SCIENTIFIC ABSTRACT PARIYSKIY, V. B. - PARIZEK, M.

• Document Type: CREST
• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R001239230004-7
• Release Decision: RIF
• Original Classification: S
• Document Page Count: 100
• Document Creation Date: November 2, 2016
• Document Release Date: June 15, 2000
• Sequence Number: 4
• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT

s/i.26/62/013/001/005/018
E021/E580
TITLE
Palatnih, L.S., Boyko, B.T., Fuks, M.Ya. an(.]
Parivgkiy-, V.B.
17,1ectron diffraction study of the substructure of
thin films of alliminiiim, silver and gold, condensed in
V.1clio
PLIUODICAL: Fizika metallov i metallovedeniye, v.13, no.1, 1902,
71-76
TEXT: The influence of film thickness and substrate tempera-
ture on the mean size of mosaic blocke; was investigated in thin
condensed films of aliaminium, silver and gold. Aluminium of
99.999',o' purity and silver and gold of 99.951 purity was used.
Evaporation was garried OV from a cone-shaped tungsten spiral at
rates of 4 x 10- 5 X 10- and 10-11 g/sec for Al, Ag and Au,
respectively. Condensation occurred on a heated glass plate. The
films were separated by immersion in distilled water and caught on
metallic holders of foil containing 0.2-0.4 mm holes. The films
werr examined by electron diffraction using the (220) ring. The
effect of heating the films was studied. The true diffraction
broadening was found by harmonic analysis (Ref.6: B.Ya.Pines
Card 1/3
Inc MOSOIC

Electron di f fraction study s/i ~,6/t,2/01 3/0()1/()Or,/() 18
iw2i/r.ri8c)
Ostrofokusnyye rentgreyiovskiye trubki i prikladnov rentgerm-
stru)(turnvy analiz (Fine f'oeiissing X-ray tijbes and applied X-rav
structural analysis), GITTL, 1955). 'rile main contribiiiiim to the
broadeningr arises from tfie small size of tI)c noaic jijocj~,. Mien
there is a markeo difference in the coefficierits of expari!4iem of'
the holder and the filin, tile 1,)tter is subjected to nl;i~:tjc
del'ur- -ition in the i)rocess of heating which is accompallied hy I
refining of' the blocks. With rapid heating, recyrstallisat iorl
does not remove this effect. Therefore, thermal coefficiprits t)f
tile l'ilm and holding jwiterinl should be approximately eyj;il. .,I III
increasing film thiclmess of aluminium and silver, the
(if tile lines decreases both in tile initial and annealod
COTItinLIOUS hCati.119 Of 1111110.1)itlyn filMS UP to 11;00C in 2-3 mir-) 1-ads
to refining of tile mosaic blocl~s, whereas heating to higher th,)i)
1500C results in coarsening. Heating silver and gold An the region
20-IIOOOC also results in cotirsening. Tile mean linear dimension of
the blocks in alurijinium film is about half that in siJver ano r.(jlfj
filins, and coarsening during heating takes place Jvss inten-sively
in aluminium. The probable reason for this difference is Lhe
formation of' highly dis.porsed aluminium oxide. The mosaic
Card 2/3

A ec troll (1.1 f*f'rac t loll s tudy . . .s/i,.!6/62/o1,r,/oot/o(,),)/oi i~
Eo2i/E58o
!ztrisctm-(- is more dism,rsed in condonsed films than in ordinary
massive samples aft,-r cold defornation. The high of
tho blocks and their strong misorientation call be judged from the
high strength of thin condensv(f filinn. There are If tables.
ASSOCT~TION: Kharlkovskiy poLitekhnicheskiy institut im.
V. 1. Lenina
(Kharlkov Polytechnical Institute imeni V.I.Lenin)
SUBMITTED May 20, ig6i
Card 3/3

24 75
S/l26/6N11/oo6/ooi/oii
E021/
E306
AUTHORS- Palatnih, L.S., Fults, M.Ya., Boyko, B.T. and
Pariyskiy, V.B.
TITLE: -Electronographic Study of Substructure of Thin
Condon-gates of Aluminium by the "Microbeam" Method
PERIODICAL: Fizika metallov i metallove-deni-ye, 196.1, Vol. 11,
No. 6, 1),). 8611 - 669 4 1 pl,atC
TEXT: The electron microbearn is suitable for studying
iiidiyldual reflections froj-.i crystallites of dimensions 100 -
300 A and for e%,ahi-atin-, the relative r,-iisorientation between
crystalliteg. Thus the electronographic, microbeai-,i is a
direct method of observin8 the -ubstructure of crystals.
Aluminium films 60 - 9-00 X thick condensed in vacuo on a
cold surface were sttidied by thi, technique. The filr were
transferred to alumiiiiui.-i foil w:Lt','i ncle, of 20 to 70 J~ .Th e
th:ickness uf t,e film was &,3timated I:)-.- a photometric r-,iethod
with an accurac-, o f 10".'. Photograph~z were ta!-.en in a hi~;h-
temperature electronc)~~raph wiLh electrostatic focusin,;. Tn e
films were 11(,atud at a rate Of -50 0Chiin and electron-diffraction
Card 1/6

24475
5/l26/6i/oi1/006/001/ojj
Electronographj( Study . ... E021/E306
patterns i,-Cre tail-.en at room te!*1:)erature , 200 300, 40o and
450 OC. T~ie mean I inear dimen!3 2on of a colier ent,,r efl ecting
rEgion for filins heated to 400 o C was 1110 - 335 A, This is
sillillar to thc Of bloLks de'terclLned
by X- ray i nv es t i ga I i ,)n a f d ef o rm ed po I yc rv~; t a 1 -9
0
The Debye ring at 1-0 and 200 C appear6 continuous and diffuse.
Heating to 30() OC re~7ults in the appcarance of intensive spots
but the general background 15 still retainod. At 4oo oc this
background is very xqeali. and at 450 OC it di._Qap-)ears, The
number of -,;pots remains practically unchan&ed on increasing
the temperature fromi 30C to 1150 'C' Photo~;raphs are included
for the (111) anq (200) lines taken from a fill-.I 125 X tilick
on an area of 20 -. heated to 300~ 450, 4C)C and 450 0C (X15).
At a magnification of 60, spots of increased blackness can be
seen on the electron--diffraction patterns taken at 20 and 200 OC.
The complete results are tabulated. The mean linear dimension
of the crystallites i,,,as calCLIlated from twc, formulae:
Card L,/6

EIcctrc)n(3,-r~:,-,)hic S-,udy
3
L c D v0
nd
L -- ~v 0/11
.L~75 /
62-4 /001/011
S/126/il 011 00b
E02-1/E3o6
C.- 0 v 1 Z-' i e , c a -.-ulw-ie of t'ie reLi3!- Ljvin~. cohe:-~nt
re'.-Icct4,j,-l5 and
IF,
5:i.~e oC '11:e cr,;:~tal~itcs increases witi-i :-ncrease in
e;'.lperature. The clegree of misor.L ~---itat ion of crystals in
fili-.i-z is ~--o:-.;c.-7iat t:,.-I:i t-,. c v.~' !,-: c s fo r
i i-, --, r ~, c r y:- 4 -- I,, T,-.i~ i.iay t.,e hi".1 rosistanct; to
Aas'Lic Lefjr;;iat1o:, anl-'. :ii-..i rate oC di'L,-,:sion if such fil;-.is.
T:ierc, arE! t,-iblc al.,' 11 rcl~,:.i-cncez3 7 Soviet
aliL 4 ro.: ',oviet. Th- ti-,,o refci-ences
'luoted are: Ref. 110. el, A.,~.. Aoeoucl~, J.S. Pruc. Roy.
--7Z
Card 3/6

24475
El ec trono -ra -,i c Sz _,cly E02 1/ E- o
:3 oc 4 A. 5 , G7 6. Weavei-. C. , llij I , R.1,1. A,._vanc os in
Physics, 1959, V ()1 7 5
ASSOCIATION; Kharihovs~-__iy ~,osu,larstven.-iyy ui;ive~'sitet i::1.
'iar ''. tate University i-,-a.
A.~L. Gar-l:o 0 (K. -0v S
A.1'.. Gor "-.iy)
A-Ili a r I h ov z3:, i ypo1itcl-._iiichesl_iy institut
ij-i. V.1. Lenina (jjia-.-'hov Poly-Lechnical
Institut in. V.I. Leiiin)
SUBMITTED: Januarv 21, 1961
Card 4/6

