SCIENTIFIC ABSTRACT BAYMURADOV, K.Y. - BAYRACHENKO, I. V.

• Document Type: CREST
• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R000204030007-5
• Release Decision: RIF
• Original Classification: S
• Document Page Count: 100
• Document Creation Date: November 2, 2016
• Document Release Date: June 6, 2000
• Sequence Number: 7
• Publication Date: December 31, 1967
• Content Type: SCIENCEAB

BATKMTOV. I.Tu.,izLzh.
..... ._'r
Investigating t'he components of the SM20-102
cotton-picking
machine with horixontal, spindles. Trakt. I
sellkhosmash. no.2:
19-22 7 159. (KM 12:1)
L Sredneaziatskly nauchno-tooledovatellskiy institut
nekhanizatBU
i elektrifikatuil, orosheyonogo senledeli5a.
(Cotton-picking machines

k-wrid. ve'lorinarnvkh nauk; FOLFTSKIY, V.A,, kand. l---clogJche9Ukh
nauk; BAYMURADOV T.B., aspirant
rrophylaxis and diagnosis of ehronical IntoxIcatione in
animals. Veterinarlia 42 no.503-76 My 165. (M:EPk 18s6)
I. Vaesoy-mmyy institut eksper'-mentallnoy vet,erlnarl~.

DIKLE3MCK, T.V.; GMRA, M.; BAYMRiTOY, U.
Utilizing waste products in Kazakhstan nonferrous
metallurgy.
Izv.AN Kazakh.SSR.Ser.okon.. filos.i prava
no.2:42-51 159.
(NM 13:4)
(Kasaidistan-Zonferrous metallurgy)
(waste products)

RACHKOVSKIY, S.Yae; BAMJ~ATOY'I,P.B..
Review of NS* Satybaldints book wSconomic efficiency of new
technolog#al processes in ferromm mtalhlr9Y*m TSvetp moto
'T I
36 no*6:94-t-96 Je $63, 1 (MIU 16t7)
(Nonferrous metals-449ta.3-lurgy)

L.B.; FIAGITOWAlY, --'.Ya.
Considoring tho tino of constrizcticn in comlzring
caj,dtal investment
variantu. lzv. vys. uchob. ZLLV.; tovet. met. 6
no.3:157-164 163.
(i.aik 16:9)
I.Moskovskdy institut sta-li i splavov, kafe6ra
ekono..u*ki i organizatsii
proizvocIstva.
(Capital inve:Amonts) (Metallureical, plants)

BJIIMIURATOIV~ U.B.
Enon,imic efft,~tjveness of raaqAr,!z.!ng- oopper
xMisIt.jng plants.
TSvet. met. 37 n:~.72vU-18 D 19,4 (MI RA n S2)

UaBsp kande ekonoss nauk
M~nvs
Determining the offeativeness of reorganisation.sM
Anlersemant Of
enterprises. Vogt. IN Kas&A, SSR 21 no.9s27-34 S '65s -
(KMA 18 s 9)

*.- BALYMMTOVA, G.
Materials on the flora of parasitic fungi on the Golodnaya Ste
Uzb. biol. zhur. no.3:&15 161. Z7*
(K= 14:6
1. Institut botaniki AN UzSSR.
(OOLODNAYA STIPPZ-X=I, PHYTOPATHOGENIC)

GOVERDOVSKkYA, A.Ya.; ~~~ ~VAQ~ KOTLYARSKkYA, A.Z.
Course of pneurmonia in cb:Udren under one year of a eZdrav,
Kazakb. 22 no.309-42 162. flk 15:12)
1. Iz kafedry detakikh bolezney falaillteta
usovershenstvovaniya
vrachey (zav. - dotsent A.Ya.Goverdovskava) NazaMakogo
maditainakogo Inatituta. (PNEUNDNIA)

BAM4URATOVAS G. T.
M~wflora of the GDlodnaya Steppe* Yopebioli kraev.medo,
noo3l
27-31 162. (GOLOISAYA STM7&-,YUNGI) (KM 160)

BAYNAKOV III.
Big etep ~rj the ~;roat.Aon of the material and
teviinical basis of
co=un."sin. Homm. Voo-ruzh. Sil 4 rio.4-8-.16 F .
17:9)
1. Rinistr SWR.

ZIIUEOV, Pavel Kona tantinovich; KAZANIN, Yurly
Ivanovich; KAYUPOV,
Aryktay Kayupovicb; 14URSALII.-,OV, Khakim
Ibragirovich;
PIGUlJ;',VSKIY, Rikolay ArBenlyevich; SHLYGIN,
Artem
Yevgenlyeviah. Prinima3i uchastiye: BAIKENEV,
Sh.A.;
0.1 r
*1 "-RIN, Ye.S.; KRIKTYIGVA, II.P.; SHUYJiOV,
4allftl-I
.U.; OX, Ij. Ik
J* akadeir, , otv. red.; IIESTEROVA, I.I.,
red.; ALFMOVA, P.F.0 tekhn. red.
[Basic features of the geology and r~etallogeriy
of the Koksu-
Tokeli area of the Dzungarian Ala-Tau]Osnovnyo
cherty geolo-
gii i v.etallogenil Kokou-Tekoliiskogo raiona
Dzhurgarskogo,
A:Latau,, Alma-Ata, Izd-vo Akad. nat& Kazakhskoi
SSR, 1962.
123 p. MIRA 15: 11)
1. Institut geologichaskikh nauk (for Zhukov,
Kazanin,
Kapipov, Pigulovskiy, Shlyginin). 2.
Yuzhno-kazakbstansku-;e
goologichaskoye upravlaniye (for Fursalirov) - 3.
Alkaderiy~
nauk E-,zakhskoy SSR (for Rok).
(Dzungarian Ala-Tau-Geology, Econoradc)

I I
All
42 .3
fur
fig
i A i i i i d d i d i i i i

v %I
BAM.-FRG,,
"The Existence of Solutions in One System of Non-Linear
Integral
Equations, It Dok AN 63, No. 6, 1948

L I
C T-T Y
!
Py
: CULTIVATED FJ'ANTS. Po"atoog'
Vef~etables'_

Cucurbits.

