SCIENTIFIC ABSTRACT A.Z. DOLGINOV - P.P. DOLGINOVEROV

• Document Type: CREST
• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R000410810012-4
• Release Decision: RIF
• Original Classification: S
• Document Page Count: 100
• Document Creation Date: November 2, 2016
• Document Release Date: June 13, 2000
• Sequence Number: 12
• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT

S/0511/62/000/008/017/134
A061/A10I
AUTHOR: Dolginov, A. Z.
TITLE: Angular correlations, in radiative nuclear transitions
PERIODICAL: Referativnyy zhurnal, Fizika, no. 8, 1962, 35,
abstract BB246
(In collection: Oamma-luch.i, Moscow Leningrad, AN SSSH, 1()61,
52~4 - 681)
TEXT: This is a review devotod to the theory of angular
correlations. The
following cases are considered: (1) Angular correlation between
two gamna quanta
emitted in successive nuclear transitions. The polarization of
gamma quanta is
taken into consideration. (2) Angular correlation between gamma
quanta In succes-
sive complex transitions. (3) Angular correlation b6tween gamma
quanta and inter-
nal conversion electrons. The finite dimensions of the nucleus
are takvn into con-
sideration, and the E transitions ELreF examined. (4) Angular
correlation between
two conversion electrons. (5) Angulair correlation of beta
particles ani gamma
quanta. Allowed and forbidden beta-gamma transitions of both
oriented and non-
oriented nuclei are considered. (6) Angular correlation of beta
particles and con-
version electrons. M-Angular correlation of-alpha particles and
the subsequ,!nt
Card 1/2

S/058/62/000/00 8/0 17/13
Angular correlations in radiative nuclear transitions A061/A101
gamma quanta. (8) The Influence ofelectric and magnetic fields of
neighboring par'
ticles and of the proper electron shell of a radioactive atom or.
the angular cor-
relation of emitted gamma quanta. The possibility of eliminating
the influence of
these fields Is considered. (9) The change of angular correlation
In the course of
time under the action of alternating electric and magnetic
fields. Ther-2 may be
both external. and internal alternating and constant fields
inside the specimen ex-
amined. E.g., constant electric fields inside a molecule or a
crystal, or alternat-
Ing fluctuating fields inside a liquid. (10) Relations between
the Cletsch-Gordan
coerficient, the Racah functions and the Pano functions are
presented. Tables of
Fano functions and different other functions are given which
pormit the angular
correlations to be determined in radiative nuclear transitions
and also in alpha,
beta, or conversion transitions.
A. Dolginov
[Abstracter's note: Complete translation]
Card 2/2

CNED111, Yu.N.; DOILGRIOV, A.Z.
Distribution of particles In the head of a comot.
Astron, zhur.
43 no. ltl8l-191 Ja-F 16,5 (111RA 19z2)
1. Fiziko-tekhrficheskily institut imeni A.F. lcffe
AN ESSR.
Subinitted Narch 129 1965.

ACCESSICS IRp mdcW4 B/oD56/65/048/oce/0548/0560
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TITLE: Thtont of rmltiple: xtmttixft~'~ 11
A,;:ojreiAcbe4kW tizlki, v. 461 no. 2. 19650
548-56o.
trcjdc scattering,
TOPIC Tim 11 rialtiple Best iering -,.I.np. !LjtstIi,- st:otterim, aniso
zransport equiition) lorce centex plau lalrer mattering
_iHOtr:;PJ,C -MUlt-i-PIC-t- Beat-
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thc
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vmny
131ca, ud pixysicia of ltuildd b-~ojle,,ii
prolilems In atomic and mutleur .3hyidae, azlirqor
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mtftip-ly cvtttercd
particles outfildt ani Inalide tbit bt,*, Tho transpoet, -tquwt4cv i:s
solved AWA C-X-
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AG'V' IIH: AF600083
AUTHORSt Gnedin, Yu. N.1 Dolglnov, A. -Z.
ORGi rhysieo-Technical InatItMe hu. A. F., loff 9,t__Aca~qemy
of 'Sciences '335M
zik 'T;-'2M-e-skr-Tn-
Fi Mem T
(
TITLE: Particle diatrik,tion An a comet hea$1
I;- b
SOURG'Et Astronomicheskiy zhurnitl, w. 0, no. 1, 181-191
TOPIC TAGS: comet, partiole dLitribution, ;iolor rAdiation,
dissociated gas,
spectral line, photcionivition
ABSTRACT: Eqiwtions are obtaintid fcr neutri,l and chnrged
particle distributions
In a comet hecd. Tha noutral jxrtlc~e ras cilittribution is
deecribed by the
transport equation oN &V
at (Or
uhere b is particle acceleration unglar solar attraction and
radiation prozioure
and S is the particle sour:e stranrLh. F!,r D ~'.ixiwllfan
particle volocity dis-
tribution function, the solution aC th,- vqwM.,,n yields
Card 1/3 UDCi 523.(6

L 22671-66
ACC NR: AP6006783
N (r, t) = 00 P (Air), 03 (r,
b)
For various val.Lae of the c~b/r rat!lv, closed form solutions are
obtained which
indicate that all particle density distributicne arrived at by tho
above assutip-
tions differ significantly from other known comet solutions. T~e
nituation is
improved if one assumes the-velocit), e1strit-ution
G G
imtead of the Maxwellian assimption. Simd3ar expressions are
derived for photo-
flissociation and photoionization rovults. 7h9 probability of
molecular dissocia-
tion is givon by
V2m,',mil(hv -
pal
2)nj M.
Particle dintributionis are Otained for 'ro~ u and VG~uy 1, where
v
'Ills
(hv - f.).
Card 2/3

L 22t--71-66
ACC NH.- AP6006783
These results show t1int the pnrticle dintribution 'in the
cc,nnt hone falls 0:3 a
Tunction or r-M, wboro m doponds on the nnttwo of tho particlo,
[U-3 Initial
velocity, accoleration, etc. In tho last, analyaln, tho
A;ure of tha comet is~analzed alon,r,- .11-rCorent appotral
l1nol nnd in applind to
the caso of the BerN:em comol; (.~.959), The authora exprea:i
aincore thank3 to
acadomician Kgro.tantineq, on whose initiative this work wan
undertaken.
Orie. art. hasi 3, flgiu-e, and I table.
SUB CODE 10 SUBM DATE: 32Msr65,/ OR13 RZF: 0031 OTH RM 002

L 02448-67-_ ~~1)ft ijp(r,)
'ATCNI, 6028793 SOURCE CODE., UR/0033/66/o43/oo4/0800/0812
AUTHOR: Gnedin, Yu. N.; Dolginov, A. Z. 4(7
ORG; Pimical and Technical Iristitute, Academy of
Sciences,,SSS.R (Fiz'Wottekhnichee
Jrrt Akademii nauk SSSRY___
TITLE: Radiative transfer in a, medium or finite dimensions
SOURCE: Astronomicheskiy zhurnal, v. 43, no, 4, 1966, BM-812
TOPIC TAGS: radiative transfer, -Mmmell equation, scattering,
indicatrix, multi-
scattering , 009r--'t".L,0 WRrrfe1.)C. . 'S6VA 0.FDAV40Ce
'*4V19r70A/ 211 /
ABSTRACT: Equations for the intensity of scattered particles
and photons inside and
outside a medium of finibe dimensions aiv obtained Dw the
Maxwell and Schroedi r equations,
Approximations at whicti these equattions coincide with the
known transfer equation
are indicated, and the connection between various forms of the
latter equation is
considered. The proposed form of the equation is convenient
for the study of
scattering in bodies of different iMometrical shapes. The
solut.-Ions of the equatic~n
are obtained in-an explicit analytical form for
multiecattering in a plane layer ',
or a sphericalvolume. Isotropic and sharply anisotropic
indicatrices for scattering
( CS
on a single particle are discaseed. Orig. art. has: 63 for=lav-
SUB COINAO I SUBM DATE: 05Ju.165./
Card I /I L_
ORIG%REF: 005/ 0711 REFt 003

ACC NR.- AP7003,218 SOMCE CODE: uF/OO56/6'6/O51/OO6/l77W1783
AUIMN: Dolginov, A. Z.; Toptygln, I. N.
ORG: Faysicotechnical Institute im. A. F. loffe, Academy of
Sciences, SSSR (Fiziko-
teldinicheskiy institut Akademii nauk SSSR)
TITLE: Multiple scattering of lxtrticles in a magnetic field with
random inhoma-
geneities
SO1MCE: Zh eksper i teor f1z, V. 51, no. 6, 1966, 1771-1783
TOPIC TAGS: random magnetic field, particle scattering,
distribution function, plas-1
ma charged particle) kinetic ejuattion, correlation statistics,
physical diffusion
ABSTRACT: In view of the fact ttat In many earlier investigations
sight was lost of
the numerous singularities that axise in the distribution
fucntion of particles in-
teracting with random mNinetic fleldi; trapped in a moving
plasma, the authors derive
a kinetic equation f:)r the motion, cf charged particles in a
magnetic field that
fluctuates in space -and In timet, and whose fluctuations can at
the same time move in
space in regular fashion with stome specified velocity. The
motion of the particles
is described by a di.3tribution function satisfying Boltzmann's
eTiation. This equa-
tion is averaged ove'.- the random ffA;r-etic field and an
equation 1.3 derived for the
averaged distribution fu.nction under the assumption that the
particle displacement
by the random field :is sma,11 ccqpax,td with the correlation
length. The derived
kinetic equation is nolved for certain sirWle cases of zero
translational velocity
C.,d 1/2

P~~~ AP7003218
and no constant magnetic fie.M., when the particle-momentum
changes are small, for a
statistically isotropic random fle:Ld., and for scattering in a
static random mWetic
field with spherical srmetzy. The transition to the diffusion
approximation is
considered and the equation for diffUsion of the particles in a
medium with moving
magnetic-field irbomogeneitiefit is derived. Orig. art. has: 2
figures and 64 for-
SUB CODE: 2o/ sum DA7z-. 3zuYS6/ oraG RLT: w4/ OTH W: 002
Card 2/2

-DOLGINOV,,;.M.p Inah.; WYNX0, N.P., Inah.; KMH075KIY,
N.I., kand.takhn.
nauk,; YUMNIENKC, K.A., In2h.
Adoption of OXh21115T steel welding In thq chemical
machinery indus-
try. Manhirie.)itromie no.4t67-70 JI-Ag 163. (KRA 17t2)
1. I:Iyevskly zavod "Boh'shevik" (for Polginov,
Iltyenko). 2. Inati-
tut, elektro-varki. Im. Ye.O.Patona AN UkrSSR (for
Kakhovskiy, Yush-
chey&o).

