SCIENTIFIC ABSTRACT BABADZHANOV, P. B. - BABADZHANYAN, G. A.

• Document Type: CREST
• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R000102810003-6
• Release Decision: RIF
• Original Classification: S
• Document Page Count: 100
• Document Creation Date: November 2, 2016
• Document Release Date: June 6, 2000
• Sequence Number: 3
• Publication Date: December 31, 1967
• Content Type: SCIENCEAB

BARADZWICV, P.B.
.-
Studying the relationship of-meteors with other minor bodies
of the solar system. Biul. Stal. astron.obser. no.22/23:59-61
'57. (MITIA 11: 7)
(Meteors) (Solar system)

IVANIKOV, V.I.-, SOLOVITEV. A.V., otv.red.; BABADZV
=Tj P.B., red;
DOBROVOLISKIT, O.V., red; KAT,62r., f3o't' rea.4,~R%V, red.;
FWWV, tekhnored,
[Methods used in photographic photometry of meteorej 0 metodakh.
fotografichookoi fotemetrii metaoravo Stalinabad. 12d-vo Akad.
nauk Tadzhik, SSR. 1957. 45 po (StalinabaA.Astronomichesksla
observatoriia. Biulleten'. No. 21) (MIRL 11:8)
(Meteors) (Photometry, Astronomical)

SAIDOV, Ka9ym Khasanovich; SOLOVIUM, A.V., otv.rod.; BABADZHAWY, P.B..
red.; DOBROVOLISKIT, O.V., red.; KATASEV,
A.M., red.; VINOGAUSKAYA, S.N., red.izd-va; FRDWV. P.M.. takhn.
red.
[Spectrophotometry of Beta IOrrao1SpektrofctometriiajB Lira.
Stalinabad, Izd-vo Alt' Tadzhikskoi SSR, 1957. 9'?p. (Stalinabad.
Astronomicheakaia observatorlia. Trudy, vol.66) (MIRA 12:10)
(Spectrophotomatry) (Stars, Variable)

AU T! MIS: YC- K- , litumber,' AS UeorCian SSR 30 -58 -6/4 5
Kebuladze, V. V. ) Candidates of Physico-Mathematical
Buklinikashvili, A. V. ) Sciences
Otorbayev, K. 0. and Babudzhanov, P. B.
TITLE: According to the Plan of the International Geophysical
Year (ro planu mezlidunarodnogo Ceofizicheskogo Coda)
Investil,,ations by UIC Scientists Of GVOrCia, the Yir,")1iV'
Republic and of Tadzhikistan (Isalodovaniya uchenykh Gruzii,
Kirgizii i Tadzhikistana)
PERIODICAL: Vestnik Akademii 11auk SSSR, 1958, Nr 3, PP- 56-58
A13STRACT: The cnrriud out by GeorGia are concentrated in
T, I iQ I I L5 !1 L I I LU Of %; UU I)) )~~ ';i, CS ,in tile Astrophysical Observatory
Abtistumani of the AS Georgian SSR, aa well as in the institutions
of the administration of the Hydrometeorological Service. The
coordination of work is carried out by" the Presidential
Committee of the AS Georgian SSR under the Presidency of
president N. I. Muskhelishvili. The investiration in the fields
Card 1/2 of geomaLnetic and t:eoelectric storms, as well as the

ftccor~int:- to the Pl,-.n of the Internationil Goophysical Year '~'0-58 -3 -6/45
li;vu~~Ii -,tjon!-, b,! tj;.~ Z~,4ejjt4,jf.,j
of Georl;ift, th~, Kirchiz
Rc-1,ublic wid of Tad,,,'-i~kistan
Vill, i'~ ti (11111 of tilt, intowlit:. ~f C0,;::IiG
for i-n the vorkint~-plan: ZhUSC 2tationary observations are
carriDd out in the Geophysical Observatory Dushet and at the
St-.kti3n for Cosinic Radiation in Tbilisi. The observations
are carried out since October 1st 1957 in a ionization chamber
of tbi? station Tbilisi. The observatory Abastumani carries
out invostiCations concerning photo- and chromospheric
formi,tions on the sun and concerninU the physical parametprs
of th;~ upper atrioophore of the earth. A riew telescope for
solar investiCations was set up in thi-i observatory on the
occas..on of the Geophysical Year. The collaborators of AS
Kirgh:.z SSR are to solve a series of important problems of
moder:t glaciology by means of the example of glaciation of
the C,intral Tyan'-Shan'. Both stationary and expeditionary
inves..igations are carried out. The astronomic observatory
Stali-atbad of the AS Tadzhik SSR carries out investigations
in thf! field of meteoric astronomy. The investiCations are
C
carri;i(I out by means of photo(-,raphic, radiolocational and
vi sua-- mathods.