A L3 CUIR .
V,-,J 5653
tH ; HLIF. - EACLCGIYA, NO. 4. 1959,
AV ~F' 0 'R

ObtaininS a Harvest from Sprouting Potatoes.

"emledeliye i zhivotnrvodstvo L!oldnvil,
1957,

N10 - 5, 70-71

The out-growth of tubers of
average and late

varieties of potatoes Is observed In
the

southern districts of Moldavia, and

In hot and
humid years also in the middle zorel

of the republic.
Experiments conducted

In irrigated plots, showed the
posalbill"Y of

using out-growing tubers with sprouts
for

s,immer plantings and.gettIng crops reaching

22
tons/hectare.
CA D
61

HAYNBAT, D. I.
Avtomaticheskaia i poluavtomatiche-
skaia svarka pod fliusom (Automatic and semi-
automatic welding under flux). Leningrad,
Sudprom-
giz, 1952. 243 P.
W: Monthly List of Russian Accessions, vol. 6,
?b. -1, April 1953

!.4% il '. . ".
"*hriiFh as a Cause of -1- t-l-ildr-n".
. Ftnil- vereroloc, i i dermatolo~ii -
"I p i /Tulletin of Venerolog;, "-er;7,atolo-
- !,-.7
Januar--lebrunn., 1951: (b 'T, i 1-1
:!0 1$ i o7T.- r '.'osco-r.

BAYNDUROV, V.S., lnzh.;TOPORSKIY, VA., inzho;
TKACHENKO, L.A., lnzh.
Pulley with a built-in planetary reducing gear.
Izvo vys.
uchabezave; mashinostre noolOtlO4-106 164 , (MIRA
18:1)
1. Kharlkovskiyinthenerno-akenomichaskiy institut i
Kharl-
kovskiy mashinostroi-tolInyy zavod "Krannyy
Cktyabr'".

POW I WK Inumwm OW"".
Z-OMMkV fift IAWUftt W4md*A*jA .4
1-244-wis " alektrobbb" -am lostv"m I nspiel" I
G'a.pwr
%&U-rgU 00 RSWUOOVAWIY Of Yaw solatIfte,
h010- --U-0) Ab..At4, IMI-w As Do. W, Me. In
ML3 T*V, AU1,,IV04" %*. OLI _FeUW gk%mt#a Umt at
awleal
1.1 MboUg I OAS
K.T: O.L m..p. ft.),
Ly. ==!`Gaw
lpwm, ra" bak is "tu" a- saftul" "I "U"m so us
ftd alorwoo" wk" Imsota'.
MMWI 'me "Usauft -ta- m -mu 1w as - a b, a rw
A003YUS&2
'046"7 -14 0-troftd"- ate*A to M. l.Uteds sc an""
adum
" 6" 4c saimm, mndholis MFU146 aw Mau" ago" or
::~= 0
UMUIM frm is" PrAw %e
ib. elerue3r- at swe" sobmfto
&US ft" Ad*Al poh.Uft gm gn
2"*4"ly ot '"4" um 6 rum-, aft" ma fta glib
Gw:dv"u4 am
awk-rarow wbou.
fts
Aftmftw~n ~ w so
Amb-.6"ALING, ago" am -
aft "*am
Tv
vdmdftr,c:~;v NAGA. W-SWIM. M-w-wedum 4c ftham
amew U~ at Rkp am"* N~due, . ft
arwoubm. '-&b-d ON" #ANN
ft. 16 ftdfJ6=r-~
ft" mks at mad 1w
us no ft" 1.
&a WIG 046 Ur
4c vw" was"
AMM of Pam& Gaftp u1
ftn MON6
AftnAEft W--,
"ANN

ZIRIYAKOV. G.2.; BAYNIYBTOVA, M.
Xffset Of the impurities of some metal ions on the
cathode
processes during the electroly*is of zinc Sulfate at
high current
densities. Trudy lust. khim. wak AN Kazakh. SSR
3:64-n 158.
kHMA 12:3)
(Zinc sulfate) (1106trolysis)

KIRITAKOV, G.Z.; BATNITNTOVA, Y.K.; TAMIDOV, R.S.
Iffect of manganese on the alectrodepositAon of zinc.
Trudy Inst.
khim. nauk AN Kazakh. SSR 3-~2-81 158. (MIRA 12:3)
(Zino) (Blectroplating) kMangausee)

KIR I UKOV v G. Z. ; -DARM
Electrolysis of sulfate ablutions of zinc. Trudy
Inst*khim.nauk
AN Kazakh.SSR 6s"3 160. (M;Rk 14:4)
(Zinc-.Meotrometallurgy)

BAYNIYETOVAt F K- KIRIYAKOV, G.Z.
I------
Simultaneous discharge of zinc and bydrogen ions in
sulfuric acid
solutions. Zbur.pr*l.kbim- 35 no.4%903-905 Ap 162.
(HM 15:4)
(Zinc) (Sulfuric acid) (Electromotive force)

BUNWHE, VA.; KIRIYAY07i, G,7.; DAY111YETOVA, F.K.
Effect of titanium sulfate on the electrodeposition of ziic
from sulfate solutions. Trudy Inst. kbim. nauk AN Kazakh.SSR
12:18-25 164. (141RA 18:2)

