SCIENTIFIC ABSTRACT FR:NESTEROV, V.Y. TO:NESTEROV, V.Y.

• Document Type: CREST
• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R001136700032-6
• Release Decision: RIP
• Original Classification: U
• Document Page Count: 1
• Document Creation Date: November 2, 2016
• Sequence Number: 32
• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTR

`ACC NR, ~ AP70Q~ 52n . _ ____._.__ .__~._... _._...._._ .,._
~clectrically neutral particles (neutrons for example), a3 well as t~.e
.flow of charged particles with energies that axceeded the ~.ur:~r~a:~cer:ce
~threshl)ld of the Cherenkov counter radiatvr~ xTh0_ 31cm-~~ te~adn~asectl~l
I~nergil~s exceeding 5 Mev was approximately ~
~t;his v~~lue is in good agreement with the values ob~;ained by other re-
~~,~search~.rs. Orig. art. h,a$: 3 figures. [~A-751 ~
Irv]
J '� ,
SUB CO])E: p`l, /g~0/ St,rBM DATE: none/ ORI4 REF: 00~+/
t)fiH REl? : 006 ~
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--f-'~..T X11
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ACC NR:
VUU~~U
r
Fig;. 1. flock diagram o� the equipment
1 -Plastic scintilaator; 2 - eandv~ich crystal;
3 -lead-containing gla~~s; ~+ -electronic cir-
cuiL-s; 5 - photomul~tipl~.ers.

