rowAved. From ZOO
I.An"u's equations for soand propagation In He It eap"Wons may
W be found for the intensity of the individual wattered doublets and
their Sum. CaLk. Wattering agrM with expCTjnwnt.
t Z-
AS&-ILA MITALLUSMAL LITINSTWE CLAISIPICATION
1.4alli ~ty 0MV oat aj,Lll;.t 414411 00 C-
T, C' --F; -ii;- a 4 A I V 1w .3
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0 w 1.,0 nil aidito
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1-f 4 1-1 1 1 1 11. -, -09
r
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h ZOO
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G1 liqmids Ats dtveloMf by IAdau (C. .4. is.
zoo
00
00 Z00
00 1 1. 1 L A atfitiLFLKAt kIrIMAIL41 C.Al%jf~(ATICk =00
O's

"C~i Wave Fquations for Particles with Variable ~'pio," Zhur. Lksper. i Teoret.
Fiz., 13, No.7-8, 1943

0 T 4
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a o :~
's o 0 * O 0 6 4 0 0 G * 0

0 0 0 0 a 0 0 0 06
'
1314h 1. 11 is it . " U 1, . 4 4, " .
r4 a
6 a- 1. A L It 1
I 1 .1-1 Ix LID it, I I .' . u
".
,

00 -00
00 -00
so -00
1;1~" d I= 111 Go kwA~ mom=.
- - -
-
-
' j 1*0

0 8! -.
.
L
11.4. .4=.
i
Sli, 1043 37
t
a
s
i
l
7
t
f
h
t
*0 s
m %a t
e
in" A a3
7
4
arloatton lit t
) a
pu
" o
and MID A
of 0 and ow 1) ljn" of Na
&wtumIng that the lutimi-
06 u, .
.
Mence Is due to doorwence and multiple scatteTinil of the un's
Th
b
ll
j
I
h

00 sation
e poesi
i
ty o( polar
n t
e aurttra spectrult, I% &jut
rayx~
4lisc
if IV,
06j zoo
0* .3
0
40

zoo

00 40
f
0 to noc"ad union Ittin lix
I go
0
0 0 0 0 9 9 0 9 0 * * 0 0 4 0 0 a 0 0 'a 41 0 a 0 0 0 0 0 0 6 0 9 0 0 0 0 0 0
: 0 0 0 0 0 0 0 o 0 al 0 * 0 0 0 0 * a a 4 o 0v 41 0 0 0 4 0 0 0 0 0 a 0 4 0 :
* 0 0

GIMBURG, V. L.
0 P01yarizatsii linly v spektre Gvecheni a nochnogo neba I v spektre i)olyarnykh siyaniy
(On the Polarization of the Lines In theySpectrum of Night Sky Luminescence and in the
Auroral Spectrum). Xcademiya Nauk SSSR. Doklady, 1943, V. 38, no. 9, p. 266-269.
AS262-S3663 v- 38

62

E E
G
NSURG) Va L,
"On Secondary Light Scattering in the Atmosphere and on Polavization Anomzlies
During Twilight, It Dokl. AN '311SR, 40, No.6, 1943

to 011TWAlln
FIRLD. WOW POLAIMS&TWO OW LWAIT 'rov.
ywoon ow Kxrttw" A"ll: 41-1 (PO IF"l
wra'snam" (w LIONT too Livim _11,1.
man: C40dwo. (campffs mr.jes (A-4-
104y) diT9r-&j q6. A, rimss. poh I-
194.1- V"I. 9.Nm Pq 370 a Mill
Fri.. I'Mi 0. 4. in, jr.4 16,
looll Fri, I-pof, ij, I. Iv. A In

GINSBURG) V. L
"On the Scattering of Light In Liqiiids.1" Dokl. AN ,"SER, 42, flo.4, 1943
P.N.Lebedev Physics Inst... AS, USSR

