SCIENTIFIC ABSTRACT SOKOLOV, V.A. - SOKOLOV, V.F.

• Document Type: CREST
• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R001652020019-5
• Release Decision: RIF
• Original Classification: S
• Document Page Count: 100
• Document Creation Date: November 2, 2016
• Document Release Date: August 25, 2000
• Sequence Number: 19
• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT

"MOLOV, V.A.; doktor kbim.nauk
Third Symposium on Gas Chromatography. Vest.AN SSSR 30 no.12:80
D 160. (MIRA 13:12)
(Gas cbromatography-Coz),-resses)

SOKOLOV, Vasiliy Andreyevich; YIEFIM40U, T.D.,, ved. red.; YENISHERLOVA,
------- -vea-.r-eE-.,- TRDODOVA, I. G. , tekhn. red.
[New methods for separating light hydrocarbons] Novye metody
razdeleniia legkikh uglevodorodov. Moskva, Gos.nauchno-tekhn.
izd-vo neft. i gorno-toplivnoi lit-ry, 1961. 329 p.
(MIRA 15:1)
(Hydrocarbons)

SOKOLOV, Vasiliy Andreyevich; YUROVSKIY, Yuriy M-Ahaylovich;KUZIMINA9 NON., I
veduyushchiy red.; FWOTOVA, I.G., tekhn. red.
[Theory and practice of mud logging) Teoriia i praktika gazovogo
karotazha. Moskva, Goo. nauchno-tekhn. izd-vo neft. i goriio-
toplivnoi lit-ry, 1961. 337 p. (MIRA 14:6)
(Drillibg fluids-Analysis) (prospecting)

YAM-EV, Boris Petrovich; -SQKQLGLV-,-I'-A.._,dOktor khim. nauk., red.
SHOROKHOVA) L.I., ved. red.; 13ASIU.IAKOV., G.M., tekhn. red.
Pr-
(Direct geochemical mothods of oil and gas pro-o ecting;
methodologycal instructions for sampling, senling, and
degas.@ing of rocks]PrianTe geokhimicheskie metody poiskov
nefti i gaza; metodicheskie ukaz-aniia po otboru. prob gor-
nykh porod, ikh germetizatsii i degazatsii. Pod red. V.A.
Sokolova. Moskva, Gostoptekhizdat, 1962. 57 p.
(MIRA 15:9)
(Gases in rocks) -

Andreyevich; GRIGORIYEV, Georgiy Georgiy-e*ich;
DOGACHEVA, ved. red.; STAROSTINA, L.D., tekhn.ied.
(Methods and results of gas geochemical prospecting for oil
and gas]Metodika i resulltaty gazovykh geokhimicheskikh nefte-
gazopoiskovykh rabot. Moskva, Gostoptekhizdat, 1962. 402 p.
(MIRA 16:4)
(Oil fields) (Geochemical prospecting)

SaMLOV, T..A.j_ T. P.j VASS07MCH, X- B-1 ANTOMV, P. L.; C211200YET, G. 0-
&,A vozbw, V. P.
"Migmt1cla pa smses of G" wist OLL, Q91r Intowity and Dimaticleallity.s
Abstract. The article gives a description of the processes Gas anomalies observed on various levels of a section and
of migration of oil and gas, their intensity and direction in surface layers above oil and gas pools lestify to The
in various stages of the existence of sedj*menf6ry rocks. vertical migration of gases and to continuous processes of
In the early stages of the formation of sedimentary rocks dissemination of oil and gas pools.
the processes of migration cause a removal of excess gases Diffusion coefficients D, for various types of rocks' studied
into aqueous medium and into the atmosphere as well vary between 10" - 10-9 cmllsec. In some cases one can
as a primary accumulation of free gases in sediments and observe the dying of diffusion of the low values of D.
their solutions in underground waters. At '*D' equal to 10-s - IV cmIlsoc. the dissemination of
During oil and gas accumulation and the formation of gas pools by stationary diffusion alone is so great that
their deposits the following processes play the main parti their preservation within geologic time can be explained
transfer of oil in a dissolved stale both in compressed go by the unsteadiness of the process and by the phisnomeno
ses and in the water, a removal of dissolved gas and oil of the dying out of the diffusion reducing gas losses as
components from the water, condensation of liquid hydro. well as by the recent, in a geologic sense, forrnafion of
carbons from gases at d6creosing temperature and pressu- these pools or by a continuous replacement of the gas
to and then oil and gas buoyancy in porous -oaterbearing due to its inflow from deeper beds.
beds and rock mass. Considering the problem of the time of the formation of
The oil and gas pool formed undergo dissemination due gas accumulations cine, should take into account not only
to The processes of filtration, diffusion as well as du to the go of a trals but also the amounts of possible gas
the solution and removal of gas and oil by the water suit.
rounding their pools.
The processes of filtration are found to be most intensive
during tectonic shifts and they can cause the clegatsing
of a pool within a short period of lime.
W"t QKWW
alfurt
ft
r*pwt to be submItUd fOr Willis CM wi
'
C=00W,
,
19-26 jow 2,963

SOKOLOV, V. A.
"Migration processes of hydrocarbons, their intensity and directivity"
report to be submitted for the 6th World Petroleum Congress,
Frankfurt am Main, W. Germany, 19-26 j-un 63.

