SCIENTIFIC ABSTRACT MEN, A. N. - MEN, J.

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• Collection: Scientific Abstracts
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• Release Decision: RIF
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• Document Creation Date: January 3, 2017
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• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT

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BRAU13, S.Ta.; MEN', A.V.; LZBEDEVA, O.M.
Experimental at -of tuning-fork filters and some aspects of
their theory [in 4Linian with summaries in Russian and English].
Ukr.fiz.zhur. 2 no-3:274-291 Jl-S '57. (MIRA 10:10)
l.Inatitut radiofiziki ta, elektroniki AN URSR.
(Zlectric filters)

SOV/142-58-4-5/30
AUTHOR: BraudeY S.Ya., Men', A.V., Ostrovskiy, I.Ye.
TITLE: A Travelling Wave Antenna with Variable Zero rlece~tion
Bearings (Antenna begushchey voiny s reguii;ruyem,.-mi
napravleniyami nuievogo priyema)

PERIOLICAL:
Izvestiya v-ysshikh uchebnykh zavedeniy - hac;Jctekhnika,
L
1J581 Nr 4, pp q15-41_1 (USSR)
ABSTRACT: The paper discusses a system of radio reception antenn-
ae that enables L or more sourcesjof radio disfurtance
coming from different 0-irections)to be suppressed. The
system was tested experimentally. The antenna system
proposed by the author consists of:(l) Certain single-
wire antennae, piacec! (low) over the earth, which are
connected with the receiver input by a special phase
rotator. (2) The paper aiso examines the working
principle of a simple antenna system of this type,
consisting of 4'r parallel antennae, connected by a
phase rotator. Regarding (1) the zero p oint can be at
Card 1/3 any value of angle (P (angle between the linc of inri-

SOV/142-58-4-5/30
A Travelling Wave Antenna with Varlabie Z*Iero iiece,tion ~earlngs
aence of' the ground wave ana wire axis 01 tne a,rtcnna)
on the path of' the corres~ondinr search for ~-.ng_Le CI-1
with the help of a phase rotator. This characteristic
of the antenna systEm can be usea both for investi-
gating radio disturbance and for direction finaing.
Regarding (~_), this aiiGws two Qisturbunces 1'rom cif-
ferent directions to be suppresst-cl. Cieari-,-, the
principie on which the 4-antenna system i s based (L),
can also be utiiizec; to sui~,_ress 4 disturbances, re-
quiring 2 four-wire antennae in series. The experi-
mental tests of the qualities of this antenna wt-re
made on C'-,- and 4-wire antennae. The autnor gives
technical data i'or the goniometer ana the phase
rotator. The latter allows - in the wave range 6.7-E-
1.3 - phase rotations ol' high frequency osciliations
within the range zero-360'with transmission factGrs of
u.3-u.7. The reiation between the rotation angle of
the phasE rotator rotor ana the cis~,lacement of' the
high frequency phases was racticaliy iinear. Exper-
Card L/3 ience in using a four-wire antenna snoof_-(, that uurinE

SOV/142-58-4-5~/30
A Travelling Wave Antenna with Variable ~_ero heception i~earlngs
the day this antenna Lnsures stabic suppression of the
two disturbances. At night it is more Gifticult to
locate the cirection of' " disturbance ana even
this was possible, suppression was not stabie. An
antenna was testea exierimentally with one or two
adjustable zero jcints. The qualities describea are,
effective i'or th(-. rEce,.tion ot' "surl'ace" wave-, anc; non-
effective for space waves. There are ! gra,hs, 1
circuit diagram, i diagram and L reierences, 1. of
which are Soviet anc 1 American.
AS"JOCIATION: Uchenyy sovet instituta rac~,Jofiziki i clcktroniki A,N
USSR (Scientil-ic Council of' the Institute of hacio
Physics and hlcctronics, Academy of' .5ciences,
Ukrainian SSR)
SUBMITTLD: January 1~)EB
Card 3/3
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5-12 Z~.

6 7 5 -j I
SOV/141-2-3-8/26
AUTHORS: Men', A.V.A.Gorbach, V.I. and Braude,_S.Ya.
TITLE- The Effect of the Separation Boundary on the Fluctuations
of Radio Waves Propagate in a
PERIODICAL: Izvestiya vysshikh uchebnykh zavedeniy, Radiofizika,
1959, Vol 2, Nr 3, pp 388 - 394 (USSR)
ABSTRAM The authors consider, on the geometrical optics
approximation (Ref 8), amplitude and phase fluctuations
of radio waves propagated in a turbulent medium in the
presence of a plane separation boundary. In this case,
the resultant field at the detector e is given by the
sum of the direct wave and the wave reflected from the
separation boundary (Figure 1). The two fields are given
by Eq (1) in which R and 0 are the modulus and the
phase of the Fresnel reflection coefficient, respectively.
The amplitudes and phases of the signals can be written
in the form given by Eq (2), where the quantities with
subscript 11011 are inean values and AE i and Ayi are
the fluctuation components of the corresponding quantities.
Cardl/k For the case r r 2 (Figure 1), Eq (1) may be rewritten
3 LK

67531
SOV/141-2-3-8/26
The Effect of the Separation Boundary on the Fluctuations of Radio
Waves Propagated in a Non-homogenecus Medium
in the form given by Eq (5), where the symbols are
defined by Sqs (3) and (4). In the case of small
fluctuations, one has the approximate relations given
by Eqs (6) and (7) and the phase of the resultant signal
is given by Eqs (8) and (9). Assuming that the medium
is isotropic, and using Eq (9a), one obtains Eq (10),
where R E and R If are the correlation coefficients for
amplitude and phase fluctuations. Eq (10) was obtained
by neglecting the small quantities given by Eq (11).
When V 1. = 2T(h , E and 4) are given by Eq (12). In
order to carry out numerical calculations, it is assumed,
as a first approximation, that the amplitude and phase
fluctuations of the separate components e I and e 2 of
the resultant field (Eq 9a) are the same as in the absence
f the boundary. In that case one obtains Eq (14), where
is the scale of izmgularities . Using Eqs (15) and
(141), Eq (10) may be written in the form given by Eq ( 6
Card 2

6 7.-,
The Effect of the Separation Boundary on the Fluctuation, of Radio
Waves Propagated in a Non.--homngen--~-,us Medbim
It is clear froin Eq (16) that, under the above asswnpti-is.
the amplitude and phase fluctuations in the resultant
signal are equal in the distant zone. However, the
dependence of the intensity of fluctuations on the -kvaire-
length, the parat-tietGr L, and the distance rI (Figure 1)
may be quite different from that in an infinite medium.
A comparison of this theory with experiment shows good
agreement and hence it is clear that in practice it is
necessary to take into account the effect of the boundary
on the fluctuations. The above solution was obtained for
the plane problem. It would be desirable to obtain a
solution for a spherical Earth.
.part4cularly in the regions
where geometrical optics approximation does not hold.
There are 4 figures and 10 refercnces, 7 of which are
Soviet and 3 English.
Card 3/70- /~x'4
3

6 7 _5 Y,
'?,'70,90
AUTHOR: Men', A.V. SOV/141-2-3-9/26
'ion of
TITLE- On the Correl-af Fluctuations of UHF Radio Waves ii-i
the Case of Propagati-on4in a Non-homogenerus Medium
I
PERIODICALz. Izvestiya vysdtkh uc;hebnykh zavedeniy, Radiofizika,
1959, Vol 2, Nr 3t PP 595 - 399 (USSR)
ABSTRACT: The propagation of waves in a non-homogeneous turbulent
medium m = n(r, t) is accompanied by amplitude and
phase fluctuations whose statistical properties are chara-
cterised both by their intensity aad correlation at various
points in space. Most of the papers in the literature
(Refs 1-7) have been concerned with the determination of
the intensity of the fluctuations and their Gorrelation
along special directions and along the direction of propa--
gation. The present paper is concerned with the case of
an arbitrary disposition of the points under consideration
A and B (Figure 1), relative to the source of
radiation 0 . Formulae are derived for the coefficients
of longitudinal and transverse sorrelation of phase and
amplitude fluctuations. It is shown that by measuring the,
Card 1/2 ~_r

67532
SOV/141-2-3-9/26
On the Correlation of Fluctuations of LT11F Radio Waves in the Case
of Propagation in a Non-homogeneous bledium
fluctuation correlation coefficient for different
orientations of the base relative to the source, it is
possible to determine experimentally the "scale of
irregularities" which on the average characterise the
non-homogeneous medium.
There are 3 figures and 7 references, of which 2 are
English and 5 Soviet.
ASSOCIATION: Kharlkovskiy institut radiofizfk! i elektroniki
AN UkrSSR (Khar1kov Institute of Radiophysics and
Electronics of the Ac.Sc., Ukrainian SSR)
SUBMITTED: February 21, 1959
Card 2/2

