SCIENTIFIC ABSTRACT SOBOLEVA, N.F. - SOBOLEVA, T.A.

• Document Type: CREST
• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R001651910004-4
• Release Decision: RIF
• Original Classification: S
• Document Page Count: 100
• Document Creation Date: November 2, 2016
• Document Release Date: August 26, 2000
• Sequence Number: 4
• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT

AUTHOR: Dahlagin, A.I. (Cand.Chem.Sci.), Velentsey, E.V. (Engineeri &
Suboleva, X.F. (Engineer).
TITLE: basis for standards for sampling residues of the ryas shale and
0
shale treating industries. (Obostiovaniye norm otbora prob
ochagovy1di ostath-ov gazoslantsevoy i slantsepererabatyvayushchey
promyshlennosti. )
PERIODICAL: Teploenergetika, 1958, No. 3. pp. 33-36 (USS11)
ABSIMICT: So far there has been no theoretical justification for the
frequency of sampling in the shale industry and the existing rules
are entirely empirical. In the gas-shale and shale-treating industries
wain samples must be taken from the coke-ash residue of retorts and
the ash of generators. The frequency of sampling may be based on
the same rules as are used for solid fuels. 11.1any investifraters have
shown that sampling of solid fuel is a typical random process of
Gaussian distribution, and the same is true of sampling treated shale.
On this basis a formula is given for the number of samples that must
be taken to ubtain a result of given accuracy. The method of
determining the number of samples is then explained. The formula is
only applicable if the sample material is uniform, and it is
considered that coke-ash residue conforms to this requirement, indeed
it is more uniform than coal and shale. The formulae given are only
valid provided that the distribution for shale residue is indeed
Card 1/2 Gaussian. This point was checked and a graphical comparison is .,riven

IPATIYEV, V.V.; TIKTOMIROV, V.I.; SOBOLEVA, N.Y.
Rate of absorption of hydrogen sulfide by solutions of arsenic
trioxide and sodium carbonatp. ZhuiZ. prikl. khim. 31 no.10:1472-i477
0 '58. (MIRA 12~: 1)
l.Laningradski7 Nauchno-isslpdovftellskiy institut po parerabotke
Defti i poluchaniyu iskusstvinnoge zhidkoge topliva,
(Hydrogen sulfide) (Absorption)

SOV/69-2o-6-12/15
AUTHORS: Soboleva, N.I., Bol'shakov, A-G~, Kortnev, AV.
TITLE: The Precipitation of Magnesium Hydroyide Suspensions in an
Ultrasonic Field (Osazhdeniye suspenzii gidrookisi magniya
v ul'trazvukovom pole)
PERIODICAL: Kolloidnyy zhurnal, 1958, Vol 20, Nr 6, PP 742-747 (USSR)
ABSTRACT: Ultrasound is used for the dispersion of liquid and solid
-
substances fR
ef 1-J79 for the )recipitation of aerosols and
jr
the coa
ulation of h
d
o
l
f 1
h
f
7
r
so
s
e
or t
, 3-5
e crystal-
g
y
,
.lization of supercooled liquids /R-ef 6-.2/, etc,. The pre-
-
cipitation of a Mg(OH)2 suspensi
on in various concentrations
and frequencies is studied. This process has great tech-
nological importance, e.g. in soda productions A generator
tube type GK-3,000 was used with frequencies between 270 and
2,300 kilocycles. The ultrasonic oscillations ranged from
300 to 2,000 kilocycles. Figure 2 shows that the preci-
pitation speed is highest after 5 minutes of ultrasonic
treatment. At low concentrations, the precipitation curves
nearly coincide (Figure 3). The dependence of precipitation
on frequency is shown in Figure 4. The strongest influence
Card 1/2 of ultrasound is exerted on concentrations of 6.61; 5z83;

SOV/69-20 -6-12/15
The Precipitatiorr-of Magnesium Hydroxide Suspensions in an Ultra6onic Field
3-31 ~/l MgC12 (Figure 5).
There are 4 graphs, 1 diagram, 1 table, and 15 references,
10 of which are Soviet, 4 English, and 1 French.
ASSOCIATION: Odesbkiy politekhnicheskiy institut (Odessa Polytechnical In-
stitute)
SUBYITTED: April 13, 1957
1. Magnesium hydroxide--P:recipitation 2. Ultrasonic radf-'ation
--Chemical effects 3. Ultrasonic radiation--Applications
Card 2/2

SOBOLKVA, N. I. Cand Tech Sci -- (dies) "Study of the kinetics of the
settlinG of IAsuspension of magnesium hydroxide in a supersonic field."
Odessa, 1959. 15 pp with graphs (Min of Higher and Secondary Specialized
Education UkSSR. Odessa Polytechnic Inst), 150 copies (KL, 47-59, 115)
-31-

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SOBOLEVA, N.T.
"Zmployment of K-preparation for pediculosis control.
Zhur. Mikrobiol., Epidemiol., i Immunobiol., No-3, 15U.

