SCIENTIFIC ABSTRACT FR:MOGILEVSKIY, G.V. TO:MOGILEVSKIY, E.I.

• Document Type: CREST
• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R001134900036-6
• Release Decision: RIF
• Original Classification: U
• Document Page Count: 99
• Document Creation Date: November 2, 2016
• Sequence Number: 36
• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTR

The Use oi' the Theory of Similarity in the Design of &let~tro~~Ma~~ets
magnetisation curves of the steels should hots. he ;~~.~
same, (It is this part off' the article that is r~air~l.~J
oriticised in the editorial note) ~ The main j.,mlar 3.t~ti�
relationship bet~~reen taro el~ectro��magnets fihat; a~~e
geometrioslly sit~ilar are tb~en givene The. a~tY~U~r c:.cnw
siders in. tarn and girres fc:~�mulae for ~ th~3 wsl.ationshig
b�tween the ampere tarns of the coils � t�,he x a.i..a ticn.ship
betty��n the txact~.ve efforts; the re~.atinnshi~- between
tho aopp�r losses ~.r: the ca,ils; a�.d the ~~elat j_,3s~s~~.ip
b�twe�~ the temp�rat:ur� rislas in the coils, The fa~;t that
the temperature r~.ses are in the ratio of t;ha co;nstan+, of
prop�rtion~lity9 as will b� ss;sn from Fq (5) ~ ~.s cr~e of
the a~aia difficulties in acing the theory oi' sj.m:i.laY ity~
for the d�slgn of eler.~tro m~~gnets, for if e~r~e of the
asagnets is of corr+ewt temperature ri..~e the other will.
either be too hot or wasteful of materials ~ T,:,� +:bt:~in the
uptimu~ design it is necess~~ry to vary thn dime~n;~ions of
the coils and magnetic syst~,~~m9 and scrordingly se~.peral.
variants ,must be designed, A further diffi.c~.~lty is tha*
Card 2/4 the magnetic induct:i,on rema:tns the same irrespec.ti~?e u~'
the di~aens:tons of the magnsi: and the magni~~uds r;f the
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lU'P~iOfl: Mogilevs]ciy, G.Y. (Candidate f Technical ~~ 23
1'ITLB: ~`~'i~ eory of ~~itnilarity in the Desitgnsof
&tectro~l~4agnets (Primenenj,ye teorii podobiy-a
proyektirovaniyu ele~tromsgnitov)
PBSIODIC~tL: vestn~.b: Elektropromyshlennoa ti p 1959 y Nr 4, PP 34..36 USA 1
l1BSTRACT: ~n �ditorial note ,states that the articl t x
the t'ull.est possible use of the theory of sirnilarit~~Por
the design og electro magnets but nevertheless it is of
int�rest both as an exaffipls of application of the theory
of similarity to the desig� of apparatus and a,s offering
a practie~sl design procedu7re d I~xisting methods of
desigr~.ing electro IIIagA~tg tyre empirical, indirect,
inaceuratl� and laboriou.~, improved design procedures are
ffiuah need~sde Th� theory oj? similarity can be a help to
rapid and accurate designit~; but its usefulness is .limited
by absence of experience oi' d�sign by this m�thc-d, by
certain inadequacies of the theory of similarity,. and by
the absence of systematic experimental data on d'.ifferent
t3iP8$ �f electro-magnets a It is stated that f+~r two
�lectro magnets to 'be similar they must be g�otnetrically
Card 1/4 similar and the physical constants of trio magnets must
the seats a,t corresponding positions and ir. par~~icu1.$r the
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Calculatioa~c of Con#m,~t Bouac a
SOV/14~-gq-2�14/19
contact ep~ring.
19ecauee o:� the simplifying assumptions adopted this
+~PP~'oximate m�thod of calculation gives high values. In
+~ more correct treatment it would be necessary to allow
for the in~~luence of the el,~sticity of the material from
which the e;ontacts a,re roads.
There are �i figures and 5 Soviet references.
A~SOCIATIONs Kafedrn- teoreticheskikh asnov elektrotekhniki, ____
Tomskiy pul,itekhnicheekiy ix~.stitut (Chair of Theoretical
~`undamental.e of Electrical ~~ngineering, Tomsk polytechnical
-~__._
SUBMITTED: January 12, 199
Card 4j4
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~aalculationa of Contract bounce
r
~~
,~
soV/1~t~t~59-~2-14/'19
If the in3.tia1 pressure is low or the initial velocity
small, t~tis formula can be considerably simplifi.ec~l to
the form of X11). It is found that the first rebound
occupies 7'~q~ of the total ~-ibration time.
The s ecoxtd; case fe then considered, where the contact-
holder si-e~ed is maintained after impact . In the a.nt erv: l
between t.w~o successive imp~~cts, motion of the contact-
holder increases the spring; compression. This reduces t:l.~
amplitudes of the rebbound butt increaee~s the speed before L
impact, anal motion o:f the contact after impact is de$critle~i _
by Eq (13). The solution to this equation is given by
expression (14) and typical. displacement curves are ~:~lottl~d
in Figure j. The total tlmle of vibration may be detEsr-
mined from Eqs (16), (17), (18) and (lg). C,raphs of
the duration of vib~~Ation a.re plotted in Figures ~t and 5.
It will be noticed that as the initial spring compression
is reduced the. vibr~stion time first increases and then
,remains practically constant. The graphs ahow'~that
erometimee 'the vibration tiro� aray be reduced by ~^edueing tl~e
Card 3/4 .initial coinpreeecion and increasing the rigidity of the
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sov/144~5g~2-x4/;i9
Calculatioxcs of Co~ai:act 13ounc e
~~ontacta b~lcause other kinder can be raduc ed in ~rious Kaye ,
C~al4u~tiv~~ of the vibration time is very diftic;ult and a
x~6umber of simplifying assum~~tions are made. In particul~-r,
to simpli#'y' the analysis twt- extr�m cases are considered:
the spe+~d o~f the c �ntact hoa.der bec~es z r
e o on impact; the
speed of the contact-holder is not altered on impact, In
most types. of equipments sucY- as contactors and x slays, ,
the second cafe is the ,Wore probable,
A~ diagram of an equivalent contact system is given in
Figur� 1. Inertia of the contact spring is either .._
neglected or added to that c-f the b~e.ll that represcnt:r tYie
moving c on.t ac t .
The case in which the contact holder is arrested is first
considered; motion of the contact after impact ig than
de8cribed by Eq {1). The sa~lution to this equation i~c
expresBed is the fora of Eq (Z}, and typical rebound g;ra~,h:~
for this cage are pl+~tted in. Figure ~. Expression are theta
derived for the vibration tim� of the contacts and t.hE> tot:~l
time after a number of reboundsl is given by expreasiora (~) ,.
Card 2/4
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y. ~ . ,~
3ov/i~~~-5~-~-14/~~
AUTHOR: .Mo~ii~ ~i . , Seaior ~,,ecturer,
TITLE a Caicu~ions of Conta~Housac e
..,_....
~'B~It~ICALs Iz+v'esti;ya vysshikh uchebnykh zavedeniy, Elektromekhanii:a,
2959, Nr 2, pp 11.1 - 11? (U83R)
I4TRACTs It is iatgo:rtattt to be able to calculate the vibration of
:new dasfac of contact. The vibration may be aa~sessed in
'terl~ of ~tl~-e amplitude of the first rebound or of the ti-~Es
.interval 'between the first and last eontaet$ ar of the
�total time for which the contacts alre ,separated., This
latter chaxact�ristic is the best as it correspt>nds to thel
total time for whicPa the arc burns and this is i:he main V
cause of contact damag�. _.
The vibrat~ton time may b� detextinined experimex~tE-lly with an
oscillogra~~h or �rtafn special instruments. The du.~ation
of vibration deperda on man;Y factors, including the current
value, for if the Gnxrent ils high the material j.s softened.
and the rebound is reduced. It is therefore beElt to make
i;he calculal:ioas or r~easurem~ent$ without current in the
circuit or with a small cur~~ent. The only type of vibration
Cardl/4 t:onsidersd ig the bounce ca~xsed by impact betxeen the
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s-s
The Design of the -~;hort Circuit�d ~'z~ ~ '~OV/144-~~~-1�-1;/1~
Voltage Coil on ~lE,ctro-~~iagn,~-ts wit~Y
screen design is given ix~ an appendiao r~hez~e are
8 figures and 6 Soviet references
ASSOCIATION:K,afedxr~..~lektric~eskikh Apparatov Khar'kovsko 0
Politek~~r~icheskog~~ Insti~uta (Chair of Llectr:icg~,1
~~~~bo~~�~~eix Y} yy ethnical Institute )
~ `~~n-~,Y elertriae~,obee
a~-v~od (1Cbar kov Eleatil~,ica1 Plat ~ ~ , , lciY
3 ,. ~,Y~
SD~tITTED; 31st {ktc~b~er~ 1958
Card 6/6
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~:+~ ~ /1~~~~8~14--13f`l