KISELIVA. T.P. ; F=HUN. M.S.; L&TYPOV, A.A.;,A_A~!ADZHUOV,_ P.B.; RUSSO,
Yu.D.; 019MINK, R.I., nauchM7 sotrudnik
Results of photographic observations of artificial earth
satellites. Biul.sta.opt.nabl.1sk.9put.Zem. no.9:16-24
159. (MIRIL 13'3)
1. Glavnaya(llulkovskeya)Astronomiebaskaya observatoriya AN
(SSSH (for Kiseleva). 2. Glavnaya Astronomichaskaya observatori7a
AN USSR, Kiyev, naeballnik stantall nablyudenly (for Yedchun).
3. Tashkentskayu astronomicheskaya observatorlya All UsSSR,
nachallnik fotografichaskoy stantsit (for Latypov). 4. Institut
astrofisiki AN Tadzhikskoy SSR. Stalinabad, nachallnik stantail
fotonablyudeniy lskusetvannogo sputniks Zemli (for Babadzbanov).
5. Odesekaya astronomicheskaya observatoriya; nach& nik
stantsit nablyudeniy lskusetvennogo sputnikR Zomli (for Russo).
6. Astrosov"t AN SSSR (for Chuprina).
(Artificial satellites--Tracking)

BABADZHI,IIOV. P.B.
Photographic obnArvations of Perseida. Biul.Inat.itstroftz.
All Tadzh.SSR no.P.6:13-20 '59. WIRA 13:5)
(Motoors-Aulpiat)

RABA OVY P.B.; SOSNOVA, A.K.
Photographic observations of meteors in 1957& Biul.Inst,astrofiz,
AN Tadzh.SSR no.29:3-15 164). (MIR& 14s2)
(meteors) (Astronomical photQgraphy)

S103516 2/bW/0 1 2/o24/o6 4
A001/A101
AUTHOR: Babadzhanov, P. B,
TITLE: The meteor seminar at Ashkhabad
PERIODICAL: Referativnyy zhurnal, Astronomiya i Geodeziya, no. 12, 1962, 69,
abstract 12A513 ("13yul. Komis. Po kometam i meteoram Astron.
soveta AN SSSR", 1961, no. 5, 54 55)
TEM A seminar was held at the Physico-Englneering Institute of the AS
TurkmSSR on December 11 - 14, 1959. The seminar dealt with studies of physical
properties of the Earth's atmosphere upper layers-by Peans of visual and photo-
graphic meteor methods.
rAbstracter's note: Complete translation]
Card 1/1

DOBROVOLISKIY, Oleg Vasillyevich; BABADZHANOV, P.B., otv.red.; SERGEYEVA, L.V.,
.0 redJzd-vf; FROLOV, P.M.
[Noinstable processes in comets and solar activity] Nestatsiorarnys
protsessy v kometakh i soln9chhaia-hktiYnost!. Stalinabad, lad-vo.
Akad. nauk TadzhikAoi SSR, 1961.194 p.' (Akademiia nauk Tadzhikskoi-
SSR,, Dushanbe. Institut aetrofiziki. Trudy, vol. 8). (MIRA'16:5)
. (comets) (sun)

43287
S/831/62/000/003/008/016
E032/2514
AUTHORS: 13.il).t(lzliaiii)v.-P-..~13-;Iz~iirev, A.M. and Rubt.5ov, L.N.
TI,rLE: Meteor observations at Dushanbe
SOURCE: Ionosfernyye issledovaniyaAmetcory). Sbornik stntey,
no.8. V razdel programmy MGG ~ianosfera). MezhcItived.
,,cofiz. Icom. AN SSSR. Moscow, Izd-vo AN SSSR, 1962,
56-63
TEXT. Tile Institut nstrofizilci Akadcmi~a nanic Tadzhiltskoy
SSR (Institute of Astrophysicm, Acade-.1y of Scionces, Tadzhi;t SSR)
ha~:. carried out photographic, visual and radnr meteor observatioliv
in accorcijmc-~ -.,itli the IGY orogrimvies ~he 'piiotographic program,.ic
involvedIt. 1) th(, study of tho n1titude, velocity and bri,,rIltIless of
~ijeteors wit'i a view to dot(-rjni))ing-th;! poysical para;~Ietors of tile
upper layers of tile ati-io-,i-)here at (-0-120 km ahove sea level;
2) comparison of those 1)(Irameters with other data, roc!zct Oatn
so as to (etermino their sentoliat variation, w4d 5) 5t',Ikl%' Of
metcor radiants :%nd orbits. The t)1iotovraphy was carried out fl-011
two points separated by .13q69 i-- Ench point -as eiliinped witil
seven HAI,A3r-125' (NAFA 3s/2)5)cn,*-r(v%,dth objectives
Y~
Car'; 1/3

Meteor observatious ;it Dus!umbe. s/6il/62/000/OOJ/OOJ/OlU
1;0-)2/E5 14
6bjective diat-v!ter LO cm, focal len.,%th 2") ct,i, frw,%e size 18 x 24 cm).
The angtilar rang,~ of each point was 600 from zenith, xji(4 each set
of cameras was set iij) on a-i adjustable base controlled hy a cluck
mechanism, so that star remailled stationary r(!l;)tive to tho
film. A spociiil rotating shutter was used in front of the ca::1eras
at one of the point5. All the observations were carried out on
clear muonles.,; ai~vllts usilig 30 t"i" exi)osklres at 10 !All intervals.
Between Jiily 11 1957 in(] December '31, 1958, 815 e.-mosures, were wmdc.
The visital observations of meteors 7ind i;ieteor troils were carried
out with IGY-pro,~.,rc~nwie instructions. nipy were made in parallel
with radar observations in jun-!-September, 19738 blit were not very
extensive. In addition, observatioy-L-of the Gemiiii"s i-.,ere carried
out on December 1953 in ixccordance with the Czechoslovah
pro,~ram..ie. Alto,~ether in 1957 and 1956, 127.7 hours w-ere spent
in o:.)servations uf meteor trails and 96.9 hoiiri3 were spent in
observing telesco )ic t-teteurs. The radar observations were ;.mde
at 4.11 m (72.93 ic/.Sec) at a pulse repetition freqiiency of 50 CPS
(Imlse length 10 jisec, power per pulse 50-70 10D. The nine-elmient
an t enn n w A s at 2-10 above the horizon, facing vrest. Th e
Card 2/3

