SCIENTIFIC ABSTRACT KOVAL, I. K. - KOVAL, N.

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• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R000825510014-5
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• Document Creation Date: November 2, 2016
• Document Release Date: June 14, 2000
• Sequence Number: 14
• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT

33-3-12/32
R.~sul-us of photogra.;)hJJ'L%; observations of Mars at the Kharkov
Astrunomical Obsem-ttoxy during 11954. (Gont.)
atmosphere is more i1ransparent a:b,:)ve the "seas" than above the.
?R(-,ont-`J3.ent s 11.
The polar oap is xvddish compared with a white screen. Th-15
c~;)nfi.-Ias pievious n~stilts obtained at the Kh.A.0. The fact
that the smoothness factorbr the southern polar cap bas a mmci-
imm value in 'the blue region of the spectrum agrees well with
N.P. I&arabashovIs hypothesis that the polar cap of Mars consists
o-' a IAiin layer of ho~Lr-frost or ice, above which float CaDud-
like forTngtions.
TIlere fire 9 tables, I figure and 9 references, 8 of which are
S.-L avi (-. .
A SSOCIATION: '.Eharkov Astronomical Observato3 (Eharlcovskaya
Astronomicheskaya Observatoriya
SUBMITTED: November 9, 1956.
A'T~IIA30,.- Idbrsa7 of Cmgnms
*at 3/1

B OVAL I p I-K ,
-, , - .i -
Intogral. brighl~,rjess of the solar corona of June 30, 1954. Uch.-
zap,,KHGII 91i2l,1-248 157. (KRA 15:3)
(Sun-Corona)

K
~M I~HASE IBOOK EXPLOITATION SOV/1391
Akaaemiya nauk .13SSR. Astronomicheskly sovet.
Pollwye solnechnyye zatraeniya 25 fevralya 1952 1 30 :Lyunya 1954 g,
Trucky ekspedJ.tsiy po nablyudeniyu zatmeniy (Total Eclipse of the
Sun, February 25, lg!")2 and June 30, 1954. Transactions of the
Evedition to Observe Solar Ec2ipses) Moscowp Izd-vo AN SSSR, 19513.
357 p. 1,200 copies printed,
FAtitorial Board: PariyOUy,, N.N.., Candidate of Physical and MathemA-
tical Sciences (Resp. Ed.); Kononovich, E.V. (Secretary); Kuzlndn,
A.D., Candidate of W-ohnical Sciences; Mogilevokly, E.I., Candl-
date of Physical and Mathematicaa Sciences (Deputy ReBp. Ed.);
Plustell, E.R., Correiiponding Member, USSR Academy of Sciences; Ed.
of Ikiblishing Holase: Yegorova., N.Bi.; Tech. Ed.: Kashina, P.S.
IMPOSE: This book is Intended fox, amateur and professional astro-
nomein interested in eclipse phertomena.
COVERAGE: The present compendium io the fourth in a series published
by the Academ~y of Sciences of the USSR on solar eclipses observed
in the Soviet UnIon. The present collection reportd on the resultB
Card 1A

Total 1:3elipse (Cont.
SOV/1391
of observations obtEcLned by scientific teams of 20 research in-
stittutions during tkv~ total solar eclipses of 1952 and 1954. The
reports Include stuebes of the oun's chromosphere, its total cor-
onal brightness, monochromatic glow, structure, polarization pho-
tometry., and colorlmotry. The results of studies on coronal
radlo emissions for various wavelengths and on the effect of the
sun on the earth's ELtld0sphere, based on the February 1952 and June
1954 eclipses, are presented. U.'he individual articles are accom-
panied by tables, diagrams and bibliographic references.
TABLE OF CONTENTS:
Foreword
Krat, 'V.A. Gradients of Chromospheric Lines
3
5
Vyazan:Ltsyn, V.T. Spectrophotometi-j of the Chromosphere, From
Observations of the Total Solar Eclipse of 1952 7
C a rd 2/8

Total Eclipse (Cont.) SOV/1351
..~teshenko, -N.V. DUtriblittion of. Chemical Elements and Electron
Concentration in the (,'hromosp~,ier6 (From Observations of the
T6t&1 Solar Ra-lipse of.'February 25, 1952) 15
gifosherilto, N.V. and.Zemwiek, Ye..Xh. Study of the Boundaries
of the Chromoispheri.6 Lines of Hydrogen, Helium and Ionized
Calcium 36
-Awall I.K. Total Corctral BM4htness From Observations of
16~4tiTS-olar Eclipses 6T February 25il952 and June 30, 1954 49
Sh,aronwr., V.V.. Total VIE~ual Photom.etry of the Solar Corona
in 1952 and 1954 62
Sytinskaya, N.N. Photo,0,rkphic,Evaluation of the'Total Bright-
ness and Color of' tbe-Solar Corona of 1954 In Yeysk 81
Kwasishvili, Ya.l. __Radiciie'try' of the SolarICorona During the
June 30, 1954 Total Solar Eolipae 83
Owed 3/8

Totaa Eclipse (Cont.)
SOV/1391
Senoliuk, Yu.F. Gener-ali;zed Photometry of the Solar Corona on
February 25, 19!52 159
Kapko, Ya.T. Photograpide Photometry of the Solar Corona on
February 25, 2952 173
Und~,'L:Lis., L.M. Photcmieti,7 of the Solar Corona on February
2!5.0 1952 187
Aliyeva, G.K. 11photomotry of the Solar Corona on February
2!5;, 1952 187
.3-Y-tiriskaya, K.N. Distribution of Brightness and Color in
the Solar Corona oil June 30, 1954 189
1 haronov - of the Solar Corona
31, , V.V. lfisu~al Colorimetry 199
Grigorlyev, P.V. and O.B. Vasillyev. Photometric Observations
of the Solar Corona With Automatic Aerial Cameras During
the Total Solar Eclipse of June 30, 1954 207
Card !V8

Total Eclipse (Cont. SOV11391
Nesmiyanovich., A.T. Photometry of the Corona of June 30, 1954 223
Konopleva, V.P. Milti-colored Photometry of the Solar Corona
of June 30, 1954 233
fladubovich, YU.A. Photometry of the Solar Corona In Red Rays
on June 30, 1954 247
Folupan P.N. Photanetry of the Solar Corona In the Green Line
A 5303k 252
Fariyakiy, N.N and K.I. Oetrova. S_pettrophotometry of Coronal
and. Chromospheric Lin~~s During the Eclipse of February 25,
1952 258
Vashakidze, M.A. Analys:'.5 of Radiation, Polarization of the
Sc)lar Corona Based on Observations of Total Solar Eclipse
or February :25, 1952 291
Card 6/8

Total Eclipse (Gont.) SOV/1391
,F~menkop B.D. In the Coe=cieht of Atmospheric Trans-
Parency During i;hiq Toital-Solar Eclipse of June 30, 1954 307
Gavrild v, I.V. and I.,G. Kolehinhlcly. Computing Corrections
of the Moon a Cooindinates From Db-bervations of the Eclipse
of June 20, 195JI attbe Main Astronomic Observ atory of AS
UkrSSR. oil
3224-
Vitkevich,,V.V. and B.M. 'Ghikhachev. Observation of Solar
Radio Endesions In the.Meter Wave Band During the Total Solar
Eclipse of Febnta%7 25# 1952 329
Troitskly,, V.S., Zeiinskew"al V.L. Rakhlinp V.T. Bobrik.
Results of Observation:'of So-lar Radio, Emissions In the 3.2
and 10 cm Wavelength During ithe Total Solar Eclipse. of
February 25.s 19~)2 andJune 301 1954 330
Molehanov, A.P.,, E.M, Qyaininen.,- A.V, M,4"-Ikov,, Al.P. Molchanov,
L.L. Myasnlkov, V,,N. Rjrsakov, F.I. Skripov, N.M. Filippov..
Results of Solar lwollp,se Observations of 1952 and 1954 in the
3.2 cm WavelOngth'. 331
C ard 7/8

