SCIENTIFIC ABSTRACT YERKOVICH, S.P. - YERLYSHEV, P.A.

• Document Type: CREST
• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R001962730001-2
• Release Decision: RIF
• Original Classification: S
• Document Page Count: 100
• Document Creation Date: November 2, 2016
• Document Release Date: September 1, 2001
• Sequence Number: 1
• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT

SoV/51-6-3-4/28
The'oscillator Strength of the -System of No Bands
obtained experimentally by Weber and Penner %Ref.3)
is wrong) because the latter workers assumed that the bands
overlap very much; in fact there is very little Overlal
(Fig.2). Acknowledgments are made to L.M. Biberman who
directed this work, and to V.A. Fabrikant for his advice-
There are 2 figuress 3 tables and 12 references, of.whieh
9 are Englishp 1 German., 1 French and 1 Soviet.
SUbMITTED:'March 17? 1958
Card 2/2

I Bibanaan, L.'-'. , 22E~2~~ and 5oshniirov, VX.S
M TIZ Or, the frobability of a Transition in the 4c1uaann-2%ua6o Band aystam
of the 02 '-018culs-
4RIODIU%L; Optlka I spektrukopiya, 1959, Vol 7, ',*T,r 4, pp 662-563 (wi.)it)
.D.4W"(;T: Kock, Cezm und Kival (Rof 1) wousured tho absoluta intensity of
a4vilon oy oxygen at 410004 at -oavelon6ths of 3000-~%00 A. They
COL,pured the expariwental data with an approAimate expression for the
intensity of amiusiou given in an earlier paper (Ref 2) and concluded
that tho oacillutor strength for the ~ichumann--;Aunge band 3ybtOM Of 02
is f = 0.015; this value Is much smaller than that dad-aced from
aLsorption by cold 02, which vas given as f = 0.16-0.2t; (Refs 3, 41.
Kock at al explained this 1-Ar6a difference be"~een the t-..o values of
the oscillator strength to be due to dependence of the probability
of an electronic transition on internucloar distances. The conclusions
of Kock at al are questioned by the present zLuthors, -Rho compare the
experimental data of Kock at al with a stricter expression for the
intensity of emission IX (Eq 3). Using the exparilaental values of I~
and Eq (3), the authors calculated R2(;k) , where Ro(;kj Is the -electronic
Card 1/2 moment of a transition, which may depend on Internuclear distance. It

Or, the Probability of a Transition in the 4ch=ana-Run~;a i~and z~yatem of tila 02
Molecule
was found that R2 P.
T a ) falls monotonically frcxa 1 atomic unit a'
3000 ~, to 0.5 Utomic unit at 5000 X (sea the dashed curve in a
figure on p 563). These values of R2(~) corresiond to an oscillator
stren&th f = 0.1-0.2, which agrees quite well with the ralues of f
dedu~od from abborptior. (Rofs 3, 4) and INIth theorotical estimat8s
(Refs 5, ~J. Usir.6 the vulculated v-Alues of Rj(X) and a set of Franck-
Condon multipliers q(v, v"), Zq (Z) was found to yield the distribution
of inten.sitias in the WIckumann-Runge system betwaan 3000 and 50G0 1. at
2000, 4000, 4100 and 60000K. These intensities are plotted as coutinuous
straight lines in +-ha figur3 on p 563. Aucknorled6.ient is xade to
I.T. YaWbov tho supplied his set of calculated Franc k-Gond on factors.
There are 1 figuro and 11 Sni;llsh references.
SUEMITT21D.- Fabruqry 3, 1959
Cu rd 21/2

69834
8/051/60/008/03/00V038
K201/Z191
AUTHORS.s Yerkovich, S.P., and Pisarevskiy, YUJ.
TITLEt A-On the Transition Probability in the y- and P-Systems of
Vk NO Bands
PERIODICAL: Optika i spektroskopiya., 196o, Vol 8, Nr 3,
pp 303-306 (USSR)
ABSTRACT: The absolute intensities of the electron transitionsito
the ground level in NO molecules have recently be of
great interest in connection with emission of radiation
by hot air (cf Ref 1). The present paper reports
calculation of the electron transition moment Re(r) for
y- and p-systems of NO bands (transition A2:E-x2n and
B2n-X2f7 ) using the experimental data on the absorption
spectra reported by Marmo (Ref 2) a-nd Mayence (Ref 3).
Calculations were carried out using the method described
by Yerkovich (Ref 4), modified somewhat to allow for the
s.trong dependence of the electron moment on internuclear
distance. The electron transition moments of the a(5, 0)
Card band (the mean internuclear distance in the vi-v"
1/2 transition F = 1.201+ A) weres Re = 0.106-0.115 atomic
units at pressures from If to 101 mm Hg in the ease of the

69634
S/051/60/008/03/00)+/038
B201/1191
On the Transition Probability in the y- and p-Systems of NO Bands
short-wavelength maximum of-the band, and
R817- 0.109-0.120 atomic units at pressures from 4 to
1 mm Hg in the case of the long-wavelength maximum.
The electron moments for the y-system were found to be:
Re = 0.129-0.11+5 atomic units.at p = 4-50 mm Hg in the
case of the long-wavelength maximum of the y(2, 0) band
(Y = 1.162 1); Re = 0.129-0.144 atomic units at
p = 10-14.8 mm Hg in the case of the long-wavelength
maximum of the y(l, 0) band (i; = 1.135 A);
Re =10-136-0.166 atomic units at p = 10-11f.8 mm Hg in the
case of the short-wavelength maximum of the y(l 0) band
(F = 1.135 1); Re = 0.154 atomic units at p = 14.8 mm Hg in
Card case of the short-wavelength maximum of the y(Oj 0) band
2/2 (F = 1.108 A).
There are I figure, 2 tables and 11 references2 of which
I is Soviet, 6 English, 3 German and 1 Swiss.
SUBMITTED: March 24, 1959

69835
8/051/60/008/03/00V038
E
201/1191
AUTHORi Yerkovich, S.P.
TITLE: Coefficient of Continuous Absorption of Radiation by
Quasi-Mojecules of Hydrogeff-
PERIODICAL: Optika i spektroskopiyal 1960, Vol 8, Nr 3,
pp 307-311 (USSR)
ABSTRACT: On transition from the excited state lsa2sa37-+ to the
9
unstable state lso2pcr3 'Z+ a hydrogen molecule emits
continuous spectrum whichu extends from 1800 to 4000
The H2 molecule dissociates then into Wo H atoms in
the ground state. The converse of dissociation of an H2
molecule, on emission of a continuous spectrzzmy is
recombination of two H atoms on collision along the
potential curve of the unstable state with absorption of
-1
light and formation of a quasi-moleoule in the 32:9
state. The coefficient of such continuous
absorption is proportional to the number of atoms in the
collision state. The present paper describes oalculation
Card of dependence,of the coefficient of absorption of
1/2 radiation by quasi-molecules of hydrogen as a function of
temperature and the concentration of hydrogen atoms.