530,145,1 2145
AV
Oil ilia
theory or (N-XcI11 n 0
VALlIcIrg" lys. USSR, 9, 1,

-5 1944.-A deve orinicni of the relativi5lic
p. 33 1
p
theory of the rarticIc (112, 3/2). Tile cro%s-Aection for
tho scattering or light (or mcsons). on the magntlic
(ortjuPAl-tnaGiicllc) moment or5ucha particle increascs
at finit with ilia vicrgy as in tile unial theory but K,-
comci c9listant forpholor( energies hi,>>( 'in ?rj)r2
h
d
M
T

w
ere nt an
-mmses.
oi~ RTV B rvit
hus, tho
Introduction of bliher spin otates leads to the cutting-
off or the crovi-section for scattering and to the
possibility of a tion-contradictory, consideration of the
Interaction of the heavy parlicle's moment Olt ilia
radiation and the nicson (laid. The thcory or (lit
particle (1, 2) Is ario-JRclopcil and this, together
with the above theory, mukes It possible to confldct
the excited states oftheproton-rewrOM and the mason
lit a relativistic rorm, L, 31 (11

v
[an' 'or
on the wavo equall r a e" "lillyrfable $Pill,
U 52-53, 194-- By Lill (1, particla
is meant one which call cnist III statci with stilm
I and j and with diMmil valluci or ilia rest mass.
*rhe miallvistic wave equations ror such a particle,
recently proposed by Gimburg, Lira said to split up
Ir, by mms of a certain transromintion or the wave
functions, they reduce to a system of equations for
a parlDcle with the Spin I and for a particle with five
mpin J, Which am lndctviidcnt of each other. It Is
shown that the equittlons for a (0, 1) particle and
for a (1, 1) particle always split 13P In ilia absence or
a field and also In the case of a certain type of inter-
action with an electromagnetic field. The equations
rot a (1, 2) particle are also separable fit the absence
ofa fldd, but this Is not the case for a particle.
L. S. 0.
IiF~ -SS3*-
_j

G11,TBURC, V. t.
the I---
2-
relic-ni-math, The IrlechallkIll of is III,--
MILO M,;:K of rxptl .data (oil tile 10. (If lolls and mols
cc And tile fre :F
llency f)f IWtIN'rt", dectrons'
MIS. as Well JLt 'J1 the rffL"t uf the e.
17,231'etic field' aral .11

-
V Ni

e
RIM -27
N
ml MQ
12 4

410
c 1 01 1 U 0 41 42 43 CO AV n
LU!
IT
j i~;
It:
it
Ise j
90.
go
WW
00
00-
full parlool me "n"lle) to. $*pal sip IQ r"'M-0-h"t
0 0";
00
"141.6 -6; f",.;v Ali of
w -W -
0 0, co
00 0 0 00 00 00 ~ I

0s 11" Aboorsdom of *a& Watifts Ww tb*
somilloof d ogkwm is As
wit-W. PAll.l. VASJt.,
;,It- is) 15(,) -Thr
tion 4;1 rAl., ave., In %IW onlo.111111C ~RAIAI 1 -40' t~-
deterillille tile Olt-ctive slunitAr.li kollim'.111 III .-nn-
1A its irilptlov. on the ollier hand. it i~ lx,-~ibll will,
OW Wit 1A the UIUAI flictill.1 tit kinetic 41JUAti-Ill I--
evaluate the numl,er J olb,lon, i-littlo- J- shr
PFULr.% .11 AIj,,,q)IJ4pO 14 ?A(IjO IAAVC'.%. ISAlth On'
flectotmitt* "Ah,km. with the rn.,Ipt:ul,-% and Ilit-ii
U411.641, Willi tile 1'41% can Ile thu, al'tilal"I
The cn-l M~tumrl for the Lttew ull,kF -n.
diti,At% pmvAiling in tht- ndto~plwrs- I, .0.,ut A
mill",ri tirn- lArgvr thazi hor cc4laxv,n. mah thr
Int)IMIllea III this talline%1,93 the C4111-tillaIP-0
.it n-sus And mAecule, in tile Wo-1.1WIV. A. drlI%t1I
fruill 14,11.0 IIIcLjalrVllWnt~. 1.

o -
8 -
W-
~
"
40-
t??
F
;F
;
f

,A
r U T I V x T
A
tj
S
A
.
J. J
YI. (
Superconductors with rumnal
--Th-
tic&l
W f
UA)
.
c
.
nE
ng
*
I
t
l
I
.
n
curren
ien1p. rsdicuts should show & norma
this 6 countetacted by a suPercon-
d
00 1 1 uctom
6oltop cm

0*
j ducting Current Jailing ervials the d. of
f
d t
d .00

0
A
o
at
ri
the resulting CurfOlt I
zero wW the thertfull current should ~Idttectxblc the

00 r1manctic rmldl produced. Also In Xv . Them]. ky$.
(U. S. S. R.) 14, 177-83. It. Rathmmum
jr
00
4
00
9
00 00
0013 zoo