Meteor obsorvationm ut Dushnnbe S/831/62/000/008/008/016
E032/E5i4
ittinimugn range was 120 !vt% (slioi~ter ranges were eut out by the
presence of mountains). A calendar of the radar observatioils*is V~
reproduced. There are 2 tables.
Card 3/1,

BABADMMIOV, P. B.; KASHCIMEV, B. L.; KRAMER, Ye. N.; TESESETICH, V. P.
"The Research of the Meteors during the IGY in the USSR."
varjamr
abstract presanted at the 13th Gen Assembly, IUGG, Berkeley, Calif, 19-31
Aug 63.

BABADZ-11AN,OV, Fulat Babadzhanovich; KRAMER, Yefim Naumovich;
FEDYNSKIY, V.V., doktor fiz.-matem. naukp otv. red.;
VERSTAK, G.V., red.; GUSIKOVA, O.M., tekhn. red.
(Collection of articles of the Intergovernmental Committee
for the Excecution of tl,e International Geophysical Year]
Sbornik statei Mezhduvedomstvennogo komit,3ta po provedeniiu
Mezhdunarodnogo geofizicheskogo goda. Moskva, Izd-vo AN SSSR.
No.12[Mothods and some results of photographic studies of
meteors) Metcdy i nekotorye rezul'taty fotograficheskikh is-
sledovanii meteorov. 1963. 3.40 p. (MIRA 17:2)
1. Akademiya nauk SSSR. Mezhduvedomstvonnyy komitat po pro-
vedeniyu Mez~dunarodnogo geofizicheskogo goda. V razdel prog-
ranmV MGG. Ionosfera i meteory.

8/269/6-3/0()Q/W1/02Q/032.
AOO 1/A 10 1
AUTHOR: Babadzhanov, P. B.
------------------------------------
TITLE: 'The density of the upper atmosphere from 'photographic bbservatiorm
of meteors in 1957
PERIODICAL: Referativnyy ihurnal, ABtronomiyk no 1' 1963, 75,
abstract 1.51.508 ("BYul. Komis. po kometam A meteoram Astron.
soveta AN SSSR", 1961, no. 6, 35 - 39)
TM The author presents thL results of calculating the deneity of the
atmosphere from the photographs of 34 meteors taken zvt the Institute a Astro
physics, AS TadzhikSSR (Dushanbe), The main information about these meteors'Is
rdi-
tabulated; the table contains numbers or meteors, dato of observations, coo
nates of radiant, extra-atmospheric velocity and masa, absolute ;!~otographic
stellar magnitude at the point of the maxim= luminosity, and altitudes of..
appearance, maximiom luminosity and disappearmioe of meteors, The valuea of-*denvi-
ty calculated from d-i-,celeration and luminosity (in the Wtial part of the tra-
jectory) of meteors a;re presented In tables and graphically; they are compared
with the data of rocket meavirements of the atmoapherio density-There am 5
Car,~ 11P

The density of the upper atmospher6- from ...
6
references.
[Abstracter's notei Complete translatian] .
Ii
Card 212

ACCESSION NR: AT4024454- S/3010/631000/013/0043/0048
AUTHOR: Babadzhanov, P. B.; Katasev, L. A.; Konopleva, Vs Po; Kramer, Ye. N.
TIT!.~: Determination of atmospheric density, temperature and pressure from photo-
graphic observations of meteors
SOURCE: AN SSSR. Mezhduvedomstven" geofizicheskly komitet. Geofizichoskiy
byulleten', no. 13. 1963, 43-48
A
ft
TOPIC TAGS: meteo~o"Ioqy, meteor, atmospheric d~~Siiy, atmospheric pressure,
atmospheric temperature, homogeneous atmosphere
ABSTRACT; Atmospheric density has been determined by Ye. N. Kramer on the basis
of 50 photographs of meteors; P. B. Babadzhanov has determined atmospheric density
and the height of the homogeneous atmosphere from 34 photographs of meteors; and
V. P. Konopleva has obtained similar Information from 10 meteor photogra,)hs.
Kramer's formula Is cited and a table.of his results given. Babadzhanov's formula
for density is alsqgiven and at teble presents his results. Konopleva4s formula
and results are aidd given. Table 4 In the original compares the daita obtained by
the three authors for Intervals of height of 5 km from 65 to 115 km. The results
also are shown in Prg. I of the Enclosure. The 'tesd'Its of all threi agree well
,wilh Jacchia (Technical Report No. 4, Harvard Reprint, Ser. 11-32, 1949) but
Car . 1/5j ~ . 1: 1,