69835
8/0 51/60/008/03/00 5/03 8
E201/E191
Coefficient of Continuous Absorption of Radiation by Qaasi-
Molecules of Hydrogen
It was found that in a wide range of temperatures and
pressures the quasi-molecular absorpt s important.
Tables are constructed from which the 'W rption
coefficient can be found under given Indoitions.
There are 3 figures, 1 table and 10 references, of which
Card. 1 is Soviet, 1 German and 8 English.
2/2
SUBMITTEDt March 28, 1959

MKOVICH
I S.P.; F1SAWjBKjY$ yu.V.
Strength of an oscillator for the S'-system.of ITO-bands. Opt.
i opektro 9 n0,2:269-270 Ag 160. (MIRA 13:8)
(Nitrogen oxide-Spectra)

ymovim; so P.
"On the Account of Significance of Electron Transitions in
Molecules at Calculation of Emissivity of High Temperature
Gas Radiators.r
]Report submitted for the Conference on Heat and Maas Transfer,
Minsk) BSSR, june 1961.

. . . I- . I . - I I I : I . I - I , , - I . I I , r - . , A r. , ! ; r 7 1 1 '1 , '. .II -
-S U U P '- L KI e k ! r,, - 9 v y a z, ' . P, i ~ . ; Z 4. :1 -Z,
ropic TAGS. optical corru-nunicaElur-. iaser optical c-rrier
re Z~"
ABSTRACT- The range of a I~kger comm,imration channel in outer spa .ce is
- I ~ ~ , - ! -A -.4 , - ~k ~ a f r a , a ( w i t h. - h e i r
Card I / Z

L 20719-65
ACCESSION NR. AP5-P-101370
t%e wavelergth has a decisive effect on the- maximum paggible range under fog
! (), g. a-t. has: 3 fgur, ~Lz,(, Ib formulas.
ASSOCIATION: none
SUB?~UT-l ED: 28Feb64
ENCL: 00
T H E R
min
Card 2/2

.- ~ I, ... C,
)MRKOVICII, S.P. I- l'ISA',,'LVSUy N.V.; . .0.
- _--- 1.1-
~bthodology of determ-'rulng the oocillator fc:-,,e.; -'Cr clactl-=
tran3ltlon3 in mol-jLulos. Opt. i spektr. 17 no-!OG-34 Jl
Oulu -1,1..g)

ALL NMI A 017254 SOURCE CODE: UR/0058/65/0OO/0i2/D071/DO7P
AUIMOIR: Yerkovich,_ S, p ; Pisarevakiy, Yu. V.; TreguLov, G. A.;
Arreshin, -7-.S.
TITLE: Optimal orientation of cubic crystals for Bight modulation
based on the Pockels effect
SOURCE: Ref. zh. Fizika, Abe. 12D599
REP SOURCE: Tr. uchebn. in-tov svyazi. M-vo svyazi SSSR, vyp. 23,
1964, 103-105
TOPIC TAGS: crystal orientation, cubic crystal, electrooptic effect,
light modulation- .1
ABSTRACT: It has been shown that in\Lelectrooptical crystals of the
cubic system the maximum transverse electrooptiegl effect takes place
during crystal orientation when the or E in perpendicular to the
plane (110) and the direction of the light beam is correspondingly
perpendicular to the plane (110), [Translation of abstract) [AM)
SUB CODE: 20/ SUBM DATE: none/
C"A IA pb

I
! , I . : . I , .4 . . I
i ,

I. - T , . . - ~,l L~ . I . I I C,
I

L 2818-66 EWT(I)/T IJP(c)
ACCESSION HRI AP5016170 UH/O( 01 006/M9/003
539.10.001.1
AUTHOR:
~ah~inr. ~G. C9
TITIZ: Oscillator strengths for the 81 rp and 0 systems or the No bands
SOURCE: 0VtikA I spektrookoplya, Y. 18, no. 6, 979-963
TOPIC TAGS: nitrogen oxide MUlator strength
optic spectrum
ABSTRAM The
((~Pt. Oscillator strengths calculated by a Procedure dev'eloped by the au-
thors I spektr. v. 9,, 269, X96o and earlier PaPers)'are reviewed more thor-
Ough4j, as a result of a more rigorous analysis which has shown that the oacill or
strength for the r system or bands should be taken to be much lower. The new cal-
culations were made with the eXWIMnW results published by Fe F. Ma=o (J. opto
Soc' Am' V- 430 11WP 1953) and J- MaYence (Ann. fts. V. 7,4", 1952). Value.
re = 0,0059 and fe = O,OV
)8 are obtained for the Oscillator strengths in the vave-
length regims corresponding to the bands 8(0# 0),p 7(2# O)p and 0(5# O):G The value,
obtained for the first band Is 0,09T. Orig- art, hast -27 formulas*
ASSOCIATION: none
SUBMITTED1 3,9Dec63 ENCL: 00 so CODE: op
im mw sov: oo4 OTHER: OIJD
_qard

61 MULK.30VA; -Q,,Xo.
Photographic magnitudes at maximum and minim- lWightness of
109 long-period cepheids and their reference staft. Trudy InBt.
astrofiz, AN Tadzh, SSR 9:66412 162. (MIRA 16.5)
(Stars, Variable)

SOLOVIYEVp A.V. Coeoeased]; YFJ=3OVAp G.Ye.
Photometrio study of 26 variable stars in Orion. Biul.Inst.-
astrofiz.AN Tadzh.SSR no.340-28 162. (MMA 1-6:5)
(Stars, Variable)

EMEK30VIIII G. YO. _
Stars, Variable
w
,rwo riew variables SPZ 1112 Oph and 3PZ 1113 OPII- rer. zvpzdy 8, No. 4, 1"-51-
9. Monthly List of Russian Accessions, Library of Congress, Ifay -1953. Unclassified.

