SCIENTIFIC ABSTRACT STANKEVICH, K.I. - STANKEVICH, MK.

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• Collection: Scientific Abstracts
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• Original Classification: S
• Document Page Count: 100
• Document Creation Date: November 2, 2016
• Document Release Date: August 25, 2000
• Sequence Number: 1
• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT


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STAI,LC,YIC 1_L-Xj.,CKiyev)
L
Hygienic evaluation of the microclimate of living quarters with
floors made of plaitic materials. Vrach. delo no. 3:110-112 Mr 161.
(MIRA 14:4)
1. Ukrainskiy nauchno-issledovatel'skiy institut kommunallnoy
gigiyeny.
(LABOR AIM LABORING CLASSES-DWELLI14GS-HYGI-FNIC ASPECTS)
(PLASTICS) (FLOORS)

STPITKEVICH, K.
Hygienic evaluation of some plastic coverings for floors. Gig. i san.
26 no.6:21-25 Jo, 161. (141HA 15:5)
1. Iz Ukrainskogo nauchng-issledovatel'skogo instituta konmumallnoy
gigiyony.
(FLOOR COVEP-DIGS) (PLASTICS)
m

STANKEVICH, K.I., nauchnyy sotrudnik
- - __ --- - 11 ---- ------ -
Hygienic evaluat-Jon of floor covering made of plastic materials.
Gig.i san. 26 no.12:81-82 D 161. (MERA 15:9)
1. Iz Ukrainskogo nauchno-issledovatellskogo instituta kommimall-
noy gigiyfny.
(PLASTICS) (FLOOR COVERINGS) (AIR--POLLUTION)

STANKEVICH K. nauchUy sotrudnik
Hygienic evaluation of plaptic floor coverings. Zhil. stroi. no.l:
12-13 163. (MIIU 16:2)
1. Ukrainskiy nauchno-insledovateltakiy institut, ko=mnallnoy
giglyeny.
(Floor coverings) (Plastics)

STANKEUGH, K. I. (Kiyev)
Experimental data on the blastomogenic action of wimarone iind
polychlor,vinyl plastics. Trach.delo no.11:108-124 N 162.
(MITU 16.-2)
1. Ukrainskiy nauchno-,issledovatel2skiy institut kommmaVnoy
gigiyeny.
I FLASTICS-TOXIGOLOGY) (GOC.TNOGNMIS)

W@
STAITIE VT!:. . ."1 ;4 J.-)Laukevychj K,I.]j kand, med. nauk; OVDIYENKO, T.L.
TOL,I -
11,
.fglonic properties of some synthetic fabrics for clothing and
fontwear. Leh. prom. no.3.26-29 il-S 165* (MIRA 18:9)

zi@
STA."@Y-EVIL.`, X.O.
,., Sr-,i,@;K.EV-
42320. Sa.@.TKJ.@,, T.r
L iGH, X.O.-Ispytaniye novoy rolovki mart-3novskoy pecht.
Nauch, trudy (Dnepropetr. metallurE. in-t im. Stalina) v-yp 14, 1948, s
19-27.
SO-. Letopis'Zhurnal'irykh Statey, Vol. 47, 1948.

c..'- I , @ @'. I - N" 7 . "
-L;'L'U@ Iy U -1-'O"1'3-=Y
K. @5.2 .1
"Detection of Deuterium Monoch:romatic Redioemission in Wavef,; of 911
6 em," paper submitted at the International Astronomical Union Radio JUstronomy
Syuposium, Jodrell Bank, UK, Aug 1955
A-40423, -Il

Category : USSR/Radiophysics - Application of radiophyiscal methods 1-12
I
Kos Jour :Ref Zhur - Fizika, No 1, 1957 No 2007
Author :IGetmantsev, G.G., Stankevich, K.S., Troitskiy, V.S.
Title : Monochromatic ql.6---cmDeuterium-RacUo Waves from the Center of the Galaxy.
I I
Orig Pub : Tr. 5-90 soveshchaniya po vopr. Rosmogonii. 1955, M., AN SSSR, 1956, 539-545
Abstract : See Ref. Zhur. Fiz., 1956, 2o669

I......... -.1.
STANIKETT,"if, K. -3., G&ZIANTS-N, G. G. and TRZOIT3KIY, V. S.
"Observation of Deuterium Lines in Absorption Lines on a Wavelength of
91.6 cm," a report delivered by B. M. Chikhachev at the S@mposium on Radioastrorwq
held at the Jodell-Bank Experimental RadioastronomIcal Stations, Manchester
University, England, is Summarized in the account of this symposium in an
article by V. V. VITKEVICH in Vest. Ak. Nauk SSSR for January 1956.
Sum. 900, 26 Apr 1956

STI XKHVI CH. K. S.
Investigating radlowave emissionef the galactic center on 9:L.6 an
wavelength [with wumarjv In *gllehj. Astron. zzimr. 35 no.l.-157-
159 Ja-F '58. (MI3A 110)
1. Radiofizicheskly inetitnt Gorlkovskogo gotsudarotvennogo univer-
altata Im, N.I. Lobachevskogo.
(Milky 1+7) (Radio astronomv)

UCATT
AUTHORSs Tu Laaa-ypo. A. Rosin, V.A.
@@V Str.zhneva, K.H.
I&Mkkn
SP4 Sku-9-0. TrAt.kiy. V.S. Khrul.v, Y.Y. ..j
Toeytlia, N.M.
TITLS. Observations of the Annular Solar galip.a of ApriL619,1958
an Wavoleogth. of 1.63, 3.2 and 10 a.
FMOVICAL: 1".Ntly. ys'hikh ch.bnykh Rdi.fi.lk..
1959, Vol 2 .Xr 2. Vp 154b 158 (USSR)
ABSTRACT; The report of a int 3 vi t -Chi= so "poditiqn to
9184. 8,1112*) on the island
Liag-sui, ( .30132-. 110
of fti'ma. The serials used parabolic reflector. or
diamot "s I : wavelengths And 1.5 . at
the Iona" tTh. fluctaatisna in the three hold of ansi-
ttvity War imi &rly 4 , 3 And 4*. Th. loctri,:l ""
or the =I. ~. parallel to one &.other. Th. bAal.t.
accuracy of intensity weasuraxont was @ 15% at the longer
wevelonathe &04 @ 20% at the ahortest. The relative
Accuracy, an averaSing period of 1 min, -4. 2-3,-..
The results are ahown in Figure I as m.asurectents at
C&rdl/3 effective Isap.,.t"O ozpr*..*d a. & p.@coat.S. or the
teftParstUre of the unwalips.d sun. Th. Value. of the
latt;W..r.(9 000 *9 (1.63 ..). 21 000 OK (3.2 a.),
I" L 10 CUL The vertical. lknex on the diagram
represent the tuat to of din* woontactw (4 in number)
a" the "4UltAttan at certain wall-knowa, spots Mrs 188
=4 186. 4 number of pogullarities "y be Acted
511tweam, a- 0.30 and 2 15 a and hot..- 3 i7' and
3W there is an increase in iztensity over what
.odght b; owP"t.d. WigUr- 2 Oh-w- 4 synoptic chart at the
Sun. . the Nr 186 group oflagats measures 36 x 10 the
effective temperature (5-10 K at 1. 63 -.) and height
0.04 a -at 1* -0) "Y.be -estimated. The curves Car 3.2 am
and 10 an " Fig-r. I are "Yq-tric.l. This "y be
"PI&L-d as duo to a Wedge-shapod equatorial region Which
Ajwr@" JA brightness towards the eastern limb of the
:%A. The longer wavelength curves a4so show a small
bkvAP* in the trough. This is duo to *limb briShusaing"
Card2/3 and it to possible to estimate its "Ount - e.g. at the
shortest ... alus contributes 4.5% of the
Intansit" or the unaclipsed Oun. The offectiv. r.di-. of
the "r4dto-suns is-also estimated as about 4% (depending
amveloagith) greater than the optical radius. The deduced
Zloes of Various constants or* in Table 1. Tt@ China
"thanked as we also Chuang Lishola, Smi Wen,
1A Chl-ftm. . Th. Aa.3c.USSR or* thanked, &Is.
A P. Holobanov. B.H. Budkin, P.P. L.Coe.mxo ad A.A.
I-alkow. Thera .. 2 figures, I table and 2 Soviet
Z
references.
A!1-PTA?7OKt 1ss2*davateLO.kly radlafieLchookiy institut pri
Qor'kov kou ualvera&tste Rzzztrth T-titut,
or GarT, ftlvareity)
SUSHITTILDi December 9, 1958
card 3/1

