SCIENTIFIC ABSTRACT KOZHEVNIKOV, K. Y. - KOZHEVNIKOV, N. I.

• Document Type: CREST
• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R000825810005-2
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• Document Page Count: 95
• Document Creation Date: November 2, 2016
• Sequence Number: 5
• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT

BOROVSKIY, Vladimir Hikhaylovich; ABLAKOV, Enver Bekovich; KOZE1HVFIKQV,
__.LOAA& _R - n DAT-rl--'-
taAtA jq~RT!qj~~h; HMVLYAUSXIY, Konstanti yei vi eh;
BRZBOHOV, A.I., otv.rect.; ALEKSANMYSKIY, V.V., red.; SHIIVCHUK,
T.I., red.; ROROKINA, Z.P., tekhn.red.
[Ancient Syr-Darya Delta and the northern Kyzyl-Kam; possibi-
lities of soil improvement and problems of land reclamation]
Drevniaia del'ta Syr-Darli i Severnye Kyzyl-Kumy; pochvenno-
meliorativnye usloviia i problema sallskokhoziatstvennogo
oevoeniia. Alma-Ata, Izd-vo Akad.nauk Kazakhokoi SSR. Vol.2.
1959. 418 p. (MIRA 12:8)
1. Chlen-korrespondent Akademii nauk Ka2akhakoy SSR (for Bezoonov).
(Syr-Darya Delta--Soils) (Kyzyl-Kum--SOils)

KC011MUKOV, K.Ya.
Quick and simple mathod of determining the abborption capacity
of carbonaceous soils. Poclivovedenic no.2:100-102 F 160. (MIIji 15:7)
1. Vsesoyuznyy nauchno-issladovatellskiy institut vinodeliya i
vinogradarstva.
(Soil absorption)

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G'L~it!-LITZ DZPWRL~ -!I' i~ U JUL. -'ran:;. All I
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of fr,-,~rturinr. Thn. cliromit(i occur.- in stoc!r-lilz- i-.a:;ncz5, or
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-molacular difCuoion and convcction currnnta -st co3~dars of
igncou3 bodins; (2) liquation, form--~(L `,y Ul- ,~pnration o-C an or-a-u~-Jnf!ral
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KOZIIEVNIKOV, X.Ye.; KONONOVA, L.I.
Chromite bog iron ores of the Serov deposit and prospects
for their commercial use, Razved. i okh. nedr 26 no.7;1-6
ii 16o. (MIR& 15:7)
1. Urallskoye geologichaskoye upravleniye.
(Serov region-Iron ores)

KOZHEVNIKOV, K.Ye.; RABINOVIGHI S.D.
Northern Ural mankanese basin. Tt-udy Inst. met. UFAII SSSR no.7;
23-51 161. (MIRA 16:6)
(Ural MowAain5--Mnganoqe ores)

KOZHEVNIKOV, K.Te. --.
-------- - ------ I
------
Rhodonite deposit in the Central Urals. Trudy Gor.-geol. inst.
UYAN SSSR no. 35:291-296 160. (MIRA 14:1)
(Ural,gonataino--Rhodonite)

rWj.; FOYAE~01.1, M.A., ~3' red.;
TARK,11ANEYEV, B.F.. rej.
[Geology of Northern Srutzl-~a brovil coal basin. I Geclogi-i~'j
S-,:~vercso,,31viriAogo 'uo 'ria. Mot-,kva, IITF dr- a,
Urala,

KOZHEVNIKOV, L.
Artimliated six-wheeler for livestock transportation. Zhivotnovodetvo
20 no*4:79 AP '58. (MIRA 11:3)
(Domentic animals--Transportation)
(Truck trailers)

KOZHEVNIKOV, L. (g.Orel)
A lesson which profits no one. Sov.profsoiuzy 18 no.10:18-19
k7 162. (MLU 15.5)
(Orel-Socialist competition) (Orel-Trade unions)

KOZHEVEIKOV, M.
Coin counting machines. De*n.i kred, 19 no.5:56-63 Vq 161.
(M:RA -14:5)
(Counting devices) . "A-
(Banks and banking-;&REipment and supplies)

xCZIEVVuOV3 M.
The over-.&IJ mechanization of State Bankfs receiving and
disbursementIoperations. Den. i kred. 19 no.11:30-34 N I&,.
- (MIRA 14:12)
(Banks and banking-Equipment and supplies)
(Automation)

KOZBEVNnCOV, M. A. j
"Investigation of Parts Rejected on Ultrasonic Inspection," Forging, and Heat Treat-
ment, Moscow, Mshgiz, 1958. p. 123-
book prepared by membe-.e of 11TOwashprom in connection with 25th anniv.
Ural Heavy Machine-buildIng Plant Im S. Ordzhorilkidzo.

KOZHEVNIKOV, M.A.
Investigating parts rojocted followirko, ultrasonic inspection,
Sbor.st.UZTM no.5:121-129 '58. (141RA 11212)
(Matals-Defecto .) (Ultrasonic testing)

BAY-AZOVSKIY, Mikhail Yqkovlevich; BORODAYNT, D.A., kand.tekhn.nguk.
retsenzont; KOZH3VNIKOV, M.A., inzh., retsenzent; RAYKHKA11,
A.Z., inzh., red.; YERKAKOV, N.P., tekhn.red.
[Ultrasonic flaw detection] Ulltrazvukovaia defektoskopiia.
Moskva, Gos.nauchno-tekhn.izd-vo mashinoetroit.lit-ry, 1959.
149 p. (MIRA 13:2)
(Metals--DGfects)
(Ultrasonic waves--Industrial applications)

VASILIYEV, P.V.., prof#,, doktor ekon. nauk; POOMAREV, A.D.; SOLDATOV, A.G.,
kand. sellkhoz. nauk; MOTOVILOV, G.P.9 doktor sellk-hoz. nauk;
NEVZOROV, N.V., kand. ekon. nauk; IA)SITSKIY, K.B., kand. sellkhoz.
naukj RODIONOV, A.Ya., kand. sellkhoz. nauk: CHARKINA, A.P.., kand.
sellkhoz. nauk; LUTSEVICH, A.A., kand. sellkhoz. nauk;,UZffEITJMV-,
M.G dots,,- ALEKSEYEV, P.V., kand. vellkhoz. nauk; ZOR121, A.V...
-4is~~ra;~ ;BARAVOV, N.I., kand. sellkhoz.nauk (deceased], NATJM~O,
I.M., prof., doktor sellkhoz.,nauk; ILIIN, A.L. kand.sellkhoz. nimk;
MOISEYENKO,F.P.0 kand. biol. nauk; ZAKHAROV, V.K., prof., doktor sell-
khoz. nauk; GECHIS, Yu.P... starmhiy nauchnyy sotr.; BUTENAS, Yu.P.,
kand. sellkhoz. nauk; BUBLIS, X.A., aspirant; KAIRUPSH, A.Ye., kand.
sellkhoz. nauk; ZVIYEDRIS, A.I., kand. aellkhoz. nauk; SUKACHEV, V.N.,
akad. r,3d.; ZHUKOV, A.B.., prof., red.; PRAVDIN, L.F., prof., red.;
MAKAROVA, L.V.., red. izd-va; LOBANKOVA, R.Ye., tekhn. red.
[Problems of increasing forest productivity in four voluries] Pro-
blemy povyi3heniia produktivnosti lesev v chetyrekh tomakh. Moskva,
Goslesbumizdat. VoI.I+.[Economic probl'ems of increasing forest
productivity and accelerating ripening and cutting ages)Ekonomicheskie
voprosy povysheniia produktivnosti lesov, vozrasty spelosti i vozrasty
rubok. 1961. 253 P, (MIRA 15: 1)
1. Akalpmiya nauk SSSR. Institut less. 2. Nachallnik Glavnoy inspektaii
po lesuomu khozyaystvu i polezashchitnomu lesorazvedeniyu Ministerstva
sellskogo khozyaystva SSSR (for Ponomarev).
(Forests and forestry-Economic aspects)

