SCIENTIFIC ABSTRACT MOLCHANOV, A. M. - MOLCHANOV, A. V.

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• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R001135010007-3
• Release Decision: RIF
• Original Classification: S
• Document Page Count: 100
• Document Creation Date: November 2, 2016
• Sequence Number: 7
• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT

300210
3/020/61/141/001/001/021
Stability in the case of a neutral ... C111/0222
There are 2 Soviet-bloc references.
PRESENTED: June 2, 1961, by M. V. Keldysh, Academician
SUBMITTED: May 23, 1961
Card 4/4

L 637-66 ZkUW/5Vm)j'r GW
37
ACC@ NRt Ap6oi5603 SOURCE CODE: @UR/0020/66/166/002/026470_2W
AUTHOR: Kolchane-vt A.. K.
ORG: none
ITITLE: Resonances in multifrequency oscillations
SOURCE: AN SSSR. Dokladyj Y. 168p no. 2p 1966t 284-287
XV
TOPIC TAGSt RlanetuT orbit' planetary satellitet osoilliLtiont parametert vector
ABSTRA02: Wtifrequency oscillations of the following fo= are studied.:
gF (I. q,
where S is a small parameter; 1 (11 @Iky - a-:,ra- - slow var iables; and
fg) are fast, (phase) variables. The concepts introduced Ewe illustrated by the
example of resonances in the solar system, In space I of slow variablesy the over-
whelming part of the points are points that do not lie on any of the resonance surfacei
4.
W) njWtM + + MW(M .=0
if the integral vectors nIq ne are linearly independentl then there exists an

L 37637-66
A(:C Nit' AP6015603
integral biorthogonal system &,j *os a blo #sop b. ouch that the vectors n,j #say r`6
are obtained from the vectors a,j a. by the integral trlan6abr transformation
at Titat + Tfta2,
. . . . . . . . . . .
0. == T,'iat+ Taft + ... - +
Analysis of tha resonances of the planets and their satellites leads to the following
conclusions: 1) the rule of maximum resonance as applied to all satellite systems and
to the planetary oyatem is that the number of resonance relations is equal to one less
than. the number of phases; 2) systems with a small number of members are fairly
homogeneous; 3) the system of Saturn and its satellites shows a clear tendency toward
the creation of a heterogeneous structure. This paper was presented by Academician
Us V. Keldysh'on 26 August 1965o Orig. art. has: 8 formulas and I table,.
so CODE: 0'6)1'L/ sm DLTz: 26Lug65/ optia REF,t oo7
12 . vmb

MoLcHMOVS &.ff.
2. usm (6oo)
4. Social,S.ciences
.7. Accounting on a co=ertial basis in constructionand bank control. Moskva.,
Goofinizdat.1952
9. Ma athlylist of Russian Accessions$ Library of Congress,, March,,1953.Unclasaified.

MOTXMMOT,, Aleksandr Mikolayevich; DUIMtSKIT, D., oty.red,;
-
--T,- -.: t., re .izd--va; LRB=. A., takha.red.
EUDIC coatrol in, coastruationj Bankovskii kontroll v stroi-
teltstva. Noakwa. Goefinisdat, 1960. 76 p. (KIU 13:10)
(Banks and banking) (Construction industry-finance)

MOLOWOV, I.Y., referent; MOICHOOT. N.G.
Nodelling of temperature distribution in a blast furnace hearth
(Tram; 'Journal of Iron and Steel Inatttutew no. 1. 1955). Stait
16 aa.1:82-83 156. (KLRL 9:5)
(Great Britain--Blast furnaces) (Heat--Tranamiasion)

HOWUNOT, L.K. .
I I .
Flexure Of plates reinforced by end stiffeners. Sudostroanie
28 @ Ar .9620 (MML 151:6)
11 15ais- (Naval architecture))

LKONID071 @Ha @
Determining the size of runners for pig iron and slag.
Stalt 24- rto.1:1&21 Ja, f64. (KMA. 17:2)
1. Gosudarstve=yy soyuzMy inatitut, po proyektiravaniyu
metaM"gichookikh zavodor,

IfawHaov A.P,
-7`4`7
@--,
Heavy infestatioa of ascarlds in a chilct. Zdrem.Belor. 5
no-7-.63-61P J1 '59. Ulm 12:9)
1. Iz kuremetalcoy aellakoy bollaitay (ClavW vrach G.A..
Bolkovalaya) Ifolodechaeaskoy oblaati.
(ASCARIDS AIM ASMRIASIS)

MOLCHMV., A. P.
MOLCHMOVt A. P. .1 ItTransitory processes. in certain systems of frequency
discrindnators.11 Min Higher FAucation USSR. Leningrad Electrical
Engineering Inst imeni, -V. 1. Ulf-yanov (Lenin). Leningrad, 1956.
(Dissertation for the Degree of Candidate in Technical Science).
Source: Knizhnaya letopis' NO, 28 1956 Moscow

HDLOMMY, A.F'..- FRDIDT. G.L.
Yarrow-band amplifiers with vibration galvawmeters. Frib.
It tekh. sksp. no.1:89-90 JI-Ag f56* (MMU Ia.-2)
(Amplifiers, Electron-tube)

@MOLMMOV A F. CMG FAM YUNG, KCROLKOV, D. V., WANG SHOU MN, tMIZABMAN, E. G.
t r E ewr@:
I
and SALCKONOVICH, A. E.
"Preliminary Results of Hadioastronomical Observations of Annular Solar
Eclipse, April 19, 1958"
paper presented at Symposium on Radio Astronomy, Paris, 30 JrI - 6 Aug 1958.

SOV/58-59-9-2io44
Translation from: Referativnyy Zhurnal Fizika, 1959, Ur 9, p 234 (USSR)
AUTHORS: Molchanov, A.P., Gyunninen, E.M., Mellnikov, AN., 14olchanov, Al.P.,
Myasnikov, L-L-TRYsakov, V.N., Skripov, F.I., Filippov, m.M.
TITLE; Results of the Observations of the Solar Eclipses of 1952 and 1954 at
a Wavelength of 3.2 em
PERIODICAL: V sb.: Polnyye solnechn. zatmeniya 25 fevr. 1952 g. 1 30 iyunya 1954 g.
Moscow, AN SSSR, 1958, pp 331 - 332
AB3911ACT: The authors give the results of the radio observations of the solar
eclipses of 25 Feb. 1952 and 30 June 1954. The residual intensities
of the sun's radio emission amount to c@. 4% and 0.98% respectively.
Card 1/1

6"6 V,
3/035/60/000/01/04/008
Translation from: Referativnyy zhurn&l, Astronomiya i Geodeziya, 1960, No. 1,
49.,
AUTHOR: Holchanov, A. P.
TIEMS Distribution of Radio-Brightness over the ZUQ!s Disk From Observations
of Total Solar LValipses at the 3.2-cm W&-v--FT-FM&%h.
PMUODICAL. V sb.: Folnyye solnechn. zatmenlya 25 fevr. 1952 1 30 iyunya 1954,
Koscow, AN SSSR@ 1958, PP. 333-335
TEXF., An attempt was made to obtain the distribution of radio-brightness
over the Sun's disk on the basis of observations of several eclipses at the 3.2-cm
It Is pointed out that, observations of different, years, at longer
wavelength. A.
wavelengths could not have been utilized, since the state of the corona changes
considerably with time. The brightness distribution presented is similar to the
distribution obtained by Alon, Arsak and Steynberg in Mar-ey by means of an
interferometer. A possible error of the calculated radio-brightness distribution
.is estimated. There are 5 references.
N. S. S.

wv/58-59-4-W6
Translation from: Referativnyy Zhurnal Fizika, 1959, Mr 4, p 232 (USSR)
AUTHORS: Yqygig,_q.S., Kushnir, V.F., Molchanov, A.P.
T =11: Results of Observations of Shift of the Effective Center of Solar Radio
Emission'@'at a Wavelength of 3.2 Cm
PERTODICAL: Solnechnyye Dannyye, 1958, Nr I - 2, pp 108 - 110
ABSTRACT: The authors submit curves showing the results of measurements of tILe shift
of the effective center of solar radio emission at a wavelength of 3.2 em
for the period December 4, 1956 - July- 30, 1957. The observations were
.carried out with the 4-m paraboloid (Main Astronomical Observatory).
Measurement, errors did not exceed 11.
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69859@
SOV/35-59-9-7128
Translation from: Referativnyy zhurnal, Astronomiya, i Geodeziya, 1959, Mr 9, p 42 (USSR)
AUTHORS: LuYan, MoIchaacy, A.P., Petrcn7a, N.G., Skripcv, Fj,
TIM: The Observation of an Annular Eclipse of the&'M on April 19, 1958, at the
4.5 cin Wavelength
PERIODICAL: Solnechnyye,dannyye, 1958 (1959), NP 8, pp.70 72
ABSTRACT; There is a citation of the photometric curve of the eclipse and the
results of its analysis. The local source connected with the group of
spots Nr 188 which were observed on the disk the day of the eclipse, pro-
duced an increase in the.emission by approximately 14% in comparison with
'he source, if one is to
the emission from the quiet Sun. The area. of t
judge by the moments of its being covered by the eclipse and unacovered
again, is near to the area of the visible group. The brightness temperature
related to thia area amounts to f"I 1,9,lo6 degree K. Two possible explara-
tions are put forward as to the origin of another local source discovered
from the anomaly of the shape of the curve, and which is not related to t7he
visible groups of spots. In one of the explanations the source is cormected-
Card 1/2, to an active region located at a height of 0.08 Ro < h 14- 0.25 Ro (Ro is

