SCIENTIFIC ABSTRACT BENKO, Y. I. - BENKOVICH, I. L.

• Document Type: CREST
• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R000200020005-2
• Release Decision: RIF
• Original Classification: S
• Document Page Count: 100
• Document Creation Date: November 2, 2016
• Document Release Date: March 13, 2001
• Sequence Number: 5
• Publication Date: December 31, 1967
• Content Type: SCIENCEAB

DERBIKOV,- I.V.; AGULINIK I I-M-; BI,;N'KOJ-Ye.I.; YMOIANIN, Ye.V.; GRICSHIN, M.P.;
IUSHIITF V. I.
Tectonics of the MeBozoic and Cenozoic mantle of the Wetitern Siberian
Lowland. Trudy SNIGGIMS no.11:63-155 160. (MIRA 14-5)
(Siberia, Western-Gtology, Structural)

- BENIKOR Ye.I.; DERBIKOV, I.V.
Question of oil and (,,as prospects. Trudy SNUGG12AS ro-11:156-170
160. (141U, 14% 5)
(SibeftE, Western--Petroleum geology)

57-N'KO, Ye. I., cand U'eol-M".n Scl -- "Teotonics of the
Mesocenozoic depositu In the territury between the Ob
) it
and Irtysh RIvers oLf the Weotern SIberian lowland. NOVO-
sibirsk, 1961. (Acad Sci USSR. Sib(~ c ~
-j o he Joint Acad
Councll ori Geol-MIn, Lieopilyij, and -leog 32ience~;. inst of
Geol and jeoph,-9) (Kb, 8-61, 233)
- 9~i -

KOVALEVSKIY, G.L.; BENIKO,-Ye.l. _.
The technique of detecting zones marked ty the tapering jut of
lower Mesozoic dep)sits as posElble pe'traleum and gas traps
(exemplified by the Bol'sYerechlye area in the West Siberian Low-
land). Geol. i geofiz. ro.9:22-21' '61. (MIRA 14:11)
1. Sibirskiy nauchno-iss2Edovatel'skiy institut peoloi-ii, peofiziki
i minerallnoro syrlya, Novosibirsk.
(Petroleum ppology) (Bol'sherechlye repion--Seismic prospecting)

BEENIKO, Ye.I.; YEKHAXIN, Ye.V.; ZHADNGVA, V.P.; MITALEV, I.A.
Periodicity in tectonic mcvements. Geol. nefti. i gaza 9 no.7:
33-35 Je 165. (KIRA 18:12)
1. SilArskiy nauchno-ionledovatellskiy iwtitut geologii,
geofizLki i minerallnogo syrlyap Novosibirsk.

;37~j*rr,?:!'l--rz,9A,,.-,ky, L.
F:)LDTAO'l KOZLONY, BULLFum OF THE HUNOARIAll GFO'.iYj'IrAL S4?~',7--Ty. (Maj~yar
Foldtani TnrsulRt) Budapest.
Traces of fauna in the clay I-Vers of the F~er br,-~Ikyard. ~'. 344
1
Vol. 83, NO. J, JulYf'OPt- 1958
Month"y List of the East Furopean A.-e3slons (EFFAI). L;-, Vol. 8, No. 3, March 1959
Unclass.

Pi*~7 YIOV, il .RaisInF swine 'or hreedingy.
Vol. 12, no. IP, Oct. 1011:6
oflia, 7~ulaaria
SC: East Europ-in Accession, Vol. (-., Uo. 3, "arch 1957

KUNEV, Mitiu; BENKOV, Benko
.Influence of greon pen :i:~,111vo- fp#!ding c~n t)rovdIng pigs.
Izv Zhivotn nauki 1 no.l.:47-52 104.
1. Institute of Animal Husbandry, Kciarovgrad.

:3EORGIEV, Isai, BFNKOV, Benko
I
~rirlua*rJal crosabreedlIng cf
and the Derman mixed breed boars. -'-.v ?hivotn rauk! I ro-3-15-
-1
l< 4. 64.
I. Zootechnical Faculty of' t`v- G. lf,,phe- A g rLi I tura 1
Institute, Sofill, Corrospcnding Member of the A.--aderq
of S,-iences, and Member o! th,? Board of E-iitors, I'Izvc-stiia na
Akadc.-miiata nn nelskostopenskite nauk-' - Zhivotnoviidni nauk""
(f'or Georgiev). 2. Tn3titi.te of Animal 1k;.91,andry, Koin-ovi7rad
(for Benkov).

BENKOVA, D.
The rootless alga WQIffja grrIj a L. In southern. Slovakin.
P. 460, (Biologia) Vol. 12, no. 6, 1957, kraha, Cze,-hoelovakla
SO: Monthly In&!x of Fast European Acessions (E::,Al) Vol. 6, No. 11 November 1957

4M

BENKOVA, N. P.
"Eleven-77ear Cycle of Geonagnetic Activity," D)kl. Ail; SLER, 33s I-o.6p 1941.
Inst. Terrestrial MaFnetism, Min. Admin. Hydroneteorological Service

i- IV 'I r I 1 -1
~ - , -G. A 1, .'r ,
Durir4y 1946~1,7'1
"0: S',(,':, ','o 51,L/, Jan 19~2.

li --,: I L.P.
"The Diurrad 1,,olyLvior of lho,,notic Artivity,11
SO: ~uia 51, 14 Jan 1952.

BFNIKOVA,.N. P.
"GeographIc Distribution of the Daily Vari:ition of Magnotij,. Activity", Coklady N117,M
(Reports of the NIMI) No 3, 1948 (1-6).
SO: U-3039, 11 Mar 1953

BFN i KOVA t 11. P.
Benl~.cva, N. P. and Fedorava, L. N., "Magnetic Activity rArrina, 194-4 and lr~4511,
Tmdy No 2p IcI4.8 (110-116).
SO; U-3039, 11 Mlar 1953

BYJI 1 KOVA, M.P.
Daily and seasonal distribution of index K. Tnid7 NIUM n0-11:
119-121 '55. (KLJU 9:8)
(Magnetism, Terrestrial)

BEWYMA - - N , P..
"Electric Current in MaSnetic 3torme."
The Internatioal Association of Goomagnetler, and Aeronomy; Abstracts
of the Reports at the XI General. Assembly of the International Union of
Geodesy and Geophysics) Moscow, Izd-vo AN SSSR, 1,P57. 46 1.
Abstract: The regular components of worid magnetic and polar storms were
studied in world' wide observations from 1932-1933. The potentials of these
fields were computed and a system of polar atom currents was reconstructed. An
increase in conductivity with depth was determiagd and a break in it established
at 900-1200 km, where Gutenberg and Repatti discovered a discontinuity for P-
waves.

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60796
SoV/ 169 -c~9 - 6 -6462
,9.9100
Translation from, Rogferativnyy zhum,al, Geofizika, 1959, ?Jr (), p 1;57-1 (~-755;4)
AU MR Ber.lkova, N,
-!,,r *,.,, n,
T~ ME The Statistics of the E-layer Az~ord-'r4z to Ots a 2
USSR lonosphere~ Stations
rIMTODICAL.-, Dokl. 7-y Nauchn. konfer~ntsli poGiryash- 'h. V-.' tk--y
Oktvabrisk. sots, revolyatsil, Nr 2, TorEk. T-rr~:Ir-lv
1957, pp 79 - 80
APSTTiACI if, is shown thal. tho~ probabil.Ify of +ho
E,j (pEs) layer dep-~Lnds or). the type of
vert!(~al sounding of the lonospher,!, wA --n rr,~'-n:d ~~f irl-i-
~~pretatlon, 'The investlgati,)n of the F', ind ~-Iz;
r-woal?d -no esnential diff6rRn.~es. Th.! r:~ FS C,.'f.-
the frequencies hE.s a maximim on apnnoKimat,~lv M~-. C,f
total number of F.. mea~~ur--menfs, th-z E-
m-')rr~ thazn a few P;:rcent. Th--~ di-arnal zoljr--i7 c-' wi*.t-. r!-x-'.7~a
during the day and night h~)ljrs and
Car-i 1/2 d-,.irlng si.;urner. are ottalnEd by cb,

80796
SOV/1 69-59-6 -6462
-Tl--,e Statistics of the E-Layer AccordJxig to Observat-Jcn2 of USISE
Sr-at !,-ns~
lonosThere s,tatlons. It was establ'iched that there is -a terd-n~y -,C,
d.-~-.rease at t~-,e A-ctlc stations with an increase in the scl ar a: r~l-v
du,lrg -n,.- .11-y,~ar c,-)rcle. For the mJddle latltud,!,q, an
,of pE-~ or the 11-year cycle was not. found.The authov d!-,iw-- tbs-
,hat IndivIduall E.. -clouds exl3t, having an extension of il )'%rdr,?d
K- -
2/2