KOZHEVNIK-,)V, M. m.
KI`/HEVNI_i0V,, M. M.: 111. P. Pavlov's teachings concerning associa-
tions, and their significance for the psychology of sensory per-
ceptions". Moscow, 1955. Moscow State Pedagogical Inst imen!
V. I. Lenin. (DisserLations for the Degree of Cand.'Ldate of Pedagogical
Sciences)
30; Knizhnaya letopis', No. 52, 2h December, 19~;5. Moscow.

KOMVNIKOV, M.11.
Some features of sensory association In visual perception [with
surmary in Hnglish]. Vop.psikhol. 4 no.6:131-139 N-D 158,
(HIRA 12:1)
1. Mizhaetagillskiy pedinstitut.
(Ferception)

ARZAMASTSEV, V.F., inzh.; K07,,HrVN1XOV,,-M..N., inzh.
Mechanization of plowshare hardening. Mekh. i avtom.proizv. 19
no.2zl9 F 165. (MIRA 18:3)

KOZHEVNIKOV Mikhail Petrovich! KHRYNIN, A., otv. red.; NADEZHDINA,A.,
WWWWWANOM" I Lzu- VK-j -IM14DUILIA, T.P takhn. red.,
(Machines for sorting and counting coins] Mashiny dlia. sorti-
rovki i peresehota monety; prakticheskoe posobie. Moskva,
Gosfinizdat, 1963. 70 p. (MIRA 16:9)
(Banks and banking--Equipment and supplies)

KOZEIRVNIKOV, M. P.
35173- 0 Drizhenit Vody Na Povorote Rusla. Izvestlya Vaesoyuz. Nauch.-Itiled.
In-Ta Gidrotekhniki Im. Vedenseva, T.ZL, 1949, *- 105-33
SO: Letopial Zhurhnltrvkh Statey. Vol. 48. goskva, 1949

'0 OV
M.P., starshiy nauchny7 sotrudnik. kandidat takhnichaskikh
' F
V M-P~
'-3~'A~'~nojxu ~.
Movement of water in the bond of a stream. Izv. VIIIIG no.40:
105-133 14q. (MR-k 10:2)
(Hydraulics)

XOZHF,VNIKOV, M.P
Principal problems of wave bydraulics and the selection of
motbod for tboir approximate solution. Nauch.-tekb.inform.
njul.LPI no.1/2:45-61 '58-
(HIRA 12:6)
(waves)

KOZHF,VIIIKDV, M.P., dotn., kand.tekbn.nauk
. - - - -- 1, -'Aj*r6x-lryAe method for determining motion characteristics of
potential waves. Nauch.dokl.vys.shkoly; stroi. no.2:235-241
~ 1 580 (MIRA 12:1)
(waves)

KOZHEVNIKOV, M. P., Doc Tech Sci -- (diss) "Approximate solutions of
so.,~e basic problems in wave hydraulics." Leningrad, 1960. 28 pp; (Min-
istry of Higher and Secondary Specialist Education RSFSR, Leningrad
Polytechnic Inst im M. I. Kalinin); 150 copies; price not given; (KL,
26-60, 133)

LEVI, Ivan Iv&noviohjKOZHEVMC,; M-P.p red.; ZHITNIKOVAp 0.8.9 tekhn, red,
[Model studies of hydraulic phencmenal Modelirovanie gidravlicheskikh
iavlenii. Mosk7a, Goo energ. izd-vo, 1960. 210 p. (MIRA 14:6)
6ydraulic models)

NEPOROZIUIIY, P.S.; I)nYAKOV, A.A.; VOZIfES121SKIY, A.N.; GIMOV, P.D.;
KACHANOVSKIY, B.D.; BASNICH, A.Z.; TARTAKOVSKIY, D.,m.;
VASILIYEV, P.I.; ZLRUBAYEV, N.V.; CIFJGAYEV,.R.R.; KOZHM.'IKOV,
M.P.:'2MOROZ, V.S.; IVANOV, P.L.; SHCHAVELEY, D.S., OXMCZOV~-
BELOV,-A.V.; STAROSTIN, S.M.; YAGN, Yu.I.; IZBAS'll, S.V.
Ivan Ivanovich Levi; on his 60th birthday. ~,idr. stroi. 30
no.9:61-62 B 160. (MIRA 13:9)
(Levi, Ivan Ivanovich, 1900-)

KOZIMVNNOVI H. P.
Approximate solutions of some fundamental problems in wave hydrau-
lics. Trudy LPI no.208:29-74 16o. (MIRL 13:9)
(Waves)

CHERTOUSOVY Mikhail Dmitriyevich, 2&s1. dayatell nauki I tekhnW RSFSR,
prof., doktor takhn. nauk[deceasedj;,KOZHMW-V
prof.,
doktor tekhn. nauk, red.; YAKGVLEV, 'T.A., starahiy prepod., kand.
tekhn. nauk, red.; ASTAFICHEVA, T.N., dote., kand. tekhn. nauk, red.;
KOSYAKOVA, G.N., dote., kand. tekhn. nauk, red.; MOZHEVITINOV, A.L.,
prof., red.; ZHITNIKOVA, O.S., tekhn. red.
(Hydraillics]GI.dravlika, spetsiallnyi kurs. Izd.4., ispr. Moskva,
Cosenergoizdat, 1962. 629 p. (MIRA 16:1)
1. Kafedra gidravliki Leningraskogo politekhnicheskago instituta
(for Koshevnikov, Yakovev, Astaficheva, Kosyakova).
(Hydraulics)

