SCIENTIFIC ABSTRACT KOLCHINSKIY, I.G. - KOLCZYCKA, Z.

• Document Type: CREST
• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R000723720019-0
• Release Decision: RIF
• Original Classification: S
• Document Page Count: 100
• Document Creation Date: December 30, 2016
• Document Release Date: June 19, 2000
• Sequence Number: 19
• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT

KOWHINSKIY-y- I-OIGO--
Influence of the Light of Stars on Refraction, Astron. Zhur., 25,, no.6,, 1948.
Member., Kiev Astronomical observatory,

Kolchinakly, 1. Qs - "On corrections to the talles of star color refractions".
Publikatsii Kiyevsk. astron. observatoril (kiyovsk. ros. un-t in. Shevchenko)..
No. 2, 19.1+80 p. 81-90j - 'Bibliog.- 15 items.
SO: U-30429 11 March 53, (Letopis Murnal Inykh Statey, No. 8, 1949).

ZNMMZIT* 1 0.
35162, 1 Toproon 0 Tdwvon Isommit Solsochay Aktlvnootl. Wletan'
Koldsoll PC Iseleft"Min ftlste& (Akd. Unk SUR), No. 2. 190, a. 9--10
SO: Lotopts' Zbwualnykh Bt&UW, Vol. 46. 90skys. 1949

KOWSMIT, I.G*
Oose features of the distribution of eruptions on the solar disk.
Pabl.liev,astron.obser.~no-3t43!-53-.'50- (MM 7:9)
(Sun)
.1

IOLCHMM, I.G.
- - - - - - - - -
Two methods for determining atmospheric dispersion. ftbl.iliev.
astronoobsore no*3183-92 1150. (MM 7:9)
(Dispersion) Wars-Akdiation)

*17,--,~'~lt..-,-"V..--"~-rmt~~ED4t,%PWE-.~ADW!M%~.4.1*1-ewwI lmiolivysiu-7-Itfl-avwlr-~;,~R.~f2!kip~IS-~,iE~?.,F~~t'le~~,D~~~.rzl-~,z~1.1~!~. "7m,
- -
BOGORODSIff, A,7.-, ZOICHINUIY, I.G.
Distribution of sunspots in longitvde. Fabl-Ilay.estron.obser.
I . no.4:41-47 15o. (MU 7:9)
(Suspots)

;el
IV
AV

General* Scientific-Popular Literature (2032)
Hauka i thittya., No 6,1953, pp 5-9
Kolchinski:r, I.G.
"How So nee ForsteUs H"venly Phenomat"(ftrainian)
Te3.19 of the discover7 of Neptune and-Plutos and of the periodicitl-of
the appearance of comst&.
SO: Referativayy Zhurnal-Astronomiya k,G~odeiija,, No 1, Jan 54* No'2,, Feb 54;
(W-30785, 28 July 1954)

KOLCHIRMY, I.G. (4yev.); COUPRINA, R.I. (Kiy*V).
Observations of Mrbos-Kondal a coust 195)a at the Main Astronomi-
cal Observatory of the Academy of Sciences of the Ukrainian S.S.R.
Astron,tsir. no,142 -.1 8 153. (KWA W)
(Conte--1953)

KOLCHINSKIYx 1. G.
"Rapid Variations of Refraction and.Their Influence in Astronometry."
Trudy 10-y Vaes., aBtromatrt konf..S PP,92-94t 1954.
qmall variations of astronomic refraction in the course of short time
intervals of the order of seconds and minAtes are discussed, Observations
confirm that if the flickering of the images is due to small-scale turbulence
in the atmospherep then the mean square value of the amplitude of flickering increases
in proportion to Lj, where L is the "Air mass" passed through by a ray in the
atmosphere. The importance of the study of the twinkling of stars for astrometry
and for the study of turbulence of the terrestrial atmosphere is emphasized.
(RZhGeol., No 9o 1955)
SO: Sm No 884$ 9 Apr 1956

30010HINOXIYI I.G.
Imot positions of PlAor Plamet Juno. Astron.tair, no-1,53:6-7
0 (KEBA 80)

---- - -----
and GAVRILOV 1. V.
IlComputing Corrections of the Moon's Coordinates from Oboarvations of the
Eclipse of June 20) 1954 at the Main Astronomic Observatory of AS UkrSBR"
(Total Eclipse of Vie Sun, Tebruary 2~,, 1,.'.52 and June 3o, of the
Expedition to Observe Solaar Eclipseis) W scow, jz4-vv tVqp, ~.57 P.

Tho astrogroph. at ths Ibis Astronomical Obsorwatory of the Acadow
of Sciences of the Vkmisisin B.S.R. InAlave*astron. abser.-I no.2:
156. (MM 918)
(folsooops) (Astromosioal photography)

OWHISsnyo 1.0.
--- - Mw
Accurato PoOltions W ths minor pbwet Juno (3) &ocording to
phatographical'observations nods in 1952. Isy.Glay.astron.abser.
i--7al.2z37 156. W& 9: 8)
(Pl"sts, Nlaor--3)

MINIKOV 0,A.
KOLMINS
Conference on problems of-stellox scintillation. Antroa.zhur#33
n*03: (WaA 9: 10)

"MIMTO I.T OMINA. AoBo
,7 resmltg of proosellus photognphe of gala3ded Mae for
compilim a oat&log of f&lnt gtarso Isve Raw, astrono obser, M
UM 2 no,103-91 ~57,, .(KrU 1292)
(ftars-Rhotographic waftnuents)

AUTHOR: Kolchinskiy, 1. G. 33-4-14/19
TITLE: Some results of observations on the fluctuation of images
of stars, carried out at the Main Astronomical Observatory
of the Academy of Sciences of the USSR at doloseyevo
(Nekoto37ye re-zulltaty nablyudeniy drbzhaniya izoora=eaiy
zv,ezd.na ploshchadke OAO AN USSR v Goloseyeve)
PERIODICAL: Astronomicheskiy Zhurnal, 1957, Vol.34, Nd.4,pp. ;8411.
ABSTRACTs Fluctuations in the images of stars in telescopes are
considerable interest-at the present time for the following
reasons:-
1. The amplitude of the fluctuations is one of the
criteria for choosing a given place for an observatory.
2. The fluctuationsg as well as flickering in the
intensity of stellar light, is connected with the turbu-_
lence of the terrestial atmosphere. For this reason
the fluctuations can be used to study turbulent non-
uniformities, their motion, size, height etc.
3. An analogous-phenomenon is also observed in the case
of the propagation of radiowaves in the atmosphere.
- Observations reported in the present paper were carried
out photographically on the 400 mm astrograph of the
Card 113 Main Astronomical Observatory (F=5.5m). The results were