,ACC NRa AP7002827 SOURCE CODE: Uj 009
/006/0714/0718
AUTHORt Boyanov, Y. D.; Baynov, D. D.1 Marinoy, Yu* P.; Partinova,
N. A.
ORG: none
TITLE: Theory of transistorized LC-oscillators having n oscillatory
circuits
SOURCE: IM Radiotekhnika, v. 9, no. 6, 1966, 714-718
TOPIC TAGS: oloctronic oscillator, transiatorized oscillator,
ABSTRACT: A theory is set forth of an n-circuit transistor.-
ized oscillator that has inductive feedback and is
excited by external harmonic voltage (see figure). The
transistor is connected in a co=on-base circuit, and
the coupled oscillatory circuitsare connected to its'
collector. Operation of this oscillator is described by
differential equations, examination of whose solutions
yields this condition of awjVtotic stability:
2bm + 2V, + dmE3 < 0,
1, 2, - n).

1-ACC NRiAP7002827
.in the general (nonresonance) case. In the notation of the
article, the above
condition means that# in order to ensure stable oscillations, the
oscillatoT7-circuit
.parameters an'd the oscillator operating regime should be so
proportioned that rk is
Ivery small and P. and b. negative; transistor voltage gain, p -
po.+ aU, + 6U,2.
jPwther examination shows.that the same stability condition holds
true for
,resormce case* Orig, art. has: I figure and 25 formulas.
CODE: 09 / SUBM D&TE: OINov65 / CRM REP: 003 / OTH REFs 001

154
AUTHOR: eaynov, D. D., Marinov, Yu. P. * Stanev, Kh. 1.

D

ORG: none

TITLE: Theory of some multicircuit negative -resistance

R.

LC-oscillators

SOURCE: Polska akademia nauk. Bulletin. Soria des

A siriff

A

sciences techniques, v. 13, no. 9. 1965, 151-154

TOPIC TAGS:
electronic oscillator, oscillator theory

ivillf 0'

ABSTRACT: Conditions of e3datence of stable self-

oscillations in a multicircuit oscillator (see figure) to

which an
external sinusoidal voltage is applied are

considered. The
nonlinear negative resistance is denoted

by R = 1/G. Operation of
the oscillator is described by a

system of differential equations. The equations are solved

so

for a
particular case when the external frequency is equal

to one of the
oscillator natural frequencies. The periodic

solution yields these
relations:
Aj-aw~A. where A. is a real root; and

4

--L 06158-67-
ACC NRs
3S1 42_a H /
j--~ --,/ , ~j. )IV, I -
1. . - i - I;

I Ali
j74 i A i A i I I I i i f i i
Liz
to,-

15(2)
AUTHORs Baynton, P. SOV/72-59-6-18/18
TITLE: Semiconductive Properties of Some Kinds of Vanadate
Glass.
(Poluprovodnikovyye evoyetva nekotorykh vanadatnykh stakal)
PnIODICALs Steklo i keramikat 19599 Nr 6p P 48 (USSR)
ABSTRACTs This is the translation of an article from the
English which
was published in the periodical Blectrochem. Soo. (USA), Nr 4,
1958P pp 237-240. The names of the translator and the
abstracter
are not given.
Card 1/1
UMMM-DC41,2.17

i
MMITAKOV, G.Z.; BATONITE.TQVA. F.Ko,
Simultaneous formation of hydrogen and gLuc on binary
cathodes in
the presence of some surface active substances. Izv.
AN Xazakh.
SSR. Ser.khim. n0.1:19-22 158. (MIRA 12:2)
(Hydrogen) (zinc) (Surface-active agents)

BAYCR, B. N.
Analyzing the effect of dullness and wear of the grinding wheel
an the
fluctuations of metal removal in internal grinding. [Trudy]
Inst. mash.,
STW no.18:61-68 164. (MIRA 1834)

SVIRIDA V.G., rukcvo~Jtall raboty; KLYACHKINA, Ye.L.; ZARUBKINA, A.K.;
BAYTINA, N.M.; LYUBOSHITS, A.I.j V13HREV5KIr, L.L.; SHOLCKYANSKITT,
Teja.) BAYCVA, M.P.
Rxperiment in increasing the productive capacity of the Minsk !Actlc
Acid Factory under the conditions of existing equipment and electric
power systems. Trudy BNIIPPT no.063-66 16i, (MW 17:10)

BAYOW, Z.t kand.takhn.nauk; LOPUKHINA, YeMo,,
kand,takhn.nauk
",-.
Shunt rwoning of aaynchronous micrmotors.
Elektrotakhnika
36 no,3.137-9 N 165o
(MIRA 18i11)

L 3295-66'__n~~-7~?/~;g(i)/
ACCESSION NR: AT5024189 UR/0000/65/000/000/0057/006i--I~
AUTHORt Fialko. Yo. I.; BjMXIShenko, 1. V.-, Chumak, Yu. V.;
&y-qM.R. I.;
Mallnik, V.- 1.
TITLE: Statistical characteristics of meteor.radio echoes during
the 1963 Geminid
shower
SOURCE: AN UkrSSR. Pizika komet i meteorov (Physics of comets and
meteors).
Kiev, Izd-vo Naukova dumka, 1965, 57-64
TOPIC TAGS: radio echo, meteor tral , reflected signal, radar echo,
radar meteoL-
obsezvation
ABSTRACT: Statistical characteristics of meteor radio echoes during
the 1963
Geninid shower were studied experimentally. The radar equipment
used had the
following parameters: A - 9.59 and 6.49 a; power, 20 kev; prf, 500
pps; and
pulse duration, 10 usec. 16 all, 198-207 meteor radio edres were
used to
determinethe distribution of radio edves with'respect to duration,
amplitude,
time interval between echoes, and distance, on the basis of the
results obtained
the following conclusions were reached, 1) Distributions of meteor
radio echoes
with respect to duration at A 9.59 s and A - 6.49 a are practicall"
identical
LCqrd 11~2

