SCIENTIFIC ABSTRACT GRIGORYAN, S.S. - GRIGORYAN, V.A.

• Document Type: CREST
• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R000516730009-0
• Release Decision: RIF
• Original Classification: S
• Document Page Count: 100
• Document Creation Date: January 3, 2017
• Document Release Date: July 27, 2000
• Sequence Number: 9
• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT


GINZBURG, V.L.,, FAYN, V.M~ Ph - 2080
T IT IIE On the Quantum Ilffects occurring on Interactions of Electrons with High
Frequency Fields in Resonant Cavities (0 kvantovykh effektakh pri
vvalmocleystvii elektronov c vysokochastochnymi polyami v polykh
rezonatorakh),
P-RIODICAL Zhurnal. Eksperimental Inoi i Teoret. Fiziki, 1957, Vol 32, Nr 1,
pp 162-164 (U.S.S.R.)
Received 3/1957 Reviewed 4/1957
ABSTRACT The authors invi-53tigated the following problem in classical mannert At the
moment A = 0 with the kinetic energy Ko - mv4 2 a non-relativistical elec-
o/
tron enters the resonator and leaves it at the moment. t with the
energy Kr. ~ mv11/2. For reasons of simplicity the electric field E in the
resonator on th! path of the electron is assumed to be homogeneous and
parallel to the velocity of the electron (such a case is absolutely real).
If E = El costit + (Eg + E,) sincit applies I 'dv/dt) = eE and vy =
sintit + (~a + E )(1 - coscj311 is obtained. Here El and
v
'
+ (e/mw) [El
.
o
= Za = 0 and Q = ZI = V?d4 are as-
E2 denote chance quantities and il
sumed to apply. d denotes the path to be covered by the electron (thick-
ness of the resonator) and T' denotes the mean square of the fluctuation-
voltage, The averaging is carried out over the corresponding assemblies
of the identical systems. The field in the resonator is assumed to influ-
ence the movement of the electrons only to a small extent so that the
terms of the order of magnitude e33 may be taken to be sufficient. Under
aV2 [(sin(cj7-/2)/(,jY/2)] a applies. For
e
t
ances
these circums
Card 1/2
On the Quantum 'Effects occurring on Interactiom of Ele PA - 2080
Frequency Field, ctrons with High
-3 in Resonant Cavities.
the dispersion of vel.ocity then Tlv_~T4 TLr-r7~M-4v-4 applies. if wr-
'lard 1/-3

S/0 6 1/000! / !2/013/)43
in i,he tneory Of c0z~lrlc- 1'ay origin AURX11cri ntl C --
Some quesLlOns . disintegration Of heaLvy,
a secondary one. due TO~.he fiu), of tie'i'li
the observed proton flu)' 15 ajo of proton "i C, - ml C rAy -
The magnituje of the I - I-- -neir ltf~-:
1e. i -rees with th - I r,e-
20,ag - halo bounn-al. Ga
WnIch eq,jal to 15 - ~r 'he
~,lane to the
~he galactic ed tha' f C:-- z T.
near 4- ol,e I'. is ~,r`e5um t-~r"t
gene 1rie r e f it or force Liff-
lot 4 L.
-n a la -VI e.
a knO, .1 --
.j., .,,-,:Iere ou, h a;
-ti - . -
in can 90
rar,""aie=/Sec
of
10 rju~'Iear dUsorptlon
C, Vs. t - CO i
he V~
'ne Gala)(Y - V fi
e Of
fr- 10 their
t, o une
rei I" e ng rle rg I e 5
r; 1
r Ia In rljejear
f
em
v-Lng !AIE' em Of f 'e.
lea L~Otl.t
a er r-ne con', c-leri"W. C J
. -, .1 - 111 f. ...
wh -ge-
i
effp-
-rA ra L.. mc
,e,r the ~Xkt: r i. 9 n
of
n,
ria-f-'Y
e mo
i"'ard 2/)

ACCESSION NA: AT3012749 S/2831/60/000/002/0013/0018
AUTHORS# Gershmano S. 9-Y Gintburg, V. L.
TITLE: Formation of ionospheric inhomogeneities
SOURCE: AN SSSR. Mezhduvedomst. komit. po prov. mezhdunarodn.
geofizich. goda. 5 razdal program. MGG: Ionooferao Sbo statey, no.
2, 1960, 13-18
TOPIC TAGS: ionosphere,, ionospheric inhomogeneities, F layer, E
layer, ionization wind, plasma velocity, ionization wind velocity,
altitude variation-of ionosphere
ABSTRACT: Some of tbe.bypoibeses recently advanced to explain the-
mechanism wbereby inbomogeneities are produced'in the F layer-are.
discussed, with emphasis on the inhomogeneities that cause flicker
of radio stars and diffuse reflection from the F layer.-The authors
analyze the conditions which determine the motion of-an ionized gas
Card 1/3