71ESSION NR. AT4' 4454
ACC 02
systematically differ from the standard atmospheTe tables published in the SSSR
reason.s for the differenpe are discyssed. The formula used by
(1960). The 1,
Baba'dzhangv and Korio leva for determining the heigh(of the homogeneous atmosphere
.p
(H-,~) is cited and their results are shown in Table I of the Enclosure. These
values were used to compute absol,ute temperatures; results are shown,in Fig. 2 of
the Enclosure. lf~~Itnsity an4t~mperature or the height of the homogeneous at-
mosphere are known'Ali is possib)~' to compute pressure by using the formula cited;
results are shown i!n.Fig- 3 of the Enclosure. I~ is;shown that the meteor method
makes it possible to determine atmcipheric density, temperature and pressure at
hei'ghts of 70-115 kin4 Orig. art.-has: 4 figures, 13 formulas and 6.tables.
ASSOCIATION: MEZHDUVEDOMSTVENNY*Y GEOFIZICHESKIY KOMITET AN SSSR (Interdepart-
mental Geophysical Committee)
SUBMITTED: 00 DATE ACQ: I 1fpr64 ENCL: 03
SUB-CODE: ES NO REF SOV: 003 OTHER: 001
Card.. 2/5

AccEssioN NR, AT4024454
A. Km
70
75
60
85
00
IOS)05
105
Height of Height of
homogene- homogene-
ous atmos-
,
ous atmos
" -pre.ssure,
here,

h ere

lev
Cno
f
K
MM Hg
abadz
anov p
a
7.30 6.87 -
. 7,08.t0,21
237
0,35 6 6-3 6,49-t0.14 '24
5.65 6:32 6,WtO,32 2D0 7.G5.10"
5,20 5,72*0.53 too 4JO-10-.0
S'fo
5
45 6,13 5.61*0,52 187 *
~-
t
, 6 2 - 1 O
1 6,00 5t72*0,28 IDD -
4
o
.48. to
6,05 5,88 5 96.t%oo 108 2,69-IV4
0.70 -5,83 6~i*0.32 2DO ijme

INCLOSUREi 01
Card 315

ACCESSION NR: AT4024454 ENCLOSURE: 02
%
iW
4P..
Fig. 1. Dependence of atmospheric density on height. I Kramer's meteor observations;
2 Konopleva's observations; 3 - Baba4zhanov's observations; 4 Jacchla's tables;
SSSR standard atmosphere tables.
Card 455
t MUM F.- ~uzxg F~
-77 -

ACCESSION NR: AT4024454
IS
1V 1/0 Uw Am lye
Fig. 2; Dependence of atmospheric
tempqrature on height, I - meteor
observations; 2 - staddard at-
mosphere tables.
Card 5/5
ENCLOSURE;
03
Fig- 3. Dependence of pressure
on height. I - meteor observations;
2 standard atmosphere data.

ACCMION NRr AR4021623 3/0269/64/000/002/0075/0075
SOURCEs RZh. Astronomiyal Abse 2*51*563-
AUTHORt Babadthanov, P. B.
TITIEs Results of photographic invesU. -11ons of meteors at Dushanbe during the
International Geophysical Year and period of International Geophysical Cooperation
CfTFZ SOURCEs In-ta astrofiz. AN Tedzh'WR., mo. 36# 1963., 3-36
TOPIC TAGS: astronomyj, meteor.. atrwspheric density; meteor atreamp International
Geophysical Year
TRAtBrATICN: A total of 545 meteors were photographed during the period July
1957 to December 1959 in accordance with the International Geophysical Year and
International Geophysical Cooperation program; of these 545 meteors 360 were
photographed from two points* More than half (181) of these observations were
processed and the geocentric and heliocentric orbital elements of these meteors
determined. On the basis of 150 photometrically processed meteors it was pos-
Card 1/2

ACCESSION NRt ARL021623
sible to determine the croas section of density of the earth's atmosphere between
heights of 70 and 115 km. The results are compared with rocket measurement data
on atmospheric densitye Most of the neteors belong to stream and swarms* Five
new awarms were identified, 2 of which Rre associated with comets. Bibliograpby
of 10 titles. Author's abstract*
DATE AcQ, o911arbL SUB CODE: AS ENCLs 00
Card 2/2

ll,'U-All,'~LIIANOV, !'.13. ; IL'~L fiC, "HE'HEV, ; V 1 1. - , .. .
_._ - _ I -. - .... - E. . N. ; _', - - : . -
Study of maWors d1iring the IGY. Ge(,fi,-,. biul. '64.
O'.1RA 5-8:4)