L
ACIN NR: AT5024189
in the region of long durations M see) and differ slightly in the
region of
short durations. 2) In the distribution of amplitudes, three groups
of reflection@
are distinguished - stable, intermediate, and unstable. The
distribution of ~
interma&ate radio echms is similar to~ that of stable reflections.
3) Distribution
reflections has an exponential character*
of intervals between appearances of meteor
Orig. art. hast 4 figures- 4p~d 5 formulas. (JR)1
ASSOCIATION; none 7
SWITTED: 2P!ey65 ENCU 00 SUB cobs:
NO IMF SOVi 003 OTHER% 002 ATD PRESS

L- 3291-66 FWT(j)/Frc/wA(d)/&A (h) i~Aw
ACCESSION NR: AT5024190 UR/0000165/000/ODO/0065/0067
AUTHOR: Fialko, Ye. I BfIrschenko.-I. y;; chuntak, Yu. V.
55'
TITLE: Some results of the utilization of intermediate-type trails
for measuring
the electrowdensi of a~mete r trail.
SOURCE; AN UkrSSR. Fizika komet I meteorov (Physics of comets and
meteors).
Kiev, Jzd-vo Naukova dumka, 1965, 65-67
TOPIC TAGS: meteor trail, radar meteor observation, radio echo,
electron density#
mathematic method
ABSTRAM Linear electron density a of ionized meteor trails was
determined from
radar observations of intermediate-type trails at X - 9.59 m. The
observations
were, conducted by Kiev State University In 1963. The method is based
on the
dependence of intermediate-type radio echoes on.a. The distribution
of a was
of 1012 to 5 x 1012
determined within the range el/cm. Distribution of inter-
mediate-type trails according to a is shown.in Fig. I of Enclosure,
where n
is the number of trails in-which electron density a exceeded a given
value. Orig.i
art. has: 1 figure and I ormula, JKN]
ASSOCIATION*. none

-L -3291-66----
.ACMSSION NR: AT5024190
SUBMITTED: 2IHay65 ENCL; 01 SUB CODE;-A~Ec
NO REF SOV: 002 ::OTHER: 001 ATD PRESS

BATRAGEMMO, I.T.;MIZXU=. A.T.;VSXMSTUTSUTA,
Yu.S.;SHKURDOTIL, V,Y,
Radar observations or meteoric activitr in JamuLry-Narch
1958.
3W. Ion. po kowt I meteor. Ali SSSR no.3:15-18 158 OM
13:3)
1. llyevskty gosudaretysmqy Institut.
(meteors)

BkrRACHEKO,, LV.; gSEKHSMTSK&Ykp I.S,; MIZERNYUK, A.T.; SHKURDODkq
V.F.
Some remato of radar observations of meteor activity. Hezhftna
geofis. god [Kielj no.205-79 160#. (Min .14:1)
1. Kiyev State University.
(meteors) (Raw %in astronomr)

h1273
A/035/62./boo/olo/b19/128
A0O11A1O1
AUTHORS: Kruchinenko, V. G., Moysya, R. I., Bayra!~
TITLE: Radar observations of meteor streams
PERIODICAL: Referativnyy zburnal,.Aatronomiya i Ge6deziya, no. 10,
1962, 41-42,.
abstract 1OA307 ("Sb. ral?ot po Mezhdunar. geofiz. godu. Kiyevsk.
un-t", ig6i, no. 1, 26 - 36)
TEXT: The Kiyev University conducted radar measurements of meteor
numbers
on the 4-m wavelength from January 1, 1958, to December 1, 1959.
33, 670 meteors
wgre recorded during 6,490 hours of observations. Equipment
characteristics are
a4k follows: emitter's pulse power, 80 kw; pulse duration, 8 psec;
frequency of
Ou~se repetition, 50 epii-receiver sensitivity, 10*pv. The
nine-element antenna
of1the "wave channel? tyie at a height of 7 m over the ground
surface is orient-
ed-in east-west direbtion. Refleated'signals were photorecorded on
a film whose
mqyement speed was 90 mm per hour. For each meteor were determined
the time of
appearance, distance and duration of reflection V. During the
period of active
Oteor streams, mass (m) distribution of meteoric bodies was
obtained. The
~~rd 1/2

S/035/6P-/000/010/019/128
Radar observations of meteor streams A001/A101
The relationCm Aml-15 Is assumed, where A Is a function of
meteor velocity v.
The differential mass distribution of meteoric bodies is
described by the re-
lation: N-m-s. The following dependence of meteor
luminosity I on m, v and ze-
nith distance of the radiant zR is adopted: I-mv3cosz, as
well as the scale of
masses in which a +2m,86 meteor is originated by a
meteoric body with m-l g,
v-10 km/see and zR-0. A +2T4 meteor corresponds to
duratlonV= 1 see. In the
GeminJdstream, parameter s varies systematically during
the visibility of the
stream., The values: 2,5; 2.2; 2.0; 1.7; 1.4 and 1.8 are
obtained for the suo-
cessive nights of December 9 - 15. For the Arietid stream,
the bLverage value
of s - 2.23. In the Perseld stream of 1958 the s-value
changes from 1.83 on
August 6 - 8 to 1.65 on August 11 - 14. In the 1958
OrIonid stream s - 1.8D,
and in the 1958 Quadrantid stream s . 1.72. There are 8
references..
V. Lebedinets
(Abstracterts note: Complete translation]
Card 2/2
I