33-4-il
some results.of'db"rvAiio:ns on the-fluctuation of images o ItIaIrS,
carried out at the ~Jdxin~-Axjtronomical *Observitory of the Ac&demy
-of Sciences of the USSIR'it Goloseevo.
~Aiiined ~etwien"1955 and IL 1956- In this. ast.rograph
~~7 "4 'corresponds to 1mm-
The- amIplitu do &'lluctuition is defined as the mean
qsquare-, value - of --% the deviation of the: given track f rom
hAve-been*obtained had the fluetua-
'tions mbeen:~'absehV~"- ~:Th6-'deviations were measured*
pe rpendicula rly, to.: each track. It is shown that
amplitude as defined above is proportional to Y'
whe-re L is the mass of the air. There are some deviations
from this law but the reasons for these are not -yet clear.
The dependence of the mean.square amplitude on L is in-
agreement wlth~theory- The fluctuations have a period of
the order of a few seconds.
The dependence of the mean square am litude on tem]2erature"
is as predicted by the theory. The 9~stribution or
am-nlitudes, according to their magnitude is Gaussian.
1.V. Gavr'ilovat A. Be Oaeginag and Yu. K. Filippov also-,
Card 2/3 took part in'this work.

flit
It
Ity fit I - t 5 !F
Hit
1 14
P-1 I
WT,
ISO
ix fit 'it
oil 1*

-k~ J~
SLU"OVA, To.Y. Eftadakmo-IN.Ye], koad. fis,!.Mto nauk; XOWHIMIY' IOGOO
kand. fiso-wt,-naWro M4; IAZ M&79, red,
[ThimulN oalsstUl phanownal "Isoychainil usbasui tanshibs.
J~rlvo To-vo dlis posbynmda poUt, L nauk. snan' =4 19580'
34 p; (Nm no
(Notoorologloal optios) (Astronomw)

UKOYKINP Avenir Alsksandrovich. Prinimli uchestiye: 0ORMU=, Sh'G,j,
jumahnyY notradulk; NOLCHINS4
. XJ,&,,.uauchnyy sotraftik;
~~-X~s,:~trudrtlki LMW
SATKOVS11Y. M.1 kand.
fizIko-mnt9mmt,n&i*# otv.red.1 LABINOVA, N.M,g red.isd-val
MMYAROVA, V.Te., takhn.rods
[Artificial earth satellites] Iskusetyanuys sputniki samli.
Kiev, Izd-vo Akad,nsuk USSR, 1938. 46 p. (MIRA 12:9)
1. Glavnaya antronomicheakeya observatorlya AN USSR (for Gorde-
ladze. Kolchinskiy). 2. Institut teplo'energetiki M USSR (for
Saykovskiy).
(Artifloial satellites)

TranslAtion.fromr- Referativnyy zhurnal;
(USSR)
AUMORS.'r Pavrilov, I.V,, Kolohinskly,
TM9:
69365
SOV/35-59-10-7855
Utronomiya i Geodeziya, 1959, Nr 10, p 24
1.0.
Determinations of the Corrections of Coordinates of the on Through Obaerv-
ati*dn'of,the Solar Eclipse Which Took Place on June 30, 1954, and which was
Observed by the Main 'Astronomical Observatory of'AS UkrSSR
1954.
PERIODICAL:- V ob.s Polnyye solneohn..zatmerlya.25 Febr 1952, 1 30 June
Moscow,
As USSR, 1958, PP:324-328
ABSTRACT:
Card 1/2
Observations of partial phases were carried out with the'astrograph of the
MO AS UkrSSR (D 400 mm, P 5, 500 m) near 'Kiyev. The southern boundary
ofthe.total phase-paased near the Observalor-j. -Observations were carried
out when:the-sky wasnot-quite.clear. Altogether, 36 photographs of partial
i6aaes 'were obtained, but it has only been possiblwto process 18. The'
measurement of th6-plates and their processing was carried out according to
the method described in the A.A. Mikhaylov handbook "Theory of Eclipses".
The -ooordiiates of the Sun and Moon were taken from the Astronomical Annual

69365
SOV/35-59-10-7855
De.terminations ofthe Corrections of-Coordinates of the Moon Through Observation'of -the
Solar'Eclipse Which Took Place on June ~0, 1954, and which was Observed by the Min
Astronomical Observat-ory of AS UkrSSR
USSR, without any corrections. 2he following corrections for the coordinates of the'
Moon were found: 4:lot -0" .684-6" .41; +0-1 . 2840" . 12.
S.G.M.
Card

KOLCHINSKIT, I.G. [Kolchyns!kxi*JkH*I, ksudoflz.-mat.uauk
Artificial satellites and religious f0los, Vauka i Shyttia, 8
no,4:37-39 Ap 158, (MIRA 13:5)
LArtificial satellites) (Atheism)

3(l),24(4)
AUTHORSs MellnikovtO.A.., and~,Kolchinskiyj.G. SOV/33-35-5-19/20
TITLEs Conference on the.Twinkling of Stars and on the Problem of Wave
Propagation in a Medium With Random Inhomogeneities (Soveshch&ni-
ye po merts&niyam zvezd -1 probleme~asprostraneniya voln v srede
so sluchaynymi noodnorodnostyami).
PERIODICALt Astronomioheskiy zhurnalt 1958, Vol 35, Nr 5, pp 819-822 (USSR)
ABSTRACTt Place of the conference and time: Moscow, June 18-20, 1958- The
congress was organized by the Astronomic Assembly of the AS-USSR
and the Institute of Atmospheric Physics at the AS USSR Committee
of organizations A.M*Obukhov, Corresponding Member of t~e AS USSR,
O.A.Mellnikov,-Doctor of Physical-Mathematical SciencospProfessort
N.I.Xucherov, Candidate of Phyaical-Mathematical Sciences, and
younger scientific contributors of the Astronomic Principal
Observatory t.11.Zhukova.
Participatorst Scientists from Moscow, Leningrad, Kiyev, Crirwm.,
.and Yaroslavl'.
The opening address was given by Professor O.A.Uellnikov. On
June IS the conference heard reports of A.M.Obukhov, V.I.Tatars-
kiy, V.M.Bovshbverov (read by L.R.Tsvang), A.S.Gurvich, L.A.
Chernow, 1E.N.Krom, E.L.Blyakhman. I.G.Kolchinskiy, S.I.Sorin,and
Card 1/2