KMIS , L.T. ; BRAUDE, S. Ta. -, OORPACH, V. T.
3:xperimental investigation of phase fluctuations in
centimeter radio waves propagated over water. Izv. v78.
ucheb. zav.; radiofiz. 2 no.6:848-857 159. (MIRA 13:6)
1. Institut radiofiziki i elektronlki AN USSR.
(Microwaves)

'7
9(9)
AUTHOR:
TITLE:
PERIODICAL:
ABSTRACT:
ASSOCIATION:
SUBDITTTED:
Card 1/1
nnv/?i_q0_7_j0/2r7
Men19 A47 Braude, 7.Ya. Corresponding !.-Tember o f t- e
A-] r.,qD and Gorbach, V.T.
Action of the 'Boundary on the Pluctuation of Radio
Waves in Yon-homogeneous Medium
Dopovidi Akademii Fauk T7,krainslkoi R17R, 10r9, Fr 7,
pp 740-744 (Ukrq7pl
Pquatlions are derived for the fluctuation of ampli-
tudes and phases of radio waves propagated along a
plana surface in a non-homogeneous mediin. Tt is
shomn that the fluctuation increases ,,:hen the ampli-
tude of the mean field drops to zero. There are 3
diagrams, 11 mathematic formulas and 1n references,
7 of which are Soviet and 3 Pnglish
T
Tnsty-tut radiofizyky i elektroniky A -I URSR Tns
tute of Radiophysics and Plectronics A'! 7krqF7R)
Y'arch 6, 195P
7-

80121
S/141/59/002/06/002/024
E1326aJolah'X.
AUTHORS: Men, _Braude,_S-Ya. an -_ - - . _L.
TITLE: Experimental Investigation of-the Phase Fluctuations
of the Centimetre Waves Propagated Over the Sea Surface
PERIODICAL-. Izvestiya vysshikh uchebnykh zavedeniy, Radiofizika,
1959, Vol 2, Nr 6, pp 848 - 857 (USSR)
ABSTRACT: The results of an experimental measurement of the
fluctuation of the phase fronts during the propagation"of
verti,~~ally polarized radio wayesSover the sea surface are
reported. The frequency employed was 3 000 Me/s and the
experiments were carried out under various nre-teorologi-cal
conditions during July=,September and October-pe~_-ember
over a sea route having a length of 33 km. The differential
method of measurement was,.empXoyed, in which the fluctua-
t1lorns of the phase differences of the signals recalved by
dtversity antennae were-employed to determine the intensity
and the decorrelation of the phase fluctuations at Var3.OUS
points of the wave front. In order to reduce the effect
of the boundary refraction, the receiving systems were
situated at distances of 2, 5, 10, 30 and 100 m from the
Cardl/4

80121
S/141159/002/o6/oO2/024
ElPj4E382,.
Experimental Investigation of the Phaft ctuations; of the
Centimetre Waves Propagated Over the Sea Surface
first (the standard) antenna. Altogether six antennae
were employed. The antennae were situated about 4 gi above
the sea surface. The error in the measurement 8f the
phase-d.ifference fluctuations was less than :t I ,even
if the amplitude of the received signals varied as much
as 60 db. The measurement showed that as a rule the
deviations 9 of the phase differences with respect to
the average value obey the normal law for all the trans-
mitter heights h 1 and the distances between the antennae.
The results of the measurements are indicated in Figures I
to 11. Figure I gives the overall distribution of the
phase-difference fluctuation for various distances between
the receiving antennae. Figure 2 shows the normalized
energy spectrum of the "slow" phase fluctuations for
various distances between the antennae. Figure 3 shows
the dependence of the effective value of the phase
fluctuation on the distance between the receiving antennae
Card2/4 and the height of the transmitter. The dependence of the
1~~

BOM
S/141/59/002/06/002/024
Experimental Investigation of the Phaspe-1fMCUUNations of the
Centimetre Waves Propagated Over the Sea Surface
effective Value of the "slow" and "fast" fluctuations
on the distance and height h I are illustrated in
Figure 4. The characteristic of "slow" phase fluctuations
for the case of an anomalous dependence on the height h I
are shown in Figure 5. The characteristics of the
"Complex" fluctuations are ill=rtrated in Figure 6. The
change of the intensity of th4v "slow" fluctuations for
the July-S-eptember period are shown in Figure 7.
Figure 8 illustrates the intensity of the phase fluctuations
as a function of the wind velocity (for the July-September
period). The effect of the sea waves on the inteftsity of
the phase fluctuations is illustrated in Figur-e 9. The
effect of the radio refractions on the phase fluctuations
is shown in Figure,1C T, o dep dizcq,of the normalized
0 . th V ep I
tio e yl a t w
mean-square fluctua ns on stle Pisildancleo"between the
receiving antennae is illustrated in Figure 11. The authors
Card3/4 ~Ir

80121
S/141/59/002/06/002/024
Experimental Investigation of the Phas5lHOEH'itions of the
Centimetre Waves Propagated Over the Sea Surface
express their gratitude to V.F. Shullge, O.M. Lebedeva
and B.F. Veber for their participation in carrying out
the measurements.
There are 11 figures and 14 references, 7 of which are
English and 7 Soviet.
ASSOCIATION: Institut radioflzlkl I elektronlkl AN USSR
Mnstitute of Radio-physics and Electronics of the
Ac.Sc., Ukrainian SSR
SUBMITTED: June 26, 1959
Card 4/4

9 (9
)
.
AUTHORS: Braude, S. Ya., SOV/20-125-5-18/61
Men's A. JE.
.,
V. Is
TITLE: The Fluctuations of the Phase Fronts in the Propagation of
Decimeter-radiowaves Over the Surface of the Sea
(Fluktuataii fazovykh frontov pri rasprostranenii
desyatisantimetrovykh radiovoln nad poverkhnostly-u morya)
PERIODICAL: Doklady Akademii nauk SSSR, 1959, Vol 125, Nr 5,
pp 1019-1022 (USSR)
ABSTRACT: Earlier papers dealing with this subject mainly take the
amplitude fluctuations of radio signals into account. The
phase fluctuations were investigated only in the zone of
direct visibility (mainly over the mainland). The present
paper deals with the least investigated problem, namely the
experimental investigation of phase-front fluctuations over
the sea. Ueasurements were carried out on the wave -,%-= 10 cm
in the case of vertical polarization during the period of from
July to September and October to December along a line of
33 km length leading exclusively over the sea within the
boundaries of the "illuminated zone". the "half-shade" and
Card 1/4 "shade". In these investigRtions the differential method was

-The Fluctuations of the Phase Fronts in the SOV/20-125-5-18/61
Propagation of Decimeter-radiowaves Over the Surface of the Sea
used, which (by measurement of the pulsation of the phase
difference of the electromotive force in some reception
antennas) make determination of the amount and the degree of
decorrelation of wave front, fluctuations in distributedly
arranged measuring points. The arrangement of 6 measuring
antennas along a straight line for this purpose is described.
In this way it was possible to measure phase fluctuations
within the frequency range of from 0.01 to 100 cycles. Besides,
provision was made for the possibility of filtering and sepamte
0.3 cycles) and high-
indication of low-frequency (e,
frequency (-,;, 0.3 cycles) (i.e. of the so-called "slow" and
"fast") fluctuations. According to the results obtained by
these measurements the fluctuations of phase differences were,
with rare exceptions, distributed in accordance with the
normalAaw. However, the fluctuations observed can be
coordinated to the steady random processes only with certain
reservations, for various cases of phase difference
fluctuations of signals were detected. The dependence of
fluctuation intensity on the intervals between the measuring
Card 2/4 points remained qualitatively equal in the case of all

The .. Fluctuations of the Phase Fronts in the SOV/20-125-5-18/61
Propagation of Decimeter-radiowaves Over the Surface of the Sea
experiments. The character of the height-dependence of
intensity was considerably more manifold, and therefore it
also served as a basis for the classification of experiments.
All measurements may be subdivided into 4 main groups:
1) Quasisteady standard type of phase-fluctuations. Most
experiments belong to this group which is characterized by
a monotonous reduction of fluctuation intensity with an
increasing height of the transmitter. Such a dependence is
found with propagation within a local isotropic troposphere
over a plane separating surface. These measurements have a
high degree of steadiness and good reproducibility of the
intensity and spectral composition of fluctuations. 2) The
nonsteady standard type of fluctuations is characterized by
a considerable non-steadiness of the fluctuations. 3) The
anomalous type of phase-fluctuations: in measurements of this
group the heig~~-dependence differs considerably from that
of the standard type. 4) The "flaring up" of fluctuations.
This state usually did not last longer than a few dozen
minutes, after which the usual state of the fluctuations was
Card 3/4 restored. There are 4 figures and 10 references, 3 of which
X7