SCIBOLEVA, N.I.
Dept Disinfestation, Central Sci. gesearch Inst. for Disinfection, Peiopels uommissariat for
Public Health., NKZDRAvA, (-lgh4)-
"The Fir-oil as an insecticide,"
Zhur Mikrobiol., Epidemiol., i Immi-mobiol., N03, 1944.

I
. . I .
-11, 11-11", - , 1~ . ..- . . , -u -L ,
Dissertation: "impregnation of i-abrics as an iinti-Pedicrilosis 'ii 'easure.
Inst of ',- *alaria, Mledical Parasitology and ifel-minthology, Acad Med 6ci
USSR, 31 Mar 47.
SO: Vechernyaya Moskva, Mar, 1947 (Project #17836)

SOBOLEVA, N.I. zaveduyushchiy (Moscow); RYABINKINA, A.I., zaveduyushchiy (Moscow);
M.N., glavnyy vrach; LEONT'YEV, F.A., glavnyy vrach.
Etiolog7 and pathogenesis of Taratinov's disease; sosinophilic granuloma of
the bone or benign medullary reticuloma with eosinaphilia. Arkh.pat. 15 no.[&:
37-46 Jl-Ag '53. (MI-RA 6;11)
1. Patologoanatomicheakoye otdeleniye Detskoy klinicheskoy bollnitsy im.prof.
V.P.Filatava (for Soboleva). 2. Detskaya klinicheskays, bol'nitsa im. prof.
V.P.Filatova (for Kalugina). 3. Patologoanatomicheskoye otdeleniye TSentrall-
noy klinicheskoy bollnitsy im. N.A.Semashko Hinisteretva putey soobahchenlya
(for 11yabinkina). 4. TSentralluaya klinicheskava bollnitsa im. N.A.Semashko
Ministerstva putey soobshcheniya (for Leontlyev),
(Bones--Diseases) (Tumors)

SOBOLEVA, 11.I.; YERAME179VA. A.S.
Pathogenesis of persistent fistulas appearing in the soft tissue in
children following injection of penicillin, anatoxin, and other
drugs. Arkh.pat. 18 no.?-.126-131 '56. (MIRA 10:1)
1. Iz patologoanstomicheskogo otdaleniya (zav. N.I.Soboleva, nauchnY7
rukovoditell - deystvitelinyy chlen AMN SSSR prof. M.A.Skvortaov)
Detakoy klinicheskoy bollnitay imeni Filatova (glavnyy vrach M.N.
Kalugina)
(INJECTIONS, complications,
fistulae of soft tissue on site of inject. in child. (Rua))
(FISTUIA, etiology and pathogenesis,
inject. causing fistulas of soft tissue in child. (Rua))

(Moskvn)
Pnthomorphological characteristics of otitiR in children during the first
fow months of life nB a comiDlication of BCG vaccination Lwith
summary in English]. Arkh.pat. 20 no.4:67-73 153. (MM 11:5)
1. Iz nntologoanatomicheakogo otdeleniyn (nnuchnyy rukovoditel'-
deystvitellnyy Chlen AMN SSSR prof. M.A. Skvortsov) Detakoy
klinicheskoy bollnitsy imeni N.Y. Filatova (glnvnyy vrnch H.I.
Kalugins).
(OTITIS MEDIA, in infant & child
Caused by BCG vacc. (Rua)
(BCG VACCINATION, com-'olientions,
ototis media in inf. (Rus)

SOBOLEVA. N.L, I-MUNEMA, A-S- (Moskva)
-- Case of generalized smallpox vaccinntion [with sunrinry in Inglishle
Arkh,pat. 20 no-7:78-84 158 (KRA 11:9)
1. Ix prozektur7 (nauchnyy rukovoditall - daystvitel'W chlen-
AUff SSSR prof. K.A. Sk7ortsov) Detskoy klinicheakoy bolluits7 imeni
Filatova ( lavnyy vrRch M.N. Kabigina).
?TLACCINIA, in inf. & child.
fatal generalized (Run))