6985@
SOV/35-59-9-7128
The@ Observation of an Annular Eclipse of the Sun on April 19, !95558, at the 4.5
Wavelength
the radius of the photosphere) above a group of spots occurring on the day of tIe e0lipse
behind the disk. In another explanation, suggested by U.S. Soboleva, and V.14, lkhsanova.,
the local source is connected with the Ur. 147 group of spots, existent in the precedLng
rotation of the Sun; in the place of this group on the day of the ealipse, an er-1- =ced
brightnesa'of the coronal line at X 5303 was observed. The processing of the section of
the eclipse curve in the vicinity of the maximum phase has shown the presence of a bright
limb contributing -@6% to the total amount of the radio emission. With the width of
the li-ib being 0.06 Ro its brightness must exceed the mean radio brightness of t'he disk Tay
60%.
A.Ye. Salomonovich
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AU@@9ORS: Iaolclaanov, A. IP. , C h e n 7a n - ,, i in SOV/30-58-9-14/:-,l
TITLE: Anrular of the @Iu:i f,-.olItseobrazno,,!e zatmeniye
soIntsa) Joint BmAjition of Soviet and Chinese S-,ientists
(Sovmestni@ya ekspeflitsiya sovetskikh i kittayskik-h ucheny1n)
PERIODICAL: Vestnik Lkademii nauk SSSR, 1958, ".',r 9, pp. 66-69 (LISSR)
A.BSTRACT: The eclipse o,@ the nur took place on :.pril 19, 1958. 22 ex-
p(arts from the Soviet Union and 31 from China took part in
the observations. The ex 'uedition was led by it. F. Kolchhnov
.from the AS ITSSR and by Ohen F,-@n-yiin from the AS of the Chinc-ac.
People's Republic (KIIR). For securing the execution of the
expedition's work a spe-ial co=,ittee was formed under
IJ Yuy-syun, Vice-President of the I.-S of the Chinese People's
Republic. in the USSR the organization of the expedition wao
directed by A. A. Mikhaylov, Chairman of the AstronomicheB'-1111
sovet, (Astronomical Council).
Radionstronomical ObservatioAs (Radioastronomicheskiye
nablyudeniya)
Card 1/3 The expedition was equipped 'with 7 r,,diotelescopes. '2he obser-

Annular Eclipse of the Sun. Joint Erpedition of Soviet and SOV/30-58-9-14,/51
Chinese Scientists
vations were carried out in a wide frequency range. The opera-
tion plan was elaborated under S. 2. Khaykin, Chairman of the
Kommissiya po radionstronomii Astronomicheskogo soveta Akade-
mii nauk 'MR (Comiliesion. for Radioastronomy of the kaitlronomi-
cal Council of the AS USSR). Groups of collaborators of the
Glavnaya astronomicheakaya observatoriya (Mazin Astronomical
Observatory) under A. -?. Molohanov, D. V, Korollkov, of the
Fizicheskiy institut ism. P. I.T. Lobedeve, ('Physias Institute
imeni P. 11. Lebedev) under A. Ye. Salomonovich %nd of the
Byurakarsk"M observatoriya Akademii nauk Armyanskoy SSR
(Byura.kaa observmtory oil the AS Armyanskaya S!-:,F) under
E. G. Mirzabekyan p@:rticipated in the expedition. Nearly all
the equipment was of original design.For the disposition of
equipment for rave leneths of less than 3 cm the d-1--trict of
t1he city of eanlya (isle of Khaynan') was chosea. The ob-
servations were successfully carried out in thu wave ranee
of 0,8 to 5,1 cm by all types of equipment. it will not be
poseible to estimat --- the final results until the analysis
of the measured vaLues has been carried out. But it can a!-
ready be concluded that there i@@ a dazzling limbus on the sun.-
Card 2/3 The results ol a provisional evaluation vrere dircus@:ed in -a

Annular Eclipse of the 'Sun* Joint :Eypediltion of Soviet
and Chinese Scientiz..,to
aeminar, .,,-hich for three Jlays- anti vaa organized bT
the A3 of the Chiivuoe Pcople-'s Republic in Peking. The re-
stilts of the observatiz,,n@@ were repcrt@-.d to the branches o'
the AS in Guanlch@@hou, @@hr;-nghiki, 1@pnking and at a meeting of
the Presidium of the .Icadem,, in Pekinr. Pro-
vious to the )rork, in Pekin,- courses were held
general problemn of tho astrophysics and rLdioantronomy
-d oractical trainirg -.@ia-u given in the place of observation.
There are 2 figures.
.ard 3/5

,AUTHORS: Vyatkina, Y. 11J., Ivanova, Z. A. SOV/108-13-to-7/13
o"Lolchanov, A. P.
TITLE: Phage Discriminator (Fazovyy diskriminator)
PERIODICAL: ReLdiotekhnika, 1958, Vol 13, Nr lo, PP 39 - 44 (USSR)
ABSTRACT: One of the principal requirements placed upon phase-
discriminators is stability of balancing. A
circuit is investigated which according to assertions
by the author, exhibits a high stability. Formu-;ae for
the computation of a high balancing stability phase-
discriminator are dedueed. The discriminator
characteristic and the stability of this circuit are
compared with a bridge circuit with the same parameters.
For this purpose the bridge circuit is investi.-ated in a
similar manner with a trapezoidal -tbst signal., The. -phase
discriminator is investigated experimentally, the results
of this work being presented in this paper. There are
11 figures and 3 references, 2 of which are Soviet.
SUBUITTED: March 26, 1957
Card 1A I

Translation from:
-pp. 53-54, # 6276
83h4o
8/0 35ra 0 AOO /00 7/00 7/0 G' 8
AOOl/A0O1
Referativnyy zhurnal, Astron omiya I Geodeziya, 1960, No. 7.
AUMOR: Molchanov, A.P.
TIM% On the Possibility of.Forecasting Appearances of Some Sunspots From
-k, Radioastronomical Observations (Preliminary Information'7-
PM11ODICAL: Solnechnyye dannyye, 1959, No. 4. pp. 82-83
TEXT: The author holds it for p--ssible to forecast the app;_-arance of optical-
ly visible sunspots from the observations of the shifts of the effective center
of solar radio-frequency radiation. 'The given method is based on the results of
visual and radio-observations at a wavelength of 3.2 cm, carried out by the LIX
Glavnaya astronomicheskaye. observatoriya AN SSSR (Main Astronomical Observatcry
AS USSR)'at Pulkovo since December 1956. The method of correlations obtained is
described In detail. Twenty forecasts for groups with the area Sp '@ 200 were
made in the time from December 4, 1956, to March 23, 195T, during which'the shifts
of the,emission effective =ter exceeded considerably the errors of measurements.
The number of correct forecast@5 amounted to 75%, the number of tbe groups forecast
Card 1/2