86852
S/14i/60/003/005/005/026
9,'@. r,7 //Y,/) E192/E382
AUTHOR: Stankpvich@ K.S.
TITLE. Saturation Effect in a Paramagnetic System witb
Three aW Four Levels
PERIODICAL3 Izvestiya vysshikh uchebnykh zavedenlyo
Radiofizikag 1960, Vol. 3,, No. 59 pp. 765 - 773
TE,XT3 A paramagnetic amplifier based on the use of four
leirels was proposed and experimentally investigated by
C.R. Ditchfield and P.A. Forrester (Ref. 1). Such a system
hits a number of advantages as compared with a three-level.
amplifier and it is therefore of interest to investigate
the permeability of the system in the presence of a strong
auxiliary field and to take into account the saturation
effect.. The problem is analysed in this article. it is
assumed that a paramagnetic crystal has a system of four
energy levels which satisfy the relationship
EI < E 2 E3 < E4 and E 3 - EI= E4 - E2 Two
h:Lgh-frequency fields with frequencies w I and w 2 are
Card 1/7

86852
s/141/60/003/005/005/026
E192/E382
Saturntion Effuct -i.n a Pnramagnotic System with Three And
Four Levels
applied to the crystal, Since the interaction between the
spins of the paramagnetic ions and the crystal lattice is
negligible., it is,,,possible to describe their behaviour by a
density matrix .' . The Schroedinger equation for the
density matrix if in the form3
A A
H eH
at
A
where H HO +-HV is the Hamiltonian of the system,
H is the Hamiltonian of the paramagnetic system in
the absence of the external fields and
IKV is the inter-action ener-gy with the external
radiation fields; this energy is defined by,
Card 2/7

86852
s/i4i/60/003/005/005/026
E192/E382
Satu.r4tion Effect in a Paramagnetic System with Three Ond
Four Levels
+ z iW.It + 7 -1. 2 t
V e + y e 'P (2)
W Me W W W W W
1 13 W 2 23
Since the matrix of the average density to (averaged
ovei- a suitable relaxation time) is of interest, the
Schroedinger equation can be written as Eq. where
6C/6t is given by Eq@ Here, at m A n -ZI
and'at m = n where -C is the spin-lattice
_IM 2 1
relaxation time and 11--2is the spin-spin relaxation f1me;
@s the value of the -lensity matrix in thermal equilibrium
100
in the absence of the field, When Ho is diagonal, Eq. (3)
Card 3/7

86852
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E192/E382
Saturat-4on Effect in a Paramagnetic Systcm with Three bnd
Four Levels
clan be written as Eq. (5). where D(t) (2c)(t)
whIch rep-resents the de-viation of the average density matrix
from the instantaneous value of density in thermal
equilibrium, The equation for D is thus in the form of
Eq. (6), where ()(t) is defined by Eq. (7). By disregarding
o
the transi-ents, it is assumed that the solutign gf Eq.
,,(6)
is in the form of Eq. (8), The parameters R, S, Y, Q and U
can be obtained from a system of matrix equationsT, these are
given by Eqs. (9). The notation in Eqs. (9) is (t fined by
Eqs. (10). A rescrant frequency of the average magnetic
dipole moment per unit volume at frequency w 23 Xs giLven by.
-iW t ^ -A
P 2Reli T+ e 2 = SP( -@LD)
2.3 32 23
Card 4/7

86852
s/141/60/003/005/005/026
E192/E382
Saturation Effect in a Paramagnetic System with Three aind
Four Levels
Consequently, the expression for the permittivity isg
= 211 T+ /H :03-
k23 32 23
It is seen, therefore, that the problem of determining
-is equivalent to solving Eqs. (9) with respect to T+
23 23
which is defined by twenty expressions of the system of
Eqs. (9). Finally, it is found that for determining X 23
it is necessary to solve sixteen equotions defined by the
system of Eqs. (14). The solution of this system with respect
to T+ is in the form of Eq. (15), where 6 and 6
23 1 2
are given by Eqs. (16) and (17). Consequently, the e:kpression
for )L 23is given by Eq. (18)9 From this it follows that the
Card 5/7

86852
s/141/60/003/005/005/026
E192/E382
Saturation Effect in a Paramagnetic System with Three And
Four Levels
permeability for a three-level system is given by Eqs. (19).
The real and the imaginary components of are defined by
X 23
Eqs. (20) and (21), For the case when the signal and
pumping frequencies coincide with the transition frequencyV
the imaginary component of "X-23 is expressed by Ea. (24) for
the case of a four-level system and by Eq. (25) for a three-
level system. From Eq. (24) it is seen that for saturated
four.-Ic:vel paramagnetic systems the imaginary componeftt@. of
the peimittivity is negative and @ independent of the
relationship between w 13 and w 23 * This property Iis
particularly valuable for constructing the amplifiers for
mm waves since it is possible to use the pumping-frequency
almost equal to the signal frequency. The independence of the
Card 6/7

86852
S/141/60/003/005/005/026
E192/E382
Saturation Effect in a Paramagne-7.ic System with Three-and
Four Levels
gain of such a system of the relaxation times of various
transitions makes it possible to use various types of
substances provided their energy-level structure is
satisfactory. The anthor expresses his gratitude to
V.M. Payn and Ya.I. Khanin for discussion and valuable
remarks.
There are 6 references: 4 Soviet and 2 English.
ASSOCIATION- Nauchno-issledovatellskiy radiofizicheskiy
Institut pr! GorIkovskom universitete
(Scientific Research Radiophysics Institute of
Goy'kiy University)
SUBMITTEDs April 7, 1960
Card 7/7

//;4 112- 2n67
7/0 (1041) 7) S/JL41L/60/OO3/Oo6/oo6/O25
(,vco /0,94 E032/EIL14
AUTHOR: Stankevich
TITLE: Fluctuations in the Radio Emission of the Atmosphere
PERIODICAL: Izvestiya vysshikh uchebnykh zavedeniy, Radiofizika,
ig6o, Vol-3, No.6, pp. 969-975
TEXT: A calculation is reported of the mean square
fluctuation in the effective temperature of the radio emission of
the atmosphere T2
a
It is shown that for wavelengths of about 3 cm the fluctiations
are given by
o.o18 OK (33)
'17Ta Vcos 0
where is the zenith angle (< 850). This formula is a special
case of a much more complicated formula derived in the present
paper which applies to other wavelengths also. The expression
obtained for 2
@=T @
a
Card 1/ 2