L 4740':-66 E WT (m ',,/E '7Pt/E T IIJP(c) ',VB/JD
ACC NR. AR6025712 SOURCE CODE: UR/OO58/66/OOO/OO4/DC)62/D()6C'
AUITHOR: Zhdanova, L. V. Sokolov, V. A.
TIT18: Investigation of the electron-vibrational and line structure of the aluminum
/oxidation spectrum
SOURCE: Ref. zh. Fizika, Abs. 4Vft
REF SOURCE: Izv. Tomskogo politekhn. in-ta, v. 138, 1965p 255-258
TOPIC TAGS: aluminum, spectral line, oxidation kinetics, flame spectroscopy, vibra-
tion spectrum, electron spectrum, Boltzmann distribution
ABSTTACT: To investigate the excitation of A10 molecules and the conditions under
which equi4brium is obtained In the flame, a study was made of the oxidation spec-
trum of Al'in the flame of aluminum powder burning in oxygen. It is established that
the distribution of the A10 molecules, which are in the gaseous phase in the flame
and produce in the 5400 - 44W A region bands of electron-vibrational structure
against the continuous background, obeys the Boltzmann law with respect to the vibra,
tional states. The relative intensities of the aluminum lines in a flame and in an
are mre compared, and it is shown that the intensity distribution is the same. The
relatively low temperature obtained from the vibrational structure of the A10 mole-
cules is attributed to the fact that these molecules exist only in the colder zones.:
of the flame. (Translation of abstract]
SUB CODE: 20
3/1 ha

,SOKOLOV, V.A.; @711DMAN, D.Ya.
Parametron with ferromagnetic films. Izv. vys. ucheb. zav.; radiotekh.
7 no. 3:350-357 My--Je 164. (MA 17:9)

SOKOLOV, V.A.; KOLLISNIKOVA, L.P.
Separation of alcohols by gas-liquid chromatography. Nefte-
.L
khimiia 1 no-4:564-566 Jl_Ag 161. (MIRA 16:11)
1. Institut neftekhimicheskogo sinteza AN SSSR.

SELIYANOVA, G.N.; SOKOLOV, V.A.
Separation of h7drocarbon gases by diffusion through porous
materials. Neftekhimiia 2 no-3:398-404 My-Je 162. (KRA lr,:8)
1. Institut neftekhimicheskogo sinteza AN SSSR.
(Hydrocarbons) (Diffusion)

SOKOLOV,V.A., prof., doktor khir.. nauk, otv. red.; VLASOIJ,
L.G., red.; RYLTJJ@., YU.V., tek@n. red.
[Separation and analysis of hydrocarbon gases) Razdelenie
i analiz uglevodorodrrjkh gazov; sbornik staluei. Moskva
Izd-vo AN SSSR, 1963. 231 p. (MIRA 16:12@
1. Akadeniya nauk SSSR@ Institut neftekhimicheskogo sinteza.
(Hydro6ar-Dons) (Gases--Analysis)

..- f,
, _-, @ @@ V -. t .
SOKOLOV; V.A. - @ .. i-i 3J , ) J. ". ; - .
Findi-rig the mc-3-., --al way to @- f ields
j @-S COnUll.3atue
with a Yi-z;h condan3a7@-a conzant. Gaz. delc :-.o-1-9:43-46 163 i,,a-P.A 17:10)
y iiaichnc-issl9dovatel'i'.ir instit-ut rirodnw,,o gaza.
1. Vseso@ya7m@r - F

SOKOLOV, Vasiliy Andreyevich
[Processes of the fomation and migration of o4-L and gas]
Protsessy obrazovaniia i migratsii nefti i gaza. Jjoskvaj
Nedra, 1965. 275 P. (MIRA 18:4)

IYUMBO, A.V., inzh.; PRITYKIN, D.P., inzh.; SOKOLOV, V.B., inzh.
Testing of a redesigned D-3500-13 sintering furnace exhauster.
Stall 22 no.2:110 F 162. (MIRA 15:2)
1. Zaporozhskiy sovnarkhoz, zavod "Zaporozhstal@p i
TSentroenergochermet.
% (Sintering-Equipment and supplies)

SOKOL40V y V.B.g arkhitektor; KUCHINSKAYA, I.A., inzh.
Using lightweight stu-mo-turea for chemical plants. Prom. stroi.
41 no.7222-24 JI 164, (MIRA -17:8)
i. T-Sentrallnyy Dnuchno-issledovatellskiy i proyektno-oksperi-
mentallr,7y institut promyshlennykh zdaniy i sooruzheniy.

SOXOLOV, V.B.
Nerves of the denticulate ligaments of the spinal cord. Doklad@r
Akad. nauk SSSR 77 no.4:745-748 AP-r 1951. (GILL 20:7)
1. Molotov State Medical Institute. 2. Presented by Academician
A.D. Speranskiy 27 January 1951.

USSR/1-fedicine Histology
Card 1/1 Pub. 22 - 37A5
Authors Sokolov, V. B.
Title Lymphatic capillaries of denticulatum ligamentum of a human spinal cord
Periodical : Dok. AN SSSR 99A, 629-631, Doe 1, 1954
Abstract : Histological and physiological data regarding the lymphatic capillaries
supplying the ligamentum, denticulatum of a human spinal cord are presented.
Six USSR references: (1927-1952). Illustrations.
Institution : The I. V. Stalin Second State Medical Institute, Moscow
Presented, by: Academician A. I. Abrikosov, September 16, 1954

SOKOIWV, V.B.
Receptors of the ligamentux denticulatum In a=. Blul.eksp.btol.
I mod. 39 no.2:69-73 F 055. (MLRA 8:5)
1. Iz kafedry normallnoy anatomit (zav. doystvitellmTy chlen AM9
SSSR V.N.Ternovokly) 11 Mookovskogo zeditsinskago instituta imeni
I.V.Stalina.
(SPINAL CORD,
ligamentum denticulatum, neural receptors in man)

SOKOLOV, V.B. (lAoskva, D-57, Leningradskiy pr., 75-a, kv.33)
Problems in eloctron microscopy tit the Suventh International
Congress of Ahatomists. Arkh. mat. gist. i embr. 40 no.5:
1LI-117 Mr 161. (Mk 15:4)
1. Kafedra normaltnoy anatomii (zav. - prof. V.V.Kupriranov)
II Moskovskogo meditsinskogo institut-a imeni I.I.I.Firogova.
(ANATOMY-GONGBESSES) (ELECTRON MICROSCOPE)

SOKOLOV, V.B. (Moskva, D-57, LenIngradskiy prospekt, ?#a, kv.33)
------ --__
Functional significance of nerves of the dentatee ligaments of
0
the spinal cord. Arkh. anat., gist. i embr. 43 no.8:35-4-9 kg 262.
(MIRA 17:8)
1. Kafedra normallnoy anatomii (zav. - prof. V.V. Kupriyanov)
2-go Moskovskogo gosudarstvennogo meditsinskogo instituta
imeni Pirogova.