- . lw~wxp~nwlawwwrlffm~ 4-
KO%AILI_-I. K. an6 WAlkSHOV, N. P.
liPrellminary Resu*-ts of the Investigatlon of the Polarization of the Moon
by Means of Light Filters."
Ragmt. :Fmisauted at the Plewrry Nmt.Wg of tbe Comittee of plo=tary Phygics,
Cc=t,,Il cd" Astronomrs.. IMw IkDv, M-22, jkq 10.
Mfft~,- -Ak lktttk SSM, 19511, &)- 8p P- 11-3-Ull)

:5 ( i )
AUTHORS: Bara'bashov,N.P.,and Koval',I.K. SOV/33-35-2-11/21
TIME: The .3tructure cf the Southern Polar Cap of Ma--s in 1956 (x
voprosu o stroyenii yuzhnoy polyarnoy ehapki Marsa v 1956 g)
TERIODICAL: Astranomicheskiy zhurnal,1958, Vol 35,Nr 2, Ip 261-264 (USSR)
ABSTRACT: Using the data of observations of Mars in 1956, made in visual
light at various observatories of the world and also obser-.ratio
in the ultraviolet made at the KharIkov Astronomical Observator
the author considers one of the possible interpretations of the
structure of caps of Mars. The simultaneous disappearance of th
southern polar zap around September 1, 1956 in red a-rid ultra-
violet light (fLg- 3,4) can be explained by the fact that at
that time the oips lay wholly on the solid surface of ,,-ha
planet in accorlance to Wright, fRef 62. The ccntrast in
the brightness between the cap and the rest of the planet's
surface observed in various parts of the spectrum is explained
by the absorbinIT, properties of atmosphere of Mars. Ar.
Ce.rd 1/2

The Structure of the Souflnern Polar Cap of Mars SOV33-35-2-11/21
in 1956
app,roximate estimation of the optical density of the planet's
atmosphere in the ultraviolet ('Cw,0.3) has been made. The
author mentions especially observations of G.1 Tik110V Ref
and Ye.L-Krinov Ref 7 -
There are 6 figures, I table, and 9 references, 6 of which ar
Soviet, and 3 American.
ASSOCIATION i Khar I koirskaya astronomicheskaya observatoriya (Khar1kov
Astronomical Observatory)
3UBIZITTED: August 21, 1957.
Ci.-Lrd 2,12

.WTHOR; Q0-28- I x.K. SOV/33-35-5-14/20
TITLE: The Ts`o-lute of Venus in the Ultraviolet and Infra ed.
(Absoly-utnaya fotorietriya Venery v ultrafioletovykh i infra-
krasnrkh luchidch)
PERIODICAL: Astronzimicheslziy zhurnal, 1958, Vol 35, Nr 5, rip 792-796 (USS
ABSTRACT- Prom August 2*,~ to 26, 1956, the author obtained ca. 60 photos
(if Venus in tho noighborhood of the quadrature. The 270 mm
reflector of the Kharikov Astronomical Observatory and ultra-
violet as wel". as infrared light filters were used. The autho
describes his methods in detail and collects the results.in t.. reo
tablet). For the evaluation a method of N.N.Sytenskaye. Lr-Re-f 1. 7
at the CibservE;.tory of the Leningrad State University was used
The author compares the results with those of I.A.Parshinjef g.,
N.P.Barabashov Z RE!f 32 and with the model of V.V.Sharonov
fRef 52. He thanks the students of the KharlkovUniversity
M.Levirrtov and O.Bugayenko for..", 71~aid during the observation
There are 5 trables, I figure, and 5 Soviet references.
JiSSOCIATION:Kharlkovskaya astronomicheskaya observatoriya (Khartkov
Astronomical Cbservatory)
SUBMITTED: August 21, 1957
Card 1/1

L'f
IMME :1 BWK EDUTUTION SOV/4302
Akademiya nauk SWR. Komiss:Lya p:) fizike planet
Izvestiya., vyp. 1 (Nevs of tJu-. Coinission on the Physics of Planets,, No. 1)
Khartkov., 1959, 103 p. :L,,000 copies printed.
Editorial Board: N.P. Barabiw3havp Academician of the Academy of ScJ:ences
Ukrainskaya SSR (Resp. M.); V.I. Yezerskiy.. Candidate of Physicit and
Mathematics (Sei,.retary); A.V. Iftrkov., Professor; Yu. N. Lipskiy, Candidate o:
Physics and Mat:11jei=::bics' wad A.T. Chekirda, Candidate of Physics and Mathemw Les,-
Ed. -. D.A. Vayrfterg; Tech. Rd.: A.S. Trofiwnko,
PMtFOSE: This -puW11cation iii intended for astrophysicists and astronomers.
COVERACM: This co:13.e Vion ve articles constitutes the first issue of a nev jam ial
on problents in :;ilanetary -physizs. The first six articles discuss the surfaci
features, polarimetry., and apeatrophotoretry of the Moctu The remaining art: tles
deal vith the p]:grsics of Iftro, Jupiter, and the asteroids. No personalities ILre
mentioned. References acnompany individual articles.
Clard 1/3 1

Neva of the Commiesion (CoMt.)
TAIM OF CONTEM:
SOV/4302
Baasbasbov,t N.P,,v and A*T, f,'.hekLrda. Types of Rocks Most Clotlely
OviTesponding to Ibose of the Umar Sarfame
KOVMP Y6. K. 11ruves-bigatiln Ija Three Parts of the Spectrum
of the Degree and. Angle of the Position of the Plane of Polarization
of Light Reflectoill Frm'Lanar Features
:Bax abashovp NP.p and X,K,, .10val" Photographic Polarimetry of the
Imbom With Light 71.1tere I--- 1 55
13ergeyeva,, A.N. 19pecit'rophotow-try of Uniar Formations 59
3arabashov.. N.P., V.A,, Yeze:-,,-aka:ya,, and V,.X, Yezerskiy. The 11roblem
of the Photomtric UWLforzV.*,y, of the Moon's Buxface
Ilytinskeyal X.N. Probable Dimensions of the Ruggedness of the
Ificrorelief of tIA, ft)n's SiuTwe 81
Card 2/3

JL
.-Mm I '~XxIX _MWITATION EOV/3923
Ak-sdeniya nwk 13:30R. Astrm3otdchaskiy sovet, Kaidssiya po Mike planet
Rez-alftaty nabl:,yadeniy Ybran vo vromwe velikogo ProtivostoymLys 1956 9. v 8
(Results of V2e Observation of Man in the UMR During the Great Oppositi- n'
of 1956) Xoiscowj, Izd-w, Mi SM., 1959. 193 P. lj,300 copies Twiuted-
Ed.: B.P. Barabimflovp Acakesdcianp AcadeiW of Sciences VkrSM; Ed.. of Publi hiz
House: V.A. Bronahten; Tech. Ed.: V.V. Br=gull.
PWOM: The IXK)k is Intended. for *Atr*aomers and astr*pbysicists., particul.r1l
those interestAd in the study of the planet Mars.
COVERAW: This is a collection of 8 arhicles on the results of observationsle
Mars durlmg ile zggpositiin of 1956. The observations were organized by t~hx
ComnltteL~, fox, thd Lxresttgation of P!qoicel, Cqnditjons on the Mon and. PL aets
of the Astrowmic Council of ~he Acadex7 of Sciences UIM,, an(I were condw bed
mainly at the southern obsermtories of the Soviet Union dwrii)g the jpreerloN4 from
August to December,, 1956. The prel'=J ary results of those observations il-tre
Carl 113

