SCIENTIFIC ABSTRACT NIKONOV, V. B. - NIKONOV, YE.

• Document Type: CREST
• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R001137220012-2
• Release Decision: RIF
• Original Classification: S
• Document Page Count: 100
• Document Creation Date: January 3, 2017
• Document Release Date: August 1, 2000
• Sequence Number: 12
• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT

.1 -
t--a--,~-,7-,- 7' -7 ~:Zl .
0 . L ,, -~ -. 7 t '~ 0
Astronoaq
*Abnoluta glee trophatormtry of the Silar (;orotv#. fit thm Timo of thov 00tv,lota 3.,)I,kr
Lclipso of 9 July 1945.0 lzvjsttym iryvakoy Amtrafiticnatskoy Ob:mrititorli. 1~ 194A
Report lio.IWW-19569, 3R 5'059020

I, I I r , -
--;,. - ~;~ ~~L.-
NIXONGT~ V.I.; KILONOTA.. T&.X=.
Absolute slactrophotonstry of the solar corom durIng the total
solar eclipse of July 9. 1945. fav. Xryu astroffs, ok"r, I pt.1t
83-101 047. (11M late)
(Sua--Coron&) (Photoostry, Astronomical)

KiRowi, 'f.B.
WAkonev, V.I. and 51konove. Z.K. '19z"rimat In photoolecttte
comp"Leas of lbrtghtwee~ of nacturn&I akies in Stafeas and
Partisaaarka.9 Izvestiya KMsk, astrafts. absorvatorit. Vol.
111* 19", P. loq~--11
SO: U- 28M, L*taplo Zhmrnallu*kh Statey, No, 1, 1"9

SE if If I rM 51i""W'At. re. r.
r I., . . 1.
AstronoW .
*%xperlwits with Pnotoelectriv.,tlCom -tri,4on of th,3 l-1,-htw;s o4' tatt 1;1,-,1t Slr4 in
Simiza rind PnrtlcmnaT)a%,* Izvestlyn Kryms;coy A3troftzlchavka7 01)servitorll, 194P
Report No. 4&W-19569. M 52.059020

- W
- H. , KRF 'I~rA. , T..
!~IT~OWUV, V. T V I and FALURAK, A - A .
NiLblyudeniye oblasti Salakticheskogo teentra v Lnfrakmsaykb luchakh (Obaervation of
the Galactic Center Foglon to Inframd Rays). Akisdeutya Okuk SSSR. Doklady, 1949,
V. 66, no. 1, p. 25-28, dlW., 6 refs.
,u262-S3663 v. 66

~-#
lot.. -!j 4-4-
~ ~ ~
, .

i-41 A~-A u u 4 0 to "I,
--- 4--L-A. J.A P 4 A A . . . . . . .
L
t A
,

-Odom*
ftip tow
A. IL
do adw
P
0o n
fkvwolnt Mt TV (
(I"(1 Is Ana" SAW fimofm- W.
a apeft
L
"A I*
404pod im 40 "
aw"ftaft*440 *90 44144 low 4 logo"

d N
C N
s
m
do follow 4
a ft so we as dklmo
am 610 A ef now
ao

't a a 0001-
(me im *a @*it aw 61 ad (10

f CAVOWN
*Kwdwmwv~L

i
me*
I
see
was
14#400 M. C~ "MmiA 400 an it,
OL i"I go S, I I Of a 0 0 1 a 0 1 do 4, 31: 4 v w
9 0 0 0 0 0 0
-- : : : :10:0 0 *

W11OF0310vt V.B.
Apr 52
vlnfrw*d Radiation of the Iftlky Wmy#2 To.1* Pavlovp Pkqs, Instq lAninp&d State Or
9 Prirv", No PP 107-109
Real naturo and struetwo of Galaxy me explained in 1948 at Criman Astr*pW~ Obe
by obeavationo in LAfrared of A.A. Nalinyaks V.1, Imovskiy and V.Pe Vik*fomv,,/~
using photosensitive cathodes. In 195~O at the ram observatoryp S.F. Rodionov
and 1. 0. Frishman used photocells to photograph in infrared the Cal&37 and found
this radiation to be 2-10% of tbo background flow.
21M

Staro, 7axAPOIc
'Zott-Ilar el octrrophotcre ter nnd th- Crlro-fjr, Astr~phynlc_,xl (15ematrry rv-
.10-mijut iris, th,,4 (UnInutinn of LAi: lit, In --m-thIn 07-:r!n- Iv-v-. I-x1j- i;rI,co. I, !tr In. r.1-
a!t,va'Icr.!, rif variabIr !stara. I.-v. antrof.z. cl,r-!r.
'c-; t b-I _,~_ Lit rf L!xslgr~ of
JIM13 1953.

of a varlahl.-I r,"j-.r -f
-v. astrof 1
"on "Ist of
thl

Stellar t%stronnnor, Stellar Catalogs, Orlr-7)
Byull. AF Gru;j ES& Abastwaansk-Va Astrof. ObservatoE&!g No lh, 1953, rp 1-2)3
Nikonovp v.
Accurate color equivalents are deduced for E52 stars in the galactic zone of
latitude 20P, It-mited, in the region of galactic center by declination -240 ad In
the region of anticenter by longitude IWO. The atcwspheric effect was oltmated, but
not light absorption b~ interstellar media.
Referativnyy Zhurnal -- AstiononVa I. Geode-.Iya, No 6,, 1954 (d-)0976)

'08n/Astronmv - SWItovmOT JkIlAug 33
"Index to Astronomical Literature Published.in tht
USSR During March, April 1953," Yu.. G. Perell
Astr Zhur, Vol 30, No 4, pp 475-478
Lists 60 &rticlea on. astronomy which.appeare~i lur-
Ing Mar, Apr 53 in 15 books and.symposia, I ep*nem-
eris, 6 Institute organs (e.g., "Trudy), 17 reri-
odicals, and 5 abstracts of dissertations. For ex-
ample, one &uthorls abstract of a dissertation, the
only one m-ntioned for the degree of Dr Phys-Hath
Sti, ist An Attempt to Construct a Fund-amenteLL
Catalogue of IMectrical Chromatic XVIYalents of
262T32
Star@ of the Spectral Types B8 and B90" by V. B.
Rikonov, Main Astron Cbservatory of Acad Sci USSR
(expts were completed at Abastu*An Astrophp Observ-
at o ry and Crimean Astrophys Observatori), Lenin-
grad, 21 pp, 100 copies.