Ymmill, Yu. It. 1: KARTAKIN, A. V.; SOROKIII, N.
P.; DOLGINOV, 1. re.
Portable luminescent inuminator, Vest. oturin,
nc,.2t89-90 162.
(MM. 1522)
1. Ix Naue"ano-isisledwatellskogo Instituta ukhap
gorla i nosa
Ministeret-m zclrtvo6khr&neniya RSFSR (dir. - prof.
Ne A,
Bobroyald3r) i ordena Lenina klinicheBkoy bollnitey
Imeni S. F.
Botkina, Moskva.
('CYZOPJEIWJLAFCtNGOLOGY-WTIPMENT AND SUPPLIES)
,(ULTRAVIOLET RAYS)

DOLGIY I.Ye.; IESUCIDERYAKOV, A.P.
Spithesis sal properti-tis of dime thylli-
(cyolopropy1methyl)-, wthyltri-
(eye lopropy-1rmithirl).., and
tetra-(cyclopropylmthyl)silanes. DAL AN SMt
154 no.6i1376-1378 F 164. (MIRA 17:2)
1. Institut organicbesl:oy khWi im. N.D.Zelinskogo AN SSSR.
Predstavelno
aked,smikom A.A.Balandittym.

DOLGINOV L S Inshiquer-. 'I'LUNTITlY. A.A., inthener.
'r .
Calenla-tiag tenpmiture olonfation in steam ducts vith
Ions oxmn-
sion places. Trwly MTOSS 6 to.2:143-150 155. (Y.LRA 10:5)
(Steam anorineerinr)

BATIK. I.A., luzhensr; DOLOIDDY, L.S., Insbener.
ONSOMMEMOSSaw,
low nothod of! controlliqg the fitting of steam pipe
systems
accordizN: to their bw2ding moment. Sudontroanie 22
no.8.115-
19 Ag 156. (KLRL 9-.10)
(Win" pipe fitting)

DOLGINOT, L.S., Inshener,
Calculating thernel (Ixpannion compensation of compeasator
*team pipes. Sudoetroante 22 no*10-.9-11 0 '56. (HLRA 10:2)
(1hpansion (Heat)) (Marino pipe fittiqg)

DOLGINOV, L.S., insh,; ZAGUSTIN, S.R., insh.
Bleotrio furnace used for heating Pipes in fitting them
for
installation, Sudostroenie 24 noA69 Ag '58, (Kim IWO
Ollectria furnaces) (Marine pipe fitting)

DOWINOV.L.S.. inah.
Designing mt*&iq)lpos with lena-tM clampleas
mTemeatorlo
Sudestroonis 2.5 iiso4t22-26 Ap 159. (HIRA 12:6)'
(Stolopipol)

.' L. It. (?4)1;cow)
"A Tiny Magnetometer for, the Wasurement of Very Weak
Magm-tic Fields,"
e paper submitted at the InUmational Conference on Physics
of Magnetic Phenom=
Sverdlovsk, 23-31 May 56-
4
.1.1

A
rA n k/,
PHASE I BOOK EXPLOITATION
338
Vtoroy sovetskly Iskusstvennyy sputnik Zemli; materialy,
opublikovannyye v gazete "Pravda" (The Second Soviet
Artificial
Earth Satellite; Material Published in "Pravda") Moscow,
Izd-vo
"Pravda", 1957. 47 P. 100,000 copies printed.
PURPOSE: The booklet was written to give the public
information on
the second artificial earth satellite,
COVERAaE: The book consists of a number of articles on the
second
sputnik originally published in the Moscow newspaper
"Pravda". BELS1.0 information on orbit, structure, equip-
ment, performan 'pe, and utilization of the isputniks Is
given. All theze data have been repeatedly Dublished
elsewhere; therefore, only a few figures a:-e arbitrarily
singled out here. The total weight of the scientific
apparatus, test animal, and power supply sources of the
second sputnik was 508.3 kg. The initial orbital velocity
Card 1/4 was about 8,000 m per second. The second Bputnik
circled

The Second Soviet Artificial Earth Satellite (Cont.) 338
the earth initially in 103.7 minutes. Its radio transmitters
operated on frequencies of 4U.002 and 20.005 megacycles, etc.
The last article quotes admiring comments of American,
British,
French, and Chinese'scientists, statesmen, and journalists.
The
book contains 8 figures.
TABLE 017 CONTENTS;
Report of TASS (Telegraph 4pency of' the USSR) ("Pravda",
Nov. 4, 1957) 3
The Second Soviet Artificial Earth Satellite (6 figures),
("Pravda", Nov. 13, .1957) 5
Orbit of the sputnik and its ehangeB 5
Observations of artificial earth satellites 8
Structure of the second sputnik 12
Scientific measurements made by the artificial earth
satellite 15
Short-wave radiation of the Sun 15
Card 2/4 Study of cosmic rays 17

338
The Second Soviet Artificial Earth Satellite (Cont.)
Study of biological phenomena under space flight
conditions 21
On the Observation of Artificial Earth Satellites ("Pravda',
Nov. 11, 1957) 24
The Upper Atmosphere and Its Investigation with the Aid of
an Artificial Earth Satellite, by V.I* Krasovskly, Doctor
of Physical and Mathematical Sciences ("Pravda",
Oct. 10, 1957) 25
Investigations of the Magnetic Pole of the Earth With the
Aid of the Sputniks, by S. Dolginov,, N. Pushkov, Candidates
of Physical and Mathemat-nMr-Stl-en7ces ("Pravda", Oct. 22,
1957)29
On the Way to the Conquest of Cosmic Space, by 0-. Gorlov,
V. Yakovlev ("PravdO, Nov. 4. 1957)
Biological investigations of flights in the upper layerof
the atmosphere 32
Card 3/4.

338
The Second Soviet Artificial Earth Satellite (Cont.)
Penetrating the Secrets of the Universe (2 figtuws), by
S.N. Vernov, Corresponding Member, Academy of Sciences,
USSR ("Pravda", Nov. 18, 1957) 38
Comments
45
Conversation of the No Sputniks. Chinese Poem by
Go Plo-zho, President of the Academy of Sciences of the
People's Republic of China, translated by V. Derzhavin
("Pravda", Nov. 16, 1957) 45
Around the Earth aild Around the Sputniks, by G. Rassadin
(OPravda", Nov. 17, 1957) 46
AVAILABLE: Library of Cormpress
Card 4/4

~j
AUTHORS: Pushkov, N. V., Dolginov, 5. Sh. 53-4-1/11
TITLE: The Investigation of the Magnetic Field of the Earth by
Ueans of
Artificial Satellites and Rockets e
jasledovaniye magnitnogo polya.
zemli na isicusstve!nnykh sputnikakh i raketakh),
PERIODICAL: Uspekhi Fizicheskikh NRuk, 1957, Vol. 63, Nr 4, pp.
645-656 (USSR).
ABSTRACT: The present paper investigates some physical and
technical aspects
of such investigations. Firsts the basic problems of geomagnetic
measurement* by means of artificial satellites and rockets are dis-
cussel. In this wily it is possible to discover current systere in
the.
ionosphere, to evalitate thoLr ilensity, anil W draw conclusions
con-
cerning the existence of electric currents outside the ionosphere.
Measurements carried out by means of satellites and rockets can furm
, of magnetic anomalies
nish experimental results concerning the clampinp
and other peculiarities of the field in the case of increasing digs
tance from the earth. These data can then be used for the verifica-
tion of various hypthesea relating to the depth of sources of regio-
nal magnetic anomalies, which is of great importance for the study
of the interior structure of the earth, The most interesting places
for the measurement of the magnetic field by means of rockets are
the
Card 1/2 zones with.tho most frequent occurrence of polar phenomena
in Arctic

The Investigation of the Magnetic field of the Karth by
Means of 53-4-4/11
Artificial Satellites and Rockets.
and Antarctic regions. Magnetic meusurements by means of
satellites
will obviously be less exact than neasurements carried out
by means
of rockets, because tie satellites are rather small, and
because
orientation changes continually. On the otber hand, it is
possible
to extend measurements carried out with Sputniks over a
longer period
of time. The following is planned. a) Inventigation of the
spatial
distribution of the constant magne-.ic field round the
earth. b)
Evaluation of the spatial distribution of the heights of
the systems
of electric currents inside and ou"Oside the atmosphere* c)
Investin
eation of the inhomogeneoiL-i struct-are of the atmosphere.
Interpretas
tion of measurements carrii.-d out with satellites will be
connected
with a considerable amount of compatation work, but it wM
yield vea
ry importiint results, The results ,btained may also lead
to new opin
nions. The magnetometers to be usel on the satellites and
in the
rockets are then discussed, The be3t results will be
obtained by
means of such magnetometer3 as measure the components of
the field or
the scalar amount of the vector and its direction. The
authors here
describe the proton magnetometer (which is based on
measuring the
frequency of the free precession of the protons)j and a
self-orien-
tating magnetometer for the total vector.
There are 2o references, 5 of which are Slavic.
Library of Congress.
AVAILABLE:
Card 2/2

-,L
Translation from: Referativnyy zhurrial, Astronomfya I
G-~,odezlyq, N: 91
(Ussil)
AUTHORS- I)o,Zlnov, S.M., Zhuzgov, L.N., Puslikov, N.V.
TITLE- The! Preliminary Report Abolat Geomagnqtl.'.~ 3.,-j STvle"
Artificial Earth 5a.tel:.Ite
PERIODICAL: 3b. Iskusstv. sputrilki 7emd I. fir 2, AS U,SSR, 191~%
rp, I
hBSTRACT Geomagnetic measuremenl;s were carried ol.it cri t-he 3rd
ar,.1f1-,1,a1
satellite, which were &..-complizhed with thc rLid of a
mag.neto-saturated pick-,-.ips. The ot-tainel wil"
utilized In the folliw:Lng ways. I.) The ~oriparisw. -if th-- of
field measured by the magnetorneter and caloulated acoordlng tcr
-I'le,
potential V~eory. 2~ glht4 comparivan of' the istolatlon of the
f~1111. -,it:,ength
of the magnetic field 5nd the Intonsity of Qie cosmic rays
rmeat-'tired on
sputnik. 3) The analysis of the it-ea over the Eastern-Sib2r'-ui
m3gneli,~
anomaly, in order to cbeck the hyp)theses on the deptli of
o~.urranee of Its
sources, 4) Investigation into tnE, true existence of an
at4rc~:;~heric dynwmo.
Card 1/1 KTki3