83440
S/035/60/OW/007/W7/CO8
AOO 11AOO i
On the Possibility of Forecasting Appearances of Some Sunspots From Radio-
astronomical Observations (Preliminary Information)
to 95%, The forecasting of groups emerged with Sp :;P 100 yielded 95% correct
forecasts and 70% of the- correctly predicted number of groups. The instants of
sunspot appearances were predicted, by approximate estimates, 1q5 in advance,
not earlier. The author holds that r6gular forecasting of the appearance of
sume sunspot groups is possible, provided the frequency of radio-observationts
afid their accuracy are increased. This will aid in estimating the arem occupied
by radio-emitting formations or t-heir altitude over the opaque, for a given wave-
,length range,-level of the solar atmosphere (fr6m the magnitude of advance fcee-
casting). It is also poisible that the area of the g-oup, near the Sun's,11sk edge
will be determined more precisely from the magnitude of the shift of rJ-.e emission
effective center.
T.V. Krat
Translator's note: This is the fiall translation of the original Russian abst-ract.
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20979
.11 t 7 7@O 00YI) // 7-41 7) 3/058/61/000/004/034/042
6, N17 AG01/A101
AUTHOR: Molchanov, A.
TITLE: Increase of radio brightness at the solar disk edge at 3.2-cm wave-
length
PERIODICAL: Referativnyy zhurnal. Fizika, no 4, 1961, 415-416, abstract 4Zh592
("Solnechnyye darnyye% 1960, no 3, 68 - 69)
TEXT: The author estimates radial distribution of relative brightness
temperature of the Sun I (r@ ) at the wavelength 3.2-cm from the magnitudes of
relative residues of fluxes F r . the letter were measured during observations
of eclipses in various years aV;he instants of.-aoincidences of the lunar and so-
lar centers: I0Q @ 6 Fres/ LSresp where PG is ratio of visible radii of the
Moon and the Sun, Brea is uncovered area of the radio disk;A Tres 4nd A Sres are
differences of respective quantities at different 1@ The processing of obser-
Vation data from eclipses of 1950, 1%-1, 1954 and 195%'leads to the value of radio
diameter equal to 1,035 R. Q . The presence of brightness increase at the solar
limb, obtained by tUs meLthod, agrees with the data of interferometric observa-
tions (RZhFiz, 1964, no 3, 3013). A.S
(Abstracter's note.- Complete translation.]
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23939
3/035/61'/000/006./o22,/c.,44
7-Z A00I./AlOl
AIUMORS: Wang*Shou-kuan, Kuo Jou-hsun, Dravskikh, A.?., Kumhnir, V.F., Mol-
chanov' A P Tavasi@sherrna, K.N., Wu Hual-wei, Huang Wei-k'ung,
EFe--n-'F-a-=S--;L, Yang- Chien
TITIE Obzervat-ions of the ann-alar eclipse cf the Sun on April 19, 1958,
a:t, the 3.2-r-m wavelength
r-ER.IODII,*AL-. Referati-myy zirurn-2-1. Astr=-omiya i Geodeziya,, nc. 6, 1961, 44, at@-
stract. 6A378 ("SoIne*hnyve dannwye", 1960, no. 4. 69-72)
TW"L- The resulne of otservat.lone of the eclipse at the 3.2-cm wavelength
are presented. DurirZ the e;51ipse the radio emission flux was measured, The pGsi-
tion of the ra4@c emission effe@-,@@ive oen-,.-s-r and devia-AO-n of radio
bright.ne-es dlst@ribu-i-ion over 4,he solar disk from circular symmetry was meas-ared.
As a result of processing the cbaerv%@.-ionrxl data @*,h-:-- 117,01lowing reFLults were ob-
tainedt residual fl-,jx at @he InEtant of maxlm@m ;h-:Lsc- amounted to 23% of '-he fIU-x
from the quiet S=; -rbe fIOUX frc@fr, gro-Ap nc. 188 was tc 6% of the
flux from a 1:,oat-ea at the edge of +he dizk 4% (7). The 1--'rightness temipera-
- re Df a s, unspct Sr - up war-- 17 x 10-OK, effe-@.-tlve tempi--raT,,.Lrs cf the quia-,@ S-an
Card 112

Observa-z-Ims of -the anrealar eclipse
23239
S/"C35/6 110001006iIO2?,'O"
AOOI/AIOI
was 21 x 1030K. The eouxce at the edge. of ths- solar d1sk was identifled, by me%-
suring @'hi@ shift of ths radtc C-MiSSICn effeot'_Ive c-enter, with groip no. 11LI which
was a eoume of zt-rons ra:dl.o smtesion diuring the preceding mta-lm of -,he Sin.
Ellipticit*7 turned ou-, t.o te less -,han 1.1.
N.
(Abstra-:-.7er's note: Complete tranzlat!@_aj
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20980
3f 171.0-N i It- 24t /I -L7) S/058/6 l/0W/004/035/042
4g,cr*( 7. A0011A101
AUTHOR: Molchanov, A.?.
Mrs.$ The spectrum. of a local radio emission source on the Sun
PERIODICALz Referativnyy zhurnal. Fizika, nO 48 1961, 416, abstract 4Zh593
("Boineahnyye dannyye",. 1960, no 4, 72 - 75)
TEM The author discusses the results of measurements, at different
wavelengths, of the flux from & local source related to sunspot group No. 188,
which were aonduated during the solar eclipse of April 19, 1958, by the joint
Soviet-Chinese expedition (P2,hFiz, 1961, M520) and in Japan (RZhFiz, '1960, no 6.
15084). @ Using the obtained'data of relative fluxes and considering the data on
4-
the fluxes from.the quiet Sun in the obdervation day, the author plo.s the abso-
lute speetrum of the local source having a peak at the wavelength of r-,,,6 am. The
conalusion.is drawn that the source observed can not be aonsidered as thin one
also at X - 3.2 am which agrees with the high value of the source effective tem-
'66 ).
perature (r-4.7 x 10 K Hence the conclusion is drawn on the possible directi-
vity of emission from sources already at:;L= 3.2 am. The spectrum obtained is cm
ared with that following from the Waldmeier model. A.S.
bstracter's note: Complete translation.]
P
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20982
3,17 io (low 1/ 24, it 2,7) S/058/61/000/004/057/042
AOOI/AIOI
AUTHOESt Molahanov, &.P., Dagkesaman skiy, R.D.
TITLE: Dependence of radio emission flux from local sources on their
position an the solar disk
PERIODICALt Referativnyy zhurnal. Fizika, no 4, 1961, 416, abstract 4Zh595
("Solnechnyye dann.,,ye% 1960, no 5, 73 - 77)
TEXT: The authors present; the result of processing various obaervations
of the solar radio emission at the 50 - 3.2-cm wavelengths; these observations
were.aarrial out in order to clear up the question, whether there is dependence
of relative fluxes from local sources i(S) - Fu(G)/Fu(O) on the distance of the
.source from the disk center. Various methods of processing were employed, among
which were the following: 1) correlationtof the observed displacements of the
radio. envission gravity center with instants of sunspot groups; 2) observations
of fluxes:from individual sources by-means'of unilateral directional radiotele-
scopes; 3) measuring mean fluxed in days during which sunspot groups concentrat-
resence
ed either in the central part of the disk or in its-periphqral part. The p
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20982
Dapendence of radio emission flux ... 3/058/6 1/(YJO/()O 4,4037/042
AOOI/AlOl
of dependence i(e) was proved for 10 am (on the basis of displacement@s of
radio emission griLvity cen@Eer and correlation diagrams for various rings on the
solar disk), as well as for )-. 3.2 am. The dependence-i(8) for wavelengths 3.2,
8 and 15 am proved to the approximately the aame and close to cos 0, although in
the case of .3.2 am the relation is somewhat less pronounced. There aro 11
references.
A. S.
fAbstraater's note: Complete translation.]
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3,
-37945
S/035/62/000/005/040/098
A0551AI01
AUTHOR: Molchanov, A. F.
TITLE: on the mutual correspondence of the results of radio astronomical
and optical observations of the chromosphere
PERIODICAL: Referatiw~Tf'zhurnal,.Astrononiya i Geodeztya, no. 5, 1962, 43,
abstract 5A332 ("SolnechrV-ye dannyye", 1960,(1961), no. 11, 64-66)
TM: The author estimates the density of hydrogen filaments, at Which the
refraction index on the 0.8-cm wavelength becomes zero and the filament proves
to be a reflector. It is pointed out that the density 2 - 1013 CM-3 is <o-
gether reall and that it is possible to obtain a good agreement between the radio
astronamicai data and the optical ones. There are 9 references.
N. S.
[Abstracter's note: Complete translation]
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85991
s/i4l/6o/oo3/oo4/Ol7/Ol9
@i N17 E032/E514
AUTHOR: Molchanov, A. P.
TITLE: A Method f@r Measurl-na the Flux of Radio Emission Due to
the Moon and the Stm
PERIODICAL:Izvestiya vysshikh uchebaykh zavedeniy, Radiofizika,
ig6o, Vol-3, NO-4, PP-722-723
TEXT: Absolute-measurements of the flux of radto emtssi@n du-e-
to the'goon and the%lun are complicated by calibratlofi difficulties.
..The use of @ an absorbing surface to obtain a calibration point
(Whitenhurst, Mitchell and Copeland, Ref.2) simplifies the measure-
@ments to some ext@ent but it is still nece-asary to determine
independently the equivalent solid angle of the main lobe o .f the
receiving antenna 11. Further simplification of the measurement of
a
radio fluxes involves the introduction of two calibration points
obtained with the ald of a plane mirror. Thi's mirror should have
angular dimensions 12' equal to the dimensions of the measured
source 11 and alternately reflects Into the amteang of the radio
telescopJto be calibrated,the radiation in the direction of the
zenith (T and the radiation from a bleck surface at the temperature
of,the surrounding air T air Under these conditions Ae@
Card 115