F
1, 29986-66 EW (1)/EW (m)/T/EWP(t)/ETI IJP(c) JD/GG
ACC RR: AP6032490 SOURCE CODE: UR/O18l/66/0D8/0C4/1227/12,~8
AUTHOR: Par4,yrkiy, V. B.; Lubenets, S. V.; Startaev, V. 1.
ORG: Plmrsicotechnical Institute of low TerWrature!W UkrSSRs Khar1koy (Fiziko-
tekhnichesirdy institut nizkikh temperatur AN UkrSSR)
1~
TITLE: Mobility of dislocatio in single-crystal potassium bromide
SOURCE: Fizika tverdogo tela, v. 8, noe 4, 199, I=-1231) 2,7
TOPIC TAGS: potassium bromide, single crystal, crystal dislocation phenomenon,
shear stress, crystal deformation
ABS7RACT: In view of the fact that the experimentally observed connection between
the speed of dislocations and the applied voltage in these crystals have not yet
been fully explained theoreticallyp the authors have attempted to obtain different
information an the character of dislocation motion in single-crystal KBr, in which
the motion of dislocations has not been heretofore investigated. The tests were
made with annealed single crystals with dislocation density 103 em-2 and with total
impurity content 2 x 10-2% . The d1slocation structure was exhibited by means of an
etching procedure described by the authors earlier (Kristallografiya v. 7, 328,
1962). The motion of the dislocations was observed by applying mechanical loads in
different manners (compression vith a deformation mchineo static load producing
Card 1/3

L 29986-66
Acc NR: m6or4qo
pure flexure in an etchanty pulsed loading of long duration (2 X 10-2 sec and abcrve)
(10-4_3.0-0 r
or short duration 'CC)). In addition, a special system was developed,
which made it possible to produce a rectangular loading pulse and measure the mag-
nitude and duration of the applied load directly during the loading,, and regulate
the applied load (Fig. 1). The operation of the system to briefly described. The
results show that below a definite shear stress the dialocations haidly mavep but
above approximately 80 dmm2 the dislocation velocity increases rapidly and then
increaser, at a slower rate. There was little difference betweed edge and screw
dislocations. The results exhibited a certain similarity with previously observed
data for NaCl and LiF. The obtained experimental dependence of the dislocation
speed on the applied load cannot be described in terms of,'&-s-ingle thermal activa-_:
,tion process with a constant activation volumep since thii-volume-decreases by
approximately 4W times on going from "mall velocities to 3Wger velocities. The
results also confirm the effects proposed by W. G. Johnston and J. J. Gilman (J.
APP1- PbYa- V- 30, 128, 1959), wherein the dislocations are first accelerated
'within a very short path (smaller than I-T p)p after vhich they move uniformly.
The delay of the dislocation motion following application of pulsed load decreases
exponentially with increasing load. Orig. art, hast .9 figures and-6 formulas.
2/3
card

L 29986-66
-Ace m: Ai,5=49o
Fig. 1. Rased loading
equipment for KBr crystals.
I - Force relay,, 2 - time
relay, 3 - paver source,
4 - paver supply block,
5 - tension metering equip- .2 ia'aww" I
ment, 6 - tension gauge, a
3
T kmemtor., 8 - semple,
9 oscilloscope,

SUB CODE: 2D/ SUM DATE: 26j'd165/ ORIG REFs 008/ OTH REF: OOT
Card 3/3 -j6

3"Solut

PAIRlYS1,T'~, Yu. s tarsh y ;a,, sc, trucir,,Lk
.'aciio te les :copes s ',r-n ',c, the
G]avriaya astrcnoi:~'rhes,:aya ob.,3, I-va"Oriya,

PARIYSKIYP Yu. M., Inzh.
Theory of combination drilling. Izv. vFs. ucheb. zav.; gor.
zhur, no.9:106-114 s-&I. (MM 15:10)
1. Laningradskiy ordena Lenina i ordena Tz;ndovogo Krasnogo
Znawni gornyy institut imani G. V. Plekhanova. Rekomendovana
kafedroy tekhniki ranedki.
(Boring)

PARIYSKIY, YU. M.
Cand Tech Sci - (diss) "Study of the performance of boring bit
in rotary-impact drilling." Moscow, 1961. 23 pp; (Ministry of
Higher and Secondary Specialist Education RSFSR, Moscow Geological
Surveying Inst imeni S. Ordzhonikidze); 160 copies; price not
given; (KL, ?-61 sup, 243)

PARITSKIY, YuJI.
Preparation of steel shot boring pollets by meann availbblu
to geological prospecting parties. Sbor.nauch.rab.stud. WI
no.2:?4-85 15?. (14IRh 13:4)
1. Leningradskly ordenov Lenina, i Trudovogo Krannogo Znameni
goriWy institut im. G.V.Plekhanova. Predstavlenr prof. P.A.
ShWphevym.
(Prospectin&-Squipmorit and supplies)
(BoringwaRquirment and supplies)

PARIY T
Breakage of rocks in drilling. Zap. ILI 41 o.2:69-?9
(Boring) (Rocks-Testing)
161.
(MIRA 16:5)

PARIYSKI-Y, YU.M..
Developing theoretical principles of vibration and combination
drilling. Zap. LGI 41 no.2s80-90 161. (MIRA 16:5)
(Boring)

3OV/58-59-12-282G2
Translation from: Referativnyy zhurnal. Fizika, 1959, Nr 12, p 247
AUTHORS. Korollkov, D.V., Pariyskiy, Yu.N., Soboleva, N.S.
TITLE: On the Measurements of Magnetic Fields and Other Physical
Characteristics in Regions O-ver the AungpntA Prnm Redin-
Qh_qPrvAt.1nns ~_/ ~V
PERIODICAL: Solnechnyye dan-nyye, 1958 (1959), Nr 9, P~, 65 - 69
ABSTRACT: A method for estimating the magnetic field, kin-atic, temperat,_-e
and electronic density from polarization observations of the
sun's radio-emlssion, is given for a suffiiiently wide spectral
cm band, using instruments with a high resolving power, For
purposes of illustration, an example of processed material on
the 1959 eclipse Is presented. The possibility of regular ob-
servations of magnetic fields with the Large Pulkovo radio-
telescope, is pointed out.
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30) SOV/33-35-4-16/'25
AUTHORSt Salomonovich, A.Ye., Pariyakiy, Yu.W., Khangilldin, U.V.
TITLEs Observations in the Millimeter Diapason of the Total Solar
Eclipse of June 30, 1954 (Nablyudeniye polnogo solnechnogo
zatmeniya 30 iyunya 1954 9. v millimetrovom diapazone voln)
PERIODICALt Aetronomicheskiy zhurnal,1958, Vol 35, Nr 4, pp 659-661(USSR)
ABSTRACTs The observations were carried out in the neighbourhood of
Novo-Mookovsk (Ukr.SSR) during an expedition of the Physical
Inetitute imeni P.N.Lebedev of the Academy of Sciences of the
USSR. The authors thank Ye.K.Karlova for the preparation of
the.apperatus and for the assiBtance during the performance
of the observations.
The reduction of the eclipse curve enabled the estimation of
the height o5 the effective layer of emission above the photo-
sphere (6-10 km +30%) and the distribution of radio brightness
on the solar disi. The comparison of the eclipse curve with
the curves of Troitskiy, Zelinskay-a, Rakhlin and Bobrik
CRef jy who observed there the solar eclipse in the centi-
meter range, shows a coincidence of some details.
Card 1/2

Observations in the Millimeter Diapason of the SOV/33-35-4-18/25
Total Solar Eclipse of June 30, 1954
There are 2 figures, and 4 references, I of which is Soviet,
and 3 are American.
ASSOCIITIONsFizicheskiy institut imeni P.N.Lebedeva AN SSSR (Physical
Institute imeni P.N.Lebedev AS USSR)
SUBMITTEDs May 30, 1957
Card 2/2

J 0 68154
AUTHOR: Pariyakiy, Yu.N. SOV/20-129-6-17;/6)
TITLE: High-resolution Observations of theladic Source Sa.6;1ttarius-A
PERIODICAL: Doklady kkademii nauk SSSR, 1959, Vol 12c, Nr 6, pp 1261-126'~4
(USSR)
ABSTRACT: In April, 1959 radio sources on the wavelengths 5.,2 and '_..4 Cm
were observed by means of the large Pulkovo radiotelescope of
the Glavnaya astronomicheskaya observatoriya AN SSSR (Main
Astronomical Observatory of the AS USSR), The radiometers
used for their meaiurement huve already been described in 41%,,,o
earlier papers (Refs 1,2). The author s-:)eaks about 4 recoreed
curves of the passage of the radio wave through the diagram
of the antenna on the 3.2-cm wavelength and about 0 curves on
the 9.4-cm wavelength. The averaged passage curves shown in
figure 1 illustrate the complex structure of the radio source
The high resolution of the radiotelescope made It possible to
discover a new bright detail of small angular extension
detail Nr 1~, of an extensive region of about 0 05 in size
detail Nr 3), and, finally, a very extensive radio source ~n
~
the 9.4-cm wavelength and on larger wavelengths (detail _Nr 2)
h43mO8s8 01
Card 1/3 Detail Nr 2 comes from the direction 17 1 (.eDoch