IJAZURIII, A.V.; SOBOLEVA, 11.I.; CHIZHOVA, Z.P.
,;Iwo observations of diffuse lymphosarcomatosis of the gastrointes-
tinal tract in children. Pediatriia 37 no-5:85-8P MY'59 (MIRA 12:8)
1. 1z kafedry -Dropedevtiki detskikh bolezney (zav. - prof. V. A. Ylasov)
1 gos-oitallnoy nediatrii (zav. - prof. X.F. Popov) II 14oskovskogo
iedit9inskogo instituta ira. pr"of. N.I. Pirogovu na baze Detskoy klini-
cheskoy Bollnitsy im. N.F. Filatova (glavuvy vrach M.N. Kalugina).
(GASTROINTESTINU sysT_P~j neo-olasmas
lymphosorcomm, in child. (Rua))
(LY-MPqOSA'-CO?,%, case reports
pastrointestinal. in child., (Rus))

TISHi.NA) Ye.N.; SUBOLEVA, H.I.; VAYTSEIWi,,L'D, M-ye.
Anomaliea in the development of the kidneys in children. Vop. okh.
mat. i det. 6 no.8:75-80 Ag 61. (MIRA 15:1)
1. Iz Icafedra propedevtiki detskikh boleZneir (zav. - prof. V.A.Vlasov)
j
II Moskovskogo meditsinskogo instituta imeni N.I. Pirogova i iz
detskoy bollnitsy imeni N.F.Filatova (zav. - pa~61ogoanatomicheskim
otddleniyem N.I. Soboleva, lavnyy vrach L.A.V6rokhobov).
,.(KIDNEYS-1UNOATIES AND DEFORMITIM)

SOBOLEVA, N.I.; YEREMEYEVA, A.S.- VOLKOV., m.V.., dr, med.nauk
Pathamorphological characteristics of osteoblastoolastomas in
children. Ortop.,travm.i protez, no,10s'U.-18 '61.' (MIRA 14310)
1. Iz patologoanatomicheskogo otdelaniya Nav. - N.I. Sobole-va)
Detskoy klinicheskoy boVnitsy im. N.F. Filatova (glavn7y vrach -
L.A. Vorokhobov) i iz kliniki detskoy khirurgii 2-go Maskovskogo
meditsinskogo institata im. N.1. Pirogova (zav. kafedroy - ehlen-
kor. AMW SSSR prof. S.D. Zmavskiy Edeiaaaedl).
(BONES-TUMORS)

SOBOL';VA, '4-
S',,uJy-.'r,z :hc- ~rc~;ea3 of the waah-ing ..~f rell~irri canned g]lj:!:-
r~-r.~ b~r means of ultrasonic waves. Trudy MM!"? 3,~7 85
1 3~
aA :L8

G A,3 Y U I i A I P
cn -,( pc~a~3slm bi tra t :V.9 ?,,_a z a J. on
r
:a t on by. z,.,B-qns of

I
~~ ~ ;,I "! f-A
Gilts YU K 1.1; .7 M.
,9-~udylrjg -,,.c process of wine bottle washing wfth the application
of riltrasr-nic waves. Trudy 1AIJITIl, ZA2-92 164~
(MIPA :31---*:)

PILISRIONKO, Y.G.; SOBOLEVA. N.M.; PONOMAREIVA, T.N.; KADATST-kYA, K.P.
Problem of natural foci of-Brucella infections. Zhur. miltrobiol.
epid. I imimin. no.1:82-87 Ja '55. (KIaA 8:2)
1. Iz Stavropollskogo nauchno-issladovatellskogo instituta Mini-
starstva zdravookhrananiya SSSR (dir. V.N.Ter-Vartanov, nauchnyy
rukovoditell prof. H.P.Pokrovskaya)
(BRUGILLOSIS, epidamiolo&r,
in Russia, natural foci)

DAVTYAN.9 O.K.; OVCHIN111KOVA, Ye.N.; SOBOUVA, N.M.
Interaction of carbon dioxide with finely dispersed calcium
oxide in the presence of waWr vapqrs. Nauch. ezhegod. Khim.
fak. Od. un. no.2:128-129 161. (MIRA 17:8)

"On the I -2s !nce ol' I -OT `.,-ation Factor in ~ulLuros of 'Jal-royhytic 31 orous i3acteria",
tl~e 1rj.o,-Ay Lr:e Aussian scientist Ye ,oro,,r Ac,:~ordin,-, to the (,)nI,~3n'.s of
H-is Art~Cle3 "On 'he Absorl-tion of 3acteria by the Lymphatic Uands", rublishing
in Husski.,,, Ar*:chiv Fatologii, (Hussian Archive of FatholoQr), Vol. 9, 1900),
-:hur Hikrobiol, ~,r-idemiol, Nio. 12, pp 68-69, 1950.