-- I
E. I ILI ~' I IL IM *11 A, 1j. Ye.
Stars, Variable
*IS Leporis, Per. zvezdy 8, No. 4, 1951.
9. Monthly List of Russian Accessions, Library of Congress, May -1953. Unclassified.

YFJWKSOVA,G.Ye.
f~
V 337 Aquilae. Per.zvezdy 9 no.1:86-88 S152. (KLRA 8:10)
1. Stalinabadskaya antronomicheakaya observatoriya AN Tad-
zhikskoy SSR
(Stars, Variable)

K-,L:-;Y3OvA' G. Ye.
Stara, TarlilblO
-RR Loporiaj Aotron. t3l"- r.1o. 125P 1952.
9. Monthly List of .Russian Accessions, Library of Congressf May -1953. Unclassified.

ERLETSOVA I G. Yu.
Stara, Variable
Mirida. 33V Draconi3. A3tron. tsir. Ne. 131, 1952.
9. Monthly List of Russian Accessions, Library of Congress, May -1953. Unclassified.

-I'rjtLL:'K7'OVA, G. Yo.
Stars., Vari-able
Brief notes on certain va~-iable 3tars, Astron. t3ir. No. 131, 1952.
9. Monthly List of Russian Accessions, Library of Congress, Vay -1953. Unclassified.

- -Af- VA,-gTt t 11NOVSVAY-0 -GP 0
Eclipses, Lunar - 1952
Integral photometry of the lunar eclipse of August 5, 1952. Astron. tsir. no. 131, 1952.
9. Monthly List of Russian Accessions, Library of Congress, MAY ' -1953. Unclassified.

EMULK50VA, ~-J.
Stars, Variable
ohort-period Cepheid UP 4154, Aotron. tsir. No. 131) 1952.
9. Mqnthly List Rf Russian Accessions, Library of Congress, VaY -1953. Unclassified.

YZMKSOVA, O.Ye.
Short-period Cepheid variable KZP 4154. Blul.Stal.astron.obser.
no.5:22-24 '53, (MM 7 -'10 )
(Stars, Variable)

TERLMOVA. G.Te.

Determining the solar apex relative to cloud s of interstellar
0&10ium. Blul.Stal.astron.obser. n0.5.'17-21 153. (" 7110)
1. Gosudarstvennyy Astronomicheakiy institut Imeni Shternberga.
(Sun)

W 'Aff.Va"P UW.R ON

E 94
-0
M
W
t-iTRO
.
-VO

YIUMSOVA, G.Yo.
- r'--44 *4~ - w J~-- imi~a~~~"
V499 Scorpl6nim. Biul.Stal."tron.obser. no.6:21-23 '53.(nn 7:9)
(Stars, Variabl*)

YF-tLEYSO1IA,, Go Ye---
ysten, Eclipse of the I'loon (4272)
Solar S
yullo Stalinabadskoy Astron. Observatorii No 7) 1953" pp 26-28
B
Bakharevj A. Mop and Yerleksova) 0. Ye.
Observations of Vie Fall Lunar Eclipsep 29-30 January 1953
The authors conpile a table of variation of illumination by the moon depending
on the phase of eclinse) by using measurements by 0. Ye. Yerleksova and No No
Suslova made with a vledge photometer during clearance of clouds.
So: Moscow, Regeratimyyp Zhurnal -- Astrommiya I Goodeziya no 7j 1954 W-31059

YJMIXMVA, G. Ye.
Short-perioCCbpheid XZP 4065 Sagittarl. Per.svezdy 9 no-3.-
219-221 Js 153. ( M A 7:7)
1. Stalinabodelmys astronomichookaya observatortya.
(Stars, Variable)

YARUKSOVA, G.Ye.
TZ Aquilae. Astron.teir. no.138:9 My 153. (MLRA 7:1)
1. Stalinabadalraya astronomicheakaya observatoriya Akademii nauk
Tadzhikokoy SSR. (Stars, Variable)
0

P;RL&KSOV.t~. G.Ye.
, -- - %".'
Maxima of stars of the Hira type. Astron.tair. no.13C:9 My '53.
1 (;tLqA 7: 1 )
1. StalinabadBkaya astronomiches'"ya observatoriya Akademii nauk
Tadzhikskoy SSR. (Stara, Variable)

-
Corrections for photographic magnitudes of stars of different
color in relation to type of plate used. Biul.Stal.astron.obser.
no.9.'13-18 154. NLRA 8:1)
(Astronomical photography)

YMUK'SOVA. G.Ye.
Remarks on some stars from the atalog of Variable Stars and
maxima of Mira-type stars at 12~1 _. ,5h. ;stron.toir. no.148:
15-16 Ap 154. NLRA 7:8)
1. Stalinabadekaya astronomichaskaya observatoriya Akadamii nauk
Tadzhikekoy SSR.
(Stars, Variable)

TOLUSOVA, G.Te.
... ...... -
Brier dAta on 10 stars from the Catalog of Variable Stars.
Astron.teir..no.155:14-15 D134. , (XLRA 8:6)
1, 3talinabadskaya astronomichoskaya observatortya AN
Tadshikskoy 'SO, -
(Stars. Variable)

URLEKSOVA, G. To.
r ,~~
Maxims of five Mira variables. Astron.teir. no.153:13 1) 134,
(XLBA 8:6)
1. Stalinabadskaya astronomichoskaya observatoriya AN
Tadshikokoy 30
(Stars, Variable)

YKRLEKBOVA, G.Te.
M-
Cepheid 55 Canis Majoris. Biul.Stal.astron.obsero no#14:
32-34 155. (KJU 9 t 10)
(Stars, Variable)