829671
9. /,~00 S/142/60/003/002/007/022
AUTHOR: Men', A.V. E192/E382
TITLE: Wideband Balancing Devices (Baluns)
PERIODICAL: Izvestiya vysshikh uchebnykh zavedeniy.
Radiotekhnika. 1960, Vol~ 3, No. 2~ pp 227-252
TEXT; The transition from a non-s_ymi;ietrical line to a
.Symmetrical one in antenna feedefs-is accomplished by means
of two-conductor or coaxial stubs which are short-circuited
at the end:~ these are shown in Figs. 1. In these systems,
a shunting impedance Z. = jW Itg G , ahere W I is the
wave impedance of the stub, is connected in parallel to the
load RH Cw)W is the electrical len-th of the stub.
The input impedance of such a symmetrical !:.ystem is given by~
I
zBX = RH~ + ~2ctg 2 j
7W
~ctg -
F2c t g2
Card 1/4

82967
S/142/6o/oo5/002/007/022
E192/E362
Wideband Balancing Devices (Baluns)
where: UK
~ = R H/WL,J (2)
From Eq. (1), it follows that in order to match the balancing
junction with the feeder over a wide frequency band, it is
necessary to reduce the parameter ~ . However, this does not
permit the elimination of the reactive components. It is
possible to compensate this reactance by means of an additional
quarter-wave open-ended line section or by short-circuited
quarter-wave loops of coaxial lines having a comparatively high
wave impedance; these devices are illustrated in Figs. 2.
This compensation does not affect the resistive component of
the input impedance of the junction.. while the input reactance
becomes:
Card 2/4

8 ^-- -9 6 '
S/142/60/003/000-/007/022
Wideband Balancing Devices (Baluns) E192/E382
XBX = RHif
1 + ctg
WK / P-1i
ctg --K
(3)
where WK and -%K are the wave impedance and the electrxcal
length of the compensating line. The above formulae are
analysed graphically. Figs. 3 show the reactive component
as a function of f. for ~ = 1 and ~';= P for various
values of P . It is seen that the perfect compensation of
the reactive component for is possible at three points
only, while in the case of the compensation extends
over a certain bandwidth. The dependence of the standing-wave
ratio on Q1,,, for various values of and P is illustrated
Card 3/4

82967
S/142/60/003/002/007/022
E192/E382
Wideband Balancing Devices (Baluns)
in Figs. 4. It is also pointed out that the balancing
junctions can be used as high-frequency signal branches. A
system of this type is illustrated in Figs. 6,
There are 6 figures and 3 references-, 2 Soviet and I English.
ASSOCIATION: Uchenyy sovet Instituta radtofiziki i elektroniki
AN USSR
(Le,ny-ned Counc~-l of the Institute of Radlophysics
and Electronics of the AS USSR)
SUBMITTED: August .17, 1959
Card 4/4

20697
S/120/61/000/001/035/062
9, 60 0 0 ( e4 IL* 0 7,, 2 4,1 9 E192/E382
AUTHORS: Meng, A-V. and Zhukq I.N.
TITLE: Automatic Measuring Line for Short Radio Waves
PERIODICAL: Pribory i tekhnika eksperimenta, 1961, NG. 1,
pp. 112 - 116
TEXT: The measuring lines (including automatic ones) are
widely used for various measurements at ultrahigh frequencies
(Refs. 19 2) but at metre waves it is necessary to employ
bridge methods of measurement, These methods have a number
of disadvantages and, consequently, an attempt has been made
to devise an automatic measuring system based on a measuring
line. The system described can be used at frequencies from
10 - 40 Mc/s. The system employs a multiprobe line from
which the signals are taken by means of a switching device.
A standard coaxial cable PK-1 (RK-1), having a length
t = 0.35 kmax (where ~ - 10 m) is used as the line; this
is helically wound on a drum having a diameter of 300 mm.
A number of probes (30 in all) are situated at equal distances
along tho line, the probes being coupled rather weakly with
Card 1/3

20697
5/120/61/000/001/035/o62
Automatic Measuring Line .... E192/E382
the line. The signals from the probes are detected by
suitable detector stages. The coupling between the probes
and the line is adjusted mechanically as well as electrically,
so that all the probes have the same sensitivity. The standing
wave pattern is observed by successive switching of the out-
puts of the detector stages to the input of a measuring ampli-
fier. The signals from the amplifier are applied to an
oscillograph indicator. Since the coupling between the wave
inside the cable and the probes has to be very low,'~the
amplifiers must have a gain of about 120 db. The switching in
the instrument is performed by a multicontact frictionless
mechanical switches; the contact pairs close in succession.
In order to reduce the interference produced by the switches
the wave in the cable was amplitude-modulated. The optimum
modulation frequency was dependent on the construction of the
switching system. This frequency was 500 - 1 000 c-P-s-, the
switching frequency being 3 c.p.-g. Additional reduction in
the interference via the switching device was achieved by
providing the amplifiar with a low input resistance
Card 2/3

20697
s/12o/61/000/001/035/o62
Automatic Measuring Line .... E192/E382
(about 7-5 kS,). Physically, the instrument consists of
three unitst a high-frequency variable generator; a multiprobe
line and an amplifier plus indicator with stabilised supply
sources. The system permits a comparatively rapid measurement
of the standing-wave ratios and phase. The instrument can also
be used for the measurements of impedances and progressive
waves, which is of importance in the adjustment of antenna
systems and feeder lines. There are 4 figures and 2 Soviet
references ( one of which is translated from English).
ASSOCIATIONi Institut radiofiziki i elektroniki AN UkrSSR
(Institute of Radiophysics and Electronics
of the AS Ukrainian SSR)
SUBMITTED: January 29, 1960
Card 3/3

;;Z 7,
25 58
)'C 4 13
--6,/730 1) 2 1. D
AUTHORS: Braude, S-Ya,, Corresponding 1,1-mter AS UkrSSR
Len A~V, and Jlabo-,'~ 7 A.
TITLE- 9 p r um -.7) d , 's c r e o u r;-- e h e a s,
cosn.]c fr,~quen----es bf~.Lw
PERIODICAL: lCkadem.,ya nauk UkrayIng Klzy~ RSR, Dopovidi, n,.-
1 ~q r- I. 4 6 - 47~
TIEXT: The ai,,,-, of ~ht ~;rticle 1.11~715 -'0 irov:-.1e cbs,
of the fl,-~zx dengiliy ;,Or --',e
the r,-~,r,- e I ish 'ha, zh.-, Pe
c, e 3 n s in ti +L. G e 9 ta b I
~rtjC.-J t~hat tie abs,'rut i!)n n
ral index eq:+~al r T e ~CS
-en f j T I n anff e. V.
zed hydrog h a Z-
C60) --as abso-7-cr. --n hy~-i---g-n
HII cannct Le fesuon-ible for s' c: n a -nance --n -~X. T-
his observ.-M.,~r-ti from May to 1960. He use:i ~.-i ~ u r: ~i r,
aer-2als, 5 m apart, each ro.,is. each --+-.v Oelnr
apart. I'lach row of Fix m in len-7ti, ~la-
Card 1/3

S/
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13pectrum of di-s-re-e S.-rce
cod froa, east *D vipq Each ocic I a a norizonla.
dipole Consist1r,-, of -8 radl-- sit.,ia'A on the cylinder vi:tn an
meter of 1 m~ TI-ley were p1aced _2 ,v~r ~he meta'Liliz~.d e.,--th.
160 measurements ~n the rangE cf "he fl~.x
of the radio--soii:._-e C~a.-31crjr-.a-A vie~r.. macie b, ~nterfey-_-,,vtric.
dio telescope. 11,.rd the flux 'en--ty I k the follov,:ng
was usedi
,P
where 4Sf ~ the v,,~dtn of the bana; P -fte dif-ference bet,"It-cr,
power of the gala~_,tic i;rruunJ "I'--ther vvi'h tho di-screte soL4r_- ancz
b) the power of tne galactic grounl ,niy, A, - effe--t-.,Ve aiea Df
the aerial; -Defficient for the whole, r~.,IJJ,o-telescope (n~)t
less than 70 ~Abs-~ractor~s note: 'A e pr:ived to be pracTicai~y in-
dependent of the an~ i~, a irox,~matciy equal to
slfiowlng the rela--ion betv.,een
The results of research a.-e g~
Card 2./3

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D,9 f au -
:,~n
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f iirurf.-~i and I So v e
67 h e
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7

vc
3 A. C
,
P P-
.