S/141/60/005/004/01-7/019
E032/E514
A Method for Measuring the Flux of Radio Emission Due to the Moon
and the Sun a
calibration of the radio telescog consists in measuring the
radiatlon In the direction of the zenith, I.e.
Tal @ Tzm + Te+ Tatm (I - M)
and then the radiation from the black body
T&Z = Tair Pa + Tt + Tatm (I
in these expressions T I is the temperature of the antenna,
T is the temperature Of the radiation entering through the side
14bes of the antenna, Ttm. is.the temperature ofthe radiation due
to the Earth's surface. oL is a coefficient which accounts for the
dimensions of the main lobe of the receiving antenna and diffraction
effects at the mirror, and P is a coefficient describing the
"quality" of the black body. During the calibration, the receiving
antenna is fixed and after rotation of the mirror-one has
, = k(d d
T T (T T
aa &I air z 2 1
Card 2/5

85991
sli 41/60/00 3/00 4/017/019
EG32/E514
A Method-for Measuring the Flux of Radio Emission Due to the Moon
and the Sun
where di is the cbf1ection if the pointer of the recording instru-
ment and k is a constant for the particular radio telescope. The
process of measurement consists of two stages, namely, (1) the
determination of the temperature of the antenna with the telescope
pointed at the source, in which case
K W AE
Ta3 = Tsm y + TZ + atm
where y is a coefficient describing the absorption in the Earthts
,atmosphere. and (2) the determination of the temperature of the
antenna In the absence of the source, in which case
Ta4 = Ts + T'
atm,
Since the position of the antenna dur-ng the actual measurement
differs from its position during the calibration process, the
quantities which are liable to change due to this effect are
indicated by an asterisk. From the above equations one finds that
Card 3/5

85992.
S/141/60/003/004/017/019
E032/E514
A Method for Measuring the Flux of Radio Emission Due to the Moon
and the Sun
@T5Y (d 3 -d4 )/(d 2 -d1j) (M/Mx)(T air@ - TZ) (3)
.InAhe centimetre range this formula can be simplified to read
T Y d d )/d - d (T (5)
3 2 air
If theabove formula is used to determine the radio flux due to the
Noonv the. solid. angles of the soxxrce and the mirror should be chaser-
to be equal and the mirror should be located so that mle is clise
to unity. If this is not possible cc /IoLK, -can be determined empidcally,
using the above method of calibration, for a number of distances
between the antenna and.the mirror and assuming that cc/mK tends
asymptotically to unity. The low temperatures of the antenna in
such measurements can be accurately determined with the aid of
molecular amplifiers, which are already being used in radioa*ohomy
(Giordmaine et al., Ref.3). Calibration carried out in accordance
with the above method can easily be'repeated under different
Card 4/5

85992.
s/j-4i /6o/oo 3/00 4/0 17/019
E032/E5L4
A Method for Measuring the Flux of Radio Emission Due to the Moon
and the Sun,
conditions. Acknowledgments are expressed to S. E. Khaykin and
--V, S, Troitskiy for valuable discussions. There are 5 references:
3 Soviet and 2 English.
ASSOCIATION: Glavnaya astronamicheskaya observatoriya AN SSSR
(Main Astronomical Observatory AS USSR
SUBMITTED: April 4, 1960
Card 5/5

S/058/6 1/000/1002/012/018
AOO 11AO0 I
Translation fromr Referativnyy zhurnal, Fizika, 1961, Ma. 2, p. 4(34, f 2Zh506
AUTHORr Molabanov,- A.P. -
TITLE: Observations of Displadements of the Gravity Center of Solar Radio
Emission at the Main Astronomical Observatory
PEFIODICAL: "lzv. G1. astron. observ, v Pulkove% 1960, Vol. 21, No. 5, PP.
114 - 127 (Engl swrimary)
TMMt The author considers the method of observL-.g solar radio emission
using the swinging of the antenna diagram. He derives quantitative relations as-
observational results with the source distribution over the Sun and the
location of gravity center of its radio emission. Preliminary results of observa-
tions of ellipticity in solar radio emission are presented, as %ell as associa-
tions of displacements of the radio emission gravity center with instants of the
sunapots. The author describes obzervations of emission sources during an annular
eclipse and makes an attempt of forecasting the rising of auntpots on the basis of
observations of displacements of the radto, emission gravity center.
Tranalatorts note-. This is the full translation of the original Russian abstract.
Card 1/1

MOWWOTt Andrey Pavlovichl LUKITANUCt A.A*f tekhn. red@
[Couroor on radio and electric engineering) Kure elektrotekbniki i
radiotokbniki., Kookya, Oos*- izd-vo fiziko-matem. lit--17, 1961,
5C/4 P41 (MML 14t6)
("tric engineering) ("-'ia)

37943
3/035/62/000/005/038/098
3, A0551AL01
AUTHORS: Molchanov, A. P., Kaydanovskiy, N. L., Feterovp, N. G.
TITLE: observations of local sources of solar radio emission with the aid
of the great radio telescope of the GAG.(Main Astronomical Observa-
tory), on the 2.3-cm wavelength
PERIODICAL-' Referativnyy zhurnal, Astronomiye i'Geadeziya,no. 5, 1962, 42,
abstract 5A327 ("Solnechnyye dannyye't, 1961, no. 3. 68-69)
TEXT: The authors reproduce the preliminary results of the processing of
15 recordings of solar.radio emission on the 2.3 am wavelength, obtained with the
aid of the great radio telescope of the Main Astronomical Observatory, the Acadeny
oil Sciences of the USSR (width of the.main lobe of the diagram 1!8). The
dimensions of the observed sources do not exceed the distance bet4een the outer
edges of t the nuclei of the remotest spots in the corresponding group. The height
of the sources over the photosphere was (0.06 + 0,02) R E)@ f-ir the source linked
with the group no. 594, and did not exceed 0.077 R(9 for"the groups' nos,596,597.
The flux of the radio emission from the sources did not vary considerably when
the sources moved from the edge of the solar disk towards its center.
rAbstracterts note: Compl4te translation] 1. Gosachinskiy
I
Card 1/1

S/035/62/000/006/010/064
AOO1/A1Ol
AUTHORS: Molchanov, A. P.. Korol'kov, D. V.
TITLE': Radioastronomical observations of the solar eclipse of February 15,
1961, carried out by the Main Astronomical Observatory
PERIODICAL: Referativnyy zhurnal, Astronomiya i Geodeziya, no. 6, 1962, 43,
abstract 6A335 ("Solnechnyye dannyye", 1961, no. 4, 62-64)
TEXT; The authors describe the program and the main results oX radio-
astronomical observations of the solar eclipse of February 15, 1961. Observations
were carried out with seven telescopes of 2-4 m in diameter at wavelengths 2 - 21
am. as well as with the Pulkovo great radiotelescope at wavelengths 3 and 8 cm.
The following data were recorded during the eclipse: total flux, circularly-
polarized flux, displacement of the gravity center of solar radio emission, and
ellipticity of its disk. One of the main results of observations is determina-
tion of' angular.dimensions of a local source related to sunspots (group No. 41)
in the wide range of wavelengths. There are 7 references.
N. Saboleva
(Abstracter's note: Complete translation]
Card 1/1

S/169/62."000/007/131/149
D228/D307
AUTHORS: Molchanov A P. and Petrovat N. G.
TITLE: Results of observations of the solar eclipse of 15
February 1961 on the-wave 4.5 an
PER10DICAL: Referativnyy zhurnal, Geofizika, no. 7, 1962, 8-9 ab-
stract!7G55 (Solnechnyye dannyye, no. 12, 1961 (19'62),
55-57)
@_Abstracterls note.-'. Complete transiation.2
Card 1/1

33211
S/-14,1/61/004/004/017/021
E032/EI14
AUTHORSs MolchanoV, A.P., ani Caremyachenskiy,-, S.S.
TITLE4 On the use of radiatio.. pattern stanning in some
radio astronomical obse:rvations
PERIODICALi Izvastiy4 vysshikh, uchabnykh zavedeniy,
. Radiofizika, vA, no.5, 1@61, 972-975
TEXT4 The scanning of the directional diagram of the
antenna of a -radio telescope provides additional information
about the source of radiation and is currently used in rad,lio
a3tronamic&I observattc@ns. The present authors report some
quantitative relationships which are necessary for the efficient
use of the method. Thus, the power of the received signal is
expanded inti_- a Fourier series and formulae are derived for the
expansion coefficie;Mts. Results are then re-expressed in a
graphical form which is tonvenient for practical appliszationz.
There are k figures and I Soviet-bloc referen@@6.
ASSOCIATIM r2lavnaya astronomicheskaya obserTatori-la. AN SSSR
(Main Astronomical Observatory, AS USSR)
Card I/I
SUBMITTED8 Deaember 31., 1960.