Uwalts of the *bsermtion w.1 Vlore (C*ntd) 8()V/3M
:-sumarized st a aoafe;enwo,of all partAcipants bold in Mosacw,, Necemadber A
1956 . The :prew.4nVpkb.`Ai.%&tion covers the investigations of Mars' surfi ,e
and atmospbere lyy photmurbry as vell va by visual obserrationop problen of
the flors. of the p1met wid the pbotametric imstigation of its lwwd1nMcn- I
Argyre zone. Re'rerenceo accompany most of the articles.
TAZX OF COMMS:
Obserrationo (it Mars in tbA~ USM in 19% 3
Tikbovo G.A. Brief Resultr,of the Obserwations of Mars by the
Astrobotmy Section Daring the Period of the Great Opposition of 1956 6
Barabashurs N.P,o and 1,11, 146~1. Rwtograq)hlp Photowtry of
Mars With L1*,t 10
SytinxbMm, W.N. Photowtvic Investigation of Optical Properties of
t.U-3 Atmospherv- of -the Planet, Moro
Shamnov, V.1'. S~wface and. Atmosphert of Mars According to PWtogmphic., 1E
Z
Pho tr-tcj, eaul Colorlzwtxlc Mmermtianis Candacted. in Tashkent in 1956 ;, 123
Caxd 0

J, I -
PRM I BOOK EXPWITATION SOV/4093
Marabasbov,, Nikolay Pavlovich., ani. Ivan Kirillovich Koval'
lotograficheskaya fotDmetriya Karia, so svetofilttrazi vo vmmya ve2lkogo
protivostoyaniya v 1956 g. (?.~wtograjkic Photometry of Mars Using Light Filt
D=Ing the Great Qpposition of 1956) Khartkov, Izd-vo Kh tkovskogo univ-ta.,
1959. 529 P. 1,,0)0 copies printed.
Resp, Edo A,T. CWikLrft,;- Eds.: A.W. Trettyakova, and DA. Vaynberg;
Tech. Ed.: A.S. Trofitwn1w.,
PW)SR: This book In inl:end*d for scientists interested In physical conditions
on planets,, and ma:r be used by students ana aspirants concerned with prdblem~
ol planetary pbyL:;ics.
""OOMM. The book disewises the methodology and results of observations of War
diwing the great opposition of that planet in 1956,, and contains tabulated da,
Cimpildd at the MaAm- Astroncutical Observatory on the absolute photometry o
Wre, The book also contains aaw results of visual observations of the Mart
mtrface. The major, part of the text is a tabulxtion (Table 4) of spectral va
of the brightness, factor P fox, different points on the continent., bright am
C,
.I ard-14--

,Phcr.,,~ -.raphic Pbotometry of Xars (Vont.) 807/4093
and polar cap of MEws: The med-n series of observations vere not mWe similtEfteously.,
but lasted from 30 to 4.0 minutwe each., end hences for each individual light 1~ *2ter,
the length of the central nerie4an of the planet, and the values j (incident f-mgle
of light ray), E (angle of reflection), and C? and t (width and 3inirth of 1=_ie
.anetocentric coordinates of the point source of light, respec -~-ar~ g1g,en
3 tive:
p
for the period fron, June 15/16 to October 21/22. The value of the phase angll-!
is also shown for each date and-, each fil:ter, The -supplewnt contains grapba ~:rhich
plot t1w distribution of brightness a3AMg the eqaator (in a band - 10*., -30*z
width) and over -the central mexIdian of theplanet. The abscissas g;Lve value* of
and the ordinatesj, values of P - 10~1 (for simplicity). There are 9 figures,
14 tables, and I:'? refer3nces: 13 Soviet and 2 Eng3ish, 'No personalities areg~
mentioned.
TAKE OF CONTMS:
1. Purpose and methodology of observations of Mars during
tb-.- great opp
. osition of 1956
2 1 Processing observational duta
3j Vinibility of Utail on the surface of Mars in 1956
4, Clouds, fogs, and precipitations observed on Mars in 1956
5. Some detai3z obvemtd on thi Xortian disc
6# Deocription of laie enearazote and chmgon in the aoutlwrn polar cap
Card 2A

MRABASHOV, R-P., PrOf.akad, .* KOVAL., 1.1-
Photographic polarimtry of the noon with light filters. INV.
KOM.Po fi1g.plALU. no.,1:55-58 159, (MM 13 '-7)
1. AN USSR (for Parsbasbov).
(Polariscope) (Noon--observations)

KOVALI. I.K.
DWee of the evennue of continents and @@as on Mars. Izv-
90001PO Is,plan* ao*lt85-A)2 1590, (UM 13W
< (*r9(punet))

BAROASHOV, N.P. [Bar-abashov, M.P.), akaaemik; KOLU-L,',_LK-
Distribution of briehtness In Iflare 1 seas. Dop.AN URSR no.2:
1153-155 '59. (MIRA 12:5)
1. AN TISSR (for 'Baremb). 2. Khar Ikovskays astronomichealmys.
observatorlya. (Rare (Plans10)

P41bv If W9 lax* sommog w %NNLJ gaNIAMW
BARABASHOV, M.P.., d1rademik; KOVAL', I,K., kand.f it.-mat onarti
Main recultv of obrervationo of Nars during 1936 at the 11harkov
Astrom,omical Orbservatorre Vienyk AW MW 30 no.1:15-23 Ja 159-
(MIRA 12.
1. AN UESR (for MWabashov)
(Rare (Planet))

30273
S/035/6 1/1000/0 10/027/,~34
AOO-I/AIO1
AUTHORS: Barabashov) N.P., Koval' I.K., Cliekirda, 1,T.
TITLEt Some results of photometry of cloudy formations on Mars
PERICOICAL: Ref,4)rativn.yy zhurnal. Astronomiya i Geodeziya, no. lo, ig6i, 66#~ab-
stre~ct IOA457 ("Izv. Xomis. po fiz. planet!', 1960.0 no, '42, 36-40)
TEXT: Blue clouds observi,.id mainly in the equatorial zone of the planet
are described on the basis of phot:ographs taken in 1958 b-.r means of a 10" ref:iec-
tor of the Khar1kov Observatory with the equivalent focus equal to 15.3 m in I
ulti6iwlolet (),3600:) and blue- (',14200) portions of spectrum. The existence oj~..
a photometric scale makos it poasible to obtain the curves of brightness dis-
tribution along the equator of intensity, when the clouds are present and at
thoir absence. The analysis of materials has shown that the presenbe of cloud"I
on the disk'and terminator does not depend on the albedo of the underlying soR~*,d
surface of Mars. The vailue of cloud-background contrasts- and the albedo of t.~Ie
oloud-s on the tenninator are higher than on the disk. On an average, the brigi,'It-
Card 1/2

S/~35/PI/WO/O 10/0 27A 34
Some results of photometry A001/A101
ness of clouds exceeds -the b6kground brightness by 14%. On assumption that I
lie
clouds studied are analogous, in their nature, to cirrus clouds of the Earth'f_~
:z
atmosphere, their thicimess ALs estimated to be 3 6 m.
1. Leb6deva
[Alo,straoter's not-ij: Complete translation]
Card 2/2

S/033/60/037/02/009/013
E032/E914
AI.VVHC)RS:. Barabashojr N' PK
1 .9 .1 -,
T3*-*TIiE,': Some Results of Stvdies of Contrasts on Mars
P112IODICAL: AstronomichesMy 4hurnal, 1960, Vol 37, Nr 2, PP 301-30"
(USSR)
ABISTRACT: It is we,11-knova. that the continent-sea contrast K f
or'
Mars has a maximum value in red and a minimum in blue.
According to meastrements carried out by the present authois
in 1956t K = 0.286 for 647 m-g, and K = 0.07 fOr
ax = 420 mp.. Hovirever, occasionally, the contrast in blU6
1%m
light reaches 80%11of the contrast in red light. Usually,
this is erplained "by increased transparency of the blue
atmosphero on. Mars. If one accepts the explanation that
the true contrast -is the saine for all wavelengths and the
apparent .,,:ontrast depends on the state of the Martian at-
mosphere, then one can try and estimate the optical thick-~
ness of the Martiaa atmosphere in blue light, from the
Q1 17 (11 /"i corresponi.,ling cont-oast. For this purpose it is assumed
V