S/16 62/000/005/067/093
D228YD307
AUTIHMS: rachenko, I. V., Mizernyuk, A. T., and Moysya,R. 1.
TITLE. Some results of meteor observation by the radar method
Ra.ferativnyy zhurnal, Geofizika, no. 5, 1962, 5, ab-
stract 5G36 (Visnyk Kyyvsk. un-tu, 1960 (1961), no. 3,
ser. astr~on. fiz. ta khimii, vyp. 2, 47-54)
TEXT: Some results of radar observations of meteors, fulfilled
according to the 1GY program, are given. The observations were
made
January 1958 to August 1959; during 5000 hrs of work 28,000
reflections from meteor trails were recorded. The annual
variation
4n "ne number of meteors is cited. The meteor activity maximum
a is in the summer and autumn months. The average ho *urly
number of
=eteors in the summer months of 1959 was somewhat less than in
the
analo-,ous period of 1958. The range distr-lbution of
radio-echoes
leads to the conclusion that it is necessary to take into account
the lobing of the antenna directivity pattern when interpreting
the
-results. The lobing of the antenna directivity pattern explains
the,
Card 1/2

3/169/62/000/005/067/093
Some results of meteor D228/D307
presence of several maxima in certain flows, though the daytime
maximum of the Perseids appears to be due to the structure of
the
flow itself. The distribulions of the hourly numbers were
construc-
ted _-4"orothe -Irietid (June 8, 1958), Perseid (August 12,
1958 an4 -
1959), rionid.(October 23, 1958), and Quadrantid (Jgnuary 2 and
4,
1959) flows. The parameter, characterizing the mass distribution
of -meteor bodies, was calculated for the Arietid, Perseid, and
Ge-
.-inid -L-'Iows and for sporadic meteors. The results'of the
calcula-
-ujions a,,ree well with data obtained by Soviet and foreign
authors.
The dis-zrIbu-'Uion of the time intervals between adjacent
radio-
echoes was investigated; this allowed the hypothesis about the
ex-
istence of the space grouping of meteors to be verified. The ex-
Der.Lment's result shows that.there is no space grouping of
meteors,
Oelongincr to meteorite flows. Abstracter's note: Complete
trans-
la-zion.Y
Card 2/2

S/169/62/000/005/068/093
D228/D307
AUTHORS: ,,.ruchinenko, V. G., Moysya, R. I. and Bayrachenko,ia.
T'ZTLB: Radar observations of meteor flows
PBRIODICAL: Referativnyy zhurnal, Geofizika, no. 5,1962, 5, ab-
stract 5G37 (Sb. rabot po Mezhdunar. geofiz. godu,
Kiyevsk, un-t, no. 1, 1961, 26-36)
TEXT: Observations were made in accordance with the program of the
TGY and -che IGC near ~h e city of Kiyev. The results of the obser-
vations are given together with~the method by which they were pro-
cessed. / Abstracter's bote: Comple.te translation--7
Card 1/1

41275
S/035/62/000/010/OZZ/128
AOOl/A1Ol
AUTHORS: Bayrachenko, I. V., Moysya, R. I.,
A radar installation at 8-m wavelength band for meteor studies
PERIODICAL: Referativnyy zhurnal, Astronomiya I Oeodeziya, no.
10, 1962, 43,
abstract 1OA312 ("Sb. rabot po Mezhdunar. geofiz. godu.Kiyevsk.
un-t", ig6i, no. 1, 44 - 48)
TEXT: The authors describe a radar installation intended for
meteor
studies. Advantages of conducting Investigations at 6 - 10 m
wavelengths
are pointed out. A block-diagram of the emitter operating on R
-1 (GI-1)
tubes Is presented. The technical characteristics of the
emitter are as
follows:X-8 m; frequency of pulses, 50 cps; pulae'power, 60 kw,
pulse du-
ration, 1OAaec. Two antennas are used when the installation is
operating:
the emitting one - a semi-wave vibrator,"and the receiving one
- a vibrator
.with a reflector. The receiver is of a superheterodyne type
with double fre-
quency change. The schematic diagram of an indicator device for
recording
reflections from meteors is presented. Suppression of pulse
noises is pro-
vided in'the recording system (RZhAstr, 1959, no. 4,,2798) and
registration
Card 1/2

K radar Installation at...
3/035,/62/000/010/022/128
A001/A101
of reflection from one meteor In the form of two brightness marks
(RzhAstr, 1959,
no. 3, 1955). The authors propose a calibrating scheme using
durations of re-
corded reflections from meteors.
B. K.
[Abstracter's note: Complete translation]
Card 2/2
I

U96o
S/194/62/000/009/079/100
D413/D308
AUTHORS: Bayrachenko, I. V. and Podgorodetskiy, Ye. D.
TITLE: Equipment for experimental investigation of the' soat-
tering-of radio waves-by meteor trails
PERIODICAL: Referativnyy zhurnal, Avtomatika i,,radioelektronika,
no* 91 1962, abstract 9-7-54 te-'(Sb. rabot po Mezhdu-
nar. geofiz. godu, Kiyevsk.-un-t, no. 1, 1961,~49-51)
TEXT: Indicating and recording equipment has been developed for
in-
vestigating the scattering of radio waves.by.*meteor trails. The
design of the equipment provides for simultaneous observation on
31, 36, 72 and 213 Mc/s. It removes errord in the film transport
mechanism by a mechanical relay, and projects the screens of a.11
the CRT's and a clock onto a single film. 5 references. CAbstrac-
ter's note: Complete tran8lation.j
Cdrd 1/1