Efrbot of a valtage with stepwise, vai7ing phase and frequency
on, a tuned amplifier. Radictakhnika 16 no-4:22-26 Ap 161.
(MMA 14:9)
1.@ Deystviteltrqy chlen Nauchno-tikhnicheskogo obahchastva
radiatekhnik:L i olektroavyazi im..LS6 Popova.
(Amplifiers, (Eleatronics))

N&16
s/o53/61/038/005/004/015
9133/E433
AUTffORi Molchanov, A,P.
TITLE@ The spectrum of local sources of radio emission
PERIODICAL; Astronomicheskiy zhurnal, V,38, no,@5v 1961, 849-854
TEXT,- At the present time, reliable absolute tueasures of the
spectra of solar radio sources are not available, The author has
therefore set out to investigate the ratio of the absolute spectrum
to the spectrum of the undisturbed component of the solar
radiation (denoted by FCA(k) /Fo(-k) ) @ He uses the observations of
the solar eclipse of April 19, 1958. Russo-Chinese observation&
were made at 0.89 29 3.29 4.5 and 5.2 cm (Ref.l@,A,P.Molchanov and
his team, Paris Symp, Radio Asbr...Stanford-univ, press, 1959y,
Ref.2@- G.B.Gelcfreykh and his team, Solnechayye dannyye,. ', no.5, 1958,,
Ref-33 N.A.Amenitskiy and his team', Solne--hnyye dannyye, no.7. 1958-
Ref.4. Lu Yan and his team, Solnechayye dannyye, nc@8, 058,
Ref.5z Pang Shou-Kuan and his team, Solnechnyye dannyye, no@4s 1960)
and-Japanese observations were made at 3,,2, 8, 15 and 50 cm
(Ref.63 H,Tanaka, T.Kakinuma, Rep. Ionosphere Res-, Japan, 12, 273,
1958)@ The sunspot group No.188 was observed as it was covered
by the Moon, A: maximum of the ratio F,,
Card 1/5 A/Po was observed'in the

308i
9
/005i/004/01-5
S/033/61/03
The spec;trum of local sources E133/E435
region 5- 6 cm, Assuming that the radiation is thermal, this
maximum can be ascribed to a diminution in transparency of 4Z.h.t
source, rKM may depend an the digtan,--e of the &our--,--e from the
centre of t e solar disc, This dependence is known for X .-- 10 @-m
(Ref.94 M.Waldmeier 9 Z. Astrophyz@, v.32@ 116, 1953,
Ref.103 M.B.Vanquois, C.R., v.240, A62, 19553@ A corre-@,tion for
this- effect can be derived from routine meaauraments of the solar
'
stlers an
radiation flux (Ref.11-; 1. G. 1. data on atmospherics, wh- d
solar radioemtssions,, Tokyo, 1959). The dependen--e on rad;.us does
not change much for A. in the range-.3-15 cm, Using the data
given in Ref.6 (as quoted above) and Ref'.12 (A.Ye.Salomonovich and
his teamg Solnechnyye dannyye, no,9, 83, 1959),, Ref.13
(K.M.Strezhneva and his team, Solnechnyye dannyye, n--.7, ?1, 1958),
Ref.143 U.N.Piddington,-, Astron, J,,. v.,119, 531t, 195!0.@ R6f.15-,
(B.N.Whitenhurst, F,H.@Utchell,, Proc, IeR,-E- V@44.j 1879. 1.956) and
Ptef.16 (C.W.Allen,, Monthly Notices Ray, Ast--on, Soc., -,117, .174
1957) for the spectrum of the quiet Sun-, it was found that
FWM + constant,. The relative -spect-rum was a-'sc. derived from th!:@
measurement of the displacement of the effeative centre for solar
radio emission (see Ref,---8% A.P.,Molchanov, Izv, GI, aE,.ron, cbsar-f.
Card 2/3

N816
S,(035/61/038/005/004/015
The spectrum of local sources ... E13519455
v Pulkove, no.164, 1959). From-the observations at 2 and 3.2 cm,
it was found that the absolute spectrum did-not depend greatly on
the-wavelength for X @ 3 am, &'similar rdsult has been obtained
in Ref.l9.(V.V.VLtkevLch, L.I.Matveyenka, Izv. VUZ, Radlofizika, 3,
no.3, 551, ig6o). The author conclud:eer that, in the rang4w.
am < < 5 am, the radlo flux diecreases rapidly, but that for
< 3 am th4r rate of deareas-e is leaw. Such a spectrum can only
be explained in termz of thermal radiation in a magnetic field.
It in astimated'that H > 760 gauzz. The author thankff
S.S.Khaykin for his assistance. There are-5 figures and
20 references: 11 Sdviet-bloc. and 9 non-Sovlet-bloc. The four
most recent references to English language-pubILcat:Lons are- as
follows: Ref.6: as-quated'in text; Ref,8: K.Akabane, Annals
Tokyo Astron. Observ. Sea.- ser:Les,--VI, na.2, 57, 1958;
Ref.ll:: as quoted in text; Ref.16: air quoted.in text.
ASSOCIATION: Glavnaya antronom-idheakaCywobservatoriy& Akademii
nauk SSSR (Main Astronomical Observatory AS USSRI
SUBMITTED: July 28S j-96o
Car& 3/3

MOLCHMT, A.P.., inzh.; NIKULIN, K.K., arkhitekt; SHAMRIKOV, N.I.,
1EWW
DuU4:Lng a now shop for the Sinarskaya pipe plant. From.
Stroi. 39no.8-.9-12,f6l. 14:9)
(Sinarskays.-Construetion industr5r)

S/214/62JO001002JO01/002
1046/1246
AUTHOR: Molchanov. A. P.
TITLE: Spectra and magnetic fields of local sources observed an the sun during the February 15,
1961 eclipse
PERIODICAL: Solnechnyye dannyye, no. 2, 1962, 53-58
TEXT: Spectra of the radio-frequcncy emissions were obtained at the GAO AN SSSR (Main Astronomical
Observatory of the AS USSR) for the flacullus at the center of the solar disc and for spot groups no. 41 and
no. 46 (classification of "Solncchnyye dannyye'). The slowly varying component of the solar radio emissioa
is mainly of thermal origin. Working formulas for the magnetic field at the source and for the "measure of
Iemission" expressed in terms of the spectral quantities show that the concentration of electrons in spots is
quite sufficient (N, 1010/cm3) to produce optical effects. If said effects are not observed, the assumption
concerning the thermal origin of radio emission will have to modified for groups of sun spots, taking "brems-
strahlung!* and magnetic radiation into account. There is I figure and 2 tables.
Card 1/1

&.40 ld.'sr4
AUTHORS: Barsukov, Yu.I.9 Mandrikov,
Nagnibeda, V.G.
TITLE: Ar@ificial radiation-source
calibration
PERIODICAL: Leningrad. Universitet. Vestnik.
mekhaniki i astronomiit no.
33539
S/043 62/000/001/009/009
D299YD303
V.I., Molchanovt A.P-p and
for radiotelescope
Seriya matematiki,
17 1 it 1962v 166 - 167
TEXT: An artificial radiation-source is described, used by the De-
partment of Astrophysics of Leningrad State University. This "arti-
ficial sun" is characterized by high brightness temperaturer almost
equal at all its points, and, when placed in the wave field of the
radiotelescope antennap it has angular dimensions equal to the di-
menaions of the sun. As radiation sourcep plasma in gas-discharge
tubes was used. The electron temperature of the plasma attains 104-
jo5 OK, and the size of the tubes is fairly large. In using only
the radiation from the middle part of the tubes, it is possible to
obtain a source with evenly-distributed brightness. The artificial
Card 1/3

33539
S/043/62/000/001/009/009
Artificial radiation-source for ... D299/D303
sun incorporated 20 ordinary gas-discharge tubes (of day-light)
;;C -30 (DS-30)- The tubes were placed in one row, whereby the radia-
ting region formed a rectangle (O.F x 0.5 m). The source was placed
in the wave field of the radiotele6nope antennat at a distance at
which its solid angle equalled the solid angle of the sun. The sig-
nal from the artificial source was comparedp by means of ordinary
telescopes, with the signal from the sung at 2.Or 3.6 and 4.5 cm -
waves. It was found that the artificial radiation-flow was 0.15 to
0.20 of the solar radiation. Hence theradiation temperature of the
tubes was about 2000 - 40000K. By putting a screen behind the tubest
the radiation flow was increased by 1*5 times approximately. In the
experiments already carried outq the tubes were supplied by altern.
current; a d.c. supply would somewhat increase the radiation flow. 1K
Hence the use of a screen and direct current# would lead to an ef-
fective temperature of up to 4000 - 80000K approximately. T-4e effec-
tive temperature could be further increased by ensuring adequate
optical thickness of the irradiating region (by adding tube rows,
for example). The artificial sun can be calibi:ated by means of an
absolute black bodyo It was found (by experiment) that some special
Oard 2/3

33539
E;/043/62/000/001/009/009
Ax%tificial radiation-source for ... D299/D303
types of resins are absolute black bodies in the cm-rangev having
a reflection coefficient below 0.5 %. Another method of calibration
consists in using a funnel -- directed towards the zenith -- which
is alternately covered by the black body and by the artificial sun.
There is I Soviet-bloc reference.
SUBMITTED: August 6, 1961
Card 3/3