--4i-~ ~-- !_"
LYALITSKAYA, Soflya Dmitriyevna: SOBOLEVA, N.N.. professor, redaktor; FORTROV
A.S.. redaktor; BARSUKO~ r-,iktor.
[Molotov stone ew-veral Molotovskie kamnerezy. Pn~ ru&. I.N.Soboleva.
Moskva, Vass.kooperativnoe izd-vo, 1955. 55 P. (KLRA 9:5)
(Molotov Province--Sculpture)

8h692
C, (D S/02o/6o/134/004/019/0-93
B004/BO6,4
AUTHORS. Maksimova, 0. P., Soboleval N. P., Estrin, E. I.
TITLE-, The Autocatalytic Character of the Martensite Transformation
PERIODICALg Doklady Akademii nauk SSSR, *1960, Vol~ 134, No. 4, pp. 871-874
TEM In the introduction, the authors give a survey of publications on
martensite transformation (Refs. 1-24). They investigated the autocatalytic
effect of this process by analyzing the experimental material so far
availab;e and by new experiments. On the basis of data found in the course
of the iast ten years for martens-ite transformation in strong cooling and
subsequent heating, the ratio between the heating effect Mand the VY
.' heafA A
effect Mcool of the previous cooling was determined or ~e-Ni`-hn"Ind
Fe-_Qjz~--Ni alloys (Fig. 1). The alloys 24r3 (N24G3) with m65% c,
4)'with 0.05% C, 23-0% Ni, 4 0M
23-7~ Ni, 2.8e,, b1n and H23r'4 (11UG 0% n
are mentioned. The curves obtained show a distinct maximum near the
ordinate (M heat /Mcool ). Therefore, the martensite crystals formed already
Card 1/3

The Autocatalytic Character of the Martensite S/020/60/134/004/019/023
Transformation B004/BCo-4-
at low temperature exerted a strong stimulating effect on the subsequent
0 -
transformation. With a given M cool 5 mheat is a constant for each alloy
that does not depend on the preliminary treatment. Experimentally, the
course of isothermal transformation was investigated in an Fe-Ni-Mn
alloy at -901C as a function of the martensite (M-1960) formed at -1960C.
(Figs. 2,3)~ Also in this case the autocatalytic character of transformation
was confirmed. The rate of transformation increases rapidly up to
M-1960 ~ 5%; a lesser increase was observed at M-1960 = 1 0%. Furthermore,
isothermal transformation was investigated under condit-ions under which
the transformation rate is low. As may be seen from Fig. 4, the trans-
formation rate undergoes an acceleration that even after three hours has
not yet reached its maximum. There are 4 figures and 24 references,
14 Soviet, 9 US9 1 British, 1 Chinese~ 1 French, and 1 Japanese.
ASSOCIATIONi Institut metallovedeniya i fiziki metallov Tsentrallnogo
nauchno-issledo-vatel'skogo instituta chernoy metalli-1--g4li im.
I. P. Bardina (Institute of Metal Studies and Physici-of
Metals of the Central Scientific Research Institute" of Perrou--9..'
Card 2/3 Metallurgy imeni I.--P. Bardin

ACC NR1
r~jT(m)/EWA(dVT/EWP(t) IJP(c
AP6008863
JbIHW
SOURCE CODE: UR/0128/65/000/01110003/0005
AUTHOR: Khenkin, M. L.,(Candidate of technical sciences); Nikonorova, A. I*
(Candidate of technical sciences); Gladyshev. S. A. (Engineer); Bolotova, Ye" 9#
(Engineer); Sob0leva N. P.
(Engine
_n~
iORG: none
TITLE: Stainless steel for thin-walled castings
SOURCE: Liteynoye pro zvodstvo, no. 11, 1965, 3-5
1-1,2
16
,TOPIC TAGS: metal casting, martensite steel, copper, corrosion resistance
I I tempering#
austenitic steels steel,, staidless steel/ OKhl5N4D3L stainless steel,, 35L steel
ABSTRACT: The steel used for thin-walled and intricate castings of parts of preci-
sion machinery and devices must display.a high resistance to atmospheric corrosion
without requiring a protective coating, a satisfactory fluidity, a high dimensional
istability, adequate physico-mechanical properties, and.a satisfactory machinability.
!Of the standard stainless steels not one satisfies ~the entire set of these relquirement=_
!Cr-Ni -ustenitic steels have a high corrosion resistance but a low fluidity, while
martensitic-class steels have a low corrosion resistance but an insufficient fluidity.
Hence it is normally necessary to employ1or these purposes 35L steel despite the
Ihighly undesirable necessity of coating it.electrochemically with zinc. Of the elements~_
1/2 C4 6 -45--_"_q