C~~rd

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Acc N~t~ _~ _nP~ooo,~o__ ____...~; __..~...~-souRO ~ _.copF::_..~_. _Ur~Jao~+B/~~/o3a/ol ~/~. ~fc~ t,/~.~~~~r '
~ AUTHC-R: ~rigorov, N. L. ; Kalinlcin, L, }~. ; i~ielior~cnskiy, k. ~ ;;
Nesterov~~V. S.'e.; Pryakhin, Ye. A.; SavE;nko, I. F+.; Eatulin, y. 'J,
IoRQ: none
TITLE : A s udy of high��energy quaryta at 'the uppar ~.irr~Its c)~ th~~ ,
a t mo s p h e r e ~~a /u~..~. ~f ~ ~ r~ t~- Cy,~.~,~. ~.. ~,~.. ~R.~ ~.~,., a~ C, ~.,.- ~-~~_ ~ ,~ .~'�..~ ~....
7~2.a ,u., ,,,~ ~ "" .- i a" Fro iJ il/n w+-..1....� 1 9 G 5~
SOURCE: AN SSSR. Izvesriya. Seriya f.~zic}zeskaya, v, 30, no. 11,
1966, 176-1'f67
TOPIC TE~C}S: gamma radiation, 'gamma counter,, gamma detection~~'--f~^~~'~-I
44--~-R,f~.-#t,, cde..,,.,;,, a ~ ~a.~.. ,e...o ~.- ~ ~ (.Jt~~'w,.- ~ u.,~..-tw
AFI4TRA('.T~ The saCellites Proton-1 and ~'roton-2 carried equipment de-
i
signed to detest gamma rays with energiE:s above 50 Mev and to measure ~
their spectrum. The equipment (see Fig� 1~ comprised a telescope
formed by a ~-quanta converter consisting o1' a sandwiched p].a;:tic scan- ~
tillator, and a Cherenkov counter with a radiator made from lead-con-
raining glass which detected the energy rind direction of gamma rays. 1._
The telescope detectors were placed inside ~i cover made o� a cintil- r
lator plastic which protected the telescope from the noise of charged
particles in ~;electing of anticoincidenrE~s. xn addition to gamma ,..~
radiation, thE: equipment was capable of z*egj'~atering pulses from other
Gard 1 _~
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!~~,~cr_ -vR, - AP70b0521
ecluipcrient arrangement wa.~ usEd try clrsY,c~ct the f'lu:; compri:,c;~v r, 1' C~rot~a
w~.th E > 1}00 Mev. The f~eometric factor of the eclu~.pment vr:.z:,
1~;3 cm~rsterad. Information from the counters was partially proces.~ed '~
on-board and the results were sent to Ear^th once every 9 ~ecc~nd~. Pre-'
l~.minary data analysis shovrs that the proton concentration ~t~~:enUity
vG.ried with a period of ~+OG ,yi~:v ,protons.
J~.xdgin from the avera~;C of three orbits, tl',.e ratio of ecncentrations
of protons with Ep > lU0 Mev and protons with Ep > ~+UO tylev vurics from
lei +0., 5 to 8.5 +0.2. The total measurement time f~~r these rc;c:.uit;~ was
4 minutes. It ~s proposed that in the future the proton spevtrum b~;
mE~asurpd as a function of coordinates B :100 1~7ev above the ~3rax.ilian anomal;~ was studied by the Proton-1
and P:^oton-2 satellites which repeatedl;,r passed over that region at an
altit~~de of 500 km.. Since electrons wi'~Y;~ er;.ergies greater roan 20 i~iev
are practically nonexistant in the inne~^ radiation belt abo~,je the __
k~razilian anomaly it could be assumed ~~hat only high-enErgJ~ t~rotc~n:
were registered by the SEZ-1 apparatus, which consisted of ~~ Cnerenlc�v
counter placed between two scintillation co~;inters which could detect ~_
proto~~s with Ep a 100 Mev and electrons with Ee > 20 Mev. A similar
j Card ~i ,_ y~
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~~ACC NR~-- A,P7000523___ _~_.~.__....______.__.._.._--..~.____--
of 2.6 x 10"2 secondary particles/c m2� se.c�stera;� . Thus t'r~L existance
of an e1E.etron flux (Ee ~ 0.3 Bev) of 2.2 x 10"~~� el/c rrt2� sec� sterad is
corraborated b the SEZ-~~.- athered data. Orig. 'art. has: 1 f~.gure.
{ Y g (WA-75l
i [BD~
~ ~r~ ` _.___ ~
v
~ S'101 , ~ 01 1 ~ i
i.
1 .Z I
~~ u ~ ~
U I
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(F7 L~ 1 1 1 1 1 1 1 i ~ i
v 0 2S 45 SB 6/ SJ J6 JJ IJ J6 SJ 6! S.9 ~~.~ i'S D~ I
., ~ W Ldtl~
~ _ ..__.
F'ig. 1. Intensity of 1 electrons a~ad ;?) protons as a j
function of latitude. Proton in~tensit;y is normalized
arith respect to the intensity of eZectr~an~ on the ',_
erquator) . j
~'S1JB CODE: 03/ SUBM DATE: none/ ORI4 RE;F's 00~/ 0TH REF: 002
Card _
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Arc-NR: a~7oc~o523~~_______~___ ---.__~.__~~.___~__._~_.__-- -__- - --___.- ~---___-,
3) a scintillation electron energy detector which is a sir~plified
version of an ionization calorimeter. Z'he scintillatoos were pla,ed
between four 1.5 cm-thick lead plates. The pulse. from the energy de-
tector were applied to a.n amplitude discriminator wriich had 6 threshold'
levels. Another scintillation counter enveloped Y>y a 12 cm-thick lead
a:h~.cld determined the peneL-ration capabi,llty of particles. ~+) A scin- ~
tillation avalanche detector served to isolate those avalanches which
were generated by primary protons but whose effect was similar to
avalanches generated 'ay electrons. Thus, the cosmic ray electrons were
measured accurately even if they numbered only 0.,~--0.3~ of the proton ~
total. ,After processing the obtained electron count data. an unex -