E
9WAM/SEC-4/Z CW/EWA(h) -4/pe-
pae-v b .4 aw j,
(ACCESSION NR: '31 ......
_Bv.2_..YAqV heyevi-B.--L #--Kramsrj-Y%- Help Timsevi
i AVrHDR, ftbadshanov,, Po.
N
ITXTLR:, 7be otudy of meteors dur~6 the q, zf!
,SOURCE: AN SSSR. Mezhduvedomet~~nnyy, geofiticheakLy komitet. Geofizicheakiy
by.q.l.leten., no, 14,, 1965, 83-88
-,-WP
n '\'~vind velocity,-meteor-ine ence
me
i
teor study$ ae,~ospheric density,
meteor maxiwum~brightness, meteor~extinction
rvey- -1.4 ernationally--colletted-datt-rdt,~ilti7n-- -from meteor
ABSTRACT: This-io--a-su,
9
iobservations dur,ing-tbe'IGY. GrOphe are-,compiled.- 1) ahowi" the atmospheric. ~1'
.density as a function*of height;:;g) giving the appearance altitude., maximum bright- f.
ness altitude, and the Oieapppar~nce altitude of the meteors as a function of their
velocity; 3) conparing the tbeorali ical brightness curves with the experimentally
iobserved'values; 4) showiag prev;'
'ilent wind velocity changes within thg meteor cone
.f ~ the atmosphere; and 5) attemp.~;'ing (unsuccess fully) to uncover some ~ def inits re-
Ilation between theJogarithm of ~'Ie dif f Sion coefficient and the altitude of ob--
Iservation. Soviet observatioas Vind-calciuAations were-carried-out-mainly at-Dushan-a-
Odeasa,,#nd the Xhart
'be, kovskiy.!;po1iteUhnicbeekiy institut (Kharl~qv Polytech ic.-
Inetitute). Orig. art. has.--- .2 `,tormlas-and 5 -f igures.-
-,Card 1/2

11
0
4
R

1. 14. ; Ye . N.
Preliminary results of photogrriphing iff,,tecru b',, the inst."taneous
exposurn method. Astron. zhur. 42 no.3-.660-664 Ky-,'e 1~5. (MIRA 18s 5)
1. Institut astrofiziki AN Tadzhikskoy SSH i Odasskiy gosu~iarstvennyy
universitat im. I.I.Mechnikova.

L 17773-66 FSS-2/EWT(I)/,TCC/EWA(d)/T/EWA(li) I~P(c) GW
ACC NRI: AP6006673 SOURCE-CODE:---UR/0209/66/006/001/0153/0156
AUTHOR: Babadzhanov,-P. D.
1ORG: Institute ot As~T2p~ysicsq AN TadzhSSR (Institut astrofiziki AN TadzhSSR
TITLE: Determining attoospheric t~Mpei~atur~e, pressure,and density from photographic
observations of meteors
Vr
SOURCE: Goomagnetizm .1 aeronomiya, v. 6, no. 1, K56, 153-156
TOPIC TAGS: meteor observation, atmospheric temperature, atmospheric pressure,
atmospheric density, upper atmosphere
ABSTRACT: A method is troposed for determining the height of the uniform atmos-
P
phere as a basis for calculating atmospheric pressure, G'ensityand temperature. Thei
initial data were taken from i50 pjjq~tqgraphic observations~'bf meteors made in Du-
Ishanbe during IGY-DIC-59. rrom these data, 119 cases were taken with smooth
~photometric.curves. Meteors showing abrupt flashes or having maximum radiation at
the ends of their paths were rejected. The resu.1ts are compared with the data of
~
'VSA-60 rocket measurements and the method of least squarei is used for deriving ths~
UDCt 523.53:551.510.535
Card .1/2'

L 17773-66
ACC NR: AP6006673
following regression equation for the height of the uniform-atmosphere
H* = 34.64-0.695h + 0.0040sh2. M
The results of this formula may be-used as a basis for determining the temperature
distribution with respect to altitude.
H* = RTlvg (2)
where R is the gas constant; 0 = 29 is the molecular wei;;ht; g is acceleration due
to gravity. the relationships dplp = -dhlH* and dplp =' I
A/V with regard to (11
may be used for determining.atmosvheric.Dressure density:,
lap Inpo in p - In ps -
iSatisfactory agreement is observed betl~leen meteor and r(,)cket data on the variatiJ
lin atmospheri'c pressure and density with altitude. These results show that the pro-1
[posed method for calculating the height of the uniform atmosphere is preferable to
.previously used methods for studying the upper atmosphere on the basis of photo-
Igraphic observations of meteors. 'Orig. art. has: 3 figures and'10,fdrmulai. [141
SUB CODE: SUBM DATE: 12Nov64/ ORIG REFt 007/ OTH-REF: 003
,ATD PRESS:
.Card.. 2/2.

A~~ NR. U,7008916 SOURCE COM UR/0033/ 66/043/006/1306/0312
AUTHOR: Jabadzhanov0._,P!.,D,,_; Kramor, Yo. N.
ORG, As6 ~physl-c7s'_Instltutev AN TAdzhSSR (I~stltut astrotiziki AN TadzhSSR);
Odessa Stato Univorsity (Odesskly goss' univeraitet)
TITLE: Orbits of bright motoors from photographic-observations at
Dushahbe tina Odossa
SOURCEt Astronomichaskly zhurnAl,y. 43, no. 6, 1966p 1306-1312
TOPIC TAGS: matoor observationg comot
SUB CODE: 03
ABSTRACT:
The p1jotographic obsorvatio;ls of meteors whose results are pro-
sontod in this. paper were made during the period 1957-1963 using camoras
with objectives D = 10,0 =, F = 250 mm and a field of view 40 x 500.
used (width 19 cm). Exposures were :from 30 tO 60
Panchromatic fi-Irl w,13 asao The following Wor-
minute. Observations were at Dushanbe and Ode
a detormiDation of time
is givo,.i for about 50ri mot4*r observ t.ionss
of fli&ht; distribution of orbital elements; su%imajor axis; orbital '6n-
ciination; eccentricity; etc. Particular att,)ntion iz. given t* motcor
associations, especially the Perseids. The photographic observations of
bright meteors confimod their relationship to comets. The matcor bodies
and comets have the same kinematic properties. According to Whipplo's K
criterion most orbits of bright meteors are of the comotary clasj. The
Mantification of metoors. for uhich K > 0 with astamida has no ad
equate
oasis because, no sin e kinmatio. critorion can boused In drawing roll-
91
UM 521..75.15

ACC NR, A117008.916
abla conclusions concerning the gone4c relationship of rwteors to
astoroids or comets. Tho distributioi of Uie orbital elemoats for
.bri&ht motooro diftara in some rMeo%3 from those for "faint" meteors.
On tho average the brl&ht vioteors move along more elongated orbits and
the inolinations of those orbits are -greater on the average than -thono
of faint metoorso OrIg. art. hast 6 figureag, I formula and 2 %;ablex.