I,IIMVMEV, V.A..-, YUNGMAN, V.S.; VOROBIYEVr A@F.; GURVICH, L.V.;
i3&q(R,Ui1, G,A.7 REZHTSKIY, L.A.; KOLESOV, V.P.;
GAL'CHENKO, G.L.,., KPOIDE'YEV, Yu.S.,- KHACHKURUZOV, G.A.;
.SQ40LOV,, V.B.; GOROKHOV, L,N,,; MONAYENKOVA, A.S.3
KOVIAROVA, A.F.; VEYTS,. i.V.; YURKOV, G.N.; MALENKOV, G.G.;
S-IIRNOVA, 11,L.7, GLUSHKO, V.P., akademik, otv. red.;
KIKHAYLOV, V.V., red.,- KARAPETIYANTS, M.Kh., red.
(Thermal constants )f substances-. reference book in ten
numbers] Termictheskie konstanty veshchestva; spravochn:PA
v desiati vypuskakh. Moskva, No.!. 1965. 1" p.
(MIRA 18:7)
2. Moscow. Vsesoyuznyy insti-W-11 nauchnoy i tekhnicheskoy
informatsii.

I
@T 7@
,-- 1, 1 . ;-.
V. ID. 30',"OLOV vill defend his thesis on "High-frequency Telepletric Channels on
Y 19.53 f or a degree of candidate
Wires 3f Elcctric Tranmission Lines" on 2 Jul
of tec'n-ni-cal sciences; at the instit-ute of Au+.r-pt---ics and Telem-echanics, USS7
Acad. :)f Sci.
Vechernyaya Moskva, @To. 14-6, 23 June 19153, p. 4

SOKOLOV, V. B.
"The Transmission of Signals of Remote Control Through High-Frequency Channels
in Power Systems" from the book Remote Control of Power Systems published by
the AS USSR, 19,54.

BARKOV, V.Ye.; BYKHOVSKIY, Ya.l.; GRZHIBOVSKIY, V.V.; PAVLYCHET, L.Ye.;
RABOTNOVA, K.I.;_SOKCLOT V.B., SOLOVIYEV, P.N.; KHMSONSKIY,
D.S.; ZV3IiIGCR0DSKIY, I.S., red.; SHMIYEV, T.I., red.; BORUNOT,
N.I., takhn.red.
[Savety rules in the construction and use of cormunication structures
and equipment] Pravilm tekhniki bezopasnosti pri ekepluetataii i
stroitel'stve sooruzhenii i ustroistv aviazi. Moskva, Goo.energ.
izd-vo, 1959. 103 p. (MIRA 13:4)
1. Russia (1923- U.S.S.R.) HinisterBtvo stroitel'stva elektro-
atantsiy. Tekhnicheskoye upravleniye. 2. Tekhupravleniye K:k-
nisterstva elektrostantsly (RES) (for Berkov). 3. Vsasoyuznyv
nauchno-issledovatel'Bldy inatitut energetiki (VNIIN) (for Bvkhovskiy.
Favlychev, Sokolov). 4. Gosudarstvennyy trest po orgenizatsii i ratsio-
nalizatsii elektrnqtantBiy (CROSS) (for Grzhibovskly)..5. Leningrad-
skoye rayonnoye.upravleniye energokh02yAyGtV& (Lonenergo) (for Rabot-
nova). 6. Moskovskoyo rayonnoye upravleniye energokhozyaystva (for
Solov'yev, Khernonakiy).
(Electric engineering--Safety measures)
(First aid in illness and injury)

BYKHOVSKIY. Ta.L., kand. tekhn, nauk; RATI@MS, R.L., inzh.; SOKOIA)V, V.B.,
inzh.
Selection of telemetering equipment. Illek at&, 30 no.2:76-77
7 159. (MIRk 12:3)
(Telemetering--Zquipmeat and supplies)

- SCtKOWV, V.B., kand.tekhn.nauk; IVANOV, V.N., inzb.; KULIKOV, V.V.,
inxb.
Protective shielding of lines carrying weak currents from
dangerous effects of 110 kilovolt lines. Felek.sta. 31
no.4:92-93 Ap 160. (MIRA 13:7)
(Eleckric lines) (Shielding Plectricity))