3 R

5 U B I

XCE I A. V.
0---- ---1- - -
Approximation method for the analysis of the spectra of non-
stationary fluctuations. Izv. vys. ucheb. zav.; riaofiz. 4
no.3:521-533 161. (MIRA 24:10)
1. Institut radiofiziki i elektronil-i All USSR.
(Microwaves)

31995
sA42/61/oo4/ooVoi6/oi8
9192/9382
AUTHORS. Men', A,V., Zhuk, I,N. and Dudarev, N,,I.
TITLEa Multiprobe measuring line with a contactless switch
PERIODICAL~ Izvestiya vysshikh uchebnykh zavederLiy,
Radiotekhnika, v. 4, no. 4, 1961, 494 - 496
TEXT-~ The instrument described was designed and built at
the IRE AN UkrSSR (Institute of Radio-electronics of the AS
UkrSSR) and has an operating bandwidth ranging from 10-40 Me/s.
Constructioxally., it is in the form of two separate units,
the radial frequency unit and a mechanical system. The mechanical
system comprises a multiprobe line, a high-frequency capacitative
switch. a capacitative current probe-and -collector and a
synchronous drive motor operating at 1 500 r.,p.m, The line of
the system is in the form of a coaxial cable, type PV-6 (RK-6),
having an impedance of 52.-TI. and a length df 10 m; it is wound
helically on a toroid,, The electrical unit of the device
consists of four circuits,~ a signal generator; an amplifier;
a synchronous time-base and an indicator (output) circuit. The
design principle of the instrument is illustrated in Fig. 1~
Card 1/1'

ii,995
S/l42/6i/oo4/oo4/016/oi8
Multiprobe measuring line E192/E382
The signals from the HF generator I , which has a wide operating
range, are applied to the input of the long-line 2 , which is
terminated by the measured load, Weakly-coupled., screened
probes are inserted into the line at equal intervals. The HF
oscillations pj-cked-up by the probes via the RF capacitative
switch 3 , the pick-up and the cylindrical co.llector 4 14-
(which is driven by the synchronous electric motor) are applied
successively to the input of the measuring amplifier 5 . The
HF signal of the generator is modulated by a low-frequency F M
and the amplifier 7 , which is terminated by a noaresonant
detector, is tuned to this frequency~ During uniform rotation
of the switch pulse signals are produced at the output of the
amplifier and these are applied to the vertical plates aX the
cathode-ray indicator tube 6 . Simultaneously, a trigger
time-base waveform is applied to the horizontal plates of the
tube from the amplifier 7 ; the time-base is triggered by thE:
signal received from the first segment of the sw2.tch, which is
produced by a special auxiliary generator 8 , whose operating
Card 2/4

11995
S/142~61/oWooVoWoi8
Multiprobe measuring line .... C-192/E382
frequency lies outside the operating range of the instrument-
In this way, a screen of the indicator tube shows the distri-
bution of the I-IF voltage along the line, the picture being in
the form of a oeries of pulses. The en%relope of these pulses
determines the phase a 'nd modulus of the reflection coefficient
of the measured load. If the signals appearing at the output
of the 'iF si-,itch are detected directly, the instrument can be
used to measure the power standing-w-ave ratio. On the other
hand, if an auxiliary non-modulated RF signal of a large
amplitude is applied to the input detector, the voltaZe
standing-wave ratio is measured. The instrument has been
testedovcr a long period of time and it was found extremely
us,~ful in the adjustment of various types of antenna systems,
matching devices, matching of feeders, input circuits of the
receivers, filters, etc. There are 2 figures and 2 references:
1 Soviet-bloc and 1 Enr~lisll - Itef. 2 - Lester Zukeri:ian,
Electronics, 1959, 32, no. 12, 64.
Card 3/4

'.--'ultii)robe measuring I
ASSOCIATICN: Uchenyy
of the
SUBKITTED: Getober
31995
S1 I It 2/6 i/t)o4/ooVc)l6/ol3
ine .',192/ E382
sovet IRE !%i.- -, r-SSR (5cientific Council
IRE AS Uki-L-"R)
15, 1960
Fig. 1:
.3 a PYD'?
7
Card 4/4

MENI, A.V.; ZHUK, I.N.
---------
Automatic measurement line for short waves. Prib. i tekh. eksp. 6
no.1:112-116 Ja_F 161. (MIRA 14:9)
1. Institut, radiofiziki i elektroniki AN USSR.
(Radio waves--Measurement) (Pulse techniques (Electronics))

MEN I A V
Wide-band "metallic' insulators. Ukr. fiz. zhur. 6 no.2:267-272
mr-Ap 161. (miRA 14:6)
1. Institut radiofiziki i elektroniki AN USSR, g. Hhar'kov.
Coaxial cables)
ectrie insulators and insulation)
M

AUTHOR: t,1enlt APVo
2930B
S/109/61/006/010/005/027
D253/D302
TITLE: Time (spectral) characteristics of fluctuations of
phase dilVerences arising in the propagation of radio
waves in the troposphere
PERT-ODICAL:Radiotekhnika i elektronika, v. 6, no. 10, 1961,
1625 - 1635
TEXT4 This is a rt of an experimental investigation on 10 cm
vertically poiariVowaves transmitted over a fixed sea path of
length 33 km, using two receiving antennas separated by a distance
d ranging from 2 to 100 m transverse to the path. An object of the
investiration is to obtain more detailed data than presented previ-
ous -!v. The spectrum of fluctuations in the range from 0.005 - 0.01
to -1 -200 c/s is studied. The heights of the receiving antennas
(h) w----e about 4 m; the height of the transmitting antenna (ho) was
given different values of 35, 18 and 9 m. The period of the investi-
gation covered summer, autumn and winter, thus including varied
Card 1/4

29308
S/109/61/006/0.iO/C)05/027
Time (spectral) characteristics D253/D302
meteorological conditions. The records obtained were analyzed by
numerical methods; one method involved "discretization" of contin-
uous records and recovery of Fourier components. Another "continu-
ous" method made us of a mechanical correlator. Narrow-band filters
with band width 1/T were used for the analysis, T being the Waly-
sis interval. The spectral distribution observed for the different
values of ho and for d = 2 and 10 m are qualitatively similar. The
data obtained indicate a tendency to sharp reduction of spectral
density at higher frequencies, evidenced most clearly at higher
values of d and hoo peak density occuring between 0.1 and 1 c/s.
Analysis of a large number of measurements confirmed the essentie-I
non-stationariness. While the general intensity of Wluctuations vas
E
stable to within 0.5 - 1 dbg within narrow frequency in%ervals
there were large variations, of 10 - 20 db or over. The non-statio-
nariness was also shown by the variations with duration of measure-
ment; with increased duration there was increase of general inten-
sity of fluctuations together with a spectral re-distribution -,Q-
nerally towards lower frequencies. Fluctuation intensity varies as
T-1, as for "white" noise. The variations of mean spectral density
Car4 2/4

29308
S/10 61/006/010/005/027
Time (spectral) characteristics D253YD302
with frequency and with analysis band width are similar for d = 2
and 10 m and for the three values of ho; mean dispersion is � 5 db,
increasing in some cases to � 10 db, and over; spectral density de-
creases rapidly as frequency increases, the relatior following an
inverse 1.5 law for d = 2 and an inverse 2.5 law for d = 10 m. The
results are in good agreement with those given for fluctuations of
absolute phase as long as d is sufficiently large compared with 1,
the characteristic correlation dimension - (2 - 3 m). Where direct
analysis cannot be applied, a statistical method is used. The in-
fluence of meteorological conditions was investigated by making
measurements of pressure, temperature, wind and humidity at four
points along the path; no clear connection could be shown between
the spectra of fluctuations and the meteorological conditions. There
are 6 figures and 18 references: 14 Soviet-bloc and 4 non-Soviet-
bloc. The references to the English-l&Rguage publications read as
follc . R.B. Muchmore and A.D. Wheelon, PIRE, 1955, 43, 10, 1437;
k,P. D%:am and B.M. Tannin, PIRE, 1955, 43, 10, 1402; J.W. Herbst-
rent and M.C. Thompson, PIRE, 1955, 43, 10, 1191; and M.C. Thompson
Card 3/4

2~308
S/109/61/006/010/00j/027
Time (spectral) characteristics ... D253/D302
and H.B. Janes, J. Res. Nat. Bonr. Standards, 1959, 63D, 4, 45
SUBMITTED: Notember 16, 1960 1
Card 4/4