YMUZKSOVA.G.Ye.
-~ -11-i'L'"I,
Maxima of 4 Mira variables. Astron.toir. no.156:18-19 Ja'55.
(KLRA 8: 10)
1. Stalinabadekaya astronomichookeya observatorlya
(Stars, Variable)

YERLEKSOVA G.D
f-.vs!Y.W-
, t.
~'t
Capbeld AT SagIttarli. Perozvazdy 11 no-1:55-58 Ja '56.
(MLRA 10:2)
1. Stalinabadekaya antronomicbeekaya observatortya.
(Stars, Variable)

TIRLYXSOVA, G.Tee
I - Stal.astron.obser.
Long-period Cepheid RV Scorpidnis. Biul (an 9: 10)
no.15:24-28 '56.
(Stars. Variable)

YERLEKSOVA, G.Ye.
Irew long-period Cepheid IZP 4952. Astron.tairk. no.170:18 056.
(KM 9:10)
1.StallbabadskmWa astronomichookaya observatorlya Akndmii nauk
Todshikskoy SSR.
(Stars, Variable)

~Q Too
VA,lm of 17 Mira variables in Sagittarius. Astron.teiric.
no-VU23-24 J1 456o MRAL 9: 12)
Is. Stalinabadskays, Astronomichealraya observatoriya Akademit
muk Tadshikokey SSR.
(star*. Variable)

YMMEKSOVA, G.Te.
Brief remarks on nine uninvestilgated stare from the IZP.
Astron.tsirk. no-171:24-25 JI 156. (MLRA 9t12)
1. Stallnubadskaya Astronomicheskays. observatorlya.
(Stars, Vurlable)

YMMMSOVA... -Jo. .. - ~
vionsw9sloom - - - -
Now long-porlod Cepheid UP 4
9_32, Biul. . ft&l. >you. obser. no. 18:
17-19 156. (Stars, Variable) . (KM 10:6)

YE"WRKSUI;~'
~-or.'rlod Of CRBSiOPPI'se. Astron.teir. no.178:24 Pr 'j?.
StalinAlmdakRym srtronomlchoskayA ohn9nmtorlyn ivnkizenjj am:.
2gazhikskoy SSR.
(Stars, Variable)

Yv-q SOYA, G.Ye.
"F
V 889 Aquilae. Astron. tair. no.181:21 Jo '37- (MIRA 13:3)
l.Stalinabadskaya astronomichosicaya observatoriya.
(Stars, Variable)

YBRIAMOVAt, G.Y~,,-.

aR *apecuias - an eclipsing variable with apsIdal motion. Astron.
tair. no.IBZ:ll Je '570 (mm lit3)
1. ftallusbMaka7a astronomichaskaya observatoriya AN Tafthikskoy
SSR6
(Stars, Variable)

pl-
g
iz
M
N
01~
-
il
o
Ng
o

TERLEKSOVA, G.Ye.
Normal minima of ZZ Aquilne. Astron.tair. no.184:21-2? S '57.
(MIRA 11:4)
1. Stnlinabodskaya astronomicheeknyn obgnrvntoriyn AN TAdzhikskoy SSR.
(Stars, Variable)

41

YERLEKSOVA, G.Ye,
Changes in the period of ZZ Aquilae. ]Par.zvezdy 12 no.4:293-297
Ja '58. .(MIRA 13:4)
I.Stalinabndakaya antronomichosimya observatoriya.
(Stars, Variable)

YERIMOVA, G. Ye.
DR Vulpeculae- an eclipsing variable with apsidal motion. Per.
zvezd7 12 no.4:298-305 J& 158, (MIRA 13:4)
1, Stalinabadekays astronomioheskaya observatori7a.
(Stars, Variable)

TIRUCKBOVA, G.Yo.
Xclipoing variable QQ Cassiopeia*. Blul,Inst.astrofiz.AX
TIsdxh.BSR no.25:23~25 159- (MIRA 1315)
(Stars, Variable)

SYC
k SMA.-a-ya-,
I
Investigativg the e"or of the fie2A of the "Industar-17'
loan of the astrograpb at the Stalinabad Aotrophysical rnsti-
tuts. Blul.astrofis.All Tadzh.SSR no.26%25-27 159.
(HIM 13:5)
(Telescope)

.TZRLIMSOVA'G.Te.; LAME, G.A., PMVA. N.B.; SATANDvA, Xjt.; IMIDpoy,
---~~-W;-FTSARXTSXIT, G.S.
QX Cassiopoiae. Astron. toir, no.'201:12 Ap 159. OMIA 13:2)
191ustitut astrofIsIkI AN Tadsh. SSRo Odefskaya, astronomichookaya
observatorlya, Gosudarstrenr7y antronoodchookly Inatitut in. P.x.
Shternberga i Antronomichookiy movat AN SSSR.
(Stars, Variable)

Phot~graphio observations of serven Cepheids. Biul. Inst.astrofiz.
AN Tadzh SSR no.29M-L-L-160e NIPA 1412)
. . 0 7cepheids)

LANGEp G.A.; PERNA, N.B.; SATANOVA, E.A.; KHolopovo Pilf.;
G.S.
Ql Cansiopoiae. Ver.zyesdy 13 no.141-51 Ap 160. (MIRA 14:3)
1. Inotitut astrofiziki IN Tadshikokoy SSR; Odemskaya astrono-
micheskays, observatori7a;'Gosudaretvennyy'astronomicheskiy
institut im. Me Shternberga i Astronomichookiy sovet AN-SM.--,..
(Stars, Variable).