. . HOLCHANOV, A.P., inzh.1 TITAKOV, A.I., inah.
Konitor tops over pipe-drawing shops, From. strai. 40 no.3.,
116-19 f62. OCRA 15:3)
(Pipe mills) (Raofs)

HOWMMVS, A.P.T inzh.; N@MINr K. f arkbitektor; TIrAKOT,. A.I., imho
new-*'tr* of building for tube-ftwing prodacti=w Pro=* atro:E. 40
no,7:16-19 t62. (KM 15:7)
(Factorie:@.-Desigtx and cowtruction) (Katalwork)

MDLCHANOV A.P., inzh.; NIKULIN, K.K., arkhitektor; TITAKOV, A.I., inzh.
Designs for prefabricated buildings of pipe drawing mills.
Sbor. trud. NII pa stroi. ASiA [Sverd.] no.8:17-28 963.
(K[FA 16.- 10)

MDLCHAN0714 A.P., kand.fiz,-matemnauk; TAVASTSHERNAY K.N.t kand.fiz.-matem.-
preliminary results of radio observations of the annular eclipse
of the sun. Vast. AN SSSR 33 no.308@-IPP Kr f63. (KIRA 160)
(Eclipses, Solar-1962)

2L-525-65 C 3(A(d)/EKC-&
AWO
b)/$W BSD RAEK(&)/LFMW=(-t)- dir/W-'
ACCWSIM RR =4/05539b@ BWK EXPWITATICK S/
VOMil"Y"t 7- po; Gnevy*ahem. 9. lf.; Dbmwatgkir. 0. Trt rrat, T. A.1 Narkar,
To Sharmar, If. va
I, Isd-w -i&Wmw, 411" bibUo
indices. 2,150 cogagr pribUd.
IG Tmc asi6piquics" et*uar an
TAArZ Of COnMM. (sbrldVdjs
rorpwczq
put 1. The Sun
Ch.I ratrod=tica
-'24
Ch* U. Lizicar kmatrt= of the am
Ch. III* Structwe of the photosphm; pamaau=,, opw,.aww -,41
Ch. IT. -Chrcacaphm - 69
Ch, T. FrolAbeiances - UA
Ch* vr. Cl=mo WOO 'w-
Chillro 801W awma 144

I

MOLCHANOVP AGP*
------
Slowly varying comonent af aclar radio emisaion and Its
investigatioa in the micraw&ve range. Uch. Zap. LO
na.323tlO7-IU t64. (MIRA 171-12)

VDLCHATIOvt A.P.; VTATKINAP V.11.
Anienna system for the radio astronomic.1 solar service. Izv.
GAO 23 no..1:162-168 164.
(MW 17:11)

MOLCIIIANOVI A.P.
- Application of the antenna diagram scanning to the observation
of radio emission of the sun. Izv. GAO 23 no.3:215-232 164.
(MIRA 1:7: 11)

MOIOURQV
@A.P
Some results of radio-astrontnical observations of solar eclipses.
Izv. GAO 24 no.1:38-56 164.' (YOUk 18:3)

ACC., 101. A -CODE.- UR/O
-�6609450 SOURCE@ 000/65/000/000/028
9/02
V,
WTHOR Eoloban0v4 A*- P,,,, Labutin,
ORG :.Scientifid'Council on-the Comnlex Eroblem of-g2bernetics AN, SSSR
Kiberrietika AN SSSR)
!@Naucbnyy.sovet po.k6mplekanoy problems
,TITLE*. On the frequency selectivity peakirg mechanism of the hearing
organ.-
_12
SOURCE: AN -431SR. Nauchnyy sovet po--kob 1 ek obleme Kibernetikas
`7@ a@ l9S6n5oY2r9_
Bionika- (Bion 297
iaimi_c SO 4 Moscow., Izd-vo Nauk
TOFICTAGS: audition, frequency selection, bioinstrunentation,
a.utonomic-nervous system, logic circuits electronic circuits dendrite
AB3TRACT:_ Anelectronic model simulalln-&-frequency selectivity.of the -
ear-bas-been developed by the autW`�rs.,;Tbe model is based on Huggins
abd-Lindlickerts hypothesis (1951),',wbiab-states that excitation of
neuron eMings of the ear-is proportional to the amplitude distortion of
the tympanid@membrsnef and further processing of signals of the primary
neurons-1s reduced to calculating tbe-derivative from theenvelopeof
amplitude distortions along coordinate X.,representing the distance
&long the membrane from the base of the eoeblea, It is assumed tb at
CC3,

L 205"-
ACC MR.
dif-ferentiation is real-I zed by nterve ondirg differenoos. The tympAntt
Imenbrene is considered a converter that converts a frequency coordina-to
i Ach8nnels) leadin rrom@
1-nto a -spade coordinate. In figure-3a the lines
I . - '
i'@i@-e-'-tonv-er'fer represent -- spirelgan -.neuron dendrites; nerve excits.- f
i I '@ I- - Clio, . i
ti-or" f
roii; a set' of tbree dendrites converges on eacb@ neuron. The trans-'.
imli-sion coefficient of the middle channel Is two times bigher than.thoso'L
sof the two-adjoining-ebannels-and its,output sign Is opposite (see
iFlgq 3b). Tbe model represents a tbree cbennal amplifier@vlf:b one osaill
!Iatory c1rcult in ea-cb cbsnhel. A diode detector ia conneated to eac
b
@Icbannel output. Detectors with hirb Inertiol -properties are used to
Isvold suppr6sairin of weak signals by strong signals, A te-Minal stage
!ba3edon scathods follower witb pen-todes is used to reduce output
-near elements, tl as
Despite the presence of nonli ie thr
cbgnnal- circuit ayatem ensures. increased frequency :aolectivity in tbe
modaY.simulating the tympanic membrane of-the ear, Orig, art*. bast.
9 figure3 and 8 formulas.,
C063
ZUB CODEt ORIG REP
o6/ SUBKDATE.- 266 t65/ 001/ OTH REF-w -001
AM PRESS.--q.12.5@-
8K

L 3CO12-65 FED/EWr(l)/b6(r)/MC-4/kEc(t) Fe-5/rq-0aa-2/h@4 GwAs
ACCESSION NR.' APS005782
AUTHOR. Abbasov, A. R ; Grehinakiy, h. Duresava, K. S rvanov, V. A
Holchanoy '.toy. Y.. I.
!&,at zevag ik P. ; MyAgqtkoy. V, 1. Pank,
G.; Y ov
TITLE: Rgd1oastronomic observations an the @entimeter wave of the solar eclipse
an 21 July 1963
SOURCE., Leningrad. Universitet. Vestnik. Siriya matamatiki, makhaniki. I
astronomfi"no. 1965, 102-109
TAC9*1' solar eclipse, solar atmosphere, residual radiation, terrestrial at-
mosphere, radio emission, suanpAl,
'4a expedition went to Simushic Island to observe the time of the see-and
ABSTRACT:
and,third radio contacts of the solar eclipse of 21 July L963 for detecting the
height 'of rapid changes! In the solar atmosphere during the period of weak solar ac-
tivity,and for measuring the residual radiation flux during the period of total
cover of the Sun. . The -detection of local sources of radio emission. froa to Sm during
=l.ecHp(F41- oRd'iteasuceidents-cf. tho taith-'s own atmospheric radiation were also
ta the expediti6dfit.task6 The aoldr disk vas@eovered with two groups of i

%
smfilpots,- of which one persisted only two days Including the day of the eclipse.
The refractlams abaorptioa,@ and proper radiation.af the Earth's atmosphere In-
fLuenced observation data.i The absorption and atmospheric radiation were -specLall
and after the eclipse. Strong fluctuati a of-the solar radio emis
measured before on
-*nd second contacts were recorded on 3.Z- and 10-CM wave-
siou between the first
tengths@ , The amplitude, of fluctuaftona diminished with the Increase of solar height-,
dad did ant de tveen the optical
Vend on wavelength. ;& difference was observed be
and radia, contact times. ;The residual radio emission corrected for absorption in
the terrestrial atmosphere: 1i given In a table in the- original article. An emission
of local Cources has been tecorded'on 4-s# 5-i and 10-cm waves. The localsource
U_-% Ideotiffed with the apot &COU0 which lasted only two days. The height of the
000 kim above
local ccurce was detetainad to'be: in a space apan ;frcn 7000 to 20,
thl, 201"r surface. Orfg.,arEi h4s:- 3 figurea.:7 tiobiles, and 4formulase-
ASSOWT1031 none A
T SUB 0009c AA e
SUMULTM). 21;
002
NO 004 ATD PIM i 3196 -
Cara

