SCIENTIFIC ABSTRACT KLIMIN, I.K. - KLIMKINA, N.V.

• Document Type: CREST
• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R000723120008-8
• Release Decision: RIF
• Original Classification: S
• Document Page Count: 100
• Document Creation Date: November 2, 2016
• Document Release Date: September 18, 2001
• Sequence Number: 8
• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT

Yertillsers and Matures
sowing onion seeds sized with groaxaated superphosphate. 9M I og. go. 1952.
Month List or Russian Accessions, Library of Congress, gone 1951, Unclo

MDMj Lop inshenerwpilot
. ......................
"MOOlght rOquirfs bml*dP- GM&W.&T, 18 no.2s7-9 7 060.
("lanes- Piloting)

AID P - 521
Subject USSR/Engineer"
Card 1/1 Pub. 93 - 8/12
Authors : Kozenkovp N. S., Engineer, Klimin, L. A.
Title ; Rod-shaped yokes for suspension of wooden beams and
joints
PeriQdical : Sbor. mat. o nov. tekh. v stroi., 6, 22-23, 1954
Abstract Rod-shaped yokes made from round steel bars for
suspension of wooden beams and joints are suggested
for ceiling construction. Diagram.
Institution : None
Submitted : No date
-7.7777F
7 T
7

KLIMI L OCRINq A*P.
AntmatLo fwl~consmptlao intor, Avi.proms 29 no,lt29-30
JA 163. (XMA 16ol)
1. OllyanowskLy avtos&vM.

KILOV* G. (Loninpad) I IMMIls To. (Leningrad)
was to increase productions Promkoopo 12 mo*12110 D
WBA 22 t 2)
Is Predmedatell pravlenlys arts2l xUlltigrusbW (for Kilov)s
2, askretail partlynoy orgalzateli artell OltditipushkRO
(for Klimin),
(Lentopsid-Toy Industry)

OWMA. Eduard Iduardaylah,, pror., mmiNA. P.r.. red.S ERMODMIMs
A*A*O Ukhn,red,
(Aketahas of the development of Mberian agricultural Ocherki
ratiltils sitirskogo assledellis, Omsk# Onskoe oblAnIskines
lsd-,ro. 1957. 105 V. (KIRA 1323)
Is Deystvitalln" oblen. Omakogo atdala Tessaynnogo geogrefichaskoso
obshchasiva pri Akadsull nank BM (for Osshelo)s
V
iN
R14

WT
KROKOMO, Tyschaslay Androyeviob: 111MINA. ?.Y.. red.; IM
Oontinuous-operst ton methods and automtlzation constitute the
moans with which to Increase la'bor productivity] Potookays
rAtody i avtomatLutella - reservy povysbanlia prolavoditall-
nostl trudao 'Ouskoe ablAnIshnos lid-Too 1958, ?0 p, (XIU 12:6)
(Omsk--Ubor produotivity)
ARM
mr-MA'V

OR100ROW, bmill Pstrovichl ZLIXIU, P.rf* red.; KIL1111M. V.1.#
tokha.red.
[Chowdoal Industry In the Omsk loonesia Region] shislabo*A" pre-
sWablennost' v Cookm okonsulabaskou ralons. Om&. Oaskes lmisb,-
a" lsd-yes 2959. 27 V. NUA l3j6)
(Omsk Provinim-Chemical industries)

KUDRYAVT=p M&N,p kand, takhn.naukj,,XjjgM
[Designing automobile roads for varlous natural condi-
tionsj Proaktiroymde aytomobillmykh dorog v raxzWkh
prirodx,wkh uoloviiakhl uchobcas posoblee Omsk# Oeskoe
knishw,o IS&VO, 1962. ~ 67 p. (MIRA 17t5)

KAGANOVICH Vladimir Yorremvichp kand. tekhna nituki KUD.~YAVTSD,
M.N., profs# otv, rsdol WHINA.P.Fog r*d.
(Te*Wcal and economic substantiation of the variants of
highuW locationj a mamall Tekhniko-okonomichaskoe abostbo.-
Yanis variantov trassy avtomobillrqkh dorog; uchebnoo pova-
bi: Omsk,, Zapadno-Sibirskoe kr4sbwe Jad-va. Ouskoe otd-
nI ; 1964* 56 ps (Bibl4oteka student^# no*5)
1. Zaveduyushchiy kafedroy proyektirovanlya &vtowbjl'rqkb
dorag Sibirskogo avtomobUsno-doroshnogo Instituta (fbr
Kudryavtsev)#
.ifj-.~!~iff~
91-11, M

I22WIZVICRO L.A.p red.1 MILSITA,, Y.I,,p redoj BZVASTITANOV,, N.S.0
red.; )=Ip P.? rMe
L..
(I?ouWry prootlas &W beist, troata=tj Idtoince pnlxvW-
styo i fArplabooksis obrabotkao Omoks Zapadva-Sibirskoo
knisbaos isd-vo. Onko* otd-nis, 1964. 198 p.
(MIRA lSs6)
Is Omsk, PolitakhWobaskiy institut. Kafedra lVashizW i
tekbnologiya lit"go proisvodotya.0

7
Aft
reLitor; VIATIN, Z#T&., redaktorl -UMIXAJ[I,,T tekhnlchesk~'
.W -
redaktor; UL T*,T&., tskhn1che.-_ --&ktor. LVIN. U.S..
tekhniaheskly redaktor.
Cladustrial taxiseloa] Trodays velbohastva v Prov7shlennosti.
Part 1. -COronia substawool cressiouskie vesbobeetva. 1954. 810 p.
Part 2. Elaorgante and simple organic compoundel N*or&&n1ch4&k1& I
elementorgantaheekis s"dinsulla. 1954. 582 p. Isd. 1-&, para. I dop.
laningrad, Go#, neuchno-tekhn, Isd-vo khts, lit-ry- Luicroftlal
(Industrial toiloolog) (MM 7111)

--T~ v-
----- -----
i JNIU i IV L
BOGDMOT# Mel XOUJBUW# T*Aol IBUOTA, N.A.; 0ARMOVOT,, I.T.# redej
ZONIS, $#A## re4#1 IMIM9 Y**Y&*#
tekhao"de
(Analysis of the vroducts obtained in the -industrial prMarstion
of VivinA from butans] Analls produktow prolsvodstva divWle
In butane* Pod rod. I.Ye0arvanove. Leninsred, 0os.nanabno-
tabdia,lad-" kh1u*l1t-ry# 19." 115 WRA 13 12)
(Butodieve) ijutan*3

VASILITSVp Mel MIXWWV9 V,A,; NORMSKIrp B.1,; DUCHMOP OOPOP
starshiy rAuehqy sotrap k&W, tekhn, asuk, retsenseat;
MUWOVj I.Lp dots.0 JmWo taklo. uukp reteensatj
RMOOLID9 lu.A,p k&W. tekbne saukp dotsej retseamtj
BAYKOj V.F.p kand. tekba.mackj dote., nauebs" r9d. XLMUXA,
To Y. redal KRTAXOVA, DaMep Ukbno red*
(Automatic control systems for ships] Oudovye awtozatisirovari-
we ustanothe lAningradp Cox* solusnos Isd-vo, sudostroits pro-
aWshlop 1961& 5" p* (MIRA 15s2)
(Marino engineering) (Automatic control)

RIWIN, Samuil Sizonovicb; 0-clUCKUKH-OV, Ya.G.t inzb.,, retsenzent;
ShlVj E.Top doktor takha. nauk, reteenzent; CMTKOV,
R.I.0 doktor fix-mat. naukp nsuchn, red.; KLILINA ..j I
red, a V--- t
[1heM of gyroocople device's) Teoriia giroskopicheskikh
ustroisty. Loningradq OSudostroonle." llt,.2* 1964. 54? p.,
(MIRA 1717)