511WROT, V.D.0
Using multicalor atectracolortmtry In gtu4ying vol*ctive ab-
sorV%lon of IntorstolUr watter, 121
134-147 "54. MBA 1314)
(ratarstelUr mtter--Spectra)
I I

Ln trom,.mta
Nb. 43 3 9/W,
Dobronra7ln, P. F.p and Nikonov, V. B.
TItIC Instrumnt for recarding the snergy dinti-111.~,ition in spectra of stars
vLz,,r. All SS,1311. Ser. fiz. 18/2', ~ngsj 268,Mar~Apr 1954.1
Brief do3criptim is given of a do-ftco fox- re=-dIrg envrgy distributions
In spoctra of stara. The inatnimrit #;~ploys Si~-,rist mdt- photo-adtipUers
and to intt~rid~)d for orp6ration in & 5(X' = xoni3:u3 talescopa. The deTico
r-e-.-,rd3 Mile ratio of tht~ photomurrmt jTod'uc-~d by the light of a star at
a given wavo Itmigth and the photocurrent rrodl~n,_Nd by a large part of the
i',-,3ctnm. 'P-m Ught oticillatAorgs cw~itid Irj the flickering and y1tration
or the imago on Ung sll;" aro complotf,17 elirvlnit.ed by the new recorder,
Tidg allzD Inclu,3c,; tho 0iro-ratic flUckerine, of 3t~%r* at greater zenith
1=.'Iitut~.on Acadct;V, Of 3CIOTMer, 7110 Cri;-",- n kftr0p-hysto Observatory
'JubMAtted

DOBBOXRLTIM. P.P.; HMMY.. T.3.
Coqmvmatlv4g stollar 4octraip*ctraphotaustaro 19V K
sotrafts.obser, 13g32-4 '55. (NIRA lit4r
(Spectrophotauster)
0140

milwyov, Y.N.
Works of the Crisman Astrolftsical Observatory an stellar
astronamr. 1xv.Krym."trofle.obser. 16:216-219 156.
(KMA 13:4)
(Stars-4teervattaits)

UXIMASOT4. S.T.; POLOSUKRINA. K.S.: LUCHELOYSLIT. D.L-,
CHWArw. 1C.1C.
Color-luminosity diagram for stare In the vicinity of the
am. lawAryn.astrofts.obsar. 17:42-88 '57.
(stars) (wirA i3t4)

I UT H (1, 9 Blanlov, 9, X., z1voynkiy, Ye. X., -20-;/2o- 12 1 - r - I ylc-~
W .1
CDrrenyording ilember, Acadeny of Sciercea, USSR, Kilinyak,
A. A., 11-.1,onov, V. B,, Prokof'yeva, V. V., S-olkin, G. Yo.
... 1___--_'
.1 .....
TITLE: .... ...
The Une of lballaltintave Elo~ctron-Opt!,:,%l Li~.-ht An~lifierq
in Astrophysics ( 0 primenonii :nnogokaek.%dnykh e1e?trcnno-
opticheskikh usilitelej sveta v Astrofi.-ike)
?EHIODICAL: Doklady Akademli nalik SSOP, Vol 121, Nr 5,
pp 8111~ - 818 (USOR) (jj-r
ABSTRACT: This paper in7enti.r.ate3 none iroblerna ~~onnected with the
application of electron-optical light anplifiers in
astrophysics. The ft-uthoro estimate t%e incrense in
efficiency of the utilization of the ph,)ton flux with
respect to the unual photographic method. Under the
lnvesti~~atod conditions, and In t:.e case of equal 41mensions
of the pictures, the efficiency of the electron-optiial
method is by 40 4.103 timen higher than in ordinmry photo-
graphy. An increase in scrtle on the photocathode of the
light amplifier reducos the increnqe in sensitivity of the
electron-optical method co-.Apared with a ucual photographic
Card 1/3 plate by 160 tirnes. An est17::ation of the sensitivity

The Une of UuItintage Electron-OptAlcal Li,,-',.t Amplifiers S'~if2s-12--f-!7
In Astrophysics
of the ligl,t amilifiers given a v,%lue of the order of IC'13.
The uae of an electron-optical Pmplifier usually cannot
increase the penetration roinfre of the telescope. BT.,t the
reMiction of the t1nes of exposure by hwnireda of times of
its nriount due to the high sensitivity of the light w1plifier
easentially changree the ponuit'alities if the antrophyilcal
Investi-,ation. The r~hort of exponure per-Lit the
Investi!~ation of rapilly varying proceGses of very faintly
visible objects ftn1 a consAder,-ible increase of the utili-
zation coeffii-iont of tl~.e aatro~.hyrlcal i,.ntrurnents. T',0,
reduction of the timen of expov%ro In very important for
aotrospectroscopy. The above-discussed considerationi
are confirmed by V.-le rerriltt oltrinei by experiments carried
out by the authors in Kqnskaya actrofizichenkaya
obnervatoriya All SSOR (CrimetuAntrophynical Observatory
AS USSR). The proper noisea of tho llglht amplifter may be
neglected in comparison with tho bnckeround of tho nky.
Accorling to tl.e experimerital values, the une of the 11F, 1-, t
anplifier pernittei n rf~.,fiwtlon of the tine.- of exponlire
Cttrd 213 approximately to a thourandth cart of t.-Iqir for-mer anoiintl

The Use of WultistaFe Electron-O~tical Ligint Amplifiers SOV/2o-121-5-13/50
in Astrophysics
which satisfactorily a6reen with the above-given estinate.
A figure shows the photographs of 2 eztragalactic nelulae,
which were taken by means of a light amplifier. There are
4 figures, 1 table, and 6 references, 3 of which are Soviet.
ASSOCIATION: Krymakaya antrofizicheakaya oboarvatoriya Akademii nauk SSSR
(CrimedlAstrophyeical Observatory AS VSSR) Glavnaya antro-
nomicheakaya observatoriya Akademil nauk SSSR (Astronomical
Main Observatory#AS USSR)
SUBMITTED: April 14, 1958
Card 3/5