ACC NRi AR6030396 SOURCE CODE: UR/0124/66/000/006/bO68AGG9
AU?HOR: . Kozhev-nikov, M. P.
TITIZ:' Wave pressure on a vertical wall
SOU-A~ZZ: Mekhanika, Abs. 6B471
Ref. zh.
RZF SOURRCE: -Tr. kourdinats. soveshchaniy po gidrotekhn. vyp. 20, 1965, 98-102
,TOPIC TAGS: wave Dhenomenetraveling wave, standing wave
-AMXLI%TIG.N: Various methods adapted to engineering practice are set forth for -the
,study of wave phenomena and a brief description of the advantages and disadvantages of
.each of them is given. Special. emphasis is given to investigations in the field of
iwave motion in a liquid which were carried out by the author using the elect-rohydrody-
!namic analog method., This research allows one to obtain profiles of traveling waves,
Iwave propa7,_,',:.~.o'a vates, the trajecto.ries and Velocities of liquid particles in the
;wave,.and wave pressure, to calculate the energy transferred by the waves, and to de-
ivelon a me-ans for determining the deformation of the wave on a sloping bottom surface
;of -C*h6 liqu-i(I. Expe:~,izental data on traveling waves are obtained for 19 waves; in
!particular, fields of -wave pressure are constructed for each of them, permitting the
force or wave pressure on a verttical wall of any length to :je determined. Ap?roxima-
e to
1~ion fornulas are given to detemine the greatest and least wave pressure relativ

iACC NR. AR603035-3
:tIhe water level. Results of this research were used to determine the force of wave
!p2~essure on a wave-protection wall on ship elevator of the Krasroyarsk Hydroelec-
Jtric, Plant. it is indicated that it is possible to apply the electric-hydraulic ana-
l
1log method to on traveling and standing waves which approach a vertical wall
I
lobliquely. V.. Ye. Pyatetskiy.
SUB CODE: 20
':-Ccrd--2

MALYUGA, V., inzh.;.KOZ INIKOV, N., inzh.; KOGAN, V., inzh.
Lightweight exterior elements using plastic. Prom.stroi.i
inzh.soor. 4 no.5232-38 S-0 162. (MIRA 1631)
(Plastics) ' (Building materials)

KOZH19VNIKOVP N*I-# inzhaner.
~7 -I., -, . - .-,. .-- j.- :--`~ ~ . ~
Economize on the power resources in petroleum refineries. Prom, aierg,
12 no-3:1-4 Mr 157. (KLRA 10:4)
(Electric power)

F-OZLIEVNIKOV, N.I.; RIZOV, Ye-F-
1~ ~ .1 . I , - - r ~- nh.
i-Min:t,~qlp the in Strunitntal ()f -i diffrrl--l i~n '~!;' - ,
D-, t 0 ' * - .
1-:2)
Soob.GAISH no.12601-43 63. rt- I

KOMEVNIE01," :,LOC-ij,r~vIcl~;
- fir. EVA,A.V.,r
1 G, AT
111KO. .
10 ["0 Z01"'t I Y
YI d
[Fourier series and the Fourier i-
Analytic and special functions. Laplace transtoriml,.0711
aiady j integra:L Fu--'e. Tlearila r-olia. '.naIiI-ichP--iki 1
.1 .
spetsinl1riye
1: 19 64 . 183 1). Z , I I 14'. 1

KOZHHVNIKO
=1a
-001-010,
Docroase in brightness of the solar disk from the center to the
linba obaorveft in spectrum region from I to 4A [with summary
in &glishl. Astron. zhur. 34 no.6:883-686 N-.D 157. (MIRA 11tZ)
1. Gomidaretvannyy astronomichoskiy- institut Im. P.K. Shternberga.
(Spectrum,8olar) (Solar radiation)

KOZHEVVIKOV, N. 1. , Cand Phys--Math Sci -- (dies) "Study of tho law of
variation of luminosity of the solar disk from the center to the edge
A
Q~r the infrared region of the spectrum." Moo, 1958. 5 pp (laos State
Univ im M. V. Lomonosov, State Astronomical Inat im P. K. Shternberg),
100 copies (KL, 16-58P 116)
-.6-

24(7)
AUTHOR: Kozhevnikov, N.I. SOV/55-'38-3-8/30
TITLE% Investigation of the Representation of the Spectral Lines in
Dependence of the Illumination of the Entrance Slit and of the
Prism of the Spectrograph (Issledovaniye izobrazheniya
spek%11ra11nykh liniy v zavisimosti ot usloviy osveshchaniya
vkhodnoy shcheli i prizmy spektrografa)
PERIODICALs Vestnik Moskovekogo universiteta,Seriya man-~metikJ., me-_kltian-ik~_n
astronordi., fiziki, khirdi 1958,Nr 3,pp 51-64 (US;3R)
ABSTRAM The paper consists of tvo sections. In the first one the
author investigates how t-he illumination of the prism of a
spectrograph has to be so that the diffraction of light at
the envelopment of the priam influences as little as possib!F-
the representation of the spectral line. In the experimental
arrangement of the author numerous eXperimental observations
of the green mercury linsi A - 5460 gave the following re-
sult : The diffraction is minimum, if the slit of the speotro-
graph is illuminated by a parallel light beam and Jif the gap
width- is normal. In the second se-,tion it is nnmerically irx-.
vestigated whether in front of the prism (or objective or
Card 1/2 slit) one can establiah a diaphragm so that the diffraction

Investigation of the Representation of the Spectral SOV/55-58-3-8/30
Lines in Dependence of the Illumination ef the Entrance Slit and of the
Prism of the Spectrograph
on the slit is decreased if parallel light falls upon the
prism. By extensive calculation it is pro-red that neither an
amplitude - nor a phase diaphragm can cause a diminution of
the diffraction a oertaj.n~ mathematically precisely
defined sense).
There are 4 figures, 13 photos, and 8 references, 3 of which
are Soviet, 2 American- I French, -1 German, and 1 Austral-lan.
ASSOCIATIONt Kafedra astrofiziki (Chair of Astrophysicti of the
-0~1 I
State Astronomical Inatituta imeni P.K. Shternberg)
SUBMITTEDt February 21, 1958
Card 2/2