I MEEMM R~MKRH-OMEW
S
/033/60/()37/02/009/013
E032/E914
SoMe: esults of Studies oi'Contrasts on Mars
ST
that Kk ;= const Eu:Ld the red contrast is taken to be
7
approximal;ely equal to;the true contrast since the optica3
thickness of the stmosPhere in red light may be taken to be
approximately zero', TILe . present paper is concerned with a
critical examination of the possibility of an explanation
of the va:riation in by variations in the optical
Lblue
ve e
thickness. Fig 1. gi -the values of the contrast for
red, green aad blue rays (curves 1,, 2 and 3 respectively)
for June, July, August and September, 1956. These data
refer to 4~:;he centxal regions of the planet. Fig 2 gives
the corresponding plot for the ratio for the
Kbluel'~?ed
same obse,,,.v7ational period. Another characteristic considei-,d
i
s
B Kre -/R* where is the albedo of the
.'L (1 d blue)
Y
VC
Card 2/3

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S1751/61/000/008/001/005

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3. /S--5-6 (/,fy// 14
AUTHORS: Kova 11,
TITLE: 15nsome
Mars in
PERIODICAL: Astranoinicheskiy
33423
S/033/62/039/001/007/013
H032/E514
I.K. and Morozhenko, A.V.
properties of the yellow haze observed on
1956
zhurnal, v-39, no.1, 1962, 65-72
TS,XT,. It is stated that all the observers of Mars noted
a relatively sudden decrease in contrast between the bright and
dark regions on the surface of the planet in the middle of
Z
September, 1956. Most observers, including the present authors, S
are said to ascribe this phenomenon to the appearance of a fine
dust cloud in the Martian atmosphere. The aim of the present
paper was to determine the optical thickness of this cloud in
red and infrared light. The analysis is based on the experi-
mental results reported by N. P. Barabashov and I. Koval'
K.
Olef,,5: "Photographic photometry of Mars using light f ilters",
Lrd-vo KhGU, Khar1kov, 1.960). A detailed analysis of these data
including corrections for the seasonal variations in the surface
contrasts, leads -the present authors to the conclusion that the
dust ,Cjoxud had mainly scattering properties and that its optical
Card [ 1/3 1

33423
On. some propertios of the yellow ... S/03,3/62/039/001/007/013
E032/E5i4
thiLckness increatied with incr.easing wavelength. It is estimated
that the optical thicknens was as follows:
Tabl. e 5
X, MIL 1340 750 647 530 430 36o
TX 0.,54 0.26 0.19 (0.12) (0.08) (0.01)
Next, using the results reported by V. V. Shuleykin (Ref.11:
physics of the sea, Izd-vo AN SSSR. M., 1953, P-589), the authors
attempt to deduce the radius of 'he particles of which the cloud
was made up. It is estimated that this radius was 1.45 11.
Finally, a calculation is made of the seelimentation rate of such
particles. It is assumed in this calculation that the particles
do not collide with each other and that convective motion in the
atmosphere may be neglected. Taking the mean 7free path of gas
molecules in the Martian atmosphere to be 10 cm, and assuming
Card 2/3
_q

M "NMI mggmswdm~" f";WAMFAMII
KOVJI.6t I.K.
Distribution of :EhlkglmtrA93 in Ow Rdge Zone of Mars
Rliport to be subgrAttod for the 4i;h Intermtional Space Science SYMPONium
(cosPAR) warsawj, It.22 junt 63

MaR.'VIENKC)i 116VO
Dagree vf EmiootbreEs of the Martlun det-lerta. Izv. Kam, po ft-z. plano
no, 4 _3 9- 3~4, Ag 16,10 RA a-8 5)
1. astlrcmbul~,heslmya ob3erva'Wriya AN Ukra'SR.

-H za REMIFOWIM25",
AQCIPISSION Mt: AT3007071&*!I~ "',/2617/63/005/003./OC),'~-7/0067
AWHORt. DLdy*chenkoj,',Y4,P, I*; Koval I I rzh
Ke; Mo erikop A* V,
TITI'S: Results of speciXrophotometric observations,or Mars in 1960-1961
SOUB CE Alt UkrRSR., Hollyma astronoaddana observatoriyao Izvestl~rajy ve 5P
not - is, 1963 s 47-67
TOPI C TAGS: spectrophatometric. observationp.intensity distributions disc radius
brithttess, polar cap-
ABSTRAOr: In view of', Vael almost total lack of spectrophotometric observations of
Mar j -the three authocrs -undertook to obtain as many photometrically standardi 2-e-d
, 1.4 ~
spect ograms of it aa possible with different orientations-of the spectrograph
r
ape;,ture., to stucbrs 1) the dintribution of intensity in the sp-fttr6,09 the con-
the polar caps n-d-the
tincritti and seas at dlffeirAnt distancas from the center _&
RLght blouds; 2)-the dial., _.jbution of brightness along the equator of intensi
the. equator of, the planet- and the dentral meridian in monochromatic rays, ine_jUd. T.-
Ing, a otudy of the spectral course of the continent-sea contrast., establishment
of fbe boundary of its disappe,~rancej and also possible shifts of this botmdary
Dart: t
J

ACM;SION,NR' AT3007874

depezi,ding.upon the state of the atmospitiere.. characterized by possible changes in'
the distribution of erienj-j- in- the speciprum of the continents* observations were;
Onde in the Cassegrair. foaus of the 70.cm reflector -telescope of the State
Astronomical Observatory of the Mcranitin SSR Academy of Sciences from 1 Cetober,011
1960 to 6 Februaryj 1561.p WQh bpectrof7aph ASP-5.p aperture OeO5 mmp 70 spectro"'
i being obtained on "Kodak OaFIIP bvt only 23 selected as best*- The authors
grama
1'Conclude: 1) The reflecting poirer of Mars (center) edgesy p;,)lar capsy Right
olou6s) according to the spectnim varies smoothly from 0*330 (lambda N 6550 A)
to OSC53 (lambda x 4030 A)p so that no dispersion waves were discovered during
the 3,960-196.1, opposition.; 2) the distribution of brightness along the radius of'
1the else (along the eq~tai-bor of intensity) at lan, bda Z. 6550 A near opposition is.
well repmente-d by rho sub, i a rho sub o cos i but with growth of the phase
the curve rises sibove the cosinusoid branch' 3) the curvature of the bright-
bngle
ness curve along the equator of intensity diminishes smoothly from the red to
1: the violat end of the spectrum.; Q the brightness curves along the equator of
inter,sity and the central meridEan coincide in the red raysj, leadine to the con-
polusim*that both polvi capq were at=ipheric formations in the period of
obselvations 5) the .9peciral course of the continent-sea contrast could not be

Card
2
13
.
,
J

VOLOTKOVSKIY, S.A., doktor tekh.rtauk; FVRSOV, V.D., inzh.; KOVALt, r.K.
inzh..; RUDI, V.I., inzh.
Operating characteristics of electric charging devices with seini-
conductor :[--~ctifiers- for use in mines. Vast. elektroprom. 34 no.8:
62-64 Ag 163. (MIRA 16:9)
(Electric current rectifiers) (Electricity ih mining)

IOKOVALt , 1.K.., otv. red.; FEWROV, Ye.P.p red.; GORYNYA, A.A., red.;
'"~'"'~'o-MCHINSIM, l.G.,. red.; LUKATSKAYA, F.I... red.;
BEREZINETS, L.P... red.
[Physics of' the moon and planets] FlziM Luny i planed.
Kiev, Naultova dumka, 19&1+. 137 p.- (MIRA 17-.10)
1. Akademlya nauk UR.91, Kiev. Holovna astronomichna ob-
servatori,.ia.