2U67
s/141/60/003/006/oo6/025
E03 2/ El 14
Fluctuations in the Radio Emission of the Atmosphere
may be used to estimate fluctuations in the aerial temperature of
radio telescopes when the width of the polar diagram does riot
exceed 201. The paper is entirely theoretical and the derivation
is based on the absorption coefficients obtained by S.A.Zhevakin
and V.S. Troitskiy (Ref.1), J.H. Van Vleck (Refs 2, 3), water
vapour concentration given by V.I. Tatarskiy (Ref.4), and the model
of dry standard atmosphere put forward by A.Kh. Khrgian (Ref-5).
AckTLOWledgements are expressed to V.S. Troitskly and V.A. Razin
for discussions and valuable advice.
There are 6 references: 4 Soviet and 2 non-Soviet.
ASSOCIATION: Nauchno-issledovatellskiy radlofizicheskiy institut
pri Gor1kovskom universitete
(Scientific Research Radiophysics Institute of the
Gorlkiy University)
SUBMXITTED: June 7, 1960
Card 2/2

87247
f9*7 S/033/60037/oo6/oo6/022
3,1730 9) E032/E5lf4
AUTHOR: Stankevich, K. 5@
TITLE-. Monochromatic Radio Emission by Interstellar Molecular
Hydrogen Ions
PERIODICAL:Astronoinicheskiy zhurnal, 1960, Vol-37, No.6, pp.983-987
TEXT: The increased sensitivity of detectors used in radio
astronomy naturally leads to searches for new lines in the rcdio
emission of the Galaxy. In this connection it is of intorest to
consider the possibility of detecting the radio emission of H + and
2
H2 since these ions should be present in interstellar gas in
appreciable concentrations. The present paper is concerned with the
calculation of the transition frequency for the hyperfine
structure components of the ground state of ions of orthohydrogen
H The calculation is based on the non-relativistic Hamiltonian
o@talned by Frosch and Foley (Ref.2). The calculation takes into
account the interaction between the electron and nuclear magnetic
moments and the spin-orbit coupling. The wave function for the
7, state of H' is obtained using the Heitler-Lbndon method (linear
combination oi ls-states). The +transition frequency for the
hyperfi-ne structure levels of H 2 is found to be 1174 + 1 Mc/s.
Card 1/2

87247
S/033/60/037/006/oo6/o22
E032/E5i4
Monochromatic Radio Emission by Interstellar Molecular Hydrogen Ions
The numerical calculations suggest that in measurements of the
absorption line in the spectrum of Cassiopeia A one can detect
s + d t 1::@" 18.
.3 NH 7-10 Hagen et al. (Ref.7) have shown that measure
0 2
ments of the hydrogen absorption line in the radio spectrum of
Cassiopeia A give NH df_!5@ (2_4)_1021. It is thus to be expected
0
that using modern radio telescopes it may.- be possible to detect the
radio emission due to molecular hydrogen ions, provided its mean
concentration is at least 0.2% of the atomic hydrogen concentration
in the medium. However, hydrogen occupies all HI regions and H + is
. 2
found only in the boundary layer, Such an average concentration is,
therefore, not very prob@zlole, There are 9 references.- 4 Soviet
and 5 non-Soviet,
ASSOCIATIONa Nauchno-issledovatellskiy radiofizicheskiy institut
Gor1kovskogo universiteta imeni N. I. Lobachev-3kogo
CARD 2/2 (Scientific Research Radio Phy5ical Institute of the
Gorlkiy University imeni N@ I. Lobachevskiy)
SUBMITTED: May 17, 1960

STAMIVICII,, K,S.
Sensitivity of radiometers with paramagneti-c amplifiers. Izv. V7VQ
ucheb. zav; radiofiz. 5 no.33609-611 162. (M.ERA "-;5:7)
1. flauchno-iosledovatellskiy radiofizicheskiy insti-tut pri GorckovskCM
universitete.
(Radio measurements)

STANKEVICH, K.S,
Some remarks on N.A.Armand's article "Fluctuations of atmosDheric
thermal radiation on centimeter and millimeter wave lengths."
Radiotekh. i elektron 7 no.71l255-1256 162. (KRA 15:6)
(Atmospheric temperature) (Solar radiation) (Microwaves)
(Armand, N.A.)

Preciae measurements of the spectrum of the discrete source
Cassiopeia A on centimeter wavelengths. Astron.zhur. 39 no-4:610-
622 JI-Ag 062. (MEU. 15:7)
1. Radiofizicheskiy institut Gorukovskogo gosudarstvennogo
urAversiteta imeni N.I.Lobachevskogo.
(Stars-Spectra)

AMMION. RRi AP3004850
p:@int being useafor all wavelengtbs ,:'-The receiver used was: &'vIdebqw(`modulaiid
tl me with sensitivity of 0.3-064K at a-16-see time constant. @ Compensation for..
U
gm
.Tr rature drift in the antenna and-its cold standard was provided by 'a g" -.dI
charge tube fed via directional doupUjr to the antenna,-: a@ further correctioA was-
Vide for the difference in steady-state baqkgmund, noise levels existing betvas
iWe measured source and its- reference poixti Absolute 'calibration'of received'
31Igne-la was made against radlitior't from a black-body disk "Moon!':'el, tii type
Wied earlier by.Krotikoy et. al. @ @@(Jzvel V*6sh uch.. zav... - R&Uofizwi
4,'@,
,
'
'subtetded an angle of 56.* 1 and-
in similar:zeasur6ments-, vhich,
@
104
j
(1961))
.
.
z0fi-,to Mi - jladiati6n
vos - elevated- 260. abow tIm hori nimize diffractimi,offects.-

id.@121C de
-:re.U-. 10ave I Vbile _,
r"
+A rAture of-tbe,disk. pending on 161no,
MI
:
aciurce r&iiatio*na,- vere ii @6 @bk rangea- The:results are tabulated, gjvIU&
b6th absolute flux density-aud, density, relative to the particular reference
ceilibration area. Flux density tended to -increase with longer vavelejigths and j
wels generey greatest from the Cas-A sorxce with a measured-iaximum of about.
-
;
-2
@
2
-i
4:
@ i
d

a maxi-
cm,'. The
the
ha
t
ms
errors are included;
50 x 10
w/m
leps
530
man calculated to be +10.5%. Thd coordinates of sources and reference- areas
-
ors are, deeply . grateful, to Ya. M. Parnas and T. V, Shikins I
eqrs given. "The autli
xmiier vhose direction the coating for the black-b d 4r ared and.