7(6)
AUTHOR: Kozhevniko SOV/155-58-3-27/37
TITLE- Observation of the Turbulence of the Lowest Atmospheric Layer
(Nablyudeniye turbulentsii prizemnogo sloya atmosfery)
PERIODICAL: Nauchnyye doklady vysshey shkoly. Fiziko-matematicheskiye nauki,
1958, 1Tr 3, pp 143-151 (USSR)
A13STRACT: The author describes the method of the direct observation of the
lowest atmospheric layer at daylight elaborated in the Soviet
Union in 1955-1956, as well as the principal results obtained
with this method. The method consists in the introduction of a
narrow aperture (at most 0-5 mm) in the focus of the objective,
whereby a filtration of parallel bundles of rays is possible so
thaton th 'e projection screen there appears an image of the
considered inhomogeneity similar to the original. The sun
telescope of the Astrophysical Observatory in Kuchino (near
Moscow), the sun telescope of the Astronomical Institute imeni
P.K.Shternberg on the Lenin Hills near Moscow and other
Card 1/2

observation of the Turbulence of the Lowest SOV/155-58-211-27/37
Atmospheric Layer
telescopes were used for the experiments. The obtained data
about the magnitude and motion of the inhomogeneities agree with
the observations of Protheroe _FRef 42
There are 6 figures, and 4 American ref;rences.
ASSOCIATION:Moskovskiy gosudarstvennyy universitet imeni M.V.Lomonosova
(Moscow state University imeni M.V.Lomonosov)
SUBMITTED: April 22, 1958
Card 2/2

AUTHOR: Kozhevnikov, 310V/55-58-4-3/31
TITLE- On the Connection Between the Energy Flux Through the Objective
of the Collimator and the Width of the Entrance Slit of the
Spectrograph (0 zavisimosti mezhdu -,r:!.-,J.cY-.-.ioy potoka energii
cherez ob"yektiv kollimatora i ahirinoy vkhodnoy shcheli
spektrografa)
PERIODICAL; Vestnik Moskovskogo universiteta, Seriya me~i~,, 4-ki, astrano-
71'
1
1958
Nr 4
pp 27-36 (USSR)
.
,
,
,
ABSTRACT: For the ratio kf(b) of the sets of energy passing through the
lens aperture of the collimator and the entrance slit of the
spe-trograph, the author obtains a very complicated closed
expressi6n (b - apertural width). A numerical evaluation yields
a curve ascending from the zero point at first very steeply,
then it has a sharp break, and then, slowly vibrating it
approximates asymptotically a straight line parallel to the
b-axis. Consequently the diffraction correctien for a bc-oad slit
Is essentially less than for a narrow one.
There are 5 figures, and 4 references, 2 of which are Soviet,
I American, and I German,
ASSOCIATION:Kafedra astrofiziki GAISh (Chair of Astrophysics at the
Card 1/2

On the Connectlia-ri Batween the Energy Flux Through SOV55-58-4-3/31
the Objective of the CcUimator and the Width of
theEntrance Slit of the Spectrograph
T ;'t, *m~v. v:' P *
":.a 1 -6 - - imeni P.K.Sh-terrbarg)
STIPMITTED- February 21, '1958
Card 2/2

!;,(;Vt ~;.!.
- I , - :,.-I
I lation of v-'!-nAt-l,:.,, in 1 01 1 - -
Gi-i.ph X ca Lcu - ".: s. -.,
zhur. 3L r-o. 1:177-1,1,1 Ja-F 161. C I'L"J"t 14:2)
1. GGojvt:c.rstvewi,,ry L-II-c'-, '., *-,, ?."...
I -*n--t-rL---,:z-.t~i'/

KO;q"jKQ-v,--v.I.; MAKAROVA" Ye-AO
Limits of the applicability of Bouguerla method for determizlizig the
intensity of light from p celestial sources Astron.zhur. 38 noJ:
536-540 Yq-.Te 161" - (Kak 14t6)
1, Gosudarstvennyy astronomicheakiy institut imeni P.K.Shternberga.
(Stars-R.adiation) ~

AUTHORS: !~ozhevnik Makarova, Ye. A.
- L0_VIjL__I
41289
S/035/62/000/010/045/128
A001/A101
TIME: Determination of extra-atmospheric values of silicon photo-cell
yield. PartI.The method of determining absolute sensitivity, in-
vestigation of relative spectral sensitivity of photo-cells
PERIODICAL: Referativnyy zhurnal, Astronomiya i Geodeziya, no. 10, 1562, 58,
abstract IOA402 ("Soobshch. Gos. astron. in-ta im. P. K. Shtern-
berga", 1961, no. 116, 3 - 24)
TEXT: Efficiency of silicon photo-cells considerably depends on external
conditions (temperature, level and spectral range of irradiation) and is also
determined by parameters of a circuit connecteci. The absolute spectral sensiti-
vity is defined as eX. = WX /E~,, where EX is spectral density of energy inci-
dent on the photo-cell, and W,\ is energy yield into the photo-cell external cir-
cuit. The method of irradiation with the Ynown irradiative capacity (ribbon
tube) was'employed for determining EX . The relative spectral sensitivity is de-
fined as.
Card 1/3 eA = e,\ /e~, 0 W

Determination of extra-atmospheric values of...
hence one obtains
\' 2 2
e)~. 0 W;~' d~
SAO _35/62/000/0 10/045/128
ACOI/AlOl
eX- E~ d-,\ (2)
If one kno,.-ir, e,~O, the absolute spectral sensitivity can be determined for any",
by.Formula (1). To employ Formula (2), one has to know the relative spectral
sensitivity. The latter was determined from the known curve of-spectral distri-
bution of the source energy. The e Al magnitude was determined from the Sun.
G. F. Sitnik's compensation circuit (RZhAstr, 1957, no 3, 1909) was used in de-
termination of the relative spectral sensitivity. Electrical and optical meas-
urement circuits are described in detail. Comparative studies of time permanence
of silicon photo-cell yield have shown that sulfur-silver photocells are some-
what stabler than silicon ones. Directivity diagrams of energy distribution in
the light beam reflected from the photo-cell are presented, The full intensity
Card 2/3

S/035/62/000/010/045/128
Determination of extra-atmospheric values of ... A001A101
of reflecte~i light amounted to 3 - 4% of the incident beam. There are 8 refer-
ences.
Ye. Antropov
[Abstracr,er's note: Complete translation]
Card 3/3

41290
S/035/62/ooo/olO/046/128
A001/A101
AUTHOR3 Makarova, Ye. A., Kozhevnikov, N,,I-, Porfir'yeva, G. A.
TITLE: Determination of extra-atmospheric values of silicon photo-cell
yield. Part II. Observations and results
PERIODICAL: Referativnyy zhurnal, Astronomiya i Geodeziya, no. 10, 1962, 58-59,
abstract 1OA403 ("Soobshch. Gos. astron. in-ta im. P. K.'Shtern-
berga 1961, no. 116, 25 - 4.5)
TEXT: The method described in Part I of the article of the same title
(abstract 1OA402) was applied to t~etermination of the absolute spectral sen-
sitivity of a group of photo-cells. Making use of the experimental linear
growth of power obtained from the optimum load.of 'a photo-cell (depending on
light intensity), the authors calculated extra-atmospheric values of photo-*
. 2
-cell yield by extrapolation of obsei~ved values. It amounts to 4.5 - 9.7 11W cm
.There are 9 references.
Ye. A.
[Abstracter's note: Complete translation]
Card 1/1