AUTHORS. Bass, F. G.,
TITLE: Fluctuations
the Pre3en:~e
PERIODICAL: Uspekhi fizi2heskikh
87576
S/05Z
BOOOB05'6
Braudo. S. Ya., Kaner, E, A., -Men', A, V
of Electroma~--netin Waves in the Tropcsphere in
of a Boundary Surfa~e
nauk, 196', Vol- 751 No, 1, pP 89-19
TEXT: The present article is a review cf theoretical rind expPrImpn4- I
s tudies on f requency, phas e, ani amp', -~' tude f I u,: lua- i--rlsf-?C fna,~n,
waves propagating- in "he trnp,~cphere as a resul" of -i'm sph-r;,.- inh-lm-.
_Peneities. The effect ~f these fluctuat;ons upon wave propagati-on in an
infinite medium was first pointed out '~y 3mclukhovsk'y; further nvestiga
tions by Einstein, Rayleigh and others (R,~fs. I - 14) followed- Hcwever,
it proved to be of essential importance to the theory of wave propagation
to take the existence of a boundary surface (surface of the Earth) into
account; this leads to interference effe7~ts and other phenomena, and th~3
theory is found to deviate essentially from the theory of fluctuation
effects in a free atmosphere. The first part is a review of essential
theoretical papers in this field First, the statistical characteristi'7s
Card 1/3

87576
Fluctuations of Electromag-net-'o Waves Jn the S/0 ~ 3/61/07 310,-1 /30
Troposphere in the Presence of a Boundary BGO~/BO56
Surface
of the electromagnetic field above the plane boundary are discussed,
after which fluctuations of the electromagnetic field in an inf4nit;,
space are discussed. In the following, the q--ia1itatf-.re effect -,f a
boundary upon the fluctuations cf this field are studiei, and a mathemat,
cal representation of the fluctuation field and of the moan field abcv-
the boundary is discussed along with some limiting cases. In the followir.,
chapters, amplitude and phase fluctuations in the far zone are dis--issed.
and the correlation of flu,7.tuations above the boundary are deaif- wi.-h. T~-.-
second part presents results obtained by experimental investigilions
of fluctuations- In the course of investigations of uli-rasonic wave
propagation, frequently the presence -)f intensive fluct--ic-ions ,f raji:
signals during their passage through the troposphere was ribserved The
investigations of these fluctuations, however, are mc%stly -f lo-al
character, so that a comparison with the theory presents difficu'ties. 1-1
recent times, investigations have been extended over larger areas (above
all oceans), so that more general results are now available. In detail, th,
authors discuss the method of measuring radio3ignal flii~tuationq, 'h"
main characteristics of fluctuations, the various types of phi3,--
Card 2/3

87576
Fluctuations of Electromagnetic Waves in the S1 53/61/073/001/303/0'14
Troposphere in the Presence o'L a Boundary B006/BO50-
Surface
tions, and the dependence of fluctuations on distance and meteorological
conditions. An experimental-theoretical comparison proves the considerabl~-
influence exerted by taking the boundary into account: It leads to a
quicker increase of fluctuations with growing distance, to a change in the
frequency dependence, to the occurrence of fluctuation flashes, to a quick
increase of the fluctuation intensity in the minima of the mean field, etc.
The problems to be theoretically solved in future consist in taking the
curvature of the boundary, the anisotropy, and the instability with time
of the medium into account. B. A. Vvedenskiy is mentioned. There are
12 figures and 45 references; 29 Soviet and 16 US.
Card 3/3

AUTHOR: Men' , A.V.-
S/141/62/005/001/007/024
E032/F,314
TITLE: On the hypothesis of the transport of "frozen-in"
turbulence in the study of fluctuations in non-
uniform media
PERIODICAL: Izvestiya vysshikh uchobny1ch zavedeniy,
Radiofizilca, v-5, no. 1, 1962, 70 - 82
TEXT: According to the above hypothesis, first put forward
by V.A. Krasillnikov (Ref. 1 - Izv.. AIN SSSR, ser. geogr. i
geofiz., 13, 33, 1949), the transport of irregularities in the
medium by wind has a primary effect on the cliange in radiowave
fluctuations with time. It has been shown that the transport
effect can be described with the aid of spatial correlation
and autocorrelation functions. It is a-ssumed in such calcu-
lations that the prop.grties of the medium remain unaltered
during the transport process and it is not -always clear whether
the assumption is, in fact, justified. In this connection
the authors investigated the possibility of the direct
Card 1/2

S/141/62/005/001/007/024
On the hypothesis E032/B314
determination of the transport effect in the troposphere
and estinated the effect of turbulent motion, diffusion,
thermal conductiv-ity and convection on the fluctuation
characteristics. It is shoim that space-tii-zie correlation
functions of fluctuations can, in most cas,es, be used to
establish the presence of the transport effect among other
processes occurrin.- in the medium and to estimate the effect
of these processes on the time characteristics of fluctuations.
A number of graphs are given to illustrate the application of
the correlation functions to these problems. These calculations
are of interest in the case of radiowaves propagating along
different routes in a nonuniform turbulent medium.
There are 4 figures.
ASSOCIATION: Institut radiofiziki i elektroniki AN UkrSSR
(Institute of Radiophysics and Electronics of
the AS UkrSSR)
SUBMUTT ED: May 26, 1961
Card 2/2

s/14i/62/005/002/010/025
t7 E032/E414
AUTHOR: Men', A.V.
TITLE: Study of the space-time correlation functions for
amplitude fluctuations in measurements on intersecting
pa ths
PERIODICAL: Izvestiya vysshikh uchebnykh zavedeniy. Radiofizika.
V-5, no.2, 1962, 287-306
TEXT: This is a continuation of previous work by this author
(Izv.VUZ. Radiofizika, v.5, 1962, 70). The results obtained in
that paper can be used in conjunction with experimen-lal data to
verify the presence of transport of medium irregularities both in
the case of frozen-in turbulence and in the more general case of
unfrozen turbulence. The experimental verification of the
theoretical results was carried out by studying amplitude
fluctuations of vertically polarized radio waves (X = 10 cm) over
sea water along a fixed path of 30 kin. The receiving antennas
were at a distance of 2 to 100 m along a line perpendicular to
the direction of transmission. The experimental procedure was as
Card 1/2

S/141/62/005/002/010/025
Study of the space-time correlation ... EOWE4i4
described by J.11.1lierbstreit and M.C.Thompson (Proc. IRE, v.43,
1955, 1391) and the present author (Radiotekhnika i clektronika,
n6.7, 1962, 232). The measurements were repeated under various
meteorological conditions (summer and autumn). Analysis of a
large volume of data indicates the presence of a transport effect
in most cases. The transport of frozen-in turbulence was Li
detected in 505 of cases. The effect of other processes
occurring in the medium (in addition to the latter effect) was
detected in 40% of all ca&es. No clear transport effect was
found in about 10510 of all cases. However, there is a considerable
discrepancy between the experimental results and theoretical
predictions. Analysis of the radio data shows that the processes
occurring in the medium are non-stationary and the ergodicity
condition may not hold. There are 8 figures.
Card 2/2

S/109/62/007/002/007/024
q. Nod D256/D303
AUTHOR: MAL"&Y-
TITLE: Correlation between amplitude and phase fluctuations
of radiowaves propagating the troposphere
PERIODICAL: Radiotekhnika i elektronika, v. 7, no. 2, 1962,
232 - 238
TEXT: The correlation between the amplitude and phase fluctuations
is investigated at a given point in space, for waves propagating
above the boundary plane in a non uniform turbulent medium. It is
shown that the correlation coefficients of the amplitude and phase)
fluctuations (i.e. the phase at the point of the receiver as measu-
red against the position of the source) derived by Chernov for an
unlimited non-uniform medium are applicable for a more general case
of wave propagation in a non-uniform medium limited by a boundary
surface. The validity of the theoretical considerations was tested
experimentally using vertically polarized 10 cm waves and measuring
at the same time the amplitude and phase fluctuations on a fixed
Card 1/2

S/109/62/007./002/007/024
Correlation between amnlitude and ... D256/D303
base of 30 km and at low altitude (35, 18 and 9 m above sea bevel).
The investigation of the wave propagation was extended into the re-
gion shielded by the Earth's curvature and as for the direct propa-
gation practically a full decorrelation of thephase and amplitude
fluctuations was observed using 100 to 200 sec averaging time. It
is pointed out that the obtained results could be of practical.
terest; by simultaneous application of both phase and amplitudt~ -.j-
thods the accuracy of measurements can be increased owing to the
statistical independence of their errors. There are 3 figures and
12 references: 11 So~riet-bloc and 1 non-Soviet-bloc. The reference
to the English-language publication reads as follows: R.B. Muchmore
and A.D, Wheelon, Proc, I.R.E., 1955, 43, 10, 1437,
SUBMITTED: December 15, 1960
Card 212