YERLEKSOVA, G,.Ye.
Photographic observations of 13 long-period Cepheids. Biul.Inst.-
astrofiz.An Tadzh.SSR no.30:28-61 161. 1.5:31
1 (Cepheids)

W-- -
YEIIEKSOVA, G.Ye.
Brightneos variation of Z Androwdae in 1941-1963. Blul.Irct.
astratiz. AN Tadzh.SSR no.37:43-1,4 164.,,
(MlFLA 18il)
It

MIKIIAYIDVIGHp S.M. I'PF~~=OVAP 199 ve I
Remote reBults of P210 inJuz7. Hed,rad,
(POLONIUK-TOnCOLOGY)
6 no,,3954-58 161.
(KM 1435)

Vof.KOV, I., rO..; R., otvet9tven,,-y vypnsk,
tekhn.red.
(No"otoy collective fares; York practices] Xclkhot imeni Yolotova;
it opyta raboty, Alms,-I'Va, Kaznkhekoe gos. izd-vo, lf)54. 54 p.
(M MA 11: 13)
I.CcllectlTe farms)

YERLEPESOV, S. N.
"Agrotechnical Methods by Which to Obtain Greater and More
Reliable Crops of Cotton atthe iPakhta-Arall Sovkhoz." Cand Agr
Sci, Sci-Res Inst of Soil Science, Kazakh Affiliate of VASKhVIL,
Alma-Ata, 1953. (RZhBiol, No 4, Oct 54)
Survey of Scientific and Technical Dissertations Defended at USSR
Higher Educational Institutions (10)
SO: Sum. No. 481, 5 may 55

USSR1 ,Theoretical Physics - Quantun Theory of Fields. B-4
Abs Jour : Ref Zhur - Fizika, No 4, 1957, 8483
Author : lerlet
Inst : Institute of Nuclear Problems, Academy of Sciences, USSR.
Title: : The Salam-Polkinghorne Classification and the F-tateron
Charge Hypothesis.
Orig Pub : Dopl. AN SSSR, 1956, 106, No 2, 236-238
Abstract : The author reformulatea the classification of elementa7-j
particles by Sal" and Polkinghorne (Referat 2hur Fizika,
1956, 33814) with two quantum numbers o,"3 and,,4, 7 tt.,th
conservation of each one individually is aasQ- only as
strong and electromagnetic interactions. With this ht
employs a concept of the neutron charge E , introduced
by the author earlier (Referat Zhur Fizika, 1956, 12632)
with the aid of the equation E -2 -C vhich nov is
,written in the form C A -3- Thi'neutron char-
'hess s by the equation
ge-3 connected with the s;ra:;g
Card 1/2

USSR/Theoretical Physics - Quantum Theory of Fields. B-6
Abs Jour Referat Zhur - Fizika, No 4, 195-7, 8483
a - f- +E tN (N Is the number of antinucleone minus
the number of nucleons)& It is assumed that the neutron
charge is conserved at strong and electromagaetic inter-
actions. In slow processes (for example in -the decay of
hyperons and heavy mesons) there occurs a change in the
neutron charge. Classification of the processes by chan-
ge in neutron charge coincides vith classification by
change in strangeness.
The author believes that the approximate law of conserva-
tion'of neutron charge., not necessarily connected with
the assumption of the existence of isotopic spins, is,
along vith the exwt Imm of consomtion of electric
and nuclear charges, the most general foundation for the
classification of elementary particles.
Card 2/2

YERLICHENKO, M.P. flErlychenko2 M.P.)
Painstaking care of machinery as a guaranty of success. Yekh.
sill. hosp. 14 no.11:9-10 11163. (MIRA 17:2)
1. Inspektor gosudarstvennogo tekhnicheskogo nadzora
Zuyskogo otdoleniya "Sillgosptekhnikill Krmyskoy oblasti.

Y,2~111111 11
F-20 Lr 161.
Creative cooperation. Ocv. profjoivzy 17 Lo. 4~;2, ,
OT-1 14:21'
(Linin:~rad--.J'hl.prdn,-,)

BURLOVA, L.Ya.; )7_9LIZAROV -V.A.
Results of the studr of cardiovascular diseases in industrial
workers; data on mcrbidity with A temporary loss of work ability.
Trudy LSGI41 72:5-10 163. (MIRA 17:4)
1, Kafedra gigiyony truda (zav. kafedroy - prof. Ye.TS. Andreyqva-
Galanina) i kafedra organizatsii zdravookhranoniya (ispolnyayushchiy
obyazannosti zaveduyushchego kafedroy - dotsent A.P. Mokhnenko)
Leningradskogo sanitarno-gigiyonicheekogo meditsinskogo instituta.

MLYKIN, A,.
Experience of technical propaganda. Prof.-tekh. abr. 14 no.2-~31 7 157.
(Nm 10.-W
1. Direktor toldmicheakogo uchillahcha so.1, Petrozavodsk.
(Petrozavodsk-Technical education)

YERIMAX-N.I.
Proteins in-the blo,6d serum of rabbits and dogs affected bY
plutonium. Radiobi6lo4iia 2 no.6:834-837 162 (14IRA 1611l)

SOV/120-59-1-32/50
AUTHORS:Goryunov, N. N., Yerlykin, A. D.
TITLE: An Ionisation Chamber for Cosmic Ray Studies (Ionizatsionnaya
kamera dlya issledovaniya kosmicheskikh.luchey)
PERIODICAL: Pribory i tekhnika eksperimenta, 1959, Nr 11 PP 130-131
(USSR)
ABSTRACT: A brief,description is given of an ionisation chamber with
a working volum& in the form of a cube. In order to calculate
the main parameters of the chamber it is necessary to know the
distribution of the electrical field within its working volume.
Since a mathematical solution of the problem is difficult the
field distribution was found by means of a model. The model
consists of a large number of points connocted with each other.,
each point being common to six identical ohmic resistances r
as shown in Fig 1. The working volume of the chamber is divi-
ded into 1000 cells which corresponds to 1000 model points. In
this way the field may be found with an accuracy of 10%. The
electric field is determined by voltmeter measurements of the
voltage at the various points. Having found the resistance
Card 1/3

SOV/120-59-1-32/50
An Ionisation Chamber for Cosmic Ray Studies
between two boundary surfaces of the model the capacitance
of the chamber may be found from the formula
C = - kr/4 V R
where R is the measured resistance and k is the scale
factor. The chambgr is shown in Fig 2. Its working volume
is 25 x 25 x 25 cO bounded by thin atainlona stool walla 1
The collecting electrode 2 is made of brass and is in the
form of a cylinder 1 cm, in diameter and 10 cm long, The
collecting electrode is introduced t1uou-h the ceramic insul-
ator 3 The chamber was filled with a mixture of 98% ar-
gon (spectroscopically pure) and 2% of nitrogen (teclmical)
at a pressure of 830 mm. H:;. . The effective volume of the cham-
ber is not less than 95% of the geometrical volume. The cap-
acitance of the chamber found by means of the above model was
Card 2/3