Conference on the~Twinkling of Stare and on the
Problem of Wave Propagation in a Medium With
Random Inhomogeneities
SUBMITZED:
Card 2/2
SOV33-35-5-19/20
others had a share in the discussion.
On June 19 the.conferenoe heard reports of L.N-Zhukova#A.H*'
Demidova, R.G.Vinogradoyap H.V.Bystrova, G.Ya.Vasillyeva, N.I.
Kucherovt Sh.P.Darchiya, V.A.Krat, Id.Kerimbekov. Discussions
Ye.Ya.Bugolavokaya, G.V.Rozenberg, P.P.Dobronravin, A.I.Zinkovs-
kiy, N.V.Bystrova. FUrther'reports on June 19: Academician,V.P.
Linnik, Yu.A.Sabinizi, N.F.#Kuprevich, N.V.Bystrova and Yu.S.
Streletskiy. Discussion: G.V.Rozenberg, A.M.Obukhov.
Questions of organization have been discussed on June 20s
1. Election of the committee "Optical Instability of the Atmo3-
phere" (chairman N.T.Kuche'rov, secretary N.V.Bystrova)
2. Election of the editorship for the publication of thereport
[A.11.6bukhov, O.A.Mellnikov (editor), I.G.Kolchinskiy, W.I.
Xucherov, H.V.Bystrova, L.11.Zhukova (GAO ks USSR), M.A.Kalistra-
tova (IPA AS USS101-
3. Reaolutiont Next congress 1960 in Kiyev.
The three points have to be confirmed by the Astronimic Assembly
of the USSR. As a representative of the Assembly GO.A.Leykin
participated in this conference.
July 17, 1958

- -Z-1j%va
Go [Zoichynolkyl, loffol,kandefiso-matonauk
Trimph of scientific foresight. lauka I sbyttla, 9 nool:47-
49 J& 159. (coasts) (MM 12:1)

-KOLCRIOXIY
Invest1gating the scintillation of stellar images in telescopes
IZV,GIav.astroujObB8r-M URSH 3 no.2:27-67 16.1.
Stars-Saintillation)
ff 0-11, 11-M-MIN R.""t

S10351611000100910131036
AOO1/A1Ol
;J--0 AOS76 )OS 7)
AUTHORi
TITLE: Preliminary,remats ofinvestigating tremor of stellar images at
the Main Astronomi6al Obsbrvalwry, AS UkrM
MIODICALs Referailvnyy zhurnal. Astronomiya i Geodeziya, no, 9P 1961, 31P
abstract 9A244 ("Tr. Soveshohaniya po Issled. mortmaniya zvezd",
1958. mos6ow-Leningrad, 1959, 145-155. Disarss., 181-182)
TMIT: A number of problems-are considered pertaining to studying the
tremor of stars from observations at Goloseyevo. 1) Calculation of autocorrela-
tion functions for detecting hidden perlodicities in stellar tremors.- It was
established that periodic struatureof autocorrelation funotions is not always
obtained, In cases of noticed periodicities the values of periods amount to
5-8.aeo. 2), Investigation O*f,the structure of acme values of tremor amplitudes
as random quantities using the principle of autoregression or sliding averages.
In case of tremors,apparently, an interaction of two factors is observed one of
which yields autoregreaslon connection and the other - periodical undamped
disturbance. 3) Investigation of long-period tremors: the results of measuringX
Card 1/2
IT

a= I Dcaer."Wivalm OU115721
Vaasoy'uzanya astremotricheakaya kOftfOMnt4IyA.
Trudy 14-Y Actrmotrichaskoy konfortataii SWII. Kiyev, 27-30 =ya 1958 g.
t~raaizaotions of the 14th Astmatrical Coecrenco of the MU, 5ola In ZIyeY
27-30 May 1958) Mosew, lad-vo M SM-11, 190. 440 p. Zrrata allp inserted.
1JDOO copies printed.
ftonsoring 4cmays, uw* MISR. Glavmva astronomicheakaya cbaermtorlys
(ftuovo).
Reap. EdIt H. 84 Zveray, Comspooding Itcrber, AWW of Sciences USSRI Ed. of
Publishing Souact U. K. Zaqcbik; Tech. Ed.: R. A. Z=areze'ra.
PURM: The book is intended for astrcnbmors and antrophysicists, particuloj~ly
those Interested In astromatrIcal roccurch.
COVZRAGZ: This pu blication presents the Transactions of the 14th Astrometrical
Conference of the USSR, hold in Klyay 27-30 May 1958. It includes 27'reports
and 55 scientific papers prcsented~at the plenary meeting of the Conference
Car& 41;4.

Transactions of the 14h 'Astrcutrical (coot,) SOV/5T21
and at the special sectional mettIA95* An SMUdIx.contains the resolutiona
ado2t*d by the Conference,'the calpoettion of the, committees, the age" and
the list of partitipants at the Conference. A brief summary In Inglieb, is
given at the and of each article. References follow Individual articles.
Th* Presidium or the Astrometrical Committee (Chaixma H. S. Zverev), vhIcb
supardsed the VieDarstion of this publiestIon, cWessam ~thanks to the
membera or the averetariatt V. M. Vasillyev, X.,G. KolleUnskiy, A. S. One-
gita, sn& Kh. 1. Potter.
TOM 07 CMT=t
lr~revord
Address by A. A. Mikhaylov, Chairman of the istrcinc~icma council 'r the
Acadow of Sciences USOR
imp= or To Ammmm cmecw= AxD emmoa-.-=.
IN XWMCO CK AWRCK=CAL W= BY VARIM 13"MMOM
Carl

Tran3actione 0 the 14th Ast. trical (Cwt,) Ooy/~pl
Yefimov, A. A., Yus M. Otry"h#Wm, an& L. A. Sukham. Photo-
electric Method for Reading the Circles of -the Merldlai Instm.
Monts
FatchikhIn, N. V. On Referenoin the Stan to Gelexies
165
'169
Onegina,% A. B. The Prec"Lon of Ue"uzlng the PositIon'of Galmdoe
with the Womm Astr~Vaph Golmrpvo .173
Chudoviaheve, 0. N. He to of ObsermtIons of Kin a at
Pulkovo in the Pori 194tiVA IT9 4
Teo Ya. Bugoilankays, azA A*! Ko Soonovao Application -cx Ithe
Blectroola Digital CCOWAir *S%nW In $me rrubl=m of Astro-
Metry
WIchInskiy. 1. 0.. Invistigotion of the nlikerIng or;star Inages
at the To-loseym Obsormtory
Card qfIX
f

KOLCHINKIT) '1000
.Lmatigating the Pulsation qf I sr, olay,
notron. obsort. AN ~~R 1.~o.,W r7lS! 3.4s5)

KOWHINSKIYp IwG*
.Autocorrelation function of-the fluctuations of directione of
light rays derived from obeervations of the flickering of star
images. Izi.Gl&v.aetron.oboer.kN USSR 4 no.1:13.-30 1.61.
(KM IWO)
(Stars) (Astronomical photography)

FEDOROV, Ye.P.,, otv. red.; GORYNYA, A.A... red.;
red.j IXKATSKAYA, F.Lj red,; MEZINETS, L.P.p red,
(Problems in astrometry] Vopropy astrometrii. Kiev,
"Naukova dumka,," 1964. 94 p. (MIRA 17t6)
1. Akademlya nauk. URS11,, Kiev. Holovna astronomichna ob-
servatorlyA.