OKUN'p Toysey Livovichj ULAIRTAMWl M.N., retsensont; STMINIKOV,
MaTs reteensenti SHALINIKOV, Gal.# nouchno rodtj
NRYINA, Mal., rod.1 KLIMA,, To.V.j red.1 S&CHUX, N*A.#
red. I KVOCHXINA# O.P.
[Wio transsitting deviess) Radtopero"iushchie ustroistya,
lod.2., parer, t dop. Leningradq Sudostroanis 1964. 539 P.
191RA 17s 5)
Wdlu

XA.i1n1N-T,TNtfl, 4. - In.
w4mlauumcolo,;V cud Toxicology - Mu)12.-raput1c PrLiarati'mo.
..,,afitub,~rcuatla Dru&p#,
Abe Jour %hur Siol., no, 21, 19r.0, 98592
Author jaimina!~P~~-
Inst
Titl.j DpuvAcp or,Llqwr In QiUrvu M viUvTubirculous
uj,#n($iti* Tro~wd vit;i Str4tmvcino
Orig Pub -,A1rdv31wr. xazamisttm, 1953, No 1., 50-53
Abstract i On ~hj basis of a stuely or 120 cano historL:s oL^ c!*,1.Ux..;i
VIC) ou:CfQr;.A from tub~rc%xloms tu;nin4tia (TH), it -,,j eito-tri
V-at, in a omingaa ~~om aZ T41, during th, fi"-. 11-2
txmtas a certain incr,.=-~; o: cytosis wA prot,,in, azd later
a gradual dearmso to wrml, Is obscm2d, AemwJ.on of
liquor buoino on t1w vaiv;:% of trcatricnt. L% m;aLt,,P-
,-n*uVuaytIc cUA hydr-)cp:talic Come of TH, cytosm. a:vl
prortzins lawar graduaUyo ASsanation in unfavoreal.: cour-
s, of t1w procass occurs on tli~~. 6ux month, by proloz~~?*
Card 1/2
31

L
xux~ L440-- PON
Oass, of combined lob oulo" meningitis with mentrSitidee of different
etiology In childred"Iwith summary to French]. Probletubs 34 noo5o
52-54 14 1564 10111)
I, So detskop 014416stre (konsulltent -kandidat anditainskift usuk
YGSAo Tratlikh) lassi6skogo asuabsoatelledovatelskago tuberkalessago
institute (djr# - kmadidet zoaitsinskikh rAuk A.K.Zed"refths ass,
direktore po muckmay obsett- kandidat maditaluskikis sank T,,D.OrwA)
(TUMUM180 MINIALt. in Info and child
with meningitis of non-tuberce Wolf)
(XIM1101118P to Info and child
with tuberao meningitis)

KUKMXAYA, L.M.
Dyngimics of the corebrospinal fluid In children with tubercultus
meningitis treated with streptompin, Zdrav. Kazakh. 18 no.11*-53
(KM 1317)
1. Is detakogo otd6loniya Xtuohno-isoledovatel'skogo institute,
tuborkulosa Minsdrave, Xasl= (nouchm n*oyoditell - kwAidat
meditsinskikh nauk.Ys*Ae Oinsburg).
(MCNINGES.-TUBIUVLOIS) (CZMI(OSPML FMID)

KHRAPOVg A.T&,j MDAMt V*I.j Prinimal uchastiYs. KUMNSKITS-IsAs
Iffsot, of forromiliaon additions on the crystallization of magnesium
oast iron. Isy. vys. uohabe say.1 ii4terno wt. 6 nolOsl3&13d
163. (ftA 16122)
1. Sibirskiy matallurgicheakly Institut,
-4T
I AN. R
ISM i El

SHVATKAP O*?,v;W5U# G,P, -fKtmwwp N.P.)
Behavior-of oxasoles-In #me elsotrophillo substitution roeae
DoP6 AN-MR no#llo2479-240 165.
(IaRA 28s22)
It VossoyusW nauabno-issledovatellskly institut moookriatAnoy
I omobo abliotykh khtniobsokikh "shchesty.

WLAN, S.A.4, KLIMISHIM. I.A.
Dissipation of light In spherical nsbuUs. TSir.Astron.obser.
L'vIv.un. PP,P9:11-16 153 (NDIA 13:10)
(hebulas) (Astropbroics)

KAPLAHo So koo and KLIMMUM, I, As
Scattering of TAght in ftherical, Nebulas
A model of a sperioal nebula is designede Its optical radius exceeding
the geometrical ons# and receiving on its internal bouw1ar7 the luminow
flow of the central star, Assumilng the spherical scattering index to be
knowns the luminous intonsitr on the boundary is computed. The abstrowtor.
I. No Minine foww Was errors In the computationo MhAstro No* 90 1935)
TairknilAr Astrnnnm- Ohmrv- j&MMka_UDmf&, No. 270 19331 U-16
SO, so*. No. 744* 8 Doc 55 9upplementary Samy of Soviet Scientific
Abstracts (17)

XAPLAV, S.A.; KLIMISHIM, LA.
Density limits for wbits dwarfs, T51reAstronsobser'LITIVOun.
no* M17-22 153 (Min 13110)
(Astropiwales)

ILINISHIN, I.A,; IWNWANSM, AA.
Some r~ks on the pr"essing of visual and photographic obser-
vations of artificial earth satellites* Blul.staeopt.nablaiske
nut.Zem, no#3115-16 058, WU l3t6)
I# Lovoyok" astronoutchaskV& obsorwatortra, sUntsiya nablyndenly
IsIviestysAWkh gputaikov Zesille
(Artiflaial, satellites-Tr"kiag)

URLSIN# L#A,; KAWIMICOg 7,7,; ITAXINA, T.Ta,j 11IX
JWjj, I.A.:
MuTlycoza N.Y., =30, Tu.D., Ownluk, R.100
sotrudnik
Rsmdts of photograpblo observations of artificial eartb
satellitese Blul 9 staeopt onabl* I A *spat Us. no.6tl8-23
159. iknk 1316)
Is Sotrudnik Astroamicheskoy observatoril in* DWI 'prdtas
Xasan' (for Urasin). 2o BotruWki stantsil fotonsbWeAlya
IsImestiezWkh qmtaikov Isoll v likolayevskon otdel*nU GI&vW
astronoulchaskoy observatoril AN SM (for Zallkhavlcb# Ivakinz)*
3e fteballnik nablyudatellnoy stantsil Astronoulchoukay *beer-
vatorli Wyovskogo gowuniveretteta ln.lv.Ars~ (for 1ILmdsh1n)*
4e Uohallnik fatograficheelcoy stantaii CY?3 Odessimy astrono-
wicheskor observatoril (for Amos*),. 5* Astrononlebeekly Sovet
AN SSSR (for OtWrlnao
(Artificial satellltse-TraekluC)

KLIXISHIX IoAs
Graphio method for oalculating the visibility of artificial
earth eatelliteso W-Ot
3-6 '59o (XM 13:6)
lo L'Yovskays, astronoulabeslays, obserTatorlyal, stantstya nablyudonly
Iskusetysaw sptulka Zeall,
satelutes-Tracking)
rma -3"