ABDULLAYLTf M.A.; BABANHANOV, S.D.
knalytic continuation of preamalytic functions. Trudy Sam. Gob.
un. no,144%101-112 164.
Analytic continuation of a certain class of preans.Ivtic Pimct.-mis.
lbldei113-117 (M2RA 18-9~

B 413 :d, '.' "I', , . (Mo a k v ,i )
-.Izatlon, the potential for reducing the codt of(production
,'If clothingo Shvein, prom, nos30 MY-Ja 165o HMA 1819)

MSE/Medicine Helmintho mid JiL--/.Fob 49
Relminthlaaie
H541cine Antigens and ArLtibodies, Analysis
*Chemical Nature of the Ccmplate Antigs" of
Certain RelmIntbe," A. M. Kuzin, S. N. Betdad-
thamov, 0. 1. Polyakov, Chair of Ors Chem.mad
Inst.. MZ BSFSB, Moscow, Uzbok ID4, Tae#kent, 2 pp
"Biokh1miya" Vol XIV, So I
De'scribes experiments an balminthe Thenia saginata
and Asoaris limbricoides. Concludes that antigen
e7olved.frordbelmintha Is a specific polyeaceba-
ride containing glucceu and also glucosamine And.
=a 45/49T~8
USSR/Metticine - Relmintbs and Jan/Feb 49
Relmint.niaels (Contd) i
ccmbined with aminq aclds. Asoarld and ox liver
antiaems have similm~ chemical oompo4itions.'
SVWtted 3 JAI 48-

BaUi~-zllanov, S. N. "On the on-cific an'uireno of
In S. ". B 1,ad,71,.anov) Sbornik pa zzootcl~imii i varazitolo~,-U, Taslik-ont,
1946, 1). 102-110.
SO, U-32" ~ 10 Apr'l 53 (Loto! 's lZhurnal In:,.-.1i Sta-,cy 11, 1949)

BABADZWkNOV, S. N.
Babadzhanovs S. N. - "Antileukopenic activity of extracts of bull tapeworm, and
antileukopenic, immunityO., Doklady Akad. nauk UzSSR, 1949, No. 2, p. 24-26, (Resume
in Azerbaijani).
SO: U-4329p 19 August 53, (Letopis 'Zhurnal Inykh Statey, No. 21, 1949).

5JUAZZ"JANOV, S.R"- 'N.1, chlon-korrespondent.
I VLAT
Leubopenic action in Oalves, of effective antigens obtained from helminths,
and the antileukopenic immunity. Dokl.AN Uz.SSR no.3:28-31 149.(MLRA 6:5)
1. Tashkentakiy meditainakiy institut im. V.K. golotova (for Babadxhanoy).
2. Akademiya Nauk Usbekskoy SSR (for Khodukin). (Antigens and antibodies)
(leucopenia)

n". 11-.1

-BABAULWOV, S.N.; KHODUKIN, N.I.
Study of the immunulogical action in man, of potent ancarid. antigens.
Dokl.AN Ux.SSR no.8;43-46 149. (XLRA 6:5)
1. Tashkentskiy medinstitut im. Y.M. Molotova (for Babadzhanov). 2. Ake-
demiya Neuk Uzbekskoy SSR (for lhodt*in), (Antigens and antibodies)
(ABcariasis)

earl
611114i
a sit I
0 o1111 1.
*it 14
iio Z
021:
On 2
6060660669411199
3. a a v 0 IT
14101, 0 0 Pit a A k 1 it cm AT IS
tv 4 a a t 4,44
'if tw$*
Ir
- ": IsA,
I
i
-r~6
Aip-41jI '11
luommilawaltIdIly 'bppwuuluivp) ami"A alit 1.41-floll
olit~w"j uplaquits -ow 0 ! jultuvw%mils %q, I I'lls amXmill
1,11WA ,, ",ql :V J,,A,!U.U,, i*bjlqjrq.t
V=. 4aA r. .11U.J.
JWA F ts"UW pit Jtjj 11 it
-jv 111tul )ql tuitil klimy 1,11v lurill umul
Istisull"1411 -141 111MI "'AM1111V `-twit
9 0. -$PRO Pf poolml
&C 'OV.9k, Qc 'I".) P '#I
-1) IWUV '011041, OPTION, -%'-W oj#114 IV V
1111111MIOR moo to vu#Aluv 041 jo sitsiou Iv3pulp sqj
101*044 o", Slit
IT. T-1- 11-
tt
at I L I
"Oe
00
00
00
r