KOVALlp IsK., otvb red*; FEWROV,, Ye.P.9 red.) GORYNU, AA.j, red.j
KOLCHINSKIYJ I,G,p reds; L M TSKAYAj F.I.9 red*;
71110w.12.1,149, asolos zed,
[Pb4ysice of the moon and planstal Fizika Lurol i planed.
Kisvp Naukava dumkap 1964. 137 p. (MIRA 17t10)
1. Akademlya nauk UBM.j Kiev. Holovua astronomichnu ob-
servatoriya, 0 ..

FEDoRoV, Ye.P.0 otv. red,,; LUXATSVYA., F.Lp red.; GORYNYAp A~Aop
red.; KOLCHINSM9 I*'Gap red.; BEREZINETSp L.P.p red*
[Studies in the pbysics of stars and diffusion matterl Is-
sledovaniia po fizike zvezd i diffuznoi materii, Kiev,,
Naukova dumkal 1964a 74 p. (MIRA 17:n)
1, Akademiya nauk URSR,, Kiev. Holovna astronomichna obser-
vat,oriya.

FEDOROV, Ye.P., otv. red.; GORYNYA, A.A.p red.; KOj&jU&KjY, I.G.,
red.; LUNATSKAYA, V.I., red.,, BMUDETS, L.P.$ red.---
(Spectrophotometric studies of active formations on the
sun] Spektrofotometricheskie issledovanila aktivn7kh ob-
razovanil na SoIntse. Kiev, Naukova duwlca,, 196.1,,. 104 p.
(MIRA 17:12)
1, Akademlya nauk URSR, liev, Holovna astronomichna obser-
vatoriya.

AZAnOVA, Taiolya Aindroyev";'SHMS, Nina Alskoandrovna;
KOLCHINSKIYA-.;.Ioalxo-ichi,nalkyip I.H.lp kand, fit.-mat.
uA.0
(AstronovV in %be Ukraine, 1918-1962j bibliographical
.index] Astronomila na Ukraini (1918--1962 rr); bibliografichnyi
pokazhebyk. Kyivj Waukove. duWm, 1965. 160 p. (14IRA 18%4)

KUCWOV, N.L# kand. fiz.-mat. nauk, otv.red. [deceased],-
MEL1141KOVp O.A.v red.j OBUKHOV, A.M.p red.; DEHIDOVA,
AsNo. red,.j KOLCHINSKIY, I.G.# red.; TATARSKIY,, V,I,p
red,
(optical instability of the earth's atmos phere] Opti-
cheskaia nestabillnost' zemol atmosfery. 14oskvap
Nauka~ 1965. 170 p. (MIRA 180)
1. Akademiya nauk SSSR, Astronomichookiy sovet. 2. Chlen.-
korrespondent AN SSSR (for Mallnikov, Obukbov).

ACC NRs- AT6003703
Comelation of flickering betwmw star imape deoreuos iubatmtially at on angular
distance of a/L (a a oorrelatioA soaU) - it the' aorrelition function of Gauss is used
or at &w angular distance of IDA it. the 02/3 law" is used. The greater: the air mass$
the lower the angle at uhlo-b"independence is achievedq Resolving power decreases
ayprociably at - higher amith ' aila* ` U sing observational data for testing
correlation) it vas found that. all,values of the correlation function between
pairs of t &a are,posit-Lys, that the correlation function R (W decreas
increi and that the radius of oQrrelatian (the value o~ Y at Whi=Wit(%)-
a 0.05) is about, lotp Oich is in taIr apeement, vith the predictid mQueo Origo arte
hast 6 figuress 5 tabless and 37 formilm.
SUB CMBs 03j, 04/ am DAT%x l5msO5 om m: oo3/ om mwa oax
:aSt ra
X6.. - -----
Card 2,1(2

U
-ACC. NRJ_
SWW1 =Rs W0_=_T6
OW 690
AUTWHi KolcMn!W6 -a.
OROS NoAtr
M)
TITL&s The beaded structurs of dar
SOMES, ALM, AA&n Ghts"s =Mk' Optiobeskaya nestobUlaost, samor
atmostery (Optical instabl4ty of-the oarth' a Atoosphom). Moscow, Isd-vo Naukas
1,965p 21,25
TOPIC TAOS t 'Mrs"i pbotcgrephic images astrograpb, A;&-,. 44
ABSTRAGN Beaded structure is ft"liently observed on photographic prints. The
distance between nodes or beads along the trail is Vpro3d=te4 uniforn. The pressalb
examination in based on trails-obtsitied at the GAO AN UkrSM (Main Astronomical
Obserrat=7 of the Academy or Sciencess,.Ukrainian SSR)p 157 prints being obtained on
a 400-m astrograph in the period fto= JawLary 1955 to December 1956. Five groups
of trails are'distinguishads 1) those with no beaded structurej, 2) those with
Scarcely perceptible, beafts 3) those with di~tinot but vaguely defined be&4s$
4) those with well-defined beads ed.9 and 5'Al those with very shar
UWWWY' sjAo ply
defined beads with approximately un1fom sikving, Of the 157 prints,-60 (37%)--abow-
well-defined beaded structure in ths trails. ---Theo* -ware -observa chiefly at high
zenith distances._ The-beads-do-not-Sipoeiii-to be,due to scintillation, TM Ay6rap
'Card
2__

ACC NRs AT6W3704
of the b"ds-in the incitl
gsi,t 20
from
--co
*7ro iv-g obi i i i n 4;-0 53 T ---T h *J: L at ~U JOWdin
unw,
k-
.....................................
As,
AA
I'do"
i aid. 4 tabUs.
mm cwz$ 0 SM DMe ORM Wa OM/ OTH MW& 002
astrophotograp!y
qa
ca!j

BOGATOT. Geralld Borlsovich; BTALIK, Gavvill lostfovich; EDLCHIRS.Irr, ML,,
red-r BoRmy, N'I.,.tskhn.rsd#
CAPP110d telsvision units] Prikladrqe televisionive Astimovki.
Moskva Goo. energ. lid-vo, 1959. 54 p. (Hassovala radlobWl~tska,
uo;320$
(Industrial television)