15
30)
AUTHORS t
TITLEs
PERIODICAM
ABSTRACTs
IrAplAn, BOY/33-36-2-21/27
On the Correlation Between the Observed Differences of the
Degree of Interstellar Polarization and the Angular Distance
of the Correspondipg Points on the Celestial Sphere
Astromaiabeskiy shurnalp1959tVol 36,Nr 2,PP 370-371 (USSR)
By evaluating the data of Hiltner J'Ref 2.7 the authors ob-
tain approxinativoly the relation
,r-f 592409240
where to the seen quadratic difference of the de-
grees of interstellar polarization (in per cents) in two points
of the firmament, wA aL the angular distance of these points
frou each other, It is reservedly conjectured that this cor-
relation "a be explained by the turbulent character of the
intorstol2ar m W *tie fields,
Card 1/2

on the Correlation Between the Observed Differences of the Degree of Inter-
stellar Polarization and the Angular Distance of the Corresponding Points
on the Celestial Sphere
There are 2 referencest I of which is Sovietq and I
American,
ASSOCIATIONs Llvovskaya astronouiohonkay* observatorlya (L'Yov.
Astronomical Observatory)
SUBMITTEDs June 29 1958
Card'2/2

3(01100)
.AUTROBSt K&plan#S.A.t &nd_L11MIshinr1.A. 30T/33-36-3-3/29
TITM Sh6ok Waves In Stellar Invelopse
PIRIODICALt Astronosicheekly shurnal,1959.1ol 36,Vr 3,pp 410-421 (USSR)
ABSTRAM The authors consider physical properties-of stellar shock waves,
the possibility of separation of the envelopes ate. The shook
waves are assumed to by stationaryt at the other handi the tntsx%j
action with the radiation Is considered. 11 contains the
derivation of the formula for the Sugoniot-adiabatio curves and
other general relations. Because of the complicatedness of the
obtained system In the following paragraphs, the authors restrict
theaselyes to espoolally interesting speolal cases, �2 In devoted
to the so-called detonation-recombination shock waves in a gas-
radiation-sixturs (these waves move due to the enoirgy liberated
during the recombination of ions In the wave front). The waves
are described by the equations
X4(6r2-3rP2") . X2
[3r 2
(2-ft) + 6r,(#2-p,) + 8-3p,
2qq,
+ _P 2+1)2
(r
Card 1/3 1 + T12(r2+8_3h)0

Shook Waves in Stellar Envelopes
Card 2/3
2
P2 x 2+1 q2 (r2+1)1
71- ' 7 9 1.7 T I f 7r 2
2 1
2(x
4(4-30) 2 5/3
r
SOV/35-36-3-3/29
The indices I and 2 denote the values btforo and after the
passage of the ways, P. PI/P Is the ratio of the gas pressure to
the full pressurej q Is the set of nascent *nergyO v Is th*,C"
velocity with respect to the front of the wave, 9 Is the density.
The system Is solved 'by successive approximation# where the faotg
that the detonation-recombination waves are weak, facilitates tho
solutions In �3 the conditions are found under which a separation
of the outer part of the envelope of a red giant taking place
with a small velocity to possible. An undisturbed separation of
&a suvslops mass amounting ca. 1073 -Z*10'5 solar masses Is
Possible e.g. if the rA4ius of the giant Is 80 - 100 times
greater than the solar radiuso the mass of the giant nearly,
equals the solar mass and Its absolute magnitude Is -4 or
.51NO. The velocity of the separating part to 50 ka/5400 the

shook Waves in stellar Znvelopes SOV133-36-3-3129
velocity of the *book ways 110 ka/sea. The place of the
separation lies nearly In the center of the radius. �4 treats
the influence of radiative cooling on the parameters of a shook
ways. It is stated that this Influence is essential even at
optical depth# of ev 30 and that it leads to a 10 - 100-fold
diminution of "he temperature behind the wave. '�5 Is devoted to
the properties of shook waves in a degenerated gas.
There are 15 references, 12 of which are Soviet# 1 American,
I English, and I German.
ASSOCIATIONiLlvovskaya astronontoheekays, observatorlys, (Llvov Astronomical
Observatory)
SUBMITTEDs Juts 2# 1958

KLIMISHINO I A, t CAND PHYS-MATH $0.11 "SHOOK WAVES
AND ULTRAION:C CURRENTS I" ENVELOPES Of STARW Kiev#
1960* tMin oF HIGHER AND Sao SPEC ED UxSSRt Kiev On-
Can or La"im STATE UNIV.im T. 0. SNEVCHINKO)* (KL# 3-610
204)0
52-,

5/124/62/000/006/009/023
D234/D308
AUTHOR:
TITUt shook waves in stare
PERIODICAL3 2eferativnyy shurnal, Xekhanika, no. 6, 1962s 131 ab-~.
atract.6% (Tairkulyar. Astron. observ.,Llvoyak.
un-ta, 19600 no. 35-360 31-42)
TEXT: The author oonsiders the propagation of a shook wave in the
atmosphere of a cold star and the possibility of the shock wave
tearing off the 'envelope of the~star. The posoibility of the-for-
mation of a planstary.nibula as a result of such tearing off-is
viewed. A,preliminary review'is made of papers devoted*to the
problems of XWfaltion of shook waves in stars, flares of now
stars, gas dynaml solutions conoerning the motion of a shock wave
in a gas with density deorissing with the radius according to a
power law. The problem is studied with several simplifying assump-
tions. In the equations of hydrostatic and radiation *quilibrium
for the envelope the mass'and.the luminosity of a sphere with:ra-
Card 1/2
Nor-
-7-
IT

3 84 IL
3/124,/62/000/006/007/023
D234/D308
60
AUTHOR: Klimishing Is A.
"i'ITLE: Supersonic flown in transparent envelopes of stars
P'.4'RIODICALi Referativn y zhurnalg Makhanika, no. 6, 1962, 12, ab-
stract 6M (Tairkulyar. Astron, observ..Llvovsk. un-
ta, 1960, no. 35-36, 43-47)
TBXT: The problem of stationary flow of gas from the star Is con-
sidered. It is assumed that the energy radiated during the motion
is not absorbed by the envelope but escapee unhindered into spaces
An estimation of the absorption according to Kramers, formula
shows that the envelope is actually transparent. An equation is
formulated which determines the variation of the velocity of a sta-
tionary stream with distance. In order to assign the velocity of
energy lose, the hypothesis of local thermodynamical equilibrium
of the gas with the radiation is used in the first approximation,
It is assumed that the temperature decreases with the radius, ac-
Card 1/2

3/124/62/000/006/007/023
Supersonic flows in D234/D308
cording to the law T T070"where T temperature at the radius
ro, qL= r/ro. Solutions are obtained for the velocity v(t) for va-
rious values ofe-X. For c~= 2 and 3 the equations are solved nume-
rically. It follows from the oalculations 'that during'the motion
of a gas jet in the transparent envelope of the star the jet is
~accelerated. The acceleration can lead to an increase invelocity
to 10 - 25 times the velocity of sound c0 at the point r. where
the acceleration begins* If co a 37 km/sec, and 0(- 2, the velocity
o4'
gas at a distance 2#5ro from the center is equal to a proximately
450 km/sec, ~-AbPtraoterl a note: Complete translation._
Card 2/2
10
OF

3. 1530
AUTHORS:
TITLF.i
PERIODICALt
ABSTRAM
Card 1/4
78002
."0V/33-37-1 -2/31
Xa plan, S. A., Klimishin, 1. _A.,, Mvero, V. H.
ott Seattlei-Ing In a Wdlufn WIth ti Movirig
A Thcory or ur
Boundary
Autrotiomicheskly zhu*rnal, 1960. Vol '37, Ur 1, ,PP 9-15
us sn)
When the motion of a gas tinder cosmical conditions In
considered, It is frequently nccc3aary to take Into
account its Interaction with radifation. Unually, the
problem in studied by combining the equatlona of motion
with the equations of radiative tran3fer; moreover, only
the case of a steady boundary in considemd, while
actually the scattering occurs either before or after
the light quantum passes through a moving boundary.
Consequently, before any modern theory of light acatter-
Ing In applied to hydrodynamic problejn3 It ij necen3ary
to develop a theory of scattering In a medium with
moving boundaries. This Is the problem of the present
authors. The following notations are uned: k, the