KOZHEVNIKOV., N.I.
Methods for determining the efficiency of photoelectric cells;
comments. Soob*GAISH no,U6:46-54 161. (KUU, 14:8)
(Photoelectric cello-Testing)

s/623/61/000/117/001/002
P- tj E032/E114
AUTHOR: Kozhevnikov, N.I.
TITIL: The scattering of light in the earth's atmosphere and:
its effect on the apparent luminosity and details on
the solar disc
SOURCEi Moscow. Universitet. Gosudarstvennyy astro'nomicheskjLy:.
institut. Soobshcheniya. no.117. 1961. 3-14
TEXT: V.Ye.~Stepanov (Soobshch. GAISh, no.100, 1957) ha B
shown that the observed optical thickness of the earth's
atmosphere is- different for different points on the solar disc,
The present author reports an analysis of'this problem, starting
with the general equation for the transport of radiation in the
atmosphere, taking into account scattering and absorption. I
Formulae are derived for the ratio of the luminance of any two
points on tho surface of the disc in terms of the observed Js
luminance. These formulte are found to be in agreement with the
results of Stepanov and '.hose of T.V. Krat (AZh, v.25, no-5, 1948)-
The analysis may be used to compute the correction for scatteringi.
6. It is shown further 'G-hat the correction may change sign and
Card 1/2

The scattering of light in the earthts.. S/623/61/000/117/001/002
E032/E114
therefore may be zero for certain luminosity ratios.
There are 2 figures and I table.
Card 2/2

4
S/035/62/000/C,10/025/le8
r A001/A101
AUTHORS: Kornilov, A. I., Kozhevnikov, N. I.
TITLE,; Polarization of radiation and instrumental contour of a spec-
trograph
PERIODICAL: Referativnyy zhurnal, Astronomiya I Geadeziya, no. lo, 1962, 46,
abstract 10A335 ("Soobshch. Gos. astron. in-ta imeni P. k. Shtern-
berga", 1961, no. 117, 15 - 20)
TEXT: The authors consider theoretically the profile of a diffraction
image of the spectral line; in summation of oscillations in the focal plane
of the spectrograph, not only phases but also polarization'of oscillations
of light are taken into account. Incident light is assumed to be plane-polar-
ized, parallel and perpendicular to the spectrograph slit. Diffraction is cbn-
sidered only on the diaphragm of the prism or the grating. The calculation re-
.sults are presented in graphs showing distribution of amplitude and intensity
as a function of diffraction angle for aperture ratios of the spectr,ograph
0.75 - 0;0; this dependence proves to be insignificant. Since the amplitudes
Card 1/2

S/035/62/000/010/025/128
Polarization of radiation and... AGO1/A1O1
of polhrized components coincide for small aperture ratios, the authors con-
clude that, In experimental determination of a diffraction profile of the
slit image, differentiating of light bundles with different polarization is
not necessary. A necessity in separation may arise only in cases of sp.!ctro-
graph cameras with aperture ratio:p,:,l. There are 5 references.
Ye. Makarova
[Abstracter's note: Complete translation]
Card 212

Ss/iu~62/000/004/002/010
B108/B102
Kozhevnikov, N. 1.
Ontica-I Pyamination of the structure of air streams in
at;t,,oziphc-ric strata near the surface
F E R i 0 DIN,, L o -, c o,,-., .Universitet. Vestnik. Seriya i'Ll. Fizika,
astronomiya, no. 4, 1962,14 - 17
TEXT: in a previous,paper (NDVSh, no. 3, 143, 1958) the author had
described a method of observing turbulences in the atmosphere by daylight.
M.,e direct sunli-ht is screened out after focusing, so that only those
that are refracted on air inhomogeneitios are projected to a screen.
rays
Gbs-~,rvations usinZ this method showed that atmospheric inhomog-eneities
16~.emz~eives are also inhomogeneous. There are 4 fiCures.
.k ~ 'TI'll,"; Kafedraastroliziki (Department of Astrophysics
3 ~O C IA ~ A.
SUB~,,IITTE'D: September 25, 1961
Card 1/1

3/17C)/62/C,05/'009/003/01(,
B106/B104
A UTIIC6S: Latyshev, L. A. , ;-,ozhevnik,ov, N. I.
T I T I -P oI the, tomj;erature fiAds ir, t. e of
bounded ..,ollo-,-., cylindor for non-unifor:r, boi;ndary conditions
zhurnal, v. 5, 1,:).
T:",~ T.- ii tao rs t ud ica -,e cm
perature field of a bounded tube
th,~ tube to its nurrou,idin6 is not uniforTi along&C
.Iie tuU~. This problem involves solving a boundary value problem of the
1,~'-'Iuce! equation
OT X (a2T +a2T + I aT
ar' ae r Or
.-it bolu-,dary conditions

6/1 70/62/uj5/,)09/()03,/C)l 0
C,lcul.-Lion of
B1 ()S/ B1 011
Z=O if z=H, aT =0,
az
OT
r a, h,(T- T,) - 00i 1,2 ,
b, aT c q
dr k
initial condition..-, T= 0, f T (1,,z~ ~nd cond-itioi,,.s o1. 1,;.,? tll
T (a, z 0,,t) - T (a, z+
aT (a, z- 0,,r) aT (a,z +0,-C)
Y - . Y
az az
It is sham that for a ,,'iven f low of :ieat as a.7 lor heat tran~;ft-.r
i Len~~iLy Oiu solutiui~ is obtainw! b~j .iuj~erj~ooin,, "lolution of A
s~-!tionary proble.,-, ivitn, nor.-uniforz, boundary condirior,.-. .nd on of
.4rd
I I

:5/170/62/005/009/003/010
calcula4ion of thc~ tompfirature fields ... B108/B1011
111 -a --, 2.onary )roblt~-., ~;-Jti-, unifor:r~ boundary conditions.
-rl ~ w(r,z) t The re3ulting analytical expxes~;ions are
,;~-11 for uce in numerical computation.
IAT1 Lja'i~ .Iviatsionnyy institut imeni Sergo Ordz,lonikid--e, g. fdoskv4-
(i',viation In8titute imeni Sergo ordzlionirkidze,
~i3-1- TTE'-') july 6, 196i
Card

43927
S11861621000100610141016
B125/BIO4
AUTHORSt Kozhevnikov, N. I., Makarova, Ye. A., Sitnikt G. F.
TITLEi Absorption of solar radiation by water vapor as observed at
various altitudes
PERIODICALt Moscow. Universitet. Vpstnik. Seriya III. FJ.zika, astro-
nomiya, no. 6, 1962, 75 -- 79 -
TEXT: It is reported that the calibration curves for the Earth bands of
water vapor and oxygen in the solar spectrum differ the considerablylym the
curves "of -; F. E. Fowle (Smithson. Ann. , 5, 171, 1913; 3, 182, 1913). These
calibration curves were recorded by the authors at the Kuchinskaya astro-1
fizicheskaya observatoriya (Kuchin Astrop~ysical Observatory) and in the
1&okogornaya stantsiya GAISh (High Mountain Station GAISh) at Alma Ata
during the International Geophysical Year. The difference can hardly be
due to inaccurate determination of the line in the continuous upectrum.
The zero line was found precisely both by Fowle-and by the present authors.
Also the light scattered in the spectrograph was correctly considered in
both cases. In the authors' opinion,' their calibration curve correctly
Card 112