1 .1 . I .
t �
I I

85198
e4." 2401 S/129/60/000/011/006/016
1b Z073/9535
AUTHORS: Ishchenko, A#Ya, and Kolchinskiyj V.I., Engineers
TITLE: Application.0if Gaseous Atmospheres for Heat Treatme t
of StainlesesHigh TemEsratu and Titanium M t
erials
e
PERIODICALt ,Metallovede%ye i termich9s
aya obrabotka me alloy,
1960, No.llt pp.25-28
TEXT: Application of high purity gases as protective
,atmospheres requireshermatica
lly sealed equipment for brazing or
l
heat treatment. Due to lack-of special equipment for oxidation-free
heating in dehumidified hydrog'en.and argon protective atmospheres,
the authors applied heating or components in hermetically sealed
refractory steel containers. This enables rapid heating and cooling
of components i *n the medium of the used gas and obtaining a bright
surface. A reducing atmosphere of dry,purified hydrogen in applied
for bright annealing and for brazindstainless chromium and
chromium-nickel steel's And alloys at temperatures above 900*C.' An
inert atmosphere of pure argon is used primarily for brazinit and
bright annealing of titanium alloys and also for their heat treatment
below.800*C. The use of hydrogen or argon for the same materials an
a function of the temperature range is due to safety factors, since
Card 1/4

85198
S/129/60/000/011/006/016
E073/9535
Application of Gaseous Atmospheres for Heat Treatment of Stainless,
High Temperature and Titanium Materials
use of hydrogen for temperatur a below 800*C is limited by ~he
danger of formation of an infl:mmable mixture. The shortage of
industrially produced high vacuum fUrnaces impedes the wider use of
progressive methods of brazing. In the Works of the authors, a
highly reducing halogenized atmosphere,obtained by decomposition of
ammonium fluoride,is used for brazing of high temperature steels
and alloys, including brazing with refractory solders. This
enabled brazing and bright annealing of refractory materials without
using expensive and complicated vacuum equipment and also,to exclude
preliminary.plating. The halogenized atmosphere is formed in a
system of two containers directly during brazing or during bright
annealing. Some details of the process are given. Halogenized
atmospheres are capable of reducing thick and stable oxide formations,
which is of great importance during brazing with solders.that
withstand high temperatures and also in sintering chromium powders
or powders of refractory alloys. A new method is also described of
nitriding stainless steel. Into the nitriding muffle furnac0small
quantity of ammonium chloride in placed. At the nitriding temperature
Card 2/4

85198
S/129/60/000/011/006/016
E073/E535
Application of Gaseous Atmosphere a for Heat Treatment of Stainless,
High Temperature and Titanium Materials
the ammonia and the ammonium chloride decompose, forming hydrogen,
nitrogen and hydrogen-chloride. Thehydrogen chloride interacts
with the chromium oxide film forming chromium chloride, which will
be either reduced during nitriding or will dissociate on contact
with the metal,returning into the atmosphere the hydrogen chloride
or the chlorine, An a result of this$ the ammonium chloride
consumption is verylow* it is introduced into the muffle only when
the cSmponents are charged in'(20 to 40 g for a muffle capacity of
0.2 m ). To slow down dissociation and carry over from the muffle,
the ammonium chloride is mixed with sand, the latter has to be
roasted at first at 6009C and dust removed from it. To protect the
surface of components against n1trIdIng, nickel plating with a layer
thickness of about 30 It is recommended; tinning is inadvisable since
it interacts,with the hydrogen chloride. Use of ammonium chloride
permits increasing the activity of the surfaces of high chromium
steel components and obtaining a high quality layer of the desired
thickness in a time 20 to 30% ~shorter than in necessary in current
methods of nitriding. In addition, a good quality surface is
Card 3/4

85198
S/l2q/6o/ooo/oil/oo6/oi6.
9073/E535
Application of Gaseous Atmospheres for Heat Treatment of Stainless,
High Temperature and TitaniuwMaterials
obtained without it-being necessary to clean the surface.
There are 2 figures.
Card 4/4

20227
8/135/6 I/WQ/004/bo6/012
A006/AlOl
AUTHORSt Shavkunov, A,,V,, Akeenov, N..A., Mugerman, Yu. N., Kolchinskiy.,
V. I.-Engin ears
Tr=: Welding of Titanium Alloys in Chambers with Controlled Atmosphere
PERIODICALs Svarochnoye proizvodstvo, 1961, No. 4, pp. 24 - 25
TEXTs The high ohemical-aotivity of titanium and its alloys requires
-careful proteetion'of the-weld and the weld-adjacent zone against the gaseous
atmosphere.' When welding.parts of complex oontours It Is recommended to carry
out welding in speoi4l chambers. Information is given on manual argon arc weld-
Ing of tit%ium-alloy 'and titanium parts in chambers of two types. Chamber No. I
is a 0.05 W 1Kh18N9T steel cylinder of 1,300 mm Internal diameter and 400 mm-
height. The cylinder top represents a cover fastened with bolts. Tvne chamber is
placed on a rotary table and can be rotated 'around the horizontal axis. In the
top and In the walls there are plexiglas3 windows and apertures for fastening the
rubber welding gloves. The chamber is equipped with electric light. The welding
burner is fed through a cable which enters the chamber through a special hermetic
inlet. The.burner is a holder with a tungsten electrode. The absence of a nozzle
Card 1/4

20227,
S/135/61/Ooo/1Do4/0o6/tI2
A0061AI01
Welding of Titanium Alloys in.Mambers with Controlled Atmosphere
permits the access to any.welding area. The chamber 4.3 connected with a vacuum
pump, an argon,oylinder and an oil manometer. The feed system and the electric
circuit are given in Fig. 2and 3."Chamber No. 2 is made of 15 mm thick
grade steel and differs from chamber No. 1 by larger dimensions, which makes-it
iossible to WW .large-size parts, The dimensions ares 2100 mm diameter; 6W mm
heightj 1.8,w volume. Two,parallel operating vacuum pumps are empl6yed. The
vacuum up*-to 3.10-ifmm Hg is prod%ko~d within 120 - 150 min. Gas consumption for
washing is about 2.5 m3. Prior to operation the chamber is blown through with
compressed'aIr and rubbed with an alcohol-wetted rig. To fill the chamber, argon
of first composition is employed.containing not over 0.005% oxygen and-not over
0.1% nitrogen. Locksmith tools, bass material technological plates and ea(VT-1)
2,mm-diameter titanium wire are then placed into the chamber and the cover in
fastened. After evacuation argon in fed Into the chamber at a pressure not less
than 0.2 atm. Durtng welding process 1 _,3 I/min argon are supplied into the
chamber.' Parts of commercial 'VT-1 titanium, OT-4 and PT -5 (VT-5) titanium alloys
can be welded. VT_I filler~'wire is employed, which is dehydrogenized In a vacuum
of io-3 mm Hg by heating to-9500 '0. Welding In the described chambers produces
high-quality weld joints, whose strength in equal to that of the bass metal. The
Card 2/4