A Theory of Light Scattering In a MediUm 78002
With a Moving Boundary SOV/33-37-1-2/31
absorption coefficient per atoml rk, the number of
particles In a unit volume; x, a geometrical coordinate;
'r - knx, the optical depth; tl' the average time a
quantum is, in a state of absorption; t20 the time spent
by the quantum before two successive 3catterings. lilien
T may also be written an 'r - x/Ct 2 where c ta the
velocity of light. Two cases are conolderedt t 1 >. t2
and t. > t.. In the first case, let u - t/t, be a
dimensionless time, v the velocity of the moving
boundary, and p( T u$, the probability that a quantum
of light absorbed at th!t depth T will leave the mediwn,
in time t. Then if P( T) is the probability of a
quantum leaving the medium at any time, we havet
an
P p (t. a) do. Z (t) p (t. u) ada:
Im
D (%) P (-F. a) R"dit.
Card 2/4

A Theory or Light Scattering in a Mediwn 78002
With a Moving Boundary SOV/33-37-4-2/31
This integral equation ip rewritten ass
i-P(t)dt'.
Fir -Ti) 0.")
or
NO - 0 ks (m)
Ifere X is an arbitrary constant. In the second ca-ve we
haves
and
1'0-11-k(l + r.)Ie-kt. k '4 It - 1) + Air' (2 JLI!
C,ird 3/4
V.- WI'Ii~'~--,'-'~L`

A*Thpory.of Light Scattering In a Medium 78002
With a Moving Boundary SOV/33-37-1-2/31
Equations (16) and (20) give the solutions rorthe two
caues. There are 5 Soviet references.
ASSOCIATIONt Lvov Astronomical Observatory (L'vovskaya astronomichft-a-
kaya:observatoriya)
NITTEDs July 1, 1959
Card 4/4

3/033/60/037/02/006/013
9032/1914
/15'C 0
AUTHORS: Kaplanj S. A.9 Ad~
TITLE: Some Notes on the Xmission TorTfght under Cosmic Conditions
FMIODICAM Agt zhurnaIIVol 37 * Nr SR)
4onomicheakiy 20 pp 281-28,5 (US
0'
ABSTUM The present authors have previously pointed out (Rafe I
and 2) that radiation, whioh is one of the basic properties
of shook waves in oosmic conditions has an important effect
on the struature of a shook wave, its motion, and the possi-
bility of its*bsorvation, The present caper reports two
now results in the theory of interaction of shook waves
with radiation under cosmic conditions, It is well-known
that the gas behind the front of a shook wave is heated to
a high temperature and this leads to a strong emission of
radiation by-the.frout Itself. Part of this radiation in
emitted in the diredtiofi of motion and DeWtrates into the
undisturbed region of the gas is abso+d, and heats the
gas, before it is reached by the shook wave-front. The
Cardl/5

dw29
8/033/60/037/0,2/006/013
B032/1914
Some Notes on the Imission of Light under Cosmic Conditions
heating of the gas before the front of a shook wave can
be calculated using the theory of light scattering in a
medium with a moving boundary which was developed in
Ref 5, In the one dimensional case, the intensity of
radiation at an o tical distance % from the wave front
is given by Zq (1:5. where Tr- knx, v - Vkntl I k in
the absor tion coefficient per particle, n is the number
of partiales per ool, x Is the distance from the wave
frontl V is the velocity of the wave front, X is the
ratio of the scattering coefficient to the total absorption
coefficient (i.s the sum of the true absorption and scatter-
ing ooefficients5l,and t is the mean lifetime of a quantum
in the absorbed state, Iq (1) is subject to the conditions
fl - x 141 1 which pond to strong shock waves
under co;2c-'oonditionsc.orTree'B amount of radiant energy
absorbed per unit volume and transformed into thermal
Card2/5 energy is given by Bq (2). As the volume element in the
gas moves towards the shook wave-front, the energy

8082~
S/033/60/037/02/006/013
3032/2914
Some Notes on the Xmission of Light under Cosmic Conditions
accumulated in it is given by Nq (3)9 since dt/dx - -1/V.
In a steady-state wave 7 V and 14 remain unaltered.
It then follows from Bq (b that the energy E is given
by Zq (4)9 where t - l/kno and is the mean lifetime of
a quantum between No scattering 4vents. In the first
approximation one may put P -dT sh in accordance with
the Stefan-Boltzinamn law where Tsh is the temperature
on the front of the shook wave and is given by
Tsh V116R where R is the gas
nnnrnY1mnt^ ralAtion in

8/033/60/037/02/006/013
1032/9914
Some Notes on the Bmission of Idght under Cosmic Conditions
Card4/5
1-X a exy(-hVn,1h ), where ;; is the mean frequency of
scattered radiation. A solution of the energy, mass mad
momentum conservation equations, which are given by Eq
with 3 given by~lq (4), determines the detailed struct-
ure of the heated region It is however, at once clear
that the width of the ' ad region is approximately
koat given
by Xq (6). In stellar,-atmospheres this quantity is small
and is of the order of a few centimeters or motors. In
the chromosphere the corona, or the interstellar gas the
width of the heated region is considerably greater May
become observable. Owing to the scattering of ligh the
higher-lying laqers the radiation of the shook wave will
penetrate into the outer layers before the shook wave
reaches the surface. As a result, the intensity of radiat-
ion at the point of exit of the wave will begin to increase
before the wave actually reaches this point. It is shown

80829
8/033/60/037/02/006/013
ZO32/B914
Some Notes.on the Xmission of Light under Coamic Conditions
that although in the stellar and s21&r,;`,taospheres the
time during which this increase in intensity due to the
penetration effect takes lpla0e is relatively small (of the
order of a few seconds) in chromospheric flares it is
considerably greater "a may be of the order of minutes or
tens of minutes. there are 6 Soviet references.
ASSOCIATION: Llvovskiy gosudarstvennyy universitet (L'vov State
-.. University)
SUBJUTMi October 11, 1959.
Card 5/5

2098
s/o34/60/OO0/2O8/0o3/oo4
2./ 9032/&314
AUTHOR iKlimishin X#A&
TITLEt A Theoretical Formula for the Intensity of the
Radiation Emitted by a Flare
PERIODICAL: Antronomichookiy tairkulyart 1960, No, 208,
P% 13
TEXT: Solar flares may be associated with the propagation of
a shook or a sound wave originating in the deeper layers in the
chromosphero* If that is the case, then the intensity of the
radiation omitted by a flare should be a definite function of
timeq the velocity of the wave front, the density of matter,
etc* The theory of non-stationary scattering of light as
developed by V,V# Sobolev (Ref. 1) leads to the.following
expression for the above intensity
(t) 24 2e(to t)
1n 36 10 V
Card 1/2

A Theoretical Formula oo*,
20898
S/034/60/000/2o8/003/004
1032/2314
where V is the velocity of the wave in km/sec,
(3 in the densitys
to in the time at which the wavo.reaches the surface, and
P in the total energy flux emitted from the wave front,
In the derivation of this formula it in assumed that
d F remain constant during the motion of the wave
n
a
the outward direction# It is pointed out that it would
be interesting to compare this formula with observations
and this will be done in a future paper in the Astronomicheskiy
thurnale S*A* Kaplan is thanked for consultations.
ASSOCIATIONs Llvovskaya astronomichookaya observatoriya,
(Ltvov Astronomical Observatory)
SUBMITrEDi Octobert 1959
Card 2/2