4. ?Sao (10,3j //,Yz) S/10' 10 12/CO2'.()" 41015
39 130 0 1-9
AUTHOR,3: Bykhovskiy, Ya. L., lzrailev, R. -A., 1,1il-utskiy, G. V.,
.51-ital'tsev, V. &., Sokolov, V. B. (Moscai)
rITM: @@cw studies on high-frequency channels in telemechanics
i-@@510DICJIL: Avtomatika i telemekhanika, Vol. 22, no. 2, 1961, 263-2-(0
TEYT: report is made here on studies conducted at the TIME an high-
C,
@reqtien c--=els in t@@iemechanics. The first part describes -an acoustic
- 1!
device of the tyFe This apparatus m:@Ices use of semiconductors and
is intended for the multiplexing of conductor circuits 6f high-frequency
c,-nneis of vnu-ious transmission systems. The rei-@'U-ion fn 450+180(n-1)
(n = 1,...,16) holds for the 16 transmission frequencies. norrm-band
frc!auency modullation '-ias been made use of to obtain a good noise-=.cof
fc--@.ture. I-lie tyt--e described here differs from its predecessor by the use
of semiconductors and in that emitter and receiver each have their o@m
current feed. Figs. I and 2 shui circuit diagrams of emitte.- and receiver.
'Llir! second -,-,i-t of the present paper is devoted to high-frequency tele-
Card 1/12

c 9 !,3 3
3111.0,) /6110 -21002/014/015
New studies on high-frequency B019/B060
phone sy--tems. Phe high-frequency systems for telephone and telemechanical
cornminications are made of new elements and intended for information
transmission over hiah- or niedium voltage lin3s. They are also suited
for rela.1, nrotection and automation systems. The units are made of semi-
conductors and miniature resistors, capacitors, and inductors, and require
thE: use of out7)ut i)(ver tubes. The third part of the paper deals with
reriotle switch systems. The nurcose of such remote switch systems in power
tr,insmission systems is firsi ex"plained, and it is stated that the
transmission lines themselves can in most cases be used for the transmis-
sion of the switching signal. A two-frequency sig-nal, a control frequen-
cy, and a signal frecuency are regarded as the best suited. A diagram of
th,a system concerned is discussed and shawn to feature a filter for the
su:)pr,:?ssion of noises having the frequency of the remote switch system..
.4 -,)ower @enerating and transmission systerr is most conveniently control-led
by conturol2ing the Dhase in a central point of the whole system. The
part of the paper is devoted to the discussion of channels for the
transmission of "he phase relation,within such a syster., to the control
unit. 'I"he system. discussed is operated with a seonrate high-frequency
channel over the @renSMj33--lon lines. The emitter consists of a crrs',al-
controlled
Lor, a two-staRe amplifier, a nc7,zer arr@nlifi@_r, a_n, an out-.-ut filter.
Card 2/

DEMUN, V.B.,, Inzh.; MUSNOV, F.S.p Inzh.; PC)BFALI'-ZHSKAYA, R.D., inzli.;
$GKOL"OV, V.B., kand. teldm. nauk
Nev THrP apparatus for remote control system- chan- Is. Elek.
stA* 34 no.5,.69-72 My 163. OERL 16:7)
(Remote control)

SOKOLOV, V.B., kand. tekhn. nauk
Line-service communication equipMant Using the wims of high-voltage
power transmission lines. Trudy VNIIE no.12:38@-46 161. (WRA 18W
1. Vsesovuznyy nauchno-issledovatellskiy institut elektroenergetiki.

SOKOLOV, V.D.; SHAFER, Yu.G.
Effect of seasons on the Intensity of the hard component of cosoic
rays. Trudy lAk.fil. AN SSSR. Ser. fiz. no.1:5-10 '55.
(MLRA 9:10)
(Cosmic rays)

SGKOLOV, V.X
Temperature corrections for measuring the intensity, of cosmic-
ray hard components; these corrections are based on teoperatures
of the atmosphere cross section up to an altitude of 5-6 km. Trudy
IFAN SSSR Ser. fiz. so 2:78-80 158. (MIRA 11:7)
(Cosmic rays) (A;mospheric temperature)

83805
C, ? 7 S/035/59/000/003/018/039
Igo el 16'1@ AOO1/AOO1
I
Translation from-, Referativnyy zhurnal, Astronomiya i Geodeziya, 1959, No, 3,
P. 49, it 1991
AUTHOR- Sokolov, V. D.
TITLE? On the Nature of 27-day Variations of Cosmic Ray Intensity
PERIODICAL. Tr. Yakutskogo fil. AN SSSR,- 1958, No. 2, pp. 123-1.28
TEXT-, 27-day variations of cosmic rays are investigated on the basis of
measurement results at Yakutsk performed with C-2 (S-2) and kk-i (ASK-1)
ionization chambers during April 1951 - June 1952 and :in 1954-1955. In distinc-
tion from the previous investigations of 27-day variations, in the present study
were calculated temperature correotions according to the scheme of Feinberg-*
Dorman on the basis of data of twofold atmosphere probing over Yakutsk up to a
level having 200-mm pressure. It is shown that the introduction of temperature
corrections, generally speaking, decreases the 27-day wave, and during the years
of solar activity minimum, 1954-1955, the 27-day variation observed was almost
entirely caused by the temperature effect. There are 18 references. LJ.Dorman
Translator's note: This is the full translation of the original Russian abstract,
Card 1/1

(3 9ooo SOVA609-4-.4061
@ranslation from- Referativnyy zhurnal, Geofizika, 1959, Nr 4, p 126 (USSR)
AU-THORS, Sokolov. V-D. S rIDIn. CU.
TITLE, In the Yakut Laboratory of Cosmic Radiation
PERIODICAL- Mezhdunar. geofiz. god. Inform. byul., 1958, Nr 5, pp 40 - 42
ABSTRACT: The collaboration of the Yakutskiy filial AN SSSR (ykkut Branch
of the AS USSR) in the investigation of cosmic ravggMn accordance
with the IGY program is described, The sta-ui=5 of the world-
wide network were supplied with standard equipment of two types
in accordance with recommendations of the Central Committee for
t@e IGY: a teleicope counter of charged particles and a
neutron monitor. The observation of the cosmic radiation in
the stratosphere permits the investigation of the stratosphere
variations of cosmic rays, their variation with the altitude
of the atmosphere, the connection between the variations in the
stratosphere and the variations at great altitudes, and the
obtaining of information on the transformation mechanism of
Card 1/ 2 primary particles in proportion to their penetration into the
41"