80795
9/ 00 S(Y-11169-1-:19 -6 -6 ~51
Irxislation from: Referativnyy zhurnal, Geofizlka, 1959, Nr 6, r,p 114) - ir~l
(USSIR',
AMORS~ BenIkova, N P. PotapCV8.
WA*I xJ
T.,
'IT 1'-E; The Variability of the Tonor3phire Pa
PERIODT'AL. Dokl, 7-y Nauchn, konferentsil, posvyashch. Vr-14~koy
Oktyabr'sk, sots, revolyutsli. Nr 2, 7cmak, Tom-~kly---ir.-', 19,57,
p 82
AB37?IA7r; The statistical analysis of the fluctuations of -he hcurly
vallues of foF2 ( 'nLfoF2) has shown that the distribution D-,
Z~foF'2 obey:3 VWa norma-l law during days wit-h a q~-il- iono-
sphere; the dispersion has a diurnal and a :~~:aZ~~nal -curse
-and depends on the solar activity. Tt was established that
t!2~,,foF'2 varies in the course of 5 - 10 min by no~, morp. thu,
O~2 MC and Lh'F2 does not exceed 20 bm. The spatial var.-Abll-
Card 112 Uty of iLfoF2 is characterized by Uhrb c-Drrelaticn -osffl~*-enl

80795
SCY/169-59-6-6451
The Variablilty uf the Ionosphere
between the zynchronous value5 of the paramet-~rs rr-~~a3ured at. 21-atictF,
lo--qte(~. at different distances. The valu^ of 9 dc,wri to 7,
moving away by 50 - 70 in latitude and by 200 in lorigitudm,
T.S. Kerblay
Card ?,/2

25-7-23/51
AUT11OR: Ben1kova, N.P., Doctor of Physico-Mathematical 3ciences
TITLE: At the "Alert" Signal (Po signalu "Alert")
PERIODICALi Nauka i Zhiznl, 1957, # 7, P 31 (USSR)
ABSTRACTj In connection with the IGY the Scientific Research Institute
of the Earth a Magnetism, the Ionosphere and the Spreading of
Radio Waves 4MIR) located near Moscow was decignated to co-
ordinate the evaluation of observations made by the various
scientific establishments in those fields within the USSR,
China, Mongolia, and Eastern Europe. To give good results, the
investigation of magnetic and ionospheric diaturbances have to
be conducted simultaikeously,by all observa'oriee in all parte
of the world. Four world centers were appointed to supervise
this coordination. NIZI(IR is one of them, the others are locat-
ed in Baltimore (USA), Pontoise (Franae), and Tokyo. When the
data from all subordinate observation stations are collected
and scientists have ascertained when the most pcwerful magnetic
disturbance can be expected, the main prognostic center in Bal-
timore will flash the word "Alert" around the globe to all ob-
Card 112 aervation stations participating in the IGY to etand by.

At the "Alert" Signal
25-7-23/51
ASSOCIATIONi Scientific Research Institute on the Earth's Magnetism, the Iono-
sphere and the Spreading of Radio Waves (Nauchno-isigledovatell-
skiy institut zemnogo magnetism&, ionoafery i rasprostraneniya
radiovoln - NIZMTR)
AVAILABLE: Library of Congreas
Card 2/2

AUTHOR:
TITLE:
PERIODICAL:
ABSTRACT:
AVAILABLE:
37-11-7/18
Ben I kova , N - P
-15-a-1-1y-and Seasonal Distribution of the K Index (K voprasu
o sutochnom i sezonnom raspredelenii indeksa K)
Trudy Nauchno-issiedovatellskogo instltuta zemnogo
magnetizma, 1957, Nr 11(21), pp. 119-121 (USSR)
Weak and strong perturbations in the magnet1c field art!
discussed, and the introduction of better indices for
the character and degree of perturbation is suggested.
There are 1 figure, 1 table, and 2 references, one of
which is TISSR/the other English.
Library of' Congret3s
1/1

AUTHOR: Den'kova., 3. P-.-- 37-12-3/12
T TTI Twenty-seven-day Recurrence of Exceptionsaly Strong Magnetic
Storms (27-dneymVa povtoi-jayemost' Isklyuchitellno silInykh
magnitnykh burl)
PERIODICAL: Trudy Nauchno-isaledovatellskogo instituta zemnogo magnetizma.,
ionosfery i ra":rostranenlya radiovoln, 1957, Nr 12 (22),
- 71-72 WE
pp 9W
ABSTRkCT: The recurrence of magnetic storms is of great value in short-
term magneto-ionooferic predictions. It was earlier believed that
the possibility of a recurring strong storm decreased vith an
increase in the Intensity of the storm. Elmever, recently collected
information indicates that exceptionally strong magnetic star 'us
develop a cluster of storms belonging to the sme synodic period and
to the same active area of the sun. In extra strong storms of
500-900 gamma M*litudes, 56 per cent are of the recurrent type;
in more moderate storms this percentage is much smaller. DIstribution
of the strongest storms ani their positioa in a group are given in
tvo tables. The majority of storms is Uned to the second stw in
the sun's rotatica. Mere are 2 tables &3d 3 references, of vhIch
2 are Rassian.
AVAMABLE: Library of Congress
Card 2.71

AMOR: &-n Ikova? ff. P. 37-12-8/12
I
TITLE: The Daily Hun of Short-Periodic Perturbations of the MectrowSmetic
Field of the Nexth (K vwvrowu o sutochnota khode korotiroperiodichesk1k),
Yommahchenly ebaktrampltnogo polys =U)
PERIKODM: Trudy ftuchno-Imuladavatellskogo instltuta zemogo mpetima,
lonoefery I raffrostrenenLya radlovoln, 1957, Nr 12 (22),,
pp. 209-213 (=at)
ABSTUM: The article disimsees sbAwt periodic variations of the earth's
magnetic field, much an alnumoidal, pasations or irregular ImpUses
with differeut m9lituden, and eraustest the results achleved by
V. A. Troitakays, and R. A. Zavakina* Mi partleul", Uw aut1tor
rejects the theory that -pulsations are ,purely local pbenmens and
expresses the copinion that electram4potic perturbations occur
siuataneowly all over- the vorld. 7bm action of mepetle fields
should alvap be exandned vith the short periodic vw1ations of
tenwric currents. The article also explains vhy certain observa-
tions my have seemed to be local: IwAequacy of thij resolving
Card 1/2

PHASE I BCOK EXPLOIATAI;'I011 712
Ben Ikova, Natal 'ya Pavj!wa--
Mezhdunarodny)r eofizicheskiy F:od I issledovaniya verkhnikh sloyev
atmosfery Mternational Geophysical Year and Studies of Upper,
Atmospheric Strata) Moscow,. Svyazl.izdnt,, 1958. 4T p .(Serie:
LektaM po tekhnike avyazi) 11,600 COPiC3 printed.
Sponsoring Agency: USSR Hinisterstvo svyazi. Teknicheskoye
upravleniye.
Responsible Ed.: Popov, A.U.; Ed.: Voronova, A.I.; Tech. Ed.:
Shefer, G.I.
PURPOSE! This booklet Is intended for the scientist and techniclari
interested in the program and ictivitteg of the International
Geophysical Year.
COVERAGE: The booklet, published by the Te-chnical Administration
of the Ministry of Communications of the, USSR, surveyo and
Card 1/4

International Geophysical Year and Studies (Cont.) 712
presents briefly the problems studied during the International
Geophysical Year, and discusses the practical inportance of
many of the observations carried out. ReseiLrch and observation av,
directed at the ionosphere, at atmospheric distiLrbances, the Earth'
variable magnetic field, telluric currents, the phenomena occlirli1j, '
the Sun, and the auroras. In the Soviet Url'LOTI these phenomena are
studied at 16 different citles scattered throughout the cuuntrr. 7`-
organization mainly responsible in supervising these geophysical
observations is the Scientific Research Ins',"itute on Terrestrial
Magnetism, the Ionosphere and Radiowave Propagation (N.-[ZxLR)' Of
USSR Ministry of Communications. The longe:-!t chapter In the book
devoted to radio investigation of the upper layer3 of the atmosph-C-,
and discusses vertical sounding-, and measurement of radlowave
absorption in the ionosphere, the measurement of ionospheric w1nds,
and the observation of atmospheric disturbances. IllWtration3 in
the chapter include flow diagrams of an ion.-.)spheric otation and a
setup for registering ionospheric winds, diagramB of the summer,
winter and night distribution of iononization in the upper layers
Card 2/ 4