%
-7
AUTHOR: Men!, A. V.
9
S/109/62/007/003/UG1/029
D256/D302
TITILE: Effect of ',,~e transportation of space inhom-c-eneit-Jes
on radiowave fluctuations in a turbulent medium
PERIODICAL: Hadiotek~Mika i elektronika, v. 7, no. 3, 19062,
369 - 374
Consicierinc- the denen~lence of radiowave fluctuations on va-
U
rious physical processes -,aking place in zhe medium it was proposed
to employ the m;asurement~s of -fluctuations to investigate in'hon-o,-,e-
neous meaia. The measurements of fluctuations could be erq:~Ioyed to
bust the validity of t',Ie I-rozen' turoulence aDnroximation, where
time dependent (self-correlation) fluctuation functions are ex-)res-
sed b,r the sDace correlation -functions, and in particular one could
examine the ;fluctuation changes produced ny the transportation with
-~he wind of lniiomogeneities in the 'frozen' medium. The trans5or-ta-
tion with the wind of the inhomogeneities was investieated oy the
author and the experimentally observed properLies of the fluctua-
Card 1/3

Er'Cect of the trarksportatior. of ...
S/109/6z/007/003/001/029
D256/D302
tions are comnarea with the theoreiical predictions. The a.,,Iplit,.zde
fluctuatiolls 01' 3000 Yc/s radio~,iaves were i-easurea over the sea
surface at 30 km from a trans,.,,itter whose antennas viere -placed at
~ieights of 35, 18 and 9 Tn. ihe fluctuations were recorded using si-
multaneously a pole antenna and one of the antennas placed at a
diSLance of 2, 5, 10, 30 and 100 m irom the pole antenna. From the
measurements the following Y.'unctioi, was deterwined to describe the
correlation of the fluctuations
a(yi, ti)a(y, t 2)
K(d,
2
a
-h
vv.--ere a(y, t) - fluctuation of the wave amplitude or -phase;
~2
- t is the tirne shift; d = y the length of the base of
1 1 - Y2 's
the :~:easureaent, i.e. the dis-.ance between the receivin,~- ante.nnas.'
The function K(d, T) was 3eterr-ined using a mechanical correlator.
The fluctuation correlation _-~'unctions were calculated assumin.:_, a
Gaussia-yi shape pulsation of the refractive indices showing good
C)
Card 2/3

S/10 62/007/003/001/029
Effect o'~L' the transportation of ... D2 50'-YI)3 0 2
agreement with the experimental data. There are 4 figures and 11
references: 8 Soviet-bloc and ) non-Soviet-bloc. The references to
th- e E ~n lish-larguage -publications read as follows: P.G. Bergii,.ann,
Phys. 2,ev., 1946, 70, 7, 11+86; D. Yintzer, J. Acous-U, Soc. America,
195-), 25, 5, 922; 1955, -25, 6, 1107; 1954, 26, 2, 196; 'R.B. luch-
more, A.D. Y/heelon, Proc, I.R.E., 1955, 43, 10, 1437; 1955, 43, 10,
1450.
SUBYITTED: June 15, 1961
Card 3/3

., S.Ya.; ZEMKO LN ; BABOKOV9 K.A9
BRADDE . A.V., a
Radio ezisai4n spectrum of Cassiopela-4 at frequencies lower
than 30 me/see. Astron.ehur. 39 no.18163-165 XA-S 162,
(KM 15s2)
1. Inst-itut radiofiziki i elektraniki AN USSR.
(St4Lr"Peatra.)
mmio "6MOMO

S/033/62/039/003/010/010
E032/E114
AUTHORS:
Sodin, L.G., Braude, S.Ya., and Men', A.V.
TITLE: Observations of the spectra of strong bursts of solar
radio emission in the 10 - 25 Mc/sec range on
July 14 and 18,,ig6i
PERIODICAL: Astronomicheskiy zhurnal, v-39, no-3, 1962, 542-544
(+ 1 plate)
TEXT: These measurements were carried out with a 10-40 Nic/sec
spectral analyser, which included a panoramic receiver with a
wide-band high-frequency amplifier (10-40 Mc/sec), a heterodyne
with frequency conversion in the range 136-166 mc/sec, an inter-
mediate frequency amplifier (126 Mc/sec), a secbnd frequency
converter, a second intermediate frequency amplifier (2 Mc/sec)
and various indicating devices. The pass band of the apparatus
as a whole was 7 kc/sec. The analyser operates with a multi-
dipole antenna consisting of 24 dipoles. The effective area of
the antenna was 350-500 m2. The width of the main lobe of the
polar diagram of the antenna in the E - W plane was about 200.
Owing to the considerable background due to terrestrial radio
Card 1/3

Observations of the spectra of ... S,/033/62/039/003/010/010
E032/E1i4
stations, weak and medium bursts could not be observed. On
July 12, 1961, at 10 hours 20 minutes U.T. there was a rapid
increase in ionospheric absorption followed by an almost complete
fading bf all radio signals between lU and 25 Nic/sec.
Immediately after this, the solar radiation flux density rose to
about 10-19 w/m2 cps and the enhanced emission continued until
IC hours 55 minutes. After the termination of the radio burst
the enhanced ionospheric absorption continued for a further four
hours. Since the reception of the radio emission was carried
out in the side lobes of the antenna no details of the phenomena
are reported. On July 18, 1961, at 9 hours 50 minutes U.T., a
region of enhanced radio emission was found to move in from the
hign-frequency side and had a sharply defined low-frequency cut-
off. The rate of drift of the low-frequency cut-off was about
2 ',~,c/scc/sec so that the spectrum was classified as belonging to
type Il. At 9 hours 56 minutes the intensity of the burst was
found to fall and at 9 hours 58 "'inutas a second burst appearad

-ro-r the high-frequency end and persisted until 10 hours 30 rains.
A
.
It ias found that the bursts were simultaneous with large
Card 2/3

Observations of the spectra of ... S/()33/62/039/003/01-0/0-10
EC32/E114
chromospheric flares. The onset of the bursts was simultaneous
with the increase in ionospheric absorption of the type reported
by k. Sheridan and G. Trent (Observatory, v.81, 921, 1961, 71).
This phenomenon may be clue to an increase in the ultraviolet
solar radiation. In the steady-state stage, the emission
consisted of a number of separate bursts which drifted at random
at the rate of about 1 Mc/sec/sec towards both low and high
frequencies. The width of each burst lay between 0.5 and
5 Mc/sec,
There are 2 figures.
SUBMITTED: December 25, 1961
Card 3/3

ACCESSION NR: AP4007177 S/0141/63/006/005/0897/0903
AUTHOR: Paz6lyan, L. L.; Braude, S. Ya.; Bruk, Yu. M.; Zhuk, 1. N.;
Ryabov., B. P.; Sodin, L. G.; Shary*kin, N. K.
TITLE: Radiation spectra of discrete radio sources Cassiopeia A.
Cygnus A, Taurus A. and Virgo A at the 12.5 - 40 megacycle frequenv
cies
SOURCE: IVUZ. Radiofizika, v. 6. no. 5. 1963, 897-903
TOPIC TAGS: radio emission, radio emission spectra, Cassiopeia A
radio emission, Cygnus A radio emission, Taurus A radio emission,
Virgo A radio emission, radio source spectrum, discrete radio source,
radio spectroscopy, radio astronomy, radio frequency spectrum, Cassi-
opeia A,, Cygnus A, Taurus A, Virgo A, extragalactic radiation, radia-
tion absorption
ABSTRACT: To check on the hypothesis that a sharp change, mahifest
in a decrease in intensity with increasing wavelength, occurs in the
radio emission spectrum of discrete radioastronomical sources below
Card 1

ACCESSION NR: AP4007177
40 Mc, the fluxes of Cassiopeia-Aj Cygnus-A, Taurus-A, and Virgo-A
were measured in the 12.5--40-Me range., for which no reliable abso-
lute values are known. presently. To improve the accuracy, absolute
measurements were made only for the aost powerful source, Cassiopeia-
A, using seven sets of radio interferometers with half-wave dipole
antennas. The other fluxes were determined relative to this source.
The 'collapse' of the spectrum at high frequencies was noted for all
but Taurus-A. The emission measure and the ratio of the normal com-
ponent of the magnetic field to the number of electrons per cubic
centimeter of the discrete sources calculated from these measurements
are 3.5, 3.5, 5.0 and 700, 700, 120 for Cassiopeia-A, Cygnus-A, and
Virgo-A. It is assumed that the decrease in the spectrum is due
either to absorption in H.1 clouds or by a decrease of the refractive
index in the source. Orig. art. has: 2 figures, 4 formulas, and
4 tables.
ASSOCIATION: Institut radiofiziki i elektronik~ AN UkrSSR (Insti-
tute of Ridiophysics and Electronics, AN UkrSSR)
card n /12 -
r-IR! #