06,

ANAL! lee

MOO

iboo
1-200

A - I L A 111T ALLMICAL LITIMATLIII CLASWIFICATION Mee
flow "NOT
we*
At a.* 4#1
U III AVA
0
ire
11, Z!, to OF;a 91119 Reg" l IV
ma I NO It I v im i a a 3 1
v

N 0 0-0-00 0

GINSBURG, V. L.
"Optical Method forthe Investigation of Stressesp" Zhur. Tekh. Fiz., 14,
No.3, 19/d,
Physical Instj im. Lebedev, AS USSR

GT~,1'7EUIG lf.
$taw 0
f the ti )r
IM yo%up'.',~nfluc
t) ft ara diqcu&gcd in the light oftivity 4nd rL litl"ON't Off
the 1,t, jelltaillostj ;1R relating
in ve-stg-ttlOns-N. A. (,_xfx.ritI and') Iworcli"al

0 900 0 o o & 00 0 0 0 oj'6`76--#-v-W7w.-7W--
6 00 i 4-6 i a
0 00 0 0 0 0 00 0 0 0 all*-
10 11 uI) V4 is 14 it it tt n a ZA Is ;A! 4 4T Q 43 at 13
)9;1011 1213 U13 ALY lap
A I C a -L-1
1. 7 4 1
bwmelectria V. thniburg
'rhmh-ti
cal. It t Prevence of a temp. gruilent currvitt in a aujim-
conductor must inenw; in an WtrojAc supractmWurtor, htjwrvvr, this
g, rftnt io comp"mied by the suptsounAucting current and henv i* not
ldlucteckd. In suvinwonductbut S"stak theIrmulting, c.d. ia not tera and -tha .09
th"tw(K-ItOrit: c1l)-tv"t es" b0 Vbwrvr4 by HwAns of tht, toagjwliv field due to =00
it.-S. A.
jG#
roe
00
00
J Z
to hoe
S S A AITALLUPCKAL WINATU4E CLAWFKATION P-90,
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e: I
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Ast Prowl. Arad.
crit. ifiscuo-j,
sian 4A rittest experimental data and their lnt"Mt&tWn (c(. Ven.
kateswarau *I at., A., INJI, 1. 2M). R. C. M. =0 0
Go 4 0
J 0
0
0 'a
zoo
'00
A I s A atIALLUNGKAL LITINAIL411 CLASSWKATICH t I a 0
1j. 11,
lit 104451 .10 on. dot I,
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AI f-- 11 2- It A JL-
00 A -
VU Ids 11111 1111141 41 QU
L-A, " IL
00 Ou the Oyromaxnefic and thletran-bortis Ysporinjouts oil 6 up r.ac.u.aducto.jri7-
V. (imAl'of (Mor. Ek-j-, T-r,l- 11111. 14, ill), :Q6 3'.".11. ill)
00
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000
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A a S L A NITALLUPGOCAL UTUAFATUNE CLASSIPICAMN
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0 Ce 0 0 0 0 0 0 0 0 0 o 0 0 wo o o o 0 0 0 o f 0 4 0 0
0
0
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.04
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'00
=00
'00
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too
600
goo
400
Soo
Ago
00
'00

0,
I A
00
00
*0
o*J
go
W-W-W
00 0
16 " -1
ly 11 14 It lit I/ It x it "'I r .
-M m 0C w
1w V. L.
LIwd,v Pbyl.
Sri. U.R.S.S., Mr. Phys. 1). 174-100945)(in
h,~wi~q
cf. C.A. 38, 61491.-A tcvkw of t
A 1 5 - I I AWALLLM.KAL UTINAILIll CLASSWICATIOP
S. M
A
b u W& AT W3 It v-q r
ip "11,110(vit Ott On 01tiff tic
0 0 0 a 0 0 0 0 0 0 a 0 0 0 : :
16 0 0 0 0 0 * 0 0 000 00
:
I I
9 11 u 11 It is 4 it x p IV it u 11
,
I f 1 119 J.. A

so
1-00
Os
-*4
-00
.06
see
=04
drad.