68 154
High-resolution observations of the Radio Saurce SOV/20-129-6-17/69
Sagi t t arl u s-A
1958-0). This is only 158 distant from the ooordinatos of
the galactic center, The flux coming from detail Nr 1 is about
-25 2
15-10 W/M .cps on both waves of the centimeter band, which
indicates a thermal mechanisin of radiation and corresponds to
the radiation of an ionized 6as and a measure of emission of
106 with Te - 10,0000K. This formation may actually be the
gaseous core of our Galaxy. Detail Nr 3 is sharply asymmetric
with respect to detail Nr 1, which is particularly marked in
the 3.2-cm wave, while it is less marked on the 9.4-cm wave, and
hardly noticeable on the 33.3-cm wavelength. This effect ca-r-
be explained only by the complex spectrum of this detail (a
combination of the thermal radiation of an ionized gas with a
brightness distribution similar to the passage --urve atk3.2 cm)
and a non-thermal radiation which concentrates considerabl~-
towards detail Nr 1, The thermal part of source Nr 3 :.s a-,-,;--r-
ently connected with the gas nebulae in the inner sleeve o?'the
Galax,y. The non-thermal component is, however, very symmetrac
with respect to detail lir 1, which is particularly noticeabl,~
on the 33,3-cm wavelength (which was investigated by V ~
Card 2/3 Malumyan). Detail Nr 2 is the continuation of the non-t~_ei-al

68154
High-resolution Observations of the Radio Source SOV/20- 129
Sagittarius-A
component of detail Nr 3, Without doubt, the ent'-re non-
thermal component of the radii*) source is physically interr,?Ia-
ted with detail Nr 1. The results obtained by the present aper
indicate the following: The bright, dense, L;aseous cort? of t1le
Galaxy with a dimension of v 6 parsec is immersed ~ntc th,~
source of a non-thermal radiation, which is highly con~'entrated
towards the gaseous core. Further investigations will maie it
possible to form a judgment ae to the correctness of This model
At present, high-resolution observations are being prepared
at the Glavaa-va astronomicheskaya obsery toriva of the."S USSR
on the wave A,21 cz,. This region must be accurately investigated
also in the optical region in order to be able to studs 'he
distribution of the absorbing matter, The author tharLks S_ E
Khaykin and H.L, Kaydanovskiy f r their instructions, and N 9-
Soboleva for help in carrying out observations There
2 figures and 8 references, 3 of which are Soviet
PRESENTED: August 8, 1959, by VA~Anbartsumyan, Academiciar.
SUBMITTED: July 26. 1959
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3,1710 S/058/61/000/002/008/018
9,1800 AO01/AO01
Translation from: Referativnyy zhurnal, Fizika, 1961, No.. 2, p. 4o3, # 2Zh493
AUTHORS: Pariyskiy, Yu.N., Khaykin, S.E.
TITLE: On Demands Which Should be Made of Large RadiotelescopesProm the
Viewpoint of Radioastronomical Problems
PERIODICAL: "Izv. Gl. astron. observ. v Pulkove", 1960, Vol. 2, No. 5, PP.
27 - 44 (Engl. summary)
TEXT: The authors show expediency of using centimeter and decimeter wave-
length bands in radioastronomical measurements. They discuss comparative charac-
teristics of two types of antenna systems: systems with symmetric diagrams of
directivity and asymmetric systems with diagrams highly extended in vertical
direction. The authors present considerations as to the equivalence of these
systems in resolving po,~er and some other characteristics, if the larger dimen-
sion of the asymmetric antenna Is equal to the diameter of the symmetric one.
There are 16 references.
Translator's note: This is the full translation of the original Russian abstract.
Card 1/1

8`351
S/035/60/000/012/009/029
3, / 730 2.4 // 2 7) // 2 AOO 1/AO0 I
Translation from: Referativnyy zhuimal, Astronomiya i Geode:,,iya, 1960, No.
p. 47, # 12257
AUTHOR: Par
&--A- YW-A~U&
MW
TITLE: Observations of Some Galactic RadioEmission Sources With the Great
Pulkovo Radiotelescope
PERIODICAL: Izv. Gl. astron. observ. v Pulkove, 1960, Vol. 21, No. 5, pp. 45-531
(English summary)
TEXT: The author presents the results of the first observations of galactic
radio sources at the centimeter wavelengths. The observations were carried out
with the high resolving power radiotelescope of the Main Astronomical Observatory.
The observations of the Crab nebula permitted the determination of the angular
1 47
dimensions, coordinates of the radio emission gravity center, and the detect on
an asymmetry of the source. The observations of the Omega nebula showed that an
essential part of the bright emission nucleus was hidden due to a high absorption
of light. A fine structure was detected in the Sagittarius A source; evidence Is
adduced favoring the identification of the brightest part of the source with th-
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87351
S/0 35,/6o/ooo/() 12 /00 9/0 19
AOO I/A00 1
Observations of Some Galactic Raio Emission Sources With the Great Pulkovo Radio-
telescope
galactic nucleus, and considerations are expressed as to the mechanism of the
emission of various components of the radio source. The observations of the 2C
1607 radio source made it possible to discover an interesting peculiarity in the
spectrum of this object radio emission. A conjecture is expressed that this 6air'-f-
is remains of a Supernova of type II. There are ':;0 references.
From author's summary
Translator's note: This is the full translation of the orig:-Inal Russian abs* ra.-
Card 2/2

22094
S/03~1/6 I /000/00_3/~~2,/04
31 1~f-e 0 A00I/AlGI
AUTHOR: Parlyskiy, Yu.N.
TITLE: On the relation between emission of gaseous nebulae in hydrogen lines
and that in radio band. A new method of determining distanCe-sto
nebulae
PERIODICAL: Referativnyy zhurmal. Astronomlya i Geodeziya, 110. 3, ig6i, 47, ab-
stract 3A410 ("Izv. 01. astron. obserN,. i Pulkove", 1960, v. 21,
no. 5, 54 - 61, Engl. summary)
I'M: The author derives basic relation to determine Intensity of radio
emission from gaseous nebulae. Numerical coefficients are determined more precise-
ly. A correlation between intensity of radio emission and emtssion in Balmer
lines is discussed. A new method of determining distances to nebulae is proposed,
which is based on comparison of radio brightness wLth brightnena in H0, , By r7learn
of this method the author determines distances to 32 nebulae, using the known ex-
perimental data, as well as their linear dimensions, electronic densities and
masses. There are 25 references. A. K.
[Abstracter's note: Complete translation]
Card 1/1

31 0/0 S/058/6 i/ow/002/009/018
e'. -/W a AOO I /A00 1
Translation from: Referativnyy zhurnal, Fizika, 1961, No. 2, p. 4o4, j 2Zh50I
AUTHORS: Bol'shakov. N.A., Pariyskiy, Yu.N.
TrEZ: Receivers of Decimeter Band for Radioastronomical Measurements
PERIODICALi 01 Izv. W -a+-(N- ~v-av- v Pulkovo" . 1960, Vol. 21, No.
pp. 162 - 164 (Engi. summary)
TEXT: The authors describe briefly radiomaters of 10-cm band constructed
at the Glavnaya astronomicheakaya observatoriya (Main Astronomical Observatory)
of the AS USSR in 1956-1957. Their fluctuation characteristics are presented.
Measurements of sensitivity and noise factor were performed with a neon calibrat-
ed noise tube. Experimental characteristics agree very closely with calculated
ones. The best results were showed by the straight amplification circuit with
three traveling-wave tubes.
Translator's notei 77ils is the fUji translation of the original Russian abstract
Card 1/1

PARIYSKIT, Yu.No
low informtion on the nucleus of our Galmq. Friroda
49 no.7:81-82 J1 160. (KLU 13: 7)
1. Glavnava astronomichoskaya obserratoriya AJ SSSR. Pulkovo.
(YAlky W-ty)