pected resu,t became apparent ~'or electrons with :EE, a 0.3 Bev. The
intensity of electrons with E~ ~ 0.3 Bev and protons recorded by the
S]~Z-12 equ'~pment is shown in rig. 1 as a function of latitude. Even on
the equato~~ where particles with energies Less than 7 Bev/sec should
not be found because of the Earth's magnetic field, 0.3-Bev/sec elec-
trons were recorded. These, consequently, cannot be primary electrons;�
they are electrons which have been trapped and retained by the Earth's
magnetic field. The SEZ-1 apparatus in the ~x~otc-n�-]. registered par-
t:Lcles wit;n charge Z ~ 1 and Z ~ 2 in the equatorial regions where their
intensity 'was 1.2 (for Z ~ 1) and 2.1 (for Z ~~ 2;r times more predom-
inapt in the West than 1� the East. Tf it is astiumed that the primary !,~
protons possess the same asymmetry, the ~SEZ-1 equipment rp~orded a flux
Card
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i p~CC NR~
i AP70bCl j~~_..._,~_._._ _.~_ _. Sp~1RCh: COUL :~ UR~vO~~I~~~(~;3~/Ul:l;~i.~/' 7~/17'r~
AL`THOR: Origarov, N. L. ; Klint,sov, Yu. S. ; t~desterov, `J. Y~ , ; ~-apvport,
:I. D. ; Savenko, T. A. ,; Yakovlev ?3. M.
I QRG: none
i TITLE: Study of high-energy electrons us.iziJ, the Proton~l and Proton-2 artificial
Earth satellites ~aper presented At the A11-U~~.on Pieeting on Physica of Cosmic
Ra~ia~tion held in Moscow troa~ 15-20 November :L9b5,,7
,~Ot~1iCE: ~{iv USSR, Izvestiya. Seriya fizicheakaya, v. 30, no. ~.1, ~ ,
~ :L9b6, 1.773-17'7
TOPIC TA~aS: satellite data analysis, proton counter, electr:~n
distribution, electron flux, primary cosmic .gay ~
~~1BSTRACT: The instrumentation of the Proton-1 and Proton--2 satei mites
:included an ,3EZ-12 electron spectrometer which could register pri:~,ary
cosml.c radiation consisting of electrons with ~ > 0.3 Bev. The fol- j
:Lowing components were used for this purpose: 1) t;wo scintillation
r.ount;ers with a differential amplitude analyzer wh~~ch registered single;
particles with a charge Z a 1. moving at a relativi:~tic velocitys 2) a
gas Cherenkp~v counter (using Freon-13 at ll aim) w~xich registered par -
L'icle.s whose- energies exceeded 7 moc2 (effective threshold for protons !-_
:ts ld Bev) moving unidi:rectionally between two sc~.ntillation counters;
Card 1
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. ,
Ar *~D C _._
~.~ ~:i ati0n Of up'rrax'~.: ~,~;': - ~~~~
~ c~~ateci wiL'h back paint t;o prevent reg ~ ~,,, ,~., ~~-- ,~
j t,j.c].es. Thc~ sc~~,t11].aGitm csountcz~;~ c4ns~~stcd of :~~v,.,a .,~,c ~� , ..~~ , _-
i ~, nth lactic s~~ntj.].latoi� plate.3 1r~ mm t,hicic. C)r,~[-i~,~ c,i"` c:r~:ar;~~.c
i ~.,j.ier~ a ~' ess ~ e ~'i 1) were c;onatr'ucted frorn 1;hc E~r~~1im-
~- ~ vs. hardn l-~- g� ~ etr~ of coamic
~ x by f1u~c
~ Binary data on the longitu~.inal effect anc~ aziontfor protons, ~ spar-
; r~iy intensity in the geomagnetic equator reg
roupt~ with energies O2 1 Bev
ticles, and nucle~li in the M, H, and VH ,~
for protons and i~n the range ei 2 to lg :Bev f~~r the rema.ining(W~a ~~, �
(zv~ ,
~ Orig. art. has: 2 figures.
i
( S?JB
CODE :
~~(,
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0'PH REF : c~01
Card
ORx4 REF: 002
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-A.CC NRt w ~AP7000519 _ -_~. SOU'RCE CODE : ~'UR/00~8 f 66 f 030 f 011~1.`l~ 3~1."l6 ~-
~ Nesterov, 'l. '~f~ . '
.A~JTHOR: Volodlchev, N. N.; C}rigorov, N. L.; ~._._..,....,...~- ~~ '-
R,~poport, 1. D. ; Ss,venkc., T. A. ; Yakovlev, B-.""~f: ~'~'
O;~a: none
~atel.l~.tc, of the Crt;ili,.cci~i com-
T1TL~:: A study made using thc, Proton-1 _ .~yQ ~I
pasitj.an of primary cosmic rays in the moderate en orgy ~~~j~n v~r~~~
,,, Gc~,~.~s.~, ~..y,1-u..a. e~ Cua~..-a- ~~an}a /v~~2 ...~ ~f'lv.~-5,~.~ ~w,r. r,s
~UUltC}~: l~x~1 ~~-~R. T~cvi:r3t~.yt~~, ~~'i,y~a, f~.ri.chc~~kaya, v. ;Cy, r~c~. 11.,
1966, 1763-176+ i
TOi'IC mAQ5: primary co:~mic ray, cosmic ray meaaurement;, co~>>::~-~~ raY
t p I , ,~,,,~.~,P_
r ,Q�v~ .L'T"1~~,'~`.,-{ ~.` C~.M.,..,��.o,r., ~,,,,,,,�_-F a�'-, r..f~o Iti ,a.,,,.5.-I,..yt.~. ~.,
~--0~~'4Y` `',""` � ,~ .~ a~ e 1 I ~. t e o f t; i~.E: �~ 1 ux ~n d
ABSTRACT: A study, madE. using the Proton-lQ~ r chromospherlc
chemical. composition of sola~icocosmica~,adgiationtis descr~ibca,. A
flare.:, and of primary galac
nuclegtratosgheric dace sad the >~a1yw
by the sinking inner radiation belt at that hei4;ht in the aYUOmaly ~re-
the intensity of the magnetic fielld a~.t the height men-
; gian, 'The compat�ison of th~ia counter speeds of
ti~~ned is less than 0.22 gs.
Col>mos 4 with those of the second :ielde~~'hanwthef~meas''urementti,dWera$13e
in the in tens'i. ty o f the magnetic i,
Card l !~ 2 _.
-- -- .'...~.^.~ e
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_ _. _
',A,C~CESSION NFt: AP4041571