RuMill"); roe
,
4. 'rhon

. ,!,Coo

:see

El -Ld-
woo
14,
it w 0
kla A 1 !14
: : N 0 0 0 0 0 0 0 4 0 0 0 0 0 0 0 4
Is0 go * 0 * 0 * 0004 o 0 04

GiNTSBURG V.
'CN TH k, 3-URFACI ENERGY MID THL BIEHAVIOUR OF S1,MPACONDUCTORS OF SMALL D1*
MVISITHR. V"'GINSBURG (J. PHYSICS N.S.S.P.), 1945, 9, OT, -30,51-311 )
(In SnI7,11 ) 1hooretical. "Ile depth of penetration of a ma!~notlc fleld
Into ft supraconductor lo discussed, and tho offoct of-thn surract) onoryy
at the boundary between a supraconductor and a vacuum or a mobal In the
normal state is stressed. It Is pointed out that bad arrooment between the
previous theories and the measured values of' the critical fields for supra-
conduction films, and madsive specimens is duo to norlect of the surface-
energy faebor. Thq reikation betviecn t e critical field and Lhe thickness
of the film is developed taking this factor into account, and gair agroomen
with experiment is obtained. GVR.
S9:.S LAMETA LLUnGICAL LITERATURE CLASSIF.ICATION

'iWWWWWwo go a too 00 906 sofl* Soo:!
0000*009*0000000000 -0 61000099900006#06:6
6311 a 1 4 1 4 1 a , t; 11 11 11 It 11 1& fl U 21 n a 34 is I? "I N X) V U Ij u is h 3; a )o Q .1 Q 43 40 a J!
A I -L- ri--L-j A--a-L-L -L-1-11 F Q I., A A --U- V1, I Z- so to U t
*0 4f
E: it 1 14, 1
WC7
00
-00
PFFV.-di"wx u. PAY-,$ =00
The intensity.
U.4.S.R., 1943.
0:0: L 9dMXjM emitted when
cr.
bisf AsIffism into snoth
do p""'a no" =0 0
__ injo a --tol, we cak- a, INIMIU0115 Of the
in The Wiation
dl.Vftic -10-41' 'A C'OdwtMta 01 UN two MMiL
is not cvisected with a cb&W Of dw vWodty of the electron. 10
plays an jullportaut tale in the luminewzme at the anodes of vac. X-
H. R. C.
ray and other electrunir tub-
i see
ZOO
Use
.)WP too
As ujs~
AVM %LA .11ALLUCrl[AL LITIOATURt CLAMPKATICA I - i
moo
W
It I .... .
(11111 Vol $in Itu K(tff It it I An I I W 1 -1 3 1
0 oto 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0
IT! !~-o !
T4 oooooiooo 0000 0 60*64 0:0 o4lie"o of* too* Soo o Go. ..:I~q

Chakistry Dielootrio Constants
"The Dielectric Properties of Cr7stals of Seignetto-.
6196trio lub9tmaw-and -of Barium Titanate)" V. Girii-.
tlwgt IMAtitut -0 of Physics Imeni P. N. Lebedsi;_A-oA-
aq of Sclenose of the UM) .10 pp
*Zhur 13ceper I Tear Fiz" Vol XV) 739-49
Reviev ofprevious work on the behavior of the di-
eleotrio-locustant aroand the Curie point. Artiole Is
reprinted-in the Journal of Physics of the USMI. Vol
ZY 107-15
31T3

Superconductivity
Moskva, I7a-vo Akademit nauk SSSR, 19116. 204 p.
(Akademlia nauk Soiuza SSR. Hauchno-popullarnala serlia)
(49-58139)
qC611.G5

LillJZLJUR'G2 V. L.
"'Theory of the Propagation of Radiowaves in the Ionospnei-ell. Uspekhi Fiz Nauk,
No 2-3. 19h6 (155-201).
(Meteorologiya i Gidrologiya, No 6 Nov/Dec 1947)
SO: U-3218, 3 Apr 1953