Ir
EFAMMWAIM

COmbimed perfomance of dlvt&Uce and
traverise statl measuremats t
Ono' Good-' kart- Ito-7:139-48 JI 162.
(Traveneg (SUrYGA49)) 15s8)

VERVEYKINA, A.K.# insh.; 00f Inzb.; NINOLAYEVSM,
Ye-Yeep inzh.; VNIONCIVA, R.G., inzh.; RTAPOLM, A.F.0
lnzh,l SOKOL, I.A., inzh.; MULIN, S.L.0 1nzh.j
EY'DELINANTt L.B.9 inzh.j ORLOV, V.14.,, kand. tekhn. nauks
retsenzent; YURGELI, B.I., lnzh.g retsenzent; FOKIN, V.Ya
in7.h.,, nauchn. red.; VOLKYANSKn , A.K. . glav, red.; SUDigV',
G*Go, zam. glav. red.; 'LOSEWVSXIY, I.V.j red,; MARKOV, I.I.0
red,j MELINIK, V.I., red.; ONKIN, A.K., red.1 STAROVEROV,.
I.G., red.; TUSHUYAKOV, M.D., red.; CHMOV, A.V., red.
[Engineering pipelines for industrial enterprises] Tekhno-
logicheskie truboprovody prouWahlenrifth prodpriiatli. Mo-
akva) Stroiizdato 1964. 2 v. (MIRA 17:12)

-f
VMVff KINA
A. K. inzh. j insh.; NIKOLAMSKIT.,
Ye.Ya.., inzh. I R,ODION06VUA- imb.; RYAPOLOV, A.F.,, inzb..-,
SOKOL., I.A.,, inzb.; SUMS, i.L., inzh.; EYDELINANT, L.B.,
inzh.',- ORLOV.$V.M. kand 0. tekft' . nauk retaenum s YURGELI B. I,
inzh.pretsenzent; VOINYANSW ~sA.Kf'
red.; MARKOV, I.I., red.; MLINIX, V.1.1 red.; UNKIN, A.X.p
red.; STAROVEROV, I G. red ; TUSHRYAKOV, M D red - CHEMOV
A.V., red..; SUDAKOV:r,.6., r;d.; IOSELOVISKU;1:4., re*d'.
[Technologital-pipings in industrial enterprises] Tekbnologi-
cheekie truboprovody pronVshIewqkhpredpriiatii. Moskva.,
Stroiizdat.- Pt,ja 1964. .784 p~, (MIRA 18:9)

IVANITSKIT, N.M., lush.; ZOLICHITSXIT IOZ - 01=10o BD#, icand, tekba,
nauk (stantslyn mimm" uvarnaya).
Imrove the organization of work at freight stations. Zhal, dor,
trannp. 40 no.~WI-82 7 058. (Nm UW
1; Ikohallnik stantOU NakhIcbevaul-Don-Tovarnaya (for lollebitsidy).
(Mailroads-Preigbt) (Loading and unloading)

GOLOMB, OorBon lmznuilovich; XOL ICE
CH Mikbail
SMORCHXoVA, Yekaterlja'NMvlov~naj SIDOROVA
TRISHINA,'.L.A.1 tekhn. red. T.s., red.;
[Finance 'Of.the cOmMudcation Bystem)
Finansy kho2jaistva
BVIAzi. Mosk*vap Sviazlizdat, 1963- 269 P- (MIRA .17:2)

GIDALMCHt M. 0.1 NOLICHITSM,_V. L.
Manufacture of papa Jules without aging In tanke and ten-
liter vessels. 7i-%~ M?r4PP 11107-3.13 161.
(MIRA 3.63 1)
(Grape juice)

SOV/176-58-7-14/17
AUTHOR:: ej,~,GuardsMajor;.Baranovq N., Captain
_Xolehkovq,,.T
TITLE$-,
onin ,,, axAged.1xiti -Tank Training Mines.,.
Reconditi 9 Z
(V,,Qs,stqnqv1eniye povrezhdennykh uchebnykh protivo-
7tankovyk4 min)
PERIODICAL: Voyenno-inzhenernyy zhurnal, 1958,, Nr 7. PP 39-40 (USSR)
ABSTRACT: The first author refers to an appliance invented by
Engineer Major M. Sklavo,for strengthening the lids of
'
anti-tank dumb mines (described in Nr 4 issue of
1957 of this Journal), Another simplified appliance
was proposed by Private Taitsilin, Figure 1) (unit
W
th 13 .. l4cm, hole
not stated), 'It consists of a plug
in the middle).screwed into the anti-tank mine (Figure
2) with a valve through which air is pumped by a
Compressor of'5-10 atm or by a compressor from an MT
vehicle. In 1-2 minutes the lid of the mine returns
to its original shapeo Another device is described
Card 1/2

6/17o/63/006/002/00 1/0 118~'_"' NI
B102/BIe6
5%/ 0 0
Kollchugin, B. A.9 Labuntsovy D. A.
Golovint V. 8
AUTHORSs
TITLE3 Experimental investigation,of boiling heat transfer and -of
the critical thermal load for-the boilihg of mobile water
J.
PERIODICAL3 tnzhenerno-fixicheikiy zhurnal, v. 69 no 29. 19639 3
TEXII t With a view to. extending -a~d,.suppl4menting. the available published'
'data a: study~lwas- made of. boiling hesit-trairief er and critical -load-'when
boiling.diatilled water' in horizontal silveriubes of 150'' ;t~ and
4 5 mm. diameters over a pressure range of 10. - 2000 n/cm2.. The"to6pera-I
-constructed* -platinum resistance themp-,
ture was measured by an -especially X
meter whose error'of meas .uroment -'did not- qxce.4d 0.040K.'.- The use of this
h'
device in conjunotion,,with dilvbr.-tubes made-it,possible-to measure t e-
heat transfer odefficient a 6T~ Ta) with a error. of not more
A
than 6T in the temperature decrease at the wall, T the tezperature,~
14%.
inside the tubet T the saturationtemperatVi 6f the water and q the
S:
1.165. and 2'e10 W The.a(q)
',specific thermal load;.q-lay,between 6 '/OM 2.
0 d-1/2
ar.,