BASS, F.G.; MEN', A.V.
Spatial correlation of the fluctuations of waves Propagating
in an infinite turbulent medium. Akust. zhur. 9 no.3:283-290
163. (MIRA 16:8)
1. Institut radiofiziki i alektroniki A14 UkrSSR,, KharIkov.
(Sound waves)

S/108/63/018/002/004/010
D413/D308
AUTHOR: Men', A. V., Member of the Society (see Association)
TITLE: The autocorrelation characteristics of phase-difference'
fluctuations
'PERIODICAL: Radiotekhnika, v. 18, no. 2, 1963, 27-36
ITEXT: Previous studies of fluctuation in waves propagated by tur-
'bulent media have been concerned with determining the space and
time characteristics of the fluctuating field, and have investiga- i
.ted the fluctuation of absolute phases and amplitudes in greatest
;detail. The fluctuation of phase-difference between signals receivedl
-at two points is also of interest in various systems. The author
.considers the derivation of autocorrelation characteristics for this
!fluctuation, dealing with both parallel and intersecting paths. For
.the case where the medium is described by a Gaussian correlation
ifunction, he determines.,,"the autocorrelation coefficients taking
into account the transfer of both 'frozen' and 'unfrozen' turbu-
-ilences. Results calculatqd for several particular cases are shovra
Card 1/2

5/108/63/016/002/004/010
The autocorrelation characteriotios D413/D308
graphically, anq appear to Oe in jualltative agreement with experi-
;Iment, TIAere are 4 f1g4req,
ASSOCIATION: Nauchno-tekhnicheskoye obshchestvo radiotekhniki i
elektroavyazi im. A. S. Popova (Scientific and Tech-
nical Society of Radio Engineering and Electrical
Communications imeni A. S. Popov) /-Abstracter's noteli
Name of Association taken from first page of journal-/i
SUBMITTED: January 5, 1962 (initially)
April 13, 1962 (after revision)

Tf
!,ACCESSION NR: AP4037397 S/0106/64/000/f)05/0014/0021
AUTHOR: Dazelyan L. L.; Druk, Yu. He; Zhuk, 1. N.;_Men', A. V.;
Phary*kin, No K*
TITLE: WLde-band highly directional antenna for decameter Wav e-
lengths
�,OURCEt ElektrosvyazI, no, 5, 1964, 14-21
TOPIC TAGS: antenna, directional antenna, highly directional anten-~
na,wide band antenna.wide band highly directional antenna. beam-
width electric control, half.wave dipole, shunt dipole, cylindrical
dipole, array element, antenna element, antenna efficiency. antenna
gain
ABSTRACT: A receiving antenna intended for radioastronomical inves-~
tigation of discrete sources and cosmic background in the 20-40-mc
range is described. The antenna was designed on the principle that
the electric control of the beam at large scanning angles can be
realized by phasing low-dLrectional discrete elements, whose large
Crd 1/3

ACCESSION NR: AP4037397
number.insures the required degree of resolution. The antenna arralf
located along the W-E line, consists of 128 half-wave wide-band
cylindrical dipoles arranged in 4 rows, each carrying 32 dipoles.
The cylinders, formed by 18 elements of 8 mm each, are I m in diam--:
etere The distance between array-element centers along and across
the array is 5.5 m. The array elements are suspended 3 m above the
I ground. The signal excited in each element is transmitted to the
output of each row through a matching balancer, three adders, and
three coaxial cables with a total length of 101 m. The toroidal
ferrite transformers used as adders made it possible in the 10- to
60-mc range to achievp a VSWR of 1.05 or better at a rated load
with an efficiency of 95 to 97% or better. The electric control
of the beam, which is accomplished by inserting delay cables be -
tween the adder and the output of each rowp is carried out only in
the N-S planes The radiation pattern and gain of the antenna were
determined by the simultaneous recording of signals from Cassiopea-A'
received with the antenna described and a standard interfarometer
consisting of two half-wav?'dipoles and subsequent: comparison of the:'
Card 2/3

ACCESSION M AP4037A97
results. At the same time the effective area (gain) was calculated
by computer, Good agreement of experimental and theoretical data
LndLcatesthat the antenna gain calculated on the basis of the &&in
found experimentally for the alev'atLon of 81' will be close to
actual, at least for the came of higher elevations@ OrL&. art, hast
11 figures and I formuLa,
ASSOCIATIONS tkone
SUBHITTEDe 04H&r63 DATE ACQs 09Jun64 EMS 00
SUB CODE: 90 NO REP SOVI 004 OTHERS 002
3/3
TH.,
1--a- ui
L-11

AP
ACCESSION KR: AP4033119 510120164/000/OOZ/009610100
AUTHOR: Bruk, Yu. M.; Men'. A. V.; Bazelyan, L. L.
TITLE: Measuring the parameters of multiple-unit antennas
SOURCE: Pribory* i tekhnika eksperimenta. no. 2, 1964. 96-100
TOPIC TAGS: antenna, multiple unit antenna, electrically steerable multiple unit
1;' antenna, musao radioastronomic antenna, antenna parameter measurement,
muea parameter measurement
ABSTRACT, A method of measuring the parameters of a multiple-unit electri-
cally steerable antenna (musa) under operating conditions without Introducing
noticeable distortion into its circuit is considered. A low-loas measuring line is
connected between the output point being measured and the load (radiators), and
the values of loop and node voltages are noted. Then, a calibrated attenuator I
connected in place of the multipole being tested, and the attenuator is adjusted
until the same values of the loop and node voltages are attained. Simple formulas
Yield the values of the attenuation and efficiency of the antenna., the impedancee

ACCESSION NR: AP4033119
radiation power, currents, etc. , can also be measured by this method. The
errors ii-tivolved are theoretically assessed. The method was used in practice to
measure the efficiency of a IZ8-unit electrically ateerable radioastronornic
antenna described by L. L. Bazelyan, et al. (Elektroavyaz, 1964, no. 4). A
5Z-ohm multiprobe automatic measuring line was used. Estimated and measured
efficiency curves are shown for frequencies within 20-40 mc. "In conclusion, the
authors wish to thank P. A. Mel 'yanovskiy and V. V. Krymkin for their help in
carrying out the experiments. 11 Orig. art. has: 4 figures and 13 fornmlas,
-ASSOCIATION: Inatitut radlofiziM i elektronW AN UkrSSR (Institute of
-Radiophysics and Electronics) AN UkrSSR)
SUBMITTED: Z4May63 ATI) PRESS: 3076 ENCL: 00
jPUB CODE: EC NO REF SOV: 005 OTHER: OOZ
2/2

L
Pae-2/Pi_4
X(t) P
4 V
AFIST R/R AGIM a /S3D
B iQqFl ~jl t Zl JT ASD(a)
ACCESGION rip, - AP5000611 5/002'i-/6]i/oori/oli/1464/146-8
S. Ya. ("orrespondi g r, mber. All
n e
AUTHOR: Bazelvan. L. L
Braude,
UkrSSE
_y"
~!JjgXg., V V.; KMrqkin V A V.; ~L2din L
TITLE., R dio emission-a*
a pectral density-of a omen discrete sources at
r
equancies of 2o-4o MC
SOURCE:--- AN UkrRSR.--_-Dopqvidi, no.
11, 1964, 1464-1468
TOPIC TAGS; radi 6- astmno M radio telescope, radio emission
ABSTICRACT: Radiation-densities of eight discrete sources of cosmic-
radiation -in them 20-40-Me band were measur-Ed with a wide-band radios
telescope.- The measurements were carried out, from October 1963
through February 1:964,. The radio telescope"consisted of two electri-
cailly controlled multielement antenna, arrays (each With 128 radiators)
spaced 470 m apart along an E-W line.. The antennas formed~the elements
o a T-shaped -Interferometer F.,ystem. -The width of' the-radiation pat-.--.
tern --of -each :antenna,- was -4.611- --at -20--146 -and -2.3'_ at 40- Mc;- the- inter- -
-at th -
ference interval quencies- 'Was 1.80:and 0.90, respectively.
ese fre
7-
Phr-se-mo-d-ulated-,.radiome.ters- (i-f.--bandiridths,-.10--1-5-,-kc) -were-- used. for
Card
:0N

- - - -I ~' - - ' - ; "L ,- L.-- .- - - - - - -- - - . . -. 7 ~'.
: ,, , . -- " , ~ I " - I , , - - : : : . -'. - ~ *- ~ -- . L ' - ' ' ' L - 1 ' , _ _ . _ _. -_ - ". . . L_ ,
-' L-- - ~- -- - -~ -.. - -1 1-1 ~ ~:-, - - - , -- --7-
' L . i ! . - ~~' :: . L_ . - , .. . "L ___; , - ~ - = , ~ ~. ~~ -- ~ - , - - --