66475'
I A
4,H 3,91t)0 SOV/20- 1?')- 1 -21 /611
AUTHORSt 11olginov, S. Sh., Pushkov, N. V.
of the Earth
TITLE: Some Results of Measurement of the Geonagnetia Field/Ty
reans
of a Space Rocket
PERIMCAL: Doklady Akademii nauk SSSR, 1,'159, Vol 1.19. Nr 1,
PP 77 - ao (USSR)
ABSTRACT: It was one of the taE,ks of the rocket., that was
fired on
January 2, 1959, to yield experimental data on the intensity
of the geomagnetic field at a distance of several earth's radii
from the earth's center. Such data a:~e of extieme importance
for the realization of the aresent t',ieory of magnetic storms
and auroras. According to the present theories, ?lectric
currents
may occur during magnetic stc,rms, which flow around the earth.
The electric currents flow at the distance of several earthts
radii - according to one kind of the theory -, bat flow at the
distance of several dozers o:;' Parth's radii, according to the
kind of theory. The geomagne-tic field was ateasured on board
of
the rocket by means cf a three-component nagnetc:-aeter, with
primary elements of magneticn1ly sn'.urated type. The
constroction
Card 1/4 of the magnetometer is shortly reported. The results
of the geo-
. ) ,

6647S-
Some Results of Measurement of the Oseomagnetic Field
SOV120-129-1-21164
of the Earth by Means of a Space Rocket
magnetic field mea:3urements, recortied by the rocket are
illustrated by a diagram. The second diagram illustrates the
variation of the intl~nsity of the geoi-aagnetic field along
the line of flight of the rocket, under the assumption, that
the field may be proluced only by sources present within the
earth. 8 coefficients of the devel- 'nment of the geomagnetic
field in a series for spherical funvtiozis were computed by
Yu. D. Kalinin. The measured valu,es differ considerably from
the computed ones in the range of 14.7.103 to 30.103 coyered
flight-kilometers., This disagreement decreases with
increasing
distance from the earth. The results of thene measurements
In-
dicate the followingi The geomagretic field is determined in
distances of 2 to 5 earth's radii not only by values,
coxputed
from the magnetic earth pz)tential, but depends B130 on
external
sources. Tht! anomalous effects may be. ciased by
a.q,7,n-vtic pherx-
mena, which occuiontwmoiJonof 1iarged particles i'n the geo-
magnetic field. Ther-~fore, it is of great interoot, to
compare
qualitatively the geomagnetic curve to curves cla cor%iie
rays
distribution (which was recorded by S. 1. Vernov, A, Yn.
Chuda-
Card 214 kov (Ref 3), Van Allen (Hef 4) and their
cooperators). A q-,*-

6647S-
Some Results of Measurement of the Geonagnetic- Field
SOV/12U-129-1-21/64
of the Earth by Means of a Space Eocket
simultaneous Qonsi.deraticn of the measirement results of the
field strength and of tho intensity of the cosmic rays
shows,that
idthoddoubt he effects, observed, in the magnetic fleld, are
connected with th,~ cc,rpuijcular radiaticn zone and are the
re-
sult of the superpos-ttion of tho magnotic field of the cor-
pusaular zone to the internal goaamagnetic field, On,- of the
most likely reasons of the magnetism in the corpuscular zone
are those points, which occur in conseqaence of the drift of
particles in the inhomogene-ous geomagnetic field. The observed
variations of the anoma.7.ous part of the magnetic field may be
essentially subject to 2 factorst To the variation of the
current densities which are connected with the energy density,
and to the variation of the -josition of the rockct, with
respect to the maximum of current den!3ity. The intensity and
the structure of the anomalous part of the magnetic field
depend also on solar activity and on the degree of magnetic
perturbation. Yo. G. Yl~roshenko and Yu. V. Afanaslyev
collaborated
in the development of the apparatus and A. D. Shevnin and L.
0. Tyurmina helpeii in the analysis of' experimental data.
Card 3/4 VK

Soine Reso*Itn of Measureizent of the Geomagnetic Field
of the Earth by Means of a SWe Rocket
6647S-
SOV120-12lu-1-21164
There are 2 figures ane, 5 references, 2 of which are
Soviet.
PRESENTEDt August 13, 1959, by A. A. Blagonravov,
Academician
SUBMITTEDt August 4, 1959
e
Card 4/4

~ 0 S, Sh-, YEROSM-,Op YO- G-, ZEMGOVj, 1. N., FUSMOV, N. V.
arA--n,-UTMnAi L_
DOMNOT
"Studies of the )Iagnotio rLeld cof the lexth and the Moon. "
rop(wt presbuted at the II Intermstioruil. Astrazutical Congress,
Stockholm, Sweden,
15-20 August 1960.

DOLGIVOVI S.Sh.; YEROSIEENKO, Ye.G,; PUSHKOV, Y.V.; IrAMINA,
L.O.
"Measuring, of the Magnetic 1"irlds of the Earth and Moon by
Means
of Sputnik III and Space Rocketv I and II,*
report presented nt the First Intl S)race Science Symposium,
Nice, France, Jan lrv6o.
National Academy of Sciences of tht USSR, Moscow.

71)
Hi
it t
A P.r
0 1 P. 4 til
al f f
;i FU 411
F P. Ell
lip. 'p. '1I
L

PHM K BCWX EXPWITATIOff SOV/4282
Ak%demtya nauk SSSR
IskusstvenuM sputniki zexlij vyp. 5 (Artificial Urth
OstellItes, no. 5)
14oscow,, Xzd-vo AN SM,, 73 ps Irrata, slip inserted,, 7,(W
copies printed.
F&BP. Ed.t L. V. Mu-nosovat IId4 of PUbUshing Bouset No I*
YVN&kluj Thche Met
Oe. M. Guolkova.
FURF=: The booklet is intended for ocientists and
engineoring and scientific
persoanel working in tha field of s]?aoe travel and
satellite flight.
"OVEP
AM: The collection of 10 articlas deals with problems of
satellite orbits,,
nagnetic measurements,, radiation.. the visibility of owe
vehicles,, the
upper atmospheret and neteoric substances. No personalities
are mentioned.
Feferenees accoMW scm of the articles.
Csxd 1/3

Artificial ftz-Wh Satellites Omt. ) SM/42U
Sedov, L. 1. S" Pocket Orbits in the Direction of the Won
-DoW._uov., S. Vht.~Yes Go Terosbanko, L. 11. Zhuzgov., N.
V. Pashkov,, and
1-.0. Nw-etie Measurements on the Second t8ovist] Space
fteicet
Vemov, S. W.~, A. Ye4 Chu&dm,, P. V. llabdov,, Yu. L
loopchev, and
A. G. Nikolayev. lbwUstion Nettauxement in the Flight of tht
second SO&"
Rocimt
Numosova, L. V.., Vs L loopebavs L, As huorenov, and N. 1.
Fradkin.
Iavestigstion of Cosudc Rsdiation in the Flight of the
Second Space
Rocket to the Ybon
Naza.rova, T. N. ibmilts of the Investiption of Wteoric
iMbstance
With tht Help of lantrupwitts Mounted In Opace Rockets
Raushenbakb, B. V., and Yo, H. Tokeirl., Some ?mblems of
Control in
Taterplanetary fpko.*
:.6
24
30
38
41
Card 2/3

9,irJ) WIP1282
Gu:~-ko, 0. V. aitermiaM.-Ion of the VistAlity Conditions
of Space
Pwkets 54
Dan-il.,,vj A. D. Concernimg; the Problem of the Formation
of No+ in
the Upper Atmouphere 60
Xiperov., L. P. Observations of Sigaals Rmn the Third
Soviet
Artifitial Earth Sate)-lite From Cape Chalyuskin 66
Yat,a,ms)dyj, 1. Jd.,, and 0. V. Gurko. Charge of the
Albedo of the
Arst PxtifinikL Earth SatelUte lbsulting; From the Action
of
Nxtexmal Factor3 71
AVAUAEU,': Library of Congress
AC/PV/i%l
Card 3/3 il-3o-6o

P&AM I BDOX EXPLOrTIMON S(NI4413
International Comic F*q Coriferrmce. Moscow,, 1959-
Proceedings. Y. III. Mosecne, 1960. 255 p. Errata slip
inserted. No. of
copies printed not given.
Sponsoring Agency: InternationLl Union of Pure and Applied
Physics. Cosmic
Pay Comais Sion.
Ed.: S. 1. Syrovateldy.Nitorial Board: 0. B. Zhdanov
(Ed.-in-Chief), 1. P.
Iyanenko (Assistant Zd.-Jn-Chief)., N. X. Gerasinova, A. L
Nikishov, V. 1.
Zatpepin, B. A. Khrenov, L. I. Vorwan, V. F. TuMmov, S. I.
Byrovatskiy, V. M.
Fedorov, Yu. N. Vavilov, and A. T. Abrosimov.
PURPOSR: 7his book is intended forphysiclets.. astronomers and
other scientists
concerned vith the ear-th's zadiation belts and cosmic ray
research.
COVERAGE: 7his is volume 3 of a 4-volume vork containing the
proceedings of
the Moscow Cosmic Pay Couftaxence held July 6-11,0 1959. Ibis
volume emtains
40 reports on the earth's radiation belts and primary comic
radiation. The
QLrd 1/ 8

International Cosmic Ray C!onterence. Prcceed!,ngs. v. III
reports delivered by Sciviet ceientists aret abstracted below.
Haferences
accompany individual rvports.
TA= Or CONTLUMS.
.1. MM MM6 R02TATION MKLTS
3. Vernovp S.N.p aad A93. Chudi0me Investigation of Radiation
in Outer Space 19-29
7his paper presents the expeximental asta, on radiation in
outer
space obtained by meajis of the 2nd acd 3rd oputnike and the
Soviet
cosmic rocket. It descAbes the instrumentation of the sputniks
and rocket, the Ugh-Imbensity inner and outer zonesp the
location
of these zories., toe intAinsity stability and the composition
of
particles in these zone;v, and the couposition of radiation
outside
the earth's magnetic fteld.
4. DoLgingy, S. Sh., and N.V.. Pushkov. Nagnatic Field of the
Outer Corpus-
eZi7r Heelo-n- 3G-31
It is stated that the Ugnetic field intensity values obtained
by
means, of t1v Soviet casmic rocket on January 2. 1959,
substantial-
ly differ ft-om those calculated theoretically. 7he way the
dif-
ference between seasimd and calculated mLgaetic field values
Card 2/ 8