AA 0837z-67 EW(l), GW/WS-2
ACC
"""6028148 BOURCE.CODE., UR10058166100010051HO631HO63
usbkinsk&
AUTHOR: Apmh skirx. G. P. Kolchanor, A*- F.
'TiTLE: Radioastronomic observations of the solar eclipse of 30 Kay,1965 at wave-
'lengths f._2T aud 3.21T czm
-SOURCE: Rif zhe.Fizika, Abu. 5M451'
-MT. BOURCEI solnechn"re dMwe, no. T, i@965, 61-65
TOPIC TAGS: solar'eclipse, radio astroncmy antenna'directivity, antenna temperature
ABSTRAM: Results are presented of observations of the total solar eclipse of 30 yaw
1965.oa the Manuae Island (0 = -1901514T'v X w -158*5T,W) at wavelengths 1.2T and
.3.2T ca. The'ratio, of the lunwr radius to the solar radius was 1.048. The widths of'
the lobes of the directieLty pattern were 1.2* and 0.8* at 3.2T and 1.2T cm, respec-
tively. The effective antenna temperature for the unobscured sun was 1500 and T50K;-
thevidth of the recording track was 25 and 5K respectively at these wavelengths.
The time constant for recording was approximately 1 second. The ratio radius deter-
mined from the obaervatioda was (1.010 0.002) solar radii at 1.2T cm, and (1.03k
0.003) solar radii at 3.2T cm. This has confirmed that at VaTelentha shorter than
2 cm. the radius decreases fr= 1.03 to 1.01 solar radius, and in the region of 1. 2T
ca it apparently is independent of the wavelength, and'r 1.01. The existence
Card 112

ACC M AR6029495 CODCr UR/0137/66/0001006166A@/DOWN
Alt
"AUTHOR z Azarenko, B. sbevskiy, L. Ye.; ff. r.; Molebanow, A. F". 11
pie M*
.,TITLC-. Study of the tube drawing voctes, on a continuous drawing stand
t
rURCE: Ref. xh. Ketallurglya,, Abs. 6D239,
r Tr@ -Vsea,. n.-J. L PmLektno-konstrukt. Ln-ta net# U mashinoitr., sh.
is., 1965, 26-41-
rOPIC TAGS: 'metal drawing, metal tube
SLATION., A study was made on the continuous drawing of tube, as carried out an a
...constructed MVTU stand. The drawing capacity of the single-thread, continuous
=
,iy
awing, stand at drawing speeds of 50,mfmin was 2.8 time& greater than that of an ope-
ating 7*S tube chain stand in the Koscov, Tube Plant (at speeds of 75 m1kin, it was
.2 times greater). The high produetivity of the mill was due to the lov friction (loss
to 10%) In the auxiliary operation, to the decrease of the metal. con-,
umption coefficient during the triming of plugged up tube ends; and to the, use of
gher drawing speeds. The drawing speed was not limited by the strength of the tube
and could be much higher than 75 ajuLn. The continuous process permits the elinina-
tion of tubst awmaLing after weldLug, the jaming and cuttigig of tube endst and pic)cl-
UDCt 62L.774.001
C4CXfd I /I

MDANOT, T.Y.; REBARBAR, T.M.; MOLGRUOV A S.
Goritintulausly operating delaq network using RC loops for
automatic #Uver thickness control systems of drawing frames.
Izvvysucheb.zsv.; tekhtekst.prom. no&'5:130a-137 t6l.
(YMU 14 --'11
le Moskovakiy takatil2nyy inatitut.
(Spinning machinery) (Antda&U*,ccntroI)

S/194/62/000/005,/'022/157
D256/1508
AUTHORS: Gagarskiy, A.P., Molchanov, A.S.t and Zavilevichp'M.L.
TITLE: Blements of the electrical circuit for automatic
control of weight irregularities of ribbons
PERIODICAL4. Referativnyy zhurna". Avtomatika, i radioelektronika,
no* 5. 1962t abstract 5-2-101 d (Nauchno-issled. tr.
Tsentr. n.-i. in-t prom-sti lub. volokon, 1961, 15,
42-54)
TEZT: A detailed description is given of the elements of an automa-
tic system devised for the weight irregularity control of ribbon on
'he A -1-JI (L-1-L) ribbon machine under development for 'the spinn-
ing industry at TsNIILV. The operation of the device is based on
changing the 'speed of the pulling rollers according to the thickness
of the ribbon entering the feeding rollers; consequently the regula"
tor is a servo system. The automatic control system consists of pick-,--@Iii--
ups measuring the ribbon thickness, an integrating linkt which-adds
voltages to the pickup [Abstractor's note: Probably a misprint of
@Ifrom the ng the signal arriving from
pickups') delay unit memorizi
C
ard 1/21

3/194/62/000/005/0@2/157
@Elements of the electrical circuit D256/D308
the integrator for a period during which the ribbon passes from the
point of measurement to the point of extensiont an amplifier link,
a control motor (rotating the pialling rollers), a fAdback coupling
link comprising a tacho-gencrator driverr by the control motor. An
inductive pickup is used for continuous measuring of the ribbon
thicknessy consisting of a W-shape transformer core with two secon-
dary windings connected tn opposite phase. The delay unit includes
a phase shifting arrangement, the phase-shif"t being proportional to
the time of delay.'It consists of four R-C links with cathode-follo-
wers in between. For the amplification of the signals a DC'ampli-
fier with strong hegative feedback is employed. The driving motor
VIH -5 (PN-5) is used, the velocity pickup is a tachogene@rgtor type
3T -7/110 (ET-7/110) - Technical specification and detailed calcula-
tions of the elements are presented, 13 figures. IA'istractorls note-.-
ComDlete'translationj-
.Card 2/2,

1,11 41,C A/ f/ Ii 14-S,
GRDINL, Tu.T.. ctoktor tekhnichaskikh nauk. GAMIAROT, Tu.T., kandidat tekh-
nicheakikh nauk! --.-
Fastening rail& on reinforced concrete crane beams. Strol.prow.34
no.12:21-24 D 156. (W.RA 10: 2)
1, GIs;vW Inshener otdola kapitaVnogo, atroltel'stva. (for NoIcha-
nov).
Wranes. derricks, ate.). (Girders)

KHAVKIN, V.P.; KOTACHMOV, A.S.
*,CM-,--, M"-
Transmission functions of the drafter. Report Ill'o.2. - vys.
I uchebip za;v,,,tekhtekst., prom. .'no. 6tl36-1" t65 (MM E&tg)
1. VkGsQ3Uznyy nauabna-isslAiivatelt'skiy institut legkogo, i
tekstillhogo mashinostroyeniya, i Moskovskiy tekstiltnn in-
stitut,

KOICENCY. A.S.,zaaluzhennyr vrach RSFSR (Koakva)
----nith All-Union CGaferance of Therpneutists. Terxa.arkh. 10
no.2:73-81, F .158. (KIn 11:4)
^t
( ZrM-DISUSXS;,

KOIGMOV, A.S., zasl=hsnnyy vrnah RSYSR.
. .--
Kinutes of sessions of the Kascaw Society of Therapeutists.
TarRp.arkh. 30 ao.6.,96-98 ;* 158 (KIU 11-0
(TMMUTIGS)

[K=,ANOT, AeS&F saalrzhenyy vrach RSrSR (Koskra)
-
W -
M--"
T
enth All-Union Conference of Therapemtiets. Terap.arkh. 3a
no-10:83-92 0 '58 (KIRA 11M)
(TURAPMICW- -CONGUSSES)

MOLCHLNOVF, L.S., zaaluzhennyy vrach qSFSR (Mook7a)
First All-Russian Congreog of Therapeut@@4, Terap.ar" 32. no.4:
(KM 14:5)
79-84 Ap -,(THERLPEUTIGS-CONGRESSES)

GAGGARSKIY, A,P., m-ladshiy nauchnyy satrudnik; HQTQHAIIOV A , mladshiy
nauchrqy sotrudnik; ZA-VIUVICH, M.L.
Elements of the electric circuit for the axto=tic control of 'the
nonuniformity of the sliver weight. Nauch.-issl.trudy TSNI1LV
15:42-54 t6l. (MIRA 18:4)
1. Rukovoditell laboratorli avtomatiki TSentraltnogo nauchno@
issledo-rateltskogo instituta promyshlenrosti lubyanykh volokon
(for Zavilevich).

1?!'ER, Yti.'.,.; F:'@A,
ti
crllitnictl-r.@
fla-,,drawing fracleo- !,-7v. vys. ucrob. zav.;
'.i-ilri"Lltnyy inotit-ift ', TSontrfillra:T-@,
dovatellskiy lubyanylkn volokon.

MOLCHANOV,, A.S.
Evaluating the quality wf controllod dratting rochanisms. Izv..".
ucheb.zav.; takh.takstprom& nof3dl.Sw-125 163# (mu 16:cj)
1. Mookovskiy takatil(w institut.,
(Spinning machiuary)

KUVKIN. V.P.; MOLOHANOV, I.S. starshiy naucYLayy sotrudri&
Practical mathod for detarm@ the ftrequency characteristics of
drafters. Tekst. prom. 24 no.7:46-51 -jl 164.@ (MERA 17 '. 10)
1. Zaveduyushchiy laboratoriyey Vaesayunogo nauchno-isaledovatelt-
skogo instituta lbgkogo i tekstiltnogo mashinostroyeniya institut
promysh-lennykh lubyanylkh volok-on (TsIMUT) (for Mblclwanov).