ACMSSICN UR: AP4039721 S/0141/64/007/00210215/022t4
AUIHOR: Bazelyang. L. L.-, Bruk, Yu. M.; Zhuk, I N. -, Henv 9 A. V. Sodin, L. G.
Shary*kin, N. K.
Tr=: Wide-band radiointerfarcmeter with eleatric control of antenna pattern
SCURM: IVUZ- Radiof itika, v. 7 . no. 2, 1'J64, 216-224
TDPIC TPM: antenna rediation pattern, antema switd-iing, ru&o astrmcm, radio
interferometer, radio emission
ABSTRAM A broadband (20 - 40 Mcs) radio interferometer with a (170 meter base,
oriented east and wP-stq is described. The interfercmeter is intended for the in-
vestigation of radio emission fran discrete sources and the cosmic background in
the northern hemisphere by directivity-pattern scanning in a + 900 elevation
sector and by using the earth's rotation. The interfei-ometer;'Iccnsists of 220
dipole plane arrays with ronote digital control of the directivity pattern in the
meridional plane. The description covers the principles underlying the control of
the bean and the awmition of the signalaq the arrmgwent of the antemaq the
control eleaents 9 the antenna dimetivity. pattern$ the antenna effective area# and
the wyWm. Vi3n. Ito large base fadlitates separation of the Boux .w radio
Card 1/4 J

ACCESSION UR: AP4039721
emission from the cosmic background. 1he two interferxmeter antennas are differ-
ent and can be used separately. Me eastern one can be used as a transit instru-
me-nt. By using the western antenna with bean scanning, it is possible to make two,
or three records of a source passing through the azimuthal pattern, with intervals
of 10 - 20 minutes. 7he resolution of the interference diapyam is 1. 6 - 0. 80 in
direct ascension and 40 - 20 in declination, at fiequencies 20 - 40 Mcs. It is
recamended that the antennas be used separately for the radio emission:of the
cosmic backgaund, in which case the resolution is 4 211 in ascension and 34
170 in decLimation for the eastern antennat and 34 170 in ascension and 4 20;
in decLirk-.ticn for the western antenna (both at 20 40 Some precautions
neoessary in the operation of the nter are mmticned. Orig, at. hast
9 figures and 2 tables.
ASSOCUTICK: Inftitut radiofiziki i elektrvdki AN UkrSSR (Institute of Radio-
physics and ElecUmnicaq M UcrSSR)
SUBH=.* MOO T Wi: 02
SLO COM-1 M9 EC NR REF SOW: 001 003
Card.----2/4_

AC(ZSSIO" N" AP4039721 RNCLMMIOI
1 2 3
12 3
Block diagram of the interferometer
1 - signal, 2 .,calibration, 3
control of directivity pattern
IIYBq UHF receiver
0 north
in
.10 sott4h
Card 3 4
az

ACCESSION 14R, AP4039721
mmosum 1 02
0
Western interferometer antenna
1 - dipole, 2 underground
collector, 3 junction for four
elementai 5 - quadrant switdhj
6 - b1nary switch cell, 7
phase Shifter
Card

BAMLYAN, L.L.; BRUK, Y-a.M.; ZFTj'K-, I.!'., MENI, A.V..
-
VIdeband hi,,"hly Airf-rticrall de-a7.eter wave arterina. Ziektro-
Ev~aal 18. no.5-zi-,-.~l My
I :7.-fl

BAZELYAN L.L.; BRAUDE, S.Ya. ; KRYMKIN, V.V.; A.V.; SODIN, L.G.
(SodinY L,H.] I I I -
Frequency spectm. of discrete sourcen in th-9 decaneter radio wave
band. Dop. AN UPSR no-5-.580-583 16 5.
(MIRA 18:5)
1. Institut radiofiziki i elektroniki AN I'krSSR. 2. rhlen-korres-
pondent AN UkrSSR (for Braudu)',.

4
Vi-
e4 I
523. 16 1-
AUTHOR, -Batelyan,
L. L. Braude, S. Ya. Ve-,vsb erg.,. V. V Krymkin, V. V.;
14en A. V_ _S~SL
'TITLE: Investigati-6n of the spectra of discrete cosmic radio emission zources at
f requdncies below ho me
!SOURCE: Astronomicheskiy zhurnal, V. h2, no. 3, 1965, 618-628
-TAC C
'TOPIC osmic radio emission, -radio emission Bouraej,-radiq,emission meas-
j
xement --Tadio~tele
scQpe--
ix T
-v:
-ABSIMACT - Th e spectra of 14 diterete.sour es.(in-the 20-4o-mc range) were 'n
t' gated at the Radio Astronomy Observatory of the Institute of Radio Physics
-from October
i and Electronics,'Academy of Sciences UkrSSR, 1963 through juiy 1964.
Al 1 obser"t-a-tions were made b tue, e n 2200 and 0800.hours local:time. 17h e radio tele'.~
Sao-,je 4mployed an. interferometer~.-and its antenna-system conaistad of - w eb
t 0 vid an
mulltielement -ele e
ctr1cally phased arrays, each in asuring -176 x 17 M and spaced
470 m, apart on- an east-west:1ine. Each array1consisted,of es i
.178 horizontal dipol
Pattern width was -40- for 20- Mc and- 20 _f6r 110 Mc, Lobe dth-of the interference
W!
Ccird

ACCESSION NI9. AP5015584
patt- n was "0 M d 0.80 for .40-M Peam declination along the meridian -
i-r 1.60 f*or..; C an C
rol delay. lines 711 e telescope radiometers were phase
was regulated
modulated by phase _cWting. the.signal.of one of.the antennas through 1800- at a
ifreauency of 6o cps. The signals of each antenna were amplified by hf preamplifiers.
The -Dassband of the pr6amplifiers and of the pnase shifter was about 20 Me. The
adjustable --passbands of-the--four--radiometers made-it-possible to--recoTd each sources
:.at-four-frequencies simultaneously (20 and 38 ; 5 M-0 - - The recordings
25,- 30-31
.1 were calibrat ed:with a standard-signal generator fed through a calibrated attenuator
mcla-g ppTft`tiEr-t o -the- 11 ripii-:Uf puts -4VL.1- t Ife -8 0- ur es--v-ere--iraasurecL-by= Cora-.--;
preamp - C
the stand d flu- e- 3c 461 tcas--k), ~ihlch at 20-Mc is
-,-paring.them with ar x -of soure
10-2-4 -,T/M2 cps Flux densities .10211 w/Me) and-th -rrors
450 X e mean-probable.e
-th
(A") for fourteen of~the sources.are listed in Table 3. of the Enclosure. On a
'b Sig,
wid previous measurements of Cas-K, nus-A,-Virgo-A, and Ta s-A,
asis of these uru
Ithe spectra of--18 -discrete -sources can be divided into-two classes:-_spectra with
a constant spectral index from 20 to'1400n- 3200-Mc (13 sources), and spectra with
a spectral index which is a function of the frequency (5 sources). Orig'. art. has:
-fi- -bs --and
-2 tables-
3. gur
Institut radiofiziki-i-elektroniki~Akademii nauk
ASSOCIATION UkrSSR (Institvte-
of Radio P of Science's
i rd*
4

OR
-is

-AM15584

13S
MTTED: ep64 SUB
ENCL: 01 CODE:,4.4 EC

110 REF,SOV: OMR: 015~ "D PM S: 4046

Card 3/4

AP5013621
o
Y _rCorresponelin
~AUTHOF41F 11 UILTSSR)
IL~z ~eY4 L X, r1u, I
_g member P
Ril:
& V-; Men A ~V Sodin, L.
T G_
15-
-decameter radio band'
e e, q u e n ey spectra of s am, discrete zources in the
SlOt RCE:' 1W UkrESR. Dopovidi -no. 5~ 1.965, %0-58.~~
TIDPir, - TIOS radio - a st ion r) e e e gplactic radl~!
rad1oA1_iecopej,.cosm1c radio soure
on
-radiation:flux of-six 1-
ATPS7 ACT. The zestOft-s are p1resented of meamirements of the,
Urr-ea In the
20-40 Mcs band. nl~ e measurements were obtained at the
'U'dastrondmical ob.-ervatory of' T
Institute-of
radiofiz:i~d i eleldroniki
V-sics and Blec-tronics) Pal
using a T-'Like band teldEpqr.)e operating
a ~a merl.Oovial '21,1e te encrive -mark described in detail earlier (Izv.
v..7, 215, 1964). The-ineasurements were-compared with the flux
Casssioppa-A iibieh -~ms chosen as the.-standard., The spectra are found to be
nc
~36if46d as bein
L - he
ar in -the _vhole frequency i~lanqe and can-1hus be C1 _g of-t
-Aped-ra). t~. a that flia noureen. t tic Co-
li it- I by he plac
ordimttes zil'