5/169/62/000/002/057/072
D228/11301
AUTHOR: Kliminb1n, 1. A,
TTTLE: Precalculation of asub-satellite point on the obser-
ver's parallel
PERIODICALt Referativnyy zhurnal, Geofizika, no. 2, 1962, jr,, ab-
stract 2G89 (Mezhdunars geofiz. god. Inform. byuloo
no. 3, 1961t 79-81)
TEXT: The author gives an account of a simple graphical method
which allows the moments and place of passage of artificial earth
satellites to be calculated with sufficient accuracy several days
in advance. Z-Abotracterts notes complete translation.-7
Card 1/1

BA01631=100210151M
AOOIAIOI
UTHCH X11mishin, 1. A
A
TITLEs On a possible cause of ths growth of ohromospherio flare brightness
PERIODICALs Referativnyy zhurnal, Asironomiya, no. 2, 1963, 54, Wwtraot
2.51.431 ("Tairkulyar Astrons observ. L'vovsk. un-ta", 1962P'
no. 37 - 38, 13 - 16)
TEM The authorsupposes that a flare is related to a shook or a sonic
wave penetrating into the chromosphere from deeper layers. In this case, the
growth of the flare brightness can be explained by an inoresse of emission
escaping Outwards with the motion of the emitting surf&** front from the depth
to the higher layers of the solar atmosphere. Applying some conclusions from
the theory of non-stationary light scattering, the author derives an approzimat& i
expression for the smount of 4mdssion j escaped outwards bly Un given Ume in-
stant u0, and during the entire time of the wave motion from Infinity to the Opa .1
tical depth r n v (u.-u) where u t/jI, (tj L 'a atom lifetim in an excited state)"
v - dlr/du katIV (k In absorption coefficient per I atoo, n In dwelf4w Of stcass
card 21-2

S/269/63/OW/002/015/03-t
AOO1A1Ol
On a possible o4use of tho#oo
V a dx/dt is linear velocity of wave motion), P Is the flux of ex1ttod energy
from the unit surface of the wave fronj. Using the derived expression the 83
obtains, for V - 100 ko/aso and n a 101 (upper chromosphere) for the time of
linear emission growth, which in maximum exceeds 3 times the biLokgr*und bright-
noes the value a4ual to v1O sea, The time of brightness growth In continuous
spectrum is longer, by several orders of magnitude, thin In lines. Thus the
mechanism oonsidsred yields solutions which do not oontr&diot observational dat&#.~,
The oalaulations can be applied to wtplanation of the effect of brightness in,
crease preceding the appearance of any luminous front on the surface of a star#
I. Ourtovehko
[Abstracter's notes completotranslation]
Card 2/2

ILUMUN, LAs [XlMsbpl LA.11 latAVCHUKt A,L.
inoroame in rwHat4oa intsualtr bJtm* the surpmo of a shook
va" to tbg - safmw of a -,bomopneous nW=. Mr. f is. Shisr, 7
noolOsUM-1089'10 '162# (MlU 16il)
1. Llmakir goouftrstmW universitat la. lvifrankot
(Sboak va. 9) (ptacnauce)
21%, p4l" I,
RMCM 1 -0--

3/033/6W9/005/006/011
2032/2514
73
AUTHORI ~Klimishino 14A-
TITLEs On the theory of stellar shockwaves
PERIODICALt Astronomichoskly zhurnalt .V.39# no-S, 1962, 887-893
TZXTt Stellar shockwavos are usually Investigated usJnS the-
"classical" theory of shockwavon in a moving gas (L.D,Landau.and
Ye.MaLifshitst Mekhanika sploshnykh *red (Mechanics of Continuous
Media), GITTL, Moscow. 1953). This theory predicts that the
temperature behind a shockwave moving with a velocity of the
order of 1000 ~m/sec in a stellar envelop* should be of the
ordei of 2 x 10 deSj whereas observatiovis indiqat* that the
maximum temperature on the surface of a npw star Immediately
after the explosion to of the order of 1,09 - 105-dog. One
suggestion to obviate this difficulty has been that the tempera-
ture is reduced as a result of the emission of radiationAnto the
IsurroundinS space* The present paper is concerned with another
mechanism responsible for the reduction In the temperature* Thusq
a atelier envelope consists of a gas-radiation mixture and the
4atter way often play an appreciable role. When a shockwave
Cord 1/4 ~ It

On the theory of stellar Aackwaves 5/033/62/039/003/006/011
9032/9314
passes through such a medium a part of the wave energy may be
spent not only in Increasing the internal energy of the gas but
also In increasing the radiation d;mity. Hance, for given shock-
wave velocityt the temperature boh Id the wave front way be loss
than the temperature given by the f1classical" theory. The
present paper is concerned with the generalization of the
Aclassical" theory and considers the thermodynamic equilibrium
of a gas-radiation mixtures It is shown that the equation for
the adiabatic curve for such a system is
7 (Y2 1) + 02 (8 - 6Y2) 01 T2 7(y, - 1) + 01(8 6y,)
.Or - -
Y2 02 JL YJ
01 P1
03 P2
where subscripts I and
Card V4
1 P2 1 3 2qpl Up, (9)
1 01 (LT2) RTI RITlelul
2 represent-th* state of the gas before

A
On the theory of stellar shookwaves B/033/62/039/005/006/011
9032/95111
and after tits passage of the ahockwavo, y is the adiabatic
exponent for tits Sant 0 is the ratio of the gas pressure to the
total pressure# T is the temperature of the mixture, q is the
autount of bound energy liberated in the wave front, r in the
flux of radiation from the surface of the*shoeltwave front and
u is the velocity of tits gas rtlativo to the wave front. This
result in then used to find tits discontinuities in physibal
parameters across the shockwave front., The results obtained are
very similar to those considered by X. P. Stanyukovich
(Neustanovivahiyanya dvizheniya sploshnoy aredy ["Non-steady
Motion of a Continuous Medium"), Qostekhizdat, 1955). It in
shown that the ratio of the gas to total.pressure behind the
shock front decreases sharply with imcreasin$ temperature
discontinuity at the wave front. When the amount of wave energy
spent in increasing the radiation density Is taken Into account,
&it is found that the density discontinuity in increased and the.
temperature discontinuity Is appreciably reduced. In particular,
for a shockwave moving with a velocity of the order of 1000 km/sec
in a solar-type stellar envelope, the temperature behind tits
Card 3/1#

On the theory of stellar shockwavos 8/033/62/039/005/006/011
9032/Z514
wave front is lower by a factor of 18#5 as compared to the
temperature calculated from the "classical" shockwave theory.,'
The general conclusion is that effects associated with the increase
in the radiation density must not in general be ignored,
There are I figure and 1 table.
ASSOCIATION3 Llvovskaya antronomicheakay^ obsorvatoriya
(Lfvov Astronomital Observatory)
SUBMITTEDi June 27, 1961
Card 4/4.
R
TR`X 5-MMAMM irif~l-

XUMMNj LA.
Detandrdag the Inars"t in radiation intensity before
the alit of a shook va" to the faas of a star,
Astrouss,ha. 391no.6tlOO6-1000 ;% 162. %(KIRA 15:12)
1. L'"vokap arvatoriya.
(S ment)
(Shook va"s)

ZILVICH, V.M.
SOSO results of statistic proce"ing of the ~#talog of the
Interstellar polarisation of star light, T31re Astron. obse-.
L'viv. un, no..39/40*-3-10 #63. (KTRA l6tU)

CalOullting d1scontinuities of gai parawtors at tht frow of
a stellar shook vavoe ISIr. Istrion. obser. L'v.,v. un, rto*n/
40tll-17 163,
ProtabIlity of a quantux emospe fron a madlux w,-lh a moTir4
boundary. 18-21 (MIRA 161li)