43286
5/831/62/000/008/007/016
E032/E114
AUTHORS: Nizernyuk, A.T., Shkurdoda, V.F.0
and Moyhyat RaIe
TITLE: Radar observations of meteoric activity at Kiev
SOURCE: Ionoafernyye isaledovaniya (meieory). Sbornik statey
no.8. V razdel programmy MGG (ionoafera). Mezhduved.
geofiz. kom. AN SSSR. Moscow, Izd-vo AN SSSRS 1962,
51-55
TEXT: These observations were carried out at the observation
station of the Kiyevskiy gosudarstvennyy universitet (Kiev
State
University) in the village of Tripol'ye in accordance with the
1GY
programme (carrier frequency 72.4 Mc/sec,-repetition frequency
50 cps, power per pulse 80 kW). A niiie-element, Yagi antenna .
was employed. The beamwidth at half-power points was 40'. The
reflections were recorded on a moving film and radio echoes
from
oblique ranges of up to 500 km could be recorded. Special
measures were taken to suppress atmospheric and industrial
interference. An attachment developed by the Khartkovskiy
politekhnicheakiy institut (Kharikov Polytechnical IrLatitute)
was
Card 1/2

S/831/62/000/006/OC7/016
Radar observations of meteoric ... E032/E114
used for this purpose and was based on the fact that the radar Y
pulses were inuch longer than the interference pulses, so that the
noise frequency spectrum was much broader. In the receiver, one
channel was tuned to the carrier frequency of the transmitter and
the*other was detuned for this frequency. Thus, the first channel
output included both signal and noise, while the second channel
output consisted of noise only. The useful signal was separated
out by means of a coincidence circuit. The meteor activity was
investigated during the second half of 1957 and during 1958.
More than 20 000 radio echoes were recorded in 3800 hours, and a
calendar of the observations is reproduced.
There is I table.
Card 2/2

BAYRAC[IFNKO I.V.
Resonance effects in radio wave
their models. Geomag. i aer.
scattering on meteor a and
4 no.2013-320 Mr-Ap,, 064.
.-HIRk 17:4)
1~11
W
1. Kiyovskiy gosudarstvennyy universitat.

ACCESSION NR: AT4034464 S/3091/63/000/002/0040/0055
AUTHOR: Moysya, R. I.; Kruchinenko, V. G4 Dayrachenko, Is V.
TITLE: Influence of the directional diagram of an antenna on
the observed mass
distribution of meteors
SOURICE: Klyev. Universitet. Sbornlk rabot po Mezhdunarodnomu
geofizicheskomu godu,
'2, 1963, 40-55
no.
TOPIC TAGS: astronomy, meteor astronomy, meteor, antenna
directionai'diagram,
meteor trail, meteor mass distribution
ABSTRACT: There are several methods for determining the
exponents In the mass
distribution law for meteors when using data from radar
observations. one of the
most common methods is based on the measured distribution of
the duration of radio-
meteors. The derived theoretical expressions are correct only
for the case of
reception of signals from a narrow sector of the directional
diagram. in a real
case reception always-is from the entire region of the diagram
and the amplifica-
tion factor of the antenpa change3 as a function of direction.
in this article
the authors attempt to take Into account the Influence of the
antenna directional
diagram In the vertical plane on the results of radar meteor
observations. The
artif)2 begins with a discussion of certain problem In the
theory of scattering
Card

ACCESSION NR: AT4034464
of radio waves on meteor trails and the method for selecting
the range of a ctron
i densities and masses; this entire section Is based almost
entirely on non-SLelet
published sources. The authors present the derivation of the
principal relations
required for solution of theproblem and discuss the method for
processing data.
Solution of the problem.required the Introduction of many
simplifying assumptions.
The problem Is limited to the Influence of the antenna
directional diagram In the
vertical plane; the similar problem for the horizonpal plans
will be considered In
a separate article. A final expression Is obtalne4 for the
Integral law of mass
distribution of the recorded meteors with the Influpnee of the
directional diagram.
taken into account. The problem also Involved a comparison for
different antennas,
differing from one another In the form and degree of
directivity. it was found
that the distribution of meteor bodies by mass differs when
the influence of the
directional diagram Is taken Into account from the
distribution law actually ex-
isting In space. The difference Is particularly well-expressed
In the region of
small masses. The Influence of the form of the directional
diagram Isrelatively
small; this Influence also Is expressed most clearly In the
region of small Masses!
Orig. art. has: 60 formulas. 12 figures and I table.
ASSOCIATION: Kiyevskly universitat (Kiev University)
SUBMITTED: 00 DATE ACQ: 07May64 ENCL: 00
Card 2/2 SUB CODE: AA N REF SOV: 004 OTHER: 007

ACCUSIM Na: AT4032228 - S/3099/63/000/005/02"/0297
AUMR1-KMhi84Sko, V. 0.1 ftylyaq 1. 1.;
TIM: Detumination of the true number of meteors using radar
obsorwatida data
SOUM: AN Vkr5SR. i4sshduw*domstv*=y*y geofistchasAy kmLt*t.
~wfizika I
astrosomiya; informatsiouny*y byulleten, no. 5, 1963, 293-297
TOPIC TACS: meteor, meteor astronomy, astronomy, radar, antegma
directional
diagram, upper atmosphere, radio meteor
ABSTRACT: In processing the radar observations of meteor activity
it is necessary
to couvert properly from the observed number of radar echoes to
the true number
of meteors for a certain sector of the sky. In this process It is
necessary to
take into account the influence of the three-dimensional form of
the dLrectional
diagram of the radar antenna. In this paper the author cites the
principal
formulas used in connection with radar observations of meteors
and derives a
general expression for the integral distribution of meteor bodies
by masses vitb
allowance for the influence of the directional diagram. The
necessary formulas
are cited for conversion from the observed to the true number of
radio meteors.
i On the basis of the cited formulang and with certain
simplifying assumptions, It
1/2