The Desi~~n of the short Circuited ji'urn on .~lectro~-,Y~agnE3ts `vit;h
Volta e ;oil
a1a~aetic; system has threF: legs;, the short r.,:~rcuited
urns ~`i~e uf~ually instals,�d on the outejr lags :far 't~ette:.
cooling! though this givEls spra~e d~.fficult.e;; irz max:in~;
secure Fixings, because the outer legs a,re ~~m:311er in
cross-erection than the cs~ntral one}s, Various methods o:'
firing the screen 1.n the slot ara illustrated in F'i.g 5
i~en the equipment is rec~u.ired to have a ve:cy long life
the screens may be a weak; link ; the ms,i,n cause of
failure being fatigue stress�s ~ caused by repe~~,ted impa,ct~
of the m~gne tic systems To inCres.se the me ch~ulica~.
stz~ength of the Bcreeng besides using str�ng ~rtaterials
of adequ;gte size it is advisable fx,rmly to Secl.zre
overhang~i.ng parts of the screen and recommendF:d
procedur~ss are i1J.ustrate~i i.n Fig 6 and briefs y
de scribed ~ Springy; dampers are so~neti.me s used t o reduc+~
~paCt ~6~1t?C~CS, See Fig ?~ SOm+etl.Ines arrangements are
made to.eit the screen at a lace � ~~
p wnxcr ~.,, not subject
Card 5/6 to impacij shocks, s�e Fig 8 ~, A numerical example o;r"
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SOY/1~!~-10-13/I ~'
The Design of the Short Circuit�d 'iurn on ylectro -~1agn:ets xith
Voltage Coil
rise at ~ point in the turn including the maximum
temperature rise o In practice t}~e part of the turn that
is trot in steel may be made of increased section to
reduce the temperature rise, in this case the design
procedure is the same but certain correction factors
are int.~~oduced. When using the procedure for the
thermaal design of short circuite3. turns it is necessary
to l~o~w the appropriate heat transfer coefficients and
appropriate values are recomm�~x],ed for particular cases
Further pproblems in the pie $ign of short circuited ~tur~~ s
in magr~3tic systems conclern the material and sh
the tux~~, its location faa the ma etic ape of
method c~ f f ixin it t o t;~e ole � ~ ~ ste~i and �the
g p If the system only
works cx,casidnall.y and ~r:ithout shack the rind; may 'be
ms,de u~~ of sheet and may be made removab le ~ ~,�e ~'~, i~ ~~i ,.
If the .r~~ are cons ids ~ablEis shoc k~~ the ring mr~rg~t 1~ ;~:~ x~x1,;q
fi,~�$ :ixl the slot . Proposed methods of fixing are
deBCril~~d and illustrated in Fig 3b and c ~. In equ_i.pmen~t
where tie coil is pe rrnanE; ntly fixed the screens ~U~ bE.
Card 4/6 used a:~ a firing device Fps shown ~.n Fig ~+., When the
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.~ (3V / 144- 5cs- --1 x)-13 / 1
The Desi~~ of the Short Circ~xited T~;,rn on Electro--~~agnet,s ~rit~k
Yoltag~e Coil
tempe~~ature rie 9 of the ring can be 200 to 2~0�C
Unl�ss care is taken the heat gene rated in the rin�;
may dat~agre neighbouring insulation. Practical methods
of constructing t:~.e shorn circuited turns on magnetic
systemic may be cL~seif ied. into t~vo kends as illustrated
in Fig 1; in one case t~,e screen is located :in a ~~lot
in the steel and in the ether case part of the rind; is
in air round the outside of the steel. In considering;
the temperatur� distribution in the ring it is
convenient to consider separately the parts that az~ in
contact' with ete�:1 only acid those that are in cont~~.ct
with air as well. A gra~~h representing the tampera.tur~e
distribution in ties short circuited turn is shov~n x.n
Fig 2 and formulae for tb.e temperature rises in the two
sections az~ given in ~q (12) . Actual values of
temperatu~r� rise are Somewhat less in air and higher in
et�~1 tban the vaaueg given by ~q {l2) and the extent off'
the arroz� is next determined. As a re$ult Eq (15) are
Card 3/6 derived, that cau be used to determine the tem~~erature
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SOV/144-5S-1G-13/`17
~ Design of the Short Circuited Ti.trn, on Electro-1~a~et~s witlx
goltage coil
+especl~ively. mhe formulae are valid provided that
the iron in the magnetic system is not saturated but
becausEa of the screening action of the shore, circu:~ted
turn the magnetic induct:lon in the unscreened part of
the pole is considerably increased. This effect may be
big enough to make th� ft~ruzulaa inapplicable . However
it is shown that with an E-shaped core the f~b.ort ~
circuited turns are usually placed on the outer poles
and bec;auae of the phaBe displacement betareen flutes the
instant; at which the force on the outer poles is a
mian.imun~ does not coincid~- with that at whic~- the ft-rce
in the middle pole is zero, therefore, the minimum force
is greater than it otherquise would be and s~>ecially
accurate analytical calctiilation of it i s not; .nece s~iary .
E~perin~ental verification of the electrical d~asign of a
short crircuit�d turn on a~ relay type R~-~210C1 show�d that
the calculation was euffi.cientl accurate . La order fo~~
the ma~setic system to wc-rk well, allowance m~~zst be
mad� for change in the re~sistanee of the ring due to
Gard 2/6 heating, which is very necessar~r as in some cases the
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y
AUTH4R$; 1~ubc~iik Y.,~., ~.,ecturer; 1� SOV/14~.-wi8-10-13/1;
of T�ebra~cal 8cienees and ~~~~~~-' G�Y,,, Cidate
TITS: y~~~, Engi;cZee:r
The ])ea;ig~, of the Short C;ircuat�~;
Magnets with Voltage Coil (Proyei-tiani ~ h~c~tro- ,
g vitka, elektrcrmagaito~~ �kgtu~go ~~' rotko,zaml~nu-
P.~RI~ICAJL:Izvesti;~a Vye ehi~. Uchebn~~kh ~, ~' px~r,~$~heniy~~)
1958, Nr. 10, pp 135-145 (~T88R) vedeniy~ B1ek~r~omelc~ini~ra,
TNACT. ~~ ale--phase a.c. �lecl-ro-~,gnets short c~~rc '
a~:~ located on the ends of the u~.ted
magnetic system, as shown in Fig 1, tooreduc~?variation
in the tcractive force . Because the turn is t~h,, re the $
variable force that acts c~n the armature is al~~a,y,s more
than a certain minimum value which, to avoid v:tbratio
should. always be greater than the combined forres du n
the spring and, the weight of the armature , E lE: ct ri ca t o
design of the short; circuited turn consists in determl '
its active resistaxlce and the power lose in l l.nln.g
~.'re~.ous,ly published d�sign procedures are briefl
Caz~d 1/6 calculat:Lo ~q (~) ar~d (?) ~~re then derived for y
n of the taro re,aistsnCe and power loss
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MOQrILEl-~B~~y a�l� ~ ~h� i TAl~ia)PA~,'BKIY,~ M.D., inzh.
Conetraatic~n �! the c~vr~ring of i~hs machin� room of a
tharmetl �1e-atric po~r~r ~~lent. gle~k, sta, 3S no. 5:28-2 },fir ~ (~,.
t 17: s)
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PROVED FOR RELEAS~�~,;,.A6/23/9 9
~'3tudy o.P t~tture at gas
ita drilling and gas to&gin~
:~4 no.2 :46-168 , Ap-Je ~ 60
CIA-R~P86-0059 38009 9 34900036-6
and ba~~teria nna~].ies dccardi-r:{~
data. Analele=
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PROVED FORE E-a4 E: -06/~3~L1.~.~ R~OQ,a59_3,F20~~9 ~ 4900036-6
~ 1~tFU 154
8~i ~~ aaachpc~=i,e~ledaral~el~skly in~titu~ y~darr~oy
g akhia~ii,.
{Osa ~-ll loggiz~g~
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PROVED FOR RELEASE: 06/23/9 9
NOGIL~~VSKIy, G.A,~
~teristiar of ~iiat dirtribatioa of sartural gases snd
~1s.~iltro~. ~` ~~ rose ~ a! gar a~ oiI fields. T~uldy
~.9:46-~b b1. (t~cR~ 15 ~ 5 )
1. ~tses~oyusnyy nauabno-irsl�d o'tratel ski
" y gAologorasve~d~~ahnyy
n�h,~ institut (vNZC~NZ) , r~l~skva.
(Gae, Nat~~]r-~tiarobialogy)
Pet'x'al~~obialogy)
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PR~~~b~i~~t'"'! eEtna�gnet~c~., ci,o,-~Ol/~ 0~~~~~t~,3t7~~$ooss-s
sions, were eli~inatrd by taking the mean conductivity of tt;-a ; ~ea,_
eu~tnente with fully conducting end fully insulated wal.l.s 4~ the
electrol.ytia: tanlt. ti figures. 5 references. ~~etrscter's note
Complete tr~a~nslation ,~

Card 2/2
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AUTi~i0R3 : Vaef l.'yev,
` TITHE: The evalu~-
cylinder -
the and of
3194 61/000%07/008/079
D201 305
V.G., V'lasov, F.M. and Mogilevslciy, G.~-.
Cion of the magnetic conductivity of the:
rectangular parallelepiped system with
an electrolytic bath
PERIODICAL: Refer~atfvnyy zh~u~tial. Avtomatika i radioelektroniis;a,