International Cosmic Pay Ccattzience6 Proceedings. v. III
SOVI"13
variid With increase 12 roeket distance from the Earth is
compared with the corl?2scular radiation intensity values
obtained on. the cosmic rocket and Plower III.. 7be
compari-
son shows tbat the obivo~rved c:banges La the Earth's
magwtic
field are velated to 11,':te outer corpu&:ular region,
and that
they might be due to 10e supe:rpositimi of the =gnetic
field
of the coquacular 2ow on t1w magnetic field of the Mrth.
7. Vernov, S.N.,, A.R. Chudakw., A.I. Iebediwky
(ImbediaskJy), and I. P.
Ivaneako. Cotqvsition of -the Mel's Corpuscular Radiation
and
Possible Wchwilsms of Ita Origination 46-49
This paper presents duta on tle composition of the Earth's
corpusmilw:- rediation obtained by mearts of tbe. Soviet
sputifte
and the coiimic rocket,. The overwheladng majority of
IxLrti-
cles in thei external none, United by =go tic lines of
force
crossing t1in Earth's irizz-ftoe at geozeenetic latitudes
of 55*
and 65'op we electrona of 20-100 Kev. Protons of
approximately
100 Nov vere discovanil in. the internal zone, limited by
Card 3/ 8

Internatiaaa-1 CowLc My Comference . Proceedings. v. III
SCV/"13
magnetic Lines of force croasing the Sw*th's surface a.t
9eOR1%POt-i(!: lAtitU&18 of 30-40*. Among the possible
nechan-
isma of origination of the Hartble corpxLecular radiation
is
injection Into the Earth's magnetic field of electrons and
protons,, producel by t~e decay of neutrons emitted by the
Farth's aftiosphere a,s it result of comic ray
irradiation.
9. KrassoveJW (Yhi,sov9kiy),, V.L., I.S. Shklovsky
(Miklovskiy)., 0. 1.
Galperin, and U.M. Svetlitisky (Svet3dtskiy). On Fast
Corpuscles of
the Upper Atsiouphere 59-63
This paper presents ex'Verimental data on fast corpuscles
of the
upper atmoiil)~ere and gl'.ves a detelled dercription of
the equipment
used. in t1mi. 6xperiment.
U. Dorn-, L.I. On the ProbLem of the Nature of Soft
Radiation in the
Upper Atmosplume 74-8o
This pa-**r emmarizes the available data on bursts of soft
radiation in the atmDeOere and iuvestigwtee th *e nature
of the
bursts in :ivlation tA3 processes on the swi, in
corpuscular
streams,, and La the Uterplametary medium. It also
investi-
gmtea the ratmre of -bbese bursts In relation to the
properties of
the gartkili!i belts of radiation.
12. Askarlyan G. A. On. the Rature of the External
Hadiatien Belt of the
Zu-th 81-82
Card 4/ 8

IntermatiorAl Cothide F13y Comlerence . Precoadinge. v. 111
5 a,/" 13
It Is stal:ad that the external radiation belt encircling
the
earth is of nuclear origin, but tbLt the explanations of
the capture
and accumiLlation of pou-ticles by the E&rth's mgnetic
field in
the course of Its lowLl, variations am not convincing as an
ex-
planation of the nature. of the exUrnal mLiation belt. A
more
convincing, explanation of t1be obsei-ved effects Is given
in this
paper*
:17. IRTKAM COSM RADIA710H
22. Charanchlyan, A.11., aml T.N. Marakhohlyan (Lebedev
Physical Institute,
USSR Aca&.uq of SAencen; Nuclear Physics FeseLreh
Institute., Moscov
Uhiversity). Ene:rgy S~poctruu of PrimLry Cosmia Particles
129-135
This paper explains the results obtained frm investi-
gELtions of the electron corq>onent of cosmic radiation in
the
upper .1qn!:re ol the utaosphere.
23. XDcharyan, N.M., O.S. SuLkyan, and Z.A. Uracwyan
(Kirak-osyan).
Spectrum of Cosmic Radit-tion Protons 136
This is azh abstract of the results obtained in four
independent
experlmentso The ruJil text has been. publIshed in Russian
in
Card 5/8

rnternLtioua.1 Cosmic HILY C=Tellenee. Proceedings. V. III S
OV144 13
the Zhurnal eltoperineritallnoy i teomticheekoy fiziki, 35,
1335 (195,B)-
111. TM: ORIGIN OF CQDaG RAIM
33. Ginzburg, V.L. Same As)vcts of the Tbeory of Cosmic Phy
Origin 196-204
This pLper elwAdLteii the following problems-, 1) The mean gas
con-
centration in -the SKL&xy (including the hLlo). 2)The role of
different; cosmLe my soumes; the inlection sad particle U-
celeration mec.13anism tu souxces. 3) The mechanism and role of
cosmic M esaLpe f'x-vxn the galactic b&lo into intergmlactic
Space; the f~A,Aion of metagLlactic cosmic reys. in tlu--
Galaxy.
4) The n&ture of comaic my movement in the SLIactic spirL1 in
connecticin with coomte rLy isotropy and chemical composition
5) The origin of the co=de ray electron component in the halo.
34. Shklovskiy, I.S. Achie-imments in RLdioastronomy and
PlAdioutronomiml
Theory of the Origin of Comic Hays 205-210
Min papetr explains the isdioestronomLeal theor7 of the
origin oJ! cosmic Mii on the basis of the IMASt, LChievements
in radionstronany.
Card 6/ 8

International Coadc My Coubtrextoe. Proceedingel. v. III
OW/4413
35. Znvhak.. A.A.,, andS.I. lArrmtoky (Syrovatokly). On the
C(mposition of
Pr1mary'Cowde Pays 2U-219
Mde paper pointis out I** invAeqwLey in the explanations of
the
composition of cosmic jWs and presents another approach to the
solution of this problem.
39. ftiletdW (ThrleteldLy),, T.P. Ptissible Acceleration of
Cbmages
by the Eleetromaguttio Wxld of the Magueti,z Dipole of the
Earth 233-238
This paper presents t1wt results of new oxmputatitm of tho
electraimagnetio fteld of is rotating dipolei, as voll an of a
corrected amlmis of I= not-ion equations pertWLning to this
field. Qr4estions repirdbig tbe divergeam between
computations in
inertial and roix6ting eys-Was of coordineteo am comsideredp
and
gener*.l conclusims vJ.th :mggxd to the noture of
distribution of
charges around in rotiating dipole imad with. regard to
analpsis of
poselble currents wm ma&.
40. Dormn,, L.I. On the Initial State of Charge d-FOixtielm
AcceIg-ration 239-244
The author immIlmes the tollowing problemat 1) Injection
energy In a
s6lar flare in the case of charaed-particIe aceeltration ty
the Yermi
statistical mecbanism, 2:1 Portion of aawlerated pLrticlon and
necessity of preliminary acceleration by the first order Termi
Cird T/ 8

3MOrmbimal Coamic W Confemnae. Practedinge. v. 111 5
W144 13
mecbmalem. 3) kwelemtiau of piLrticles of the wAldium
belveen
approaching mgnettic alonts: nourelativistic Cace,
relattilstic
casep and the catie of jarticle acceleration from very
low
onergies to relm6tivietle anergies Omudmx enerm- of
accelerated
particles in various eVecific casew cowpreesion.0 -tbe
plasm
coluum under lahlratpry- cmd1tions and under
conditions of solar
flAres,, collision. of magnetized clouds in
interplaustary.Lad in
IntersUllar space,, and col.31mion of gkUztes.
AVAUAKS.- Libraz7 of Congress
A44waftea
Owd 8/8 10-18-60

DOLGRI-IM, Sh. 5h. -4 -f -
ResearclAnC the %gpetic Field of the Mcon, -dpwl.
report prc-sented at the International Symposium on
the moon, held at tile
Pulkovo Observatory, Leningrad, USSR, 6-F. Dee 19-0.

c: C, -A--.t C-7-~~- c"ic ricl., f--=
LIE ll,,~ -.Z~,tc-Y C'-' U.--, L. 7.
L. C., !-..V
C. C t0
C, G.
0-1 11-:,; o,- ti-,z VL--Ir~bllaa
UQZLOV.;Kjy,
V. V.
Ca V. 1.
0- L.
CT 11-,'--~,-.--t---,j !:!I
0', C;
T. 17.
C.% X--:r c -i e7
Cz
rc,iort3 to it,
WtlshL--~;tGn D. C. 1-7 (V-tc,",cr 1931

1972 S/169/f;;,/000/008/034/053
0 A006^101
AUTHORSt D-04tinov, Sh. 311., Yerasheako, Ye. 0,, Zhuzl;ov, L,
N., Pushkov, N. V
TITLEt Investigation of the magnetic lunar field
PERIODICKLt Referativnyy zhurmal, Geofizika, no. 8, 1961, 12,
atetraot 8080
(,"Geomw*tizm I ateronomiya", 1961, v. 1, nc. 1, 21-29)
TW: Information is given on experimental problems and -Sets
about the
lunar field, obtained during the flight of the second Soviet
space rocket. An
analysis was made of the sensitivity threshold of the
measuring instruments from
data of measurements in the wejLk terrestrial magnetlo field
at 45-60 thousand km
distance from the Earth's center. The noise lovel in the lunar
orbit space was
analyzed, and measurements werts made directly near the Moon
down to 55 Im distance
from Its surface. As a result no indioations of a noticeable
lunar magnetic
field were detected, It was estimated that thit dipole
magnetic: moment of the
Moon can be only less than 1/10,000 of the magietio moment of
1h9 Earth. I
(Abstracter's note: Complete translation]
Card 1/1
The authors' summary

DOLGINOV~ Sh. 8h., PUSRKOV., N. It.
"on Scue of the Barth's Maguetic Fleld Invelltigations
in Outer 3pace"
Soviet Papers Presented at Ple=7 Meetings of Comittee on
Space &.-search
(COSPAR) and Third InternatioW. Space Science Symposium,
WILshington, D. C.,
23 APr - 9 may 62.