Cl tm VOW bdmfntbj was digested by 0.1 at pH
ed portka was pptd. with CWI and
a down. The supernatant was tevtral-
lib"O.OPP d'Islyted &M the antipa pptd. with
acetont It WAS rcdLuolQ In HlO and rcpptd., JUst with
aretom'swi then with sk. Glycogen was then Olty"ated
bv salivary amylase, sM the antigen p td. twice vk1th ale.
VA ti4m antigen was thus prt4,d. wbl& contained a stuall
amt. of cubohydrate (10 S-17 94" reducing substances
ft-la Dot &tn) after 2 G. lt~~lysis In IV HIM) 16"d
Lon. tuatetial. S. Lev~kna

KOMPARPSEV, H.W.;-~BAWZHANOV, S.R.; KAMBULIN, N.A.; YRGOROVA. T.A.;
TUMMANYAN, A 0A.
Results of an investigation of the anthelminitic properties of
some plants of Uzbekistan. Ned.zhur.Uzb. no.7:51-55 n 158.
(MIRA 13t6)
1. Iz kafedry farmkologii (xav. prof. N.W. Kompantsev) i
kafedry obehohey gigiyeuy (sav. prof. S.N. Babafthanov)
Tathkentskogo gosudaretyennogo meditainakogo instituta.
(ANMMMMICS) (UZBEKISTAN-BOTANY, KEDIGAL)

BABADZHANOV, S.11.; Dj-ioao, Ii.m.
- -
Session of the Uzbek Republic ScienLific Society of Hyg eniats in
1959. Mod. zhur. Uzb. no,6,-73-75 Je 160. I~MiA 15--2)
(UNEKISTAIL-PUBLE HEALTH)

BABADZIIANOV, S.N.., aspirant
EtioloUy and clinical course of bronchiectasis. Mod. zhur. Uzb.
no-5s60-64 MY 161, (MIRA 14:6)
1. Iz kafedry- gospitallnoy terapii sanitarno-gigiyenichaskogo i
pediatricheskogo fakalltetov (zav. - prof. O.N.Pavlova) Tashkent-
skogo gosudarstvennogo meditsinskogo instituta.
(BRONCHIECTASIS)

BABADZHANOV, S. N.,
Amount of certain electrolytes in the blood of healthy persons under
the olimtic conditiona of Tashkent. Mod. zhur. Uzb. no.6:45-46 Je
,61. (MI-(A 15:1)
1. 1z kafedry gospitallnoy terapii sanitarno-gigiyeni4eskogo i
pecliatricheskogo fakulltetov (zav. - prof. O.N.Favlova) Tashkentskogo
gosudarstvennogo meditpinskogo instituta.
(FUGUOLYTES) (TASHKENT-BLOOD ANALYSIS AND GIMUSTRY)

BABADMANOV ~ S. N. ;_ DEMENK0, N. 1-1.
Meetinge of the Uzbek Republican Hygienic Society during 1960.
Mad. zhur. Uzb. no.7s79-80 31 161. (~IIRA 15:1)
SOCIETIES)
(UZBEKISTAN--PUBLIC HEALTH

ijAi3ADZHAliuV, S.N., prof,
Imunity to holminthiasis. Mod. zhur, Uzb, no.8:46-53 Ag 161.
MIRA 15--l)
1. Iz kafedry obshchey gigiyony Tashkentakoeo gosudarstvennogo
meditainakogo instituta,
(WOW,b, UTESTIhAL MiD PARA61TIC) (IIOIUNlTY)

ROMPANTSEV, N.N., prof,; BABADZHANOV, S,N.t prof.; WTBULIN, N.A.,
dotsent; BAMIOVT,'-Te-.A-.'~A8sisteit
Data for a study on the anthelmintic properties of some
plants in Uzbekistan. Mod. zhur. Uzb. no.9:13-15 S t62.
(~9RA 17:2)
1. Iz kafedr farmakologii i obshchey gigiyeny Tashkentskogo
gosudarstvennogo meditsinskogo instituta.

BAMDZILMOV, S.N.
Ccntont of jmlns!~imn nw-t cah,hm in tho blood qorum cf
hylxirtens'lve patlent%, in hot ilimqfoi. Mod. -.I-,ur. Ilzb. no.4:
38-42 Ap 1613. 0-1-11HA 17-4)
1. 1z kafe-dry gospi.tal Inov tf-r!jp!A. (VIV. - 0.11. "UVIC)VO
poJlatrlchc.,.7~!,ogc,, i Ir.U.13 -
ko~:- I ~Vent skogo
gosudaro %
L, om0rii t.!3 !~jl, -~ 1 rn, 1- 1 tutti .