AOOI/Al0L
AVIRMs Dimovs N.A., Nikonov, V.S.
TMA9 ftotool*ctriaal determination of &qutv&I*nt widths of If pin early
SUM I
PERIODICALt ReferatiMy zhurnal. Astronomiya L Goodoslye, no. 10, 1961, 22, ab-
stroot iom6T (Ouir. Krymsk. astroriz. obsery.w, 19W. v. 22. 176-
Mo SKI. summew)
Mr. t Tha author& discuss, tht possibility of direct photaelectrical deter-
mination of' equivalent widths of spectral lines by th**differential atorine
method. In, this method, light fluxes are measured from the portion or speatrua
w,hich Includes the line being studied, as well as those from two portion& of con-
tinuous spectrum to-, both sides of' the line. The m*&*ur*ment& oC the both light.
fluxes are, oonductod tT seem of & single photomultiplitr andaltemate. every D 5
see. Fhotocurrents from the line and continuous "otrum are integrated ltvl;p;~-
dently. The method described was applied to determination of equivalent widths.
of H 24in spectra of 22 6tars of spectral classes 09. - 40. Observations *stab-
lishea th* possibility of organixing the large-ac&lephotoelectrical daternina-
Card I/V
46

IL;
S/035/62/000/010/016/128
MO I/A 10 1
AUTHORSs Mekrasova, S. V., Nikonov, V. B., PolosukhIna. N. S., Rybka, Y*.
TITLE: Photoelectric magnitudes and colors of reference photometric
stars In Kapt"m are". 1. Some problems in methods of com-
piling ftwdamental photometric catalogues
PERIODICAL: ReferatIvM zhurnal, Astronomiya I aeodezlya, no. 10. Ij62, 30,
abstract 1OP44 ("Izv. Krymak. astrofiz. obzerv.", 1962, v. 27,
228 - 240)
T14T. A catalogue"of photoelectric magnitudes and colors of reference
photometric stars in Kapteyn's areas Is necessary ~o reduce zero-points of
scales of stellar magnitudes to a single system. an well as In allowance for
atmospheric extinction. The authors set forth the task of obsgrvation of all
reference photometric stars in 139 KdLpteyn's areas ( 6> -15 ). In the ruture,
observations should be extended to the entire southern half of the sky. Two
methods are briefly described (Ye. Rybka and V. B. Nlkonav) for compiling such
catalogue. Both of the methods are applied to the same observational data ob-
ined In Crime& by means of an A3T-7 (AZT-7) meniscus telescope. In move
L
Card 112.

s/o35/62/ooo/b10/016/128
Photdelectrio magnitudes arA colors of... Ao0011A10l
detail these methods were described earlier. Observations of 14 reference
stars In 7 northmost Kapteyn's areas are utIlIzed (results are tabulated).
as well as of 17 stars of spectral clazaes DO-V2 from Johnson's list. Meth-
ods of observations and processing are described. It turned out that both
of the methods yield errors of the aame order (0%1), however 141konov's meth-
od Is more economical in tlwe consumption and makes It possible to control
more reliably the constancy of!the photometric system. It was decided to use
the latter method for the further work on the catalogue (individual observa-
tions are directly extrapolated beyond the atmosph*re). It Is established that
Instantaneous values of the gradient of extinction factor versus stellar color
relation should be used in compiling catalogues of stars with a wide range of
colors. There are 14 refernees.
B. Fesonko
(Abstracter's note: Complete translation)
Card 2/2
f

-14 119-,
5/033/62/039/0(j2/011/014
E032/E314
AUTHOI-S: Butslov, H.H., Kopylov, I.H., Uikonov, V.B.,
Severnyy, A.B. and Chuvayev, KX*
TITLE: Experiments in electron-optical photography of
galaxies in hydrogen light using the 2.6 m
reflector of the Crimean Astrophysical Observal;ory
PERIODICAL: Astronornicheskiy zhurnal, 4. 39, no. 2, 1962,
315 - 322 + 3 plates
TEXT: Detailed studies of extragalactic nebulae require
the use of large telescopes. As regards detecting apparatus,
the use of ordinary photographic techniques in conjunction with
narrow-band filters necessitates long exposures and in therefore
inconvenient in practice. The authors have investigated
therefore the possibilities of image-converters as a means of
avoiding these disadvantages. An Image-converter was sat up
in the direct focus of the 2*6 m reflector of the Crimean
Astrophysical Observatory. The Immediate object was to investi-
gate the hydrogen emission in a number of galaxiris. four* light
colour filters were introduced In front of the converter and
Card 1/3

S/033/62/059/002/011/OL4
Experiments in electron-optical ... 9032/9514
the screen or the latter was photographed by a motion-picturn
camer&* Altogether 58 galaxies were photographed in Ha
and other light. Photographs or io of these are reproduced
and their reatures are described C',IIGC 604, 1569, 4214, 4449,
4490, 4736, 5194, 5457, 68az and 69461. Many unknown clouds
of hydrogen- emission were detected in the galaxies. In nany
cases there is no correspondence between hot-star clusters aiv]
4ydrogen clouds. The hydrogen component shows greater concca-
tration in the equatorial planes than the stellar conponent.
In some galaxies the nuclei consist or isolated condensations.
The dimensions or the nuclei in H M light are in s(mie cases
appreciably largerthan in other light, although in a number of
cases the reverse, situation obtains. In several galaxie3,
streams or ejeati6no. from the nucleus, which are vinible ottly
in. Ha lightt were detected*
Card 2/3

AGAPOyf re.S.; ANISDUV, V.F'.; NUMVt V.Er.; FROYOPTEVA, Y.V.,,, 511OCK, -S.K.
E"rimmtal appUcation of television technique for obserntions
of star*, Izv. Kryu. astrafts. obser. 300-19 163.
(MIRA 17c1)