L -2603o--66
ACC NR., AP6008863
enhancing the fluidity of stainless steels, Cu is the most effective. In this con-
nection, six melts of the newly developed OKhl5N4D3L martensitic stainless steel (up
to 0.08% C, 0.8% Si, 0.7% kin, 14.5-17% Cr, 3-4% Ni and 3-4% Cu) were tested for flu-
idity, as a function of temperature and shape of metal. Tests of various intricate
thin-walled (1.5 mm thick) castings confirmed the definitely satisfactory casting pro-
perties of this steel -- high fluidity and absence of hot cracking. Since steels used
for thin-walled and precision castings also must satisfy high requirements with re-
spect to corrosion resistance in non-coated state, high dimensional st4bility, and
machinability, these properties were also investigated for M15MWLIAteel as com-
_~_f__0KM_hl55:N4Dh steel is such
pared with 35LI88teel. Findings: the dimensional stability
that, after its air quenching from 10200C, 2-hr treatment with cold at -70'C and 2-hr
.tempering at 600*C, this steel remains stable in time even in the presence of tempe-
rature fluctuations of from +150*C to -40*C. Compared with 35L steel, OKhl5N4D3L steel
displays superior strength p-roperties (1.5-2 times higher) as well as superior cor-
~
rosion resistance and superior machinability (30-40% higher). Thus OKhl5N4D3L steel
may be accepted as a replacement for 35L steel.wAch previously had to be used for
ithis purpose. Orig. art. has: 6 figures, 4 tables.
SUB CODE: 11, 13 00
SUBM DATE: none/ ORIG REF:
2/2
Card

ACC NR' AT6012412
SOURCE CODE: UR/OOOO/65/OO0/OOO/O329 0333
AUTHORS- Nikonorova, A.J.; Simeonov, S. L.,,- Karabasova, L. V.; Dubovaya, Go VO;
Soboleva, N. F.
ORG: none
TITLE: Coefficient of linear expansion of irylustrial titanium
SOURCE: SovaBhohaniye po metallokhimii,, metallovedeniyu i primeneniyu titana i yego
splavov, 6th. Novyye issledovaniya titanovykh splavov (New*research on titanium
alloys); trudy soveshchaniya, Moscow, Izd-vo Nauka, 1965, 329-333
TOPIC TAGS: expansion coefficient, titanium alloy, metal property / VT1-1 titanium
alloy
ABSTRACT: To determine the cause of the large scatter (AC~ = + 1.85) of the
coefficient of linear expansion _9~_' -titanium alloys, the expan on coefficient and
texture of the corresponding me were investigated an VT1-1 s ecimens. The
as measured over the temperature interval of 20--
coefficient of linear expansio ft
120C with a dilatometer, while the texture was determined by the x-ray method. The
coefficient of linear expansion was significantly affected by the texture, with three!
types of texture definable with certain values of the epansion coefficient: 110107 '1
small-grained texture corresponded to (9-,3--10.3) x 10-0 1/degree; no definable- -
terture corresponded to (8-5--9.2) x 10-'D; and IU0017 large-grained
1_j 1/2
A
1*4 7 FW P

KAYDANOVSKIY, N.L.; KOROLIKOV, D.V.; SOBOLIVA, N.S.. KHAYKIN, S.E.
Polarization of radioemission from sun spots as observed on the
3. 2 cm wave. Dokl.AN SSSR 112 no.6:1012-1015 F 157.
(miaA 10.-5)
l.Glavnaya astronomicheakava observatoriva Akademii nauk SSSR,
Pulko-vo. Predstavleno akademikom M.A. Leontovichem.
(Sun spots) (Radio astronomy)

r. . . ' .." .. V ,
SOP(` 1, In, 11-'~ , ~~. - ~. , i~ 1). V. !~".
. I ;. ~. 1 . ; r. J. I , , , . ".
"Study of the Polarization of 3 cm Radioemission of the Sun,"
imper subi~.iitted for Lhe Symosium on Radio AstronoiW, Paris, 30 Jul - 6 Aug 58