ACCUSION NR: AT403,2228
is possible to determine the total Locrewent of the earth's uses
during a year
from the falling of,usteor natter. The derived annual value is
approximately
1,120 metric tons. Orig. art. hai: 22 forsulas and I figure.
ASSOCIAnON: AstroamIaMakaja abservatoriya liyevskogo lpsudaretvamogo
=IveraLtsta (Astrosonica,l Observatory, Kiev Stata University)
SUMUTND: 00 DATS ACQs IGApr64 MM: 00
XVi 009t A& AD RW WWt 006 OTEM. 001
2/2

ACC-NRi-AR6019485 SOURCE CODES WQW6W00O WW5760
AUTHORs Bayrachen)w, Is Ve
TITIEs Nature of the radio eabo from the head of a mateoir
SDUAGEs Rafe abe AatroDoniyaj Abee, 2*519581
REF SOURG&I VLWWk KyyiVelke 1M-`tUg Sorg astronog...no. 6, 196 4#
92Jn
TOPIC TAGSs meteor observation,, radio echoj, meteorArail.
ABSM1ACTt Various theories on the radio echo from a meteor headare
discupsods The
Braun-Kayser diffraction theory does not explain the phenomena
observed because the
authors applied it to unnaturated. meteor trailsp whereas the
echoes were observed most
often during the scattering of radio waves on saturated meteor
trails. The Cook and
Backin3 theory.. which is based on the YkKinloy and M13lmgkn
hypothesis on the Ultra-
violet radiation of a meteor as the source of ionization in the
front of the meteoric
body, vas not confirmed experimentally and cannot explain the
short-livad-character
of the radio echo echo from the meteor head@ A qualitative
explanation is given of the
nature of the radio echo from a meteor head. It is based on the
conventional theory
of the formation and disintegration of ionised meteor trails. It
was shown that the
following is necessary for the formation of the schot (1) the
formation of a trail'at
an altitude of-100 ka, which ooomra In fast meteoric bodlesp (2) a
large radiant
UDCs

AGGWSION NRI APW31636 8/0203/64/004/002/0313/Q320
AUTHOR I ~Bqr
-V-
MUM Resonance phenomena during scattering of radio waveal at meteor
trails and
their models
SOURCEs Geomagnstism i a=noidyas ve 4, nos 2. 1964, 313-320
ITOPIG TAGSt radio wave scattering., meteor trail., resonance
scattering,, plasma
'resonance
s gas discharge tubes dielectric constant
-ABSTRACTi The author has used a cylindrical gas-discharge tube as
a model ofa
!meteor trail, The length and cross section were chosen in keeping
with the range
of waves considered in the model experiments' To obtain the
necessary concentration*
of charged particless it proved most convenient to employ. a model
in the centimeter
Yange of waves, On this basis the author has fm*niahed experimental
data on
resonance scattering of radio waves at this model of a meteor
trail, He has found
that the phenomenon of plasma resonance begins at linear electron
densities of
'1(A2 electrons per centimeters but at this noncentration the value
of the averaged
adielectric constant of the plasma must be negative* When radio
waves of'traneverse
Cardl/2'

F7 -J; Pr-
t
'm )4 60,,r) 40.
ALUHOR: Bayrachenko, 1. V.
TITLE: Men!-,urements of initial radii of ionized meteor trails based
on the simul-
tp-neous observations of radicimeters at two wavelengths
SOURCE: Geomagnetizm i aeronamiya, v. 5, no. 3, 1905, 46o-W,
"Y'
TOPIC TAGS: radio ec' t trail meteor trail measurement
RjV-1 r-i~ i of ionized meteor tral'., wt-r,- determined --in the
basis of
tit, wavelengthE:, t.ht, listFinct- fn-,.i, otservatic;111
V~-I-r i ty. A I 'I' ti.'s WFLs capalble of
.-if tk trpt~i -,it two wavelength-
dM-at,1011
r(,auIqt(,d within
-n- i
'io-je x T,. ~:',F,t.Cor-ms 7h~,
tw~- two-guui C? tubea: two traces -gerc Lisied for am-
p! itude-tJ me display of echoes and two for m4eteor slant range
measurement. The
Card I
6

=wNt
L 63562--~,5
jACCESSION NR: AP501~106
0.1-1-sec sweep duration permitted the measurernent of meteor
velority. The amDlitude-
time chara(-terl~-,tics 'khe ra.6ic~ f--chc) fr(~!n the tr;til
appcar~ng on
Cjj~ ~ C77 Cit, 1 1 V "h f, U -r
A i c k d
4:0 1 .nol h; i ir.l s f ro n-. i C) C? v r nr ~2evi cc rc~ccrded
F
t

~L -04098-67 - EVr1 - G.41WR -
F-AC-C N-Ri- AR60-2~~77-
SOURCE CODE:
3/HD57,
AUTHOR: Bayrachenko, 1. V.
TITLE: N-atz-re of radi;'echo.from the heat of a meteor
SOURCE: Ref zh. Mika., Abs. 3Zh396
REF SOURCE: Pro pryrodu radioluny vid holovy meteora. Visnyk
Kyyivslk. un-tu. Ser.
astron., no. 6, 1964, 92-97
TOPIC TAGS: meteor trackingo radar meteor observation, meteor
trail, radio echo
ABSTRACT: The author discusses critically differopt opinions
concerning the nature
of radio echoes from the frontal part of a meteor,.
Arail (diffraction theoryj, ultra-
violet hypothesis). A qualitative atplanation o~ the nature of
radio echo from the
frontal part of the meteor trail is presented, starting from the
usual theory of
formation and destruction of ionized meteor trails. To obtain a
moving radio echo
it is necessary to have the following: a) the trail must be
produced at an altitude
on the order of 3DO km, i.e., the meteor body should enter the
atmosphere of the eartb
with sufficiently large velocity, b) the zenith angle of the
meteor radiant should be
large, c) the surface of the critical density of the electrons
in the trail should be
approximated by an ellipsoid of revolution. A possible condition
for the occurrence
of radio echoes from the bead of the meteor is the breakup of
meteoric bodies. [Trans
lation of abstract]
SUR CODE: 03)W
ki,
Card
W'47~ '-.-
3/1
-