S/'035/62/ooo/oo5/037/098
-7, /7j AC55/A 10 1
3,172,0
AUTHORS: Kuznetsova, G. V., Parlyskiy, Yu. N., Soboleva, N. S., Khanberdyyev,
A.
TITLE: Observations of solar radio emission during the eclipse of February
15, 1961, on the 9-cm wavelength
PEERIODICAL: Referativnyy zhurnal, Astronomiya i Geodeziya, no. 5, 1962, 42,
abstract 5A320' ("Solnechnyye dannyye", 1961, no. 4, 65-67)
TE.XT: The results of observations of the solar ecl--'pse of February 15,
1961, are described. The observations were carried out with the
aid of a paraboloid,D - 4 m) with azimuthal mounting. The open end of a round
waveguide, into which were inserted a quarter-wave plate and a ferrite modulator
with "0 cps modulation frequency, was used as primary exc:.ter. The half-power
0
d~rectf_onal pattern was 1.5. As radiometer, was used a three-traveling-wave-
tube straight amplification receiver with an equivalent input noise temperature
of 4,5000K and with a passband of 300 Me. The circularly polarized component of
the radio emission and the nonpolarized radiation of the Sun were recorded. The
recording was effected on an KM -09 (EPP-09). The antenna temperature of the
Card 1/2

S/O 335/62/000/005/0 37/098
Observations of solar radio emission ... AC55/-'101
Sun outz;lde of the ecllPse was 5,500oK. The Moon was usod for the abt;olutv 22
calibration. The flux from the Sun on the day of the eclipse was 125 . 10-
,.,:att/m2cDs. The opening of the co-ronal condensation from 8h 17"'.5 to 8h 20min
(universall time) was ascertained from the examination of the eclipse curve.
Under the assumption that the source has a round shape (D,--1!2) and that the
condensation has the shape of an ellipse with semiaxes 0! x 1!14, the Brig.'
I K and 2.75 - '100 K
ness temperature was calculated and proved to be '~.l - 1090
respectively; i.e. it proved to be higher than the temperature of the undisturb-
ed corona. No polarization of radfation from the condensation was detected,
which is indicative of a sharp directivity of the polarized radiation, this
directivity being related to the radial direction of the magnetic field over the
spots. The residual flux during the maximum phase of the eclipse was 40 - 50%.
M. Gorelova
rAbstracter's note: Complete translation]
Card 2/2

~'-_ -PAR IY-SKIIY.p --iU-."-
Structure of the nucleun of the Galaxy. Aotron,,zhur. 38
no.2:242-246 Mr-Ap 161. (MIRA 14:4)
1, Glavnaya astronomichookaya observatoriya AD SSSR,
(minty Way)

?o8e,o
6/03-,/') 1/~ 3-/ 1 (~ 1~ A, I I
70 1,-7 2- 1, iF 2
M iariy-,kiy, Yu
T111 E un uie intercnari ,c oi (,,a::- :;evween thE .\ucleus anu
t t,, eCorona of tn'. u.-A laxy
PERIODICAL- Astronon.icne,,;hiy zhurnaj., 1~ol, Vul. 3~, :~o. L,
7
)7(,l
7
ri-'XT: Accordin '. to -Ii ui.- ior-- _)i iteutrai N- u r o,~, (- i,
(Var ~iioeruell et ~Ii - i~(-'I ~ A) L , c tj a :~, at ttie cc titre ul: L'IC
Gaia---L,y i-:uves iii -ie perij,h,;r,jI (I~r(-cti i- T,ie arni at
a d-L .5 T a I-IC U L, 1 7:1 k I ~C fl-o- Litt CC'I)Lre j., -xtii;,, ,[it.., a ra".1al
velocity of al,ouL it. (, i. t i i (- (-, ~ , i ~-- 1- si 6 (1 ol t it? cuiAre
tjler~'- are irag;iwuts t) i L I I I." ~j I jl~ 11;~ I I C I I';JuVe 1-11t.11 J'IA -1 1 LI I
velocities bettre-ei. ?') aii,, 15(, k~ i ~ /.s e c Fie total awounL of
ga,s l(--avjn,4 t,ic rcL,ion R e 3 1, C L s It-)II L 1. ~) I.: . Wi tii a
C 0 11 t L I I u ') 1 1 --3 e s C, a " F '-) I ~- , w s - I t - ,t ! I!~ V C' 1 L4 C i t "' " I I (~ C e1-111
r:-,gion sliould 1~(--cojj.e F- ..i-tv in tAhout IL, vear~- I-i r 1.1 s
criziliec t I oil, Oort and Rougoor k16-1. ~~) i14VC 5UtQ-,eStC-U L,,at
ttiere is a co-itinuou~~ -iniliix ni vas into tne cti,tral rc-.L,~ion of
Card 1/6

C8
k- ri t ii, j 1; 1 ( rc,l.lj. 'c
ttic Giilaxv 1r,)m Likf- "t-ilo" . ic L~i:, i., ,i-ldej hy t.ie
1:,agllotic i leld, Into ti-tv )I t-ie mcie us o~ L.Ic
.~a lax V ci t; (I t11 f I' I I
, C cl V U t L V C e I It I- IF 1 11 t 11C I i t I C' UZI J- aN Y.
T'lle p1
-ebrlit t.,)(2 IL ;11:,
tly i, (.) t n c~z I ~, L .,,x L ~4 a t u r j ii.-, L , i u j I it i i t?
of til(-- Galaxy t ~-l c1 ct I'm T*f at .,, c, \,t:,1uc1tv
v dul-111".. a tim e c; t IS (1~, c ( ii (- lie tis -L t y o I t-ic iii
t!l C !la 10 rX 1, () ve t I c t io j, 'j-k -i-ver. hy:
d~l/dt
i4
if tile g;AS IS lleUtVa I tlleli lOV-16e(-l t'l~: LiCnSitY IS
sufficiently high, i t sti,-,d lie sf-cii in t~ie 21 cil, Jille.
J1, Oil the otill-.1- litind it 'i 1(jill!'ed, thull ,I c(1ljtllju(w~l
ul-cl I
t;iervai i-adio emis-ior, wili lie oI-,-,iel-vcd tm It-(,,.Iu
t;ic iow-irc--juency Tlon-lnurr al Pini--ion will be ab--,orbcu anu
tne It line Nvil .1 api ear Lii t he o;,t ic:tl ri~S~ion. Jill t1le
a
Card -'-1/6

C'JI-i" c ~l L; 011(~' sh"As v
1 1;C i t- I-,,.: iI7e i, it n i-, j c I i e J6 canriot conLroji-
hii.., th~'lt Cl !,;IV reach - 10 . (, 1; L, I'-
I Lil till. o tic I " r J d a 1, (.) v ~ Lil,
~_I. tk! -, ;, .. I I j) r, ;i.,:; i )i 'L ii v- -1 F Llfll~ L il
r;l - . -1 - I I, " r 0 1 '.) r k 1)
tc
I- V ;I t i k) 11.1; Q1 t I I (' t I I
v. a j r;l ~1 I o iliji, d x'()v j_J e 1111 01--il L I ,!l ai_-" C
n cit t;l t f-. (if t1l( allu also Z11 )ut L.1(
t( J\ I; A I V I, C !:1 0 t' YV
. ~, ) tnal. t:it--
L t C f'!1C I r i u !; o ! t t2
(I V T ik r'-I k, I t im t pjr a I v 6 t I I a t
Jo
M Ina X
1,wl X 11i"1 X
1-111.1 1( t!lP field iS iJSS1:;%CG1 to
C,,ird 7)/6

S/U 3 3/6 1/(j36/UU,;/U.1U/U I I
ull tile 111tc-rclIallAe . . . . E02/E314
be nut vt--r-y diffurent iromHhalo Im 3 x 1U- 6 Ot Ttic
E- 1,j C i t I o!j mUut Liatisfy tile follOW1.11,ir itIOCIUO.Litionj
W1 w
P11 11,1alld
d3f / dt
2 1 P' if" Its
The figure shows the values of V V and
m in 1112.11
vmax as functions of tho radius R in Itpc (the volociticn
are given in cm/sec). It is concluded that: 1) tile gas
can flow in onlv in ail ionised state; 2) the inflow
velocity is of the oroor of' a few tens of km/s cc;
3) tile inflow radius is not less than l.j );pc for tile
Card 4/6