ft404
In the Yakut Laboratory of Cosmic Radiation SOV/169-59-4-4061
atmosphere. The equipment for stratosphere investigations comprises a
telescope counter for measuring the intensity of the cosmic rays and a set
for measuring the temperature and the pressure in the flight altitude. The
equipment is carried to the stratosphere by sounding balloons, For in-
vestigating the intensity variations of cosmic rays beneath the earthts
surface, a counter equipment of crossed telescopes has been developed, Con-
sisting of a device placed on the earth's surface and d(ivices placed below
the earth's surface in depths of 7, 20, and 60 m of water equivalent. The
main purpose of this work is the investigation of the energy spectrum
varia:tion of the primary particles on the basis of the observations at
various levels below the earth's surface, and the study of the alteration
of the intensity variations of the /A--meson component in dependence on the
thickness variation of the absorber, The time frequency variations of extensive
atmospheric showers of cosmic pys were also investigated in the range of the
ultra-high energies (1013 - 101 ev), which has been studied relatively little.
Bv means of a standard neutron -monitor placed on the earth9s surface, the
intensity of the neutron component of the cosmic rays is recorded, which it
most sensitive to variations in the low energy range of the primary spectrum.
Card 2/2 LN. Teren-ttyeva VK

.3, / 0 3@9669
3, 1 go 0 16@/61/000/005/032/049
A005/A13Q
01
AUTHORS: Kuzlmin, A.I., Sokolov, V.D., Shafer, G.V.
TITLEs On the 27-day variations of cosmic ray intensity
PERIODICAL: Referativnyy zhurnal, Geofizika, no. 5, 1961, 13, abstract
5 G 102. (Tr. Yakutskogo fil. AN SSSR, Ser. fiz., 1960, no.3,
111-115)
TEXT: The authors studied the nature of the 27-day variations of
cosmic ray intensity on the basis of data from recordings at Yakutsk in
1957-1958, Using the epoch superposition method, they determined the
amplitudes of the 27-day variations in intensity of the neutron component
at the earth's surface and the hard component at depths of 0-7p 20 and 60 m
of w..e.. They show that the results obtained do not agree with the as-
sumption that 27-day variations are meteorological in nature. In view of
the fact that the minima of the 27-day variations coincide with effective
magnetic storms and that the ratios of the amplitudes of the 27-day varia-
tions of the-different components are close to the ratios of the amplitudes
Card 1/2

29669
S/169/61/000/005/032/049
On the 27-day variations of cosmic ray intensity A605A130
of the Forbush effect of these componentai the aathors assume that these
two types of variation are of common nature. They 3alculated the spectrum
of the primary variations of intensity that satisfies the experimental
results. In high energy regions the spectrum has the form:
&D a (0- 5 # 0. 7)
D
N.K.
[Abstractor's note: Complete translation.]
Card 2/2

S/058/62/000/006/018/136
A061/A101
AUTHORS Kuz' min, A. I., Ye-f Krasil'nikov, D. D., Skripin, G. V.,
Sokolov, V. D., afer, G. V., Shafer, Yu, G.
TITLE, A study of the variations with -time of --lifferent cosmic ray compo-
nents by one-point observations
PFFIODICAL. Referativnyy zhurnal, Fizika, no. 6, 11.)62, 53, abstract 6B371
(In collection: "Kosmicheskiye luchi", no. 3, Moscow.. AN SSSR, 1961,
64 - 79, English summary)
T- A recording apparatus of the Yakutsk cosmic radiation post is de- V/11
@@cribed, and the principal results of a study on variations of intei@sity are
pre@@ented. The following instruments are laid out on the surface of the Earth:
a neutron monitor, two shielded ionization chambers, and counter telescopes
recc,rding vertical and oblique cosmic ray components. In addition, counter
t-lescopes placed at depths of 7.20 arid 60 m water equivalent record the muonic
co.m!Donent in the energy range of 2 - 109 1011 ev, while the continuous frequene
13 101L
rec.)rding on latitudinal atmospheric showevs yields information on 5- 10
Card 112

stidy of the ...
S/058/62/000/006/0!8/136
A061/A101
Tho values of the barometric coef h of diffgrent components
dr- OOL@,,Aed, as well as -the prinlApal ot av IniinstAgation of 27-day and
day variations of intensity. PhenDm,@Ina obstr%.,-.@! Iur@,ng magnetic storms
arr@:,b-.ie@'Zi d@-srribed. The interrelation factors ut--f.wa-en variations of intensity
--r and :3econdary cosmic ray COITIDone-n4- up t-o @rergiew-@ c,f - 700 Bev
-1 &t -:-P 11 wJ .'Frtes@! faet,,rs are utilized 'Lor the analy,-Is of :,ome types of varia-
of inten5lty,
IN. Kaminer
CAc@-+ra@A-@rls note: Complete translation
L

3728,;
2,0 e B/169/62/000/004/068/103
_0 D218/D302
Shafer, Yu.G., and Sokolov, V.D.
TITLE: Some results of stratospheric studies of the intensity
of cosmic rays at Yakutsk
PERIODICAL: Referativnyy zhurnal, Geofizika, no. 4, 1962, 13, ab-
stract 4G67 (V sb. Xosmicheskiye luchi, no. 3, M.,
AN SSSR, 1961, 143-148)
TEXT: A report is given of the results of measuring cosmic-ray in-
Uensity in the stratosphere above Yakutsk in 1958 - 1959. The ra-
di@Ltion was recorded with the aid of a double-coincidence counter
telescope. During one of the flights of the sounding balloon,,-the
stc..tistical accuracy of the measurements at the maximum of Ithe alti-
tude curve was at least 2 %. In many cases a major reduction in
the intensity was recorded in the intensity while the Forbush effect
was taking place at the earth's surface. Over 20 daytime and night
fliehts were made in 1958 in order to determine the diurnal cosmic-
ray effect in the stratosphere. On the average the intensity at
night is higher than in daytime by approximateiy 1 0,fo at the 500 mb
Card 1/2