International Geophysical Year and Studies (Cont.) 712
the atmosphere, photographs of registrations of high frequency
characteristics recorded at Moi3cow and Mirnyy, a photo of a vertical
sounding control panel at an Ionospheric station, and & view of
an antenrat setup at Mirnyy. The author points out that studies of thT
up-per layers of the atmosphere will provide extensive -material for
improving forecasting techniqu,!s, especially in forecasting magnetic
Ionospheric storms, and will increase our understanding of 3hort-wav,~
propagation phenomena. The bo3k contains 1.8 illustrations (dlagram:7
ar--l ohotosraphs), and a supplement which gives a calendar of regular
world day3 and worl( meteorological intervals. There a~,e 12 Soviet
refeg;encea. ,
TABLE OF CONTENTS:
Foreword 3
Introduction 4
Basic Problems of the IGY 9
Card 3/4

International Geophysical Year and Studies (Cont.) 712
Radio Investigation of the Upper Layers of the Atmosphere 11
Studies of Geomagnetic Variations 29
Studies of Auroras 33
Rockets and Satellites During the IGY 38
World Days and Special Intervals
Conclusion 44
AVAILABLE: Library of Congress
KMIksv
10-14-58
Card 4/4

GINDIN, Ta.Z.; =IN, G.A.; LOZIIISKIY, A.M.; MASWICH. A.G.; ALIPM, la.lo.;
CIMMESIM, N.Y.; SHAPIRO, B.S.; GAIKII, A.M.; GORWY, O.G.; rOTOFA,
A.P.; KOSOV, I.I.-, FXMV, A.T.; S3MOV, A.D.; CHOMY. T.N.;
TAKOVIAV. V.I.; KIKHATIAN, A.A., otvatatTonun red.; -BJW=Aq.-N.P.#
doktor fis.-mat. nauk, otyetetvannn red.; SILKIN, B.I., red.;
PODOLISKIT, A.D., red.; PMJSAKOVA, T.A., tekhn. red.
[Preliminary restate of the scientific rwisarch on the first
Soviet artificial earth satellites and rockets; collection of
articles in the Ilth section of the IGT program (rockets and
satellites)] Fradvaritellays Itogi na=hn~,ykh Issledovanii s
pomoshchliu perrykh sorstskikh iskasstvsnrqkh oputnikov senli
i raket; sbornik stated. (X:L razdal progrww7 MG - rakety i
slmtniki). Koskva. Izd-vo Akad. nauk SSSR. No.l. 1958. 148 p.
(KIRA lltIO)
1. Russia (1923- U.S.S.R.) HashduYsdoristTsixvyy komitst po
j:m-ov9deu-1yuKezhdun&rodnogo geofizichaskogo god&. 2. Chlen-kor-
respondent AN SSSR (for Kilchaylov).
(Atmosphere. Upper-Rocket observations)
(Artificial satellites)

ALIFIRT. Ya.L.; BINIKOTA, N,T,,_otv.red.; OMMI, L.T., red.izd-va;
P(MYAK0fk-V-T-.T-..~ - -tekhn. re 1.
(Propagation of radio wavl)s and the ionosphere] RBaprostranania
radiovoln i iononfora. Moskva, Izd-vo Aked.nauk SSSR. 1960.
48o p. (MIRA 14:1)
(Ionospheric radio wave propagation)

TIMINDVAt W.P.
lonoerhars. Nothdnnar. goofix. god no.8:21-23 160.
(MIRA 13 -13)
(ronospheric research)

0/904/61/000/000/011/0
B21 e/D308

Au"01M jj and. Potapova, N. 1.

-TIT 4n'effeoV 'aidalo eXplostons on the ionosphere
:~SMOgt DokladrNmuchnogo.simposimma, po ionoefere..
Rostov-aalli~bom 21-22'aprolya 19060 g. V rlssdel'
pro my, X06--!1(ionostera). Rostov on the Dout
gra
Ind-vo Ro uAiv. 19610 127-132
TM: Results taken from -the. World Data denter were used to
investiga te ionospheric disturbano'es of non-solar origin during
the-1958 nuolear tests over the Pacific and Atlantic Oceans. It
.
ik: ',,was found
that the exp cot ai~ an
1 on at'.off on Augmist It 19589 had
I
,
. - .. - -- - -- --t- - '.m __ - io - L ~
__I A----
__

Card i
!f'q
8/904/61/m/oO/011/011'.
An iirf a c tof.. D210308
of August 129 19589 ware invailigate'd in-a aWlar way. Here,
the effects were somewhait diffir"ekit-i, Thus ,at a distanoe of
km from the aioicenter~~, thii ,ivsm: mi nnna
a

Card
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txi

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1 I
01 I
6
D
1/ OO
ON/
8 904J
/0
/
Of kt of. D218ID308

lootronagnet a suaroy. .1heire !are3 fipros and 3 ta'bles.

SOCIA2.110N:
A 1 8, tut! tisna, ionosfo:ry
ma a
rn ti
fn
-
-
rad
rasprostz~msttlya (Instit
ovol3tAN SSSR u
.

,1667
S/570/,',1/000/019/007/008
6/, c7 tO -0 B107/'BlD4
AUTHORS: Ben1kova, N. P., and Konnova, R. V.
TITLE: Relation between ionization of the F2 layer, solar activity,
E.nd the sine of the solar anlyle
SOURCIF Akademiya nauk SSSR. Institut zernogo ra(-,neti,.,.r.-.,1, icnosfery
raSDrostraneniya radiovol.n. Trudy, no.. 19 (29), !761, 115-11
TEXT: The amnlitude of the daily variation of median values of the cutoff
frequency for the F2 layer is defined by the equati.on
AfoP2 = fo'32 Max - foF2min' the ratio K, by K - foF:?max /foF2min. In a
paper (Ref. 1, Astr. zhur., 37, no. 1, 135 (1960)), A. I. Likhachev used
observation results of the Tomsk station to qhc,A tie dependence -if the
above quantities on the sine of the iolar ani-le to be such- 6 foF11 = B-sinZ;
K = A,oinZ. There is a certain rule between the const-int'~ A and B, and
solar activity. The rresent paper :,ivf-,,3 an evaluation of observations by
the stations Yuzhno-Sakbalinsk, Alina-Ata, Rostov-na-Doivi, Simferopol' .
Its aim was to find out whether Likhachevln method was oultel for long-
range forecasts of foF2. The equations are preferably act un in two terms:
Card 1/3

31667
S/570/61/000/019/007/008
Relation between ionization of tile ... B100104
F = a + A-sinZ; LfoF2 = b + B-sinZ. A and B change linearly with the
relative number W of sunspots. a and b also increase somewhat as W
increases, Table 1 gives the graphically determine] values for
measurements of the Yuzhno-Sakhalinsk station. Deviation is low in
observations made by the stations Alma-Ata, Simferopol', and Yuzilno-
Sakhalinsk, somewhat (,,reater with Rostov-na-Donu. The reason rr.ipht be
that up to 1958 a hand-operated ion probe was used in Rostov which did
not allow exact measurements of the daily foF2 due to the limited
frequency range. Result: Tile linear relation between foF2 and,,sinZ, found
by Likhachev, holds for middle latitudes, at least for 40 - 50 north
latitude; the formula is preferably set up in two terms. The coefficients
are proportional to the solar activity. Checking and physical inter-
pretation of this rule with the aid of data obtained by stations at
different latitudes would be of great interest, The relation -.a hardly
suitable for the practical calculation of the daily foF2 variation. There
are 2 figures, 1 table, and 1 Soviet reference.
Card 2/3

31667
S/570/61/000/019/007/008
Rel,,;.tion between ionization of the ... MOW
Table 'I. Yuzhno-Sakhalintik etntion moasurements.
Table I
roA W
W B b A
1954 7 0,2.7 0,()0 0,74 C, 20
V)55 49 0, w. 0,19 0,94 C.2.9
i9r)6 M i.M 0,-m t.42 (1, 4:1
I'M 20 i'M 0.38 I'm (1.4,
1158 241 t.92 0,37 Ip (1,44
11-355 220 1,71 i 0,35 t. 62 (1,41
Card 3/3

3/169/61/000/009/038/056
D228/D304
AUTHOR: Deulkova, N. P.
TITLE: Ionospheric resea.rch in the USSR
FERIODICAL: Referativnyy zhuzmal. Geofizika, no. 9, 1961p 8,
abstract OG65 (Geomagnetizm i aeronomiya, Y. 1, no* 1,
1961, 4 - 20)
TEXT: Ionospheric research fulfilled in the Soviet Union in 1957 -
1959 is briefly reviewed. The principal directions of the work were as
follows: (1) Regular observations; at a network of ionospheric stations;
(2) investigations of the ionosphi-re with the help of artificial satel-
lites; (3) investigations of the quiescent ionosphere; ~4~ ionospheric
disturbances and the ionosphere of the high latitudeal 5 winds and
pouring movements in the ionosphere; (6) the ionospheric propagation of
radiowaves; (7) ionospheric forecasts ; (8) development of new research
methods and the designing of equipment; and (9) meteoric radio-inve iga-
tions of the ionosphere. There is a bibliog aphy with 140 referenc:!.
Z-Abstracter's notes Complete translation.
Card 1/1