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AliSOCIATION: Radiophysical Scien

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ASSOCIATION: Nauchno-issleclovatellskiy radiofizlcheskiy institut pri Gorlkovskom@

un!lversitete (Sclentific Rese"ch-Institu-Ce of iMjo 11hysics 'ity)
, GorLk& bivers

SU.IKMD: 2@jan63
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SUB CODE: 003
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STANKEVIGHY K.S.; BONDAW, L.N.
Fluctuations In atmospheric radio emission. Izv. vys. ucheb. zav.;
radiofiz. 6 no-4:669-673 163. (MIRA 16:12)
1. Nauchno-issledovatellskiy radiofizicheskiy institut pri
Gortkovskom universitefe.
-
@ :@;@ I II - , . ': -

ACCESSION NR: AP4017031 S/0141/63/006/096/1.098/1102
AUTHORS: Lastochkin, V. P-7 Si,ankevighi- K S.-
TITLE: Measurement of the absorption,,coefficient in th6 atmosphere
in the decimeter radio band
SOURCE: IVUZ. Radiofizika, v. 6, no..6, 1963, 1098-1102
TOPIC TAGS,: radioastronomy, radio emission from sun, radio emission
absorption,, decimeter radio band, absorption coefficient, solar
radio emission, solar radio emission absorption
ABSTRACT.* Radio emission from,the suti was measured wit@ an 8-meter
parabolic antenna at 25, 32.5,'44.3, nd 56 '5 cm. Error-s due to
the variation of the apparatus parame ers were eliminathd by cali-
bration against radio emissionfrom a..nearby mountain, @hich was
found to be almost absolutely ];lack to" the radiation. @bsorption
at the zenith was found to be 0,.05 dB at all wavelengths. Addi-
tj
Card

A
N
ACCESSION NR: AP4017031
tional checks were made against the intrinsic radiation of the at-
mosphere. The absorption in the atmo@phere was found to be linear
with the cosecant of the elevation angle within the range where
the effect of the antenna side lobes could be neglected., but the
experimental values exceeded t@ose calculated by the Van Vleck the-
ory (Phys. Rev. v. 71, 413, 1947), by an approximate factor 1.8.
The discrepancy is attributed to Van Vleck's erroneous assumption of
a continuous energy spectrum for the oxygen molecule. Orig. art.
has: 1 figure, 9 formulas, and 1 table. "The authors are sincerely
grateful to V. S. Troitskiy for interest in the'work and for valua-
ble remarks."
ASSOCIATION: Nauchno issledovatel'skiy radiofizicheski@, institut pri
Gor'kovskom universitete (Scientific Research Radiophysics Institute
of the Gor'kiy University)
SUBMITTED: 04Jan63 DATE ACQ: l8Mar64 ENCL; 01
SUB CODE: PH, AS NO-REF SOV: 002 OTHER: 001
Cord 241-

S/033/63/040/001/002/016
C-032/E314
AU'JJ10RS: Lazarcvskiy, V.S., Stankevich, K.S. and Troitskiy, V.S.
TI'PLE: Absolute precision measurements of the flux density of
the 3.2 cin radiation from the Crab and Orion nebulae
11SRIODICAL: Astronomicheskiy zhurnal, v. 40, no. 1, 1963,
12 - 16
T ELI T The f lulvl density due t o the discr'ete source Tau A
and the Orion nebula was determined absolutely, using the method
dezcribcd by one of the authors at al. (I:zv. vyssh. uch*zav.,-
Rauiofizika, 4, no* 6, 1961), in 'i-ihich, the received signal is
conipared urith the thermal radio emission of a perfectly black
disc placed in the Fraunhofer --zone of the ant*enna. A parabolir-
antenna, 4 in iri diameter, x-ras employed. The beamwidth at -half-
power points vi-as 571 and the real sensitivity of the radiometer
at a time constant of 64 see was 0.2 OK. Measurements on the TauA
r .1 d i a t ion were carri ed out at d1f f erent parallactic angles - It
was assumed that th .e degree of polarization was 705"1 and that the
position angle was 1480. Since the reception was carried 6ut with
horizontal polarization,the observations had to be reduced in
Card 1/ 2

K117DVLEV, V.V.; STAN,KEVICH.,_.@-,,�-,,
Effective height of absorption of radio waves in the centimeter
band in atmospheric oxygen and water vapor. Izv. vys. ucheb.
zav.; radiofiz. 7 ho.1:175-176 164. (MIRA 17:3)
1. flauchno-issledovatellskiy radiofizicheskiy institut pri,
Gorlkovskom universitete.

''ACCESSION NR: AP4024478 @S/0141/64/007/001/0175/0176
AUTHORS: Kuzovlev, V. V.; Stankevich, K.,S.
ITITLE: Effective height of absorption of radio waves in the centi'
meter band by atmospheric oxygen and water vapor
SOURCE: IVUZ. Radiofizika, v. 7, no. 1, 1964, 175-176
q
TOPIC TAGS: absorption, absorption by oxygen, absorption by water
vapor, radio wave absorption, decimeter band absorption, effective
absorption height, absorption height seasonal variation
ABS'PRACT: It is found that for a real pressure and temperature dia-
tribution in the atmosphere the effective ;ibsorption height of oxy-
gen is not constant, but subject to seasonal variations amounting
to 5 � 0.2, 3.9 � 0.4, and 4.6 + 0.2 km in the summer, winter, and-
spr.:Lng or fall, respectively. The-reason'for the seasonal variation,'I
is the dependence of the effective height oin the earth'a surface
LCard 1/2

ACCMSION NR: AP4024478
temperature. The effective height calculated for water vapor shows
no r(itgular behavior and has an average value of 1.8 km. The use of
the effective height becomes unadvisable during the time of c-M in-
version. Orig. art. has:.l figure.
ASSOC.IATION; Nauchno issledovatellskiy radiofizicheakiy institut
pri Clorlkovskom universitete (Scientific Research Radiophysics In-
stitute at the Gorlkiy University)
DATE ACQ_- 1SApr64:
SUBMITTED: lOJun63 ENCL: 00
SUB CODEE: AS, PHI ".NR- REP: SOV: OTHERs 001
Card 2/2

ACCESSION NR: AP4039719 S/0141/64/007/002/0202/0207
i
AUMOR: Stankevich, K. S.
TITLE: Radiation spectnn of the discrete sources Cassiepeia-A ard Cyfpus-A in the!
centimeter and decimeter bands
SOURCE: IVLrZ. Radiofizika, v. 7, no. 2, 19649 202-207
TOP,rC TAGS: radio astrmany, radio spectrm, discrete radio source, centimeter
wave, decimeter wave
ABS'MCr: The latest absolute maasurements of the radiation fluxes f-r(M Cassiopeia!
A and Cygnus-A obtained at NIRFT and elsewhere were analyzed and canpax-ed. In
order to check on a hypothesis advanced by the author earlier (Astrcn ;:h. v. 399
609, 1962) that the spectrm of Cassiopeia-A beccmes steeper in the centimeter bandi
It is shown that the spectrun deviates appreciably ft-an the simp16 relation AvI
previously proposed, for whereas the range frcm 3.2 to 25.2 an can be well des-
cribed with a spectral index a = 0.87, the transition region between 2!;.2 and 31.4,1
an corTespands to a't.- 0 it is shown that while a full theoretical expli-viatim of
this singularity is 'c'Rfficult, for lack of data an the spectrm in.the range 21
10 an and particularly of wavelength 3 on, sane qualitative. interpretaUmn of the
1/4