The theorf 6f wited rj_t;'-t rt-h~q 4f d nl~nrmv ".Irfl
I'vady-li-tT74-st., Ami
N. fxhcd.-. J. No. 2,
3X1uIVXA -11w timal
effmti- Crfi,% f.r th, wal i-ing 4A 11,-
11y itattletes l1rat intwa-,cs with cm ray: t!li,, cm-
tratticte. the exiAl. fludiumi. TW4 i, dq~- to iji~, UIC', ill it t I.,
watiott of thQ V-1d (A (fie 111.1vurtic "t. (pla"Isi"guctic
t,ltjiuv%it of the vattering putick tilt the motitin tif this
litoment h~vt 1w-c-4 iivCt,,vt!A, Avvnimthit. ter Ow prol;,t-t
fir.14 fil-thi, qTla"t-am r M~i'" ;,wk tit Ote twet-ity M
flig% Omit'. (hi 11troton alld the licittrall tilt L-Xcitvif
*tit it Slihl Ili :J/2 IW flirt %VT. 11A (tit- C:tA' .11 ill', tilt' M
',he l"."timptiZin (A the f...1istelmr C4 'Utes %1 ith it -phl (if
etc., xri~cs_ 11, thi., itive;tigatiall the reLitivi"tic Ifivory of
tit" INW11.1" It- 4-ilt'.1111C Of Wlig M .3 Q110 With A 11ill of, I
mid M-A mV, Vmit tit a A!Aiv with 1,;,l V. mul n~t
Imli'l Fis'l. J~, it"T, j It i, ~hwwll tji.tt tho rMitmi
for thr of light (44 11jr,titis) ml tilt fit guctic
((Jll,%qbh;kg;1c1i0 flivillefit tit wcjs I 1),irticte M fird iji-rcjv~3
"ith tht, elwlyy %.,; 'tit tit(, 11'"'d thplity, hill U411 r,)r imititis
litr4j".4 Pp > (I($-fj - jullikIl R N-cmicq comt. (ill, ~ rt-wif
11w tl,~Iwy IFtetid'. twing Tllit7;. the 111tru.
~
whith Is ackillutte to av%wotit
fur the P.-q?cr fktii Af that J*wtict~. i1wmcnit. Itudi to (fie
clitting nq of t1w CjTYi3 S(-',tinu fix Atilt to the
militrilitr of the intm, COO of the h(-AVY lKirtirle's mmm-lit
Ivith 11i'm radiatiort'attil tn--%Ii flvId. Tl-.c r0atkistic thkory
of Ti juirtichi b-41"111g, in fint. jitilti,., -~A 511fil of lillity and im-.13
in[ mul in allotheirstatil it ~Jlitj (if g arill Imm, ill. tio [tho been
d"VtOred, Tilt x;iWtlu;! of 110if h,, t1ii, 111futef 'If CL
bas stot t%.1,A,

818. 0.14 THE DIELECTRIC PROPERTI" OF FERROKLECTRIC citysl-ALS
AND BARIUM TITANATE.-V. U.S.S.R., 10, No. 2.107
, _ V. Phys"
19"). The pgolvortim of forroW~i a and of barium titanate am di"il;;i
in Wasoction Witli tho tkarmodyn4vanal com"oration of a phase trasisition from a
IRM-Pyoce to A-pyruslectrical crystal. Experimeatal data show that
Iransitloo Is fWW C a is really Of the continuous type. the value of a
tending to inlially by the Curie point from either side of this point.
IWOW tke transition poot Is T" tlis behaviour of ferroelectric crystals is
complicated. as 04y split in as the dimensions of which an determined by
ibis coaditiow A ah- m'-Ira-- It Is a physical peculiarity of the"
--hounces the' reversal of the d 9.YipoWitation may be attained In com.
parstively weak 4" which do not ",,,ad . - volt 'cm Thecharacter.
istic Whiting into domalas at a lives temperature and the j~;;ical properties of
rroolectric crystals are determined by the Asp* of the specimen and the conditions
on its boundaries. The problem of saturation, however, remains ambiguous. The
large value for o;'-, lattims of Un pwavoltils type accoauto for the presence of a sown
value of Bmu*s Intlemy. Cs. a cwtais " loosonoss " of the lattice. which increases
with increasing ireight of the metal prodod" the titaute. wW Is especially great
in the cam of am. thut costributing to the 'ce Of pyTo-nwdifi-tim. Ths
proponin of symmetry, of IW latuce adods =;XbW olpyro-andpieso-viectric
ility
pbenomovia. In HaTiOs. the Curie poWt Is elmakaneously the transition pKAnt of a
non-piezoelectric into a piuoeloctric oUte. WM such transition them should also
occur orientatioral twinning rendering the whole crystal non=' soeloctric, This is
known to happen at 573*Q when the transition to "Marts place, its modulus
=swfo. but unfortunately the phase transition in quartz is of the first type in
# changes by jump Imt dose net po~ a sharp temperature dependence.
CoWing barium titanato is the &bssoce of an electric ikkl and external stress sbr,--14
lead to a non-piesnelectric state. bemuse of the occurrence of orientationat twinning.