no. 7', 1961, 7, abstract 7 B38 ;1'r. Khar'kovsk, pc-li-
tekhtu. in-ta, 1960, 30, no. 1, 41-48)
TSXT: (3re~hs are given for evaluati~~ magnetic conductivity be~~
tw�en a reai:attgular parallelepiped end s cylinder at given georaetx~i-
cal dia~engicins. The graphs werE: taken ~ueing an electrolytic tank
with internAtl dinens~,ons 45 x 80 cm. T'he magma tic conclucti vity w~~s
det�rmfned i'rom the Qreasurementza of an electric conductivity ;~aral.le-
lsppaped between tao eaect~odQa, a cylfn~3er and a rectangular paral.-
lelspip�d rrl.th en a.c. potentie]. being applied to the electrodes.
The errors ~ltae to the field diei:ortion in ttu tank of fini to dimcn.-
.~
Card 1/2
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PROVED FOR RELEASE: 06/23/9 9 : C

thin tbi opts loggiz~ ~rosprating sott~od. Sav. geol. 3 n~.6:119-].2~3
~! r~+0.
~~IRA 1.3;11)
x� Tam" nanchno-i~~~.~dovatel~~l~iy gralagar~vedactu~ry neftyag-oy
inip ti tnti.
Oil well lagging)
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Geochemical Oil and Gaa krospecting Methods Spy.-~~;_~;{3_~,,.~~;~~~
use of radiametrzr and ,;eoahemical methods of c,.i 1 and. qsl~
proepe~^t~.ng in Rur~anza., A report by L Stegen,. ~Ifunt?ary),
was read on gas-surveying works; a.Yars~.l on the problem of
the adaptian Gf r~~idiLing hydrocarbon bacteria to how tez~..
per~~turee~n ~eo~h,}mical� microbio'~ogical and r~~dic~metrica!~l
methods ro be emliieyed ,.n the individual distr7,~:t;~ of tr~E~
USS;q ware apprG,ved at th� mE-"ting;n m}iese met'r,ad:~ muelt be
used in complex ;vaysy ss~pecially in Siberia Central A~~ir~
and the other new I~rpBpE!Cting areas :i.n ccnfor,~n~ty wi+.r~ �tie:ir
concrete geological conditions, It was suggested thslt a per-
mani3nt a~;ang interdepartmental s..ientific ani a;r,*%:ad.ca:
council be set up within the getup of A v15a f'cr a re .p _.
van~t theoretic~:i and practical questions
GeoPh+y + ca?_ prospect irg--USSR
Card 4/4
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Geochemiaal 011 and Gas Prospecting Me~thode ~'iV-25-`i8_9=%~S,'~d[
gae-analytical methods t>.nd deviceo (law-tempert:~tu:eY ^hrc~cn,~.-
tographic and others. The experience in gas ;surveying ~ln the
USSR was commented on b;r B.P. Yasenev' , Yu�Mr. 'turovs~:iy :spoke
on gae care eampl.ing by el�ctrical. meanaf Several rE~parts wer:~
concerned with gas eurvc~ying and geocherni.r.a~t prUC;~~ecc~n~; mt?-
thodrs in individual Sov:Le t regions: the ~'imano-~l'echvi a gss
and oil province, the Sc~ratov oil region, the ~;as de~;osi is of
Stavropol' and on the K~~la Peninsula. A;,A. Ceadekyan and
G.A. Mogilevskiy spoke un foreign gas and oil ~~rospectin,g re-
search and the geochemic;al and micro-biolagica~. methcda em-
ployed in the U~. Professor W. Schwarz (Shv~lri;s), East iJer~-
many~ reported on experitaental work on the basi.? ai the mlcrc~-
biological method of aia and gas prospecting, ~'rofe,,:~ar A
Luchter (Lyukhter), (Po:land), related poflitiv~e results o:E' the
application of the microbiological method in Fc~land Yu
Yuranek, (CSR), reported on gas-surveying, b~.tuminalr,~gir~gl
and microbiological work in the CSR and releva>�7t ctud.i.aq
conducted by th.e Ins tit~zt neftyanykh issledcvaniyy Bw~no ~~:
Research Institute in Brno} on the design of h~.ghiy e=.Pnsit~ve
analytical apparatus fo:^ the determination of hydrocarbon
gases. Professor S. Ra~gheyev, (Rumania) , repo�ted or., ne~ly de-
signs of an analytical sapparatuas for geochemicF~l nro::~pecting
Card 3~q D. Bishir and I. Kostes;cu reported on the exi~e~�ience of the
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PROVED FOR REL SE: 06/23/99: CIA-R~P86-005938009934900036-6
on and the ensuing gen~aral problems of Frospec;tirg la~v g~~o..
chemical methods; Professor V.A, Sokolov was concerned with
the :migration of the hyd~^ocarbons and the formation of ga~l~;.a,;,e~
gasobiochemical and othe~~ anomalies and the prircli,lewl of the
geocilemi.~a1 methods of p~~08pecting for anti disccvPrin ,,
and oil; Professor 5.1, k;uzneteov spoke on problems c~~ncern-
ing microbiologi~~al methods in prospecting for oil and gaol
depo~~ita; the radiometrical prospecting methods for oil ar~d
gee apFlied compt~ratively recently in the USSR were explaint~d
by Professor F.A,~ Alekseyev; Professor s7.lin-Dekchurin consl~
dared. problems oj' the motion of deep subsoil wr~t~ers; z'rofFSSOr
A.Bo Ronov spoke on problems of organic r~3rbon i~~ th~~ Sedi_
mente.tion rocks cif the Russian platform in connectionwith
oiI and gas prospecti..ng. Several papers dealt w:;th prl:~ble;ns
of the methods, technical aspects and apparat,zs ~^egi~irw~d in
this prospecting: the nature of gesobacterial a.nomalief3 anli
a rational metl-,od of thei~^ phenomena, hydrochemic:al inrresti-
gatio;ne at oil prospecting;, soil and gecchemical itldicatlol7s
of oi;l and gaa axidtence, the luminescent a~ethud of gtudy~ri
and d:le~oov�ring g,~s and o~.l depoei te, the geochemic~s.l xor;a7 ~
ity o~� subsoil aatere and their importance a~ith respect to
Card Q/q oil occurrence, chromatographic methods of as ~ ,,,
$ nn B.~ ,} 518 ,
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:'
AUTH4Rs SOV-2~-58_9-24/42
Scianeea ~ ..~,~,;,,,, ,
~R11~ G.A. Candidate of Geological and 3~i;;eralo ,
1~osca~rrj ,~. ~$.
TITLES Ceoahemical Oil and Gas Prospecting Method
met~~dy poiskov nefti i ~;aza) s (Ge~okhimiche~3kiye
PERIODTCAL: Pri:coda, 1958, :Nr 9, pp 107_.108 USSR
ABSTRACT; The Presidium o:f the AS USSR has studied and a _
suli;e of the geachemical meeting in Mosco~ on theoinatiative
of the AS USSR and the Cosudaretvennyy nauchno-tekhniches '
komitet Sovita bfinistrov SSSR (State Scientific-Techni kiy
Committee of the USSR Council of Ministers. ThE>! meet:inal
was prompted by the resolution of the XX CP Congress togi~..
crease Soviet oil production from
and gas production from 270 to 320 mii].oonmcubi~rm~ons,
within the next 15 years� The extension of natural gas sour-
ces :ts of special importe~nc� in this connection ffere gao-
chem:lcal methods may be u~.seful in addition to the geo h y1_
aal and structur~~1-drillin P y
sere presented ~ g Prospecting, A total of 27 pe.pera
Academici+sn D~I
Shcherbakov openE,dbtheomee~~nsc~ndtists.
achievemonts. A.A. spy! Member Correspondenf~ ,~foth~ms and
Card l~q USSR delivered a paper on the character AS
of the element migra-
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5~,01QT~ T.A., o+tv.rrd,; 8,sUK0Y, A.A. ~ rsd,; QiTCHIN~IICOT~ I.M�. ~d�;
SO'~, g.I.. prat.. rsd.; .Alm. T.d.. prat. ~ ~r~d.; ~ET.Ag~
A. A. , kaad. gs ol.-^ins ra log. neaJk, red. ; MO~II,~S[1T, d� A.. , kgsul:.
~. ,.~~...~.-w-~.i~.....~,..
geolago�~m~,nsralog.nauk, red.
[paoobamiaal methods of oil an~i gas prospecting; stndis~a of the
oontersnoe on gaoahsmiaal methods] t#sokhieaioheskie metody poinlcov
aettiaxyilch i gasovykh. mestoro$hdenii; trady �oveahcheni:ie po ~~eo-
kbimiaheslcim metodam, Moskva, aprel' 1958 g. ('MIRJ 12:I2~
1. ~cademiya Weak SSA. Inetitut geologic i regrabotki goryurhik2t
isl:opaTe~lch. 2. Chlen-gorrespondent !ii SSSR (tor Saukov).
(t~eochsmical prospecting) (011 tields) ((fie, H~atural)
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~~set s S#I~ning
~a 1~1 Pub. '~''~ - 21/x'1
- At~~iQr ~ ~ubbats, ~. I.
~-ID P - 111.0
~tl~ ReWi~~~ Ct` Q~. A. ~~�gil�v~~ki~'s bo0~c orob~.o
- o~ v'esti~,ation dP t#aa ,~tnd Oil Dap a ffi
.wi~~~,rppi~/w~w..~ww r~ ~~.~rw~r.rQ~Iri+((Y~~~~aiir~+~{r
~r`i~~tigi~ : ~Q~t R iLilb~-a ! v� �~~! ~lO~ 7~~7~~ Q 1~5~
ca 1 I~te t~hod
~kb~trsct ; e rQwiewer poi:Yta out the ai$nificance of the book' a.s
th+~ t~nly publical~ion since 1~3 describing i:he applioe,-
t~.an q~f the micrgbiological method coordinal;ed with other
~~~l~t~~t~~l xethode of eurvs9l~g, such ae thts hydrochea~.cal
enc~ x~ter-gaasouM method.
~titutiox~ ~I ~~~M~neft (~3ureau o!' Theflretical and ~xperimenta].
I~~'o~s~ttion. - CEantral geientif 1o RtsearCh xnatitute
fc~ ~~ahaniaation and Labor in the Petroleum Industry)
'~t~et~
s ~~ dst~a
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APPROVED FOR RELEASE. 06/23/11 CIA-RDP86-005138001134900036-6