-2
r~ liv AP502.1256
V 0635
~jgjapc v T e An.' 3 11 or-- v ,in
V.
-v&tIons of art I f! e~ q r' 4 q
t:, g v. P r~ C,
AC t
'T r

AV, `)-2.12

T-., SIN 9141 AY5012T56 (m/oo,.70 /65/161 /UO6/12W/l 300
13 - -y
YL*~ Arislmlv, V, F, Teflop
Prokof'I li, S1 rienok ~J,
F~ 9'ralt ust ion o f the thre%bc I d A c iiq i t y 7y' k-pA t 1m, ~hr~igh at, p I I &r
F U 1X;k1ndy v ~ I
T!,eVS: 1 4,* t i4,,rqtt-n, fi'-, i RLr -bap v-,,tt I o,.
.tFuht flux wmourowm~
t
-W- 'Me threghc.,11 oensltl~~,.Ty -f v F1 1~ 1 1e 7, vl'.h it high
al alm= Ito i %1 1 mr-3 d h I r 110 x on A Y! I.y hoo hoor
To~
i i u, r, t ~tdiy determinA-d frui) ot,-i a r r thp Crimman
observator,/ with tore TM-500 -.M. VJ The
um-ftitive 'r? 4-yvt4m vqn dovr~lope(,, r"r -)tMo"Ving, i1totovit ftmrs by re"tirfrig
01 ~u ft -,f nij-.10, rky rn?liation:..
",a ~Agafla~wt

EM
I (V N51 41150 12758
~q in Irl g. I of Lhe En, w*n ~-h h .-Fi r I Mpnt. a j 1~(
-r.,i -w4l t;hr-,nhol .1 sens I t. I vi t y r th4s TV klyst (-M cul Nted. 11 t
~F] . I Ard thnt the two? of Fj jr h a h I ivnI v wn s P, y9 I em ~,,c),Fet her 'ei th a
-..A --ite 'to I OFIC-Opm v I U WA a It pr, a t. ALIT I* ti rpt~r--,,A. -10. 1 --t 1 f~r fn-,-
emporntres run4O ng f r,~,v n^ vs, i &I ne cnriIn t:~ :lnp mi n,,te . rbin appricisiches
limit cf 4--t,ecting &0 r-vr~'~y vrum MI-1- has!
W)id I table, lip)
iiT :OR i Krymakays Dbaervn-,,rly-i Akpw,~m,! n;%-,-ik 8SSR (Cri,%e4n
P.)V.- 004 ~THR ik FD P 11.1,rtS I~M
00",

I I W M-rYTT Im. F -
T
Iftonav, T. F. OProblms of mathmatical trdxdxg In the
Itechtdcums'.0 Min Education RSFSR. h6acm Obl&A
Pedecogical List. Moscow. 1956. (Dissertation for the
D"e of CaMidate in PedaCogical Satence)
Sot Wahnsys latopisf. No. 27, 1956. Hoscow. PaCes 94-2,09; 111.

T F.
Ail'=# I-",
rm first $&-;A* Makewich prize ~ givm to the following to#"g
Candi&te Qf TseWcma Sciancer A* M Assanow, Togimers W, 1, Tomhehiny
TO IP* mikawrt D. r. xastm*o, s. ca isrinchow, I. s* xurkay, x. x. Lashakovag
N* go Tambukt Aw A* &a&tnLkcw and a. To- Litvin (Axitomebilo Works ijmd
Ukhacher) for their paper *Investigation and Introduction of tht Process of
Nitroemeatation b7 Direct Isothermal Hardening in an Alkali rnside Muffleless;
SquipwmtOs theIr design of a muffleless furnace heatad by vertical radiation
tubes in of interest.
Rosidta of .the 1958 Com"Ution for Obtainine Imeni D. K. Chernev and Imeni
V. A. Minkovich Prim# KetsUoyedemiju I temicbeakeys. obrabotka mt&Uovv
1959# ice. 6# pp 62-4

MMMO,p T-L-9 MUM,, PAIR.1 NZMV,, T.Fj TMLMS=g A.G.
%Isc 40 Khm stool for the half-Gas" of Suldmabdis &I""
4XIOse KetanaTed. i term. obr. mat. xw,4tl5.l9 1@ 161,
(KMA 16# 6)
(Autimmabilos-Aitles)
(31401 411mrs-Testinc)

- Irmw, T.Y.
Some evidowe of p*trolew-baartag potoatlat of tb* Went liberiam
lmlmd. Naft.khow.34 w.6:4" AC 156. (mm 9: 10)
(Siberta,
geetW)
Irosterw-Fatrelaun

3(0) . SOT/20-124-2-4-3/71
'AUT301: Nikon Z_
TITLZ: Authtgenic Iron# Sulfurq Organic Carbon, and 31tuaina In tho
Kesozoic Sediments of the 19ast*rn Uril ReCion (Lutigon4yo
shol*zog seraq organlcheekl,~ aglerod I bItumy v ogadkakh mesa-
toys, Vostoohnogo Prii
ParoncAL: Doklady Akademil nauk 6SSRt 1959s Vol 1249 Er 2,
pp 592 - 394 (USSR)
ABSTRACT: An in known, the organic substance is oxidized by authigenic
oxide Iron and sulfates. This oxidation may t:ke place to a
considerable extent within short periods (Ref 102). The
process mentioned In the course of which oxidation iron and
sulfate-sulfur are reduced to widespread (Refs 3,4)o The
authigenla Iron Is precipitated from the solution an oxide-
tIon Iron (Refs 5.6). Sulfur to carried away from the regions
of denudation and accumulates first In the seitsvnts as
so 2- unless It migrates as a component of the organic sub-
4
stance and Is eabodded. Part of the organic substance Is
Card 1/4 decomposed by redox processes, This takes place the sore