GINSBURG) V, 1'.
"On Nuclear Scattering of ?4esotronsp I' Zhur. Fiz., 10, NO.3, 1946
Lebedev Phys. Inst., AS USSR

14 111)) go bla hill 190041 Q&I map*
-
A A lk
004
00
*02
00
Sy 01
small
Phy'. (U.S.S'Rj
1'eackf6dw dWb lish
of The
"JUM
can't Id Jj-u
uto a julm.
4 11111rcundua-- Td.-- y
state are or a' Ik vacuum ("Mr a nm
the IftrIJI'l
Tile omit
diff., in Ihc."j'j" age
'"'11Y Of the nonnal and
ucti,4
j
IKv"I% 1c) be exenti&l f, the IFUjxrc 11
'd th~ too
""Pt" On (he dntructlm4cOffect d.
Magnetic ficid. 61
goo
Arild
H.
-I L A ANTALLURCKAL WINATIMIC CLASWKATICII
via- $1.18111. see
0 j-0--v j L WOO
I 11A
cr IV 0 a 11 01 An A I afW .1 a, III
It a fil V
u X AV 00 LSJ; I
* 000 a
0 0 0 0 flee 0
K-~;E
ig
ME

W, -44SQU
V, Landau L
~-,a and j2; M
c*'s I
P) 1-1 Af Akad. Nauk -SSSR 8.
1;()
lpi,;~[ lfosj~ov (,o, I 'ni% V 77 1 42
6, 222, 7. 104. IS 3
ILews NO.

A
A
'-~2352 5H.% F5~ 5W
on 5 r2 0
miar n& n ip t4 dl I M
-99 - S_ IT
S:~K2~
L. CA Acad Scl. UR o. 6T40-90 (1946).-
sun*,.q cotona is
h7Fr-opagation or rvidio-waves in the
,d. and it is shown IhIlit the study of solar radiation
"arnine
in the radio-spectnim gives a means for mcertaining the
temperature of the corona. Recent experimentnt rcsullt
and deductions from these [Abslr. 2112, 2861 (1945).
2450 (1946)l am criticized.
N- Wxdw

Jan 1947
Superacnductivity
Xlectremagnetism
"On the Nonlinearity or 11sotrooiagnetic Processes
i.n Superconductors," V. Ginsburg, Institute of
Physics lawl P' N. Tabedev, Acadmy of Sciences
Of the UMr'-1
Ojournal of Physics" Vol xr., No 1
Ageneral discussion is given of the relationship
bet,veen the number of electrons n and velocity v
In-& supercenductor andL of the equation for the
penetration depth d in terms of n,v,o.,e,, and in.
26

V. L.
USM/PjMo Uaves - Absorption Feb 1947
Radio waves - propaption SEF
"On the Maission of Microradio Waves and Their
Absorption In the Air," V. L. Ginsburg, 18 pp
"Izv Ak Nauk Fiz.". Vol XI, No 2
.knalysis of new methods for generating microradio
maves of less than 1-ox vave-length, and discussim
of the absorption of microradio waves in air.
?,I 1IT11h
ftilk

Beftaylar of terrointiqatic aubstances M me vicinity of tho
In,-
Php'o k4m t
-
4 Mac
1119
",
jeard
17 Kid -u
7 ,
u
.
.
.
e
P
(
selle traiiMtiosi near the curit pulut 0 Is V
it
pl~u:jr transition of the 2nd kind (I.e. without latent beat and
with a dkeotillnuum change of the beat capacity), It can be
t ren led lit a nulogy in t lie prev ious treat men t of the Beignetto.
elec. tralikitiou (cf. C.A. 40, 5WRI). rhis treatment I, it"
froin the arbitrary a-mumptiumn underlyinir the theory of
Wr+m Front thc coudition of will. of the thermodynAmir
poirntial, file Spot) I Lill ellui magnetization Af. lit F 4 0
(

14 At.' wherr, a and 0 art 7
fulictioull of (lit! litc.-sure p alld of T; a'$ - (()a/ZtT)T - 0;
f); and dAf.%1dT - ",?/0*. In the presence of a
firld If - 2ajV + 20AP. (6,111011)r - 11(2~ + 43031"),
and the Initial nu-%ceptibility X, nmr the Citric point x
1 /241'1 ( 7' -:- 0) or x - 1/1 pf(0 - 7), lit 7' > 0 or T < S.
resp., i.e. tit the saine IT - 6 1. the lat"ptibility In the
ferrormagnetle range is hall that In the pararnagnetic range.
For the beat capacity Cw (at con,4t. Af) at 7' > 6, CmdT
'
Ta'd(Al") w (r12)1
d(l1x)1dTjd(Aft), Find, in the -.icinhy
of the Curit poEnt in a weak field (both at T > 0 and T < 0)
CWT - T
C
th
;d(M')
t
t
W
i
h
hi
on
.
a
rary
o
e
e
ss t
eory, t
s
forinifla Is vnlid only lit the vicinity of 0; futher from 0,
the magnitude as' depencls on T, Ctinqt(Ittently, a, cat
be dod. only front the SJC)t)C of I /x In clo" Vicillity 0.
N. Thon
IhSf. ;#P. P TV - L A V t?