PROVED FO E: 06/23/9 9 : CIA-R~P86-0059 38009 9 34900036-6
:......: ..,:r
c A
-tea ~~~{r~~ ~'91k~4,f1, ~' ~ .:-~
S ` s~ ~- !~
.R{
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~~. Gas, Alatural -Stavropol' Region
't. Results a:[ a bactarisl aurvery conducted in the rc~~~ion of Stavropol' (Caucaelus. )
Tzv.Glav,upr.geol.fan. no. 3. � 19b7
l~lon~h]r,~r Li~eLe o,f ~,is AoCe fans, Librriry off' Con~rese, ~'~s, 1~-;3, i)r~~.l~.~~~'j ~c~.
APPROVED FOR RELEASE. 06/23/11 CIA-RDP86-005138001134900036-6

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APPROVED FOR RELEASE. 06/23/11 CIA-RDP86-005138001134900036-6

APPROVED FOR RELEASE. 06/23/11 CIA-RDP86-005138001134900036-6

APPROVED FOR RELEASE. 06/23/11 CIA-RDP86-005138001134900036-6

APPROVED FOR RELEASE: 06/23/'1'1: CIA-R~P86-00513800'1'134900036-6
APPROVED FOR RELEASE: 06/23/11: CIA-RDP86-005138001134900036-6

PROVED FOR RELEASE: 06/23/99: CIA-R~P86-00593
11'I.~31tT~, ~. A.
~1~2R (Thy becteriet~ meihad of rrc~~~ ~~cting for oi.1 end r~~turnl p_r?aen) BektPriial ~r.5�i
metod rezvsdki rya neft~ 3 trirodnye gazy.
SQ ~t R~ayec ~e~~ 1~te~dr,, ].0 (12) : 32-43, ~94Ci
APPROVED FOR RELEASE. 06/23/11 CIA-RDP86-005138001134900036-6

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~~,4~.i.a~~,. ~,.~t .~ t ~. ~ . ~ ~ ~ - ~ ~ t a a r ~I sri M rv ~i >r r ~n � o ~ w
Wt t46~ 1~i` ~;'i'i'it
" li~:FtN4 sate ttritstt{- ~Gt- _. �+ 'I�
i i
~� �
F ~~~
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~ ,p~vwk~r tiaiiai et tM ~ ~� t
dw-iM r+ulew +~+~ m aei ,leul� ~ ~*� �
~ aa~eu, d fir. '1'1-~ ~tb ~tilwla+ A �
M~In wt !tMi 1wi.~~~~+.t M~-+la~
Nli tM t~ Mlfrlr~l IiCtNNi1 tb- {M AMA 1~ . 4~
f~ : a��
;~ a��
a�!
f~.~j�~~
~~
~ti- .
:~
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Ri!�Ilk~ /(nALLY~NLN. id1'ttRt~iM[ ttatiu-1ta1NlM _
M ....w.r.ww~ r{r aps 4i
r il�'. w~ M � w~ R s +e as a s
�~�~i��������
rx- :.~.;
{-Qki tur{~r
-t~Ally.- '._.._.___,_ lAlltl t i711f iSr~ t{i _ ,
T r !~ is - s r a o . . ~ v ~ ~ r~ i ~ ~ ~
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~~

APPROVED FOR RELEASE. 06/23/11 CIA-RDP86-005138001134900036-6

PROVED FOR RELEASE: 06/23/99: CIA-R~P86-005938009934900036-6
1~t~}I1~iV~xIY, ]D.H., prof.; T~iTA~liM11N, ti.Ye,., doteent; bAPIJiS~I?, A.w. (Stalin~ad)
~""'~"~~~,wr~Yiw~1~1
Rational ~ '~ of the rectorcarc~ioecope. Klin.,~d. 37 no,~:
9609? aZ ' y9, (~~u- iz : to )
1. Ys leated~r takxul'tete~koy terapii (sar. - proP.R.~I.KoPilevekiy~
Stsl~n~radekogo ~aditeit~~eko~ inetituta.
(')
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tI~ !. X11, P'i;f
"~tibio~ilci 3 ilcb lcliniaheakor~ pris~z~i~je (~tibioti~e and Their
Cliniol"1 IIse~, 19~T
APPROVED FOR RELEASE. 06/23/11 CIA-RDP86-005138001134900036-6