Authiganto Iron# Sulfurp Organic Carbant and Bitualas, r- 12*-124-2-431TI
Soy
In the Mesozoic Sediments of the lastern Ural Raglan
quickly the thicker the original mass of the oxi4lzer is.
For thIs reason there exists a certain Interdependence bet-
woon the stages of accumulation of authigenic Iran, sulfur
and the organic substance. The content of authigenic Iron
Inarcases along the arose s*ctIon of the Mesozoic from the
Upper Jurassic to the Cenomanlan, It then rapidly decreases
and later an Increases again. Due to this fact 2 periods
of accumulation of authigenic Iron are expressed In the do-
nudations (PIIG 1). The distribution of Corg Is also cyclic
and inversely proportional to the Iron concentrations (Ref
Sulfur# as one of the elements which are the most capable
of migratLon (Refs 11012) was washed away and accumulated
during ths, great transgressions (Jurassic-Talanginlan# Al-
blang Turonlan-Oligatenic) In the sediments, love&t times
when iron was little nobilb. There to a high sulfur content
In all loamy strata (0-4-0-0). The concentration of A-
bitunina, decreases In the Jurassic until the Cenomanianp
while the Iran content Increases. In rocks from the Turanian
Card 2/4 to the Oligocenic which contain less Iron but more valfurp

Authigento Iran# Sulfur, Organic Carbon, and Bitunina SOV12o-124-2-43171
in the Kesozolo Sediments of'the Eastern Ural Region
the concentration of bitumen Is strongly reduced. This
took place in connection with an accumulation of large
quantities of sulfate while C to not loss than In older
sediments. The rocks of the JuMsic-Talangintan rich in
Corg and bitumen# however, contain such sulfur# I.e. even
more than tae organic substance Itself. Sulfates are practi-
cally lacking. In the sediments of the Turanian-Oligocenic
sulfur In mainly of mineral origin (about 0.23% of pure
sulfur)* The content ofsulfate sulfur and that of bitumen
are inversely proportional to each other. The Irons sulfur#
C org' and bituminous content on the whole increases tovards
the central part of the Khanty-Manslyak basin; the maximum
amounts of these components are found towards the western
edge of the basin (rig 2). The strongest concentrations of
authigenic Iron are found In loamy sediments at greatest
depths, while they are bound to the edge In swidy deposits.
There are 2 figures and 12 Soviet references.
Card 5/4

. Authigente Irong Sulfur, Organic Carbon, and Eltunina. SOT/20-124-2-43/11
In the Mesozoic Sediments of the Kastern Ural Raglan
ASSOCIATION: Tyusenskoye torritoriallnoyo geologicheakoyo upravloniye
(Tyusen'Territorial Geological Administration)
PRISENTED: September 20, 195st bY S- 1. Mironov, Acalemician
SMWITTED: September 199 1950
Card 4/4

111LOrNOT. T.Y. -- -
Katritation of oreanic carbon, bituawas, w4 ho&Ty bosocarbans
throughout the profile of Xwo-Cenosoic depcwtte In the eastern part
of the traw-Und region vItb rteard to the occurrence of petroleum
as4 Va. OWd. AN SM 1)4 20-3t654-657 6 160* (KIU 130)
1. flusecak" koffy1skscafs geologorwmedochwye sksWitalys.
VWstawleno skad. NoWe Itrakhonu.
(Siberia, %stern-fttroleas Cooloff)

HOURSKIMP GAG; KIKOWT -V.Ft; FROKUPKKKO, V.I.; fMKIUp L.T.; ROMARP F'.I.;
STEICHKOVO G.F.* nauchayr red.; MMMI 5: SIX T.I.,
vWwbobly r4d.o UUMCMIRUDLEAYA, AsO.0 tskha*red,,
(My wello of the U.S.S. U.; Sere saw key val2 (Tyummul Provisse))
Hbrssavo)*L~t opernala skwaskfm (Tium-laksla dGiwtf),* lentagred
Goo., nauchco-tokhne lsd-vo nefto i gorno-Uplivnel Ut-rrr loningr.
ot&-I*. 1962. 220 p. (Leningrad. VxesollasWi nefUaml naucham-
bwWavatallskil geologormodochr4i institat, Trudy,, me.195)
(KM 15 t12)
(Elerszovo region (Tyument Province)-Geoloa)

KIKWVO T.r.
SIPUlsomes of the bitawn coutdat Ln ore~&Lo matter for oU pr
pootft* Trudy SNIIGGIIG no.26tl456150 C62. (NINA 16 M
(Ktumms) I ~ (orgaide matter)

quqmitim of em" In pe &POOLts " dopma4at cw ma d"Ah
of eowwrmeo. lbkl., AK SM 147 no.3eTlD-= 1 162o,
(au 15112))
14, Tymmok"* torritarialluo7a gwacgichot*M upravlmiyw.
Pr"stavlato skadodkca K.K. Strakhov7s.

HIVONOV, V.P.
DistrIbutlan of heavy IWdrocarbons as an all and gas proffpecting
indicator. Geol. neftl L gas& 7 noJs25-429 JI 163. (FaRA 160)
1, XV XIIGG.
(mathar's)

NIFOROVO V.F.
Composition of the crudea cf the northern Oblvalley.
Geol. neftl i gaza 8 no. 1:20-23 Ja 164. (HIPA 17:5)
1. Tytimenakoye territoriallnoye geolcgicheakoye upravleniye.

-411MVC7, ;.Fl
ODearefiqs in ttey 4c -%I !roIr In Q-0) 2atitudinal 01~1 Valley tnr,~d
on a study of Vvit. rxrFut. Al field. Neft,*67RZ.geol. I jr-f-Vz.
I
nc. 1114-16 165. (MIRA 2915)
1. IIrj--nr,-nrkciye tf-rrItArIallnoy!, rt~ologlcherkoye uiravloni!n.

- lnrwwl, V.F.,,,
I . :,-17 0 , !,: .
Gavnj in tha o-'! fjeId3 cL' i`rcv~n-,,-, , .-I ~f
i. gfor. no.5110-12 165- ( ! 1' 1 -1, A I - : -, ')
1, Tyummkoye t~irrl tcrl till noyor.~ vr%,/1(,rI
- I

Lr

WC)DIKH114, P10"
G.Yd.,
[Technical and econor-IC, prindi'lCis Or the hant treatmnt
of retalel Tekhnicheskle i ekonotdchnskie osnovy temi-
chookol obrabotki metallov. YOPWR, YA5hir,06tr0"nie#
1965. 450 P. (MIAA legli)

JIIKOZIOV, V. F.
Variation of gas composition within gap fields. rokl. AN
SSSR 165 noo4t927-929 D 065*
(11IRA IM12)
1. Tyumentikoye territortallnoye gcologl&erkoye uIxavlenlye.
Submitted July 3p 1965.