~aV'l V VJ
II"U tw. 4,21WA -TO.Wtv
~60 YV
m6ly the RIAOTI
vsp~b ID.
ngle'.Q~ -Of 60 an
. . . . . . . . . . . . . . . .lalbloz '!b~!MAbn6andc6nuldi
Cak Ahat arlp 6 1
-. 6# .0 es v
b Aile ethods used may acbmifif for
D
le p vqtomt rn
IV
In. b .1h1d.bbla-Vtor of II&I as a function of -mavelength, -
ivj pf the
ft

v

-.Ast:to*lillmlcal-O]7-------~-,,--
Smjinrl XzD;_ 1)
~ e--n
niar t IhV I s- of the Martian surface up)n dust
4~011teml~. SumMUTIziDg, ille aIftthq'V.'0DOkId6If'th tba-Martlan n~~osphere has, basically,
clkaracterlaij'a~ ~oxm th '1' , -of Maxs It fundamentally explainabie
9 01'ei -0. CO Or
as ihai of its out nurfDrei. The DoIOU'S'B 8uPpPoBition of a IbnoTdto powder surface seems
qW i-,e piIausible. The tr~:* brIghtnei� -bintri t' ofMartion continents and seas become
col'apittely wuOed-ow: j::y 4000 A. In the bandwiddt_4000
-fil-' - -b h 0
M31
-tr
0 116, Ln V Alai% n atmos-
or !Ion artl6atj Which behave in an anti-RELleigh,
and- left ol''6500 Ai
Mlt~ierv~6 i~tgard to k9hit scattierft'i.~ J U) th6
WYaWl. -b- wiilwidlfiJ6,f OU.Pe_ 6-kar
Iii of t
M g fian atmosphitrein
~ard-A6 edgm. 'Obtbival4 d -hould
Mini t Ni.0tudir-Of the surface alono v
n:th GHW" vieklmi- 3 lableB and I fonvula.
A
06MATIOm'- Gl~
ia~AN-UkrSSR Kiev _(]kIg_In
AM MrASSRIi
. . . ...... .~;'.

At L
v ril nghtl
J
IW
0 %4/06/00fto#0067,
tk
t~6mormrm
it�jw 03~gvapb~ery ~rl a. Fhika,*,6vxj-* I plane%
564714757,',
Utlkli di tribution Mortianafjnos-.~
Photoelectric observation
ci&AaractlD)rJllUCS Of thd',~-~
i6filbba tl f, tbb I ~ pf ent~jiklif~--T
~_mq pwp
p5no ba h
-p - otc%
-14,06 U, d I *
e4av i t(id tric
clod vo vc p wo! m
g 0MY4 M
-eri~wo~
a6z
1 --alametpitrahalt6 vwre- made foi:'~
)Iitudeol:*
1 VI elms

b _d
2,
dy-
T
"
'dbvi4 -b
,v
-for th 1:6661. S,

bd' W' bwbbfiv6tj~ Wcuy!k-. 00*~(*M #Oiji'w niti i2W b
PV~ ~0 bn -600
I
th Msible
4n, 9.. -
-j d"'
-for- AVIII. V
-V'% bu iev the
v Itig 41~6tlW
forn,,. 'Tbel conclusion Ardraft lhait Or~ Maitlail iiffinmphere has significant 1xite abB
orpta(
al w: Dxmd 3550 A. ut, hasv2 I.,MeB and 6 formudus.

MINN IN
YAKOVKIN, A.A,.q otv. red.; FEDDRO7, Ye.P., red.; AKSENTIYEVA,
Z.N,, red, BARABASHOV, N.P.., red.; BOGORODSKIY, A.F.,
red. 5 GOIMPTA, A,A., red.. I.K.p. red.;
rSEMAlr*,
KOLCHINSM, I.G.,-:red.; F.~' red.;
KOVALENKD, LD.j, red.
(Figm-e tmd. motion of the moon] Figura J. dvizhenle Luny.
Kiev, Nauk,.'-va durrka., 1965. 135 p. (MIRA 18:7)
1. Akadertd-ya nauk URSR, Kiev.

KOVAL "I -t- E A.
_ ~'.K., otv. j A.; KOVALliKO, L.D., re
[Problems iii astrophysics; study of the atnospheres of
Vemis and Nirs. Abstracts of the ra-ports) Voprosy astro-
fizik.i; issledovanie atifionfer VenerY i Flarsa. [Tezisy dokl.adov]
Kiev, Naukova dianka, 1965. 164 p. (MIRA 18:9)
1. SoveEbehimiye rabochey gruppy po issledovaniyu planet zem.-
nogo tipa) Kiev, 1964.

wvwmm~ m mm- a ZWMRAM~IEWUINE; luu~ffljnl~j~
77756URCE 05697oo Fcp,~5
of'Ov btightne a2
ifthiii -Oohotoig distribution over the disk of
I
R W331MV.SDURD aj-i6_i~~;tviniayur, oi
In 31A i j5s 19659 iommth
~3191 mart .'L
-P1Sn4t'~7_e1PU_ In, h nos~,'.._Gauac tin iutttlb~Uont atmosphere photo
TO* t kiord'. Ag t d
"TRUSUTION U: ~b' atti h~t t: In made! i1jo cbrrat~A:-.0bae, rved cuives of the brightness distri-
thp-~disk'oi forAbe entk~e'.set of - diatcirtions caused chiefly by the
6i -lose pmvp -Be obsen;utions of Mars and-stars by
a$ lparallel
th, i.l. inethod or, ib _16xk6,~"a -r"jg' were begun ir. 1965 at the Main Astronomical
n
&"ALWrom reflector. The
p-rofilen obtaixiedi. fu*a Wi orwit-iow ~ are well approxbmted by a - Gaussian-
dilli0ibul4on,:, This raaiilt, ~"aa UNO'd1*r mi apprtuKiinate correction of the photoelectric
prof ileir, ~of Yhws obtaiin~d:: in the M~Powpmtiwof :L963i., Par - r. rater with 6oo
erg
tho'corrocted curve U'r th9,,iI6orw.,vo In trAghtness toww-d; the limb ban a shape that
is 610811! to -VM937 (1 ;4,1 the "jqao "a ;1~ncidenco of tka solar rays)j, irwtead of the
Ld X4',,
3

WIMM
PLkKSENKO, N.A.; ROVALI, I.R.
Characteristics of the distribution of imprity elements in
the rockli of ~J.Iiceuus-ferruginous formation of the Kursk
Magnetic Anomaly and their ganetic significance. Dokl. AN SSSR
161 no.l:,.2104.'13 Mr 165. (MIRA 18:3'1
1. Vorcn(3zb.skJ.y gosudarstvennyy universitet. Submitted June 8,
1964.

ACC NR,
AT6033321 SOURCE CODE: UR/0000/66/000/000/0018/0030
Avmoa: Bugayenko, L. A. - -Bugayenka, 0, 1.; Kovall, I. K. Morozhenko,
A. V.
ORG: none
TITLE: Electrophotometri.c sections of the Mars planet disk in thespectral range
of *,:he 355-600 rn/.,;..inter-va1
SOURCE: AN UkrSSR. Fi,,,,ika i planet (Physics of the Moon and the planets) Kiev,
Naukova dumka, 19-56, 18-30
TOPIC TAGS: Mars planet, star, Mars, brightness distribution
A13STRACT: Electrophotometric sections of the images of Mars and of some stars
sttuated at a small angular distance from the planet were obtained with a'70-cm
reflector at the Main Astronomical Observatory of USSR in 1956. The information
now being published represents the experimental part of an investigation aimed at
correcting the brightness distribution clarve along the disk of Mars by calculating
the influence of factors in the earth atmosphere. The authors thank.Z. Merkulova
:a rd- - -3. / 2
KC NRs AT6033321
and. V. Pipko for their assistance in calculations. Orig. art. has; 5 figures and
3 formulas. [Based on authors' abstract]
SUB CODE: 03/SUEQV1 DATE: 19Mar66JORIG REF: 017/OTH REF: 003/
LCc,rcj 2 / 2