DOW32!CVP Sh. Sh., I-035.-OV, II.V., MUMMA, L. 0.,, FRYnTNOV, I.
V., t*jl('L X Z-7-2GAV, L. N.
"Scme of the Conatant Geo%46metlo Fieli Meftuicmronts CiaTled out
n-nm
Sputnik III o-mr the Territory of the LOSR."
Soviet paper presented at the Plenary Mbetin&s of Co:nadttc,e on
SPILCO Rosearch
(COSPAR) and Third International Space Smposlun', Wash. D, C.0 23
Apr - 9 ~4 62.

42154
S/203/62i/002/001/002/019
1023/122.5
ATUPIORS Do1g1no%,,.,-'h*Sh,, Yeroshenko,Ye,G., ',.7huzgov,L.11., and
r1 1.9 hR 0 v 174. V .
11 IT U, Magnetic measurements of an axktomatle Interplanetary
station to Venus
PERIODICAL: Geomagnetizm I Aeronomiya, v,2, no.1, 1962, SB-40
ri
EXT: A t1wee-conponont magnetometer to measure the magnetic
.1 ,
fin1d norr Vowis &nd a inagnatic varlometer to mousure t:-.Ie field
during the voyrigo wero Ir3talled on the automatio Interiplanetary
station (AIS) to Venus. The threshold sensitivity of the vario-
It' ineter vias 21-, tho range - 0 to 50 Dat .1
a from the var ometer
wore Gbtained on Fobruar-y 12 and F7, 1961. The magnetograms for
1~'ebrusry 12 (distance from Sarth: 165000-175000kvi) are given
togother rilt), data from the Moscow observatory (q) = 550 ). The
vqrlatlons of the two mngnetograms were Rpproximately the same*
Data of February 17 (distance from Earth: lo9xlO6km, duration of
Card 1/2

S/203/62/4)02/001/002/019
1023/1223
;.;agnetic nea;iuromontses-
monq,n-arnents: '112 min.) shot, almost constant vnluets,
During the
same period vr,,riRtlons on were quite big: 2-0-215-j- .On
Fobruar-y '7, 19610 the AP'~'wao In the oorpusculrAr stream
(assumption bagod on data from a particle trap), The magnetic
field of the stream vms leri than 0,.f in the direction of
the axis
of t1v3 transducer. 0,Lts- on the n(nitron component of cosmic
rays it can be deducod thm; the field or the atre(un was weak
also
on Earth. Georiagnetic, d1sturbancos oan be explained by &
direot
interaction of the cor-puscular stream with the geomagnetic
field.
There are 3 fl~~,res,
ASSOCIATION: Institut, zemnogo magnatizma, ionoafory i
rasprostranenlya radiovo]AAN SSSR (Institute of
Terre.stvial Magnetism,, Ionosphere,, and Radio wave
PropaE,ntlon, AS USSR)
SUP311.11TTED December 6, 1961
Card 2/2

8/2C-3/62/00*.VO06/004/020
A160/AIOI
AIMIORS: Dolginov, Sh. Sh., Zhuzgov, L. N., Puahkov, N. V.,
Tyurminap IA. O.$
11~a _rcic~v
TITLE: Some results of measuring the constant magnetic field of
the Earth
with the third artificial sputnik of the Earth %bove the
territory
of the USSR
PERIODICAL: Geomagnetizmi aeronomiya, v. 2, M. 6, 1962, 1061 -
10`75
TEXTt The author prenents some results of measuring the constant
magnetic
field of the Earth with the help of the third Soviet sputnik
above tie territory
of the USSR from Pay to June 1958. A brier descripti6n Is g1ven
of the metro-
logical properties of the used equipment and of the method o1!
elimiraiting mag-
netic board noises from the sputnik magnetograms. It was
determined tha-t the
deviation may be represented by t1uee harmonica whose mean
anplitude values
equal Ulm - 1, 500, U2M - !j00 and U, F = 20`3 7 . A comparison
or the i3easured
values of the gecvnagnetie field intensities with the values of
this Intensity
permitted to establish Uieir agreement irithin the limits of 0.1
- Ilf above a
Card 1/2

Some results of measuring the... S/203/62/002/006/004/020
A16o/Aiol
major part of the USSR territory,'including the Siberian world
magnetic anomaly.
The conclusion is illustrate6. by a limited number of typical
magnetograms ob-
tained on the segments of thc trajectories traversing the whole
territory of
the USSR. The material yielded by the magnetic investigaticns with
the third
Soviet sputnik permits to fully determine the possibilities or
carrying out spe-
cial magnetic experiments. 1) The main harmonics of the Gaussian
series can be
determined with a precision of 0.1%. 2) With the help of a
long-lasting sputnik
the real existence of the exterior sources of the magnetic field
ha-- to be found
out, not taking into consideration the theoretical valuei of the
field, computed
from the ground data. 3) Flegmlar work should be done on the
secular- variation
of the geomagnetic field. 4.) In o~rder to obtain highly accurate
date., the re-
quirements for the complex of auxiliary equipment should be
determined. 7here
are 12 figures and I table.
WOCIATIONs Institut zeninago magnetizma, ionoafery i
rasprostraneniya radiovoln
AN SSSR (Institute of Terrestrial Magnetism, Icinospherti and Radio
Wave Propagation, AS USSR)
SUM= I July 10, 1962
Card 2/2

i-1341'- 63 EW I /BMWES V) AMCASWESM-3 Pe-4 aN
ACCESSION NRj AP30073371
s/02.93/631001/001/0055/oogl
XUTHORt D algilMy. ushko v. N, V.
...........
TITLEt Investigatia
tbA t!AXje_tj_~-_ i a I d t nsp~cel/
SOURCHI Kosmicheakiye issjedc)v&jjjyS,, V, 10 no" 10 1963, 55-97
TOPIC TjkG!)
11 V69116tic field, terrestrial magnetic field, inter-
planetary wedium, lunar.magnotic field, outer radiation belt,
mliguttORP119re, milanetic storm. solar plasma, ring durrent. geomat-
notic field, venmelau ih.iigA*t1c field
ABSTRACT: Experiments). d,jitis on tha~msgnatlc fields of t1is
eartIft,
moon. and interplanetary wpace' obtalned by Soviet and U, S. rock-
ets and missiles, have ba0n:vurveyeid, and the results of measuria-
mcints mada near the aarth, Lu the outer radiation belt, and at the
boundary of the geomnanofte field havis been compared. It vas found
that the onergy necerstiTy tv create and maintain the outer zone is
upplied by the sun, but the mechanism whero'by the solar plasma
:
nergy is tranaferre4l to the magnetoophere is still not clearly
understood. It has mot: yet be~tn jusip1ble to determine with finality
Card l/ 2

AtCESSION
where os: whether the classIe eurroont sy a to= 4s
vac I a to dwith nhe main
phase of Magnette storms alrtvially exIats. It has been found that:
at distances exceeiding 8 11. (r&dius of the eiarth) the misaiiured
values of the field cin the ds,; anti night sides s)f the earth
exceed
those theoretically cowputiodo 2) the direction )f the field ~&t
dis-
tances up to 12 R(t diffe-re from 31) to 60* from the directloa of
the
dipole field 3 i~oncide-rabla field fluctuation.o are noted in the
region fro m 10 to 1.5 Re, 4',1 no noi:ablm differen.:e exists in
the
characteristics of tfie torrestrial field on the day and nighc
sides,
5) a transition zonot probably exints in the 10 -to 15 R region
e
between solar plaisma and the geomagnetic field, 6) inf 0rmation is
lacking on comparative-con4litions-In the 12 to 15 Re region, and
7) it is poasible for a nsj~netitt t'rail to exist on the night
side-
Future attempts vill be mad's ~o obtain convincing proof of the ex,
istertcat suit localizati*6 of' the current ring of magnetic stoxms
and
a precisti ostabliahnfint of this topology of the isagnstic field at
great dilitances.
ASSOCIATIO11 : none
SUBMITTEN OlDec62 DATS AfAs 210ct63 Ma 00
SUB CODEs AS 110 IREF SOV 1 037 OTFERt 066
Card

DOW331M, Sh, Sh, and BULANZHE, Tu. D.
Present state of magnetic mmasurement teohniquesp
Title, Conference on problems of' marine magnetic
surveys (hold In Moscow in
P4m!il 1962,
Source; Oknanologiya, v. 3p no. Jq 1963, p., 752

DOLGINOV, Sh., laureat Lenindkoy preniAlp
kand.fix.-featem.nauk
Terrestrial magneldiss. A,v.i kosm. 1,6 no.7t26-32 Jl
163o
(Magnetism, Terrestrial) (MIRA 16:8)

YM)SHENKO, Ye. G.; DOLGINOV,- Sh. Sh.'; ZHUZGOV, L. N.;
FASMSKII, U. V.; ALEKSANYANj,
11. M.
"MAgnetic Investigations on the Electron 2 Satellite."
report presented at, t1v 5th Intl Symp on Space Science)
Floreace, Italy, 12-16
May 64.

~)-2/FW WEED lt~o
I/P1 - V S/ 020 64/15 06-A272)l I ,z)
A CC Z S S.I 0 It 1.1t; AP5001$'06 P~e~e -4 MO2
ON,
AUTHOR: --Gr:Ln!xauz. Y.. -Sh-. Sh.;. Be31rukik-h,,.V--.~---;
nhemko. Ye. G.,; "TIT K.;
TITLE: Pbaervationn. vaing th;s artificial astellite Slioctron..2 of the
ci:>rrelativa betueen vuriat Ions of ths) ~magnetic field aid strcams of
POSItIVC 11)n3 In3ldO the- ttrrmstr4AI i%a9POA.9Apbvre,v
SOU RCE AR SSSR. Dok*lady' V.~ 159, nt).-60 1964, 1272-1175
rorlC UOS: artificial saaellltef-magqo~tlpme.ter posit,ive ion" geomag-
netic field, magnetootphervA. i-adiation belt. flu),, inttneityj
negative
ton, theivratical flaj~di ajot~841*.difstznce
AB$TkACT'- The artifi-aial tontellite "Electron-2, equipped with maltne
n-d - T-- -ionit of
--tatitttftj~ -A a--trap - rt*tv- -d positive
all energie3b their ILuxesi witb eacr3ias of norit thark 100 evi and
all three ctimptInnn-ts of thii geomagnatio, field in th,a r-lagneto-
sphere an4 at radistl.on biilts. Reenided data showed a corritlation
between 1:1,e variatlom) of -'#,be magnailc activity on the tarrestrIal
112