ACC NRI AP6002912 501INT CODE: 1JR/02R6165/0001024/0074/0074
INVVITOR: SheRelyskavxkfZ, K. N.; Strrlannov, K._.,.V. Shkiyarov, 1. _11.: Orlav, T. V.;
141 kot
toy_t V. F. Assonov, A. P.
ORG: none
TITLE: Steel for aurface-har&,nod parts. Clnna 40, No. 177083
SOUR(;E, Rytilleten' Izobretenly i rovnrnvkh zn.0ov, no. 24, 1965, 74
TOPIC TA(,!!: steel, surface hardened nreel. mnn$,.nne-ie contnfnfnz steel, silicon con-
tainIng steel, chromium containing ntcel, shallow hardenable steel
AT)STIMCT: This Author Certificate introduces a steel for surface-hardened parts con-
tain ing 0.4-1.2% carbon and alloyed.with mangaiiese,silicon, and chromium. To obtain
steel with a specified bardenability, one of three alloying elerents is added In a
specified amount and the conLent of the other two Is limited. For example, in steel
containing 0.3-1.4% manganese, the chromium and silicon contents are lir-ited to 0.15%.
and 0.17%, respectively.
Steel with 0.3-1.4% silicon should contain 0.15% chromium
and 0.20% manganese, and steel with 0.3-1.8% chromium should contain 0.20% manga-
nese and 0.17-0.27% silicon. (AZ)
SUB CODE: Ill SUBM DATE: 29Dec6O/ ATD PRESS:41116

ZA'YY.OVP S.T.; UATMOV, P.Ya.; NIKIFOROV, O.V.; F.GVALI, *0'.",'(1.; V.I.;
1, - P
RUBINSKIY, P.S.; LIFSHITS, S.I.; Y-rNSTAPEA', V.F.;
VOZLINSKIY, A*G.
Using oxygen-blGvn converter steel in auto-mobilo nam:Afactiire.
Met. i gornorud. prom. no.4:26-31 JI-Ag 164-
(M."-',,A IP:7)

';I-M-C--,', V.G.; G.F.
Uso of thn precipitAt'lon In agar reactim for the detectim
of the 9--,thrkx antigeti IL arilmal orpns. Vom-e-nede thur* ri(~* It
53-54 Ja t66 1911)

icl_ Ali I it, It
Heatir,F f 1-:).~er trng.- ri-r-frzi w-' -F. f'~'c zi
~3

RKMV, V.I.,V / ,
-----~;o~dtonAr fodder yeast at tiv) Kotlas,,; s1cchol plant.
Gidroliz. i lesokhIm. prora. 18 no.3j24 065. (14IRA 18s5)

AIXLOSCNv S.Tp SLOW, V.I.
aftet at dflutlea m the debw&opmtlon of la"Bum in
the pnoeme of leilme Kklme I takh, tepl. I manl 10 W.39
n-u Nr 165. (KIPA 18i11)
1, Vaskmidy wdem TrWev"e Kramme Zamwal instiWt
mfUkMM4b*sk~y i p9my promphlemmoti in. akad, Gubkim.

HIKODYNIN, i. L.
KlK3NWj, T. L.t *PrincW*x or Constructing a Systex of Forest Park* in the
Suburban Forest-Park Zone or the City of Leningrsd.,* Kin
Higher Mucation USSR. l4ningrad Order of Lenin Fortatry
Engineering Acadwq iment S. K. Kiror. LenL-cr*d,, 1956.
(Dissertation for the Degree of Candidate in Agricultural
Science)
So: ralshnaya Lqtoplal, No. 19, 1956.

AMYOT' L.D.; RKINNOT, T.K.
TWooplasty of arteries in an infected wound; experimental observations.
You. mod, thur. aa.WS-30 If 157 (am 12 17)
(ARTIAM, experimental#
homonlasty of arteries In infected wdm. (Run))
(WOINW AID 11MRIM, experimentale I
ease)

AX)R&WA, Z.r., kmaj7hfaichookikh tank; KKOIi,,OV Ir 9
- of,
lopoliroqualwhLy ob7wmnwstL a Co usuchnogo
motrodnike
TribidrugWutairls "Id ad Mle mate @A a Wffor la
"Powatimc lanthauLdes by mans of Lon WWANWI*
clWomatopaphy. IXT. TSIM n0.3$196405 162, (MM 15:9)
(mutarlo seld')
(Chrmatopaphic awlyals) (Ran earth YAUIN)

NMUW;, T.N.1 SAKMCHr, A.A-w
Keeiria *uT=t oourft-t*r with alliom r"Uflor for mm, in
.*loctmwt4LUurgiwa axtorprises. IMoottricheatro ac*12s5"i
0 f62. (XML 15,121
1, Tsoooyawqr *lektro+Akbmish"kiy imUtat I~i rmins,
Msatri* currmt restifiers)

Lic t,_!, i
"The Iqeatigation of Oscillation Fluctuation of a Klystr_.-
Considered randca amplitude and phase modulation of klystron oscillationG,
caused by rwidom processes connected with the electron flov. Experimental measurements
of oactUation parameter fluctuations showed a coincidence with the theory ftmt deve-
loped by 1. L. Bernshteyn.
report presented at the All-Union Comference on Statistical L--IIo
Physics, aorlkly, 13-18 October 1958- (Izv. vyssh uctverwr zmfed-Phdlotekh.,
vol. 2.. No. 1,, pp 121-127) COMPLETE cazd under SIFOROV, V. 1.)