I V.";< i y C (I r() 1::1 ;l 1 11, 11') T. j ('~ 1~ t I I a 11 '4~ ;'C 1 1, 1
I I'ZI r, y I I " t c 1;. 1) 1~' c I o I t I I
the Galaxy ,,,it by o1 it!~e cari:!Ot
correct !:-)-nce, ior ;it,, anl Jo~-.' ra(lills 01 about 1('(; lic '-.lc
( ''!M, -, 11" :,it. k 1) Al-(- I:nt It lnZly i-
t,;,It t'll" (Iljtf low oi ,iai fruj:t Lii~- e( tArc of our Gniaxy all(!
f rat., tm- -mc 11(~iis of -~ I i -; oj tim- sai,.o nature. ..,hen al'i,iied
to unrtl-, j.!vchat).ibu; Joiiui to .I figure of' aLout
J (i1, 1-1, [I(.L-Lc , 1(~Jd ll~ t1le nillo of 'I --j I C!l i ~-~ a
-jC
e -L I I! t. v I v
~t C 1-~ CL:.J M; e ~s t OTIS
1- (2 0 1- V I Q , r r c u
astI-()IIC'l!-:LciIesk;Iy3 observltor-va
t1jin .1istrorion.icai ul,:~erv,--torv,
Acauel..y ol .-Cicnizes, :-3:0
it"ou
31U

PARIYSKn,o IUONO-
Dietribution of optical wW radio exisBion in A 17. Astroh.zhtw.
38 no.3%483-486 Iq--j-e 161. (KMA 14:6)
1% Glavnaya astronomieheakaya observatoriya AN SSBR.
(Nehilae) (Radio ast-roww)

13 Ai I,
AUTHOR: Parlyskiy,_Yu _N
30 1
S)043/6i/038/005/061/015
E133/E435
TITLE: A model of the Orion nebula from radio observations
PERIODICAL: Astronomicheskiy zhurnal, v-38, no-5, 1961, 798-808
TEXT: The large Pulkovo radio-telescope at GAO AN SSSR was used
during 1959-w6o to study the Orion nebula. The first series of
observations (autumn 1959) were made at 9.4 cm, using a super-
heterodyne radiometer with a bandwidth of 20 Me. The
coordinates of the brightest part of the neblila were thus
determined. The result is compared with other values in Table 1.
A further series of observations (February 1960) were made at
8.25 cm with a more sensitive radiometer (passband 500 Me). The
,scans were corrected for the time constant of the apparatus and
for the directional pattern of the antenna (half-power width = 31).
To determine the kinetic temperature of the nebula, the author
develops a method proposed by C.M.Wade (Ref.18: Austral. J. Phys.,
v.2, 388, 1958). The brightness temperature is connected with the
kinetics temperature by
Card 1/~ TB . Te(l - e-T(Xly) W

30813
S/033/61/038/005/001/015
A model of the Orion nebula ... E133/E435
Ye being the equivalent kinetic temperature, and with the integral
flux by
P TB (x, y) d--dyL e-(x-Y)dxdy)-
ct CZ (2)
Assuming x(x,y) =-To VX,Y), this reduces to
TL Tjs (x, Y) dY9 (3)
-00
Y(To) can be calculated nu erically from the observed
distribution of brightness temperature. If the values of flie
integral flux are known at two frequencies, an average value for
Te can be derived from the expression for the op-~ical depth
3.08.1028tp
which can now be written as the ratio of the optical derAlis at tli-
two freque ncies in the form
Card '2/.# 102

30813
S/033/61/038/005/001/015
A model of the Orion nebula E133/E435
The two frequencies were chosen to be 9.4 cm (Pef,3 F T Haddo:k
C.M.Mayer, R.M.Sloanaker, Astrophys, J- v,119, 456 1954) and
75 crii (Ref.8- C.L.Seeger. G,Westerhout. H,C,van cle Halst.
Bull, Astron, Inst. Netherl- v,13. 89, 1956)~ The flux at
9.4 cm was reduced by 11% to agree with absolute measures made ai
9.6 cm (Ref.12. N,W,Broten, W,J,Medd. Astron, J- v.64. 324, 1959)
On the other hand, when allowance was made for the direc-ional
pattern of the antenna, it was found that the flux should be
increased by 10%, The flux at 75 cm was riot corrected, The
fluxes used were
X1 = 9,4 cm, P, = 450 x 10- 26 W/M2 c'p.'S'
k2 = 75 cm P2 z 230 x. 10- 26 W/M2 c"P'S~
The average kinetic temperature is 117150~K + IOCO^K, The data
are now sufficient to calculate the flux from the nebula at any
wavelength (Fig.7) As can be seen from F19.7, agreement with
observation is good ex~ePt at 3,5 ni, This latter may be duc. t,-.
the presence of gas outside the region :.onsidere!d, The author
now works out the distribution of ionized particles iriside a
Card 3/S',)

'), () P, I "
S/033/61/038/005/001/0!z)
A model of the Orion nebula E133/E435
sphere of radius 10'. The total mass is 1.16 M" about 6 m,
being concentrated in its brightest ~.entral parY having ;t diar~-'rt-
of 3 The smallness of the deviatic,n at 3,5 ry, indi-a'es 'hot
there is not more than 40 M,-, outside the 10 srhere A
of 450 pcs is assumed. ME~optical observati.ons give 104'K f~)r
the kinetic temperature Extensive work on th4E X3726/kY29 1:r-,
(Ref.19 D.Osterbrok E.Flather Astrophy:s, J, 129 1 1960)
gives similar dimensions for the region concentrated round !h6
trapezium The ele-tron density determined by optical methud.-~
approximates to the maximum in the line of sigh--,, Rartio M",h, 1,
give the mean square density Differenzes i-n Lhe tw,:~ are
interpreted as d,-e to a -Aoud structure in the nebula Th i:
density fluctuations appear to increase with distante f-~,m tnt
trapezium 1/14th of the volume is oL.~upied by --louds a~. th-
centre of the region and 1/36th towards the edge The rad13
6mission is smaller than wc,,,,.Id be exp(-,,, ted on the basis of the-
HP f lux- Obser va t ions incti -i t e ,he pos s ib) e presence of t a., -
moving - louds in the neblala It is pos.~Ible thu-r,~fore that Ii~
discrepancy in flux is due ?o ignoring ollisi~)naAl f,r,)
Card 4/4

30813
S/033/61/0'58/005/001/015
A model of the Orion nebula E133/E435
initiated by shock waves. Acknowledgments are oxpressed to
V.A.Stupin and R.E.Burv for assistance. S.I.Gopasyuk,
N.N.Milthellson, S.B.Pikellner and S.A.Kaplan are mentioned in the
article in connection with their studies of nebulae. There are
10 figures, I table and 39 references: 10 Soviet--bloc,
2 Russian translations of non-Soviet publicationts and
27 non-Soviet-bloc. The four most recent references to English
language publications read as follows:
Ref.9: D.C.Edge, J.R.Shakeshaft, W.B.McAdam,-J.E.Baldwin,
S.Archer, Mem. Roy. Astron. Soc., v.68, 37, 1959;
Ref.12: as quoted in text;
Ref.19: as quoted in text;
Ref.37: T.K.111enon, Astrophys. J., v-127 36' 19513- H. van Woerden,
40 lewell.' Stanford,
Paris Symposium on Radio Astronomy, ed.
California, 1959, paper 71.
ASSOCIATION: Glavnaya astronomicheskp~a observati3riya Akademii
nauR SSSR (Main Astronoin cal. Observatory, AS USSR)
December 24, 1960
Card 5/16"-

20M
S102 0 '6 1 /11 7/0 -1 1
3, t7o 0 B1 04/B209
AUTHOR: Pariyskiy, Yu. N.
TITLE: The particulars of N~;C 4486 radio emission
PERIODICAL: Doklady Akademii nauk SSSR, v. 157, no. 1, 1961, 49-50
TEXT: In December 19599 radio emission from Virgo-A (NGC 4466;M 87)
was detected by the radio telescope of the Pulkovo Observatory.
Measurements showed that the angular dimensions of the source as measur-
ed on 9.4-cm waves are considerably smaller than those determined by
Mills (Ref. 1: B. Y. Mills, Nature, 17o, lo63 (1952)) or, 3.5-m waves.
Pariyskiy repeated the measurements with a sensitive radiometer on
8.7-m waves. One of the graphs taken is shown in Fig. 1. A checking Of
several graphs showed that thEy practically agreed with the theoretical
directional diagrams of antennas. This allows to conclude that the
angular dimensions of' the source do not exceed one arc minute. Observa-
tions on 3.5-m waves gave an angular dimension of 61. Using these and
other results published earlier and taking into account, measurements
made at Nancy (France), in whicn the angular dimensions of this source
Card 1/4