L: 23291-65
A4XI:SSIOff .11; P. iAP5001286
surface aind the Intenvittiii-of --positive- -tons -and the-magnetic
fj'.el.d far from tho earth, This corrolation was observioid on quiet
days
zind on days vith -nagnetic disturbantoo. Humorous negative ion fluxes
vere recorded,on vlaf;nttically quiet d;y During this time, the Magna-
,,Pa.
tomoter Tecorded a viaf,netlc field of' r,jgular Intensity although
Itt
eacneded tht theorctical fieUby 20 -t. The ma)iinum duflection from
the thaoictteal field was dettictod oil. the apogee of thit satellite.
On 12 February 1961j, sill nagnvtlcobi~~irvatories on the eartb
recordcd
while the trap in the
114tis'll I te 'recorded -1somitive Ion fitlittlo excusively 0all
Intotlatty
of 4-10-10, jLt tills ~tdvlz the, sat-bllite was at svo:gee. The
nagae-
t-oin-oteT. zatorded j~ In -the magtietic fIeLd. Orl.g. art.
hasov 4 ti-guress (EGI
M S C I A TILON
915B1141 TTS 0: 15Sel)64 ENCL: 00 S118 ("OnEt r-5 S v
110 RE FS QV 003 OUERt 008 ATD PRES�: 31*73
212
crc
c

GRINGAUZ, K.I.; DOLG-~~01!jjbjft.j EEZRUKIKH, V.V.;
YETIOSHIM, Ye.G.;
ZHUZGOV, L.N.; MISATOT, L.S.1 SOLOMATRIA, E.K.1
FASTOVSKIT, U.V.
Relation between magnetic field variation ani
fluxes of positive
ions within the uirth's magnetosphere as observed
with the aid
of an Electron-2 ;satellite. DAL PV SSSR 1Y)
no.6tl.n2-1275
D 164 (MMA 1811)
1. Predstavleno Wcademikom A.L. lUntsem.

L 2885-!'36 TT/C;S/GW
;),CCESSION NR: AT50236W U.1/000016.5/000/OCO/0336/0341
I f, ;
inov. Sh. Sh V.
4A.MHOR: GringauzL!~,.-,T.'; ~AL .,,Betrukikh. V.-, Ye-oahetiko,
Z~ 6t
1L.; fjqgq~-qv, -K.; Fastovskiv.-U~ V.
JITLE: Comparison of w'.a-ultatteous measurements of mapa~~kq p
J~I!U' and o.91tive ion
!flux within the Earth's magrecosphere recorded by the Elektron--2
satellite
!SOURCE: Veesoyuzu.%vq konfer t~LtyAj~o fizike
koamichesko&~~-PTS~9.~""tva. MloscOlIft"..-
1965. Irtiledovani3ra kosvicheskci&o prostranstva (Space res,earch);
trudy kc,nferentsii,
iMDSCOW, Izd-vo Naulta, 15165, 33f-341
ITDPIC TACS: space envil'DURC11to tonosphliric physics,
elec1'"q__dgnjjj.tY% Ion density,
!earth misignetic field/Eleilrtrou I satellite
iABSTRACT: Measureatents of ctiatrged-particle flux and magnetic
field at a height of
6-11.6 R (R, Earth's raidlas) ivere made by BLektxnnr.Z.\?'-Tbe
particle._ trap used wng
ic-spable o1 recording posi-ItLve ton flux with ion energy in excess
of tbie-pA-ential
Idifferenco of the satell,'J.tom w'i(:h respect: to its environment
and electron flux with
electron energy in exceiv of 100 ev. The m~nnqqmeter,Vwith
orthogonally arranged
sensors, sras capable of measurlzg the magnetic ficid-In'tho range
)f +120 x 10- or&
l

2885-66
ACCXSSION NR: AT5023603
in each-ciYaponent dirtiction. Its~:thrtffihold vas 2 x 10-S erg.
The satellite meet-
ureimnts, when conq)areid wit1h tola-~ activity data In the fom
of KP Indexes recorded
via ground observatorles, eluw int:onsiatencies in the
correlation bet-veen the vari-~
ation of magnetic activity on the! Aarth's surface and the
variation o[ the geomag-
netic field intensity and therged ~particle flux as measured by
the satellite.' It
,Is uncertain thether these observ,,tlona caa be explained by the
solar wind penetrating
the twignetosphere or by near-earth, plasma due to charged
parti,-,les accalerated" by a'.
yet unknown mechanisto. Orlij. art.' has: 6 figures. [BDI
ASSMATIMN nona
SUBMIMD: 025ep(6 ENCL: 00 SUB CODE: HSI IV
wo REP Sm. 003 OTHERt 008
ATD PRESSjqW
JIr
I

L 2a in (d /M (h
i Fs~.~2A:vrrm/mv)_~vtFx/F OVIG S I
ACCESSION `NR: AT502*31504 t~OOD/000/0342/0356
01~
AUTHOR: Dolginov, Sh,. Sh.o. !1eroshnk2j_Y.!. Zhur, ov
TI TbE: Investigation of the earth's n!gnetosp erel;~ in the
radiation beli: '~'z'one
In rebruary-April 1964
_M j6RAP kosmichesk go pr2pIrnAtya. Moscow$
SOURCE: Vsesp),uznayi~ konferitntsir
1965. Iss~3Td_oia_m1y-a k_6s_'if_c6~z1Gj_o prostranatva
(Space research).; icrudy i:'onfervnt-qi1.
Moscow, 12;d-vo Nauka, 1965, 342-356
TOPIC TAGS: geomagnetic field, ge-*agnetism, magnetic storm,
artificial earth sat-
ellite, radiation belt, satellite -Jata analysis
-ABSTRACT: The authors give et detiLtled report an the
"Elektron-2" \i satellite inchud-
Ing orbital infortmation and tolemD-tercd observations In the
region of the outer ra-
diation belt at distanc S of 3-0,, Hapetonietric measurements
indicate that there
is an outer magnetic fi:la &u,ing -he calm of the day
associnted with the protoris
and electrons of the radiation bel%s. This conclusion Is made
on tbe basis of C:cTr,-
paratively limited vbaervatloTi t1rot. rurther observations
by thD "Elektron-4" at
other orbital. p:osltlons with vespoot to the line between
the sun and the earth
Card 1/2

-L 1285-46
'/,CCESSION 11R: AT5023604
ishould gEve more definite ink"w'Jon on the extent to which the
observed effects
Tray be attributed to the railial-imi zone. Peculiarities observed
In the dynamics of
tile mallnetospherm far from tile bomdary zone, and offecta
obeierved during polar.
stoms my be connected with the irystarious mec)anism responvible
for magiletic
'Stoms. "The authars considor it thEtir pleasant duty to thank
those who ussisted In
,analyzing the materials durAng pniparation and i.-onduction of
the experiment." OrLg
iart. has: 9 figtuvs.
ASSMIATION: none
ISOBMITTED.- 02SeP65 ENCLt 00 SUB CODE1 ES15V
INO REr sov: oio OTHER: 025 AV PRIM:
A,
1 Card t2h,

L 2992-66 FSS-2/0"WT (1)/F31,'v) -3/]'CC/FWA (d) TT/GS/'GW
ACCESSION NR: AT51:e3643 UR/0000/651000/000/06OW614
AurdOR: DoW.11 761
I..; T min.A., inchevio, M.-
Ch___
TITLE. Experirv=to; in the vorld mttgrietic survey program
kVseeoY-uznga, kcnferenbti~ji c
SOURCZ: A _anaj~yq 4o owi,
_1~~.qzike kosmicheakojp,p
1265. isa-e&"*i~i.,.,4 k-o'-B'-MC~iiiVigo'-pi-ostr'an.s'tv~a _Np t r
Adp-ac'e reaearch,,; trudy konfe:-entaii.
Moscow, Izd-vo WaWta, 196~5, 06-6114
TOPIC TAG13: geome4 1pietic fteld, geomagnetism, secular magnetic
field, sticular
magnetic variation, artlfi~lkl i!azl.h satellite, aeromagnetometer,
pmtor, magnetom-i
eter, EK4 M=j&MjjftU% 11 5 mgmAometer
T116 10 1,4,
ABSTRACT: A briefs review is given of the various attempts to
obtain a world-
wide magnetic-flell,11 map. The wie of artificial earth satellites
to map the
1q_LnpSnetic field Is shown to be! the most efficient of the
various methods
'Jused'.7 For optinum efficioncy in a single experiment, a
sabellite must have W1
orbit inclined -bo the 'e4uatorle~L plarie by 85', as had several
of the Cosmos series,
The low-number 7,oamos BerRea 63-jeh jvLA_qtM.:g�)rcsrried proton
magnetoneters
aboard, which e;3semtially meastree the frequency%%f proton-f'ree
precession in i0he
earth's magneti2 4.1,eld. The diiiaammitages of this type of
magnetometer were
Card 1/2

L 2992-;66
ACCESSION NR. 105D23643
alleviated in the later Wows ser-Wo (Oosmos-49) by uning
self-tuning mapetomete6
vith logic circuita. One such dt!vi(,.4!, c .;~atlelpm-4,
automatina.11y se:Lects and
analyzes the optimum &i[pnal dtiring w part of the free nucl
ear precession period
of the proton. TV) sucIll deilcaii on Connos-119, set 90'
apart, had a measurewnt
accuracy of 2--3 gaiiso. Ms4petl c field wasurements vere
taxen by both the COSMOS-26
imd -49 vehicles al', altitudes of 2'rO.-40:1 km and 2To-490
km respectively, during
Harch and October :).f 1964. Typical inagnetograw from these
meastrements axe shoien
separately,. Recomenndations aro madj! for further scientific
investigatiens vith.
magnetic-field chai.,4~s to better dete:rmine the earth's
geomagnetit field End to
Correct the coefilitkiente of the Gausnian series. brig. &A.
has: 4 figtres. (041
ISSOCIMON: VP-T;,-so-.truzntVi% konferentoiya po rizike
Moscow (All-Uhton !N)nference qn..gp
Ace Phy q
BUBNITTZ D: 028ej.)6!i ENCII.- 00
NO R" BOV. 005
()TM: 004
kosmicheiskogo prostranistva,
SUB CODE: FSISY
ATD PRMS:0
Card-?1?.hA4