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~Rav~aFr~R~~Ei~fb~ai~~t'~ ~alr4 wit~~ha on ats[io~ao f-i,.~p Q~goss
Ia rush a ways the rpia interaat;toa c~aa caurs a aoasquilibrinm o ,rla-~
ties is Zeenaa auble~elr. P P
Ths pt-obability of collisions virh reso,aapc.e
~~hotoas it greater than calli~ionr of hy~drogsa stoat with slactroan
~Lh� pla~ta. The*e is � probabiifttr that to active coro~aal raRiop� sip
ciyoaaic orientation o! stoat sxisitr, cav~~ed bit rsronaacr dirp~erriott of
1:a ~vanta. OYisattd brdroRsa atC-tN� ara :located in the field ~~f con-
t:inuoua radio eeirrioa with total polar~lsatioa, or is assert-'Like co~-
dlitioar~ Ths radio eaietioa o! corooal 1~eterogaasitie� occurn at as
optical depth which slitiaate� the relic-ubeorptioo !o radio liner. The
"'Maser" uechaair� can probably exirt in iicti~� rsgioar sad t se-i tad
�'~tburrtr gar be apeciiie eiotocbroaatic s~adio liner of hydrogwn~ io
heliua~ tad other eletentr o! corooal is~saa.
th� liasee-like otture o! t s. P it is necsrrarp to prose
art. bass Z figurer sad ZT~oraolario ou~~bdrrtr bT experiaent.' Otig.
gtTB CODBs 03/ BN~t DATBs Z40sa~6S/ OatC Rgts 010/ OTM tB!'s OOS

APPROVED FOR RELEASE. 06/23/11 CIA-RDP86-005138001134900036-6

FOR F~F~ / 9 : --G1,A 9 OQr90 ~4it; Oa 36
;rasprostraasoira radiovolo As! SSS;Rsesao~~D �agoetissa, ioaosfarr i '~--._..
7CIT1.Et Oo tba Ks~ar aafnro of, �a~lar rad;to ontbu
------_. rn t s o f type I
S{OOStCE s aaomagoetisA i aerono0lya, v. 6 ~~ ao. 5
~ 1966 ~ 809-81 ii
T'OPTC TACSs �olsr flare, o�nochromatic rsd~~,~
color radio eeission, Zeamao ePleab ~ ~sna ~rmetl,c f1e1dN
plasma, solar physics, maser theory ~ elacerom spin;, solar
IABSTRACTs Peculiar
propaxtias of type-I solar radio outbureta~are=
l.) monochromaticity of the 2---4-M~: baad~ 2) hi h o
o1E this radiatioa~ 3) close correlation of radio tr etotal p�xexisation
solax activity and iocreasad radia- emissi,~o in theyAe I outbursts w:ttb
mc-st iaportaat property is the aonlochromr~ticity by which rs,u~e� Thn
outbursts difler� Eros other aoaequilibri~~v s o t i� t7Pe of
ea~issioos. A oooequilibrine coaceotretioi~ ofpaentralsolpr rad;to
is Zeesan sublevels caa occur to the atso~~phere of a hydrogen ato�s
Spies of free sloQtrooe io a rasnetic pla~~s� are or ctive regions. .
~+d 11Z tented by tree , mag-
..,...
~.ZZ
APPROVED FOR RELEASE. 06/23/11 CIA-RDP86-005138001134900036-6

PROVED FOR RELEASE: 06/23/99: CIA-R~P86-005938009934900036-6
'~Ia~LI~': Ifs}l~~'~~ t7l;z~;t~cto~;i~;l,>ft fa2:' U~:tc~i'2nitl,(ilu2l of lvcli,~Lii~s(i~(i i:a2,;i;i)ric..:~. c~;'
in:.:n~~tic fie}cIs oz active arc;as
:~CDCi}ACT:; rc~f, r}~. tlati�or:omiya, Aba, ~. 5 i, iii7
ITII~ ~~OUIiCi~; Sb. Solnc:ehn, aktiv(lor~t', ~,~. ?. iVT. , tia~;:,~~, ; ~~;,, 1 l;i-: ;;,
'(J~'iC i.~CC~: ~o,~r 2na~Yn~tic 1~'iC? :: I, ~ff ~}i t,~~1~�r-
minin;; the lon;iiudinai corr,potiC((i: 01 a I(.C:1C}, ~'}1E; nlc'i(~2^iLtG..,i X17}i iS i)a:i :.i,Ci,~ C:;.I-i
' to an original c3e.S1~;21, WhICh UT1i1K~ triG f.;C'(":Gr~::ly 3CCE'pJt(;d ~aC~GGCIt G(:S.~;C'i, "_.. ~..,
Gill}~ ore nzlotamu~tipiier to rnaKC measu2'Gn',c2:t y Q` $ G 2Ticl;inG%iC I.i:iC: G,:~a.;~ ;:,~ iii
ti:'I:"(;S Oi the S~aeciraT line. n b~.~t:f: G~ti~i'%C'~tT7; ~t~iCa .:E:f,LL"(}fl ~.~lufT'uiT. ~ CSI ~~ -, ';;~:
~, iii.; :;,,, -," C,-
gi�~:lj)}l, aS W1.;11 %i~a foril~illaa i~ir Cia.lGlll~t~.(Gli [~(~ ~.:~(, V'Jcj:ltl.ii~ }i~al'iai'i7t;yE.,i'~ t~f ~,d(E~ ~/ii1.r�/L'r�ii~?
and the calibration of ttie instruillent arc pre~cntc~d. (See ai:;v ~,Lhl`sstr,, r;~%::,
1. Iii. 3II3). Eiblio~ra~hy has16 re~erenct;s, ('~ ranslation of abstraci:J
~~ 1/1 SUS CODE: O8, 09, 20/; " ; ,. UI)C. 522, tE17
APPROVED FOR RELEASE. 06/23/11 CIA-RDP86-005138001134900036-6

APPROVED FOR RELEASE. 06/23/11 CIA-RDP86-005138001134900036-6

SOURCE CODE s t1R/o269j6~/4o0/aoEt/oo~,s/Doss
,AUPHOR; hogilevaki~E. I. ; Zhulia , I . ~-. ; toshpa , B, A.
~TI7PLE: The IZMIRAN solar tower installation
~SOl1RCE :
Ref. zh. AstronomfYa, ~. 6.51.434
1RE~' SOURCE: Sb. Solnechn. aktivnost'. N
o. 2. M. , iNauka, 1965, 108-1].7
TOPIC TAGS : soaaY+ to
~ leacope, solar. spect~rutaa, specttrographic analysis f
TRANSLATION: The ATB-3 IZMIRAN solar towi;r is described.
'group (D = 440 mm) are nownted on the u .The mirrors of tt:e coel.ostat~
'tire optical assembly The clock mechan~om isdconl;rol~gdlal tube-which hou:-es they en- ~
thro h a
~ power ~ lifier. bY'+~ 3G 11 sound generator '
P The main mirror of the telescope has the following pars- ~~~
~iet~ers : D = 375 nm, F = 17 m; the Cassegrainian reflection is F = 27 m.
se~~- is equipped with a complex hnrizontail spectral assembly which operates~aseaes ec-~
tY'o1~raPh, a spectrometer, a spectroheliogr~aph, and a sPectrohelfoscop~s. The spectro- ~
~gra~~h uses airrors with F = 10 w; the GOI diffraction grating has 600 lines/aua. The ~
~balfwidth of the instrumental profile in the IVth .
Rhe theor`etfcal value -order ~ 0.026 A (this is larger than
by- a faCto9c- of 1.4) . The ina~tallation is equipped wit h a mrn~o- '
ahrc~atia guide. For visual and photographic observations in the Ha line (a~n IPF lyy I
1~2 1~1~: 522.56
APPROVED FOR RELEASE. 06/23/11 CIA-RDP86-005138001134900036-6