20317
S/)20/'61/137/0 ~_ I/ ",,7/1",~'
The particulars of NGC 406 ... BlD4/B2C)g
an 8.7--cm waves were found to be 1.5', one may conclude that tne size
of the source depends largely on the frequency used. The emission
center of the 8.7-cm waves was deter-mined in order to clarify whether
the source is located in the center of the Galaxy or is due to an
ejection. Highest accuracy of the measurements was warranted by the
use of a stationary antenna. This was done after the Yoon and '-~ie
source had paosed across the directional diagram of the antenna on t~~e
same day. The coordinates of the nourco were found to be:
a1960,0 = 12 hr 28M158 + 18. This means that the radLo einission (-omos
from a region 45" + 15" west Df the center of the spherical Galaxy, in
the direction of ejection. These measurements were conducted by Q.
Shivris and V. Prasolova. Further investigations on the exact
position of the source are intended. There are 1 figure and
2 non-Soviet-bloc references.
Card 2/4

The particulars of NGC 4486 ...
203:.7
S102 61113"Irl-01 /007/02
B104Y3200
ASSOCIATION: Glavnaya astronomicheskaya observatoriya Akademii nauk
SSSR (Main Astronomical Observatory of the Academy of
Sciences USSIQ
PRESENTED: September 28, 1960, by V. A. Ambartsumyan, Academician
SUBMITTED: September 18, 1960
Card 3/4

V. A.; PARTYSM Yu N
SODDLEVAP 11. S.; FRMORDVO
Distribution of polarized and nonpolarized radio enission in
the Crab nebula. Astrom shur. 40 no.1:3-11 X-F 163
(NIRA 26: 11
1. Glmvnaya astronomicheskaya observatoriya AN SM.
(Radio astronormy) (Nebulae)

20736
D,' ~ ;'6 1 / 1 z 7,
.3, / 73 o (o 2-7/
(- '7 Y 7 B104/V212
A UTHOR Pariyskiy. Yu. N.
TITLE: A new source of radio emission in centimeter waves
PER16DILCAL. Doklady Akademii nauk SSSR, v. 137, no. 2, 196!9 307-509
TEXT; In 1"Aarcn, 195.0 observations cave been made with the giant
rad i ot t-' e q c r, pe in i~ulko-,ro of thE! 9.4 cm radio emission background of a
galaxy which :9 located in a certain region of the Mlilky Way. A new
:;c.urre a -a~iic e-.iigsi(.n bias been establisned at ax, inclination of
i_ is 'ocated 'n t ne of tne iiilky Way, The fol:ow-
he P1 F,
r 6
rd i r! a',, -- a i i-- givpr. for the source. a 18 "3m38
ing cg, I I
,q56 ~ 1 9
and ne hmenslo,,. of the source is given as 7hese
coordinate-~ agree witt, source n(D. 44 of the Westerhout Catalogue, wizr.
scurce "C!.~O" (,f Tfie second Cam*oridge Catalogue and with source "8 -t ")!I
of Mills, The flux of the 9.4 cm radio emigsion amourtc to
'200 -)G)~10- 26 W/m 2 cycles, that of tine 22 cm radio emission to
Card /-15

20736
S/02 0/61 /13 7 /002/100 7,'C -) C
A new source :-f :-Id~o emisslon B! 04/132 - 2
185.10 W/P_ cycles and that of the 5.5 m radio emisnion to
1900-0 zh W.11 --yzles~ TI-9 spectrum described here, does not have any
aompopent~, -.,- "fie shorlwave range which is contrary to the spectra of
radio s-_,ur.-- cf II kiy)d,, Thereforet the auther is convinced that, here,
-it -,he
a trermi~ Jmjoz ,ni is present which is dominating in , centimeter
range- G. A, Shayn and V. F. Gaz have not been able to identify
photograpn,ir,aiiy any visible emission, even though lon,~ exposure has
been used. i-e- the v:isible portion of emission does n)t exceed 400
I-Abstracter's note. dimension not givenj. The author concludes from
known absk~rpliori data from this direction that the sou,-ce might be a
galactic object. The spectrum of the described object in the meter range
is typi(~al ioi- triat of a magnetic bremsstrahlung. Furthermore, the
opinion is pointed out wrich has been held quite often at the present
time, that galactic sources of a non-thermal radio emi3sion are
residues from exploded supernovae. Considering the ma3nitude of' the
minimum energy necessary to prove a new radio source, the author is tx
able to show that the energy which at present ir in a radio nebula is
Card 20

20736
S/020/61/137/002/007/020
A new suurce of radio emission B104/B,"12
much larger than the energy which is released from a supernova of the
I, kind. The radio emission, in question, might be explained by
compression of the magnetic field in an expanding nebula shell at usual
density of the primary cosmic particles in the interstellar space,
The supernovae are taken as the origin of primary cosmic particles;
this agrees with L S. Shklovskiy. The author thanks S. E. Khavkin and
N. L. Kaydan,3vskiy for their interest in his work, and the collective
of the Simeizkaya astrofizicheskaya observatoriya (Simeiz Astrophysical
Observatory) for making available unpublished material. There are
1 figure, 1 table, and 10 references: 4 Soviet-bloc and 6 non-Soviet-
bloc.
ASSOCIATION: Glavnaya astronomicheskaya observatoriya Akademii nauk SSSR
(Main Astronomical Observatory, Academy of Sciences USSR)
PRESENTED; September 28, 1960, by V. A, Ambartsumyan, Academician
SUBMITTED: September 28, 1960
Card 3/3

ZAKHARENKOV, V.F.: KAYDANOVSKIY, N.L.; PARIYSKIY, Yu.N.; FROZOROV, V.A.
Observations of discrete radio sources at 3.2 cim. wave lenith
at Pu-lkovo. Amtron.zhur. 40 no.2:216-222 Yx-Ap 163. (MIRA 16:3)
1. Glavnaya astronomicheskaya observatoriya JiN SSSR.
(Radio astronoiky)

KOROLIKOV, D.V.~ PARIYSKIY, Yu.N.~ TIYDFEYEVA, G.M.; IKAYKINR S.E.
High-resolution radio-astronoideal obeervations of Venue.
Dokl.AN SSSR 149 no.la65-67 Mr 163. (MM 16x2)
1. Glarnaya astronomicheskaya observatorlya AN SSSR.
Predstavleno akademikon V.AiKotellnikovyza.
(Radio astrononw) (Venus (Planet))

PARIYBMY: lu. N.
"The structure (IT the NUDIOUS of the GaLqy**
report Weemted, at the VKU/tMI B'T lum an wA MW'Iwnlc Clouds, Symposium
No. 20, Camberra and. Sydney AustmIla, 18-28 March 1963.
Palkow ObservatAvy

ip Z)
f /V- ,
Empi'l 'T. YU.N.9 TMYSMA, G.K., IMMY, S.S.
IB19b PASDIUUDZ log Onervatim of Toms aM OWItar at -go
ftlkm Obarvatmy.
ftport to be oubmisted for Me kth laurmaoma spwo eviame 9)
(OWAR) Wasmg 2-12 Jm
f~,_

.Acar-wimi im: AA0176D9 6/0033/64/043./001/0003/0006
AUMOR: A~t; Timofeyeva, G. M.
TME: Structure of the Cyg-A and Vir-A radiosources
SOUME: Astrcacmicheskly zhurnal, v. 41, no. 1, iA., 3-6
TQPIC TAGS: Cyg AP Vir A. radiotele-scope, stellar ratiaticn, ZIGC 4486
ABSMOT: Cbservaticas on the Cyg-A and Vir-A radiosources at a wavelength of
3.02 =vere ccnducted in January and February of 1963 using the large Pulkovo
radiotelescope, which has a resolution of about 11. The results were essentially
as follom: Cyg,-A. The source is asy=ctric and the anoilar magnitude of its
western cmpcE7en_t is as low as 15". The positional angle of the axis linking both
ccmponents is 125* + 150, which is higher than that found at wavelenaths of 10 Ma,
21 mm and 1 netcr,*Zid agrees with previous Pulkovo observatims indicating a
marked dependence of the interccupaaent distance, the ecuponent effective magni-
tudes and the intercanpcment radiaticn intensity cn thevave length. The absence
of interacmpment radiatim at 3.02 = is very likely. Vir-A. The radlaticn of
the principal body of the NGC 44W galcxy, observed at f, =2cm, is considerably
less than that found in the decimeter and meter bonds. Ucmversely, the ecatribu-
tim of the central source, whose angular dimension Is-411, is lnversel~y propm-
Card

AccEssiou im: AP0176og
tion,al to the wavelength. . The character of the radiotelescope image suggests a
significant deviation of the genuine shrpe of the central source from the Gaussian
cUrVe vhich may be explained by a poGsible existence of two minor sources 20-3VI
apart. "The aulthors; would like to tnruik S. E. Khaykin for his interest in the
work., A. B. Berlin for his help in maidn- the observations and designing the ap-
paratus, and D. V. KorolIkov for his criticism of the manuseript." Orig. art.
has: 3 graphs.
ASSCCIMCK: Glavnaya astroaaniche-sloya observatoriya Akadmil nauk S S S R
(Main Astrcacmical Observatory,, Academy of Sciences SSSR)
SUBaTTM: 2lhMay63 DATE=: law-64 MEL: 00
SO CME: AS NO W SOV: 004 aMER: 001
Cord 2/2

Yu
.