S/169/61/000/008/043/b53
A006/A101
AUTHORS: Ben1kova. N.P., Tyurmina, L.O.
TITLE: Analytical concept of the geomagnetic fiel-:1 on the Soviet Union
territory for the 1958 epoch
PERIODICAL: Referativnyy zhurnal. Geofizika, no. 8, 1961, 34, abstract 8G240
("Geomagnetizm i aeronomiya~', 1961, v. 1, 110. 1, 87 - 103)
TEXT: For the 1958 epoch, the geomagnetic field on the USSR territory is
represonted with the aid of coofficients of expansion of the geomagnetic poten-
tial in series in spheric harmonics. The results are compared with charts. A
comparison is made of data pertaining to tile East-Siberian zone of the global
anomaly for a series of epochs, and secular changes of this anomaly are discus-
sed. The authors' summary tl/
[Abstracter's note.- Complete translation]
Card 1/1

- BEINIKOVA, N.R.; BONCHKOVSKAYA, Yu.S.; SHASHUNIUNt', V.M.
Iorosph,3ric disti~rbancas of July lr~-18, 1S159 according to
obsorvations at ionospheric stations of tl.a U.S.S.R. Geomag.
i aer. 1 no.3:36~"373 MY-Je 161. (H IRA 14: 9)
1. Institut zemnogo magnotizma, ionoafer:r i ra3prostranenlya
radlovoln All 3&;R.
(Ionosphare)

AO~~)/A 1-0 1
AUT1X)N:;: Berilkova, N. P.. Ytidi2vich. A.
I t, s ar ~i ln.~
TIME: Dl--irnaL varlatlo,is in the en, k, f:1
of the IGY
PERIODICAL: Geoniagnei.izryi I aeron,)Tniya, V. 1, 11(). 72;D
TM: The alithors in-if!stigatr-d Ltie distribiAt.1cr., cf bia-~?:,-.~Its from jata -1
41 ionospheric stations on the northern nemispnere. Tic m-rLxi,77,jr,, of blla,7!%~,j~ re-
currerce was determined for each staticii ditiring the winter, summer and
Of thE IGY. To reveal generDLI regulari--,ies of blac?ou*:; maxima isochrone sy~tfpml~
were plotted arid m,,axirmxn rec.irrence was registered from -data c4' thie !~-Y. Ir.
geoma~;netic coordinates the isochrones Df maximum recurrence for al-I ~-easonz -were
ovals. whose shape was controlled by the zone of a,.irona poia-ri3. When ipproacnirkg
the p~)Ie, the time of the =Lximurn is shifted from the night to the day hc,~rs. 11,
polar coordinates (local. geomagrk,~tir ~Imx~ qeries as azimuth cLnd tr,e
magnetic latitude as it radiiis) th,~, dep~-rideneo of th,~ tinn- of blaci:rol'
maximim on the redu~,ed geomagrietic la-11.)Nde has a spIrall shape. Ik compzu-1,io-i wttl,
analogous spiralshaped distriblitton3 of' magnetic d~lriilg
Card 1/2

.3/6 IAO'
Diurmal vari:tf-.tOri3 in the occurvt~n("e (W... A / A 10
seasons within -,he sumo- periorl ot ttm*- s-icms, Lhat the max-'rmim. of
on la+lt.lide pl = 6C0 1 5 hY ? 3 ~---rs t-i advan.--e of '~h- maximum uf
4.
currenc:e . 1A I t*r. tie d~'j 01 1) 1 1 k ()'J j I-, j,
The r:-y ',ho~ pr~?,,ent' ;t,idy a!'-l (,r.
previous data; this io possitiLy r17 r-:- trl~- fa--T~ -'Ilrlt Inagrie'Ic DLnd
ser-llat:.on~3 i'vorr. lit-le-ren, t-.acl heen : c,r.-.T-)a red
and 14
PO S 0 C 'I AT 10 1; : 1 n F, T: i ZTP.-I i oros 4: 'F- ry r va
.kli Z:')-'p (.I-ls- i I- L? 'DJ r ! d 1 1-:
-'irnl C)~ hadr)wav- A -
S 'J'11111 7-
Card 2/c",

S/20,3/6 lt,)O' /00~7,/024/028
A T'r f C) R S B(, n' ko v 4, N, r. , F 11 ge M. D.
T-1 TLE - Ionc-sphevic li zturb9naes on November 10 17, L?;O
FEB-.0D:,7A'-! Geomagnetizin I aercnr~nilyn, v. 1. no. 1'J61,
7~XT . Data obtained on m9gnoto-lonosrheric di,:;1-urbsoncPs :.n "JY 1959 were
(~C,M,-ared with disturbances of November 1960 and concl,.isloriZ wert-~ drt~v(n c-1 *-hr-
z~re2tr%m of gec-effective radiatic-n of the Sun and the. natare j.,f dis,,-.,ftances.
'11-.e ~ji-'-tributlon ol absorption in the Ionosphere fr(~rr, datsi of Zt s~atinns i~~ ce-
preStented In graphs, Which 3h-DW algf,' changes in the average values of tha,
H-ccirponent of' '1,he geomngnetic fleid in Moscow, the rr,~rent,,, of'
flares and the sudrien -oa=ence-ment of magnetic stcrmq. 11. was f-irld thal~ cl,,rr;mr)-
slpheric flare5, accompanied by a h1gher intens-1-ty of ;~.smic radiation, entailed
at--orption of the !--,I order wnlen wis caused by par'.11cleE with a!,, energi of se-
veral dozens of megaelectron volt. In spite of the high g~-:-eff1:1.enc7 of the
flares on November 10 and 11 (Ultravlolot radiation, ralic raalsallon and
cular 5treamz;) fast and cosmic particiea were appare.,-tiy ~-o, g---n?rat,,d in then
(-i~tlh an energy of ten megaele..:tron volt and more). Vhen x-.~lyzI,-ig, tale 1,-.tens,-,.y
~7ard --12

Ionospheric disturbance2
S/20)/61/0`1/30~ lu24/0~-
of ~~rrz-j-z~ular ra~lia , lon, of tne~c t'lhrr-s an at '.emp~ made c,!' 1v 1,~; a t 4 ,,.g .,- e
,c~outhern '~-oun arL,7m~~ of tne penetration zcne c." cc~:r~,-;.qc ~en Crcm ',he magnit,--do,
D-, varlallon-z, )!' the geomagnetIc fleld. For the acljv~, parIC-i )f N,ver-'-~er 12,
va.!--e,- calculatei varied frcm ')3 '~:, 60~1, whilsT, th-
at-*,,tined 46 G. flere q:-e 2 figure::, I tar-E arA
Sov.e*, and 2 ricn-Sovllp- ', -blu--- .
A S: NT - lnstitl,,~ zpmriogo magnet!.zma, lonosfery radi~-v--.'n
AN SSSR ( of Terrestrial Mawn(-*ism, Er~ ani~
watior. of Rad!~~waves, AS IJ33R)
SUDI-T 7~HD,~ A ugu,~ t I ~ 1 9f.,
cl"l-d 2/2
I

S12J'~/6 1 1 27/D29
A,~,6/AIiJI
AUT'HO'113 Be r1 T-a-bin, Ii. L. , Flig,7?1'
T I I L:-, Solar -adioburf-its At 28 M-i,,acycle 12, 1 ~'I
PFRINICAL; G-o-;agnetl-m I afranumiya, -.r. 1, nf). ~11 jt)~'J'
TEXT, Co5mlc radlo-emissfan at ~,8 Megacycle "requency L.,3 vejtiarly re?ccrri'd
at thE' Ionospheric department of UMIRAN for the puryos--~ ),,' st~idyirig ionuspheric
absorption. An a-alysis of the recordings showed that in sxie cases efircmospheric
flares caused a greater Intensity of signals, which was particularly high during
the chromospheric I'larv on July 12, 1061 . The data ::-ecor%1vd show thaL the chromo-
spheric I'lare was accompanied by vadlobursts of type-3 Il and IV wl.ich were Strong-
ly di,"ferent as to tirre and nature. During bursts o1' type II And IV, the l1adio-
rad'.a-.1on 'ntensity Increased In the centimeter, met.;- and 50 1,1ega(-yclP rangf,
meters) . This Cact does riot cont 11-n the concept Una!-, the SPOCU-11171 Ot' type 11
bursts rapidly decreases with reduced f'requency. Th--~ different nature or' radlo-
radla"lon during Il and TV type bursts confirms E.I. Mog1'-,Pvs?iy's ~iypot~lesis Oil
dif,"erent mel~hanl!-,ms of gonfvation: plasma, In th,, ,jolar atrrnonphe:-
Card 1/2