SOV/120-59-1-32/50
An Ionisation Chamber for Cosmic Ray Studies
found to be 2.4 pF. There are 2 figures and 3 Soviet rofpr-
ences, 1 of which is a translation from English.
ASSOCIATION: Nauchno-isoledovatellpkiy institut yadernoy fiziki MGU
(Scientific Research Institute for Nuclear Physics of the
. Moscow State University)
SUBMITTED: January 22, 1958.
Card 3/3

GORYUN(TV, N.1d,) YF.11:,'fK,IN, A.D.
Wide-range discrete time-delay pulse-height, converter, ?rib. i tekh.
eksp. 10 no.100-94 J&-F 165. (MRA 18:7)

1 21
3/152 60/002/000/003/027
73 19 k7g- 17 4 D299 1504
AUTHORS: Goryunov, N. N.9 Yerlykin, A. D.v Zatsepin, G, T., and
Kamnev, A. B.
TITLE; Study of cores of individual air showers
SOURCE: International Conference on Cosmic Radiation; Moscow,
1959. Trudy. v. 2. Shirokiye atmoefernyye 1Vni i kas-
kadnyye protsessy, 71-79
TEXT: The experimental setup is described; the results of the ex-
periments are given. The principal apparatus consists of a system
of ionization chambers which operated in conjunction with the com-
plex setup of Moscow State University (see article on P. 5p same
Trudy). The ionization chambers were disposed in two rOWB of 60,
respectively 64 chambers each. The large number of chambers made it
possible to obtain a continuous pattern of ionization distribution
in space. The lower row was shielded by a triple layer Pb-C-Pb.
The graphite layer acted like a converter of energy (of nuclearac-
tive particles into electron-photon energy). The energy fraction
Card 1/4

31 21
YE627/60/002/000/003/027
Study of cores ... D299 D304
imparted to-le-mesons was estimated; it Was found to be approxe
0.2 to 0.37. In processing the resultaq the main attention was de
voted to the case when the shower axis passed through the ioniza-
tion chamber system. According to cascade shower theory, the axis
of high-energy showers can be localized in a small region. It was
found that this holds also in practice. The position of the axis
was-d-6termined by two independent methods, without any discrepancy.
The showers recorded during a certain time interval were represen-
ted as a "point field", whose abscissas and ordinates give the to-
tal number of particles in the shower and the energy flux in the
core, respectively. In order to ascertain the relationship between
the number of particles N and the corresponding mean energy flux
E, the various points were averaged. It was found that for N =10
E = 104 relativistic particles. To one and.-the same intensity of
shower there corresponds a whole range of values E, whereby the
spread of the points increases with decreasing intensity of shower.
The character or the ionization distribution in the vicinity of the
shower core varies. In the majority of canon, the ahowor han an
Card 2/4 1-

s'P6'27/60/002/000/003/027
Study of cores D299/D304
elementary structure, i.e. the ionization density has one sharp
maximum. In some cases, a broadening of the core was observed;thus,
out of 39 showers with N 105, one third belong to complex-structure
showers. It was found that the ionization-denBity distribution can
be expressed (in the majority of cases) by a power law of type
P(r),_1/rn, up to r`_-"1.5 m and various n. The lateral distribution
function of the energy flux of the nuclearactive component was
constructed. The mean energy flux of the nuclearactive component
was found to be 4.6-103 rel. particles = 2.3-10 12 ev. This was com-
pared with the mean energy of the electron-photon component: 2.80
104 rel. particles = 2.8-10 12 ev. Integrating the lateral-distri-
bution function of high-energy nuclearactive particles over a ra-
dius of 2.5 m about the axis, it was found that such a circle con-
tains 0.9 particles with an energy >5-10 11 ev. (for showers with
N = 105).' Further, the energy spectra of nuclearactive particles
in the central regions of showers of various intensity were con-
Card 3/4

Study of cores ...
31521
S/62 YD 60/002/000/003/027
D299 304
sidered. Finallyo the observed energy flux of the electron-photon
component was compared with that calculated according to cascade
theory. It was found that the calculated energy-flux exceeded the
observed one 'by a factor of 3 (for r = 1.5 m), and by a factor of
8 (for r = 12 cm). There are 9 figures and 12 Soviet-bloc referen-
ces.
Card 4/4

r r i tek~,~a t-k~4~,r
vl;r" 1A)
a Ar,. (I f! n. a P h g ht ~4 d
T 'N Ski
Si ISR I K
g- t"n -th
-daAn and-Aisc n 0- f fres impter-a-var the firnifiktions
and suitable for operation with a pulse ionfisation chamber to suggested in
p?--R-nt artic-1-!. This symem has a tlynamic range of The error of pulse-

hip , Rht I #-I p r r~ii na t irm int i ')i* in t ti~ -A r 14 a n
t fn I A T I -T F' T I I
N( j R P

"5024654
Ijklm, AD
nFA I none
S0vWz 0=1 Vjt/0048/gS/02q/009/l73T/l75Q
TITLE t Energy loss by ultrarelativistic
ports AILl-UULOM conference on d0mic Ray-
SOUFCE:
!no in electromiagnG Ic interacti(OKS AS
lice held sm st 1964/
AN SSSR. Izvestiya. Seriya fizicheskayAt Y. 29# 10* 99 19631 1751-1160.
secondary cosmic rayt muout pair production, brmastrahluug
'TOPIC TAGS$
7as energy loss In earth (Z - 10, A a 20; z m 13, A a 26) and water of high
AMTRACT9 has been c&lcu-
tenergy (1010-1013 ey) nuons due to breosstrahlung am pair production "-(but not
lated nuserIIcally with "all the corrections thet *are now wall understood
##radiative- corrections or direct interactions with &tOm1c electrons) taken Into ac-
one of the corrections, that for the finite size of the nucleus aOd screening
count. some detail am It is shown that the best Val'
by the &tonic electrons# is discussed In R.r.Christy and SAU-
ue of this correction for Pb20S is 30 % less than that found by
oak& (Phys. Rev., 59,414 (1941)), Screening by &tonic electrons leads to considerable
energy dependence of the breanstrablung 1088; It Is suggested that differences In csl-
culating the screening effect may account for the discordance Of the vAlu" Of brems-
strablung loss that are found lathe literature. Taking proper account of high energy
1/2