ACCESSION NR: AT3012749.-
component in the ionosphere, since a clarification of this question
can serve as a premise for the construction of a theory of "ioniza-
tion winds" and f~rmationof inhomogeneities in the P layer. It is'
concluded from various estimates of the possible plasma and wind
velocities and the resultant variations of the electric and mag-
netic fields in the ionosphere that the formation and motion of in-
homogeneities of ionization in the P-layer is not a hydrodynamic
problem but must be solved with allowance for the earth's magnetic
field, the electric,field, and the fact that the gas as a whole
does not move with the same speed as its-ionized component. The
nature of the ionospheric winds and*ionospheric inhomogeneities must
be ascertained by clarifying the character of the distribution of
the electric field and the velocity on scales that are comparable,
with the dimensions of the earth's sphere. The particular partial
problems still to be considered-aret the transport of the electric
field in the F layer from the diurnal region and the related circu-
lation in the F layer, the passage of.different types of low fre-
Card 2/3

ACCESSION NR& AT3012749
quency waves from the Elayer into the F layer (capable of becoming
propagated in a weakly ionized gas), the influence of the earth's
magnetic field, and the inhomogeneity of the atmosphere with alti-
tude. Orig. art. hast.12 formulas.
ASSOCIATIONs None
SUBIMITTEDs 00 DATE ACO: 220ct63 ENCLt .00
SUB CODE: AS, Al NO REF SOVS. 005 OTHER: 006
Card 3/3

AUTHOR:
TITLE:
PERIODICAL:
84o62
S/181/60/002/009/003/036
B004/BO56
Ginzburg, V. L._
Some Remarks on Phase Transitions of Second Kind and the
Microscopic Theory of Seignettoelectrics 7A
Fizika tverdogo tela, 1960, Vol. 2, No. 9, pp. 2031-2043
TEXT: The author discusses the problem as to whether transitions of second
kind have the same character in superconductors, liquid helium, ferro-
magnetics, and seignettoelectrics, and differ from one another only by the
value of one parameter. Corresponding to the theory of phase transitions
developed by L. D. Landau (Ref. 2Y, the author writes down the series.:
=(k + al 2 + (P/2)~4 + (y/6)1 6+ 6(grad 1) 2'(1) for the thermodynamic
potential where (b09 a$ Pt y; ,6, are functions of temperature and
2
pressure, and 6(grad 1) is described as correlation energy. Because of.
thermal motion, ~ fluctuates round a mean v6lue ~0.(Zhe)series in
2 41~
first approximation gives correct results aq ~Long as Ll 0 and
T respectively, are small as compared to The condition
Card 1/3

84062
Some Remarks on Phase Transitions of Second S/181/60/002/009/003/036
Kind and the MicrQscopic Theory of Seignetto- . B004/BO56
electrics
6 T > X2/(6/c(,g)3 (60)2 (5b) is writtOn down (x Boltzmann con-
./0 > 9 - ~T
stant, 9 - temperature of the transition point). 6T = 0 T, T =~ 9,
2 1
6c = (af) Qp- . The character of transition thus depends only on For
9 16 fT'
superconductors it is found that fT -3-10- , for liquid.helium, fT -0-39
and for solids, fT - 0.03. Therefore, no anomalies of specific heat are
observed in superconductors. Likewise I fT is anomalously low for ferro-
magnetics. For seignettoelectrics, above all'BaTiO , it is found that the
parameter 12 = 6/ap is anomalously great, whereas3the fluctuation is re-
latively low . This qualitative statement is quantitatively investigated
by means of a model of anharmonic oscillators, and for the frequencies of
BaTiO3 it is found that 6it(g) = -VaT~T1rp1 -6.3-10-11; KIP t(Q)=2jW(5TPV,
and for wavelengths Xt - 2nc/6Jt (9) - 3 mm; 6jz, t - 1 .5 mm. (~L-m/2e2ffN' 11
0
concentration of the dipoles). The author considers detailed experimental
investigations of the behavior of substances near the transition point to
be nec essary. There are 35 referenceg: 22 Soviet, 9 US, 3 British, 2 Dutch,
and 1 German.
Card 2/3