s~'az9~P~4/oa2lc~o3/a4a5/a4s~1
,~L~TFiOR: `-ernov, S. N.; Zlestc:roW, V. Y'c.;; 5avr,~~nko, X. A�; ~Y~nVrir~,
'; ~~, I. ~ ShF~rv'ina, K. N.
~ ."];TLE: Ge:og,raphical ir~ti:nsit:y d,istri'.~~ut;Lon of radiat~.on iia th.e reg.lan
I-i~ox poinnts (at
lesser latitudes fax L =~ 3 and ac greater laiatu~~�s gatr L ~= 4).
verti~~alt geagrapt-~c lati,tu.ds; hari~aant.alt geogxa~-hia langitu~de
Card 4/4
-,_ _~ ' -
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i
' ~4CCr;SSZOIv NA, ~'~~'4O3~i,3C-1
f're.~~uency of occurrence of ~turnras also is d.tap,l~ar.e~d in th~~ dir~~cliur, o� Y.
As, a result of inv~esti,g~3~t;Corse made on the sat:ell,tte "Kosiaosa4" i.t has beenafogund.~Y
that in a broad range o1~ ;lon$itude~3 there i,s a t~isp~,acentE-.nt of the
m.sximum in the outer rA~l,tFitinn belt; on magnetically, quiet d,a.ys il~ thetdis~Cy
of greater latit:u,~e~ then :Ls theF case on ~nagrl~:t#.c~-l~.y distut'bed days. FieCcioof
t1~~= Enclosure shone, the K~;cagraph c p,peition c~ g
c:le~,s in the outer r~diati,u~ ~'~ � ~hE~~r~axima o:E intensity of parti-
TE~1'tsov and N. y~ ~'isax~et~.kob�or; par~icipationsln I.�rhe auth+,~z�s th,~nk h"I, V,
an,d 4. F. Gorska~ya for ar:$istance iii finalizing~the~da 8p~lment, L. V. Drozdova
ed the maps of, drift paths eaC aa~ious heights". Orig, art, l~iae : 38Eiguresf andilh.
table.
ASSOt;IATION: lvana
SUBMITTED: 19Nov63
SU:B t:~1Dg; AA
{
I
Card
DATE A0f,-: 2t~!fay64
~o RSVP ~ws ~a~ob
FNCI,: 02
dT88R: Q45
~I4