Ali THOPS: Korollkov, D.V., So SOV/26-58-1-15/36
TITLE: New Data on the Radio Emission of Sun Spots (Novoye o radio-
izluchenii solnechnykh pyaten)
PERIODICAL: Priroda, 10,58, Nr 1, PP 87-80/ (USSR)
AB3TRACT: The study of the radio emission of the sun spot areas permits
an imagination of the physical conditions in the solar atmo-
sphere above the spots, where several peculiarities can be
observed due to the existence of a strong magnetic field.
The polarization of the emission measured on various wave
lengths, can be used as a characteristic of the magnetic field
for vErious effective altitudes of the solar atmosphere.
Formerly the polarization of the sun spots, radio emission has
been observed mainly within the ranges of decimeter and meter
waves, for which the corona is responsible (over 50,000 km
above the photosphere). in 1956, observations of the polari-
zation of the sun spots' radio emission were made on the
31-cm wave in the Main Astronomical Observatory in Pulkovo.
Radiation in this range originates from the upper layers of
the chromosphere which is about 10,000 km above the photosphere.
Apparatus for these observations were prepared in the Fizi-
Card 1/3 cheskiy institut AN (Physics Institute of the AS) under the

New Data on the Radio Emission of Sun Spots SOV/26-58-1-15/36
direction of Professor S.E. Khaykin and senic.c, scientific
assistant N.L. Kaydanovskiy. For some spotE, the magnitude
of the polarized component of the radiation attained 5 % of
the radiation of the entire sun. The polarization indication
was connected with the polarity of the magnetic field on the
photosphere. Right-hand polarized radiation corresponds to
the magnetic north pole; left-hand polarized radiation, to the
magnetic south pole. The linear polarization did not exceed
0.5 ~- and could not be connected with visible changes on the
sun. The partial solar eclipse of 2 Dec 1956, was used in
Pulkovo to determine the dimensions of the radiation areas.
The effective temperature of the polarized radiation is 400,000
centidegrees. According to present concepts, the chromosphere
consists of individual strands, the hottest of which can have
a temperature of up to 150,000 centidegrees. The areas respon-
sible for the radiation that created the observed effect
Card 2/3

New Date on t~-,e Radio Emission of Sun Spots SOV/26-581-1-15/36
probably have a temperature of 5 x 10 6 degrees and a strong
magnetic field. These could be the so-called coronar con-
densations that are sometimes observed in the spot area,
There are 2 diagrams, 2 graphs and 2 Soviet references.
ASSOCIA7ION: Glavnaya astronomicheskaya observatoriya All SSSR, Pulkovo
(Plain Astronomical Observatory of the AS USSR, Pulkovo)
Card 3/3

83802
/),7 S/035/59/000/003/014/0--')9
3, 1.720 A001/AQOI
Translation from; Referativnyy zhurnal, Astronomiya i Geo-deziya, 1959, No. 3,
P. 39,-# 1946
AUTHORS., Kaydanovskiy, N. L., Ikhsanova, V. N-, Soboleva, N, S., Tlmofeyeva,
G. M,, GeV freykh
TIT-LE- A Great Burst of Solar Radio-Frequency Radiation of March 3, 1958
PERIODICAL- Solnechnyye darjiyye, 1958, No. 3, pp. 72-75
TEXT. The authors present the results of observations of radlo-frequen~~y /X
radiation burst at a wavelength of 3.2 cm. Observations were carried out at the
Pulkovo Observatory simultaneously with a polarization radiometer and the great
Pulkovo radiotelescope. The burst was connected with a visual flare of Class 3
and radio bursts at frequencies of 208, 60 and 178 Me. The imaxlzw= flux from
the burst was 10 times higher than the flux from a quiet San, The degree of
circular polarization, being equal to 7%, remained unchanged during the burst,
The angular dimensions of the activg formation which gave rise to the burst were
c.,d 1!5. Effective temperature,-jlO 'K. The difference in the coordinatea of
Card 112