8M29
'?OVLZO X/L4L/5j/002/o6/oio/024
AVrIMz 91"Now- Y.N. BL92/9382
TITL9t ravestl6ation of the OsellLation Fluctuations in a
Klystroa-GSBerato lip
PICRIODICALs Investiya vysshikh uchebnykh sawodenly, RadioClaiks,
19590 VoL.2. Nr 6, pp 9L5 - 926 (USSR)
ABSTPACTz First, the problem in investigated analytically. Under
the assamption, that the resonator of the klystran can be
represented by an L, C and R *quivaLent circuit, the
dynamic equation of the system ist
di
- a v - RL M
4t
C +I
It- 0 1 + ft /2U )dvl /dtI
where v to the alternating voltage across the capacit
Cardl/4 L is the oscillation current Li the equivalent
circulto

$01V
5/141/59/002/06/010/0241
raw4otIgation or the Oscillation Fluctuaft2"ZIPS Klystron
generator
The second component in Itq (la) represents the current
induced by the *Leotram bean. t a in the cathode current,
Z 0 is the average electron transit time (from the
resonator to the reflector and back) and V a is the
voltage applied to the rtsonatore tn order to investigate
the oteillation fluctuations it is asaw-ed. that theme are
due to the shot noise and the Clicker effect in the
at*ctron bean; the th*rual noise is neglected. XC the
shot- a=d fLicker-eCCect directly induced currents are
denoted by C M and C M and the components due to
L 2
the reflected bean are denoted by CI(t) and C20(t) , the
dynamic equations of the system can be written as Cqs (2)
and (2a). goploying polar coordinates r and W (defined
by the last equation an p 9L6), Kqz (2) and (2a) can be
rewritten an Kqe (3) and (3a), where f and If are
expressed by tqs (3t). Zxpressions for the amplitude & d
Card2/4 n~K

802V
S/L41/59/002/06/OlQ/a24
Investigation or th* oscillation FLuctualijJ95112a KLystron Generator
phase, fluctuations are therefore given by gqs (4) and (4a).
These can also be expressed as gqx (51 and (5&1. Tht
solution of th*&* shows that the spectral densities of the
amplitude and rrequencr fluctuations are given by Kqs (61,
(6a), respectively. If theigonerator is isochronous,
thw spectral donsities of thoamplitudes and frequency
fluctuations art given by Zqz (7), and (7a). Those can
further be transformed into Sqs (8) and (8a). Tht effect
or the CLick*r noise alone on tho, earpLitude, and ftequency
fluctuations is described by Rqs (9). The problem was also
investigated ezp*rLm*ntal1y& the equipment employed in the
easurements was ximilar to that described in R*C 2. The
;
esults of tho experiments are illustrated in figures 3,
alad 5-and in two tables on pp 924 and qi5. Figure 3 shown
ther frequency dependence of the spectral density of the
frequency fluctuation for a klystron operating in various
modes. The spectral density or th* amplitude fluctuations
as a function of frequency to illustrated in Figure 4. It
to found that the experimental results or* in good agreement
Card3/4 with tho theory. For the normal operating modes the

9DI2.9
SAW59/002/06/010/024
Investigation of the Oscillation FluctuaR891112& JELyxtrou Generator
ne"wrod spoctral line width in 0.1 to 0.5 a/sl the
spectrum band of the ampLitudo fluctuations varies between
20 and 50 Nc/s and the xpectr&L d*nxitr Crow
to-iL6 to 10-15 c/o.
There are 5 figures, 2 tabL*o and 8 ref*rences, I or
which is Znglish and 7 are, Seviat.
ASSOCIATION: Mauckno-Isslodavatel'skLy radiefitichaskLy institat
pri Gortkovskon universitete (Sel antific -rag earch
RadiaDhysicm Institute of Gor'kLy UuLversity)
SUBMITT&D: Nay 17, 1959
Card 4/4

S/l4l/60/Q03/oc6/Q2t/o2S
E192/E382
AUTHORs Nikonov, V. N.
TITLA: Concerning a Method of Measuring the Amplitude
Fluctuations of an oscillator
PERIODICALs Izvestiya vyeshikh uch*bnykh tovedoniy,
Radlofiziks, 196o, Val, ~* No* 6o pp. 1129-1130
TEXTs Recent work by Hgggblom (Ref. 1) described a method
of measuring the spectral density w,(OJ of the amplitude
fluctuations of a klystron oscillator in the low-frequency
region. A block diagram of this equipment is illustrated in
Fig. L. The investigated oscillator I is frequoncy-stoduLated
by the oscillator 7 ; the modulated output of the oscillator
in applied to a crystal detector 2 where the doubled modulation
frequency to separated. A signal is then detected again by
means of a vacuum diode 4 and itp spectrum is analysed by
means of a spectral analyser 5 The calibration of the
instrument Is performed by means of an oscillator 6 which
produces a calibration signal at the Input of the analyser.
Card 1/2

S/L4l/6oj'oo3/oo6/O.- it/025
Concerning a Method .... F192/E38:!
The above method of measurement is discussed In now* detail
and it to shown that, in his experiKents. Hdggblom (Ref. 1)
measured the spectral density or the asplLtude rLuctuations
of the klystron oscillator over thefrequency range from
3Q.001 to 30.1 Vc/s instead of the frequency range 0.001 to
0.1 kc/c (ax was assumed by lfdggblom).
There are I figure and 3.referencess 2 Soviet and
I non-Soviet.
ASSOCIATIONs Nauchno-issledovat*10skiy radtafizichaskiy
Lnstitut pri Gor1kovskam univerattete
(Scientific Research Radiophysics Institute
or Gorlkiy University)
SUBMITTEDs April 29, 1960
Card 2/2

t594Y
AUTKORlt MaLakhove A.N. and Kikoftov# Y.N.
TITLZs Correlation of the Amplitude and Frequency
Fluctuations In Oscillators
PERIQUICALs ISVG~tiya vydahLkh uchtbnykh cavedenty,
Radiorialka. 1961. Vol. 4, No. I$ ppo 104 r IL2
TEXTt It to assumed that the signal produced by the
oncIllotor to expressed byt
X(t) a A.[1 M(t )I cog IWO t +
where m(t) and V M are rolatLvo fluctuations of
amplitude and frequency which arokin the Coro of stationary.
random processes such that
0
where the Line above the systbaLs represents statistical
Card 1/8