APPROVED FOR RELEASE. 06/23/11 CIA-RDP86-005138001134900036-6

.~..~ .6 aw~ti~/i�~ aw ____..~.______ _.__._~__.._._.~.~._~
ACC ivR, AP70023Sb ~ St~RCS Qp~= vR,~o243/bs/oos/oos/oasa/ass?
A,UTl~DRs iQ~tleshov_a, ~P. P., llevek~,i� E 3y
aIRCs Institute of 1~x'i'estriel Maststotia~I~ggp~.a,~o ~d~Rgdio xNav~s Propagation, ,AN.~._ j
S~$. (Institut soaatiogo ,magnotisa~, ionosfory i tasprostranoniya radiovoin AN SBSR) j
~'ITLEs Energy characteristics of ionos hp oric disturbances and tho natura of ~
,goQma n$ etic~ d ionospheric disturbanoo ~
gOURt~s Ooomagnotlsm ! aorono~miya, v. 3, no. S, 1985, 8S4-8S7 .
Tb~~IC TAGS; geomagn�tic disturbance, for-oapheric disturbance, magnetic e~torm, �'
solar corpuscular radiation
ABSTRACT: A comparison has been made betW�on th� plnnotary characteristic of
ionosphoric disturbance and the enorgy characteristic E o! goomagneticl storm.
IC is shown that there is a oorrospondenca botween the activa periods of geormgna~tic
and ionospheric dist4rbaaoes, reflecting the structure o! the n~gn~~tic field of a
solar corpusoular strea~a With aforce-free ma~tio field. The equation of iond-
station equilibrium !or the entity thickness o! the ionsophere is u,sod to determine
t:he frolationship between and 6. The dependence o! change o! the ter~!pa~raturo o!
aaoaphere and ionoopb~re on ~, detef~ia~uf lros �at~llita decelaratlon, in used. the
s~uthora discuss the problem o! the tran~alor o! the enerigr a! a diaturbanc:� froa~
the magnetosphere to the ionosphere by aeaeu o! ltx+�ixequer~cy hydr~magnet:ic saves
wfiic!- ~ssipate is the ionosphere.
Card 1 UDCt S.S0.382.2
APPROVED FOR RELEASE. 06/23/11 CIA-RDP86-005138001134900036-6

~~ ~ 7
t+:'~ ~ ~ j ~ t t
M
+~4 ~ ~~4 a ~ a~~,~ ~ ~ y:"~'' A~,~"5 y~ ~
# J
` ~ Y Pb ~ .a a ~~Y 1:.. "~i C 3f ~ ~ ~i ` ~ ~ ~
f J
- ~ ~ ~ ~ ~
~~
- 4

~
4 :4Jf ~ k h$ Y

a. i
~ - - Y 5 ..

~
?L ~
,t i - .. ._. _,

i,.

3 r
~
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y
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d
jS :�
,
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~
,

~ ~Z
ny.
;
'drr
~~
~

o ~
, yy,
e
v~..t. 1..._ _u
APPROVED FOR RELEASE. 06/23/11 CIA-RDP86-005138001134900036-6

APPROVED FOR RELEASE. 06/23/11 CIA-RDP86-005138001134900036-6

APPROVED FOR RELEASE. 06/23/11 CIA-RDP86-005138001134900036-6

ACC NR,
AT6023730
-- ---- - - - -- ------ - -- - -~~ _ fr. 1
` condition for macroscopic motion if the solar plasma in the chromosphere and corona
is compressible. llsing this model, the appearance of solar low-ever cosmic r s
is possible With the plasma cloud in which the burst and magnetic fie were generated
retaining infected protons. The geomal~netic disturbance is a consequence of the
interaction of the magnetic field of the corpuscular stream with t;he magnetosphere.
This approach to the problem does not ~~equire a solar plasma with a frozen magnetic
field. Analysis of synoptic maps of tt>.e deviation distribution of critical frequer,~-
cies in the F2 layer Pram the median vt~lue demonstrated the existence of regions with
increased and decreased frequencies . D4aximum negative deviations Ixcurred in the
geoma~etic latitudinal belt of 40--75" and coincided with the beg:tnning of magnetii~
storms � l~egative deviations Were located in regions of magnetic a~iomalies . Positi~~e
deviations of critical frequency occur during weak geama8netic disturbances and depen
�on the Beeson. They appear in regions of magnetic anomalies. Varjiations of critici~.l
frequency is the F2 layer increase xith the geomagnetic lat_tude~ aed they at+..ain
maximum value in the auroral zone. Orig. art. has: 4 figures. [EG;
13U8 CODES Ok/ $t~M DATE: none/ ORIG REF: O10/ 0TH REF: 001/ ATD PRESB:~~~,Z
.__ ;
APPROVED FOR RELEASE. 06/23/11 CIA-RDP86-005138001134900036-6

T~~~ r~ iit aavRC~ comic: vR/~es~/6~/0oo,~ox~/ao~6/o05-~
AU~SOA: , le~sti~~,,; Zev~cina~R. A.; ~,arrrava~YeT.,_.Y�; I~r_, ~.. -'. ~~--/
OTC: none
f~ ~
TITLL: The nature of time-space distribution of ionospheric disturbances
SGURCE: A!1 SSSR. Mezhduvedomstven eo zi,~heski komitet. V' razd~el progran~np- ,,~
MGG: Ion ra. ornik statey, no. 14, 1965. Ionosfer~gyye issledovaniya, 96-93.
~' PIE TAGS: K ionospheric disturbance, solar rind, F 3,t~er, geomagnetic
Field, solar plasma, critical frequency , solar corpuscular radix+tion, atceoepherie
ionization,~atmoepheric dieturbanee, ionospheric absorption, eynoptic'aieteorology�gyp
ABSTRACT: Ionospheric perturbations are associated xith solar corpuscular streams
and the magnetoaphere.~yAn increased disturbance in the F2 layer at high latitudes
is connecteQ xith additional ionization and structural disruptions of t e lower
ionosphere. Data obtained from 60 ionospheric stations during th,e IGX~~ere used
in analysis of the spatial distribution of anomalous absorption in the Northern
and Southet~n Hemispheres. Absorption maps have been drain and cc~pared xith solsr~
processes, ionospheric disturbances, and perturbations in the geomagnetic field. -~
Ano�ualous absorption begins several hours after atype-IV radio burst and covers
the polar cap and the auroral zone. During weak absorption, preeminent "shock
zones" and quasi-spiral regions are formed alloxing direct entry of high-energy
solar corpuscles. A corpuscular etreem model wlth a forceless me$netic field wss
umed for ionospheric disturbmees. A forceless magnetic field is a necessary
Cocd_1L2.._ -- .. ~.. _ _
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'{ .were based on the photoepheric lin� of iz~,n ~ ~~~p,z,
~tor 8-14 euc+ceeeive dgy~c for Janus e1;o
~arezro used. In ordgr to detenair-e the ~' August and October 1458
'ot the ruzgnetia field ~d magnetic tlgx of local z~egiona
variability of tield~r it wasdnece the character of the struatu;re ar~d
~rhich is ex~t ~ ~ interpret the aagnetograms,
~e~Y caQaplex, and construct maps of isogauases -- lines
of equsl values of magnetic field ~-trength.
'an exaxcple of such isogauss maps. one ~ ~ 1 in the text ie
diatr~,butiw~ of the local magr-etic tield~ i~netheY~o~~pattern oi'
'ern yes of activity makes it ditt'icult to make such an ~ south-~
on the other hand the probl~a was r'acilitated analy~ais, butt
;verb canplete data on calcium tlocculae. by the av biltty of
colas virtually coincide with re ans where th~undaries of th~a floc=
~5 gauss. It was found that the pattern of emagi~etia tYeld exceleda
spot and ~n an active region is di.ftez~t.~8 of the flux in a
d~ae of the abaerlc� of a Tea can serve as evi-
dirsct relationship batxaen c~nanges of the
nagr-etic tlu~ ~epote and variation. of the ~Snetio t,lztzc o~ the
.. region , Orig. arl.. has s ~ ti
~PRSs 34,593,' ~ur~s a~ 1 formula.
r