L 4486.-66
A:~C* NR, AP5024654
pairs andipairs in which the electron.and the positron have greatly different energies
leads to considerably greater pair production enefty loss than has been proviou*ly as-
mumed. The energy loss d log Z/dx (3 to the muon energy and x in the depth in the ab-
sorber) of 1012 ey muons In water due to bremastrablung to 10-6 ca2/g, and that due to
pair production is 1.36 x 10-6 C02/g. Orig. art. beat 11 formulas, I figure, and-1
table.
BUD ODDZ: XP/ OMM DATEt 00/, ORIG art 002/ OVK Mrs 001
6D
-1-C'ard 2,
1

1ACC NRi AP603703& SOURCE CODE1' UR/0310/66/000/011/0029/0031
AUTHOR: Yerlykin I. (Deputy chief designer)
;ORG: T*K B for Hdyrofoils IsI66 ?a
Isudam na podvodnykri kryl 'yakh)
TITL'E: FundamentaL tren6 in designing hydrofoil river craft
Rechnoy transport, no. 11, 1966, 29-31
'TOPIC TAGS: hydrofoil, shipbuilding engineering, n
~ABSTRACT: Fundameptal trends in thei development of high-speed ships are discussed on i
ithe basis of recent design experience, in particular that relating to hydrofoils. j
iThe hydrofoils of phe "Raketa" and "Meteor" types and of the "Burevestnik" and "Beloruh,
;are discu'ssed in detail, and their vital statistics are given. Further developments
;foresee an increase in speed to around 60 km/hr by the use of aviation gas-turbines,
.water-jets, and half-submerged propellers. New projects also provide for 2000 hours of
Iservice without overhaul, the increased corrosion resistance of propellers, higher
strength of the hull, foils, and shafting, and improved measures against noise. Orig.
art. has: 6 figures and 2 tables,
SUB CODE: 13/ SU6 DATE: none L
I
rd 111 UDC: 629.124*9*040.001.2*

YERLYUN, Lyudvig Andreyevich; SHAROGORODSKIY, S.G., red.
[Practical advice to radio amateurs] Prakticheskie go-
vet7 radioliubiteliu. Moskva) Voenizdatp 1965. 239 p.
(MIRA 18:7)

SIRDTIRk, Galim Nikolayevna; T.VVTIII Irina Semenova; KALIKHMAN, L.Te.,
retsenzent; SOLODXIN, . .. r-e-Taktor; VINOGRAWVA. N.M.. redaktor
i2datel'stva; KaASNATA, A.K., tekhnichaski7 redaktor
[Book of problems in hydromechanics] Zadachnik po gidromekhanike.
Moskva, Izd;w*o *Rechnoi transport.0 1956. 132 p. (MLRA 9:10)
(Fluid mechanics-.Problems. exercises. etc.)

FlLIFFQV, Vladimir Grigorlyevich; YERLYKIII, L.A., red.
[Djaplacement digitizerml TSifratory paremeshchenii.
Moskva, Voonizdato 1965. 143 P. (MIRA 1814)

AUMIYEV, MikhailYakovIevich, prof,p doktor tekhn, naukj VEIN)NITSKIY,
1.0., r~tmenzent- YERLYKINA I S., red,; SIUMIKOVA, Z.V., red.
izd-va; BODRGVAyl-'F'~4~-
[Hydromechanies) Gidromekbanika. Izd.2.p perer, i dop. Moskva,
lzd-vo "Rechnoi transportp" 1961. 326 p. (MIRA l5t2)
(kdrau3ica)

DROMOV, levgonly Afannslyevich, kand. tekhri. nauk,, dots.j
pj4,OKjjOjlOV, Vadiv-, Ivanovich, kand. tekhn. nauko dots.;
FLATjyjjtATGV, Aleksandr Potrovi~:hj kand.telhn. r-auk,
dots.; YERLYKIII, L.A., rod.
0
tFundamentals of computer technology] Ostiovy vycllii3litel'-
noi tekhniki. lzd.2., parer. Moskva, Voenizdat, 1964.
463 p. (1,9RA 17:9)

suPRYAGA, N.P.; L.A..,,. inzh.-mVorp red.; MURASIIOVA,, L.A.,
tekhn. red.
(Continuous wave radar) Radiolokatsiia, s nepreryvnym
izlucheniem. Moskva, Voenizdato 1963. Ul p,
(MIRA 17:2)

I B.I.; yE:RLyKll;o L.A., inzh.-mayor, red.; SOKOLOVAp
YEVDOKIMOI'p G.F., tekh6.-re .a...
(Antitank rocket weapons] protivotankovoo reaktivnoe
oruzhie, Moskvaj Voenizdatj 1964. 91 p. (MM 17:2)

ZAYJWOVI yu.K.-. IjRLyKJN~ L.A., red.; 14EDNIKOVA, A.N.9 tekhn.
red.
(Transistorized voltage converters] Preobrazovateli na-
riazheniia na poluprovodnikovykh triodakh. 14oskval Voen-
p (MIRA 17:3)
izdato 1964. 3-01 P-