MIOWHAIIIIOVP A.S.; V.i,.
I" amission fur,;,'Jc@- c.T the drafltc-r duripg the lor-a! bmeakin6
J. ran 7- .@-
of fibers. lzv.vyv.urhab.2av.; tr-,kh,t--kst.pro=-. no.3:220-12-4 965,
(MIRA 18:8)
1. Hoskovskiy teks"J"Ai,71y institut I Vaesopizn@y nauchnc-issledc-
vatellskly institut hgllrogo i teks.tilvnogn@ m@3H-nostr-qjuniya.

KHAVIKig-,V.P..; MOLCHANOV. k.S..
Dynamics of t". drafting process in the nonlacal, fibe.- splitting.
Izv. vys. ucheb. zav.; takhe tekso ram, no.6,.99-104 165.
(MIRk 19:1)
1. Roskovskiy tekstilInyy institut i Vsesoyuznyy nauchno-isslede-
vatel'skiy inatitut legkogo i tekstillnogo mashinostroyeniya.
Submitted September 23, 1964.

MOWMOV, La V. @ I .I
1. @ KThe Tichnolow. of Complex an(I Mixecl Fertilizers. 11 R Te. Pestov, Nauvh last TJdobr i
Ineektof,=g Iin ra. Saomoylov. 1919-1939. PP 59-71 (1@39) Ehin Referat Zhur 194-0. Yo 6, Pp
8809 (last. Insect/yuuc. in ra. T. SaMOYI(M)
SO: U-237/49, 8 April 1949

MOLO WOV,@ A.; T.
"Mixing of Fertilizers." 21. To. Pastor Chemizatim Socialistic 4V. 1940, NO 5, PP 59, Khim
R ferat Zhur, 1940, Ro 10-11. pp 45 Inct. Insect/Yung-., ta 'fa. V. SartV.,lov)
SO: U-237/49. 8 April 1949

MoLuix-ov, A.. v.
(See Brezobrazov, Tu. H.) "The Physical an(L Physical-chemical Properties of F4rtilizera.fl N.
Te. Festov, Rauch Inst Udobr i Insektofung im Ta. V. Samoylov, 1919-1930,. pp@ 62-3, Khim
Referat Kh-ar, 1940, No-, PP 89 (ME: Inat. Insect/Yung. in Taw! V. Samoy-lov)
SO: U-237149,.8 April 1949

MOMEnOT, L. V.
mThe Ancla of Flow or*Riat of Fertilizers, either Fre&@y Poure(L Omt or un&er Fressure,4
N. Te. Peator, Ag T. Hironava, Zhur Xhim Prom IVIII. No 10, pp 19-22 (194@)
(lust. Ingeat/Pubig. -in. ra. T. Samoy'lov)
SO; U-237/49. 8 April 1949

2046
4
V-
4F ,-1
40 0 -0 -.41.1 -16.

Pfacts"ll Ala PROP011fit; (21"1

NOW
d
V

to -
u
@.,,t
'dgfined did the crM. "tiXt. obtafeed by Actochem.
h
b
W I
e IRVU
SOMM U
CDWW and CMt9. t
ClIkWinalion Of
"a as prod" of ".Lmofoos Inekkat to the prooems. -
A pradtletion of WwWorocyclobe- was@
as fed thmgh the top of a`
tfkd ca a tab
Q11
wafe
.
.
g
MwnuwbIkCIymsupp1 throughtb* bottom, The
Slip rue at kvdwx U was reguiated so as to suinAy tomwill for
VI
th
M
h
b
I
e
SS
ts exte in
ut to prrmt
raw in# wit
QH*
b a CCU W the 6
Ohms
cutated t
i
JI
O
-
c
r
&
I.
at 60-4'
lexachforocydahezatiet was
"
t tht tcov
.
.
.
p
at a Mte whkb'
tt
h
h
b
d
b
om
e
o
t
contimtoistly temoyr
t
roo4
Insured Its dc*td emm. W the drained liquid. The
god rwfl t. was histilated by a 1-kw. limp, From
=
roe
the tapped liquid was diverted to a 2ad
thi.
a with the CI
d t
00 W o ret
coluinn where the Wand was cituse
it contained in soln. but am yet reacW, From, the 2od
colutim, the mixt- was 41reded to am traporotor where
COH& was driven ad in the prttence of HsO.
Unreacw
S go#
The condensed CAU440 was cooled and wpd., and tbc@
CjEorcturacdtathelotcoluma. Afterdrivingog"
the remaini,%besschiorecydahexane of any COGAM
im poured to add 1W where It was airrad
sdWiried. The ptoduct was tUterect, washed to a nentrat
rewion, old dried at ala-WO 24 brs. In tbegO C%PtA::
approx. GA% CA abAv the theorttkal qMtItY re"ised
1% Is talken to
ox
Of this ap
CJIX4 was tised
f Woo
.
.
or
d tat firmationo(COC4.
c
!*loss and the maisehar
,
v
tbe. ellk@ based an CI was 90.9 and
In these cqK1@
Oae@ L A Sn&UVMCAL
a,
foseh
M
6
c

goo
.
baxed an
1
o!ft .
n
%

S~ 04 1 11VA410-MIT 016V dot 414421 an FO-W all
'T 'A 'A I. S 1 04 0 01 a 'I IN a S A
00
0
_
@o 0 T& 0-o a -
-

BEZOMZOT.,Yu.N.; KOWHAOT,A.T. .
fl,-.~z".-.~,:-~~l"!...~~-,..-,--,.. :@-
Patting the experimental and production plant "Hexachlorand'g I-ata
operation. Rhin. prom. no. 2:56-57 F147. I (wM 8:121
1. YauabVy rnfftitut, po, udobreniyem i insaktafungisidan imeni Sm-
moy-lova
(Chemical plants) (Benzene hexachloride)

ho-M�RW
"Automatic removal of. dust from the dry filter of the DT-54 tract,,or."
MHANISAGE, ZEMMMSTVI, Praha, Czechoslovakia, Vol. 5, No. 20, October 1955.
Monthly List of Ea@-,t European Accessions LC, Vol. 8, No. 9, September 10,59.
Unclassified.

GAR, K.A.;. MOLCHANDY, A.T.; BEZQBRAZOT, ru.N.; DOOVITSKIT, A.M.
Using the ash from Cottrell filters of electric power stations
as filler in preparing dusts. (Trudyl ffIUIr no-156173-89 r55,
(MM 9:10)
(Insecticides) (Ash (Technology))

,All (I t414 Ivo (/" A v,
HA"wiAud-xwA&slVyevich; GAR,
BRUBRAZOV, IKurir Kikolayevich;,,#QJC
Konataatin. Arka(L'yevich; RMARSKI'r, U.S., red.; SHPAK, Ye.G.,
takha.red.
[Hexachloran. Ita characteristics, its manufacture, and uses]
Geksakhloraa, ego, avoiatva, poluchenie i primenenie. Nookia.
Goa, nauchno-takhn. izd-vo kh1m, lit-ry, 1958. 315 p. (MMA 116)
(Benzene hexachloriO

50) 06215
SOT/64-55-6-T/28
LUTIEORS t Molchanovt L. f., Bazobrazovf ra. N., Lbramyanj re. P.
TITLEt Enrichment of Nexachlorane by Means or Repeated Lpplication
of the Mother Liquor
PERIODIGILLt Khimicheakaya promyshlennoott, 1955, Nr 6, PP 46T - 490 (USSR)
ABSTROTt The most,widely applied and.most economical nethoda for the
separation of the f-isomer of.hexachlorane,(w commercial hex&-
chloro cyclohexane.@, which is an active insecticide, are ex-
traction methods. ..,They have, however, -the -disadvantage of
yieldhg,& prodixot containing.a, maxiaux . of.,70% of the isomer
only and a by-product of inferior-.qualIty.-These shortcomings
can be eliminated by- using the nother liquor which remains
after the filtration of the main product instead of the pare
solvent. The mother liquordissolves the f-isomer and the
readily soluble components. of.,hexachlorand,-Mkorea&.~~,tbe
difficultly soluble components can be,.-fi-Itered off. Lfter the
mother liquor has-been used 4-5 times-as extraction agent it
is, evaporated, and a, product ia obtaInad which (as the above
mentioned filtrAtion residue) eontains-only-little -is aaer and
S
is processed,. aIr-used-for the p-rodaction of 6-isome
(Ref 6).
Card 1/2 L scheme (Fig 1) of the separation of hexachlorantinto the main
product (with about 95@ of r-iaomer), the filtration residue,