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� ~~.. ~~ ~~ SOURCE CORE! UR/0203/f-S/005/006/ 1092/ 1094
~ AUTHOR: Zhu 1 i n, I . A� ; ,^Pfo~~,~i~y ji~.w~lr~irl
ORGs Institute of Terrestrial Ata,grtetism, tho Ionosphere end Radio ueva
Propagation, A,N SSSR ~Instltut zamnogo magnstisms, ionosisry i raspro~tranoni;~a
radiavoin AN SSSR)
r
TITLE: Variability o! the !luxes o! magnetic fields o! spot~a and �
_ feculrse
SOURCES Qeoa+agnetiam i asronomlye, v. S, no. 4, 1965, 1092-ri094
TOPIC TAt~: solar magnetic field, Soler !scale, tagnetic field aneaaurement,
sunspot, magnetic field flux
SUB CODE! 03,20
AHSTRACTs ~ this paper an attempt is made to determine quaL'ttative
the nondspendence at the variability of magnetic fields of apots~and
a~jaaent tac~lae on the basis gat same data an local zsagnei~.c fields ~ ,
'on the sun obtained at l~ourtt i~il.son Observator~- durir:g the IG? period.
The basic data consisted of m~ygnetograr9t~ of the longitudfr-a1. c~o�ponent
of m~etio fields on the iron ~~bta~ned, ones a d~r~ The aesaents
_ Card 1/2 _ _ _ UDCs '523.745
.-,
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I~ItAS~�EL~, E.k.; MOGILh'VuKIYp E.I.
Solar aetoivify and Lhe geoelectric ca~rp.ex of ~}~ricn,~. ~~f ~x.
a.~)
biol. no.llit92~95 ~ ~. (M I ~.A ].~~ . k
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PPROA~VC~L~F. Q~ R$F~F~y~~E: 06/23/9 9 : CIA-RCP86-0059 38009 9 34900Q36-6
UU 1r t of these waves, the energy of arder~~d osciU-atx~c~ns
result of thg decay in stab ~yturbulant noise and is not obsoi`v~tic energiesckis
E erted to the epeotrum es oP ~netia ~ ~ 6
is cony ~ ondenae between. densati
of az~y ~,-que c�rresp "wave" ~.nter�pr�tation oP the data from j~ari,nar II. Thesla
an ar~vtnent against any otl'tesis of a corpu$ streau with a 't frozen"
data genara13,Y contradict the E,s that tlxe meastxetaa~8 of '~enua atthe oar
~gngtic field. The author aonclud ~ not contrad,i
e iaa etic f~.e1.d in a solar csarguscula-rated w~itimut conf'11ot on the
V on th ~ but may be interP
mcaasuranents of Mariner II, stream ,;tith a week magnetio f~� 4ri~;. art. has:
assumption of a ~ o ~ ~ ~ ~~
figures, 1 tabl ~
ionosfery~ i raspro~3tranen~,y'a radiovol~a
o r;eti,zma, a~tid Propagation of
~,SgpCJATxQN s ~titut semr~og ~ . neti$~ the Ia~~+~~
AN SSSR (Institute of Terreatrasl ~~ag
Radio Waves AN S~;xR) �~.
DATE ~~,s 3~r~ r~tCLS v~
~s,~rrTID: lgDec63 art~.R= ~~
NO REA' SOQ s 0~2
SUB CODES ~
Card 2~2
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,IIGCESSION I4R s AP1~o3162k

AUTF{OR s Mogil~rskiy, ~. I.
S/02 03/f~l~/001~,/002 /0213 /02 23
TYTLE s The pos sibl� structure of the magnet~.a field of a corpuscul~~r stream
s-ffeating the eaz'th as detez�mined bar measuz'enients on Mak^iner IS
SOURCE: a�omagneti~-n ~, a�ronora:iya, v. li, na. 2, 19611, 213-223
'~7PIC TataSs magnetic fi�1c3, corpusl:ular atr~3am, Mariner II, ma,~netc~spliaz~o,
turbulent noisy, shock cave
dBSTRACT s The magnetic field Was m~~asurad o-i Mariner Ix by a three~�con~onent
fluxgr~te magnetometer having a seuns:ttivity oi' }, 0.? ~antma. MeasurF;r-pn':.s of the
magnetic vector and the parameters I~f tho p~,astna ar� ~aportant~ bec~~~asf, from them
it ~.s possible to detet~ne the thr~ae-dimens:i.onal structure oP tl~ � .a~..otia field
of a Solar stream affecting the earl~h. The data are preliminary, t t:t ;,hey far
surpass the previou$ data on measurecents of the magnetic field. ir. ~s sue. as a
Card 1/2
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PROV~~~~2~ (~. 1T8A8Tlu~810I/i~~~ ~Ol~ [:ORf~PU~,ftr~~I'~8it1 tSll~r~,~l X~th 00036-6
Farce-Free I~gnetic Field to the l~~gnetosphere and Ionosphere of the Eerth."
report et~mitted for Ultra Lax Freq~~ency Elertrom+~gnetic Fieldr- 5ymF, Boulder,
Colo, 17-20 Aug 6j+.
Inst of q'erreetriel Me{~netism, Iona3pherP & Radiowave Prapagat:i.~on, AS USSR
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PRO~(~~ , ~:, 0~6/2~1.7 7.t- ~~A~-R,pP86~0059 38009 9 34900036-6
t 6~ �
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PPROV~~ FOR-~?�~E~S-�z-86L23~~~t--CAA-.~QJ?.8.6..O~,:a.7.3.Fi2009934~00036-6
~~ , `; rat+rdtiwd lbde th 4tb 2otabaLioaal /paa ~r^pottin~ (OOSl~A~
~~ 2~1Z Jwi~ 63
~?
"'.
' ' '
~i
! 6. ~
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PROVES FOR REL-EAS.F~-~/~/Q~,~i ~p $1 nR~P86-OO~~~~QQ,~ 34900036-6
If A 160,%i Ia0~1/ ~~/00?/~2~
relation between T .
scale corana x and the z magnitude. :Phis relation is dif
irregularities fert~nt for various-
FeXN ions are different, ~ 3) 't'he macroscopio velocities v
Doppler origin. The characteristj:contour of emission lines is of the FeX and
plasma is invests ated motion of multic not of a pure
(E ~ ID-6 g in the pre~;enee of weak non- barged x-ions in ~
v/om) in aoronal irre stations ~s aoron,~1
gularities. Theo rY el�atric fields ~,
and the relation between T baerved Inequality of T ~ r-
fie acceleration of x and x may be satisfaetaril x T
ring anon- ~e x-i�~ in '^'a~ electric fields o~eaxcplained b e
stations Y the speci-
lY appear in r"S' macrosoopi,; plasma motion we tive corona regions,
'the active corona ~� ~ +~ electric fields s r
These fields adequatel e6lons with inhomo eneous m po adi-
author eonoludea b Y explain thel characteristic ins ' agnetic fields,
lines Y pointing out that inve,~ti ations ofuality of T
pave espeaiall g the ooronaz , Tee The
in the active regions of Y used for determining the eleetro ~d.ssion
the earona, magnet.lc conditions
~OCIgTIONt Institut zemmio a There are 2 figures,
g maBne'ti zma, i onos fe
~ 3.SSR (Institute of 7"er'restrial ~ i r~pY'ostraneni.ya radiovoln
Wave Propagation, AS L~'~) ~Snetism, Ionos
i sUt~IT!`!~= august 1$, 1y~2 ~~ arm Radio
- Card 2/2
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- nci~~iw w - r-~~_or~oQC_nn~-sd-~ ~R009 934900036-6
~~. ?9N,R,. -
A 1(0/A 101.
AUTHOR: Mogilevekiy, E. T.
TITLES The motion of rratlti-charged coronal ions in a �agnei;oactive solar
plasma
{ PERIODICAL: aeomagnetizm i aero~namiya, v. 2, no. 6, 1962, 1041 - lOj2
' T'FxTs The author investigates the possible nature of the distinction
between the values of the electron temperature of the corona Te, determined by
the ionization theory, and Tz -the te~aperature of multlchargeR z-ions, deter-
mined" by Dopplersa contours of coronal emission lines. The first successful
experiaser-te carried out of the radioiocation of the Sun at s frequency oP 3S,2a
Mc permit the ae8umption that the effective electron temperature in the corona
at a distaQce of 1.5 R� ie about 5.105oK. The author diascueeee the essential
inequality of Te 7 Te on the basis of a number of warka and summarizes the ob-
servation data as follows. 1) The effective temperature of the z-lone (Tz),
determined by the contour widths of the corresponding ions,, is systetaatioslly
higher (snore than two times) than the electron temperature Te. 2) There le n
Card 1/~
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PROVED FOR RELEASE: 06/23/9 9
Internal structure of a~~~.r~r.,~.
CIA-RO~~~ ~-~j~~R~9/~~~.Q0036-6
IG4fi 2292 v ~ vl
r1c plasma. The r~nergv trf:n.~~c~z~ted b~~ these law-frequency (T~ O.I-
10 sec ~ vraves (~ 2.10'5 �r~/crl`~.seo) prov idea an every 1'l~~x suf-
ficient to produce man,~atic ciisturhances (,~ 1022 erg,~sec ). ~'he ~E,
earth passing through the corpuscular stream twice cros.les its ma~;-
netic field, and since ,~~ithl.n the stream the magnetic fj.eld is
almost zero, each major r"a~;n~~it5r v~ith reap�ct to th� magnetosphere
(i~4~ 10)~, generAtes ma~rr,�t~~acoustic shock waves in the magnetosphe-
Card 1/2
f%,
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,~~ ~~, ~ Ajj~j~ ~7
~l /
I
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ifYp~~th�e;l,s of c Y02~ / ~ C~1/~.~C4IC}I~
/z2, ~
..,.
"~� Institut cer~no
r8$ProstranenigQ ~diovol~' i0nosfe;~ i
(In9tit,~te of Tf,rrestria,l ~~kademii nauk
and Rad i ov~ave n ~ 1~het ism S,>SR
USSR) 'r0pa8ation, Acad� , Ic~nosphare
SU.~ibiIl'~'DD � ~' �f Sciences
Dec9r~er 6, 1:61
AuSU"TATIat � s hYP�the_
nor,, in tho rAd i.at ton bcslta,
ex2~eriment yyhicll cc,ulc~
a detailed a ~.I"c~ti � or rePuteptheent there is r~o sin 1
comparison withysateil ti~ta above h 8 e
da,tA collected on ~, ~othesis, onlq
sis, There is 1 fi lite datA a~111 ..arch and their
pure. Trove or re.flate thi
orE~u;~cu:Irzl� so?s.r str�amg...
cont~ ~
Card 3/g
. ~..�
,~