Ituols:mwip ;wuxlui A-mliavi r ai hutp-jo~xfr amop;uu-n suop
0--lqj -al ')UPLIUAM VIAIVILN11 ;UPIAM; cnl 1JU17
Quivs *qj ;o u-)i li Yo nLm. lunj ~Xwlj,
P3j)UVxl-W-3 Dq Attu .j(jv--Lhaiui ait-tibl; v j)
put, jruo&~qjio axe -,,f I's ,q1 pute
I + f f- 1 00
pw,!v,iqo Gi q.w.).so_4
irl . ,Q.
.
W10j al u2
. 13 jo slqx
imm.roi.al, aq~ (joclvmba puooo~.~ ,
31~UIIJOA
J,j) J.Xtno tim If .11-
In
w,,i if qw, 1 j.-
z 3, 0 v > 0 '--;)1 UUT PAiOO

jo fzscm ,q i
I N1
.

QITJ 10 qLlovl"jo-z .ml)(i-ij -iiwiDarij xrj-vl~ I ~)Cj o1 pzwnagi? A
-)Ur)v-l)o3 ruxialurill XM, v P-cm,
Pur?
ED
.;)2,9ns; ci uoiivnr,;) -,Aorlo; atil jrP
"IV
0141 DIOU31) (f,-- A I.T I.->-] -,I III su-.11 I UV.YSUO:) J0
-)31!1 - -d, 3qi -tiq A
-.iw ; v. lo n ~iuaaoduio- . am s. rm
:bqi ji-on otp ';)jdwtrc~) isitj r vV (1)
sajqTmjv,%. imonunum) ~ij [).~quzy-)p an, Mot=
JO C;3alZ t3p IrUJOJUl OtJ4

-
-
3ly
m alop
lul
l
A
in
'
.)J351
f-ijqrijrA
j
q q
4
p
;)qj,

30 V11-D.1j, ap .Jrwal IT 1.. 01 1)11?q ;)(I ~vul :)Jai-.U;)TTI la
PR
--TV'Ll Dql PUt '%'Tiol l0tl 11 ;)A CV
"
r
)
~
U
li
)
.
~
.
1~1
A!
7
Lliartilpio
7

vidi.;
JO )[jj ',~
_)jjf, Qj!jkjvUj
-
'
u V1 t 1
(1i-60 LU
,q
C5
Q43 UO -llrlf~l Pu- 'A -~qSUMVi~ F-

repre-suit-ation ot, tile
authors at*je-rt the
q3cratur L, am.-I nnake t he ~TTr,-:t'()tjS aS,4(-.f
,quare UnCtioll ')I thr,
(o Yi M
C;' 'D' (4). This oversight, however, hard"), affects tnt- argu-
Ments, of the di~!;cuss'on.i -mice the equanw~ ~1~ Ld IM-4
t4 infinitely many -alues of the spill, the author", pO-Stl 1.1cf,
S, (Af.1 AfadO. - k
ladditional equanon J') + 1) E,
constz-lnt. In dhe Particle's rest -system thc! t- It k" r 0
P-j,~k) is stiown to hold for,a lixed , I ue of
Oic angular raomenturn. The pv5,-sible spin valwea am ;h ,.1.
o~w
LritegCrS I whicti , ritify (6) aud the coaditio~ (Cf-11 (3)
Consequently, jfz i-must be an inregrr. For~a vM &. r-h-
CZ Mnists. if JQ-5, a-finite aq,~~:erbi,
additional -asolutions. may he fo-and,
(11) The foregoing dkcvmiori may be P,~asidcrably Szerll-
GV er.-dimd by using the rpsidmi (31 1. D4, ;'-';eAfand and M. A.
Neumark on the vr6wry (infwiri,- dimersiondl)
tiorm of the Lorentz qmup. L-These rc-%A-,~,
have cnea.,V
been publislied [Acad. S6. LSSR-
(1946), 17.ve-stiy~.i jULad. INAul, SSSR~ SOX,. Mat. I 1 4, 2-
504 (1947). Ehe5e Rev. S. 152, 9. 4951 C X. alsQ I
T
Ciandna, Proc. 1?-o,;, Soc. London. Ser. A. 189.
(1947); V. Bargnmvri, Anm of Nlath- (2) 48, 508-64")
thc&e Rev- 9, 132, 133, ] 'nie xro.-ducible unkary :-rprt-tenra-
Lions aze charac4r~--MC4 bV trIC -luatioll.5
L ~ jo m, ~ M,,;
jvj,r,cjj 11iji(I for cve~r-,, vectorw ,he rept-L-sent- 'pacn.
Th't Operawa, Af,, are the COr"bpond-trig