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s/845/62/000/004/001/013
Mea.@urement of ... E192/R182
instilated and volta@,Ps of opposite signs are applied to them.
A certain charge proaiicea by the nputron-ionizing current is
stored on the collecting electrode of the chambers during- a
unit time A t; the magnitude of this charge is proportional
to the intensity of the neutrons and the charge on be measured
by the method described by N.L. Grigorov (TJFN, 8. no. 4. 1956).
In this method the charge on tl,e collector electrode is-converted
into a voltige pillse of definite magnitude. The pulses so
obtained are applied to the input or acnthode-follower tube-, the
pulse is negative and if@ of about 850 us duration. This pulse
is applied to an amplifier and then to a nonlinear amplifying
stage, where it is lenrthened to about 4o msec but where its
amplitude is still proportional to that of the input pulse, It
is then fed to a switching audio circuit. whose output signal is
in the form of an audio i-11se of 3 kc/s; the duration of this
audio pulse is proportions]. to the chargestored on the collector
electrodes of the chambers. The audio pulse is applied to a
counter which records the number of cycles. The circuit
for measuring the charge is based on directly-heated tubes.
The equipment was used between August 24 - 29. 1959, in flying
Card 2/3

L; @@ 2 5' 9
S/845/62/000/004/002/013
E192/E382
AUTHORS: �.pkolov, V.D. and Kapustin, I.N.
TITLL: Counter equipment for investigating the neutron
component of cosmic rays in thelatmosphere
SOURCE: Akademiya nauk SSSR. Yakutskiy filial. Trudy. Seriya
fizichoskaya. no. 4. 1962. Variatsii intensivnosti
kosmicheskikh luchey, 10 - 12
TPXT: The equipment is intended for measuring the density of
the slow neutrons of cosmic rays at high altitudes (for instance,
in artificial satellites). The neutron-detector is in the form
of a proportional counter, type CHM-5 (gnl-5), filled with gaseous
BP- The amplitude of the ionization pulse in such a counter is
muL higher than that produced 'Y16 elativis@!c particles; the
pulse is due to the reaction of B (n, a)Li 18s a result of the
capture of a slow neutron by the nucleus of B . The concept
adopted by W.P. Staker (Phys-Rev., 80, 52, 1950) and W.O.Davis
.Phys.Rev. I
1 2 80, 150, 1950) was utilized to eliminate the pulses
due to other effects. Thus, a second channel with its own
detector wasiprovided. One of the channels utilized a counter
Card 1/2

176i
s/845/62/OOO/Oo4/oo4/ol3
E032/E314
AUTHORS: Shafer, Yu.G. and,Sokolov, V.D.
TITLE: Seasonal effect in the cosmic-ray intensity deduced
from measurements in the stratosphere
SOURCE: Akademiya nauk SSSR. Yakutskiy filial. Trudy. Seriya
fizicheskaya. no. k. 1962. Variatsi! intensivnosti
kosmicheskilch luchey, 119 - 50
T The cosmic-ray intensity was measured by the counter
telescope described previously (V.A. Belomestnylch, Yu.G. Shafer,
Tr.YaFAN SSSR, ser. fizich., no. 2, 47, 1958). The figure shows
the results of an analysis of the 1958 daia in the form of mean
monthly variations at different pressure levels. As can be seen,
the amplitude of the seasonal variation reaches 8% at the 300.mb
level and decreases with altitude, reaching approximately 61,16' at
the 60 mb level. This indicates a considerable contribution due
to Low- energy ji.-mesons and shower proc ess es due to changes in 'the
atmospheric density. Both effects act in the same direction.
In summer, the probability of decay of low- energy it-mesons Is
increased owing to the increase in the geometrical height of the
Card 1/2

S/845/62/000/004/oo4/ol3
Seasonal effect in .... F,032/E314
atmosphere and this process removes both the ii-mesons themselves
and their decay products (low-energy electrons) which were not
recorded by the device. At the same time, the density of shower
particles is reduced owing to the reduction in the atmospheric
dens,ity and hence the probability of spurious coincidences in the
telescope is also reduced. The opposite picture is obs *erved in
wint or. If this interpretation is correct, it is to be expected
that the seasonal effect will not be observed with a single counter
or will be small owing to a considerable general radiation back-
ground in the atmosphere. This is a preliminary report; data
for 1959-1960 are being analyzed. There are 2 figures.
Card 2/2

1122 7o
s/845/62/ooo/oo4/013/013
e o E032/E314
AUTHORS: Shafer, Yu.G. and Sokolov, V.D.
TITLE: The effect of magnetic storms on the intensity of
cosmic rays as deduced from measurements in the
stratosphere
SOURCE: Akademiya nauk SSSR.. Yakutskiy filial. Trudy. Seriya
fizicheskaya. no. 4. 1962. Variataii intens*lvnosti
kosmicheskikh luchey, 139 -*141
TEXT: The results of a preliminary analysis of experimental
data obtained during intense and very intense magnetic storms are
reported. The cosmic-ray intensity was measured with the aid of
the counter-telescope d@3scribed previously (Belomestnykh and Shafer,
Tr. YaFAN SSSR, ser. fizich., no. 2, 4@7, 1958). The intensity was,
in fact, measured in 1959 at the 100 mb level. In order to compare
the effect of a magnetic storm in the stratosphere with its effects
'at sea-level, use was made of data obtained with a neutron monitor,
corrected for barometric pressure, and the intensity of the hard
component of cosmic rays corrected for bursts and barometric
pressure. The effect of a magnetic storm on the intensity of
Card 1/3