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i .. _ . .........�....._........~.,..,,.,....,_. .. ._ _ .,
` ACCE5SION Pl'R: ~~P~w~-3481a1 ~ S/t32'93/l-~i/At-;x/~Z/pzgg/0295
AUTHOR: Vernov, t'f. N, ;- Meru feyeva, lit. N. ;~ Bfesterc~}t, V. Y~g. ; Savenka, I. A. ;;
Shavrin, P, T.
TITLE: Cec~graph:[c poai:ti.on 4:~ the max;lma c-f' partt~cle intEmeity in the outer
radiation belt at: ~loa t~ei.ghts
SOURCE: fCo,~miGhesl~:iye isslealovaniya, v. 2,, no. 2, 1964, 2,69-295
TOPIC TAGS: upp�;r aCmosphere� radiation be;lt:, outer r,tdial:ion belt, aurora,
radiation inCensit:y ~a~axisnum
ABSTRACT, AR a resr~].t of investd,gatians by Che sect+nd and third Soviet space-
: ships, the position of thy. maxima of icttenai.ty bf pa,rticleiii in the outer radio-
, tion belt ha~a been eat:abll:shed experime:ntall;~ at all lomgil~~:udes. Tire experi-
mentally determine+i i~wCar�sity rr-axima in the outer t'a~di~-i.iori +aelt az�~s situated .
at different longit:ud+as approximately along C.he drift p~ithfi, of the ~~~.cror pointf~.
However, in two :-ara$c:sa of Ion,gitude {fxam -l�iO ~o -~'iOo ancC from 5Ci to -~Do} in
' the northern ;E:~:~nisphc^r~a an~i in magnet%c~tlly ~:4n~ugst,ct regions L']~er�~: ~s a di~ap
pla~:ement of t~liQ position caf t:he inten,~i.ty m�r.:~cima in the dir~p~ti~:~, of gze~ltez
~~ values S,. Tn the t.tr~t oi: the :aentioned r�gi~on~ the po~3:[ti,o>..
BtdCLOSURE : O1
o ~__,~,.,..._.~..~...--~-- ~ ~-.. 00: d'0 9U 1l~7 JSt7 JB4
~ ��Jbd7 �JSO �J20 �00 -60 �v 0 0
�� ~ g,eagraptxiitioits of points of m%I,nim timuaidcountingerateeo�dthe STS-S coun-
g Open aLrculea denote eh+:I miY
radiation cour:ter:. the crosses denote the minimum
ter according to data, from thy, second s~:tella,~~� data~,�ro~ the th;~rd satellite-sh:p;
counting rate of the S9;S4~ ~cour~ter acco:~d~.~g
ll.ed ~:it~clBS denote the minimum photocz~ult:LpliFaz cmumrcai~n~c'.n~;rrat~ of ah~eaSTSoS
the f~
the third satasllite�sh~ip; ~~'ba tri~-nglaa denote tl::e mi.n ~~ .., Che ,~ wares de-
counter counting rates uacordiing to data r~roan ountex~ta~~cordi:-g~'too jata, ~~'om the ~,atel-
note the minimum cout~t~.ng ~:~ate of the 5~,S 'S ~.~
,{ sc-os-a". the solid line ie the c:oamic. re.y equator es ~:ixed by Kellogg.
~~~~ 3T~
- ._._ ~~s
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.~ ~
ACCESS~II3N NF: AP4034ti(10 S/0293/64/042/002/t)280/0288
AUT1iC1R: Basilovii, R; ZZ.; Vernon, S. N,; Westc:rov, V. Ye.; 1Pisaret-ko, N. F.;
Savenk~,~, I. A. ; Shavr~n, '.P. I. ,,
TITLE; Inve,~tigation of cosmi+: racliati.on at: heights of 200-350 krr, by the satellites
"KosmoE+ 4" and "l~oemos 7" .
SgURC,C: Kosmicheskiye i~ge~ledo~-~~ni~ya, v. 2, no, 2, 1964, 280-288
TOPxC T.~.t;~S: artificial IBatellit:e, cosmic r~~dif~tion, cosmic ray E:quatar, cosmic
rays, r,ricjiatian count:ex, inner radiation bi3;lt, radiation belt
' ,AIiSTRA.C;I': As the result o.E an ~analysi.s of the counting rate of STS-5 counters
~~arried alboard the: satellites "Kosmos 4" ar,~d "Ko:Smos 7", iC was possible to find l3
~~,clditiori,a',l points on the cc>'smie >cay equator'� rn ~lt.soymadetht poe8ir.bleitoddtscover a
t:ion of the counting rate a� tha: STSaS counts
i'elatinns;r~ip between the radiation registered b;i these counters and primary cos;nfc
,nays. T~h~ regular longitude var~tation o� t'Ihe S~:'S-5 ~ounti>,ag rates .in the neighbor-
. ~ hood of: tl~,e equator, the, relatioY-ship of th~a counting rate to the ~n,~gnetic rigidity
'cutoff of the point of mleasuremer-t and tlse ~^ege 1~ounCe~atwhich can~beirelatedato
propert.i~~s of the r~idi.at.ion regie~tered by the
c~~d ~/3 .... ._ ... _._ ...._ . _. _... ..... _ ... __ .. -
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ACCESSION Nlj: AP40~:6242
i;oc~mos-4, launc'h~=d
the 1960 satellil:e,
,~,rilWn from the data, obt:aine~i by ~ah,le of me~s-
;~6 April, 19be2, carr~i.ed an e~Ct:ernal sclt'-t:illomete~:' tai ,~r�
totes.]. er-exg:Yi ~'el'aaSe, but also thE: to`-fP.Pnclo~urepgiv~!s
~uri.ng not only
' ',titles with ~nergie.sl ga-eater that sea~~;ethe ~ene:tgy release E
' 'the counting rate I~ (partials./ct'n /
E/;~ (kev) , representing 'tti~e average ene~.f;}'
{~ie:v/cm2/sect r and ,tY-e rat:tp Values i,n the table axe aver"'
',~r~el.ease per ~;ingle rE:g~,ister~d'~ particle.
ver thy. flight s,egme~Lt falling wi.thi.n 10� of tr-e cosmic: ray
~ ;~g�.d o ~1s tail be seen, the: E/N
if f,/tv ~~~ct:ually repretcer-~~a
I eq~~ator for 13 crordlrSofol00hke'~~uallocaever,
! ~�}ues are of the of t',he r�ountez by two ~~Y~
! ~;~eadings caused by L'he simuitane~~{u~ radiation belts or
electrons may possil~~l,~ be 'relateli to l;eePThe xee-ulta confirm the
~. e:i~ct:rical roc2sserl :Ln th~~ ionospher13� lOz to 105 part:i~�~
~ oaf law-intensity ~
Prest:nce, apar~antl,~- ,const,~-nt, ..
s$cr.atexadi~tn,1 elan t'ron nra~os~I~B with energies greater�.t an~, }
1 - -� ... ~.. ~'
~ ; c.le/+.m / ~ ....
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y402b;142 S/0:'.93/E~4/OOZ/001/Oi50/U1.5~3
ACCESSION NR: Al, Neaterov~
` Shavrin, P I ; Pisarenka, t3. F.,
AUTHOR: Savenko� I. ~'~� s
V. Ye.; Te1'taov, M. 'V.; Xerafeyeva, V. N.
~.nt of soft radiati.ot~. in thc~ equataridil latitud~.a from
TITLE; Measureme.
the "Cosmos-4" s+3-teZlite a v~. 2, tto. 1, 8964, i50-153
SOURCE: Kasmich~i~,skiye issledavaniy ,
~: r ~ ~ cosmic ray equa~t:or,
~ radiat:io~n o~-Pasursment;,, rACiiatiom belt ~ soft radiatiL+~~i,
'~ TOPIC TAG:i: Casmos~-4,