5/188/62/000/006/014/016
Absorption of solar ... B125/B104
represents the features of the absorption of radiation by water vapor.
Fowle's curve, which was plotted under laboratoty'conditions tit 760 mm Hg,
is suitable only for observhfions at low altitudes (plane) and not for
those at altitudes exceeding' 2 - 5 km. There a~e'5 figures.
ASSOCIATIONi Kafedra astrofiziki (Department of Astrophysics)
SUBMITTEDs April 12, 1962
rard 2/2

4r- KqWvul KOVj__N.I.-
Optical method for studying the structures of air flows in
the sitrface layers of the atmosphere. Vest. Mosk.un.Ser.3:
Fiz,,astron. 17 no-4,.14-3.7 ji-Ag 62. WIRA 15:9)
1. Kafedra astrofiziki Moskovskogo unJversiteta.
(Meteorological optics)
(Air flows)

h5165
3/188/63/000/001/009/014
B164/B102
AUTHORS: Kozhevnikov, N. I., Makarova, Ye. A., Sitnik, G. F.
TITLE: Model of the water vapor infrared absorption band
PERIODICAL: Moscow. Universitet. Vestnik. Seriya 111.
astronomiya, no. 1, 1963, 54-61
=,(T. Theoretical models of band absorption are discussed in order to
interpret the 1R absorption in the 1.12 p band by atmospheric water vapor
(GAISh no. 126, 1962;*VMF no. 6, 1962). The measuremen-to were made with
the OKC-11 (IYS-11) spectrograph of the Kuchinskaya astrofizicheskaya
observatoriya (Yuchino Astrophysical Obseryatory) and at the Vysokogornaya
stantsiya GAISh (Ifieh-mountain Station GAISh) near Alma Ata. The.
experimental relationship between the residual radiation intensity in the
1.12 A band existing after the absorption and the amount of absorbing
wa-,er vapor is compared with the theoretical results. The agreement with
the model of R. M. Goody (Quart. J. Roy. Meteorol. Soc. 78, 165, 1952) is~'
fairly good. The authors calculate the absorption in water vapor on the
assumption that the lines in the absorption band have different intensitle-8--
Card 1/2

,nodel of the water vapor ...
S/168/63/000/001/009/014
B164/B102
and are at different distances from each other. These results show that
the absorption coefficient is not constant within the band, so that the
amount of absorption measured depends on that section of the band chosen
for the investigation. This was confirmed experimentally. A modified
formula according to Goody for the residual intensity observed is given
by averaZing the absorption in the frequency interval of the band
considered. The exl)er~mental results are Idiscussed'on the basis of this
formula. They are found to be in satisfactory agreement. There are
5 figures and 2 tables.
ASSOCIATIGN: Kafedra astrofiziki (Department'of Astrophysics)
SUBN'LITTED: IMay 11 , 1962
Card 2/2

KORNILOV, A. I.; KOZIMTKOV tL. I.
Polarization of radiation and image contour of a apectropaph.
Soob. GAISH no.117tl5-20 161. (MIRA 15:10)
(spectrograph) (Polarization(Light))

IMHEVNIKOY,-H,T.., MMMVA, Ye.A.; SITNIK, G.F.
Absqrption of solar radiation by water vapor accoring to obaer-
vations conduoted at different altitudes. Test.Mosk.un. Ser.3:
Flz..,astron. 17 no.6173-79 N-D 162. (MIRA 15--12)
1. Kafedra astrofiziki Mbskovskogo universiteta.
(Solar radiation-Obser7ations) (Water vapor)

KLYAKOTKO, M.A.; KOZIIEVIIIKOV, N.I.
Character of large-scale motions in the solar photospher,3,.
Astron.zhur. 39 no.6:981-986 11-D 162. (MIRA 15:11)
1. Gosudarstvennyy astronomicheskiy institut im.
P.K. Shte.-nberea.
(Sun)

ACCESSION NRt AP300'1774 S/0186/63/000/00~/006610069
AUTHOR: KozhevaLkov, N. 1,~
TITLE: On the question of fluctuations of the index of iefractLon of..
li*ght waves in the surface layers of the atmosphere
SOURCE: Moscow. UniveraLtet. VestnLk. Seriya 3. Fizika astronamiya,
nos.3, 1963, 66-69
TOPIC TAGS: atmospheric op~Lcs, refraction, light wave,, Lnhomogenet~y,
atmospheric turbulence, refraction index
ABSTRACT: The structural function of the fluctuation of the index of
refraction in the surface layers of the atmosphere has been determined
by a method of direct observation. Two Kolmogorov-Obukhov functional
relationships, based on the theory of isotropic turbulence, are em-
pl'oyed to determine the distribution of the structural function of
the index of refraction and the least mean.dLatance between two
regions in space:
Card 1/3

ACCESSION NR: 'AP3001774
D 2 cn2 13
n(*F19 '2) In (~I) _n ('2
Dn(Flord n(~,)-n(F,)2 1'2'~rlj,
where Dn(Fj,T
he 2) Is the structural function of the index of refraction,
nR) is t value of the index of refraction at point Y, Cn is a con-
ritant&L is the-outer scale of turbulence, and 10 is the inner scale
of turbulence. The optical system used to observe the fluctuatLon's of
the index of*refraction Ls'~~shown diagrammatically. The inhomogenalties
are divided into 2 groups: 1) thosewLth a mean size oflu2.5 cm, and
11) those with a mean size ofov9-10 cm. The mean distance between-in-
homogeneities is plotted as a function of the magnitude of fluctuation
of,the index of refraction for both groups. The Index for group I is
seen to be near unity, while that for group 11 exceeds unity. A liiie.ar
dard .2

ACCESSION NRi AP3001774
relationship exists between the mean distance between inhomogeneities
and the magnitude of fluctuation of the index of refraction for group 1.
It is concluded that% 1) the Kolmogorov-Obukhov law is fulfilled for
the'observed fluctuations of the index of'stmospheric refraction,and
2) for the inner scale of turbulence 10 42.5 cm. Orig. art. hast 4
figiires and 4 formulas.
ASSOCIATION; Kafedra astrofiziki MGU (Department of Astrophysics. MCU)
SUBMITTED: 020ct62 DATE ACQ: 09Jul63 ENCL: 00
SUB CODE: AS NO REF SOV: 006 OTHER: 000
Card 3/3