71
~ACCWSIOM )Mj A"019W

AMORt 11imishim, - 1. A.
ITITM Certain remakki am, the role of radiation offeeU in the theory of stellar
shock waves

SOMCB: AN UM Astmomichookly movet. Aptoblem *I "so

TOPIC TMt sstrousmW, stellar astrosepyl.star, shock we.*# stellar otmapharep
star envelops
'ABSTRACT: Certain results of a.st"Y of radlatiss effects is the theory of stellar,
shock vav*s ore pro,stated. If a shock vs" moves In * star ou"lope with a "I.
I
ocity of about 21000 10 As vsm frent, determined for
14009 the temperature behind A
.
strong thook vav*o by the expression T2 where R is Mw gas oomatsmAt attalms
.20 mkillion dogrjosp At mob a tomperstwo the radiation proom" Pr 040 is 0
.the sam order or vves greater than the Sas prosSIM" VS a cut vhore tD is the
Maw g
f th
d
it
th
t
I
"
I
t
d
i
m an
an
s
o
am
a
e, o9
s
s
o
e 4w
y o
parameters at the of
trout of aush s maw It Is woessaY7 to do=
the',enorgy of notion of of she& wag In Us Ims rm Will -be sa.
7A 7

AMMION XR1 AT40196"
Itoreass in radial4on donslir bohl" Us wave fronts As a nnltp for aw mA 00-
.4 gas-,
to" wave volool,ty.,the %be boat of a vow antag I&
rimilation aiztarp will be less them I&He&Ud by the formals, -for ordim" shook
wavvs, moving In gas, ]MbW,Uw front of a allwq shook wev the toqpwatme is
determined usims the tomd&
who% is the ratio of ths gas prosou to the total pressure behind the
front. The temperature behind tho,froat of a wave moving at 1000 h %S -3
0000 1 ly 30 ums-~
**lop* such as the em's will be of the order of 700 41 opproximte
lose than the value *btsized using the usually accepted formulas 00246110 '"re
W
contend that dme to the decreasing density, of Abe modiva as vvloeltr of a amok
I
VA" approaching the surfacoo &A also 0* t*Woratw* bobbA the freatip will lmkm,~
crease sharplt, However, this `Ls true enly as long as Me optical depth of the #14
'It part of Us she& wgve amwa
v&v* froat is esusiderably greater, than witys
is radimted by Us vav* frent, end seaspas #to AnterplonaUtw. "so So
turo behind the as
f"at of a SAMU obook vajv Is detemis"Ay so..
JW --
V
dd V11 J+ t+
cad
, ~OrO4,~- I.
U 41 ".It -1
~

IMP-
'ACCENION )MI AT4019W
4r in the case of a gas-riku IT
&ties mixtaro
IN
*~hero is the energy flux from #4 vavv troutp which in the first approximation
can be &owned to equal ZvortaTelIL to the optical depth of the wave froati
is the Stefa*41*ltsnmn constantl lit the donsi* of an undisturbed m"=* At
optical depths oft 30 shock wav Ivalmosconce will begin. and " a remalt the
tem behind the. &book wave front decrems iobarply and Us shock wav it-
perature
'm*lf is slowed dowme If tboAlmuslonless "Is iiy of movement of the Wav to
Mmtl .44 1, where k Is the absorption cooftlelont,for a sloglq partielop a I& the
`4uautity of particles in a unit volmmej t, is 0# &#&* tim of promes
of
tun in the absorbed state (tl 1(~Ostc for a resonance spectral line and tladj&,-
vhoro C is the recombination coefficient associated with coatimme
&S
sion) j the intensity of the smorging rmUMAM 1(t) has an *3"
0; . U
on time
"Vh9re to is the timme of oft"It6"O of the, Aook mV at Us sortasm, It tons-6
that in the atmopborea of AfAWS.Ma MW a" 60 Use lmlvod Is a brubbis"

ACCMIOK Mgt "'Ah
0196"
amral socoads, Origo arto b"t 4 h
across* is rolatknly dwrt
ASSOCIAZIONs Aa$roneolobsoUr so"* AN SM (AAr...d"I'C~tI)
4' '11*171
.00
smano MP69
MU Aft
A
I= Mgt AS 4w
i4
I.X
4 '.i
4f,
,4F
4/4

KAPLAXp S.Aq KLIJUSHIN# LA,
Methods of analysis of interstellar turbulence, Astronozhur* 41
no.2t274-281 Mr-Ap 064* (MIRA 17t4)
1. L'yovskay& astronaidaheakaya observatoriya i Radiofizicheskiy
Institut. Gortkovskop gosudarstvennogo universitetas

--j gt-Tp !7t-~Aerf ! "I =7
N R t AP4043954 S/U()I)/b#4i04l/004/065?/066l
&UTHORt K&PIon, S. A.& KltmLshin.- 1, A.
fIT1.9i On the structure of a ~hRr-"av
a
GOURCEi Astronoutchookly shuicnet, v, 41, no. 4, 1964, 657-661
Torl(' TAGSt shock wave structure, shock wave emission, nonetationary
qatterinR. Liptht scattering theory, heated gone temperature
ABSTRACTs Calculation of the structure of a shock wave with gaigpityn
(calculation of shock wave parameters) to considered with the as* of
t1le rcqtilts of the theory of nonstationary light scattortnr in a medl-
uni -aith movinR boundaries obtained earlier by the authorle Aatrnno-
zhurnal, 17, 9. 19601 Ukrainakiy fietcheskly thurnal, V.
I)e)o). The stationary one-dinenstonal motion of an ideal Kee,
effected by the emission flow F is considered. From the conditions
f -ir con voi rvat too of mass , energy, and momentum, undet thr 44 -ztImption
ti,ar nresqure and internal anergy of the nondisturbed aliq Rre neglt-
oxprossions for the temperature T and the I Inu F at sk river.
;-Int are derived ILL terms of VD, n, y, R and , where Vo it the tit-
1/3

L 7o48-69
ACCESSION M AP4043954
itiol velocity of the emission front. n - oolc. whert og to density
of the flowing gas and o to the donsity of the nandisturbed gas, y is
the isentroptc exponents R it an Ideal gas constant, and viathe molec-
'ilar -eight. on the baste of light scattering theorv, differential
equatioas fcr the source function b(t) are written and their solutions
containing terms T+ (temperature behind the shock wave front) and T_
(tempertturo ahead of the shock wave front) are derived. To determine
the unknowns T. and T, szpressions derived earlier for T and F for
ioraodiate values behitad and ahead of the shock vivo front are used.
1 -3,em of four equations is derived from which T 40 T_ n and n- as
f,jtirtion; ot V. and P0 are calculated. From the ca IC ul;tel values of
ind T , temperature and pressure in the heated zono can be deter-
ffilfled. Tt ii established that the temperature in the heated tone
varies with the distance from the shock t.-avo front according to tha
exponential law. Th* rosulte obtaine,d are applied to the study of the
prnp4KatLon of shock waves to stollor envelopes, It 1* shown that
cemrer4~uroe In the heated zone immisdiattIv ahead of and behind the
sh,,o:k wave front are of the ones ordtr. Orig. art . has t 14 formulas.
113

7o4b-65
ACCESSION NRt AP4043954
ASSOCIATIONt L'vovsksys ostronovichooksTs obsorvatorivo (.k'wow
&&I-conLomical Observatory)
SUBMITTEDt 07oct63 ATD PRESSe 3104 ZNCLI 00
SUR CODE1 KZ No Rtr SOVI 010 OTR9Rl 002