satelli~We ra'di~ation ~ICausr.ula1rtradi~at:ioxi
sputnik,
count rate, ener.l~,y re. l.~.ase, .cD~rp
utni.k (19-20 .At-gust 1.960) carries a
' ABSTRACT: The s~l.conf the part i c i es ref the
~rrrifirial radiation ~~elt ors appt`oxi7~ately 3 rnonti7s. f'ar art>its o{ 2i0�3E,~ lr~;~ the
dose caused by the artificial radiation bolt 20 days aster it:s formation w~~s aln,r,;1:
,;~ tIfT1G:i a5 i~-lrge �3s t~"1C dos,t CdUSCd 1)y CO~fI11C rcl(llat1l7r1 In t:IIG rl~itU-"al I)nlt5,
{- h E:
depend~nCe af` the n~eall da i I y i tat~~ns i ty caused by the r�~~e~ 1':ram ].0 ~;~~trt~.clr_:rl . c.m~~-'
,~ ,ec`1 at h~ j~0 km (o:rb.i t�~1 :,h.a.p ];l) to~ ? part.i.cl�~f~ .ct~"~ ..:,(;c~'1
~~t h-~~0 ~;m (or~:~it~.l ~aip I.1:1). '1'hel~~e o.re 6 f'i~ure.~ rarad 2 t~.ble~.
.3U13;ti+I'.L"~.'~D: ~F,i, ~;~;mb~:.~r 12, 1~.~E~1
i~e1~d 2~2
APPROVED FOR RELEASE. 12/02/11 CIA-RDP86-005138001136700032-6

APPROVED FOR RELEASE. 12/02/11 CIA-RDP86-005138001136700032-6

~~I' ~ _ r
~ ..ip~ ,1' ~ ` ' i
~� ~~ _' ~~c~~ ~~Ut
,~ .~
,r~u.E~,~atfotz pradt~cec~ in chromos~~heric '~aursts ;, can present a radiation'
~ ~ , ~ .
,'1~:~:~tax~d. i~C-tXl(~ data on cosmic�r~adatot~. ~~~ dur~.n~ 19at~-1959 are
s ~ ' ~ .~~,:st~d.. a~~rstemafiic ~orccasts of s~olaxF ~ur$ia Accornpana,ed uy the
~'` '~etns~>aon ~a~:. ccsm`c radiation ~~e very ira~porlrant for the prevention
_ ,' ' ~.~ ~ c~~o~~r~e ~Q x~~d~.ation ha2ar~!� Suc1~~ n method o~ �orecastin~ could
~~ `-'b+~ t~ rc~+~~~d~:~ ~~ ~ xadatt~.ax~~ ot~~ the 6~pace ship. I~ the theo~-Y
,: o;~ tk~~ ~x�~.~~in o� cosm~.c rarliat~.on, dev-el,opecl by '~.~. ~habanslciy ands
}` ` ~~ ~�~~~. ~ev~t-;~'iyy .is t~;~u.e, thin any ap~:~ea~;~anGe t-~ c�s~~3.c radiation ut .
,_`~ ~ tli~ -n~o~n~t ~,� soi~" burEts ougY~t to b~. acconrpan~.ed ~S' the mission ;
1 ~ ' .off ~fxm~a ;r~~tiation. St~oming u~, the ~tbsoxl.~etd dose-rate is strongly
F~'', she ~l~.ght altitude and
z~ ,. ~ d~~~~eY~dent can the incl~.nation o~ t'h~c- os, bit, !,
~~,;~~ t~icl~clc~~~ss 4~ the space ship's proi.ectioYt. There are 14 figures
;.
~~ ark; ~- tab;l~~~~.
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_ .j`~:
�` ,'IF
Y'
I:
~~�
~;
Fry~~
v.:M~ ~.
i
1;)i: _
~. y.k ,,
.. ., _ ..._~,... ..._ _ ... _ ._,_, - . ~-a~s5~ 6z/i~02/aaa/als/a4a
/7~M5 3a~.
~i icy 4i ~t. [o~~ti ~~~'~. ~ -
axtd Y.h+~ ~,a~;:ytude o~ absorbed dOome~rf~
Y n~ ~p1~lc d~ atrlb~xtLOn me~lhs of rod
~. .Chi ~er~~i ~ ~tlese resu~.ts were abta~.ned ~y xhis '
.'a ' ~ '. ~ ~:~~ ~o~is:i~t~n~ o~ sca.ni.~.~~~.aria~. a~h~ ~ ~~r~:ooE th~sr.~diation, ~'
r ~ ; ,.+K~~~,~mtw
~� F � . t?t~ta,~~t~1~n'~, e~~~~ the det~rm~.n�ra~1~3.~1e~ ~tzd ~o ~.~~:~~ure tt~e~�a~cit~e~~
~~ tht: E. Y
~~~ ~:s~~,m~~~:etR'~ey~,~}ty~~"~ry{ m~rctory' cle~v~i.ces -a~.,th ~~ l~.trur i~to~a~ ~t~,ro ~1,ohe .
` Icr +~4~s,r ~.{. ~Ydlt~ ~. Vy ti G[i1~+ti�
, .~:. a~,s�~bl.+w ~~ ~anduc'~ ~h~s~: mea~~ix~ ~t~e a ~~ g~3umr+~d f day far the
,ras g .
k > ,~~ ' ; ~ abaar~ed dose rate Eras .
~._ ~ .~h~ ~3'V'~r,~~:~,e ~ ~~ " s res~ec:t'i~rely; the a.l~sarbed d�se-x�a e
s~oand: a~:~c~ ~~xd ~~'~~ ~na.~ ~ ~, ~, 7 rnrad, de~endin~
r, s vars.~d,~r~.t~~~r.~s~?~ct~tQ the rac~a.at?on '~~1ts,
,~ `- :R,ns~;ct~ t~l~c ,,,pace sh~.g .
~~~~ ai Mori of the or ua~
~; ;~ +~n t~kie y ~ :~~o ton ~:lu~trs a~' the iuternAl 'sac? t ~.~ t ~~ re
r 4_}t ' ~ :tt eras f'i~und ~hc~t the F ,~. v,~ a ,s~at~st~~n.t i.a~ can~:r~.butian
~f~he ~ra2~.3.ian ~~.atnal.'y may ;~-~ ~ is
- ~ . ~~ ' r~ off' ,~ ~ . ~ and ~ .:~ rnrad day .
~?~o Thy aver ~.~~ dos'.-x�ate :a~~ 3
. ;. ik4 the d?~sert~ate. ute.~ ~~ S~t7 'l~n t'k~~ al~~3cErbe~. da~~-hi.~h a~.t~.-
~ $ '~lU~ Clr~~'1, , 7L`7,.TS~~";~' ~4wi~:l:L~ ra.G,~al.zan
,;- ~ ,Che ~rea~xtoe a ~ ~~~.c~~.a~~~c~~:L ~:C~~rts
r ~ ' ~+.~ ~~x~ad F~1~iy . i,ho~a,~~i. r,~r. ~ , . ~ ~~tt s o~ not
,~ i`~ ~'~ i~u+w~~ t~~'',~ ? *~,~ ~Co same s~ec~.~~.c, ~;n ~tr~.~e ea,~e a~ f~.a.u
,~' . #~hi~~ ~x`~,y__ not. obaexyv~~ a~~ se r:~ I.eve: .
titu+~~a v~T ;~~-D�~34'~ ~ca~n,, +ar~ly so~,ar ac~~~r~~.a
t y _._ Y
I+
~.
~.~
.. ... . .:.. ,-i-
APPROVED FOR RELEASE. 12/02/11 CIA-RDP86-005138001136700032-6

.. - - .~ -- t } .
~~ ~~ ~f~~~ ~~/vas/~os~/oi$/ova
,, tt ,
~ ~ .k~ti~~~'~7'~
~~r~t4~rraY ~.
T .~~w � ~ ~~1.~FRNM~i!~ t, l~{,~� } 5aven~ca, ,i ,Q�
and

-~. 'lii
'~~~~'~s - _
~ ~~~o~~~
~adiatio~+~' a~G` ~'~titudee of ~.80~340 km
and
.
~ ~:~3~`.. ~ ~ -
~f~ ,r ~ ~ ~t-~~+ r~r~N~{/i~ ~~ ~~~ LN~~i#1~~~ C1 ~'fe~kl~ ~~iM~4i~{s
_ _ ~ aa~
'7
. ~0~1~~~~~:;
` Preblem~r l~crrsmiche~koy ~b~alogii, v', ~. Ed, by N.
zd-vo S~SR,
1
~~oscow
l
V
`~
~
%
d die
1962,
~, : kya~t and .
.
,
.
o~.g
�:
!y
a~
< 170190
,,
R fir-
~~~~~p the t~xperiraents, cond~u~c:tecl on tt~e Second and ~1zi.rd
~' ~~ao_,~ .Ship y~t~lded the following n~~ ~~ulta: An external rada,at~.on
''' k�" belt t~,k~, the earth was detected at an a):ttude of:' 180-320 lan; its
' ~ ~ honrR+~~~c~.es c~ex~e del~.m3tcd at a~.~ lot~.ga.~;udes. '.t~~e dependence of the
nte�~~ity' ~~ laxt~it~de wad, e~tabliehed far the e~:ternal radiation
~. is ~ `belt., the ~`:riten~t~ increasing sharply i~ the ~a~.th ~t~.antic a~ ~.n
~; o~~e~~ re~~ona ~ lbwer~.rig of the internal radiation belt to 230-
; .320 ~~: ~aa abs~ex~ved in the region of t~i~e ~xazilian magnetic anomaly.
~. 'tie ct~,~t~~:huLion of cosmic radiatiaz~ around the ~;labe was measured.
r hard 1 ._~_.,...~.._..~~..:,~..w._~~.,.:~..~w...:.~~..~..,..,~.. _.~ -~... ~__.__.__._..~.._r__...~ _.... -. _
- ..__.
~~.
_ .
-_
APPROVED FOR RELEASE. 12/02/11 CIA-RDP86-005138001136700032-6