ACCI
8R' AT6033322 SOURCE CODE: tIR/0000/66/000/000/0031/0044
AUTHOR: Koval', L X.
iORG; none
TITLE:: Position of the maximum brightness on the disk of Mars
SOURCE: AN UkrSSR. Fizika Luny i plan.et (Physics of the Moon and the planets)
Kicv, Naukova dumka, 1966, 31-44
TOPIC TAGS: optic brightness, planetary atmosphere, Mars planet, Mars
atmosphere thickness
ABSTRACT: The rfa.SUltS of the photometric processing of several photographs
o-f the 1..-)Ianet Mars, obtained in 1956 for several phases along the equator of
intensity, are given. It is shown that wj,th a decrease in the wavelength the o~tical-
br,ghtness maximum shifts from the subsolar point to the limb. In the case of pure
scattering, the optical thiekness of Mars' atmosphere and the surface albedo for
blue and green rays (429 in,,~and 530 rn /,/- ) are estimated for spherical indi-
catrices on Lambert's ground, In the caiie of pure U11 diffusion, there is no agree-
ment between the theoretical curves; this indicates the existence of true absorptionf
Lc~,,d 1/2
ACI: NR% AT6033322
Orig. art. has: JC) figures and 2 tables. [Based oil author's
in -the spectral regioi:i
abstract]
SUB CODE: 03/SU13M DATE: 19Mar66jORIG REF: 0'03/OTH REF: 002/
2/2

KOTIL, F.-
Disnertation defended f*r the degree of Candidate of Agricultural Sciences
at the Institute of Foroat and 'flood; %'Idberian Branch
"Role of the Pine Tree .-1,n Increasing the Productivity of Low~-Bonitetic Oak
For-Dsts of the NorthwesG Caucasus."
Ves1mik Akad. Nauk, No. 4, 196), pp 13.9-145

KOVAL I PI.P.
.Si3vicaltural.cconordo evaluatlon of some types of oak. and
pak-pine forests in the northiamUrn Caucasua. Trudy Inst.
lesa All GrUZ. SSR 10%205-214 162. (MIRA 170)

BELENIKIY, Dmitriy Mikhelevich; KOVAL', I.V., ved. red.
[Main conveyorts] MagistrallMe konveie:ry. Moskva, Nedra,
1965. 220 p. (Mln 18: 5)

SUSI-v,ERJI M., prof. dr., DrSc.; C'SARIX, A.; HAVRILA, L.; KOVAL J.-
DINKOV, J.; J.111LONICKYS.; s,rOLITA, J.; SVATY, I.;
ZRIJBEC, P.
Incidence of scleroms. in eastern Slovakia. Cesk. otolaryng. 14
no.ltlCI-13 F105.
1. Ortoryngolos:icka. klixiika Le-karskej fak-ulty University P.J.
Safaril:a v Kod.ciacb (prednosta: prof. dr. M. Suster, DrSc.)
a ORL ciddelenia Obvoclyiilio uvttivu narochillio ~dravl, Presov, KoOcc,
lhmwino, Spiv!~Va Nova 'Teri, Michaloveo, Poprad a Roznava,

KOVAL, J.
Unusual Ca8e of foreign body (raw potato) in the pharynx. Cook.
otolar. 6, no.30.44-145 June 57.
1. Otolar7ngologicka klinika UK v Kos Iciach, predzilosta doe. MUDrs
Miebal Suster.
(PHAMM. foreign bodie"
raut potato, surg. (02))

SUSTER, M.; JUVRILA, L.; KOVAL, J.
Course of semore esophAgeal wounds in current combined therapya,
Cesk. otolaryng. 12 no.6:37NM D 162.
(ESOPHRGUS) (ESOPHAGITIS) (MEDIASTINITIS)

KOVAL. Jan, inz.; SLA'VlKp jMmj inz.
Possibility of ualrig acetio aoid for wood delipification.
?apir a oelulosa IS no,llt,'O,'15-~216 N'63.'
1, GeskoalovBmska akadomie ved,, Chemioky ustar Slovenskej
akademia vied, Brctishiva.

ROVALI, _L-A.
Selection o:~ forrulas for computing on calculating machines
errors caused.by the effect of relief in gravity prospecting.
Izv. M, Kaizift. INIM Ser.gfiol. no.2:120-3,24 162. (YIIRA 15:6)
(Calculating machines) (Gravity prospecting)

KAZHKINA, A.O.; KOIAW.. L.A.; LYAIIPICHEV, B.I.
~-Ili~--
*Eleotron mathenatice" im the service of geophysics. Izv. P14
Kaza1h. SOR, Serogeol. mo.)tloo-101 162. (MIFLA 15:7)
(Electronic calculating machines) (Geophysics)

-41
Ay1w.60"
NV
Fbf 4'04WE dixtj ..a -gra
irjmstrio sur
-19
~Idldifii -7sb -17
173 7-,
th
can ai computers; hence, a clues-
jid
in bzt'o '-~:.theimq e-isary radius 'for calciulating I
~C
".Ps. of this 6 Of reliat.. w4wh "H
r us,-s iorl :r
ort 06t, or the~drrecVbr rP7
o 3o ihd b0ii~dc~iOn I'pr tho~attraction ol'. tha:-
C~i6n) i F It~.isz-propoui~d to-c al Ie 2zte
the effects.
in. whipb.*-tl~e- Attl.-actUn of the -intemedJA -Ia
he ~t4~h: mwt;~ be: a en leratio
t into.consi~
conditions
7
"J~

-tb-
, M'
ell V.46
On I bliu
ou
~,t!r the. rad -86 o, to;
rac
yl
-Wun
-S
Rt
4 P
tA
-it
0:
!6E
25 tm
"s

GIC)INA, Yu. V.; SOFRDSIYNK')V, A. F.; KOVAL', L. A.
Wear resistance of --.ombined coatings under the effect of
hydro-abrELsive friction. Izv.vysoucheb.zav.; chern.met,7 no. 4:
124-128 164. (MIRA 17:5)
1. Sibirakiy metallurgicheskiy institut.

-ACCE.'ZION n: AP403Y104
S/0148/64/000/004/0124/0128
AMOR: Grdinaj, 'Cu. V.,; Bolrosheakov., A. F.; ICo L. A.
TITEM: Resistance of Ocabired CoatinEp During Hydrodbrasive Wear
son. CIE: IVUZ. Cha=ayu Metlauurgiyap no. 4, 1964, 124-128
TOFT" TAGS: difftsion Laye-*, heat treatment, hydroWbrasive wear., calorization,
titanization,, chrome pl.31ing, siliconizing
AM;TRACT: In an earliez pa,.,?er the authors investigated the properties of
diffusion layers pr&1uc,.-d b,-(COjTb'h7gchemical treatment with heat treatment, and
they continue their 1researd'a by reporting additional test results. Slems,
ch4kers and segraents vere exposed, to hydroabrazive vecx. The treatment consistee6
of calorizing (9150-10000 C) for 12 hra, titanizing (1080 C) for Id hrs.,
sia~ -conizing (1030-1100 C) for 11 brs. and chromizing (3-150 C) for 8 hrr.. All
pall:;s were deveaseft and nitrided at 500-550-520 C for 70 hrs. The
airt,1'Lors found that vew, resistance depended not on),tr on microhardness but also
on microstructure, brittlen ess of the layer and . te at conditions In Wnich Pulp -
an,1 coal lines aa well as Lot steel runn rs were. simulated. Although the method
Card
1/2

Accsssiw Nit: AA033704
appears somewhat complIcated., it is rea=mended for many parts exposed.to
hydrosbrasive wewr. OrLS. art. has; 4 figures and :2 tables.
ASSOOLMON: SibirsIdy matfLUurgicheskiy institut (Siberian Metallurgical
Inatitute)
SUMITTED -. 08Jui63 ACQ,: 07May64 ENCL: 00
MM ["ODE; IA. NO BW COV; 001 OniER; 000
'Card 2/2

Iffect of prolonged administratIon of qualltatively different foods
on periodIceLl votor function of the small intestine. VOp,pIt. 1!j
no.20-1.1 Ni-Ap 156. (MLOA 9:7)
1. Is Institutih fiviologil Kiyovskogo gosudsrstvennogo universiterta-
Imeni T.G.Shevchenko.
1"INTMOM' SKALI,
off, of food of varlous typ*s on motor funct. (Rum))
11POW) effects, I
an small. latest-twil motor funot., off. of prolonged
aftin. crf varIcas foods (Bus))