L 45241-66 FSS-2/E4T(1) GVWR
-ACC NR.
AR6023289 SOURCE CODE: UR/0058/66/OOOiOO3/HO571HO57
AUTHOR: Moysya, R. I.; Bayrachenko, 1. V.; Mftll nyk, V. I
06
ORG: none iA
TITLE: Radar system for velocity measurements of meteors~e
SOURCE: Ref. zh. Ftztka, Abe. 3Zh399
REF SOURCE: Radtolokatsiyna ustanovka d1ya vymiryuvannya
shvydkostey
meteoriv. Visnyk Ky3dvsl k. un-t . Ser. astron., no. 6, 1964,
115-119
TOPIC TAGS: radar system, velocity measurementtmeteor
ABSTRACT: The block-diagram and some assemblies of a radar
system designed
to measure meteor velocities are described. The basic parameters
of the system
are as follows: wavelength-6. 49 m, pulse duration-10 #&see,
repetition
frequency-400 pulses/see, pulse power-50 kw, receiver
sensitivity-5 it v.
[Translation of abstract] JDW)
SUB CODE: 09/
.'d l / i .1r ~

L 0692b-67 WTM GW
ACC NRs AR6025345 SOURCE CODE. UR/0269/66/000/004/0055/0055
AUTHOM Bayrachenko 1. V.; ellnik. V. L; Moysya, R. 1.
TITLE: ;Ome raults of meteor observations on two wavelenths
V/
SOURCE: Ref. xh. Astronomiya, Abs. 4.51.435
REP SOURCE: Geofiz. i astron. inform. byul., no.8, 1965, 25-28
TOPIC TAGS: aeovensomr, radio astronomy, meteor, meteor trace radius
ABSTRACT: On the stAtion "Tri Wye" of the Ki ev university,
radiolocational obser-
vations of meteors on the 31.26 and 46.2 me were conducted during
October-December
1963. Based upon an analysis of common amplitude/time
characteristics, the initial ra
dii of the ionized meteoric traces were determined. The average
magnitude of the ini-
tial radius was re I a. The dapendence of r on atmospheric density
is proposed in
-08
The dependeonce of the initial radius upon m teor ve
the form: e
locity, Y, has been obt In the form vi rrv*33. [Translation of
abstrac
tj
SUB CODEt 03
egk
C,rd- 1/1

ACC__N_R_s__M5 02 629 6 SOURCE COM UR/3133/651000/00810026/0028-.-
0~
AUTHOR: Sayrachenko, I.- V.; Mel'nik, V. I Vloysya, R. 1.e:Se
ORG: . Kiev State University Kiyevskiy gDsudantvennyy universitat)
TITLE% Some results of meteor observations at two wavelengths
SOURCE: AM UkrSSR. MezhduvedomtvewW geofizicheskiy komitet.
Informatsionnyy
byulleten'. no. 8, 1965. Geofizika i astronomiya (Geophysics and
astronozW), 26-28
TOPIC TAGS: moteor trail, radar meteor observation, riometer
ABSTRACT: In order to atu4 'the problem of interact cc of radio
waves with ionized
meteor trails, a special radar system was developed which makes it
possible to ob-
tain amplitude-time characteristics of a single meteor trail at two
wavelengths. The
system has the following parameters: carrier frequencies, 31.26 He
(A - 9.59 a) and,
46.2 McA = 6.49 m);. pulse repetition rate, 500 pps ; and pulse
width, 10 psec.
Observations of meteor trails were conducted from October through
December, 1963.
The initial radius of a meteor trail was determined from the
general anplitude-time
characteristics obtained at the two wavelengths. This initial
radius was found to
depend on altitude not only when the mean free path of air
particles In changed but
also when the initial energy of evaporating free atom is changed,
since the average
altitude of. radio echoes is a function of meteor velocity. Orig.
art. has: It figures.,~_~
[JR.]

-L _VJ4V9=0f _1kW_kkPj/r0Z1j_,4/bW111) KLW/LM
AM NIG 32436 SOURCE CODE: UR/3133/66/ooo/009/0153/0156
AUTHOR: 'Bayrachenko, I. V*.
ORG: Kiev State Universitj (Kiyevskiy gosudarstvennyy universitet)
TITLE: The.nature of resonance pbenomena during radio
wave-Acattering by meteor-trail
models
NV . I
SOURCE: AN UkrSSR. Mezbduvedomstvennyy geofizicheskiy komitet.
Informatsionnyy
byulleten', no. 9, 1966. Geofizika i astronomiya, 153-156
TOPIC TAGS: radio wave scattering, meteor trail, plasma resonance
ABSTRACT: Theories on the nature of plasma resonance are reviewed
on the basis of
experimental data on resonance scattering of radio waves by models
of meteor trails.
Experiments were conducted at A = 8-13 m with a cylindrical
gas-discharge tube
%nside diameter, 1.02 cm; length, 70 cm) containing mercury vapor.
During the
transverse polarization of an incident wave with variations in the
discharge current,
a seriesof reflected signal maxima, believed to be caused by
resonance phenomena v4s
observed. Pundamental and higher resonance modes vere observed,
which behaved
similarly under various conditions of scattering. Theories based on
models of cold'.
plasma could hot be confirmed experimentally. Higher resonance
modes are attributed
to the motion of hot electrons. This phenomenon indicates an
interaction between the