[ACCESSION NRs AP4032729 6/0033/641041/002/0362/0365
AUTHO)tS Soboleva, N. 5,; Pariyakiy, Yue We
'01
TITLEs asibLItty- of - observing polSTI-S40-AP , of thqirual radio
emission from planets
SOURCE: Astronomicheskiy zhurnal, v. 41, no, 2. 1964, 362T365
TOPIC TAGS1 thermal radio eni ssion, effective radio emission, plane-'~.--
refraction, asteroid, planet satellite, radio astronomical instru-
ment, radar reflection coefficient$ permeability, polarization,
integral polarization, terminator, ionosphere, planetary atmosphere
ABSTRACT: The moon is a dielectric, but the emission layer in the
centimeter and decimeter wave ranges is beneath its surface. The
emission beam passing the surface is subjected to refraction. Recently
this effect was detected in Pulkovo by experiments on waves of 3.2
and 6.4 ca. It can be assumed that the radiv emission of Venus on i
the 3-cm wave length in caused by the.rigid surface of the planet.
Radar data obtained from Mercury# Venust and Nars showed that the
/Z

ACCESSION NR: AP4032729
refle~;tion coefficient of these planets Is equal to 0,1 and the
permeability Is about 4. Polarization of planetary radio emission
is possible when the planetary atmosphere contains an ionosphere
within a dipole magnetic field. The rotation of the polarization
plane is greater near the magnetic poles than in the equatorial plane.
No Integral polarization exists at very high frequencies, but It
appears at the terminator, where the dtffarence in brightness teup-
atures of the Illuminated and the dark surfaces Is great. Orig. arte
hasa 3 figures
ASSOCIATIONs Clavnaya astronomicheakaya observateriya Akademii
nauk SSSR(Main Astronomical Observatoryp Academy of Sciences SSSR)
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No REP Sao 005 OTHIRe 005
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PARI*YSKTYI lu. N.
"Galact-i-- rad-'~,i, suur-c-:, at "-., *!" - .11
ie,~ e r c
paper presented at !2t:, Geri AsE;emL),'.-,-, int..' Astronomi:all ljn~,,Ail ~;iamt . f% ..,- -
3 Sel I'J4.

711! ~, ~-. ~ I
I ~; Z-.". ; , I

GOLINEV, V.Ya.-, F4kIy-SKIy, U.N.
Right ascensicnB, stnjctu:-e, and spectra of 20 exLraga--,aC'-%!:
sources from observationo at Pulkovo at the i4avelengtt. ~f (,.4 cm.
Astron.7hur. 42 no,W05--315 Mr-Ar, 165.
1. Gjavnaya astronoz~.ches,raya observatc-riya ~14 SISSR.

GOL Y a.; Pi F
F -1 EL t,~
nebula at t-i, cm, aave 3:
by t' e so I a,- surer cc rDna --ave. 11~~

, E F- . ; --YSK--Y , y'- . N .
r E, 4 4 -, - - f~ -' - I ' -
,. S - C, - - 4 ~, . . - . , .
Gor-ifusion e~'fpcts and "FtrF7,~, -- - ,e s . : 11
(:11 -R: ( . -, . 1
87-103 164. 1 1~ A I-,-

..e-:-"3 of
W11VID ~ongth cf rr,,.
Is: 10)
2 . Z I, avnaya rorom ' che ~.rka.,-a c.:.t se -vr.-~-.~riya Ali' S.

GOLINEV. V.Ya.; NOYOZZHILOVA, G.G.; FAPJ.YSKfVY
Y
thP 6ECIA.n Ir -4
rin gale' '.1
a-
by means of the large ra~-Jo tFltocope . lulkovs.
za-.-.; raci~-.flz. 6 ric.lzI83-785 1659 ~i (M-IRA
't. GlavrayR ~.ql.-crwm~ nez-3kaya ~~b-zar-va!~~rlya AN $S-'~F.

PAR129K, Bohu3rir; SCHWARZ, Steftin
Sexicharacters of the multiplicative semigroup of integers
modulo m. Mat fys cas c?*AV U no.1963-74 161.
, Katedf.4 matematiky, Slovenska vysoka skola technicka, Brati-
.iava, Gottwaldovo namesti 2.

PARIZEK, B. j, SCHWARZ, S.
Multiplicative eemigroup of residue classes. P. 136
HATMATICKO-FYZDULNY CMPIS. (Slovenska akademia vied)
Bratislava Czechoslovakia
Vol. 8, no. 3, 1958
MontILly list of East European Accessions (EEAI) LC. VOL. 9, no. I January 1960
Uncl.

PARIZEK, B.
"Rema.rks on the structure of the multiplicative semigroup of residue
classes."
P. 183 (Matematicko-Fyzikalny Casopis) Vol. 7, no. 3, 1957
Prague, Czechoslovakia
SO: Monthly Index of East European Accessions (EKAI) LC. Vol. 7, no. 4,
April 1958

PARIM, E., inz.
Help of testing rooms in the improvment of product quality.
Strojirenstvi 13 no. 12: 881-882 D 163.
1. Kovotechna, Brno.

PAR122T', IN2.
S!'et:i fc)r I
. . I ~-? ~'. L 7 1, r ~, ~ - -. , , I- - -
) 'ItO T a'~ I i~- , I " z ~, - '~ -- ~- J' : , , ~ - : I - - - -- 0~- ` , 1 164.
-k 1:
1. ?].ynoprciak- ,

ROZSIVAL, Vladimir; PARIZEK, Jan; LICHY, Josef.
Data on some problems of apinal, cord tumors in childhood. Sborn.
ved. prac. lek. fak. Karlov. univ. (Fb-ad. Kral.) 6 no.5tsuPPl-*.
647-651 163
1. Nourochirargicka Otnika (prednostat prof. Mr. R.Petr) a
Neurologicka klinika (*ednootst prof. Mr. M.Sercl. Drso.),
Karlova Universita v Rradee Kralove.

PAEIZKKI JIRI -
science
Parizek, Arl. Kastrace kadmeim. Praha, Statni sdravotnicke nakl., 1957.
99, 12 p. (Babakova sbirkA, 4)
Ml)nth3y Index of U-st European Accessions (EFAI) LC. Vol. 7. lJo. 12. Dec. 58

1-11MICk Sec-3 Vol.11/3a %docrinology Nov 5?
2213. PAf1iZEK J. Czechoslovak Acad. of Scis. Lab. of Physiol. and Pathophysiol.
oT7e_t_ab_..7_P_rague. *The destructive effect of cadmium ion on
te5ticular tissue and its prevention by zinc J.ENDOCR.
1957. 15/1 (56-63) Graphs,2 Tables 3 Illus. 10
The s.c. administration of cadmium salt.-; (cadmium chloride or lactate) to rats
and mice leads to acute destruction of the testes, with destruction of the semi-
niferous epithelium and interstitial tissue. These changes in turn evoke castration
phenomena, but the atrophied accessory sex organs retain the ability to react to
testosterone propionate, Within 20 days after the injection of cadmium, prolifera-
tion of fibroblasts In the interstitial spaces under the albuginea begins and is ac-
companied by an extensive formation of new blood vessels. Later, new Leydig
cells appear; this is followed by a gradual return of the endocrine function of
the testes. The spermatogenic epithelium of the seminiferouB tubules. on the
other hand, does not regenerate even 133 days after the injection of cadmium. The
simultaneous administration of a large dose of zinc salts protects the testes com-
pletely against cadmium damage.

oiten
'--DTC.4 Ss?c V, '101 1 -)ad ` r)10FY -W 59
1500. DEOXYCYTIDINE IN URINE AS AN INDICATOR OF CHANGES AFTER
IRRADIATION - Paffzek J. Arient M. . Dienstbier Z. and
Skoda J. La__ --Ph- ~__ Pathophysiol. of Metabol., Czechoslovak.
b. .7 Y... -
Acad. of Scis, Prague 2 - NATURE (Lond.) 1958. 182/4637 (721-722)
Graphs 2
Rats were X-irradiated with doses up to 600 r. to the whole body. Their urine was
collected for 24 hr. following irradiation. and examined for deoxyribose usi..g
Dische's reaction. Increase in elimination was found. The substance responsible
is deozycytidine. The amount of this substance in the urine is a prompt and sensi-
tive indicator or irradiation. The normal value of about I mg. per 24 hr. is raised
to about 1.5 mg. by only 10 r., to about 7 mg. by 600 r. This effect is not due to a
renal factor (tested in nephrectomized animals). It could be eue to release of the
substance from nucleic acids, or to accumulation because of blocked synthesis. In
contrast, the excretion of thymidine in not changed by the radiation doses used.
Quastler Upton. N.Y.