S/2()~/6 1/~,O -VU27/028
Solav vadiobursts at 28 Megacycle frequency ... k-,;',6/A 16 1
In the case of type 11 bursts, and sync hr-) tronou s radiatlon (,f rclat~vlst!'7 elec-
trons In the case of type IV bursts. Diere are 1 I'Igi,re ani 2 S,),;I(-t-tloC
erences,
ASSOCIATION,, Institut zemnogo magnetizma, tonost'ery I rasprostrareniya rajtovoln
AN SSSR (Institute of Terrestrial Magnetism, ionospl-.ere and
gation of Radiowaves, AS USSR)
SUBMI'r= September 11, 1961
Card ;?12

BENIKOVA, N.P.,, doktor fizikc-mat. naukt otv. red,.; SHAPIO, 3.S.p
otv. red.; GANGVUS, A.A., :red.; SIMCMD), G.N.p teldin. red.;
SINK121, G.S., tekhn. red.
[Papers )Sbornik statoi. M)skva, lzd-vo Akad. nauk SSSh. (Ro-
rulltaty inalodovanii po progra=o Mazhdimarodnogo geofiziche-
skogo gods). No.10. [Ionospheric studienllonorfernye iosledo-
vaniia. 1962. 154 P. (1-URA 15: 10)
1. Akadeniya nauk SSM MezhduvedomotveruX~ry -eofizlch,).qkiy ko-
r-itet. V razdel prorr,=y XGG. Ionosfera.
Mnosphoro)

BZNIXOVA,--N,P.
Oonference on ionosphere, Goofia,biul. no.1204,-56 162. (MIRA l6l5)
(Ionosphere)

MN I KOVAj. N. P. - _ -
All-Union Conference of the Ionospheric Research Section
of the Interdepartmental Geophysical Cozaittee, hold at
Ashkhabad on FebruarT 19-23, 1962. Geozag. i aer. 2
no-3:577-578 My-Je 62. WIRA 15:11)
(Ionouplieric rosearch--ContTes3ea)

SI") 03/ 62/002/0 04/003/ 0 1 B
.5on lkovi, nrid Tyurnimi, L. 0.
'I
-,o mrnot., fifil, of the equa ~or Ial ciari-ont
p. 7 Goorrjignet'.zin 1 novon=17tl, v.23, no.4, 1962" 635-641
_11-1 I~hc, alith,-rn calc,ilnto thti mqgnetic field of the equatorial
c-=-rent rinj7 for, any pa!nt on tho surfade of the earth a in
thW_- thin wirrort f lovis t on[-, jurf--,ce shrmod iil~o the forca lines
of the dII-Jole field (r a nnd -)os.Ltioned symmetricall-v
,..,!1.h rezr,ect to the ua~iator. Lgroement botwean the theoretical re-
.9ii:_t.3 nr~ the exporlmont,il lat..t-j6e distribution of the geomfignetic
%mrintion 1.3 bost ob,,~'Inod for a current ring, ,-iith a
an,-: f -1, virront d ans lt~, j b - c cos2 The -,Agnetilc -mc.I"eAIU-~
(en1clilrAe~ tho . gnetic storm of june 1,
o fLh i~) v i rig ma
-.5 10 C;s n,7r,o-~:3 -t-ith th,3 result.-3 of other authors (-"e
0: E.:,7.%'ostin. The field, its description and Anrily3is.
A,.,1hinpton, ID47). (.,"of. 9: _'.I.Akasofu, J.Cain, cmd S.Chspman.
Cpi,d 1/2

--/ ""03/ 6~,/ OO-,,/004/,3c3/-DltcI
1046/1242
Ic C'1-01(" of ...
-'.013-40P6). 71,J concluslom ::on-
firm oxtra.onosphcr-!.c cli-ront t,.-:o
radiation beltb a F, (tho outer bolt) and a = 0-10 R (~tha
outF,rnost, or t I"i ', r1) (-,- '-'hcra are 2 figures find 3 table-.3.
IISSO'IATION: institut zcmn~)j-,k) msgnetizrwia, Lonosfary i riisprosstra-
neni-vu rndi'ovoln A.N S'-,SR (Institute of Terrestrial
...-gnetlsm, tho 7onosphere, nnd rrop!igntion of Radio
Wavej, Af,
S T 7n 1-17~ in: A or
6 2
-rtrd 2/2

-RE114KOVA, N.P.
Conference on the ionosphere held in Nice December 11-17, 1961.
Goomag. i aer. 2 no-4:79,4-797 JI-Ag 162. (WPA 15zlO)
(Ionouphere-Congreaves)

ADAI-10 N.V.; BENIKOVA, N.P,; ORLOV, V.P.; 031i'OV, J.K.; TYMMIN L 0
A.P ..
Spherical analysis of the =stant magnet ,Lc field for the epochs
1955 and 1958. G3omng. i aer. 2 no.5:91+9---962 S-0 162.
(MEIA' 15:10)
1,, Institut ze=.:)go magnetii=, ionosferir i rasprostraneniya
riLdiovoln Sibirak-3go otdel,3niya AN SSiR i InatitLIt Matelnatiki
o vychislitelIrqm tsentrom Sibirskogo otditileniya All SSSII.
(Magaetism, Terrestrial)

BENIKOV,%, N.P.
Sixth Corf,3r#-.rjce of the PmurOi Com.-jinslon of th(: IrQ!rnational
Advisory Counittoo on Vndio (hold in Gpnova from Jum, 7 to 23 ,
-5:3017 'j-0 '~~2. 11 1(,)
1962)). Gcomg. i aer. 2 no (,,!X, 15:
(Ionospheric radio wave propigation-Corgre.9r;es)

BEN I I',, V". N' P,
Studief; of the ionospherc., Vest. AN IfISSR 32 no.6,.I-".-lj2 Je '~;2.
(mIRA 15:i-
( Ion o sphe re-Congre oo es)

:KHMSTIKOV, I.A.; BENIKOVA N P doktor fla.-maten. nauk, otv. red.;
Y.T
MIRTOV, B.A., and.viz.-natem.nauk, otv. red.; IERLSTAX, G.V.,
red.; ISAKOVICH, T.D., red.; PODCL8SKIY, A.D., red.; FDLENOVA,
T.P., takhn. red.
(Fapers ISbornik statei. Moskva, Izd-vo Akad. nauk SSSR.
No.ll[Physics of ozonoopttere and ionospherelFizika ozono-
efery i ionoefery. 1963. 662 p. (MIRA 16:2)
1. Akademiya nauk SSSR. ?Iezhduvedomstver.nyy gfofizichfiskiy ko-
mitet. V razdel programmy MGG.
(Atmosphere, Upper)

~j *, / ~ /v t I, /~ , 'A/ .11 311
kDAM, N v , BrAqvA, w.p., cnov, v.p., osTpov, m., rtvQTXA',' L-.O-.
-- I
C&ICU]Atgd 1Mgn4t1O field Of the Earth, (USM)
report submitted for the 4th International Space 3"Itenee 3yuposhm (OOSPAR)
Warsav, 2-12 June 63

h521h
3/203/63/003/001/oil/022
106 1/k1 26
AUT1,1ORS z Vasillyev, K. N.
TITLEt The Z layer in low latitudes as investigated on the schooner
"Zarya"
P-WRIODICALt Geomagnetizm i aerono;jiya, v. 3, no. 1, 1963, 68 - 93
T-'- XT -. Ionospheria observations, in addition ~Lo geomagnetio measure-
Ments, were conducted with an AMC (AIS) ionospheric recorder on the non-
magnetic sonooner "Zaryall in the Indian and the 2acific Ocean in 1959 -
- 1960. A report is given of the analysis porform6d on the results. The
latitude di3tribution of the f 0E layer at all hours of a day is described.
Special features in the equator region (ledsening of the f 0E layer in the
region of t*-,ie geoinagnetic equator) are shown to become more manifest in
ti-.e morning and evening hours, and to smooth out at midday. The daily
course of tne f0E layer can be described by the formula f 0E - K coon .
n differs in the morning and evening hours. The "alue n in the oorning
varies appreciably with the latitude. It is a maximum at latitudes of
Card 1/2

A
S/203/63/001/001/011/022
The i~ layer in low latitudeaft..'... A06-i/A126
200 and a minimum at the gdographic equator. The-re are 5 figures.
ASSOCIATION: Institut zemnogo magnetizma, ionosfery i rasprostraneniya
radiovoln AN SSSR (institute of Terrestrial Magnetism,
Ionosphere and Radio Wave Propagation AS USSR)
S UBM.-L TTED iJuly 27, 1962
Card 2/2
MEN

ADA14Y N.V.; BENIKOVA, N.P.- OfW)V V.P.; WEAN, N.K.; '17AMKEU, L.O.
- .9
Spherical amlyajo of the constant geomc-~gnetic field for the period
1%5 through 190$. Pt. 2. Geomag. i aer. 3 no.1:121-126 Ja-F 163.
(MIRA .16:4)
le Iwtitut zemnclgo maumetizmal iononfory i raspvos~raneniya radiovoln
AN SSSR i Insti~ut matarLatiki a vy0hislitelInym tsentrom Sibirskogo
otdoleniya AN &;SR..
(~4netism, Terrestrial)

ADAMP N.V.; BENIKOVA N.P.- ORLOV, V.P.; 051POV, N.K.; TYU',YPA, L.O.
. - - ---.P -I . I
Spherical analysis of thc permanent goomagnetic fiel,j and
secular variation. Geom.g. i aer. 3 no.2:336-353 Mr-Ap 163.
(MIRA 17:2)
1. Institut zemnogo magn.(,tizma, lonosfery I rasprostraneniya
radlovoln AN SSSR i Institut matematiki s vychislitelinym
tsentrom Sibirskogo otdeleniya All SSSH.