JUM
ICDVALI, L.A.
I - --.- --e
Role of aoeiqlchollne and adrenaline in the motor regulation of the
small lutesMne, Nauk np, Kriv. un, 16 no.17;103-111 '57.
(MIRA 13:2)
(AGETIMOROLINk) (ADRMLINX) (IMISTINICS)

KOVAL', L.O.;.1Q13R0VOL'SKArA,.Z-0- LDobrovollslkat Z.0.3
Comparative aharacterietiat of the e-!fect of acetylcholine and
carbochollne on the MDt'Dr function of isolated sections of the 11mall
intestine. Muk zap. K)rlv. an. 16 no.18:83-88 157.
DURA 13:2)
(.ENTFST.EM) (GHOLIIM)

3(X4LOH, P.G. [Bohach, P.H.h, KOVAI'Al. )~.A. [Koval', 11-0.1
Mechanitim of reflex influenoen from tho rectum on the motor
activity of thn emall intestine. Fiziolahijr. [Ukr-I 5
no-3:329-336 Hy-Je 159. (MIRA 12:10)
1. liaukovo-doslidnir institut fiiiologii K!Llvslkogo derzhuniversitetu
im. T.G.-Shoirchonka, viddil fissiologli travlenrqu i krovoobigu.
(INZESTOES-IHMMUTION)

17 (.-z' 4)
" SOV/21-5 9-7-2 5/2 5
A U T!
16R: Yovallp 1,. 0. (Kowai'L

TITLE: Action of .1drenalin and Acetylcholin o-P the Blood on
the *Kotor *Tunction of the Small Tntestine Through
the Central 7ervous System
PERIODICAL: Dopovid;i Akademli Nauk Ukrainslkoi RSR, 1c)59, 1qr 7,
pp 806-810 (Ukr9TR)
ABS-ITRACT: On introducing adrenalin into Vie isolated blood
Istream of a dog's head connected with the body by ner-
ve connections only, tl-e motor. activity of the intes-
tine io ir-.hibited (1-at-ent period of reaction 20 -45
seconds). After the inhibitory phase - second, exci-
1~ation phase sometimes Sets in. On introducing ace-
tylcholin into the blood stream of the head, inhibi-
tion of the intestinal motor function also sets in
rr from t1lese date, and tile
afte3'10-120 seconds. Proceedin
t
:7esi)ltrz of experiii-:ents on stimulation of the vagus
nerves on a back~-rourd of the inhibitory T)hase after
Ca-d 112 introducing acetylcholin ~,efoTe and after adrenalec-
tomy of animals with a crushed spinal cord ard severed

SOV/21-59-.7-25/25
Action of Adrenalin and Acetyl.cholin of the Blood on the Motor
F,..inction of thie Snall Intestine Through the Central Nervous Sys-
tem
vagus ne3-ves (with undisturbed circulation) the mo-
tor function during the second phase of acetyloholin
action it, effected Rs a consequence of the action of
the lattcr through the central nervous system e,nd the
influence of the ndrenalin of the adrenals. T:~Ere are
3 diagrams and 4 references, 71 of which are Soviet
and 1 'Freach
ASSOCIATION: Yaukovo-doslidchpy instytut fiziolohiyi tvaryn pry
Kyi-trs)t:omu derz,-.iavTiomu universyteti, Scientific-Re,
search In:-3titute of Animal Physiology at Kiyev
.1
Dtate University)
PRESENTED: D.S., Vorontsov, Member AS UkrF'):,R
SUBMITTED: 'Pebrunry "), 1959
Card 2/2

EDTAL L.A. [M)val 1. '6.0.:P
Iffect of acet',rIchelins and adrenaline on the motor activitY
of the tivall Intestine as related to functional atato and
age. YI.2iI,ol,,zb1xrjIk-rj 6 no.,W13-220 Mr--Ap 160,
MU 13:7)
1 Inst!Ltut fl lisiolog-11. shivotzfth Uysivskogo gosudaretveun)go
Qiverslteta Ain. T,,G*- Meychouko. otdol fixiologii pishcheva-
reuiya IL Imovotibravitcheniya.
(irritsvims) ('(MOLnM) (AMMULM)

KOVAL', L. A.
Cand Biol Sci - (dios) "Role of adrenalin and acetylcholine
in the control. of the motor function of the small intestine."
Kiev, 1961. 1.8 pp; (Academy of Sciences Ukrainian SSR, Div-
ision of Biological Sciences); 110 copies; price not giveh;
lisl,,; of author's wo.,~ks at end of text (12 entries); (KL, 6-61.
sup, 20?)

MALI, L.A.
t- I -!,- 1.1-11 ~, -11.
Uao of olectroido computers for cUculuting gravimetric terrain.
Izv.All Kazakh.11-SR. S(,r.gool.i;,auk no.4.96-10-7 163.04IRA 16:9)
1. Kazukhsldy -,~31itukhnichesIdy institut., Alma-Ata.

KOVALI, L.G. [Sovall, L.H.]
Zooplimkton of tha nortliweistem part of the Mack Sea. Nauk.
zap. Od.biol. sta, no.3127-4)'~161. (laRA 16:6)
()MACK: SU-ZOOPLAIUMN)

KOVAL', L*G.
3001410"bbhmateristice of the development and distribution of
sooplankton in tho northwestern part of the Black Sea. Vop. ekol.
5z98-1C0 162,, (MM 16:6)
1. Biologicheakaya stantaiyet AN UkrSSR, Odessa.
('Black Sea-Zooplankton)

~Ww I - , --- - - - ---
J'Kov-a:ll, L.H.)
Zooplmnkton of Festern Sivash. Pratsi Inst. gidrobiol. AN USE
no*35;41"49 160, 0 (MRA 14:4)
1,Sivash-4ooplankton)

VwMal.
KOVAL' I L Novallp Tj*Ho]
t9a.-I
Zooplemktan of Iake Molochnoyea Pratsi inst. gidrobiol. AN UBSR
no.35,138-,W! 160, (MIRlk .14: 4)
(;olochnam, Lake--Zooplaz&ton)

KOVAL I. Ley. Milchal ch; YAROSTAVTfEV , Boris Alekseyevich; GUROV I S. I
- RX.L
red.; KU7,NETSOVA,, A.., takhri. red.
[From small-scale to over-cLU mechanization] Ot maloi makha-
nizatsii - k komplekanoi. Moskva., Mosk. rabochii 2961. 202 p.
NIRA 15:2)
(Assembly-line methods)
(Moi3cow-Electric machinery industry)

KOVAL I I L. M.
Modernizing the c:~uutch of the hydrau.Uc drive of a press.
Mashinostroltall no.8:14 jig 162. (MIRA 15:8)
. (Powor presses-Hydraulic drive)

KOVAL', L.P.
Scientific:and teibnical conference at the Volgodonsk Combine of
Synthetic Fat Subititutes.. Masl.-zhir. prom. 27 no.9:48 S 161.
(MIRA 14:11)
1. Vneshtatr*~y koi~respondent zhurnala "Masl.oboyno-zhirovaya propor-
shlennost'".
I-Oils and fats) (Acids, Fatty)

XCIAL v 9, M. A.
EOM'.. M. A. - twntgeno-Van *graphic Method in the braluation of the Changes of
t1us Permeability of the B1wd-C-,,m7IW Vessels in the Aresence of Inflazmation,
Olqvrimental-Clinical Invoutia ation). w Criwan State Had Inst imeni 1. V. Stalin,
Slisfera poll, 1955. (DinseriAtl an For the, Degree of Candidate in Medical Sciences).
SOs X izhm-va 3 Seytegber 1955
9.