ACCESSION NR: AP4039719
observed spectrum of Cassiopeia-A can be made by assuming a radio emission spectrum
described by a single spectral index a = 0.8 over the entire range, witli the devia-
tions in the interval from 30 an to 3 aa regarded as supplementary radiation super-i
imposed on this spectnn. Estimates give a value a2 = 1.8 for this supplementary
ra.diation index. In the case of Cygnus-A the radiation spectrum has an index that
increases continuously with frequency, without any kink, fran a = 0.75 in the meter@
band to a = 1.5 in the centimeter band. Such a radiation can be interjp.,eted as
being due to a stationary electroi canponent and "relic" electrons. 1"nie author is,
grateful to V. A. Razin for a discussion and valuable rermwks.: Orig. art. has: T!
i
f
gures, 2 formulas and 2 tables.
ASSOCIAMON: Nauchno issledovatellskiy radiofizicheskiy institut pri Q:r1kovskcm
universitete (scientific Pasearch Radiophysics Institute at the Gor'kiy Univwsity):
SUBVILITE 21Jun63 ENM: 02
SM MrC.- AA NR IMF SOV: 014 VIHM: 006
COM 2/4

ACCEsSION NRiAP4039719
Spectrum of
discrete source
Cass:LopeJ--A in
the centiweter
and decimeter bando
%Oard
3/4
Nee

ACCESSION ICU AP4039719 ZNCLOSURZ t 02.
off -.-Spectrum of the discrete
source Cygnus-A.in the
centimeter and decirnetei@
bands
JIM
Card
4/L;

.LASTOCHKIN, V.P.; STANKEVICU, K.S.
Experimental determination of fluctuations in the temperature of atmos-
pheria radio emission. lzv.vys.ucheb.zav.; radiofiz. 7 no.4.,7139-70,0 964,
(MIRA 18 -. 1)
1. Nauchno.-Issledovatellskiy radio.flzicheskly institut pri Gorskovskom
universi. tete.

LISTOCHKIN5 V.P.; SORIN. Yt:.M.- STIANKIDTI.Ch, 'K.S.
of rad-io emi-55ior- of t'he dis,,7z-ate saurcj of
L.,@plljs-A. Alzi-tron. zhur. L'I
1. Aauc@n, 0--i @@ Ole-dov ate 17 [e-mail] Inst-itut P--"
uroll-o-skom wi@*hersite`a.

'A
L 34469-65
ICCES11' ON UR: o6030@`
AP-5 0
i 2

.l
ISSOCIIATION. Nauchno a
--19 ledovate! IS* -racliofizicheskiy- institiit-Tri: Gor 1-koirskom- - -
.6iversitete (Scientific- I@e'search Institute of-Radio P4ysics a@ Gorky Sta
te
Univ irsit
SUBMITTED: -.16Apr64 ENCL: 00 SUB @CODE: FA Ec

NO FMi SOV4 001 000
' SS
ATD PM
, 3213

[,:",.,'3 TO Ci I 'UN, -',r IF.; ST A N.' V I Cif
Metisurf,,rrertL of at.,,nospheric ru'dic wnave %h-:1 -w1i'velell-t",
3.' cri. iz-.-. v-vs. uaheb. rad4 f-' 7, '1 r.r-
1. Nauchno-issledovatellskiy radlofizicnl@-kfy iinz@titut pri
skom unlver,,;itete.

F.' If S. k. STANKEUCH ,
K. S.
Measurement of radio wave absorption in the atmosphere at an
altitude of 3200 m. above sea level at a wavelength of 1.6 cm.
Izv, vys. ucheb. zav.; radiofiz. 7 no.6:1186-1187 161*.
(1,11FA 18:3)
1. Nauchno-issledovateilskiy radiofizicheskiy institut pri
Gor-lkovskom universitete.

a do-at 7 skly radl n-f-'-.z'

FL-7870-66 -EWT(~)/FBD/EWT(-11/-]~jgr.(k)-a
ACC. WR: AP5026722 WCE CODE: UIR/0141/65/008/005/1044/104
@ K
atik
v
v
Ul
k
h
Autim K
D
r
t
V
P
S
t
l
o
an
ALe
oc
e
ev
r
.
,
.
d
.;
.;
,
Ep
@
.
ORG: ft ific-Researc A Physics at Goltr Un veisi y qAS@
Ulauchno-issledovatellskiy radiofizicheskiy institut pri GorIkovskom. uriversitete)
TITLE: Measurement of the absorption of decimeter radio waves in the e;tmosphere -Z7
- lo44
SOURCE: IVUZ. Radibfizikep v 8j.' no. 5. 19650

TOPIC TAGS: radio astronoWq atmospheric radiaiion
, radio wave absprption, deci-_
.
meter wave

ABSTRACT: The vertical distribution of the temperature of the intrImsic radiation
of the Atmosphere was measured at engths 16.3,, 18*9.*
wavel 21 and 30.6 cm in the
altitude range from 5 to 306- The directivity patterns of the antenna system at
half-power level were 241, 30's 351., and 401. The brightness temperatiwes of the
atr;Dsphere were determinedly comparing the antenna temLperatures for. sIIFM&lS ftm._
the' atmosphere with the disetete source CassioDaeia-A. The t6tal ibsoi-ption.:,"
-the
at the zenith could be dertermined f@rom the meawared and theor6tical'yalues of
arrt'enna temperature as a function of the altitude angle, 7he total'absorption.
the zenith direction was found to be o.66 db 115% for all tempersitiWeap 00=68-

Card uDc:. 621.371.166---

Acc: "50L,6?22
-'th'
-i poniLing to a zenith temperature f 4.1K,forlhe emission ftca. 6% a1bg0jelmans-V
lp
OrJ.ig. art* has, 2 formu3A
.10 1

SIM;,, CODE: .,03s-*.17/, SUBM DATE-.. 23APr65/ ORI RU: - W2/
G

f 7"

Card 2/2

4
-5 r D/Ftl UVjWul )/EFC- Gl/ws-4
i@ 63ogi
-
-NK
PIMSnMr AP5020354 UR/0141/65/008/003/0437/0440
523,164,4,
N. H.

I _Pdarl L. N ]@rotikov,. V. D.; Stankevich, K@:: S Tsey-t1jr-,
AUMOR: q
5S,
'in the de@
Tili me rem vas
jLE: Spectra of-so nants of.superno -imeter band
SOrjRCE! IVUZ. -Radiofiz.ik4, v. 6 no. 3,' 19655 437@440
TAGS-: ra-1116 -al-f.

TO1*jIC 8 ron
eter:w
omv. decim tect@um ana ys-isi
aveO
@pernqva_
q
..
- ._,._,
_
.
T
12-
@
tigaied.
ources SN 1572 IC -443, and- V1. 44 were inves
ABSITRAM The ;pectra of,s
decilmeter band.frequencies oAl@, 960; 740 'and -513: tic,
using a - radiometer withl-.4 sens3.--
4
tiVit)r on th ord- s n e-constant and a nearly linear'response
e. er of -19K at a-1 eco d-tim -

It--was
ndthe working@portion of its dynamic range., against Virgoi 9
Cyg@aus-A, and Cassiopeia-A. :@Extended s6urces--IC 43. __V_ 44- bad _identical_spectr@
-and,
indices in the-decimeter-and-meter bands- but-SN-1572 exhibited- a @diffdrent-
t IL index in the region,frcrai%178 to.,513_@Mc (&=_-Oi23) -than in:the rest: of ,the.'metdr -'@-,
anddecimater bands, (d= 0.68) *:_.Tables, cite data foi- 960, 740i.and 5 13' mc.@ Orig
art: has: 2 tables.