Some Remarks on Phase Transitions of Second S/181/6O/Nft9/OO3/036
Kind and the Microscopic Theory of Seignetto- B004/BO56
electrics
ASSOCIATION: Fizicheskiy institut im. P. N. Lebedeva, Moskva
(Institute of Physics imeni P. N. Lebedev, Moscow)
SUBMITTED: February 10, 1960
x
Card 3/3

80876
s/141/60/003/02/023/025
E032/E314
AUTHOR: Ginzburg,_V.L.
1W_ MMU09mm-
TITLE: On the Possibility of a Determination of the Magnetic
Field in the Outerl'~`Solar Corona by Examining the Polarized
Radiation due to Discrete Sources Transmitted Through it
PERIODICAL: Izvestiya vysshikh uchebnykh zavedeniy, Radiofizika,
1960, Vol 3, Nr 2, pp 341 - 342 (USSR)
ABSTRACT: The presence of an ordered magnetic field in the solar
corona can lead to a rotation of the plane of radio \Y
emission passing through the corona. The radio emission
of the Crab nebulat'~~s the radiation in question. it
passes through the corona during June and has a polari-
zation of approximately 790' at 3 cm. The polarization
is characterised by a position angle of At = 148-i49
For 10 cm waves the polarization is 3 :t 0.50% and
It= 142 -4~ 50 . There is evidence that at long wavelengths
the polarization is smaller. In the corona (in the plane
of the solar equatori the 3electron concentrat on iS
(Ref 7) N - 7 x 10 CM at n = 5, N 10 cm at
Cardi/4 10 and N - 2.5 x 10 3 CM-,) at 20 It

80676
S/141/60/003/02/023/025
E?3j4E3A4
On the Possibility of a Determination 0 e agnetic Field in the
Outer Solar Corona by Examining the Polarized Radiation due to
Discrete Sources Transmitted Through it
2 2 9
follows that for 5 to 20 , w 0 4T( e N/m =. 3..L8 x io
N -,' 2 x 10 14 -8 x io 12 and to eEl/mc =
=-1.76 x io7 H - 105 - 105 sec Moreover, the
frequency of the radio emission w '-IVc/k - 2 x 10 10
sec-I at X - 10 cin . Under these conditions the
propagation of radio waves may be looked upon as quasi-
longitudinal for practically all angles a between tile
magnetic field H and the direction of the wave normal.
The difference between the refractive indices nt for
normal circularly polarized waves is
2 3 16 3
An = w11W0Cos a/W =_ 5.6 X 10 HN cos a/w The
rotation of the plane of polarization after passage through
the plasma layer is given by Eq (1), where the integration
is carried out along the ray which in the present case can
Card2/4 be considered to be rectilinear. In order to estimate this

80876
s/141/60/003/02/023/025
On the Possibility of a Determination oMMEA-a-'gnetic Field in the
Outer Solar Corona by Examining the Polarized Radiation due to
Discrete Sources Transmitted Through it
effect it is assumed that:
106HNL cos a
where L is a certain effective path longth. With
-2 5 -3 -,%-
zt 5 H ^- 10 Oe, N --' 10 cm cos a 1 and
L ~ IR0- 3 x 10 11 cm the rotation of the plane of
polarization is LINT = 6o0 . When =10 , H ~-- 10-
N - cm-3 Cos a - 1 and L - IOR9 the rotation is
AT,-- l' The relatively strong dependence of the
rotation on w should serve as a useful additional
effect. There are 9 references, 5 of which are Soviet
Card3/4 and 4 English.

80876
S/141/60/003/02/023/025
JO~A/EAI
On the Possibility of a Determination o e a4gnetic Field in the
Outer Solar Corona by Examining the Polarized Radiation due to
Discrete Sources Transmitted Through it
ASSOCIATION- Nauchno-issledovatellskiy radiofizicheskiy institut
pri,Gorlkovskom universitete (Scientific-research
Radiophysics Institute of Gorlkiy University)
SUBMITTED: March 25, 196o
V)~/
Card 4/4

GABIKM. 0.; GINZ,8094J.L. [translator]
Achievements and objectives of the industry of rubber products
for engineering uses in the German Democratic~kepublic. Uuch.
i rez. 19 no. 11:296-32 N 160. 1 (MIRA 13:11)
1. Nentrallnaya nauchno-tooledovatellskaya:.ioboratoriya
rezinovogo zavoda 9111be", Germanskaya Demokraticheskays,
Respublika.
(Germany, last--Rubber goods)