APPROVED FOR RELEASE. 12/02/11 CIA-RDP86-005138001136700032-6

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~~~
J ~J G
~~

U"'HUI~~ ~
? ~

VE;TnUV, J ~ PJ , ~
Cc~rrr-.~}pon4~a.n~~ ~~;ii>mbc~r :~ t;i; ,~J~~, J 1Vt !; l`.t~r
c A~ U~
~
.
r'
:
'
~ I . A~ , Shavrin, Id~~steruv 'J ire ~ ,,
)J ~ I ., , ~ } .
,
~
~s:.r., . ,,,
ndt
...
,n, ~~~ U~at~>r I:~t~rji,~ti.{,n ;,~~l.t r, f' 'r,hcs F;;~.7.,t}, ,~, ;,,~, 4'...~ ~7.t~tu;J{,
~~.1'.i~~Vl)1CAh 3 ~iC�lCt(;1-11}I�:! T1i.111iS J~J~~~ laO1Ca.�~('~y ~ V ~l~tJ~ �1t1 /~, ~ Jfi~ , ( ~~ .. ~l ~ ~
TEXT: The second ~aviet satellite w'tiose orbit w~.s at :gin aitltude of 3U"( - ~
3j9 km had an auton~~atic storage syst~:m w~~ich r:n~bled it to rne~~:~ure contin- ~i
uously the radiation intensity in latitudes of +65�.. The scintill~ti:r. I
-1F~(H'EU-16} pl~~otomultiplier ,end ~.~ i~aI(T1} cr,~sta_1~
,,
ccn~ntE3r cc~nsir~tE:d caf r~ ~3~ �~,,i I, s,
The energy t;hro~~~'~t~l~~i c, 1' t;pi.i~a ~~t,ur,t~~r w~~., ;~`a k .v. 11r1
counter was also used. ivieasure-rients sh~~~~rred that t~1a c~~ui~t~.n~f r.~t~.~3 ~.,I' titr.s
scintillation counter, from the ,~tluator to latitudes of 1-~}~ �- >v�, i.ncrz~d
sec to 10 ~- 1?_ ,~ulses~crr~~sec In i'~titl':7.eS fro!::
from 3 - 5 pulses/cm~ ~~ '
+5~� to +65�, t1~le counting re.te increase) to ~'~C - E~OO f,a~.:,es/cm~ ~ sec :.rl
most cases. The authors :lssurne that this increase lr. x-ray intensity i~~
caused by ~~artialeu of the r~~di~~ticn belt of the arth Ta prove t'r~is
C~~rd 1/?.
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E; ~at,~x� of cosmic rays according . ~ ` ' %.u' _ A., 5havri.r-~ P~ I.~. r+ea.~_c,v.t~.....~..~___~.
N. ~'.
"~' ~'I'i;E, F E~.~u~tor of ooemic rayt~ ~-~.cc~rdAr-~ to data of the second
~~ soviet ~paae~hip
CALs Zhurnal ekeperimelntal'T7oy i r:~;.~retirheekoy fiziki, v� 4~,
~;' ~1 L t
~~L;': The use of earth sate~lt;es frr ,ier,ez'::~t,ing ~ da*ermined
r~~~yk, ''rom whic7Y the structure oi' the ge 71rre~,.t.te'.'s~+f r~fi t~t~.eas".he~~~,Et:cai. and
and jvi-ich pexmits the crieckin~ ,~z ur,e c~
emx~ix'ical approximati~~n of this field offer, 'a eFU~4tox~~f~~ostnic~raysiVer
the measurements made on the earth. thus ~ ..t-� q ~ sn ~;� accurratel~~
and especially i.t� effect, on th~a geophy~tii~;s..i phenomena
~rhe second spaceship -~1so con.taxrAf~~a a ga~~-discharge counter
s.i.u~~..ifAd, ' 1y iztt,erroga-
wY,~,sa pul.se5 v~ere fed tc~ a zata matez� x';x~~,h vr~,~i a?.it.omr.~t ''{~~.
tr.ird :~,nute < ',Jpon ccrn~iiar-d from
ted 'ny a diurnal storage system eveiy
tr~Q earth the information stored by this sy`'' em v,as Y�r =nsm~tted to the
i~ax'~+,, 1/~
Y~
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APPROVED FOR RELEASE. 12/02/11 CIA-RDP86-005138001136700032-6

APPROVED FOR RELEASE. 12/02/11 CIA-RDP86-005138001136700032-6

APPROVED FOR RELEASE. 12/02/11 CIA-RDP86-005138001136700032-6

`~11i; c()~+r(-1C^-K'~~y ertllFltor
3/~,tJ~)/ti.l./~i{iii/~~, f iJ rt/ J. ....
i, U ~, .. /,~ �, 1.
1,
-2 h' T-'at,lcuv ::t ,x l.. (,t_t'r of co~tutac i'~zcl:~~-t;i.l,t- iur ,~.l~.1: t.r~.iti,tt.
across the equator. Zt is noted thlt the co~;mxc-ray ~n< ~1ct~:-,1111,
SU(~l~C~ : f~.lci~iCl(~fi1.1 ya 111.111}`: ;~.~:~ f) . ~:-i14.115 S l.'V(,;;il V i 4' '7 ~)I! t:lii.;. J ,I r ;;I) !. .
no.l]-, Mc)scc):a, lyf~l. i~c~~.:l't.i-tty rtIca-ktl korak)1.c,~- ,
T~kT: It is 1)o~-rtte(i uut t}tat t:he use of stztel.i.::.r4~ti II1
determination of the cosnLC-ray e ,u~rtor, i. o. the ,~cu~r~.1t)zlc~t i.
pcs:~tion of the line of rnini.lnum intensity c>f r,rir~ary co::::lic rar~~.~
7T1 "t Y.)i"r;V:1.~711i3
has many iidvantac;es over t~:~rrustria:L meclyurer,tertt2~
paper the authors rel~ortecl the ciete;:~min.zLiort of r~t~i:tc~ t>r1 tlti:~
equator' wit1~1 the alci of the :~ecc�nd ~:;osrizc Sovi.(,t ypllct':,c1,-:~ lilt
or,.ly 2U hours. Tl-le apparr,tus Inount~~c~l oft r,}le t:hi: ~' s~)ac~;l:s.;)
~.
included a has-discltarc;e hako~en :. ~i~ ,_ ' 7 ~.~'-r~-`~) co;~ntt:r ~.~nci ~.;
scintillation counter. (~aZ:TI). T.Ile counters ~�:ere p.ka(.eti inszcle
the s ceship and were surrounded l,y a :screed of i~ettae~tl ~; and
Card 1/~
a
~.~
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APPROVED FOR RELEASE. 12/02/11 CIA-RDP86-005138001136700032-6