WsM ra@d 6@1 'ch ki nstitut,' 'or kovs om

ASS715@ b`IATIGI: Hauchno issledovate xy i izi es
pri
3.y 77@

-tDIEWT(l).. Q11VIS-2
_&6 _F ------ 7@*
ACCI.SSION NR: AP5020672 UR/0033/65/042/004/0705/6708:
523.164.42
AUTHOR: Lastochkin. V. P.; L!OLis,_R. B.; Stankevich. K. S.; ToS3ttlin K. N.
TITLE: Using lunar occultations to study the Crab Nebula
SOUR.CE: Astronomicheskiy zhurnal, v. 42, no. 4, 1965, 705-706
TOPIC TAGS: radio astronomy,"nebula, lunar phenomenon
ABSTRACT: During lunar Occultationef a discrete source, the rad,io,waves emitted
ky 1:,@@e source are diffracted by the surface of@the moon, and an observer on the
earth slees a distribution of intensities -which corresponds to the Freanel diffrac-
tion region. ft occultation can be considered as a diffraction on the edge of an
infinite half-screen. The width of the interference bands gtnerat#-doby-, supertd-@..
Isition of the diredt raym and those reflected 'from @_the: -spherical lunar..surface,,lin...
Ja plune ijerpendi-cular ..to -the.-incident rays and pas&ing.thr9ugh the.center of _the,-\'
moon,, going
4a
2
-(vheve, a is the. radius. of, the@ moon);, to.. smaller -.by qjj qt
f
LCard...!/

L 1940-66
ACCESSION MR: AP5020672
the first Fresnel zone VTR (R is the distance to the moon)j, and
consequently the average distribution of the field cannot be alteredby possible
Interference effects. Experimental data on the distribution of:intensity, during oc@_@;:
cultations of a source with extremely small angular dimensi6ns agree well with the,
diff-iiiiction pattern of an infinite half-screen. Ordinarily# the antenna is directe
toward, the discrete source during observation of an ,occul@ation, so that@ 1 the moon@ id
a mov.1.ng screen. If temperature changes in the antenna due to passage dfAhe7lZoon
throuj@,h the'-radiation pattern --during occultation.--of'the sotirce are disregarded,theri
.the antenna temperature is.prpportional to:
TA F (0. 4p) 2'(0, q) 1(9 x, 4p) A dip,'
where -the 0 axis is along the direction of motion of the.sourceo F(69 Is. the: an.;.
tenna pattern, T(e, 4) Is the distribution of brightness from the eouj@m and
10- at,) 4) is the distribution of intensity from a point source for.the citse of di
fraction on the edge of an infinite half-screen.
nR t
X X
1`0 x) (0 2
41

Three occultations of the Crab Nebula by the.moon wer.. observed at'535
Mc. These occultations wpre used to obtain data on the angular dimensions of the
nebula and on the shift of the effective emissionzenter. The position of the
emission center for the nebula is given in Table I of the,Enclosure,,where a and 6
.;iven for points of the source -located on the intersection of-thei., source,
a
re 1;
directiow. of mobion with the edge of the lunardiB!E. "The authors are sincere13
gratoful to A. G. Kuntgevich5gnd V. S Lazarevskii,@Idr making the astronomical cal,
culations, and to 0. N. Shipule6ind G. N. Nikulin'for help In making the measure-.:
utents.11 Orig. art. 4 figures, 6 formulaeg 1 table,

@T vs-,.,r@',f@,@,

_L_ 1940-66
ACCESHOK MR: AP5020672
ENCLOSURE: 01
Table 1.

Transit time of AngUar PositIonal

Frequency, Pic the edge of the diamete
r
-Oc
cultation
moon through the
(1950)
(1950) angle

center of the-: 7.
source

535. h
18 509
OIP30f 9
10.-2
21059!4
:5.5f@_
746

20 07M-3*
5-3P20t
3 '0* 128 21959!3 @-5.5#
2780
180
4 005
5 3jr J4
3
t
0 4
21059!4
5 1.
1080

60

15 0770
M
5.31 2

9 6

to.4

21059 3 0

236.
412
:1270

I cord,4114

2-9195-66 EWT(I)/T WR
ACC NR: AP6008281 SOURCE C OD r,: UR/O 109 /66 /011/003 /-0451/04.515
AUTHOR: Stankevich, K. S Tseytlin, N..M.
ORG: none
TITLE: Effect of exciter defocusing on the accuracy Antenna measurements
S,:',',URCE: Radiotekhnika i elektronika, v.@ 11, no@ 3, 1966, 451-455
a, antenna calioration
TOPIC TAGS: antenn
',A:BSTRACT: Varia1ion of maximum antenna gain with distance is considered for
'V;:Lrious values of the phase error at the aperture which may be c-aus ed by an out-
i of-focus condition of the exciter. Small error in conventional antenna measure-
mehts at R @@ ZD 21 X is ensured only with cophasal irradiation of the aperture (the".
exciter situated in the mirror focus). In real antennas, an out-of -focus condition,
changes the gain ratio G /G.. which must be taken into account in accurate
Card 1/ 2 UDC: 621.396.67.012.12

L 29196'_66 E@.1T(d)/EWT(1)/EEC(k)-2/FCC GVI/V'S-2
ACC APt")008260 SOURCE CODE: UR/0109/66/011/003/0,445/0450
_33
I S
0,U]"HOR: Stan:@e@vich 1@.
ORG. none
4
TITLE: Absorption of centimeter and decimeter radio waves by molecular oxygen
in th.-! @jtn2ospljq
SOURCE: Radiotekhnika i elektronika, v. 11, no. 3, 1966, 445-450
TOPIC TAGS- radio wave absorption. aimpspheric p i c-a
ABS'f,'RACT; The J. H. Van Vleck ronresonant relaxation-type radio-wave
absorption theory (Phys. Rev., 1947, v. 7 1, no. 3, p. 413) is disputed. The
absorption observed in practice can be better explained by aspin-spin interaction
between oxygen molecules. Careful measurements of absorption at 8, 9. 10, lis
12, 13, @'4' 15, 18. 1, 2 1, Z5. 7-cm wavelengths were conducted using the same

L 29l.q6-66
IT =-AP6008200
method for all wavejengths. The effective altitude of the absorbing atmosphere,
largely dependcnt on the atmospheric temperature, equals H,tj - 5:t 0. 2 km for
summer and 3. 9 10. 4 km for winter (Van Vleck's H 5. 3 km). New measure-
ments at 10 cni conducted by radio -astronomic methods at sea level and at
3. 2 km above the sea level yielded H,)j - 4 km. Using the latter value as a basls'@@
new values of total radio absorption in the atmosphere are given (tab6lated) for
3. 2-58. 2-cm waves. Orig. art. has: 1 figure, 19 formulas, and 2 tables.
SUE, CODE: 04, 09 SUBM DATE: 25Nov64 ORIG REIF: 008 OTH 004@
Card 212 4

STAMENVICH, K.V.
Characteristics of new sumer varieties of apple. Biul.nauch.-
tekh.inform.TSGL no.2:24-28 '56. (MIRA 1@:I)
(Apple--Varieties)

STANKEVIGH, K.V.
Characteristics of now fall varieties of apple. Biul. nauch.-takh.
inform. TSGL no.4-82-8? 15?. (MIFU 12:1)
(Apple--Varieties)

STANKEVICH. L.
An improved inspection pit. Avt. transp. 34 no.7:34 Jl '56.
(MLRA 9:10)
(Automobiles--ftintenance)

ST.AM=Ic@,, 1-.. A.
STAMVICH, L.A.; KOVALIKHIIIA, N.Y., tekhnicheakiy redaktor.
@: i 7
[Efficiency and inventiveness In road construction; the repair
of road building machines) Hatelonalizatelia i lsobrotatellstvo
v doroshnom stroitallstve; remont dorozhnos troitelL, nykh mashin.
Mosk@a, Izd-vo dorozhno-teuhn. lit-ry. 1953. 58 T-Y. (XLRK 7:8)
(Road macIninery-Repairing)

LJ
c D *
n s
L u t I

IT (0) SOV/16-59-@-47/47
AU?HOR, GL-.1-r.rb, Y..K.