ACCESSION KR: AT4035360 9/2623/63/000/126/0003/0024
AUTHOR: Makarova, Ya. A.; Sitnik, G. F.; Kochevnikov, N. I.
TITLE: Some of the optical propertiee of the earth's atmosphere and the water
vapor content revealed by observations at Kuchino and during the alpine
expedition of the State Astronomical Institute (GAISh)
SOURCE: Moscow. Universitet. Gosudarstvenny*y astronomicheakiy inGtEtut,
Soobshcheniya, no. 126, 1963, 3-24
TOPIC TAGS: astronomy, astroclimate, atmospheric optics, atmospheric water vapor
content, atmospheric transparency, meteorology
ABSTRACT: The spectrophotometric method was used to determine the water vapor
content in the earth's atmosphere at different H20 bands from 0.94 to 1.47/A
with an accuracy of about 57.. The observations were calibrated against:
aerological data. The calibration curves constructed on the basis of observa-
tions at the alpine station and at the Kuchinskaya astrofizicheskaya laboratoriya
GAISh (Kuchino Astrophysical Observatory) provide quite reliable data on the
water vapor content in the earth's atmosphere. It is concluded that anrological
ascents are suitable for the calibration of spectroscopic observations,.
Card 1/3

ACCESSION NR: AT4035360
Comparison with approximate calibration in the laboratory reveals a systematic
discrepancy, but this only suggests that laboratory experiments must take into
account the change in meteorological factors with height in the atmosphere. The
water vapor content in the atmosphere is th.ree times less In summer and five
times less in winter at the alpine station than over Kuchino (in sumier). The
water vapor content over the alpine station in summer changes approximately by
a factor of two during the day from morning to noon as a result of melting of snow
in the nearby mountains. At Kuchino, on a plain, there is no particular change
during the day. An increase in the water vapor content toward noon near the al-
pine station leads to a decrease in the atmospheric transparency coefficient.
Since the increase in water vapor content occurs gradually, the Bouguer curve,
which is usually used to determine the transparency coefficient, will remain a
straight line for the most part but the transparency coefficient computed Zrom
this curve will be erroneous. This error increases with a decrease of wavelength
and with an increase of the water vapor content of the atmosphere. With an
increase of water vapor there is an increase of the solar aureole and an increase
of the deformation of images. Similar phenomena caused by the summer melting of
vnow should be observed at other mountain observatories. In winter, when there
ie a continuous snow cover, there ie no diurnal variation of water vapor content
Card 2/3

ACCESSION NR: AT4035360
and the aureoles caused by light scattering on water vapor particles are small.
The water vapor content in the atmosphere in winter is only one-half or one-
third as great as in summer. "In conclusion, the authors wish to thank A. 1.
Kiryukhina, M. S. Murashava and R. N. Kluneleva, specialists of thu Otdel fiziki
SoInt6a GAISh (Division of Solar Plkysics of the State Astronomical Institute),
for assistance in making the observations and in processing the data". Orig.
art. has: 3 formulas, 11 figures and 5 tables.
ASSOCIATION: Gosudarstvenny*y astronomicheskiy institut Mookovskogo univeraiteta
(State Astronomical Institute, Moscow University)
SUBMITTED: 00 DATE ACQ: 25May64 ENCL: 00
SUB CODE: AA, 99 NO REF SOV: 005 U1118R.- 005
Cord 3/3

KOMMIKOVI N.I.
Some peculiaritias of the image of A speettal line in case af an illumi-
nation of the input slit of a spectrograph with a parallel light beam.
Soob.GAISH no.126s25-30 163. (MIRA 17t2)

KOZHEVNIKOV N.I.; MAKAROVA, Ye.A; SITNIK. G,F.
, ~ - , -1 ? i,, -- , , I
Model of a band of infrarad ra&ation absorption b water vapor.
Vest.Momk.un.Ser. 3:Fiz. astron.18no.] - 54-61 ja-7 163o
(MIRA 16t5)
1. Kafedra astrofiziki Moskovskogo univerisitata.
(Speotrum, Infrared) (Water vapor)

KOZHEVNIKOV N.I.; SITNIK G.F.
P
Absorption of radiation in a spectral band composed of lines
whose contour is duo to the Doppler effect and damping. Vest.
Yfosk. un. Ser. 3: Fiz., astron. 18 no.2:67-74 Mr-Ap 163.
(MIRA 16:6)
1. Kafedra antrofiziki Moskovskogo universiteta.
(Spectrm analysis)

5/033/63/040/001/008,,1016
E032/E514
AUTI I ORS: Kozhevnikov, N.I. and Klyakotko, M. A.
T-, I T L i Dotermination of some parameters of large-scale
motions in the solar photosphere
P:,'-,1OD3CAL: Astronomiclieskiy zhurnal, v.40, no.l. 1963, 6-L-70
Ti-~T: In a previo us paper the authors put forward a method
o~'studying the longitudinal motion of nonrecurring sunspots.
In the present paper a more detailed analysis of the method is
and the results of its application reported in the previous
paper are analysed. It is shown that the average modulus of the
0ifterence in tlie velocity of two sunspots separated by a latitude
intcrval "q) can be approximately represented by a function of the
f ((p) = a sin 2 rr (P + (3)
T
%-Aiere TOP) is an aperiodic function. All the graphs of ji~-Vj n
v.iven in the previous paper can be approximately fitted with
t,lij.s function. An adequate representation is obtained by putting
TOP) = K(p. It turns out that the parameter T reaches a minitnum
Card 1/3

Dot or mi nation of some parameters ... S/033/63/040/ooi/008/016
E032/E514
at times corresponding to mininium solar activity and then increases
-%gain. This is deduced ti-om analyses of data for 1882-1896. It is
still, not clear whether the variatinq of T has a period equal
to the eleven-year cycle or the twenty-two-year cycle. Analysis
of the data for 1897 and the following years should yield an
answer to this question. The parameter X is found to increase
ano decrease in synchronism with the degree of solar activity,
although this must be confirmed by further analyses. Th,!,
amplitude a increases as the minimum of solar activity Is
approached and then decreases towards the solar activity maximum.
All the results are in agreement with the assumption that the
meridional. component of the motion of photompheric matter is
mainly governed by the latitude (p of the point under consideration
and, to a much lesser extent, by the longitude. It is, therefore,
very probable that the motion of photospheric matter may be
divided into zones inscribed on the sun in the longitudinal.
eirection. The parameters'of the motion will then vary from
zone to zone and the width of any given zone *ill be relAted to the
period T. On this assumption, the width is found to vary during
Card 2/3

L)etermitiation of some parameters ... S/033/63/o4o/ooi/oo8/oi6
E032/E514
it -iolar activity cycle between 5 and 80, decreasing towards
activitj I'Allimum. It appears that the width of all the zones is
roxq,kly the sante, although this must also be verified in more
(lotail. Finally, the effect of the inclination of these :rones to
the equator ib considered and it is shown that this inclination is.
n,)t likely to vary since if it did the effects would be in
coritradiction with observational data. The results of tho above
cannot, therefore, be explained by this type of effect.
There are 10 figures.
~,z; 0 C IATI ON Gos. astrononticheski.y in-t im.- P. K. Sliternberga
(State Astronomical Institute imeni P. K. Shternberg)
:~Ulsl'-iiTTEO: November 16, 1961
C;ird 3/3

KOMEVNIKOVf N.I.; MAKAROVA, Ye.A.;
Effect of atmospheric pressure on thti half-width of oxnen lines
in the 1.27 band. Astron.zhur. 40 no.t').-1095-1100 N-D 163*
~)4 F
(wmA 16:W
, ~ j 4,,,14
1. Gosudarstvennyy astronornichf3okiy J11,-
. -, k, m. P.K.Shternbdrga.