17, 4- -1, M ft-h
~C) G;h
"SION N,,. AT40149114
AUTHOR: Klimishin 1. A.
Some approximate solutions of sas Wamic 11 equations
-AZE: AN SSSR. Asio-onomichaskly sovet, Voprosy* kosmogonii, v. io, 1964.
jo;cmy* magn;tnoy gidrodinamlkl I kosmicheskoy gazodinamiki (Problmns In magne-
aisd cosmic gas dynarnics and cosmic gas dyinmfrs). 146-153
T -AGS: sLelldr latmosphere, astrophynics, magnetohydrodynamics, cosmic gas
flijinics, shock wave, shock wave dissipation
ABSTRACT: in recent years, a number of authors have developed approximate methods
ror the solut;on of the equations of gas dynamics in appl'tar;on to the study of
indi., dtal specific astrophysical problems. A brief re-4view of such studies has
:),-eri ~resenteA by Ono. Sakashita and Ohyama (Progr. Phys. Suppl.. 1951, 20) and
Sclitzman (intern. Astron. Union. Symp. N 12, Sologna, 196i ,). Some of these
s have not yet been exploited fully and It is these rrethods which are dis-
iy the author. Part I Is a discussion of methods (or the study of the dis-
-).)-,ion of a shock wave In a stellar atmosphere. Part 2 anaiyzes the pcissibiiity
i,ie extended atmosphere of a star being maintained by pe(iodic shock waves.
,,,.,ft,),revIews studies of the structure of a shock wave accompanied by radiation.

L 20129-65
ACCESSION NR: AT4049114
in zhis relatively brief paper the studies of 219 authors are cited to Indicate
thdt the possibilities of soiving the three mentioned problems have by no means
been eAhaU~ted. "in conclusion, the author wishes to tha-k-J. A. Kspijn and
V. G. G~orbatsk[yjor sustained interest in this paper and nurnerous discussions of
the problems presented". Orig. art. has: 8 form-ulas.
ASSOCIATION. none
SUBMITTED: 00 ENCL: 00 SUS CODE: AA, ME
NO REF SOW: 016 OTHER: 015
Card 2/2

AR6013394 SOURCE COM UR/0269/65/000/011/0042/0042i
AUTHORt Klinishin, 1, As
TITLE1 kuaysis of the structural functions of nonthermal comic radio mission
SORCEt Rafe sho Astron"i"t Abs6 11-51-384
REP SOURM Tairkulyar Astron. obsery, L'yovsk,. un-tat no- Op 1964P 5-4
TOPIC TAGSs space vapetio fieldg radio missiong cosmic radiation 0-0'%M&,roA'%c
ABSTRACTs The resultswof a deteraination of the structural function of the inter-
stellar Magnst o fi*44000rding to fluctuations of the luminance temperature of
cosmic radio mission are presented in tabular and graphical form. j?r"slation, Of
abstraC9
Ion OOD31 03
-1/1 J~:~ UDCs 523.164,523-151

POWSHMA, N.A.; KUSHNIARUKO V.A.1 VA.
ilinterIng of Mlnioptarus schrelbersti MiAt CbIroptArs)
in Transcarpathies r4ol. %bur. 43 no.5M2-78) 164 (M 111A 17 0
1, Ifttodra scologli posrwoottsykh blologicheskoga takulOtOtA
Ltvovskogo gosudaratyumog-i univeralt*tae

CMJBWSKI,t Jakubt UMUKp loWla
ikoration of ur"poln and 17-lot"terolds In pationts vith
roWratory Inodficiencys Pol, uvbo mdo wwneto 33 oo~Ss
80-M '63~
1e Z n KUniki Chmob Vownetrsnych AN w Blalymstoku Kisrowniks
Prato dr nod. :* Chlobwoki,
Rx$MTW lxs=Cw=)
27-Mftwmm) (mors IN)
MM) (PMMMW HW? DISZAM)
i

KLi M-2 A.
7707, Klimkaj A, Vmtrikolkho%noya dewkratlys. VIIIWIS# Goopoitnevehizdatg
1954. 56s. 209m. 5,000 sks. 5OX4--% Litov* Yas.-(55-3517) 338. 1K
80t Knizbmaya latopist, Vol. 7# 1955

rMKAITF., 1.
G:-MRAPIfy & GTOLOGY
MOKSLIFAI Pqklr-SDUI,
KLIMKAITF.p 1. Some data about the gas conditions of watar of Lithumda
lakes. p. 107.
Vol* of 1950*
Honthly List or East Euroman Accession (EW) LC Vol. 8, No- 3
harch 1959, Unclass.

-.-, r -0- )

ILDCMTICRo AM.
Inhibiting effect of Ut on secretion of the Castric gLLndee Top
fisiol* nos5sSO-8? 053* 815
Is Obarnovitekly modltolnokly hatitut, kafedra tormallngy
fislolo It
folulo Juicat
socrotiono off, of fato Inhlba &otion)
(YA"O effect*#
,on gsotric secretion. Inhibe &otton)

Cosparative analysis of the effoativenese of treating k"rtension
with reserpine wA other routine methods, Sov, sod. 24 no.61*411
:0 160. (KEU 130)
L Is perrogo terapevt1aheskole otdolonlys. (say. M.Ya,
w , IP$kmp) I .I .. I
sterstva putey moobsbabaWye
ION)

KLIMVICH# VoPol VOMTWj M.P. (Hooku)
.. . . . .. ... .... .....
rmportance of the revorpine toot in the remorpine treatment. of
hypertension in the poWinico Sovonede m302-95 162*
(WA 2515)
1e Is Ob"yedinennoy pollk2bild Mbdaterstva patsy soobehobenlys.
(naaballulk A~Oo Sarkleovp savoduyubabaya 2-a terspeyticbeskim
otdol"iyeat M*TARO kukaya) 0
~ (10 1 1 11 1) (OPERTUSICK)

ILIKKWCTUTIjO,
Development of Camunisa and control of puMio bealth by the
Plartya &elk* apeaugs'9 so.2d.045 7164,
1. Vilniaus Valat.V.Zapaiko Y. universiteto 7W istorijos
katedrae Mokslinis vadovas: doc.1allavick".
- t '
, t SAMP I -it M-00',"I
U
il-, NOR NO
ft

KLIMKIEwicz MlIn ) ROSE, Andrzej
:~--A
Case of multiple infected pulmonal omboli 1n the course of
streptocaccal osteomyslitts, Pol. prsell, radiol, 29 no#4t
387-392 il-Ag 165.
1. Z Zakladu RadialogiiInstytutu Gruslicy (MorounAki prof.
dr. mod, K, Desowxk*) i & Oddstalu XI Instytutu Gruslicy
(Kierownikt does dr, mod, B. Kappioni).