TITLEI Th
"r.i.i- R.p.bltc.. Scimnttfl. -d Practical Co.f.r..c.
:
th Eti *log Y. Laboratory E;ld..I-Iogy and Prophyl-1,

r'r.13 D
o
rPidmo Hepatitis (Botic.I....
Kz
PERIODICAL,
'
Zh mal mihrabloloelt i i ... 1959.
'
p
;r
g,pp 155-1 57 (US@R
)
A33TRAC?i *he Htpubllcan Con'drence, oz Epidimic Hepatitis was held I
h
-
8d.oao, froz 2 - 10 D.-o--r 11@1-5 ...4 -a tt.nd.1 by "D p.
son . --inly practi.1,.4 fro.
Ri.:1 stution., ropro!ionta.-tv- of all %he Ukr.L.1..
1*qy -1 '... or the
cf
-d
.icr- biI
pid.zi*lcgy
t:
.
t. .In ddt I.. d@1.4.. at, @dd from the In.t%tut" of
'
'
VI u Dtj;&:dG of be U
rology and Infactiou z t.N, USSR, tho Lonin-
gmd.kfy institut oysper-att!'m4y nedit.iny (Initit4to of Ex-
p.ri.ontal X.41.in., Lnx.jr.4), tl-. Lm.Injrx.d.kty ..mLt@r@o.
gigiyvnicheakly medit3inak-y tAstttut- (Sanitary-Hygri-
I ln4titt . L-in red), a- a!.. tLo, U.s.o., Ut..k, T-hk-t,
us
-
4
d
Card 1/4 I ,.
k,
.As
Ibi I, G r- j, Chit .tknatad mcrilh%barovsk Institutes of
Spidwalology and Microbiology and Institutes of Vaccines and
1:,:r. 'he Con.1* ..... h.--,12 p-1-r:.t@.@'Id;d'b%on6*n-
ti:!l,
or. u htd on, u!.$
Ppr he I iI n oa g.t
of :.d..io hopatitim in da,volopirw chick bry" H-
U h racko), in h-n dabry@- i. t. ;'.". ":.u.
Mingradl and I. zp Is h- ... (!!.N.
_Zlkgu and I.A. Kara..,., Tashkent. -:L@ on
the co.pI*me-.V-rr.-.-nMr-r.. I in with no n.bacturial adsorbent for
the specific diagnosis of ;:tlom.a di.ease. Verifying obser-
totion wort "do by N.D. Pr kury.k... and Is.C
'Lou'aloov: thf1o'bor'notitut -=fojgtsimm=ykh bol:znoy ( In3tit4to of
I r.osious Di.a.... ) or 1h* ANR' ZSSR . by 1.1
ik r'@'Ih*vchmnlo ("iy.,),
S.K. K.rap.ti (L-ing ad), 14. Ater. (Cy)- St-
V:.o a (Ashkhabad). Ac.ordlma to the Od.... I.-tz"u"t'. Ii"Ept-
4 1Mogy and Utcrobiology, this can bo used for dat,c-
ling virus antigen in faces (r*.Y. Lycnovskaya) and detecting a
C.rd 2/4 rise in the fixation antibody titer in patients (0.11.
3.2.t.ky,s). )1'V. B.Zalytz end q-1, 3ing " (U..c..) p.k. on
th "Ll"" -h @ldolAtl,"Y, K'@@
..Ir:So) 7.k on the di: of d.,.r.
n. Prof jolj@@ ..In (L ni.gr.d),
) .I.;, _-
V-prop:trovok)
botki.-. dt ...... Y. 1'.
Wake a. o(xllYv,) spoke 0 1 the a-
12 ___r r (0d:f )fectt___ pi
text as&Ion _rTlr_aay@ T-";i:
ran non41 ......
pr.-
.. c.. of droplet transmission of in.
or, on
faction. Corresponding M-bor of the &UN, USSR, Prof ... or N.@.
M-ikin and A.P. 4 .... :tr.,t,.d the pid-L.-
and jaundicol a. ral of Volkiw.
%KnJ M.-k4-A19jXLD_(qor'k Ly)
dis &.a. lqL Rqa@at"k (Inar1kov)
Card 3/4 -..ris*d the uc.Wisful results of cawis-globUlin tr-.t..nt
oI.pron, 1* had been in ccolo.at with :14-1-h.pa.titl. pati-t..
11, Cc fre@.a.gr..da.%be .*ad f.r. .paho.i,ng the r1J..tf41-
minal inv..ti g. tis@@4h patient. 1. the USSR
of Ho ,:nd for a rono
Kr ph on the tiolcgif-d tki dt ... %..

TISHCHMO, I.T.; -STAMVICH, L.A.
Some epide;@o@logiea@eaftres of'the morbidity of epidemic hepatitis
(Botkin's disease) in Kiev during a six-year period. Zhur.nikrobiol.
epid.i J-w=. 31 no.l-.W-143 Ja 160. (NM 13:5)
1. Iz Kiyevskoy gorodskoy gianitarno-*pideziologicheskOy btaUtOll.
(ray-HwAnns, is ious)

SOFIYEINKOY N.ya.@ sum@!CH, L.A.
Rare cases of typhoid fever complications and their epidemiological
significance. Vrach. delo no-4:136-:M'Ap 1610 (KMA 14:6)
1. Kiyevskaya gorodskaya sanitarno-e idemiologiches-kaya stantsiya.
(TIPHOID FEVER

PANYSHEVA, I.I.; STANKEVICH, L.A.
Indicator method for the detection of diphtheria bacil-U.-Lab. de-
lo, 10 no.3:183 164. (MIRA 17:5)
1. Dorozhnaya sanitarno-epidemiologicheskaya stantsiya Gorlkovs-
koy zheleznoy doragi.

, STANK.EVICHY. L.A.
Clinical characteristics of periodic schizophrenia according
to catamnestic datae Zhur. nevr. i paikb. 64 no.1:85-92 164.
(MIRA 17:5)
1. Dispansernoye otdeleniye (zaveduyushchiy - doktor med.
nauk NA Zharikov) Instituta paikhiatrii AMN SSSR., Moskva.

ZHARIKOV, N M - LEVIT V.G.; POPOVA, M.S.; RATNER, 1.0.; STANKEVICH, JL.A.;
SWbNOVA, L.M.
State of schizophrenia treatment based on data of an.
outr)atlent study. Zhur. neyr. i psikh. 64 no.6;911-918 164.
@ (MIRA 17sl2)
1. Institut psikhiatrii AMN SSSR, Moskva.