CresOw of meeptrvas and "iftn" in comk roys.
GuIlT ts. Asir. plip(t 11fort'l. Fit. 17, M 4(11047);
AIX Ityan. el s1.. C.A. 41, IL%krA.--A mul'arkill of the
prothielkwe tit sne"ruts. and itidicutr% th.&I I lwy are
gvurralcd by the adiur uvistril c-suilmment- (if cu,mic riv-
The no ,of '%Ufs- is al%o nearly the no. of act t of creat ion of
killit"l."I. unil F
N. Let b te. C,/, q.

eratom of Ow Lorenuz grour.); tl-,.&r precise form depehd~,,,
on the paxticuLx- rrflun6on wh-Ch haslven Chosen,
(T in mm-1Z of vecter or vinor quantities. In (7a). a may be~
any real aumbet-, j itti irkugraj 'or halHottgral (includirlj~~
A;-
j - 0). The equat ino (31)) rranutims valid; t ChaI74Cterizes thel:
irredu6bie of the rotation gmup WWCYI~1.,~,~~~:~
-Accur. Two dif1crr.-tr a4 li,oe 1eadtoinN_tdv.Wentrepre,,:
w.nmborv.s, For the case disc=mi above, cc-0. [Reviewer
T"
n rA C.. ~It~rr C\i~~r Al-so rcfmc5entatiorm for
which ummoz in the form (7a).] If the equ~4.~
600's ~tridl tied, arm obtains, in the rmt hystelm'
11 +1 Z- ~J. Here 5 i's parsitive and intLvrzl;:
or hau uat-qb -,0 ~dlfvg as I (or j) is integral or hwlft
T
iii, ~st of a- and j-values, an-d--
of spin value3 -.xppeat*.
Mitt- af,~mng
pio~,&_,xbte variants of the equatima.
(1) Arid dit, ko thor-, meabon a 5trious difficWlry of jae
theiwv p-opo.;iwIl .\~. !,.h,,Nvu by Fierz and Pauli [Proc. Roy
t -N 1'3, 211-232 (1939); thc5e Rev. 1.
Ch'O Ciectmmagnetic fiel-I Cannot,
be de~,cribcd b,, rcp1,Zn_TT/rx;_UiT_tJii Operator,
[1~ (ie h, )A.. (A. the comwrients of the four-vu-Ccor,
potrantial) if the of the particle is grzatex than une.
Additional wave t inimt hm introduccd, whioli vaniah
in t-he abmzoce of chc eivcu-omaF Si
,netic field. A milar diffi
Culty here, and
~hc molon haw not, yet surcetded
in urrating the intr-tactiou the clc=magnetic field in i
-1 "Xatisfactor V Bargrinanx (11rincccon, N.
Y

in Fj:!vehrvki A
1307. Theory of Wsotrons and Nuclear f*ovco. by V. L._G &burg.
buk ji, No. 2. April 1947. 36 v. I In 4uns"J'a"I
This article is divided into four immin sections; Introduction. the wave oquationx for
mesotrons. nuclear form, md difficulties which arise from the present theories.
Utvier the section m wave equations for memotrons. the author discusses the relation
of sesotrons to slectromognstic pol*s.

GINSBUROj V. L.
"Solar and Galactic Radium Hadiationt 11 Usp. Fiz. Nauk, 32, No.1, 1947

GINZBURG, V. L. ?A 34T88

Oil (be Use of Ollorpikov's Effect for Ilia pro~ftgft%
"idla ((;. If. AMC
_._ It -1 1947, 1 56. No. J.
ME. A71M
pp. 153-1