L 02976-67
Ew-r(l) /.-:s s.2/Fcc T-..P/,,,w
SOLMICE C'011---- : -uli/(,-,O--O/*-t')6,'17,)/003/05T4/0577
AUTHOR: Dolginov, Sh. 13h.; Yeroshenko, Ye. G.; Zhuze9v
ush~~.)y, i.., V..
ORG: Institute of Terrestrial MHnetism, Ionosphere. and
FadicwRve Ilropagation, 'L
Academy of Scien ff',T) i ( I n s Tt- u t -,--e n -n c I ~ 5
-:-110 j -ji I Ii-f'j'r r) I- '-r Aj p r -cs i c n I a
radiovoln Akademil naWE'SSSR)
TITLE: Measurement of the mapetic field in the vicinity of the
moon by the Luna-10-
artificial satellite
SOURCE: AN SSSR. Doklacty, v. 17D, no. 1966, 574-577
TOPIC TAGS: magnetic V 'eld, lunar orbit., lunar satellite P
tvAtogoe- FA'VioCdA//r.,P..-/r.
.- niq 6w c r, dir~fE'Lo
ABSTRACT, The magnetic field i tensity in the vicinity of the
mc,on was measured by
a three-component magnetomete tarried on Luna-10. The
magnetometer measurement
range and its threshold of sensitivity in each direction were 50
-Y (1 y - 10-5 Oe)
and 1 y, respectively. During the lunar orbital flight the
satellite rotated
around a given axis. The magnetic field components parallel (TI,
) and perpendicular
(TjL) to this axis were measured. The absolute and relative
errors in measurirg the
resultant magnetic fieldwere-estinated to be '10 y and 15 y,
respectively. Dt;.ring
the observation period (3 April tc. 4 VAy 1966), the total
magnetic field and Its
components fluctuated in the follcwing ranges:T = 23-40 y, T11 =
18-38 y' ard
TL a 12-16 y. A correlation was established between vuriations
In T and T11
ard

-L 02976-67
ACt 14
and changes in the magnetic activity index. It was not possible ta
establish the
presence of a lunar dipole magnetic field or the Earth's
magnetos:pheric tail by
means of these direct observation methods. The most reliable
average value of Tj,
obtained was 15 y, which exceeds the Interplanetary value for the
name index cf
magnetic activity. It is hypothesized that the moon is
magnetical'.y permeable. The
authors express their gratitude to E. I. Magilovskly, V.
_N..,Orbidko,
Afanas~e and V. P. Li!j~k. Orig. art. has: 2 figures.
SUB CODE: 03/ SUBM DOS': 27jul66/ oRiG REF. G01/ OTH REF- 003/ ATD
PRIES:
5099
?/2

ACC NR: Ar7W)7600 Ct):):;: U!(/0293/66/00,14/006/OC.80/o899
AUTHOR: Zhuzgov, L. N.; Yoroshonko, Ye. G.
ORG., nona
TITU: IivcstIrra.-icm of the mapi,5tic .'iold from the
sentallIte '"Aina-1011
SOURCE:. I~o5mlchcakiyc issledovanlya, v. 4, ro. 6, 1966,
880-999
T0111C TIGS: lunnr satellIte, mignatic field, solar wInd /
Luna-jk
lunar satallite
SUB CON7: 22,03,20
ABSTIUCT:
change of -tho index of magnetic activLtty at the earth'a
zurfaco. The
error of the ab5oluto scalar value of tho 'it-,Id is
astLnatod at +10 -Y
Comparison of the zieasurod field valu:!:; In tlie region
of t.'-,a pc:,-.Lcc.,I*klcr
and apocenter and evaluation of possible distortions of Une
field by the
solar wiiid inCicaro t~aat the zo(:,n does not have a field
of a dipole
nature. '."hc author* di5cvss thitt pIob'.qui of
ujot'l-oz-, the obsorved C' old
can bo idantifiad with the of solar oriZin, (10-
i, formed or*trap?cd by a moon havin.- fiiilto
cond-activitq and
Compari:;-n of mcasuxi:zonts in perioda Of t-hG full and
now moom faUs to
inaicate a. dixact extent of the earth's za,-nutic field On
the niF)ittI-_o
side to Ustancos 60 R,_;;,.
InAls is a or. obsorwitions of -%-'a :mZnoIAc fiad of
;.-,Of-u ar
ncij~ribarhood of the i:oon mhoao intonsity durLr.Z o
time of obsorvations vai-led in the ranZa 24-40 y , in
agreezont
1 Card 1/7 j;,)n

ACC NRt APM17600'
The authors, th-,nl; Yu. V. Afanaslyevq 17. Lyulilt, and C. IN.
Alc!t-:;Oyova
for participati.-Z in thtb preparation of tho apparatus. Orig.
art:.. has.,
3 fo=ulaa, 12 figuras and I tabla. Lgas: 39,7161

DOLGINOV, Te.A.
Struature and origba of 4Turessic depressions In
the alpine
Caucantm, Sov,geol, 1 tio.11:88-105 N '58. (HIU
12:4)
1. Moskovskly gosubaretvemW univermitat Imeni
X-VoLomononovs.
(Caucitnue-Geology. Structural)

DDIGINDI..
-_.,
Host mobile sows In the CaucasuB. Izv, VY8. uchob,
zava,; geol.
razv. 1 no.12.-64-710 D 138. (MIA 1;1;12)
IsMoskovskly goisularstvonVT univervitet im. M.V.
Lory)nosOva.
(Caucasue-Goology, Struatural)

PIGIMOV. TO.A.
Peculiarity of tectonic boudInage in sedimentary strata.
lauch. dokl. vys. shkoly; geol.-geog. nauki nool,460-63 '58o
(MIRA 12:1)
I.Mookovskiy univorsitet. goologicheekly fakulltet, kaffidra
dinawl-
cheskor geologii. 0
(Geology, Structural) (Rocks, Sediventary)

DOIDINOT, Te.A.
Characteristics of faulting In the nres of the old
viclaus of the
Caucasus. 1xv. vys. uobeb. say.; geol. i ran-Y. 2
no.'?360-69 J1 '59
O(IU 130)
1. Maskovskly goundarstyenn" universitet.
(Caucasull--Yaults(Geology))

DOWINOV, Ye,, A., Carol of Geol- Hin Sci -- (dies) "The
Structure and. Genesis of
the Jurassic Depression in the Central Caucasus," Moscow,
1959, 23. pp, (Moscow
State University im M. V. Lamotmoov) W, 7-60, 10T)

AAI_At --.
.
Struetunil'pUn of the Greattr Claucasuse Vilste
Novh* 'imo
Sort Mole, 990yog geoleg pog, 14 noJilOSI-116
1511.
(mriu. Lli:6)
It Kafedra dinaffilaballWpologli Moskoymbp
univernittita,
(Caucasus.. Go ologys Structural)

I)OWINOV, TO.A..
Jbw,th coaf erence of po e t-grt. dun t q 8
tudents BrAl 70ung
scientists of Moscow State UnivereityO
Ts,,Vqrvn&ucheb*
zav.; pol.l raive- 2 no,IU128-136 N. 159o ,
-,. I . (KU 1.316)
(060100.)

-- DOLGINOV, Ye.A..
Block movements In tho mega-unticlinorium kernel of
the Greater
Caucasus in the Jurassl.ic. Vest.M*.un.Ser.4: Geol
15 no.li
3-10 160. (MIU 14:4)
1. Rafaira dinaideheskoy geologii Moskovskogo
universiteta.
(Caucawas-GetAogy, Structural)

BEIDV, A.Aj_.DOLGIN0V,--T*.k.j KROPACHEV, S.M-aj
ORLOVp R. Tu.; SOKOIDV, B.I.
--- ----------
Cherkeask-Ulaml laterpil disturbance of the atr-cture
of the
(Preater Gavcavus, :Czv. AN SSSR. Ser'. geol. 24
no.6124-32 Je 160.
.? (MIRA 14:4)
1. Hookovskiy gosudi !retvennyy universitet.
Waucasus-Gsol*, , Structural)
.0

.. v." f. .'I
UI)Ai.:; : ~ ~ o" i.;. ,, . ; '~'J 7-".. 1 ,I,'. ; , '~) -
phi, J-wq, vIth I ?:,, ~~2eanllrg vesEelso
it! 'i- - infoi-m.Ser.1.1a a hinostroi.
n:).4",-8 162, (MIRA 1828)

BELYAWPUNA, M.N.; DOLGINOV, Yedi.
Genesis and the structiural, position of granites in the
northwestern part
of the Yenisey Range. Vest. Mosk. un. Ser. 41 Geol. 18
no.6:5~-68 N-D
163. (MIRA 18:7)
1. Kafedra diamichoskoy geologli Hoskovskogo universiteta.

DOLGINOV, Yo.As
Chnracteriatica of 1,be develorce-it of the
Sayan-Yinincy fold area,
Vest.Mosk.un.Ser.4: Geol. 19 no.5tlO-16 S-0 164.
(MIRA 17t:L2)
1. Kafedra dinamichookcy geologii Hoskovskogo
imiversil~eta.

1471'Y j".. I 'I-;. ~'. i~ , ; "A! I t li c 0:.!
6
~? . ''.. - 1 "I ;:, i '. * -,' ,
4.1 1-, -1. !,r-ur-t!j r;~,.-. Ir. jit,r t '- vc.". , -
-:, I , - , . I -,
"t! r, 1 0, 1 i)~ -:~ !" - 1~ ;
k
. no."t-i7-31
1. 1 - " r, i : , -,, ~ 1'.

inz.~.j RODOV, S.H., Lath.
--R i
I-klhoda of auppor.ing inclAnod conveying gidlarisi3.
Prom. strot.
42 nf).1007-38 0 164. (MIRA 1,7111)
1. Dn9pr3patrovskly Mi4l Gosudarstvennogo inatituta po
proyektAro-
vanlyu, issledovardyu J. iupy-.&nl)ra stalinykh
konstr-,iktsiy, i moaL:,v.

DOIBINO
-!'VAPI-M... kand.tc)Jin.nauk,, starLhly
prepodavatell; SYIBITSKIY,
11.p gruppovoy in2bener-konstruktor
Polyethylene is a gool substitute for nonferrous
metals. Mor.
flot 23 no. 12:29-31 D 163. (MIRA 17:5)
1. Sudoremontnyy ravod !.meni Parzhakoy Kommuny
(for Skibitskiy).