BAUDZHANOV, S. N.
Inorganic phosphorus content of blood serum In atherosclerosis
under the conditions of ~ !-.:' climate. Vop. biol. I kraev. med.
no.4:412-415 163. (MIRA 17:2)

KWANTSEV, N.N., prof.~ BABADZJWIOV~ S.N.y prof.; KAMNUT, R.A.,dotsen'.
KRYZHI24KOV, AX., dotsent.; BANNOVA, Ye.A., assistent,
Study of the anthelmintic properties of plants in Urbekistan.
Med. zhur. Uzb. no.6s24-1 gh; the equations of the flow lines are
\j
Card 2/3

82587
S/022/60,/013/01/04/010
C 111/ C 333
On the Plane ProbleLi of the Open Flow of an Incompressible Fluid
+ )t
X 4.. Cqnst + fj(h)
hv ain o~, 1~
sin(d � ~~.l. const + f (h)
Y hv jinA 2
where
(35) arc tg ( ot + -c I + const
while f 1 and f2 must be determined from the boundary conditions.
The author mentions N. Ye. Kochin, J. A. Kibell -,-.nd 17. V. Roze.
ASSOCIATION: Institut energetiki i --idravliki AN Armyr-nsko,, SSR
U
(Institute of Power EngincerinG and Hydraulics !,S
'rm"'L
.,L , nska-va SSR
SUMMITTEDi March 10, 1959
Card 3/3

88834
/0';t000
5/15 61/000/001/006/007
B023YB064
AUTHOR: -B&ha an G. A.
TITLE: Motion of gas in a long gas pipe at variable consumption at
the end of the pipe
PERIODICAL: -Izvestiya vysshikh uchebnykh zavedeniy, ITeftli gaz, no. 1,
1961, 99-103
TEXT: Tho author proceeded from a system of Eq. ap tpvi
ax 8;
ap a
at (pv).
P PgRT'
which he obtained from published data, and studied the pressure, the velocf-
ty,: and density of gas at.non-steady motion which is due to a varying gasl
consumption in the course of one day. In (1): denotes P pressures
card 1/6 -1

88834
S/152j61/OOO/OO1/OO6/-6bj---
Motion of gas in a long ... B023/BO64
v velocity, Q density, '"he coefficient of resistivity, 6 the hydrdilic
radius. To integrate the linear syBten of Eq. (1), the author performs
a partial linearization by writing dorni the averate value in the limits
of consumption variation
I j
OV b const. (2) instead of: Siv . After excludine ;from the
(-86 Sb
linearized system (1) v(x,t) mean Q(x,t) and writing p2(x,t) - P(x,t), an
2
Eq. 8 P b OP (3) is obtained. The author treated the
Ox2 777- - 7~-t
! P
following boundary- and initial problems
with x.- 0, P P constant (4)
OP RT 2
with x - 1, -~x-- - 406 G (t). (5)
with t - 0, P POW (6), where a is the
2

Motion of Cuo in 3 Ion,(,; ...
88834
3/15 6 1 / C 0 0 / C - C, I / C, C 6 /C 0~
B023 064
YB
surface of the pipe line cross section; G(t) is the 1-iven fumction char-
U
acterizing the law of consumption variation at the 0nd of th,-, pipe line;
P (x) is the function icharacterj'zln,-,~tlhe lar. of variation of thv-squar,?
0? ure alonC the pipe'lne at steady-state conkitions. TI-c- function
press
may be represented z~-. follcvo P (x) = (P CY) v-,here, P und 1.1p,
0 A A.
are the squares of ,,recouro at the be,-inninC and the end of the pike line;',
1 is the len.-th of the -ine line. If the variable coefficient P- is
replaced by its averaoe value at steady-state conditions, Eq, (3) reads as!
follows
P11,= (POCPT-1 P"+ P;
A, + Pm
Toi-xi Y1111111C111le (3) 11PHNICT IMA
alp b ap
Card 3/6

yotion of -as in a lonC ...
88834
S/152 61/000/001/0r-~/007
3C23/Bc64
is solved by tile method of the oi,erational Calculus
n:,.x
2 STF j 21
P(X, 1) A.
2
r
S11 MIX
n shl --
2
t
sin
2ac I
01 c - (to
,h,
2
0
u IC P2 _P2 (I (P-1),V
b
Card 6 R71
Vt C

,',:otior, of gas in a long
88834
S/15 61 /OC)0/901
/006/007
B023YI3064
If the solut ion obtuined for p(x,t) is introduced into Eq. (1), v(x,t) is
obtained and Q(x,t) from Eq. (3). Vi"hen determinilini_- v~x: '1~ , the exact
equation, and not the lineari,-ed one~iZl taken. For v x t, , -the-1-7thcr
obtained the followin,-:
xx
4 -1 COS-
21
ccj M
2 (10).
ac-. 21
sill
-9-
The law of the variation of cons!imi)tion is determined from the formula
Card 5/6

Motion of Gas in a long ...
38834
S/I 52/61/000/001/co6/66-7-1
B023/BC64
G(x,t) - cod. The author adds th!it the function G(t) can be accurately
determined if the Craphical of t;lls C011!,u1,!1)tio:1 is
On the busio of the law of the vor4~ation of function G(t), the inteCral
can also be eeterm ''ried from*Eu. ()), Lt'ld thll:; it is 1.)0.93ible tO Solve the
problem. There Eire 3 fiuures; 3 tables, and 3 Soviet-bloc references.
ASSOCIATION: Yerevanski Gosudarstvvnny,,, universitet (Yerevan State
Univcrsity~
S U D 14 1 TT 1:0 DSeptember 51 1960
C ard 6/6

BABADZHANYAN, G.A.
One problem of the unsteady motion of a gas in long conduits.
I zv. AN Arm. SSR. Ser. fi z. -mat. nauk 14 no.3:121-131 161.
(141RA 14: 8)
1. Institut energatiki i gidravliki AV ArmyRnakoy SSR.
(Boundary value problems) (Gas dynamics)