ADAM, N.V.; BEN'KOVA, N.P.; ORWV, V.P.; OSHW, N.K.; 71YUPLMINA, L.O.
Synthesis of the geomagnetic field accorling to the coefficient!]
of spherical analysis. Geomag. i aer. 4 no.1:151-160 Ja-F'64.
(MIRA 17:2)
1. Institut zemnogo magnetizma, ionosfery i ruBprostraneniya
radiovoln AN .1%SSR i Institut matematiki 9 vychislitellnym
tsentrom Sibirskogo otdeleniya AN SSSR.

ACCESSION NR: AP4043264 8/0203/64/004/004/0748/071,2
AUTHOR: Adam, N. V., Benlkova, N._P., Orlov, V. P., Oslpov, N, K., Tyurmina, L. 0.:'
TITLE: Analytical representation of neoular variation
SOURCE: Geomagnotizm I acronomiya, v. 4, no. 4, 191A, 748-752
TOPIC TAGS: goomagnotism, geomagnetto field, georniignetic field secular variation,
secular variation
A13STRACT: A study has been made showing that an arvilytical representation of the
secular variation (SV) of the geomagnetic field based on six harmonics, is adequate for
representation of world 8V with the same degree of accurary as world maps of SV compiled
directly from observations at magnetic observatories; it Is also shown that the analytical
method can be used for compiling maps of SV. The synthesis of SV riaps was accomplished'
using a grid with grid lines spaced 5' apart In longitude. The grid was somewhat more open
to the south of 60*S and to the north of 70*N. The values S X and S Y ivere derived using the
mean coefficients Sgn M and A hn M, ccimputed from S X' and SY in order to exclude the
potential-free part. In accordance Altli the assumption of the existence of an outer part
the vaLlues 4Z were computed using j j n and fKmu. The quality of the analytical maps
was judged byoompWng maps of the di7ferences eh, betweem. the initial values SX, 6Y
N

ACCESSION NR: AP4043254
and S Z used for analysis and the values obtained as 'a result of the oynthosis. Figures I
W 2 of the Enclosure show the IMILAN (Institute of T4-.irrestrial Magnetism, the Iono-
sphere and Radio Wave Propagation) maps of d S X and 4 S Y. The 4 values are given
In gammas; positive values are represented by solid and negative values by dashed isolines.;
The maximuxa discropancies between the initial and now maps, +30Y , was in the southern
homisphero; In the northern hoinisphoro they did not exceed +10)( . 'Cho discropancies in
X, S Y and S Z on the IZMIRAN SV world maps do no L have a rogul;xr pattern, except I
that in the southern hemisphere A J_ Y is generally negaUve. The val1jes,6SX and A 4 Y
are of Llic order of +5Y and only in the south polar cap do they attain 40'( for 6 X and 20Y 1
for S Y. For A ~ Zihore is an Increase to +15"y in the Atlantic and a sharp increase to 60-r'
in the high latitudes of the southern hcimis~hcre. The IZMIRAN maps also were compared
with the values S X, S Y and 5- Z directly at 63 magnetic observatories; the mean discrep-
ancy for the three element.9 was +91( *. 77he analytical method Is thus its accurate as graphic,
meCiods, but does not involve the subjectivism involved in use of the latter. However,
graphic and analytical methods could be combined; the first to beat for areas fo-t which little
data is available and the second Is bent foi; characterizLig regions of rapid s%ular varia-
tions. Orig. art. has: 3 figures and' 2 tables.

ACCESSION NR: AP4043254
ASSOCIATION: Institut zemnogo magnetii,.ma, ionosfery I rasprostranealya radlovoln AN
SSSR' (Institute of Terrostrial Magnetism, the lonosphore vnd Radio Wave Propagation, AN
SSSR). Institut matematiki s vy*chiolitollnym tsentrom, SCI AN SSSR (Imitituto of Mathematics
and llio Computation Center, 80 AN SSSR)
SUBMITTED: 04Fob64 ENCL: 04
SUB CODE; ES NO REP SOV: 004 OTHER: 001
Co;7d- 3/1

L 1892:&6 EWT(1)/FCC/1EWA(h) (W/GS
ACCESSION NRt ATS022835 Ult[OOOO/65/01)0/00010224/0228
AVMOR: Benlkgya. N. P.; LuM94ol'shava. A. H.
TITLE: VarikbLlity of ionospheric paramterg
SOURCE, Vaes-Dyuznoys soveshchant" Vo koamofiaLchoskeau nap~Avlsni
yu_-
Lealedovaniy cosifd 1W49Z_jLq'ks Yakutsk,, 1962, KosaftheskLye luc i L
rays and problems in costmophyafts); trudy sovesh-
chanLya. Novosibirsk, Redizdat Sib, otd. AN SSSR# 1%5, 224-228
TOPIC TAGS: I' layer, statistic distribution, critical, frequency, ionosphere
ABSTRACT: The variance of hourly values of the critical frequency of the 72 layer.
F2, was determined from the formula for a normal distribution:
where;k and A, are the upper and lower values and a Is the median value of a
u
given parameters and the formula
m) (in
Card 1/2

L 1899-66
ACCESSION NR% ATS022835
was used to find the deviation of the distribution from the normal distribution.
Datat cbtained from vertical sounding of the ionosphere during the ICY. t the
a
Yakutsk, Yuzhno-Sakhalinsk, and Tiksi Bay stations were employed. It is found
that the variance of the hourly values of the ionospheric parameters relative
to the monthly median is largely 4,u4 to a regular seasonal change of the
paraneters. The characteristics a and 6, calculated from the quartile values
of th,e parameters, characterize the general variability of the ionosphere 4"
can be used advantageously for practic&I calculations of the range of Working
frequencies and other practLcal'problc=s of radio communications where possible
deviations of ionospheric paramters from monthly median values met be evaluat*4
Orig. art. has.- 5 figures, I tables and I formulas.
ASSOCUTION, Institut xemogo mqmtLxma L ramprostrananLya radiovoln
(Institute of Terrestrial Ma"tLsu and MAdLo Wave ProjiAption)
SUMMED: 290ct64 IIN04: 00 SM COM ES
NO RU SOV: 003 MUt 000
Card

1jr VU _q:kYGD
Acc NRt 6 0 5M SOURCE CODE'.-i~k/6CU076-.V[6o-oToo-o7o-o!-BT6-oY3-,,,
AUTHOR: Adam N. V. ; Ben'kova, 'P. ; Orlov_,_V. P. ; Tyxumina L. 0
ORG: none
TITLE: Secular variationa of the field based on data of a spherical
analysis
SOURCH: AN SSSR. Institut ' fi'ziki Zemli. Nastoyashcheye i proshloye magnitnogo polya
Zemli (The present and past of the 4&rth'a magnetic fiald). Moscow, Izd-vo Nauka,
1965, 18-33
TOPIC TAGS: earth magnetism, georagnet.16c measurement, spherical analysis, Gecular
variation
ABSTRA,-,r: This article concerns the principal geomagnet1c field stulied by tile method
of spherical analysis and its secular variations. The authors deriv! an analytical
expression which approximates secular variations. They examine an the basis of this
analyti.cal expression certain problems of the nature of secular variations, and
attempt: to use the results obtained for forecasting the field. The authors, having
previously used spherical analysis for plotting charts of isoporic lines in the polar
caps and having obtained sufficiently good agreement with charts plotted from obser-
vational data, conclude that the sum of-'the first six terms of a'spherical harmonic
series permits representing the morphology of secular variations with the same degree
Card 113