SOKOLOV, V.D.; SHAMI Yu.G.
Albego of slow neutrons in the atmosphere at a depth of 30 9/cm-2.
Geomag. i aer. 2 no.5:836-838 S-0 162. (MMA 15:10)
1. Yak--ttskiy filial Sibirskogo otdeleniya All SSSR.
(Atmosphere) (Neutrons)

- - , --- - - - - ---A-- - - - - - -
- @,- SIA-FER, V. D. SOKOLOV, N. G. SKFYABIN, V. F. LUTENKO
D-'---clbution of Cobmic Bay Intensity in the Atmosphere upto the Altitude 500 km.
repcrt submitted for the 8th Intl. Conf. on Cosmic Rays (IUPAP), Jaipur India,
-@-i4 D-c 1,-,63

PALIY, Georgiy Yakovlevich, polkovnik v otstavke; SOKOLOV, V.D.@
podpolko,mik, red.; MIKHAYLIK, V.F., kapitan.. red.
(The Sixth Heroic Battery] Shestaia geroicheskaia. I,-!oskva,
Voenizdat, 196-4. 89 p. (MIRA 18:3)

BADISHOV) A.P.; BEBRIS, K.D.; VERESOTSKAYA, N.V.; DANOVICH, L.Ye.;
DRIGUN, V.N.; KABICHKINAJI S.I.; NOVIKOV, M.I.; SOKOLOV, V.D.
Improvement of the methods for the preparation of tread
rubber compounds based on BR under the conditions of Dne-
propetrovsk Tire Factory. Kauch. i rez. 23 no. 3:5-9 Mr 164.
(MIRA 17:5)
1. Nauchno-issledovatellskiy institut shinnoy promyshlennosti
i Dnepropetrovskiy shinnyy zavod.

.L :Lr)691_6@, YSF(h) IF S8_2/EWT (1) /EEC(m) /F.G(O -i/E1101 (0 -2/&WG(v)/FCC/EWA W)
Pi -4/Pl-4/PP e -"/I)v b/Fb - 1, AEDC/-*:@.
ci
t /SWA (h) ro_4/Pe-5/Pq_4/Pg-4/
A FFT C /A FM DC /S S D - 31RA. D C /A PG CIE S D ( t ) /E S Di ) /A E DC Oa IS S D/BS D/A F-ft/A FMD Alt, FE 11 R/
AFTC (b)/AFTO (-a)/ASD-3
ACCESSION NR: AP5000175 S/02,93/64/002/006/0928/0932
TTIGwAis
AM'HOR.* Shafer. 1u. G.; Sokolov V. D.- Skry bin, G.; L)MtLt@nko V. F.; Yary*g"
A. V.-, Salimzibatov, R. B
TITIZ: Intensity distribution of cosmic rays in the atmosphere to a height of
500 km
SOME: Kosmicheskiye issledovaniya, v. 2, no. 6, 1964, 928-932
TOPIC TAGS: solar activity cycle, cosmic ray, geophysical rocket, single counter,@,-
ionization camera, Kosmos satellite, cosmic ray albedo, magnetic storm
ABSTRACT: In the period from 1958 to 1963, during a decrease in solar activit
cosmic ray measurements have been carried out by means of &go h sical rockets and
sat-11ites of the Kosmos _@_Me.,,,Geophysical rockets were equipped with single
counters and ionization camera!@. Satellites of the Cosmos type were equipped with--
1.5- nting telegcop 4@"for measuring the
@@,ionlzation cameras single counters, and cou
-cosmic ray albedo. Rocket and satellite launchings were scheduled for days with-@.:-
out magnetic storms and quiet sun. Primary cosmic rays were measured at heights
of :100-500 km. The cosmic ray albedo measured by rockets equipped with special
Card 1/2

L 1.56gi-65
ACCESSION NR: AP5000175
dev ices was found to be insignificant. Numerical values of measurement data show
a slight increase in particle count with height. No indications were found which
would associate systematic variations in the intensity of primary cosmic rays.with
the eleven-year cycle of solar activity. Orig. art. has: I figure and.3 tables*,
ASSOCIATION: none
SUBHITTED: Dtlay64 ENCL: 00 SUB CODE: AA, SV
NO IEF SOV: 003 OTRER: 008 ATD PRESS: 3144
card '2/2

L 2_175L6@ EdG(J)IFS~-21S.IT(l)lr-,WT(m)IEWG( )/FCC/T/El,;C-4/EEC(t)/E-IIA(h) Po-4/.
_Fe-5/Pq-4/Pae_2/Peb/Pi_4/Pb_4 IJP(,)/,Sb/,v,,,L/,SD(,) AFM(a)/AF4-fR/FSD(t)
ACCESSIONNR: A.P5000176 GW-21WS S/0293VC64 006/0933/0935
AUTHOR: P@@er Sokolov, V.D.
Yu. G. , krX2!j1n, N.G. Dergeym, K
Salhymibarov, R
TITLE: cot @aupper atmosphere, primary cosmic radiation, cosmic ray appara
30MIle r tus
cosmic ray asymmetry, cosmic ray albedo particle
'SOURCE: Kosmicheskiye issledovaniya, v. 2, no. 6, 1964, 933-935
TOPIC TAGS: Some results of measurements of east-west asymmetry in the Intensity of
pK!Mgry cosmic radiation
A.BSM?.ACT: Measurements of the east-west asymmetry of primary cosmic radiation were
made to heights of 500 km in 1962. The measuring apparatus was placed in the upper.
compaxtment of the rocket directly under thenose cone. The latter. was separated at a
L
height of 70-80 km. The apparatus (shown schematically in.Fig. I of the Enclosure) con
sisted of a system of many counters,- collected Into three groups of triple-coincidence
telescopes with 3 to 5 telescopes in each group. One' of these groups sampled particles in
@avertlbal direction. The two other groups of telesc9ges were mounted in the "east-west!'.
Plane at an angle of 600 to the vertical. The rocketsNI(Yere stabilized in space with respect
to azirauth and relative to the zenith with an accuracy of @--20. These measurements made
Card 1/4