in l IJP(0) JOS/WW/GD-
AICSC TN ~R.
AT6029317 SOURCE CODE: UR100001661000100010156oE6el.
,'!AUTHOR*. Labunstov, Do Ae Kollchu&Lns B. A.j Golovin, V. S.; Zakharovas E. A.;
k jVlLdimirovaA_L.tN.
jORG: none
TITLE: Investigation of the mechanism of the nucleate boiling-of water using
Med moving picture photogyrap
_,30
SOMCE.. Moscowe EneroetichesKyinstitut, Toploobmen v elemontakh energoticheskikh
ustanovok tHeat exchange in fo-vier-lal-allition units)o Moscow, Izd-vo Nauka.. 1966,
156-166
TOPIC TAGSs nucleate boiling, high speed photographyp heat transfer coefficient
ABSTRACT: Tho e)Teriments were carried out on a ~-shaped silv r platea The specific
heat loads in the experiments varied from 40 x IV to 150 x 1~ wattsA,.. and the
pressure from 1 to 100 bars. The article describes the rosults of an investigation of
the following characteristics of the boiling mechanism; tho mapdtudes of the bubble
densities on the heating awfaces., the values of the breakaway diameters,, the
macroscopic boundary angles., and the average frequency and rate of growth of the
bubbles on the boiling surfacoo The experimental apparatus consisted of a vertical
cylindrical vessel with a removable cover and a condenser. The experimental section

ACC NR: AT6029317
was a 99*99% silver plato'bent at a right angle., having a thickness of 0.2 mm and a
width of 2 mms and placed on its wide edge, The load an the plate was created by a
low voltage direct current* Before the experiments,, the surface was given a special
preparatory treatmentp after which it had a cleameos of Class 6by GOSTJ769-51* The
working fluid was distilled water with a aalt content of 0*2-0.5 grams/ . Two series
of experiments were made; one on fresbly prepared surfaces and the other on surfaces
which had been used. The experimental heat transfer data are shown in a table* The
following conclusions were drawnt' 1) the values of the beat transfer coefficients for
surfaces which had been used were lower than those for freshly prepared surfaces;
2) there was observed a sharp decrease in the breakaway diameter with an increase in
pressure; 3) the rate of growth of the bubbles slowed down sharply with an increase
in pressure; 4) the average macroscopic boundary angles changed only Slightly with an
increase in pressures Origo arts hast 17 formulae, 11 figures and 1 table.
SUB CODEs 20/ SUEM DATEs O5Apr66/ (BIG REN 010/ OTH REFt 013
Card 2/2 not

OL
J
"ACCESSION NRs AP4042471 8/0294/64/002/003/040/003
'ACCESSION NRI
AUTHORS t Labuntsov,,'D.-A.1 Kollahugin# BcAsj Golovinp,V. 8.1 Zakharova, go Ae
MOO
dZi Labunts
Vladimirova,, L., No
ro"_ N
.TITLEs The study of bubble growth during boiling of saturated water under vlds:~tl,
ITIE I Th study
pressure range by means of high'speed,motion. pictures
Yr 5sure r s by
SO~ MI T~
~SOURCZs -Teplofisika vy*ookikh texperaturi,ve 2# 110s.3p 1964v IA"53
ploe
".10PIC TAGS: va
Por-bubble, boiling water notion pioturem wetting angle# water
i,saturation pressurep,motion-pioturie camers SK9 XH
I-ABSTRAGTs The growth of vapor.bubbles.frois bo water in a pressure rang
iling
2
to- 106 bars and 40 to 150 Wolt/ki heat supply was studied by high-speed moti.
pictures. The light source was a SVDBh-1000 mercury lamp and the SKS-114 camera
was a 1000-to-4000 frame/second instruieent. Analysis, of bubble growth rate shows
a functional dependence between bubble radius R and time Tr-
who" numerical '009friois
nt
Pm2
In
c" + coo 1)$ (2 coo OW,
rd do

z0
0 .
got
4
P~ 0,04
0
OW
cop0 4
f 40 0
10 'coo,
SP .0
~904%tk4voo
See p 0%4
VP
hood
tco 6
'tit 6
loo 0~
4
to 0
X,40
%G dA
kosp b, 9.
'cl 1 4~,,,O
dJp 10
SO), 4p e so
.04
N
V
% so

GOLOVIN, V.S.; KOLICHUGIN, B.A*1 LABUNTSOV, D,A.
Beat transfer In the boillng of ethyl alcohol and benzene on
the surfaces of various materials. Yush. fiz. zhur. 7 no.6s
35-39 164. (MIRA M12)
1. Energeticheakiy institut imeni G.M. Krzhizhanovskogot Moskva.

AP6008837 SOURCE CODE: UR/0294/66/004/001/0147/0148
AUTHOM Golovin, V. B.; Kolichu B.A.; Zakharov& E. A.
tu
ORG: Power Institute im. G. M. Krzizhanovs (EnergeticbesWinatt t)
TITLE: Measurement of the rate of growth of vapor bubbles during the boiling of various
liquids
SOURCE; Teplofizika vysoklkh temperatur, v. 4, no. 1, 1966, 147-148
TOPIC TAGS: boiling benzene, ethyl alcohol, water, vaporizations gas bubble
r"STRACT: The authors obtained data on the rate of of vapor bubbles on the heat-transfer
surface during the boiling of be11z6neA`ethv1 alcohol, and water for -different thermal loads and
saturation pressures in an Wxop~ermentalset-_up dose ibed elsewhere (D. -A. Labuntsby, B.
Kollchugin, V. S. Golovin, E. A. Zakharova, L., N. Vladimirova. TeplofiziMa -vysola~h"..
temperature, 2, No. 3, 446, 1964). The exper1rdints wardiii6rmid *ith'9010W 'Biiv-e,r* and
nickel-plated copper, using the methods of the earlier work. The results of the Primary pro-
cessing of motion picture data showed that, for all the cases investigated, the relationshin.'A _-v;rj
(where R is the vapor bubble radius Via the time of its growth on the boiling surface) is
revealed quite distinctly. This m2e it possible to calculate the values Wft. which are
tabulated for various liquids and mode! parameters. These data, together with the results of
the earlier work, obtained during the boiling of water on a silver strip are shown In a diagram-E
The new data confirm the fundamental conclusion's of the earlier work. Orig. art. has.- I figure,
I table, and 1 formula. UDC 536.423.1
Card 1/2

Construction ImIustry - Accounting
"Calculation of capital construction," 14. F. DYachkov, Reviewed by: 1. A. Kartsev; 2. K.
,Kollchugin., Bukgh. uchet, No. 2 1952.
Yonthly List of Russian Ancdasinng, Library of Congress, Lay 1952, Unclassified.