L 10913-67
ACC NRz AT6021011
of s0ematization. This scheme is characteristic of r.,odern world ii;oporic charts
plotted graphically from the data of magnetic observatories but without the element
of subjectivism inherent to the graphic method. Spherical analysis is recommended
both as a method of analytical representation and as a method of plotting isoporic
charta. Since one of the important characteristics of the planetary part of secular
variai:ions is western drift, the authots estimated western drift for individual har-
monics by means of spherical analysis of a constant field and secular variations, and
by the shift of the centers of world anomalies. They also examined the latitudinal
and longitudinal distributions of drift velocity. The velocity valLes obtained from
the coefficients of spherical analysis of world charts of the total field for the 19551
epoch,, and from the secular variation charts for the period 1954-1959, are calculated~
The velocity values were found to fluctuate within -0.47 to +0.12 deg/year, two
characteristics being noted: 1) a decrease of the velocity for high-latitude obser
vatories and 2) asymmetry in the distribution of velocity between western and eastern
hemispheres. The velocity values were higher for western observatories than for
eastern. To eXtrapolate secular variations to the present or forthcoming epochs, iso-
poric charts of 1954-1959 were used to forecast the 3ecular variations for 1960--1965.,
A comparison of the coefficients of the spherical analysis of secular variations re-
vealed that, with the present accuracy, the coefficients higher than the third order
can be conside:,-ed constant, and the coefficients of the first three orders change in
time within a net interval, fluctuating about averages that are constant or almost
constant in tine. It is concluded that during a 50-year period the-nagnetic moment
can decrease by 0.5 . 1025 CGS, and that the position of the geomagnetic pole will

ACC NRI AT6021011
0
shift along the latitudinal circle from 291*46' to 291"52'. Combining palcomagnetic
and analytical studies of the geomagnetic field can be quite fruitful, in particular
in regions west and east of the centers of world anomalies. Orig. a:rt. has: 3
formulas, 6 tables and 6 figures.
SUB CODE: 12,08/ SUBM DATE; 2lSep65/ ORIG REP: 007/ OTH REP: 004
3

L 071.91-67 z.,V111KC
A=NT7=602101 SOURCE CODE: UR/0000/65)'000/000/0033/00417
AUT110R: A am N. V.; Een'kova N. P.; Orlov, V. P.; T~,,turmtna, L. 0.
ORG: none
OF
TITLE: Calculation of the ge-omagnetic fteld atrength based on the coefficients of
spherical analysis
SOURCE: AIJ_5SSR. Institut fiziki Zemli. Nastoyashcheye i proshloye z1agnitnogo polya
Zemli (The present and past of the earth's magnetic field). Moccow, Izd-vo Nauka,
1965, 33-41
TOPIC TAGS: geomagnetic, field, geomagnetic measurement, magnetic field intensitY,
cartography
ABSTRACT: This article is devoted to a calculation of che geomapneti.: field strength
based on the coefficients of spherical a-aalysis in ordez to obtain ini-ormation on the
distribution anti character of the change of the geomagni!tic field at farioua distances~
from the earth's surface. The first step in this work was to determine the coeffi-
cients of a spherical harmonic series in order to calculate the geomaj;netic field in
circumterrestrial space. The starting data were the maj:-,netic charts c-f the MIRAIN
and the British Admiralty for the 1955 epoch and the values of the maFnetic elements-
at unevenly distributed discrete points. A subsequent tiynthesis of t~,e field on the
earth's surface and its comparison with the starting data showed that the beat repre-
Co.rd-

_L 074gi-67
ACC Nit, AT66il6if
sentation of the field is given by the i:oefficients calculated with respect to world
charts. The elements X, Y, Z were calculated by the Fjmn of the first six harmonics i
for a network of points 5* with respect to latitude and 15* with respect to longitude.i
The coefficients obtained from the MIM charts were used for further calculations.
It was found that spherical analysis carried out for world magnetic charts gives an
analytical representation of the distribution of the field on the earth's surface withl,
the same degree of flatness and with the same errors ati the world magnetic charts on
which the analysis was based. Spherical. analysis offers a sufficiently simple and
easy method of calculating the magnetic field and its gradients for large heights.
The absolute errors of calculation decrease with height in proportion to (a/r)3 or
even more quickly, but the relative errors remain constant or decrease slightly. Tak-;
ing this into account, as well as the rapid decrease of old harmonics with height, the,
authors assert that at large heights the series of spherical harmonics provide a high 1
accuracy of approximating the magnetic field sufficient for various problems of inves-1
tigating a constant field and for interpreting satellite observations. An analysis of
the 1955 IZMIRAN charts confirmed the systematic shift of the earth's magnetic center.
The theories of the origin of the geomagnetic field scarcely touched upon the problem
of the eccentricity of the field and the authors wish to call the very fact of eccen-
tricity mid the systematic shift of the magnetic center to the attention of theore-
ticians. The representation of smoothed world charts by series of spherical harmonicsi
up to the sixth order is not, in the opinion of the authors, the limit of what spheri-1.
cal analysis can give. With a sufficiently large number of observations pertaining to' F_
one epoch, a spherical harmonic series can provide a more detailed picture of the 1
Card 213

r; I I
3 tables, and 4 figures.I
i
: 004
i
I
L
i
I
-L 07491-67 . - -
IACC NRi AT60210.12
- . . - I - 11

0_2 TT/(,W
E,,r(1)/Fr_C/FS`
?6oo -5/00h
ALL NR_s_AF'Ol: SOLUCE CODET U10293161 /003/01463/0L6
AUTHORS: -Adam% N.V.; Ben11cova,_',1. ~.; Tyurmilia, L. 0,
ORG: none
TITLE: Geo gnetic mav construction from satellite data
SOUi-1'CF,t Kosmichoskiyo issledovaniya, v,. 4, no. 3. 1966, 463-468
TOPIC TAGS: geomaLpotic measurement, goomagnotic field, harmonic anal is, a="xMMPz;;Lr
Saba! i6a absel latiol CA"-to ~ ^4L~ 1
ABSTRACT: A =t? is presented of the total miagne~ic field_._inte_nsit,f at 4,00 kn, over
the Soviet Union. The data for constructing the inap wcro obtained from measurcnonts i.
from the third artificial earth satellite (195b). The measurement:i were reducea to
the value at 4C0 km according to the formula
AT
T"* Th +_~h_ (h - 400).
An insufficient number of measuremento iaa made to obtain the verbical j;radient
.',ATIAK directly. Consequently, tho 6radients were calculated ort the basis of F_
spherical harmonic analysis of world magnetic maps (1955). Detailji of the analysis
and the construction of the map are C'~ven, and the accuracy is estljaated to bu 350 Y.
Orig. art. hast 2 figures, 2 tables, and 6 formulas. [04)
SUB CODRt 08/ SUILN DATEs 17J,pr65/ ORIG R&F: 00 REF: 001/ i
ATD PUSS:t; TV OTH
Card 111, .L,_550-3 2i528.Q67-4

L 23136-66 EWT(1)/FC(* GW
ACC NRt AF'6006677 SOURCE CODZi UR/0203/U/006/001/0179/0181
AUTHORS: Benlkova, N. P.; ~4avtj A,,; Tyurad L. 0.
ORO: Institute of Terrestrial Ma netism, the
Wave.g,,_A.4 �Pi (Inatitut zemnogo magnetiamaj, ionost'ary i raspro;Ptraneniya radiovoln
AN S,~~R)
TITLk:t On -the accuracy of analping worldwide Mp.jUc~'~aps of 1960
SOUFd'$Ei Geomagiietism, i aaronomiyat vo 6, no* 19 19,569 179-181
TOPIC TAG3z geomagnetic field, harmonic analysiaj research ship
ABSTFAM Distribution of total magnetic field was computed through coefficients
of spheric;d. harmonic analyses for 1960, Different combinations of apIlerical-
harmonic coefficients were used to compute for each of We b1troa rectangular
coordinates of the field. TheoreticiLl values of the field were -then computed
according to, each sot of coofficAentv. To avalmatm the accuracy or this approach
by spherical harmonicaf corq>arisona were made between the values obtained here
with values taken from worldwide maignetio maps for 1960. Checks were mde of evaz7
Card 112 UDC# 550-389

L 23136-66
ACC NR, Ap6oo6677
5* of latitude and l5c of longitude, Comaparisons woare also made with data from
the Zarya for the Pacific, Indian, and Atlantic Ocomm for the period 1957-63,
reduced to 1960. Checks were made at 372 points. ';k"he theoretical value3 were
also compaxad with average values from magnetic obss)rvat oz. Variation in
fielil (for horizontal coinponent) waa computed to be 260 Of. was Reasured as 2861
on the Zarya, and 290 rat land observatories. The difference btitween computed
values and the Zarya values for the points of comparison are plotted on a world
map, and isopleths of difference are drawao Orig, art, has 1 1 figure and 1
1 tables
SUB CODIs OQ/ SUM Wls 06Jul65/ ORIG RZFj, 001
Card 2/2

PETROVCIC, Ferdo; BE21YOVIC, Bianka
Gonad dose exposure during diagaostic procedures (menuurement). Rad.
med. fak. Zagrfib 8 no.2:188-194 160.
(RADICIIETEr) (IONADS radiation eff)