VMLMMA', N.Ye.; STEPAROV, 11-F-
Additivity,of thelf.-eleitron energy of condenfiRd arm&tic hYdrO-
carl=o calculated by the free electron methodo Mmr&ot*ktekIIim*
1, no.118,4-90 Ja-F 163. (MIRA 16 s2)
1, Mookovskiy gosudarstve=7y universitet imeni lomonosavas
(Hydrocarbaw) (Chemical structures)

i
AUTHORS: Diogenov, G. G.,.jerlykovt A. M. SOY/'150-58-3-3/52
TITLE: The Reciprocally Reversible System of the Acetates and Iodides
of Sodium and Potassium (Obratimo-vzaimnaya sistema iz atsetatov
i iodidov natriya i kaliya)
PERIODICAL: Nauchnyye doklady Yysshey shkoly, Khimiya i khimicheakaya
tekhnologiyal 19589 Nr 3# PP- 413 - 416 (USSR)
ABSTRACT: The reciprocal system Na, KJJCH COO# J was investigated by
3
the visual-polythermal method. (vizuallno-politermicheakim
metodom). Since the melting points of N&J and KJ are com-
paratively high, only that range of the system which is close
to the binary system CH 3COOK - CH 3COONa was in vestigated.
The authors investigated:The binary system CH 3COOI?a - Haj
(Table 1, Diagram 1). It has a eutectic point at 23 mole% N&J.
The sodium acetate has two polymorphous modifications with
the transformation point at 3260C. The binary system CH COOK -
KJ (Table 1, Diagram 1) was also investigated. It is anilogous
to the former system in many respects. Potassium acetate has
Card 1/3 two modifications, its point of transformation being at

The Reciprocally Reversible System of the Acetates SOY/156-58-3-3/52
and Iodides of Sodium and Potassium
2960C. The binary system CH COONa CH COOK (Table 2, Diagram 1)
3 3
and the binary system HaJ-XJ have been investigated by a
number of authors. The diagonal,cectione were also investigated
t)
below the temperature of decomposition of the acetates (3100
3800): CH3COON& - KJ (Table 1, Diagram 2A), CH 3COOK - NaJ
(Table 1' Dia ram 2A). In addition , 12 different sections were
investigated ~Tables 2,3 and 4f Diagrams 2B, 2C and 3).
Diagram 4 shows the projection of the liquidus system Na,
K 4CH 3COO, J to the ground square; the single sections are
discussed briefly. The eutectic point is at 22009 38,50%
CH3COO14a, 8% NaJ and 53,3% CH3 COOK. Another triple point is
a point'of passage (prokhodnaya tochka): 3010, 74% CH3COONa'
13% CH3COOK and 13% NaJ. There are 4 figures, 4 tables, and
7 references, ahich are Soviet.
Card 2131

The Reciprocally Haveroible System of the Acetates 30'f/156-58-3-3/52
and Iodides of Sodium and Potassium
ASSOCIATION: Wadra khimii Irkutskogo gornometallurgicheskogo
instituta (Unair of Chemistry of the Irkute) Hining'and
Metallurgical Institute
SUBMITTED: October 30, 1957
Card 3/3

ACC -_ NRi .- AR.60-18962 S.. OURGE C-OD 9: W/b27f/(,6/0!j.)/002/AO09-/,K669
AUTHOR: Tatkin, L. Z.; Yerlykov, IT. S.
TITLE: A multicircuit time delay relay using contactless alemento
SOURCE: Ref zh. Avtomat telemekh i vychisl tekhn, Abs. 2A59
REP SOURCE: Tr. N.-i. proyektno-konstrukt. in-ta tekhnol. mashinostr., no. 1, 1965,
44-51
-'TOPIC TAGS: time relay, delay circuit, electric relay
ABSTRACT: A tine delay relay using contactless circuits is described. It was devel-
oped at the MIT mash. The relay is capable of generating sequentially up to 25 time
delays from 1 sec-up to 16 hr. The time delay relay is based on the pulse counter
principle utilizing the MKO-LC ferrite-diode cells. The utilization of these cells
assures a maximum noise immunity under workshop operating conditions. The 50 cps
power frequency s6rves as a choke. The pulse counter counts down from. the preset
time interval corresponding to specific number of pulses. The desired time delay
is set up by means of switches. These are calibrated to read directly in seconds,
minutes, and hours facilitating easy manipulation. Tha relays have a relative error
of 0.5%. Tests have shown them to be highly reliable. (Translation of abstract)
7 illustrations and bibliography of 4 titles. T. R.
SUB CODE: 09
Card-ill UDC: 621.318.563.5

YZERLYKOV, S. 11.
"On the Determination of Temperature Stresses in Bridge
Spans of Steel Beams Joined to Reinforced Corcrete Plates." Cand
Tech Sci, Lqninprad Order of Lenin Inst of Railroad Transport
Ergi-neers im-ni Academici3n V. .1. Cbraztsov, 'Olin of Transportation
USSR, Leningrad, 1954. (KL., No 8. Feb 55)
SO: Sum. No. 631, 26 Aug 55-Survoy of Scientific and Technical
Dissertations Defended at USSR Higher Educational -Institutions
(l4)

CARAN'"IA,
),ntlbiogr&.-,i of -dysenter.'n ha~llli cri dat's of th,~ X'--azrnolar
TorrItc7ria'J. SariltarV 7:1!dealolcgl~-al StAtll3n-
rio,,5:465-4(-6 My (MIRA 18-.6)
1. KraAnoyarskly me-ILtainskly institut.

YERLYKOVA, K.L. (Krasnoyarsk)
Muskrats in captivity. Prirodm 54 no.8:125 Ag 165. (MIRA 18:8)

YERLYSHEY, P#A.q PodPolkovnik raed. sluz-hby
-
Treating lacrimation in pathology of the puncta lacrimalia. Voen.-med.
zhur. no.11:81 N '56. (NLRA 12: 1)
(LACRIYAL ORGAIM--DISMSRq)

YY.RLYSHBV, P.A. (Leningrnd)
Activntion of the upT)er Incrimal duct in nn irremediAble function
dinarder of the lower Incrimal duct. Vast.oft. 71 no.1:36-39
Jn-V 158. (MIRA 11:1)
(1ACRIMAL APPARATUS. din.
aurg. of upper duct in funct. dinord. of lower duct)

r- YERL-YSHEVP. P.A,
Use of elastic plastic sounds in.,atenosin of the lacrimal canals
and the nasolacrimal duct. Vest. oft. 74 no.2131-34 161.
(HIRA 34:4)
(IACRIML ORGANS.-DISZASES)
r