ACCESSION KR: AP4033634 8/0188/64/000/002/0052/0055
AUTHOR.* Kuz'miny*kh, V. V.;_.Kozhevnikov, N. I.
TITLE: The problem of the accuracy of determination of the source function of a
plage
'SOURCE: Moscow. UniveTsitat. Vestnik. Seriya IIX. Fitiks, astivnomiya,
no. 2, 19649 52-55
I TOPIC TAGS: astronomy, solar activity, solar plage, solar photosphere
ABSTRACT: A study has been made of the influence of errors in observations of
the plage-photoophere contrast on the accuracy of determination of the source
function of a plage. The observed discrepancies in the temperatures of plages
I cited by various authors can be attributed in part to observational errors. A
method is proposed for correctly estimating the order of the value ST. When
determining models of a plage from observations of the plage-photosphere con-
traot in a number of wavelengths it is possible to have differences between
models obtained for different A , in part caused by inaccuracies of observation.
At the same time. in photoelectric observations it is admissible and legitimate
to have discrepancies in T in the "hot" region of a plage of the order of 30-SOC
1/2
U

I ACCESSION NR: AP4033634
and in the "cold" region of 70-120C. Orig. art. has; 3 formulas and 2 tables.
ASSOCIATION: Kafedra nebeenoy mekhaniki i gravimetrii, Hoskovskiy tin-
iversitet (Department of Celestial Mechanics and Gravimetry, Moscow University)
sumaTTEDI 27Apr63 DATE AOQ: 30Apr64 EXCL. 00
SUB CODE: AA NO REP 80vt 005 MM: 003
iaid
.212
~F- VIV

KOZHEVNIKOV., N.I*
Comparison of E14asser and Goody's models of the spectral
absorption band of the infrared, radiation by wpi---- vwnnrs. I;oob.
GAISH no-131:3-9 164. 't~ ! '; - - -
Radiation absorption in a band consistiiig of irregularly
disposed lines. Ibid.110-15 (HIMA 17:8)

KOZHEVZIIKOV, N.I.
yers w�t'n various altitudes to the
Contribution of atmospheric Jw
phenomenon of the twinIcling of the iwila limb. Soob. GAISH no.1339
3--9 164.. (MIRA 17:8)

ACCESSION NR: Ap4oi4447 S/O 188/64/000/001 /0071/0080
AUTHOR: Kozhevnikov, N. I.; Kuz'mInYekh, V. 0.
TITLE: Temperature distribution in faculae
SOURCE: Moscow. Universitet. Vestnik. Serlya 3. Fiz. astron.,i)no. 1, 1964. 71-80
TOPIC TAGS: sun, solar physics, solar facula, facula, astronomy, facula tempera-
ture
ABSTRACT: Seven different ways in which the source function for a facula can be
expressed are explored. It is shown that the behavior of the source function for
a facula cannot be the same as the behavior of the source function for the photo-
sphere. The source function for a facula should have a "kned' at a point corres-
ponding to some value of the optical depth -C. on the basis of previously publish-
ed observational data and using the proposed model of the source function, the
authors compute the dependence of the temperature of the facula on optical depth
for various wavelengths. it Is demonstrated that deviations of the ttunperature of
faculae from the temperature of the photosphere have a systematic variation with
a change in wavelength.. Orig. art. has: 5 figures, 3 tables and ig formulas.
ASSOCIATION: GOSUDARSTVENNY*Y ASTRONOMICHESKIY INSTITUT IMENI SHTERNIIERGA (State
e6rd. I 4z

ACCESSION NR: Ap4o)7617 S/0033/64/041/001/0087/0()89
AUTHOR;
TITLE: The form of the image blur functiois for the solar disk edge
SOURC9: Astronomicheskiy zhurnal, v.. 41, no; 1, 1964, 87-89
"
TOPIC TAGS: solar disk, solar -disk edge, image -blur, solar disk Image blur,
image blur functiorl,,.Wanders fun4tio;) 0
ABSTRACT: Measuring the intensity distribution over the solar disk edge requires
correct location of the edge, which Is not possible without taking the blur effect
into account. Sinii Wanders' bi6r Qnctlon is 6npi~ical, It was of "interest to
d2fine the limits of its effectiveness and to find the exact form of the function.
Stating that a blurred edge of the solar disk results from light beams passing
through a turbulent atmosphere and that the deflections in the solar disk edge
image are proportional to the fluctuations in the refractive index of air on the
path of a light beal, the author derives a formula which represents the form of
th~ blur function.' As shown In the Enclosure, c6mp~rison of the authors formula
with the Wanders function revealed good approximation for a 10-40 cia diameter
telescope. Orig. Aft. has: 9 formulas and I graph.
Card' 1/3 1 :1 .1

ACC.ESSION NR: AP40~617
AS~OCIATION: GOSU6A:RSTVENNY*Y ASTRONOMICHESKIY ~iNST'ITUT IM. P.K. SHTERNBERGA
(State AstronomicafInstitute)
SUBMITTED: 101)ec4, DAT~ ACQ: ISMar164 ENCL.,. 01
SAI CODE: AA NO REF Sov: 00' OTHERiv 002
Card 2/3

KOZHEVNIKOV, N.I.; KIIZ'MINYKH, V.D.
Structure of a facula. Astron.zhw,. 41 no.21323-331 Mr--Ap 1614.
(MIRA 17:4)
1. Gosudarstvennyy astronomicheskiy institut im. F.K.Shternterga.

BARUZDIN, V.I.; WIMOCHKINA, Te.P.; KOZHEVNIKOV, N.I.; SWALOVICH, A.F.,
red.; CHIMYAKOVA, K.P., telchn.red.
[Collection of problems on the probability theory] Zadachnik po
teorii veroiatnootai. Moskva, Mook.aviatsionnyi in-t, 1959. 46 p.
,(MIRA 13:9)
(Probabilities--Problems, exercises, etc.)