15949, S/L4L/61/0041001/0091022
QrrelatLam of the AXPLitudo E192/9382
averaging. Zn order to doterodno the spectr~al density of
the power fluctuation V K(W) . It Is necessary to determine
the correlation Function q?,(T) which, in turn, is dependent
on the correlation functions or the amplitude fluctuations
frequency' rLuctuations (I ft) and crone correlation
U These functions have been dottradned for saw*'
#special cases (Rot, L - S#M* Rytov - Zh=Fo Vol. 29, 304, M,
1955). On the other hands In this work an attempt is made to
-find .COO and Q.,(T) for a large range at
Oscillators. It"is assumed that the oscillator signal Is'
governe4 by tho*foL!.owtng dltCormtial equation (Rot. 2 -.
A,N. Malakhow Izv* vyssh, uch, zav. Radiofiziks. V01. 3,
.241, 1960)1
d'
it's -,F + E(f).
6-0
Card 2/8

~1141/61/004/001/001022
Correlation of the Amplitude ... U92/9382
where S(t) represenis the noise* The fluctuations -S(t)
and G(t) are expressed by the CollowLng equations (ReC. 2)s
+ pNi (~a + a
Lt.L + bLZ4 + b49Q/4AO
a ps (a lc a It.)/GA
0
zq* (3) can also be written In a more convenient formt
9, )/GAo
whore VJL (aabu + WS NThe noise oaw*bo expressed by
9(t) 2 (0004(a00 C.L(t)OWN 00 (6)
Card 3/8

SIL41161/004/OOL/009102'2
CorrelatLan or tite AmpUtuds eL92/9582
lo
L(t) are GLowly changing CunctLons of time.
where 191(t) and 9
It Is shown that these components can be expressed by:
.function of the noise is given by:
The correlation,',
COS(.t) d..
which can be approximately be expressed by:
A*(,c) cot (w,-!) - A (LO)
where and. ~A'L are slowly changing functions which are
defined bye
Card

Correlation of the Amplitude ... F.192/9582
io. (U) COO
46
(2) VIP M (N.
Ali( s .
By solving Sq* with respect to s(t) It to found thats
c(t - C)O-pCdC (Viji
where f M (014, Ic-L + ej-'I, )/'Ao s The final. expression for
the am 11tude correlation functLolb, derived an the basis of
Sq., (IC9 I* In the form:
Card 5/8

S/141/61/0041001/009/022
25949
Correlation oC the Amplitude SL92/Z39Z
0
A (,- + Y) 4- Y) -PYdy
W)
W
0~ 2
From this it is "sy to find the spectral dwwitjr of bhe
ampLitude fLuct*atlonx; thisIs expressed by:
2 2 2
VC40 2WO-(CL)/6A (p +-X2 OLS)
iihown that the corroLALon function 'for the.
Similarly, it is
frequency ftuct~tationm is given bys
As(-. ++ AI(i y)
-,,I dy .4:
2
(20)
At(-:,+ y) A'(- dy.
Card 6/6 2

S/l/a/661/0041001/0071G22
Corr' lation of the ANATM ... 9192/E362
whil: the croms-c*rrelation function 'for the fluctuations In:
+ y) + A"(- y) dy +
CA29 I P (22)
+ S At(- + y) e -,-y dy
The above expressions are used to anaLyes ;oftQ'sP4cLaL cases;
0
2) the derivative, of Wit (w) Ln the vicinity of w a 0'
is ftot'~Gqusl to,26000 and'.
the nolso is avach tkat its op4otcum in tfte vicinity of a
has &'width comparibl'o with p or'Leas than' P * Frm the
above it In concLu#ed that for the existence of crone correlation
between the amplitude and frequency fluctuations of an oscillator
it is necessary and sufficient that one of the following
conditions be fulfilled:
Card.7/8

S/L4l/61/Oo4/OQVOO(J/QZ2
Correlation or tho- AmplW499 ... E192/9362
a) .81multaneausly. t% A 0 and b.L 4 0 Is tfio came when an
oscillator to nontsachroncual 0
b) simultaneously, &,i A 0 and aj. A-0 , which abourn when
the lefthand-side portion or Sq. (2) contaLns,even as well as
add derivatives, and
c) the spectrum of the noise in the vicinity of a 0 in
asymntetrIcal with respect to a 0 . It is clear that In all
actual oscillators at Least the third condition Is fulfilled.
It to therefore, necessary to take Into account the cross-
correlation between the frequency and ampLitudw fluctuations
in d*terminlng the spectral line W xW of the oscillator.
There are L ftgureland 8 Soviet references.
ASSOCIATIONOO N^ujhno-IxsledovatoVxkLy radLqfLs1cheskLy
Institut prL GorOkovsk6n un1versitato
(SciontLftc Research RadkophysLes Institute at
GarOkLy University)
SUBMITTCD: Fob' ary 28, L960
Card 8/8 TU

33U2
sAW61/004/006/009/017
2192/1382
9-6 0 Po
AUTHONSi Nalakkov, A.M., Mikonov, and Razina, T.D.
TITLE; Some methods and results of measurements of
amplitudo-ond frequency-fluctuations In oscillators
PERIODICAL: lavestlya vysshlkh uch*bnykh xavodtnty,
Radtoftstka, v. 4., no. 6, 196L, to52 - zo6k
TEXT.- Two methods of measurement of the spectral density
of frequency fluctuations are hmown (Ref. 2- 0. Middleton -
Trans. IRZ, RD-I, 56, 1954; Rof. 5: I.L. Bersht*yn, Izv,
AN SSSIN, ser.fix., 14, L45, 1950). The methods are discussed
ad evaluated and one of them Is employed to measure the
aramoterz of an experimental oscillator. In g*noral, the
:
easurement of the fluctuation spectra in an oscillator to based
on the system Illustrated in Fige 1, which consists ofi
I - a discriminator; 2 - detector and 3 - anal]ftr. The quest-
chromatic signal applied to the Input of the discriminator to
in tko Core:
Card I/ItY x(t) - Aa [I + Q(t)1con (Wat + ~_a Wdt) (1.1)

)3222
sA4i/6i/oo4/oo6/ooq/oi?
Scmee methods and results of os.* 9192/9382
where a(t) and -%)(t) are stationary random processes having
a cress -correlat Lou function '~r such that
0 0 , a 2