MIM. J. ---
Hechanism of the effect of cadmium on the testes. Cesk. fysiol. 7 no.'.'.:
249-250 WT 58.
1. laborator pro fysiologii a patofysiologii premeny latek C-SAV. Praha..
(TWTHS, eff. of drugs on.
cadmium (Cz))
(GAMIUM, eff.
on testes (Gz))

HOISGOVA, A.; FALTOYA, HRMIA. Z.; CUTTIL, F.; KOPECrY, H.; IAT. J.; PARIZEK, J., .
Studies on the mechanism of adaptation to dietatic changes and to other
stimuli in rats. Cesk. fysiol. 8 no.3:195-196 Apr 59.
1. Laborator T)ro fysiologil a patofysiologii premeny latek, CSAV, Praha,
Predneseno na 111. fyaiologickych dnech v Brne 14. 1. 1959.
(ADAPTATION,
to food composition & feeding rhythm in rate (Gz))
OFGOD,
ndaptation of rats to food coamoBition & feeding rhythm (Cz))

PARIM, J.; A31MIT, M.; DIMISTBM, Z.; SR)Rk, J.
Mechanism of nost-irradiation desozycitidinuria. Cesk. fysiol.
8 no-3:230 Apr 59.
1. laborator pro fysiologii a patofysiologii premeny latek CSAV,
VYZI-,alnTW UBtav hygieTW, epidemiologie a mikrobiologie, F~rsikalni
ustav fak. vseob. lek. KU, Chemicky ustav CSAV. Praha. Predneseno
nn Ill. fysiologick;yoh dneoh v Brno dne 15. 1.1959.
(NUOLMOSIDSS AND NUGLWTIIM, in urine,
desox,vcitidine in x-irradiated animals (Oz))
(RO7,NTG-VN RAYS. eff.
urinary desocycitidine in irradiated animals (Cz))

LOJDA, Z.; PARIZEK, J.
Ontogenetic development and topochemistry of testicular
dehydrogenases with special reference to zinc and to cadmium
necrosis of the testes. Physiol. Bohemoslov. 12 no.6:512-517
1163.
1. laboratory for Angiology, Faculty of General Medicine,
Charles University, and Institute of Physiology, Czechoslovak
Academy of Sciences, Prague.
(TESTIS) (ZINC) (CADMIUM)
(OXIDOREDUCTASES) (GROWTH)
(LIPOAMIDE DEHYDROGENASE)
(VITAMIN A)

tMIZM, Stnnislrw; PARIZEK, Jir3
Loonlirvition of mitochondrin 4ir"i fill I'llinto lit
nouropil. 8born. vocl. prim, Irik. fnl(. Knrlov, OnAv, fk nos4t
501-504 1 65.
1. Nounichi-rurgickii klinilm (proubinstit profs MUDr. R. Peltr)
a hiattvicky ustRV (pro(bintiVit pruf. MUDr. J. Ilr(inti(in, M-3c,).
Karlovy Univorq1ty v th,adel Kralovia.

PARIZEKS J.; I-04EGEY, 5~; VAVROVA, 1~
Concealed presenc-e of g:jczm ir, a 4, yeax-,,-!,j .h--ij!,Jj, ~,eslr,
neurol. 26 no,5:;301-303 5 :7~3,
1. Neurochir-urgicka klinika lek-wske fak-ulty KU v Hra&-1 Kralov'5,
prednosta prof. dr, R. Petr Detska khnika lakarske fakulty
KTJ v Hradei Kralove, prednosta prof~ dr. J. Blecha,.
(BRAIN NEOPLASM) (GLIOBLASTORA MULTIFORM)
(OPTIC NERVE) (GEREBEIJAR NEOPLASM)
(INTRACRANIAL PRESSURE) (BLPIDNESS)

V j-"U
-1 C, 1,
Of
-cr
e co na ey
:;I-naziort Of
L o: o, -.ic n-~rvu
Ine I-c 'IV,-, Of in-zLe~,.,; Of Of c-

%'loft
1. vo 1
Accp-,,,,:in(7c, (:f c~ -p-r-
F9.
:s L,'-' Vol.
Flortt" 1-7 Ld-fft of East U)r)pl.;Ul 0,

PARIZEK, Jan
Healing of irradiated and non-irradiated heterotranigPlants in
spondylodesis by the Halstead-Samov tecbnic. Sborn.ved.Tyrac-
lek.fak. Karlov. Univ. (Hrad. Kral.) 6 no.3:Supplememt:391-393
1163.
1. Neurochirurgicka klinika; prednostat prof. KUDr. R.Petr.
ir

EADVOMIK, Pavel; PETR, Rudolf; BERAN, Jiri; DROM, Vladimir; PARIZEK,
Jan; SCHMMERY, Ctibor.
High frequency generator for stereotactic electrocoagulation
constructed by the authors. SborT,.ved.prac.lek.fak.Karlov.
Univ.(Hrad.Kral.) 6 no.31331-334 t63.
1. Neurochirurgicka klinika, Universita Karlova (prednostat
prof., MUDr. R.Petr).
4-

MACA, Jan; PARAZFK, JaroElav; DOUTBEK, Milan, inz.
Rolling stock and the management of operations-, a discunaion.
Zol dop tech 13 no.2:33-35 165.

KAS, Vaclav, dopisulici chlen; KCSIL, Vladimir, dopisujici chlen; KAWDRA,
Augustin, akademik; dr.; TOMSIX, Boleslav, prof.;
PATOCYA, Jan, dr., kandidat biologichych ved; CHURY, Jiri, doc. dr.i
PAV, Jaromir, dr.; JANDA, Jiri, dr.; KANAY, Karel, inz.; ZAVADIL,
Zdenek, inz.
Discussion of the report of the scientific secretary of the
Czechoslovak Academy of Agricultural Sciences. Vestnik CSAZV 7
no.1/2?100-118 6o. (EEAI 9:7)
1. Vysoka skola zemedelska a lesnicka, Brno (for Kas, Parizek,
Tomsik, Chury). 2. Vysoka skola zemedelska, Praha (for Kosil).
3. Predseda VI. odboru 3eskoslovenske akademie zemedelskych ved
(for Kalandra). 4. Vyskumny ustav lesneho hoEpodarstva, Banska
Stiavnica (for Patocka). 5. Vyzkumny ustav lesniho hospodarstvi a
myslivosti Ceskoslovenske akademie zemedelskych ved, Zbraslav (for
Pav, Janda, Kana~, Zavadil).
(Czechoslovakia--Agriculture)

Al --L LJ,f U., --'
Vyorane ka,)itol,- z obeene zootechnikv pro posluchace veterinarni fak-ulty.
praha, Stat!Li 2e3 P. (Ucebni texty vysokyCh 5kOl)
0 11 -
DA Not in DiG
Monthly Index of Kast LuroPean Accessions (10,11) LC, Vol. 8, No. 4, A -ril 1959

SU,T=. Given Names
COM'U7*. C7,-cli-rlovakis
Aeadarde Decree-: cent, DVMI
Affiliation: 7-not -algal-InatitAfteffl V,Iterinary Froulty Veterinary College (Ustav
zootrf--.',~y veterinerni fakulty VSZ) Brno
Source:Prsgue, Sbo i;!; GSAZV Veterinarni No-dicinap Vol 604), No 7, July 6~1; pp 579-5"'
Datat "Heating irp, -1 Lations for Stalls Housing Save with Newborn Piglets"
SPO 961643

GDOVIN, Toms; tA9ZExY-*--
In co=emoration of the 65th birthday of Emil Pribyl, correspondent
member of the Czechoslovak Acadepy of Agricultural Sciences.
Vestnik CSAZV 6 no.8/9:544 '61.
1. Dopisujici clen Ceskoslovenske akademie zemedelskych ved. 2. Clen
redakcni rady Vestniku Ceskoslovenske akademie zemadelskyeh ved (for
Gdovin)
(Pribyl, Emil) (Czechoslovakia-Agriculture)