M.A. )-and. mod. wift.
Roentgea vasographLa date of vascular changes in experimental tubercu-
lous inflammation. Vest. rent. i rad. 33 no.6:22-28 N-0 158. (MIRA 12:1)
1w* Iz Ni!kuah-ao-lasli)dovatellsliDDgo instituta travmatologii, ortopedii,
i protezirovaa~ra 3. Stalino, (dir. - kand. mad. usuk. N.V. Novikov).
(TUBER.3,19IOUS, exper.
-rase, changes, angiography in dogs (Rua))
(ADIOUIMPlY
in t1bera., determ. of vasa. changes in dogs (Ibis))

XOVA11, M.A., kand. 'Mail. usuk (Talta, ul. Voykova, d.10); VLASOV, I.V.;
ritaka,ra, A.A,~
Use of vaisography In inflammatory diaeasou of tho extremities. Ncrj.
kh1r.arkh. no.5:68-74 S-0 '59. (MIn 13:3)
1. Xhirurgichoaklye ctilelen1ya Alushtinakoy gorodskoy bolinitsy I
Yaltinskoy gorodskoyibollnitay. Nauchnyy rukovoilitell - zaveduyu-
shchiy kafedroy fakul:ltetekoy khirurgii Krymakogo meditsinekqgo
instituta proJ!. P.P.1,;TSaran1ro.
OmMgKITTXS,~ LOWER) (ANGLOGRAPHY)

KOVAW. M.M,, inzh.-makhanV.-
~I ?
i
Universal tractor-m')unted loadler. Hokh, oil' , hoop. 9 no. 8;3 of cover
Ag 158. (MIRA 11:8)
(loading tud unloading)
C~Igrlcultural machinery)
i~

N
B011DARENK0. M.G. C.Boncl3renko, H.H.]; VORONHZHSKIY, V.1. (Voronezhalkyi,
V.I.]; KITITTSTA, Z.P.; KOVAL', M.N.; KOLOPA, V.D.; KaLSMOY,
0.0.; MOMINSEATA, Te.D', Cjtj~' ?""At D KMA, G.H, [Kukta, HaM.1j
inzh -qmkhan.; PIVEYVAR, S.G. [Pivovar. S.H.J; SOLOVET. V.I.; OIJWI-
;Zi;, G.A. Mefiranko, H.A.1, red.-, GLUNKO, 0.1. (Hulenko, 0.1.1,
tekhn.red,
(New agricultural machines] Novi sills1kohospodaralki mashyni.
Kyiv,-Derzh.vyi-vo sil'alkohospodaralkoi lit-ry URSR, 1959. 231 p.
(MI1RA 13:4)
(Agricultural machinery)

KOVILt.? H.. F., Engineer
"Nev Principles for Designing the Genaral Layout of Heavy Machine Building
Plants (Wi4h a Gentz-alized, 'Itore shouse of Basic Raw 'Materials)." Sub 25
Jurt 51, moscow Order of the Labor Red Banner Construction Engineering Inst
imeni V. V. Kuylayshev
Di,~sortations presented for science and engineering degrees in
Mom:= during 1951.
SO: SUM. No. 1480, 9 May 55

KOWLIII H.N.. karid. tekh-ri. ni-mik.
Joint upeirational toOmnlogy of IndustrilA. ifator, and railroad
trannport. Zbel. dor. transp, 14 no,2t3R.42 7 158. (MIRA 110)
(Trunaportation) (Railroads-7relght )

KOV)W, M.N., Ic9Lnd.tekbn.nauk
Drawing up general plans, for beavy industrial plants in
connection witb water and rail supply of raw materials.
Trudy 14IIT no.105:243-287 158. (MIRL 11:9)
(Material handlirg)

~ =~lm - - - - - - - ~Ml
MVAL', M. P.- Maqt:cr lltat Sci (diss) -- "rite fauna a-ad"cellulusolytic llct-~'vfty
of the in-`Lcrol~lora 03-. scars on cows". Leningrad, 1.959. 1.7 pp (Leningrad V,:!t Inst
of the Ain Agric USSR), 1-50 copies (KL, NO D, 1959, 11.0)

mummill"m
EMMUMN
UBE
dyopepsiff of calves.
Veti~rjnariia (Mlffik 18.-6)
1. Qrodn.,~rxk'iy 5nstiLat.

M.P., kand. viateir. i;auk; WiFlKO lovo
Caiis of carbamle18 pofecn-!~ng Ln 4-, Pc
0 164-
1. Grodnenakiy
2. Glavnylr valt~tdnaxiVy at"arAsit y-o b-:2 tl>--A bolnz-~,-Exi
zhivotnykh Grodiens)ugo
Vas I ko) .

VTASEENTSKIT, Dtaitrly Wikolaiyevich (Stmehevs1k7l, D.,K.1; KOVAL, X.T.,
red.; RXIOMINA, M.3' , takhn.red.
siga:flcance
(Interuational
of the seven-year plan for the
develolmient of the Vational cicononiy of the U.S.S.R.] Klzhna-
rodne zziacham&La somyrichubho -planu rowvytIm naroduoho hospo-
darstva SRS:. Kyiv* Tyd-vo Akadinauk UM, 1959. 72 p.
(KIU 13:3)
(Russia-loonomic policy)

GjW.jHA. Ivan Poidoh [Hsnzba~ 1.1h.3; JEOVALI, N.V., rc.)d.; BUIT, R.O.,
tekhn.red,
[First collective farm in Out Ukraine. 1917-19201 Pershi
kolektyvai hospodaretva na Musaini. 1917-1920 rr. Kyiv, Vyd-vo
Akad.nauk URSR, 196o. 154 p. (MIRA 13-9)
(Mcraine-AgricuLture, Cooperative)

7 ------
1 7
E W? Lr d).
.KWA(41& ovw~tvmw /M
AP s'AP
0040/0043
60-00610 iSOUMEwCODE.- UR/0129/65/0iWoli/
-IKOVA1 y
OR -is~i',~~Oiik6poll,ikiy.~uzhixotrulm;iyy zavod)
G .,'Nikotooll Southern Tuh~e~v
_7
Ef 1' et of temperature -ind itte of heaking on rbe'&ri!41n sizelof Khl8Nl2*,r steel
e
SOURC.R~.- Mttalloveideni~e: I ob Iri;obotka nekallor, not 12, 1965 40-43
4A gr'alnaize~, st-sel '~'UMV antun,heat vrent, furnace/
TOPIC GS:
XMN.Lif steel
A] knnulii #~iclmiiis' -of khl,)jU2t stegil (0.08% _0.01~z
1.411% Mn. 0.66% Si,
0 66 7,",,"6 -1. ~ 1~z 11439%!' ;Ti),
NJ. 0~ 3A wt from cold-rolled boiler superfiester
tube4i,*,,; imrij he -i t-860-4260C, o:ii:~ neiressing.,-the temparstureby,50-10VC at a time*
for_~ 3 i!~Az, -and; air-cool4d,: with thi'~vobjowt- 4 4erternining7 the conditions under
ir Wm6g'snei ty eah,: be maxitilied'.t h
wit the use of different fur-
Aa r6l'
.in uctiosk, b6z.
d lcpntljq~ leir) showed ihot the most suitable fur-
nad4A*6i_tk1s * -purpose, to ~thw cintintwus iollc'ir ~futvaxe, -(fuiaace -length 10 a, travel.
int. rill'te aftubes 6.4 =)'uin,; tim4srfiiure~ 12(Ki-12300c) ~ The 'higher the heating rate,
the highat is: the mad '. to obtal U *.roughly id
temperat antical grain.size. In
additf6n, the' affect OUTN
C a q&x* v*s investigated 4ra specimens of work-
hardattod w'6#4 ircu twa~Wjt~ Aubdvw d triiji speciians of Ti-free OHM steel;
cakd~,j
-/2 JOB6421.785.16j620AS&S

Moldavia's produott on the Internatiolial wirket. Vnesh. torg. 42
no.9:44-45 162, (KERA .15:9)
1, Preideselatell Gcoudarstvemogo planovogo komiteta Saveta
Ministrov Violdavokoy SSR.
(Moldavia-C=merce)