~;; c
S/'~,G� ~~looo/c~oioo6/o1~
D299~3a2
Cosmic ray equator~~~
Thereby, it i s nc l~~nge:i
~hys~.ca1, phenomena or_ its positi.on~
necessary to introduce barometric tf?mperature an{~ temporal��
variat~.on corrections ~> Thy, eauiprrleni; of t}~e 2nd SoviE~t Sput7~i.'~
contained a Geiger ~:ounter,, ~~n aui;onamoue mer:~ory~--~dev~i-ce ~ arjd
a aratus, The memory device permitted measuring
telemetering pp
the latitucb dependence of pr7.mary co~~~~c~.nadtheldata~ the err ~
:intersection of the equator , In 1~ro ~ �~
t~~~~ la~t:'tt~.~cie ~lcpendence ~~~~~s rc.~~.- ~, ~(
pl,r:,.cal .f~o.rinula descr.ibin~; ,,;int:~ fc~~~ lat~.tudc:., bk,.~c,y~,, 4C-
structed only from expertmen"dal ~
Twent ==two yatitude curves, obtained fro deter.rriinentheJpc:sj.tior~
y u~~tor ~ rrc;re uses t
of the geograph~.cal eq ~ ~ e� y t}~e equator c)f
of the minima cf cos~r~~c.;.ray intensity ~y,
~ ~ 7!he obtained equator of cosmic radiation ~_s
co~~mic xada.ation, ~ ' `1''n~:
yn.ompatib~e vr~th a d:ipal.E; rr:,cr~e~. ofy t;~t~; i,
obtained equator is ir. food a~;r~'eruerit ~rrifi~r~.ulatfydr~bcu~l�lyc~;~`;;;'
~uenby and Weber , as well1ajciy~urte ar..dt8(nor~sSo`J:Let~t)1. ~~ ~�
ar~d Sch~�artz : There are ~
Gard 2!~
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.. ~,
;~
;�1'[4~ ~ r~U~1 ~~'D~,~-~D~, ~'~i:a~ ;;~SE~()~61,/lC)~}0/~1~/I.j~G~~)1~+
1
D2~~)/D302
Savenkoy y Sha'~'r:in, ~'� I ~de:~terov,, V,
AU`r~~o~~s ~ r . A.. ...
Ye ,. S; a.nd ~is~renko k N ., F ,
,I,1,~~J, Cosmi o�~ray eq,uutor f'ror.~ data obtained by r~euns
of the 2nd Se~viet 5pu~tni.k
Akade~ny~~ rial~k U~~SR. ~I:~k:usstvennyye sputnik
SOURCL~
Zemli~ noo 'f0o P+io~;co~r~ 19b1y 45x4?
TEkT ~ The use of artificial s~~te 1~~-llov In ~radvant~~~es~~overe
equator of cosmic radiation h~.~, tYie ,.ol g
terrestrial investig~~t;ions ' (,1) many intersections of~ iod tea``..
for at various points d'.~ri.ng a cor~~pa:ratively short ~'
(2) dirE�c t recording; r~.f. t.hP ~,rlmf~ry ~~omponent of cosmic radia-
equ~a.tor ~~
tion~.~hencey the pos.3ibi~l.i..ty of ~~ de:tailf~d :study of the artic~u=
of cosmic radiation at various moments of times ands in p
larS the possibility of ~;tudying the effect of various geo~
Card 1/3
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APPROVED FOR RELEASE. 12/02/11 CIA-RDP86-005138001136700032-6

pater radiation belt of 39 km over the .,ntir
Card 1/4
-�
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APPROVED FOR RELEASE. 12/02/11 CIA-RDP86-005138001136700032-6

APPROVED FOR RELEASE. 12/02/11 CIA-RDP86-005138001136700032-6

Detection oP ~lvw ;ye~:.trona
~6easuring the Humidity of
! ~.> F rzx
~? ~ - !' i' Ca v :x ~ttl l LlL1 c~ h e n
by ~., ~ ap tur~~ ~.r~d ~ ,..'.~ , ~� Neutron
the .',ci1. ~.nd ita~.rl,r ~.~.y ~'.ear::~ cif t;Y:e
Method lace
late) to determit.e the thertn~~d~r, `'~~ au5{:dtlie~ cadmiumnrapio i�
p of i a C?J`3~.1'~--- 1?
of me~isurernent~ Ibis ~ r..~,u ,n dr-ns3a.ty. The results ob-
pz�oportionaJ. to the thermal t-~''-
ed b tYie field tf~sT wex�~ ~or,E,ar_F~d t,~i.th tlac~se obtained by
tarn Y r ~ and a special
a. 1>ozon pro~~,,'~~-ona] � ^~~~-te~ S:,1M�~~ v
mear,.e of .~ .,~^, ~ e~ ~ Frm lif ier dis-
rad?.ometertubs ~~ 7tl;e re;~ults obtaineu:
tubas: PQTK;;..,~t~ ,-.i ~ ,.~ radiation
criminatcr; ~^ ,~