83802
S/035/59/000/003/014/039
AOOI/AO01
A Great Burst of Solar Radio-Frequency Radiation of March 3, 1958~
the burst and visual flare made it possible to determine that the altittude of
I
-'-.he burst over the photosphere amounted to 0. 1 There are 8 referanc es
N, S. Soboleva
Translator's note: This is the full translation of the original Russian
abstract,
Card 2/2

82055 S/035/60/0()0/03/04/009
"%2- 0 - AOO1/AOO1
Translation- from. Referativnyy zhurnal, Astron-omiya i Geodeziya, 1960, No. 3,
0. 41, # 2310
AUTHOIRS- - Gellfreykh, G. B., Yen' Zhi-khu-a, Korol'kov, D. V., .17jzhkov, N. F.,
.., P an'_7 T--, T--
Soboleva, N. S 6 n Run yueZ
Y 1 TL. E Preliminary Results of Observations of the Solar Eclipse on Apr�l 19,
1958, With Polarization Devl,~es of Gentimeter R&nge
PERIODICAL-. SoLnechnyye dannyye, 1958, No. 5, pp. 66-70
T M, -. Recorded ourves of varietion-s in the int;5ns-ItZ,- of solar radio-
frequency radiation on the wavalengths 5.1, 3.3 and 2.0 cm are prazxeknt~~d, The
records w9re made by means of pclarization devio~~--s on- th~q Hainan island (ChPR)
during the observation of the solar eclipse on April 19, 1958, by the. Soviet-
Chinese expedition. The main results of the anal~-,Is of th,s rjurva~ are. described.
lh--y warrant the conclusions on the ixistence of ~ local source of radlo-
---fre 'uency, radiation.X'Vonnected with a group of sun-apots which was present on
the Sun's disk on the eclipse day, and or., the speotz,.Im of this source, The
values of brightness temperatbureT b havs be~~n, obta1-nr--d, as well as the va:Lues t~r
Card 112

SOV/58-59-12-28202
Translatlon from: Referativnyy zhurnal. Fizlka, 1959, Nr 12, p 247
AUTHORS, Korol'kov, D.V., Pariyskiy, Yu.N., 3qboleva, N.3,
TITLE: On the Measurements of Magnetic Fields and Other Physical
Characteristles Ln Regions Over the Runs,pnts Prnm Rqdir,-
ftspryAtinns ~V \IV
PERIODICAL-, Solnechnyve dannyye, 1958 (1959), Nr 9, pp 65 - 69
ABSTRA-_`T- A method for estimating the magnetic field, kireti.- temperature
and electronic density. from polarization observations of the
sunIs radio-emission, is given for a suffiolently wide spectral
em bapd, using instruments with a high resolving power, For
purposes of iilustrat.ion, an example of processed material or,
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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89123 S/058/61/ooo/0o2/0i4/o18
A001/AO01
A Study of Local Zones of Solar Radio Emission by Po2arization Observations at
Centimeter Wavelengths
several million degrees, are associated with sunspot groups. The radiation of
these regions is , as a rule, circularly polarized, and polarization degree
amounts to several tens per cent. Polarized radiation regions have sharply out-
lined boundaries, and their dimensions are approximately-equal to dimensions of
nuclei of the corresponding sunspot groups. Radiation of these regions is com-
paratively s-.`,able, the flux varying usually slightly during the existence of the
group. Assuming the thermal mechanism of radiation, it is possible to determine
magnetic field, kinetic temperature and density in radiation regions which are
located at an altitude of 0.05-0-07 R Q above the photosphere. Methods of
determining these characteristics are described and estimates, made on the basis
of observational materials, are presented. There are 29 references.
Translator's note: This is the full translation of the original Russian abstract.
Card 2/2