DOLGP~I)VA, M.Ye.,Cnrid 1'ech Sci --
(dis3) "Intem3ification
of the combustion of natural gas in the
smeltitir, furtiace.11
Baku, 1958, 16 p:) with ~Oc'&.'t'2" (1,11v
of Htrlier P, Ucation
U&SH. Azerbaydzhan order of' Labor tied
Hanner Ind,.istrial
Inst im IA. Azizt~ekov) 150 coples (FL,
?Y-118, 106)
- 97 -

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J-0-9 at? 9.
an
op.
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to ~v a
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tit za!sr .41cm 0--a, "T."S 1 20
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Poi'd :ruzz
IWORZCT

DOLGIROVA. H.Te.; AIMS1117HO, P-H-
Cupola furmace using natural gas* Gaseprome 4
no.901-35
S '59. (Yurnikess) (Gas, Natural) (MIRA 12M)

-18(2,5) SOY I Z'8-59-9-5/25
AUTHOR: Dolginoira, M.Ye.. Candidate of Technical Sciences and
Engineer
TITLE:
Industrial Practice in iron MeltinE; with the Use of

,Nat,ural GRE
PERIODICAL:
PP 16-18 tUSS11)
Liteynoye proizvodstvo
Ur 9
1959

,
,
,
ABSTRACT:
In the cour,~;e of 1957-1958, the Bak-u
liachine-juildIng

Plant inieni X.Montiny the &ishlinskiy
Machine-Buil-

dina Plant, and the 6hip-building Ylant imen~
P--,rIz~,skaya

F-cmim;1aa intzoduced the method Of iron Melting
with

the use of' natural cras as foel. i~.t the present time,

thfire are eight Iron-mell(ing cupolas working on natu-

ral. gas
in. operation. 1he heat value of natural gas

varies from 800 3 to
8700 calories. is Is seen from

"
'
figure 1, the temperatures attained at burni J,-

e mi-
(fh
natural gas are sufficient for iron melting
'

The
ninium requizec. temperatures 5U0" 550

gerieral furnace
construction is given in --igure A

special burnDr to be used with
the furnace Is given in

Yigure :3; it is provided. with two
channels for mixing
Card 1/2
natural gas and air inside the
burner. ii-Ile required

SOV . 128-59-9-5/.25
Industrial Practice In Iron Melting with the Uae of ~Iatural
Gas
ji.1,aB-air ratio is 1. to 10. The o-ptinum speed of the
gas-a-ir mixture outlet is 35-40 In/SE10. Ttie required
air pressure amounts to 500-1100 mm of water column.
'j:he natitral gas consumption having Ain average heat
,ralue of 8400 calories is '100-110 11, the correspon-
ding air consumption is 1000-1100m per ton of char-
ge. .1~'xperience has shown that cust iron melted In a
as cupola possesses better mechanical properties
han ithen produced in a coke furnace. The simpleness
t
of ga,; furnaces construction enables their building
sit a r.-ouipa:ratively low cost. 1hore are ' graph, 2
tables amd 2 diagrams.
Card 2/2

DOILINOVA, Me,.
Fla r, t .'c lialve'.1. lzv. vvs. w+eb. i nef' I
I cta- 6 n-~.",.-
120-L?3 '63. (14i R;~ 1,7.- 81
1. Azerhi.ydzhanskiy r~`tl ~ vl-

S/203/61/001/005/003/028
A006/A101
AUTHOR: Dolginova. Yu.N.
TITLE: Determining the degrait of polarization or the solar
corona from ob-
servationc made durl:rLS the solar eclipse on June 30, 1954
PERIODICAL: Geomagnet:[.zm iteronomiya, v. 1, no. 5, ig6i, 646 -
649
TEXT: The author attempts to determine polarization of solar
corona at dis-
tances from 1.5 - 7 It 0 from the center of the solar disk. Data
are used which
the author has gatheretl during thei solar eclipse on June 30,
1954. (NIZMIR expe-
dition to the Kozelets village, 7!j km from Kiyev). Photographs
of the corona
were taken with a three-objoctive? camera with polaroldes,
producing pictures oi'
the corona at 3 positiDna of the polaroids, Photometry was made
in N - S, W - E
directions, The degree of polaritation nnd the position of its
plane were deter-
mined by D.A. Rozhkovf;kiyls graphical method (Ref. 6. D.A.
11ozhkovskiy, Astron.
tsirkulyar, 1956, no. 166, 13) ba.sed on V.0, Fesenkov's
formulae (Ref. 7: V.G.
Fesenkov, Astron. sh., 1956, v. 588). Such graphic
determinations were made
everyyO.2_5 R 0 withlin a range of 1.5 - 3.0 R o from the disk
center and every
0.5 R E) at larger distances. Ecperimental and theoretical
polarization curves
Card 1/2

S/203/61/'001/005/003/'028
Determining the degree A006/A101
are close for the polar direction,trat differ for the
equatorial direction. Polari
zation in the latter direction depemils apparently more on the
corona shape. Data
on polarization angle OL-(in degrees) are tabulated and
illustrated. To estimate
errors in the values obtained, relative errors of,4 p/p were
determined for dif-
ferent distances from Vie disk center in several directions,
and absolute errors
for the polarization anillecx. For distances of 3.0 and 4.0 R a
from the disk
center,ff~ p/p was equal to 15 and 615% respectively; for 5 R 0
the error exceeded
1OC16. For both mand p values the ~YW direction proved to be
the poorest, as shown
In tabulated data of anj:les 01, . On the whole the
determination of angles OL is
accompanied by greatet vrrors than deterinination of p. This
may be due to Inac-
curate accounting for dispersed lig:rit, Inaccurate orientation
of polarolds ancb not
sufficiently precise determination of position angles of
photometric sections, con-
nected with the small scale or the -:orona image. We author
thanks G.M. Nikol'skiy.
There are 4 figures, 2 tables and 9 references: 6 Soviet-bloc
and 3 non-Soviet-
bloc.
ASSOCIATION: Institut zemnogo magnetizma, ionoafery and
rasprostraneniya radiovoln
AN SSSR (Institute of E,arth Magnetism, Ionosphere and
Propagation of
Radiowaves, AS USSR)
SUEMITTED: July 29, 1c,151
Card 2/2

TTa
S/214,/62/000/006/001/001
D207/U308
MTHORS: Akin0yaa,'S.T. and Dol inova Yu.11.
TITLE: Chromosph,6ric f Lam, s and radio bursts of 1U tyj~pe on
July 121' ~nd 18t 1961.
P-MIODICAL: Solnechnyye darmyye, no. 6, 1962, 61-65
TaXT: Radio tole scope tj at UJURM recorded on July 1.2 and
181, 1961 two sti.,oiig radio bursts of 1U type frcclucticie's of
208 and
.545 Mc/s. Thes-i,: bursts accoraparLied chromospheric fl-ares of
5+ magni-
tude-which occurred on the same days and were recorded at the Qbser-
vat-Dry of GAD AN US,11:R ands, at I'MfIlUal. m analysis, of these
bursts
led to the folloitirq,1 conclusions, in full agreemcrLt uJith the
-or',!.
published carlier: (1) I!he inmrimma of the tFirst stage of the
radlio
bursts of V type if) clotle in timc; to the maxitmit-it of the
flai~e bright-
ness; (2) The begiming ~Ibf Out coco-nd ntarfe of the Wr6ts ort
July 12
ith thei vaomeni; of C,cctioti of an eruptive f Ailaracilt in the
Coincided w
region of the flare; (5) The ejection and collapse of a filame"It on
July' 18 precadtd the mx~mum, Nvightn(iss of the flcirc, uhich may
have
Card 1/2.

S/214/62/00,D/006/001/001
Chromospheric f larefl ... D207/D3O8
been due to Cac unsharp Olvision betwen the firnt and sccozid
stagcs
of the radio A-claowledgmei-tto are made to Doctcr F. Ftrstcn-
barg.from the h2inrich Ifortz In.,ititute for supplying the
records of
some radio bursts, and to rtaff imembers of GAO 'a-l U36il L.A.
Gvxto-
venko ard V.V. Orlova for the supply of the records of the July 12
flare. There arc 2 figuras.
ASSCGIIVICIII: Institut zennogo magnetizma, ionosifery i
resprostran-,
iya rndiO'%tDln LIVIl SSSR (Inatituto for Terrestrial
Magnetion, lonouphere and Radiowave 1ropagation, "S
USSIO

ACC NR:
AR7000BOG SOURCE CODE: U11/0058AG/000/000/1104301043
AUTHOR: Akinlyan, S. T. ; Dctlg'Lr~qya,. Xy,.,N.
TITLE: Relationship of large chromospheric flares to type IV solar
radio
emission bursts
SOURCE: Ref. zh. Fizika, Abs. 9Zh313
REF SOURCE: Sb. Solnechn. aktivnost'. No. 2. M., Nauka, 11165,
183-198
TOPIC TAGS: solar radio emission, chromospherqi flare, radio
emission,
geomagnetic disturbance, solar flare
ABSTRACT: A study is made Df the correlation between strong
chromospheric
flares (class '> 2) and type-IV solar radio emission bursts and
geomagnetic
disturbances. An analysis is made of data obtained during the K"XY
1958-1961 by
participating observatories (a total of 20 flares with accompanying
type-IV bursts
and geomagnetic disturbances). A correlation was noted between the
behavior of
the photometric curve of chrornwtospheric flare intensity and that
of the first stage
of type-IV bursts (bursts in the region of centimeter waves). The
second stage of
C.,d 1 / 2

ACC NR, AR7000896
type-IV radio emission bursts accurs within the decimeter- and
rneter-wave range
and after the chromatospheric flare maximum, coinciding with the
initial stage of
the accompanying burst. The irelDCity of the source in the corona
during the second
stage of the burst is r%--l 1000 km/sec. This velocity
corresponds to the velocity of
corpuscular streams within the! rmige of -the Earth's effect. The
determining factor!
in the magnitude of the geomagnetic disturbance is not the class
of the flCrXe but the
intensity of the second stage of the burst. The greatest
magnitude in the second
stage of the burst is produced by chromalospheric flares with a
heliographic
longitude of t 40% N. Soboleir. [Translation of abstract) [SPI
SUB CODE: 03
.AY

I* -) lit
L
HAKHINTA, P.M., inshener; D(TAINOVEROV. P.P.
Transporting lime-grpsum solutions with pumps (without gyprum
hArdening
retarders). Biul.strol.tekh. 10 no.11:1) Je '5). (MtRA 6:8)
1. Ukrainskiy fili&I Byuro tekhnichookoy pomoshchi stroltel'stvu
Minister-
stva stroitel'stva. (Plastering)