- - IMLI CHUGIN, X.
C~,j.wwIM. a
Accounting formaterials based on uniform nomenclature. Sukhg.uchet ,
16 no.2t25-27 7 157. (KM 10-.2)
(Prices)

BIWIP P.P,, kznd.tekhn*naukp redg-KOLICHUt I,Z,, redol OU BOY,
S.M., red.; NOCHETKOV, Ass I& i,-rwV-*TTdVMIIWA~ L,A,, takhred.
[Designing and building granaries, flour, groat, and feed
mills in the 'U.S.S.R. in 191?-195?1 Proaktirovanis i
stroitelletvo sernokhrenilishch, sukomol'afth, Icrupianykh
i kombikormovykh prodpriiatii v SSSR, 1917-1957- Nookya,
Isd-vo takhn.1 skon.lit-ry po voprosam =komollno-krupianol,
kombikortoovoi prom. i elevatorno-skladskogo khoz., 1958.
235 p. (MIRAL 12:9)
(Flour mills) (Feed mills) (Grain elevators)

KOLCHURINAI A.A., Cand biol Soi (disB) "Study of anaphylacto-
genic properties of arsti-diphtheria serums by various
ri k
methods arties of diphthe 0
,,and the prop
anatoxins in cow-ection ivith their iwanogen-
Kazan's 1959s 13 pp (Min of Health U' State Sci Res lm~t of
Microbiology and Epidemiology of SouthIst-1906w4he USSR ff)Licrol~)
k-I
250 copies (KLj 28-59j:125)
36 -

MCHMIL, A.A.
Reactogenlo properties of pertusels-Uphtheris, vaccine. Report To.1t
Senlstlxing properties of the prtumale-diphtheria vaccine; author's
abstract. Zhur.mikroblol.-epid.i immm. 30 no.10t32-33 0 139,
(MIRL 13s2)
1, Is rananskogo nauchno-Insledovatellskago Instituta epideutologil,
i gigirevy.
VROOPING COUGH Immol.
PORMIA lummol,)
M

T'"TAMIK
CMTKOTA, G.A.; UBZLXDTL, A.*.; MOLCHURM, A.A.
Vhlto nice as objects for t6 experlmntal d9termigation of ji&-
Obyliwtogenic properties ef therqmukia sera, Zhurm'vl*kr6blol,',,,
sPidol In= .3'O:no.22i33-36 3 1599 (KIRA 13:5)
1. Is aoguW*tv*Uuw kontrllnogo Institute, inqui TaraLsevlch&.
pharamol.)
Clk~y)

----------
.
IWLCHURIU v A.A.
Sswitizing 'Lctivitv Of antl-innuenza horse serum folloving
'ntranaBal admW#trktiOi- Zhw- mikrobiol, spid, I 4=mln, 31
no. 409-102 Ap l6o. (MIM 13;10)
1. Is Kazanakogo'instituta apidemiologii i gigiyeny.

'1014MMA, A.A.
ansitising proportion of diphtheria anstoxins; muthor'sabstract,
Zhur.m1kroblol,spid. i Immm. 29 no.2:123-124 7 158,
(Him 11:4)
1. Is Usnnskogo instituta, spidesiologii j gigiygny.
(DIPHTMIA)

-2,W21. -Wwmm - , -
KOLCHURIHAp A.A.
ft~ of the biologima'propertiee of vaccinal Influmm AZ
virus straJ,noo Vopo virus 8 no.5#559.%4 8-0163 WRA 17t1)
1. 'K 11
on th n37 Inettut meditainakikh biologicheakikh pre-
pargtdv- Imeni L.A.Thrasevicha Hinisterstva wiravookbraneniya
SM, moskma.

LCHURINA. A*A.
Determination of the-specific avidity of type A2 influenza virus. Vo
virus* 9 noo2iI88-191 Mr-Ap 164# (KRA 1782250
16 Gosudarstvanay kontrolinyy Institut meditainskikh biologichaskikh
preparatov imeni Tarasevichal Moskva,

KOLCHURINA BOIDTOVSKIYJ, V.m.
Study of the interaction of inhibitor-sensitive and inhibitor-
-resistant vaccinal strains of the A2 influenza virus Vop.
virus. 10 no.1:61-66 Ja-F 165. iMM 18:5)
1. KontrolInyy institut moditainakikh biologicheskikh preparatov
imeni Tarasevicha, Moskva i Institut virusologii imeni Ivanovskogo,
MoBkva.

83351
S/139/6o/ooo/oo4/008/033
E032/E514
AUTHORS: Kollchuzhkin, A.M. and Koleanikov, N.N.
TITLE: Electromagnetic Interactio Between Finite Non-
relativistic __P_a_r_t1-c1es
PERIODICALsIzvestiya vysxhikh uchabnykh zavedeniy, Fizika,
1960, No.49 PPO'87-97
TEXT:. Recent experimental and theoretical studios of the
structure of nucloons.have'produced muck valuable information.
Among these are the electron'scatterinSNexperiments of Hofstadter
(Ref.1). However, structural effects become appreciable only
for electron energies of the order of 150 MeV or more, in which
case radiational corrections.have to be introduced and various
competing processes take place, for example Tr-meson production.
This complicates the analysis of experimental data. The
theoretical formula obtained by Rosenbluth (Ref.6) was derived V11%
for the effective scattering cross-section using the first
approximation,of the perturbation theory. This formula applies to
relativistic point electrons.scattered from nucleons having
spatially distributed charge and magnetic moment. However, nucleon
recoils were hot taken into account and the use of phenomenological
Card 1/4

83351
S/l39/6o/OOo/Oo4/oo8/o33
2032/E514
Electromagnetic Interaction Between Finite Non-relativistic
Particles
form factors was not fully justified. In the case of heavy
particles the internal structure already becomes important at
non-relativistic energies. Hiida and Sawamura, (Ref.8) and
Nikishov (Ref.9) have also used the first approximation of the
perturbation theory to obtain an expression for the differential
cross-section for a finite electron characterized by electric and
magnetic form factors.and 'scattered by a heavy and finite target
particle. In the present paper the,scattering of two non-
relativistic particles with spatially extended electric charges
is solved using the Schwinger variational method so that the
solution obtained is more accurate. The scattering of finite
(L.e. spatially extended charges and magnetic moments) particles
is treated on the Born approximation but the structure of the
particles in taken into account. The charge distributions are
assumed to be spherically symmetric and the magnetic interaction
energy is taken to be of the form
Card 2/4

83351
S/139/60/00o/oo4/oo8/033
Z032/8514
Electromagnetic Interqction Between Finite Non-relativistic
Particles
r I r2l
pit, ei'2I
dv1 dv 2' (26)
VM r
12
where p is the magnetic moment and a the Pauli spin matrix.
The final formula obtained for the difierential, scattering cross-
section is of the form
dcr

dJI
a (x) 1
0
3 2
1 5e +
I