L 21757-65
ACCESSSION NR: A-P5000176
it possible to estimate both the cosmic ray-intensity in-iks vertical - east and west direc-
tions and the number of cases oi local showerso. The experimental value of the effect of
east-;west asymmetry (Key) on the basis of the expression
west east
Kex 2 .100%
west 'east
had a inean value of 26+ 2%. However, the value Ke determined in this way will be masked
by albedo particles. If the particle energy spectrum Ts assumed to have the form AE-K and
if the earth's magnetic field Is considered a dipole, beyond the limits of the atmosphere the
intensif;y in a vertical direction will have an average value of the intensities in the slanting
directions
+
west east
IVert' 2
Card '2/4
MEE=

.L 21757,-65
ACCESSION NR: AP5000176
The enierimental value of the mean intensity obtained from the data of the inclined tele-
scopes was -greater than the int6nsity measured by the vertical telescope. This difference
Is not mdom and,can be interpreted as the absence of a contribution of a significant quan-
tity of albedo particles to the intensities recorded by the vertical telescope. By knowing
.the intensity of the albedo particles it Is possible to find the mean value of the effect of eastm-
@west as.,Mimetry of primary cosmic radiation (K), using the expression
West east
K 100%
vert
'it was equal to 34% 1 3%. The predicted value K, determined from,the theory of geomag-
netic effects using the integral energy spectrum of primary cosmic. radiation, is 35-37%.
.Thus, two indapendent methods for determination of K give values in agreement
within the
limits oj-' error. Orig. art. has., 3 formulas, 2 figures and 1 table;,1.,
'ASSOCVLTION: None
SUBWr'rED-- 12May64 ENCL: 01 BUD CODE: ES
NO REF SM. 001 OTHER: 002
Card @/4

L 21757-65
ACCESSION NR: AP5000176
ENCLOSURE: 01

G
2)
@
Figure 1. Sketch of place-

' 0
Oinstru-
%'!".
ment of measuring instrum@
s
..0, ment
.
,
ents in the upper instrument,"%.. _
Compartment,,,,-
comp;irtment of a rocket.

1. apparatus for measurl
ng
east - west asymmetry
,
D-group of vertical and
H-gi.,oup of inclined triple
coincidence counter tele-
cope;
2. shielded single Geiger

counter;
3. doxible-coincidence.
couqter telescope;
4. ionization chamber;
'
B. single unBhielded Geiger
cotLater.
Main body
of Rocket
Card 4/4

5-JA(h) Po- /F /Fe- e
/@CWG (v) /EEC (t) /EEG -2/Pab/
11 32218-65 DMI)IFC0 14 q-4 75/Pa
M--7- -GS7GW/V;3-2
ACCESSION NR: AT5006964
S/0000/64/000/000/0029/0036
AUTHOR: Shafer, Yu. G. of physico-mathematical s
(Candidate qiences);
Sokolov, V. D.; Krymskiy, G. Skryabin, 14, G,
TITLE: Seasonal variations in the intensity of cosmic r in the stratosphere
SOURCE: AN SSSR. Yakutskiy filial. Institut kosmofizicheskikh issledovani-Y i
aeroiaomii. Geo- i geliofizicheskiye effekty-v kosmicheskikh luchakh i polyaray"
siyaniyakh-(Geo- and heliophysical effects in cosmic rays and auroras). Moscow,
Izd-vo Nauka, 1964, 29-36
j
TOPIC TAGS: cosmic ray, stratosphere, standard level, ionizing component, mu..,
mescm, temperature coefficient, ozone layer
S"RACT: The intensity of cosmic rays in the jtratosphere was measured in Yakuts
A
B
d@r'ing the period 1958-1961. 'Temperatures on standard levels were taken into
consideration. in processing the observation data obtained. The-numbers obtained
by means of instrument counting relate strongly to the presence of mesons a The
main ionizing component in the stratosphere. r--onsists of the* electron-photoft com-,@-
ponent and disintegration particles; therefore, seasonal, variations of the goeral
Ionizing component of cosmic rays depend upon p meson disintegration under the
-,c

SOKOLOV, V,.D.
I
-Measixabilit.17 of alb@--dc neutrons and some experi=eental resultq.
Izv. Ali SSS'R.Ser.fiz. 29 no.10:1913-1915 0 165.
(IMIRA 18: 10)

i @ DX.- W
L
ACC Nil: AT6027218
SOURCE CODE, UW606076610061000106wflolol
43
AUTHOR: Shafer, Yu. G.; Sokolov, V. D.; Skryabin, N. G.; Salimzibarov, R. B.
ORG: none
bt
TITLE: Cosmic ray intensity In the stratosphere over Yakutsk during the period from 1958
to 1962
SOURCE: AN SSSR.. SihjLi@,qk9yt_qtdeleniye. SIbIrskiy institut zemnogo magnetizma, ionosf
rasprostraneni@g
I
ra vol . Issledovaniya po geomagnettzmu I aeronomli (Studies in geo-
magnetism and aeronomy). Moscow, Izd-vo Nauka, 1966, 97-101
605wj'r- t-ay lescere,
TOPIC TAGS: cosmic ray intensity, A-9ka pfe---- , graphic data processing/y,9/