BENKOVIGF--1--L4-
Ltributione toi sequelae In the bass of the skull with special
reference to thig sella turcica. Rozhl. ahir. 40 no.11:743-747 N 161.
1. Uinilm nemooi nervoyeto eyetemu Luganskeho statniho lekarokeho
Inatitutu, reditel kliniky prof. I. L. Bankovic.
(BRAIN wds & inj) (SELLA TURGICA wds & inj)

dElVeOVIC. -)
IKIC, D.; B W OVIC, J.
our investigations on the veaue of various types of anti-ty-phoid
vaccines. Actn med.iugosl. 9 no.1:38J~4 1955.
1. Centralni higiJanaki zavcd--Zagreb.
(VAccimw AND VACCINATIONS.
typhoid vacc.siqmr. of various types to determ. choice
vacc.,results (Sor))
(7Y'PHOID YNER, immmiol.
vacc..exper. of various types in determ. of choice
vacc..results (Sor))

:k'KIC, D.; RXIMVIC. J.
Anti whooping coik,:h vaccine prepared by viirious methods, expe-
riments on nice. ixta moMugael. 9 no.1:46--53 1955.
1. Centralni Higi'.enski savod--Zagreb.
(Y/,C(,*INM AND VACCINATION,
whooping cough vacc.,variedly pripared, exper.eff.
detorm, on vice results(Ser))
(WHOOPING MUGH,
vacc..varledly prepared, exper. off. daterm. on mice,
resultu (Ser))

-f.,7 3 L,'.V IA 7 ic ro b io r
!
lo

m;,~ P, inz.
.1., 1 ,
-..-T , ".." .:
pro*t)l. ~_,; of 'i_ ! III:' P!l ~ -"' ;~' ;;" i - - -
Lj,,varst,vo nu,1/2:11) ... 1"'. 1;~')
1. 71 ":! . T~", -,

KISS, rorant, oklovelea geposzmomok; CSERDAVOLGH, Laszlo; HAJDUO lBtvanj
BEIIKOVIGS, Jozeef; TWYAK, Bono; SOSKUTI, Andras; TOROK, Mihaly drv-,
-SUTt- F~rl gayes; GATT, Geza.; KOVACS, Iajoa; rEIM~F.S, Zol';ar.; MAG--
Laszlo; KOVACS, Gyulal AUETSWALD, Jaronj 30S, Jams; D'.:OSZEGHY,,Dmielp
prof
Manufacture and use of gan appliances. Energia es aton 17 no.1%
30-35 Ja164-
1. I&npagyar (for Kins). 2. Vegy-terv (for Csernavol.gy-i'l. 3. 0-r-
szagos Koolaj- es Gazipar.1 Troszt (for I!ajdu, Szas2r, Anerswald).
4. Pecsi GazszDlgaltato VaIlalat (for Bonkovics). 5. Airvanyolaj-
forgalmi Vallalat (for Terr.yak, Soskuti). 6. Epitesugy-; Minisz-
terium Iparterv 1-kiszr'ci Omftaly (for Torck). 7. Orazagos Villa-
moserergia Felugyelet (for Gati). S. Epitesug,~i Ilirisz-xrium
Uor LaJon Kovacs). 1). Ga-,keszul6kgyarto Valialat (for Delieres).
10. Epitestudoriayl Intezel~ (for Gyula Kovacs).

SZUCS, Miklos, dr., a kemlai tudomanyok kandidatusa; SZASZ Frilryes;
IMIYITAI, Janoso dr.; BAVJS Jozeef; '7ACIMMSZKY, Ferenc;
GULDEN, Otto; TEMIYAK, Berlo; MK", Jazaef; DIOSZEG'3Y,
Daniel., prof., dro; TOTH, Istvano
Questions of vocational education pertaiiiing to the gas in-
dustry. Energia es atom l! no.10-11 Ja'(4.
"0 Fovarcoi Gamnuvek (for Szucs); 2. Orszagos Koolaj- es
Gazipari Troszt (for Szao:s and Bunyital). % Makolel tle-
hezipari Iliszaki Egyetem (for Dioszegh-y).. 4. Voszpremi
Vegyiparl ILsz-aki Egyetam (for Toth).

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BE,_K.Xi~;: I . L Glinic.-I ririnifi~rtrltlons of trp-tunA of tht! Pnterior nortion o-^ t~o
Yline f skli-11 Problems of Nouropoir,,ar, Mos...
0
The rirst -)p-tient, ~L yerr old, -hot himpelf with P. revoltor. He r un c o n r c * iu r
f o r 6 dv_', 9 . ~7ubre ,ue tit 1,~, the -e wafl .rin sm in on the ot~riln on the ler-..
.311riteraily -.,Pre Mindriectr w1tKout ,upIlInr re,,cti,--n to lij,,ht (t:e o tic
nerv,,r z)nrn1yq1q of thr Ird, Lth nrid 6t-, nerves, Ard ~tzuiesti.psin in
the ilistributiin of the l9t dlv',~~on of thP 5th nerves. X-rayr, -howe!' thfk-, ~rhe
r d entered throu.~', the ,-~nmonr, !)ortion of t:,.e rlr'~.t 'e-norril borle: it
billIpt ha I I
Tiroduct-O two ja~7red chrv-:~elq ench a7mroximiltely o.ox lcm. in dittmeter
the ~odF if tho sn-enoid In front of the nie of ti.e tintorior clin,)ids antli iind
finally lod.-PO in the r.nterior nortion of tr,,o left zy-.,m,4. T'-,o C_-F war, norwil ur.d
the nreumoencei~,rilof,,rilm %nf~ withnut glgrilfirAn ab~,ortnallty ei~en -)' the ba-ril cigtorrip.
After 6 there was no ch~tnpe but 18 manthc Inter Dtopir war, le,;- rnd t'np-e
wrie-. qome ,ctivp m,)vement of the eye-3. The serond man, ped :)I, -1i,) ed ~,.nd fell
while c.-,rryinp a 75 k~~. bale which frrictured Mq He w,.r, urlnon-ci-~llr for
2 hours --ne. blel; frrm 1. ~~e ripht ear. '~ubrequpntly, wit'l-, t'np ri;-:.,, e.;rp ~.p (41!ifly
the outliner of objo~,,t~~, (t~-.e nevve ecume nale). Also )n r!p'-,t the-e
com-)Iete o--)hthalmo,)1v,;-1n witi,. plosin, absence of corre.11 refleyor t7en~ptior, 'In tae
1st diviriin o~ the ~,.Ui no-ve arid uerrioheral t,,-Pe of 7t,, rierve oaltv witi,)ut lorr,
of ta,7te. The rie-ht Pir i,rum witn runtured. A-P )[-rays showed fr. rtureq of the n -er
lpteral i)ortions of rii-,ht o-bit. Two months Inter ti.e lid coald ~.e rRised
T'.-p next and ELd('uc'1o:, the eye were
seen and 5 dayF lpter abduction, In 3 more days Rellic w~,_, 1
~, 0 1,71ted. ~th
nerve furi~tlin ret-irno(' t-, normal FAnd the 5th lm-)ro-wed -11 -htl.,.-. T'he o )tic-- rita-rve
remaine" unchringed. T I.-I'er' lake- C; - , bri d,,-e
S`/: Neurol.ogy & PoYchintry Section VIII Vol D No 7_1') nec. V111,11)

BF'." *,()'FjCff, T. T,.
Renlimich, I. L. -- "C'Inliml dt-ip,-)-I~ of tr-lim-it.it I-, t~,~ "r-ritnI f7ranlrtl
.7 neyro~.-hi virg-i I , 190, lo. 3, n. 5 '-60
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Ti -lu- I e Tnvr):-; biir~i f' on -)r,
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Abs Jour ROf I., I
Abstract 1:5,MO nnA kept in .-. so 1,1 t ~-*,. ono
1:10tOOO (1V); killed at relfri; er-ituion
temp,rature with a SO,, L-on of :--~erthio-
late 1:10,000 I-ld T).-C:;(~I-VeA -It, thl-~ r,.-IT7,0
temper"Iture (V); killed
by means of ultrisc,,i,-.('[ and pre.-,~,inred in
physioloc-ical solut-'cn (V1); mic--obes
were lrill~,d -aituh 75" alcol' ^0' and i-)re-
'0
serve,"I in 251,o' cllcol,,ol (V1--,); :Tiicrotes
were killed ait,,. aceton,_: e --v e d
in phiy~-,iolo,-,ic-il ool~it;Jc- (7111).
London pe.-tusz;is vacc:.n-2 lls~ld "3
control. Fourteen ','!~-,D mice
were infe(,,'U-f:,d b-,, iptl,.-.i.cereb--.,l --dmin-is-
tvation o' 100 DL5C). Of tl.~, l'or7,.,)l
Card .2/3