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s/z~3 az/ao~/~~;~,~~~~ ~~z~
I;'Ypothc�ffiSe oP r~irpusrul~r s;~~.n.r streams
...
A Graph shcyws the structure oz' the cor use
interplanetary space. mhe mA~;xletic trQ oular streams in *he
c~ontQins protons with energies u p P such a
p~"otons can be either of solar orito several Bev. Theseaaneruet
motion oP the cloud Prom the .,un toithar. trappsd Burin ~ is
characteristics of the mRF;netic tra a ..arth. g the r
analy$is oP thc~ spectrum oP low- p an bo obtained ~uali,tative
the data #'rom the Soviet rocket togVenua an y a detailed
8Y pr imarq cosmic rags . :'hou ld
satellite "Explorer ;t" be cQnPi.rmed by PurtYdierr�m the
will prove that the mn? American
L,netic i'i~sld oP the streameisunotgfizadii
the plasma, but theca is
the stream itself. ~ ~~ magn~9tic field beyond the bound,~rieanoP
ca:n be expll~ined b carious geomagnetic and ionospheric ef~'scts
y the ir~teracl,ion of the magnetosphere end
1o;nosphAra with the atrear~,
e%ci,~lainvd b Goc>mggn�tic dia't~'bancea cannc,t bo
y the radiation halts o.~' the Earth, because
oP a g9oma,gnet is storm is 2 to 3~ t inisa hi
Rher than the tota,lnener
Card 2/3 gY
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,.,
~/~j/~ i/aa~/ao5/o2~/a~8
aoo6/aloe
a~ORS; Mogilev~k +
__ -~,~~.. I . , Akin yen, S , T,
TITLE; On the radio radiation ~pectrun of t
YPe
IV bursts
PERIODICAL: Geomagnetizm i aeronorniya, v, 1, no, 5, 1961, 8~3
~~T� The authors analyze ob,~er~rations of t
spectral rangy for the p YPe N radiobursts in a wide
pur ose of revealing the nature of the first and second
phase of the radioburst.o The speetr~urn of the initial phase is a curve incre _
ing monotonou$ly with higher frequencies, with a relatively low intensit i as
meter range, In the ascend phase, the intensity of radia red.iatian :Ln^reaserthP
with the wavelength, The spectral
the initial peculiarities oft
phase can not be due to .magnetic bremsst,rahlun i adiobur:;ts show that, %~
radioburst which is preceded or aecorn anted b a t g` It is a type_1,1 ~/
phase is explained by magnetic'brems~atrartlungy~f relativiatieselect~~, Second ~~
tions are given for the spectrum of ~~adia-radiation and energy spectruun^of'Equa_
trons. The analyai$ shows that relal;ivistic Flectrans, determining the radelec_
radiation observed, can not arise as a result of a single flare but are contin_.
Card 1/2
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Some 3/169 6~,/000/olo/a34/o53
properties of... 1?228~304
ra,dl.osplsah, odours near the r~ment of for obromorphara flare ~ e msximwa,
whereas the beginning cf the a~ypa SY rr~dioaplash it oloee to the mamec~t.
of the start of the election c~ the eruptive pratuberance-filament.
(2) The substantial (especially on the frequency 545 Me~s) ~eakeninr, Q:t
the intensity of the Type IV z~adiosplash is noted if the location of the
o~'o~,phere flare is nsax the limb; there is no such relatiGnshi.p ~c,x !
the Type IT radiosplash. (3) The floK of energy in a Type I:V radic~~
splash :fa about i - 3 times greater than in a 1.,
peouliarities of the Z`YPe II radiosplashs Certa., r
Irons and ma~gnetio fi lrlsneoessary for theoradionoiseroFativistic elec-
are briefly discussed. L Abstracters not�t Complete translati~pla~ e.s
Card 2~2
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~.~
IUT~$s x
TITL?~t
PERIODIC1Ls
S/l6g 61/000/0~0%3/053
D228 D3o4
,dkin ~yan~ 3. T. ~ and ltogilfaw~iy, ]~. I.
Some properties of
with the ooncli tions
oorpus cular f'1 ow
Type 29 radiaepiashes in oonnecti.or
off'' generation of the geoeffectivc~
Ref era�tivr~yy zhurnal, GBof izika, no. 10, 1961, 7
abs traot l,Ot~q�1 (Ceoma~eti$m i aeronomiya, 1, no e
1961, ]156-163) s'
~T= The analysis of the r~ecordin of
The resulting etati+otioal ourve~~ of the distMbut~pna~-OePlashes is cited.
TYpee IY and II radioaplashee iii time show o�rtain oh the intensity of
arities ~hioh ma3-, is particular, be used gor determin 8oteristic
flare. The eorrela,tions of , pecul~. ��
and TTI and wi th ohros~oephere~g IV radiospla,~hss withithoae~of pe of
flare ~s location 1 area are considered TYPes ZZ
on the ealar disc. The conclusions tromethepanalon +h~
are as fo~,lowes (1) The ape II radiospl,a$h~ �hich eoe
ys is
Card 1/2 Pr des the Type I3T

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LL notes Complete trans_

Cam 2/2
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PPROVE~ FOR RELEASE: 06/23/9 9 : CIA-Res/~69 ~iS~Q~~~4~00036-6
D228 D304 / V'`v/ /'~ ,
dU!'SOR: ltogilevekix, YE. yt� _.
~,~~~
~ penetration ~~f looe~. m8gnetio f ielde into the eUlax
TITLRs
oorona ~d the g~�~'stion, of gsosffeotive oorpueau ar
f logs
P~tI0DIC1-Ls Ref�rativxsyy ahurnal, Geofiaika, no. 10, 1961, 7,
abatraot 1040 (,aeoma6netixm i aeronomiya, 1, no. 2,
1961, 1y3-155)
s The possibility in invitstigated of the pb~emrieieace,minedcin
TF~'
photoapheT'e f i�lds into the esl~' ~eogeaeration sad outflox of the sun's
oonneotioa vi.th the oondition tie fields enter the oorona to-
radiation. It 1s $hovn that loo~~l me-8~e the gotual Feeble ma,gnetic-
gather with the ohromoephere olo~xds vhioh Derry
field that arises in the plasma Isloud duria8 its mo'ven�is oon$ dared of 1
local magaetio�fisld o! the phetQOTherQ~,arholo d8rrith the sotual field
the outflo~- of the g+soeffeoti~ ~
Card 1~2
i~
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PP RELEASE: 06/23/99: CIA-R~P86-005938009934900036-6
. ~ AKS~tYRN, S. T., ~~'~.
"Some P'eaturea of the IV l~~riioburgts." ((S1-~A-1~ )
r~~rt ~ubmi tt~d rax the In�k.l,. Cc,lz!'. ~n '~o9~~t.~.C ~,,- ; ,;ri,A 'r~�ts`~'; St',arrr. t i!. iA,P':
Kyato, J~~sn 4-;15 3~pt. I~UI,.
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