Zt$ACZKMKAv Jadviga; PIOTROWSKI, MuUnj SZWARC, Maria;
KLDOMICZ, gall!l&
A caso of suitipio papinow of the trachea and main
bronchus, GrusUca 31 no.9081-967 163.
10 Z Oddsialu n Instrtutu omitcy Kisrotmiks prof, dr
Ve -Tarossevics Z Zekladu Radiologil Instytutu Gruslicy
KisromAki prof. dr 1. Ossawaka
(BRONCHIAL XBORASM) jTRACHEAL nOnASMS)
(PAPMCHA (THORACIC RADIOMAM)

IMBSKA-MAKOSA., Zusamal KU)TTp Wria; ROWINSKA, Eva; ~
KOZIORMSXIp Antoni : .
Diagnostic difficulties in the pulmonary fibrosis* Gruslica
33 no.7s605-623 JI 065#
1. Z Kliniki Chorob Pluo (Kierawniks doc, dr. P, Krakovka),
s Zakladu Rodiologii (lisrowniks prof, dr, L Omsowska) I a
Zekladu risjopstologii (Kierowniks dr. A. Koslozow k1)
Inetytutu Oruslicyo

C)IODK(WKA, aterahlao prof* dro sed.j mjwwic;~ naiin; norawill',
ZAJICZKCWFJ4 :&Mgao
Prlmw7 anyloidosis of the Immr r"piratory traot. Oms1lea 3)
no*3tW-246 *0656
11 V Oddstalu 11 (prof, dro sed4 Ve Urosawlan)l z laklaft
Patologii (lieromika prof. 4r. sod, So Chodkovska) i z ZWada
Radlologii (KierounAt profo 4r. mod, go Onoovska) Inetytuta
Orusliay, - throswao

"Mi
MEMI, Jerzy, drj_ IvArian, zgr;
itevieva of piblications, Tuth pap mortka
J 1 '64,

Wal- M
WC.
IUUXMCZ# Antonil XLIN=CZs Vitold
phodn-o pwg=ww por*=w (P*U.) I= (CyprWdast
Ostsichthyss) on Va torritorles of tho muth of the VistaU
River, NoWd mates ;nyrod Ws to.12slg-143 162#
10 X&to&a zoologii Systomtyosmjp Uniweraytot, Lods.

J(VKK, An, doo. drel SKALBA# Hanrytp doc. dr.1 KL IWICZ. Usts
~- D7
MIMIUCHOVICZ# Uebs
Histoohemical reactions of alkaline phoephatases and adeno-
stnetriphosphatase In hwm plaaanta In tvlation to the
poriod of pregnancy. Andokre Pole 16 no*3001-312 Nj%.J# 065.,
if 3W&d Histologii i ftbriologli SlAwkiej Akadowit Wyomoj
w Zabrtu Werovalkt doo, dre Js, Jonek)l It KlInIka Polounletwa.
i Chorob Kobdocych Blasklo Akadmadt Hadyoznsj v Oltemiu Wo-
rowniks doc. dr. Ho Bkal is

JONEX, Janj SKAW, Henryk;
LLI ZO Zdzislav; D"IECWHMIC2p lach
Study an the behavior of louelne anin%eptidass In cancer of
the uterine cervix. Ginok. Polo 36 no.MRS-Ml S 165.
I* Z ZeklALdu Histo*,ogli i Enbriologit Slasklej AM v 7Ahrzu-
Rokitnicy (Kisrowniki doe. dr. mod. J. Jonek) i s 11 1113iniki
Polotnietwa I Chorob Koblacych Slasklej AN w ljytoslu (KIerowniki
doe, dr, mod, Ho Skalbs).

ILIMINj lot kapitan
First steps of the party condttoo of a nIIIUz7 =its
Sib" no,2169 ~J& 161.
3
Russia--Army.-Political activity)

NO-
C TAGSt CoWgMia. altim;~
ABSTRACTs This Author Urtiffoate pments a qvArts asta'.'-oised gmvimt4r-
altizeter containing Cmvisister aid alUmter systma in %* fwu of Golitain
pandulms. To increaseAhe soommW of wisuresents without forced electric Uwnw-
ezatic control and to deoreass, the weight of the device. the axes of rotation of the
elastic quartz system are placed In a horiumtal plane p=allel to each other.
These elastic systems are made In the form of & ecossm mnolith and are VrovAded
with se-Pamte optical systems$
ASSOCIATIOUs nons
SMUMED% 23J=61
NO RV SOV 1 000
Card 1/1
am$ 00
OM I OW
SooM Act

LYZIIIN,t ASWAS# L.,, tokbn. red
[YOM#W; bandboak MA guide from 14mlainsk tA N04-16-12nimei;
yuUmoditell-spravochnik ot pristani Minusinsk do pristani Du-
dinM# lad.2.p Were i dope Krannoiarski trasmiarskoe kalsh.
noe isd-vot 1953, 208 P, (KMA 15 t 12)
I* Yoniseyakayo reab"s puvkhodstvo.
(Irenisay Vallay-Handbooksp -s=,als# *to*)

KLDWMo M.V.p aladshiy *uohrqy motrudnik
Mitterialm an the cooperative maniW7 and hWenic descriptlon of
individual harzAd substances in the produation of syntbatic
isoprens rubber (dimethy1dicumet dimmm alachol and high-bolling
,fractions of vat residues)o Gis. L sane 25 no* 6%85-87 Jo 160.
(KMA 34s2)
Is In Mookovskogo nauchno-insledovatellskogo institute, g1glyeny
i sanitarii imeni F,?., Iriamm Ministerstya sdravookhmnenir
(AIR-P=TIDN) (VATIR-FOUA)TION)
(RUBBER INDUSTRI-4MMO ASPECTS)

ILIKKINA~.N-V.p mladshly nam hnyy actrudnik
Hyglertlo standards for reservoir water with regard to Injurious
substances from the production of synthetic looprene rubber,
Gig. I woo 24 no,,618-16 is 139. (MM 1238)
1e Is Xoskovskop nawhno-Issledovatellskago Instituta saultaril
I gigiyany Went 1,13rismam Ministerstva adravookhranenlys
(WAM POLUMICS
by Injo substances frost prod* of synthetic
Isoprene rubber, byg. standard* of substances
Pus))
(MIBM
inj. substances from prod. of synthetic
Isoprene rubber In reservoir water. bygo
standard. Ohio))

KLIMKINAI N. V., Cand Med Sci (diss) "Hygienic standardization of
reservoir water from harmful substances in the production of synthe-
tic Isopropene rubber (isoprene and dimethyldioxone)*" Moscow, 1960.
11 pp; (First Moscow Order ofLenin Medical Inst im 1. M. Sechenov);
200 copies; price not given; (KL9 17-60t 169)

KLIMKINA, N.V.
Experimental basis f or the permissible concentration of
dimethyldioxans in bodies of water. San.okhr.yod.ot ugr,,Prox,
stoch.vod no.50-27 $62, (MIRA 17s6)
1. Moskov3kiy nauchno-iseledovatellakiy inatitut sanitarli i
gigl"ny imni F.F.Erismana.

KLIMKINA, II.V.
Experiontal basis for the poruibbible concentration of isoprons
in bodies of water. San.okhr,vod.ot sagr,pron.stoch.vod no.5:
28-43 162. (MI-A ;7t6)
1. Moskovskiy nauchno-itialedovatellakly institut sanitaril i
g1glyany imni F.F.Eriamna.
Af

SAVELOVA, V.A.; BRIJKO Te,36; KhIWINA, N.V.; RUSSKIKII, V.V.
Experimental basis for the permissible concentration of cyclahexanal
in bodies of water. San.okhr.yod.ot sagr.prou.stoch.vod no.5t
7843 162. (MIRA MO
1, Moskovskly nauchno-iseledovatel'skly Institut sanitarii i
gigiyany imeni F.F.Erismana.

SAMOVAO V.A.; KLIMXINAm LIP
ftperimental basis for tbe awdum permissible cyclohexam cOD-
centration in the water of reservoirs &W rivers. San. okhr. Yod.
ot sagro prom@ atoobe Yode no.6#30-45 164-
Experimental basis for the m&xJuum permissible cyclobexanone
exime coneontration in the water of reservoirs and rivers,
IW06445 (MIRA 1813)
1. Mookovskiy nauchno-issladovatellskiy institut, gigiyany IMIGni

SAVELOVA, V.A.; BUY, U.S.; Kqmnu,-N-.,I.
Experiwntal basis for the maximum permlazible con-
centration In the w,ter of renorvoirs and rivers. San. okhr. v0d.
ot sagre prom* stochs Yode no,6146-63 164.
(MIRA ISO)
1. Monkcrvokiy nauchno-isoledovatellskly inatitut glgiyerq Ismai