L 29:1.88-66 EWT(1)17 A
SOURCE CODE: UIV0016/65/000/011/0138/01 8,:,!@
ACC NR1 AP6019122
S
IoTop, Stankevich. L.A*j Popova, A&:
AUTIIOR: Trukhan, P.T.; Tishcheao.
DobiAovskayat A. R.
ORG:,, Kiev Institute for the Advanced Training of Phvsirjnna (Kiyevskiy. institut.'-@Z_.
miological Station
usairershenstvbvaniya vrachey): Kiev Municipal SdnitaZL-&pide
(Kiyevskaya gorodskaya sanitarno-e heskaya stantsiya); ]Lod o161 skiv
pidemiologic
Area Sanitary-Upidemiologigil Statinn, Xley (Sanitarno-epidemiologicheeka3m
stantaiya Podollskogo rayona Kiyeva)
TITLE: Use of gamma globulin.to prevent-infectious hevatitis-In-c n,.
'groups of-childrene@ b
ResiAts of epidemilogical observations among iie paper
was presented at the meeting of the Kiev City Society of Microbiologista
Epliemi.ologists and Infectious,Diseases Specialists on 30 September 190.
SOURMs Zhurnal ~nd,krobiologiit,'epidoid6l()gii'i-immiiiobiiilogtiono.0 11
TOPIC TAGS: - gamma globulin, hepatitiss epidemiology,, 4-minizationp man
ABSIL'RACTt _jn September 1963 saw 5000-cNadran In nurseriesp kindergartens#f,
sul, grade schools in Kiev were immizedTwith a sIngX* 3 al dog
of humen.
i goina glohilin 'while an equal number aftwed as controls. The observation
period of
months consisted of two intayalst (1) October 1963 to Mar
aml, (2) Arkil too, September 1964. The incidence vj@ hapatitle ONO the
1/2

LYUTKEVICH, Te.K.; STAMVICH, L.I.
The Peatovo-)(aknatikhe uplift on the northwestern spur of the
Moscow synclase. Gecl.ebor. no.3.^169-184 '55. (K6BA 8:61
(Moscow Region--Geology, Struatural)

SUNKEVICH. L.I.
Now data on the stratigraphy of the Lower Ordovician In the
Russian Platform. Dokl. AN SM 105 no.2:343-344 153.(KWU 9;3)
1. Pre"tavleno akad,smikon D.V. NalivkInys.
(Aussish Platform--Geology, Stratipaphic)

STAMMVICH, L.I.
Mineralogical composition of brown iron ores in the Kerch deposit,
Geol. zhur. 17 no.4:23-32 157. (MIRA 11:4)
(Kerch Peninsula--Iron ores)

_TANKEVICH _,,Qvna; DOLMATOV, P.S., vedushchiy red.;
S _,LyudmiIa Ivan
BRUSKIN, D.M., vedushchiy red.; YASHCHURZHINSKAYA, A.B., tekhn.red.
(Key wells of the U.S.S.R.; Festovo key well (Novogorod Province)].
Pestovskaia opornaia skvazhina (Novgorodskaia oblasts). Leningrad,
Gos.na,achno-tekhaicheskoe izd-vo neft.i gorno-toplivnoi lit-ry,
Leningr. otd-nie, 1961. 91 p. (Leningrad. Vsesoiuzny-i
neftianoi nauchno-issledovatellskii geologorazvedochnyi institut.
Trudy, no..182). (IMIRA 15:8)
(Novgorod Province--Petroleum geology)
(Novgorod Proyince--Gas, Natural--Geology)

PEYSIK, M.I.; STANKEVICH, -L.I.; YAROSHENKO, V.N.
State of underground gas storage in the Leningrad industrial
area. Trudy SGPK no.3:103-124 162. (MnA 15:10)
(Leningrad region-Gas; Natural-Storage)
(Prospecting)

"Uperience in OrganizatIm of Hicropetrograph1c Re-
search in Field Parties An Siberia," L. 0. Stankevlcb,
G. 1. Gendrikhovskaya, 3 pp
"Razvedka NeW No 6
Discusses technical problem not in making micro-.
scopic studies a@ rocks during geological expeditiam
LC
57T46

- -W
@;; -I STANKEVICH, L. 0.
L) "COntribution to the Mineralogy of the Sedimentary Ore
eposits in the So-Ahern Ukraine and Crime&.* Dr Gool-Min
sc-131 Moscow State U, Moscow, 1954. (AshGeol, Feb 55)
SO: jum. No. 631, 26 ug 55 - 5urvey of Scientific and Teahnioal
Dissertations Defleinded at USSR Higher Educational Institutions
f14)

STANKSTIC41, L.O.
li-,O"-!P@@---:-,
Calcium rodochrosite in the larch deposits. Dokl.AN SSSR 105
n*.6:1328-1331 D 155. (MIRA 9:4)
l.Dnepropetroveldy gornyy Inatitut Imani Artema. PredstaTleno
akademikem N&M.Strakhe"me
(larch Peninsula-Manganene ores)

STAMVICH.. 3@.O. @
Composition and origin of metalliferous silicates in tho Kerch
deposit. Min.sbor. no.11:159-169 157. (MIRK 13:2)
1. %ran Institut iment Artema, Dnepropetrovsk.
(Kerch Peninsula--Silicates)

STANKEVICH, L. 0.
Doc Geol-Min Sci - (diss) "Mineralogy of Bedimentary ore deposits
of the south of the Ukraine and the Crimea-" Moscow, 1959- 15 PP; ,
Moscow Order of Lenin State Univ imeni M. V. Lamonosov); 150
copies; price not given; (KL, 10-61 sup, 209)
0

STANKEVICH@ L.O.; GEIIDRIKHOVSKAYA, G.Gh.
Calcium rhodochrosite of the Kamysh-Burun trough. Min. abor,
no.l6s435-al 162. (MM 16:10)
1. Gornyy institut imeni Artema, Dnepropetrovsk.
(Kerch Peninsula-Rhodochrosite)

STKNKEVICH, M.
I -- @
@ `.I_:v':;-,, . -
Kaking plain and reinforced concrete products on press-roll
machines. Stroi.mat.. izdel.i konstr. I no.ll:lj-16 N '55.
(Reinforced concrete) (.KIJIA 9:5)

OIANKEVICH. M.10
Use of a fast method for the cy-tological diagnosis of malignnnt
neoplasmse" Lab.delo no.6:13-16 I-T-D 158 (MIRA 11:12)
1. Iz Ob"yedinennoy gorodskoy bollnitsy No.28 (glavW7 vrach N.A.
Pastukhova) Oktyabrlskogo rsyzdrFLvotdela, Moskva**
(GANGER)

STANKEVIGH, M. I.
Cytological study of breast tumors. Lab. delo 8 no.3:22-24 Mr 162.
(MIRA 15-5) @
1. 28-ya Gorodskaya bollnitsa (nauchnyy rukavoditell - dotsent S.L.
Gorelik, glavnyy vrach M.A.Pastukhova) Moskva.
(BREAST--TUMORS) tDIAGNOSIS, CYTOLOGIC)

STAIIKRV K., inzh.
Prested and rolled concrete. Biul. tokhn.inform. 4 w.9:4-?
S 1-58. (MIRA 11:10)
(Precast concrete)

STANKEVICH, M.N., kand.tekhn.nauk
Rolling reinforced concrete products under high pressures. Trudy
NIIZIJB no.21:122-126 961. (FJRA 14:12)
1. TSentrallnaya nauchno-issledovatel'skaya laboratoriya No-3-
(Precast concrete)