3/035/62/000/()05/036/098
3 _U0 A055/Al01
Kuznet'sova, G. V., Soboleva, N. S.
IITTLE: Observations of solar radio emission with the Great Pulkovo radio
telescope in May 1960, on the 8.7-cm wavelength
PE'RIODICAL: Referativn3~y zhurnal, Astronomiya 41 Geodeziya, no. 5, 1962, 42,
abstract 5A325 ("Solnechnyye danr-*-ye", 1961, no, 3, 70-72)
TE=': Y.nc authors reproduce the results of the observations of the Sun,
-;F-de in 'ay 1960. on the 8.7-cm wavelength, with the aid of the great Pulkovo
radio telescope with 2!9 diagram. The bright-nes--otemperature of the coronal
con"'onsations (sometimes greater than 2 - 3 - 10 K) is estimated. The tempera-
ture and the size of the radio emission burst of May 13 are also given.
N. S.
!rAbstracter's note:. Complete translation]
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379),2
2-0/0 S/035/62/000/005/037/098
3,172-0 A055/AIOl
AU7HORS: Kuznetsova, G. V., Pariyskiy, 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
FaRIODICAL: Referativnyy zhurnal, Astronomiya i Geodeziya, no. 5, 1(;)62, 42,
abstract 5A3206 ("Solnechnyye dannyye", 1961, no. 11, 65-67)
T----,?T: The results of observations of the solar eciipse of Februa-nj 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
wavegiiide, in'~o which were inserted a quarter-wave plate and a ferrite modulator L/
with 30 cps modulation frequency, was used as primary exciter. The half-power
- tfonal pattern was 0 . -traveling,-wave-
d4rec~ 1.5 As radiometer, was used a three
tube straight amplification receiver with an equivalent input noise temperature
of 41,500olr and with a passband of 300 Me. The circularly polarized component of
the radio emission and the nonpolarized radiatio 'n of the Sun were recorded. The
recording was effected on an 31111-09 (EPP-09). The antenna temperature of the
Card 1/2

S/035/62/000/005/037/098
Observations of solar radio emission ... A055/A101-
Sun outside of the eclipse was 5,5000 K. The Moon was used for the absolute 22
calibration. The flux from the Sun on the day of the eclipse was 125 , 10
watt/m2cps. The opening of the coronal condensation from 8hl7m" .5 to 8h2omin
(universal time) was ascertained from the examination of the eclipse curve.
Under the assumption that the source has a round shape (D.1-1!2) and that the
condensation has the shape of an ellipse with semiaxes 0 1
?5_x 1.14, the brigbt-
ness temperature was calculated and proved to be 3.1 - 100-K and 2.75 - job K
respectively; i.e. it proved to be higher than the temperature of the undistui'b-
ed corona. No polarization of radiation from the condensation was detected,
;-.,hich 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
FAbstracter's note: Complete translation]
I
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29571
7 S/033/61/038/004/005/010
E133/E135
AUTHORS; Korollkov, DV., and Soboleva. N.S.
TITLE, Results of observations of polarization at centimetre
wavelengths during the solar eclipse of April 19, 1958
PERIODICAL: Astronomicheskiy zhurnal, vol.38, no.4, 1961, 647-651
TEXT: Measurements were made at this solar eclipse to
investigate an effect found during the 1956 eclipse. This was the
appearance of polarized radio emission at 3 cm in the region of
sunspots, Preliminary results have already been published (Ref.3,-
A.P. Molchanov, Chen Fang-yung, Vestn. AN SSSR, No.99 1958.
Ref.4., G.B. Gellfreykh, Yehn' Jih-huaj D.V. Korollkov,
N.F. Ryzhkov, N~S. Soboleval Wu Wang'-tyug Chen Klung-yuen',
Solnechnyye dannyye No.5, 1958. Ref.5~, D.V. Korollkov,
N.S. Soboleva, G.B. Gellfreykh, Izv. Gl. astron. observ, v
Pulkove, Vol,21,. No.164, 113, 196o). observations were made at
2, 3.3 and 5.1 cm~ At 2 and 5.1 cm the total radio emission and
the I and V Stokes components of circular polarization were
measured~ the components V and Q were measured at 3.3 cm
(Q depends on parasitic effects in the apparatus),
Cord

29571
Results of observations of .... S/033/61/038/004/005/010
E133/E135
Fig.2 shows the original traces at 3.3 and 5.1 cm as the Moon
covered, and uncovered, the spot group. Also shown is the rate of
change of antenna temperature with time. Fig.3a is a diagram of
the spot group showing the regions of polarized radiation.
From a consideration of the angular spread of these regions, the
authors find that they are actually elliptical in shape. It can
be observed that the regions correspond to the umbrae of the spots,
but are slightly displaced. This effect is due to their height
above the photosphere (see Fig.3t")). Measurements of the bright-
ness temperatures of these regions, made by various observers, do
not agree very well owing to the background radiation from the
solar surface. However, the following average brightness
temDeratures for the ordinary (TBO) and extraordinary (TBe) waves
were obtained.- = 4~4 x 106, TBo = 2A x
X = 5,1 cm, TBe 106
X = 3.3 cm, TBe = 1.6 x 1o6', TBo = 0.9 x 10 6
X = 2.0 cm, TBe + TBo < 0~4 x 106, TBe - T Bo