SCIENTIFIC ABSTRACT KALININ, Y. - KALININ, Y.
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S
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100
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December 31, 1967
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SCIENTIFIC ABSTRACT
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KALININ, Ye.V dotsent, hApd.tekhn.nauk
~M--
Study of certain regularities of a pulse discharge. Elektrichostvo
no.3:89-92 Mr 162. (MIRA 15:2)
(Electric discharges)
KALININ, Ye.V.; KARPOVA, 0,V.; TSEPAKINA, L.P.
Dependence of the discharge potential of wet insulators on tho
duration of applied voltage and intensity of the rain. Izv.
NIIPT no.8:343-350 161. (MIRA 15:7)
(Electric lines--Overhead)
KALININ,._Tq~,V+,_--kand.tokhn.nauk; KARPOVA, ON., inzh.; TSEPAKINAy L.P.j inzh.
Dependence of the discharge potential of wet insulators on the time
duration the insmUUirbeing subject to the action of the potential
and on the intenvity of the rain. Elek.sta. 33 no.2t5g.62 F 162.
(MIRA 150)
insulation)
(Electric lines-Orerhead)(Bleotric insulators and
khr niuk , fir),
1 .;7, it; in the ~;f tho rw~asur rient r-f' ii(.
Elektriclle.-Lw,
~6 (mllo.
inst-;-'at pcj:~t,,yann-~,go
tj~7 [i
ACCFSSION NR: AP50AO963 SIG 104/64100010169 /0068/00 73
AUTHCA: Kalinin, Ye. V. (Gambdate of technical scienctsm); TikhodAyev,
(Can-JidaLe of u, -tencea); Kalmar, 0. (Can-lidaLe W t!ch; -aj- sciai 4.
it I E;
Ko outova, D. (Engineeri
TITLE; Wflt flaorhover voltages of long insulallor itrings
SOURCE. Elektrichetrldye stantiffl. no. 9, 1964, 68-73
TOPIC TAGS, insulato,: ctring, flashover voltage, Lnoulax0e tesl
ABSTRACT: The results of wet flashover tests of superhigfi-voLtilqe SLring
insulators are reportE!a. A 2 x750-kv cascado traneforml-T !,11pplieli ~-7-orr, it
byrit;hronous generaEor was used as a source of. t4II&L Voluages. 5t.riniga
3v 10-32 PM-4,5 M.Suiatorfi and 12-30 F1-8,5 insu,144ora mere spray-lr. %inth
cherr..:ally purified uhtn-crn) water at a rp-tc of 3 mrnt,'miti legt~ml for
fiash:,ve ID tO DU kV. WAII-Ien--al dAa In tahulated. At Inno,-
----------
overs cascaded the string. At higher voltagoo, sonic ax-cs atrual: tk4e suppi:4,tinj;
steel gi.-der, awa frQm the string. at &till. h4gher vo~tape;,, Wheindily azd'Oelt
Y
flashover voltages came close to each other, pr act ic ally 41 &&O-.1irger occtiiriteAd
between the shield ring and the girder. It io con,cluded that: for
lir.es. the number of imitz in the string can be uelec-,!td on Ov~ bfullis of thia liry
flasaover voltage. Orig, art. haii: 9 figuires, 5 formnlas, and ii tabla.
ASSOQIATION; NJjPTj
NII energetiki ChSSR (Scientific Research Powcor- Mafomorlavg Xnat4l Wto p
SUBMITTED: 00 EKOL,: 00
7 7--,-- _77" 7"-i
AT4o45616
AUTHOR, 3ronfman, A. rX[ead of' high voltage- laborallorf);, KAU
_j44jjkx
date of technical sciencea, Supervisor of a sector of high ;~Ltlgo
Solomonov, 14. M. (Candiclate of teclucical sciences, Sonior rtseEmclt u9sociate
T1,rLE: Investigation of the diatharge cliazacterin tics uf rinitilmotic iomlve dischurgeo
for 500 lcv lines
SOURCE: Dallmiye elektroperedachi 500 kv (long-distance Crumsmijauticill Of 500 W.
electric powers; sbornfl- gtatey. Meacovi, ILd"vo Encrgiya, LIM4, IN)- 190
TCPIC TAGS: high voftage ljn-a,, powar tiae, ujeotrft,. power jr1wrisidigiolorg, VOINAge
overshoot, voltage discharge, magnetic vallre discharger. 1;1gjh,,1ninj4 at-"ster,
breakdown voltzge
AWTRACT: The discharge chnracterlatics of two, types of m.4;neiAe disehargora; umid
10 kv I fnw,, -ere iyn,eatigatod- the. lightrang arrester. demeribi-A -nin-sously by t",
.1 1., d ~ AA I I A,41~ 1,1, ni'd
. ..... .........
CoO
-,NR- AT4.045616
--...ALCCEZIO -- -----
thus necessary to favesUffato =id lbe natx!rt~ b lho vi*lag~eol zor4u
v"Joug Lileinfintg and to ascerWn that m cormt coordinatloth (Wa(lo betwem 64~ "-.41rk
-% uniforro, and tho vnifivirm arrami tho valve olomOlls. ;Sivelfivatio4mi caltl
----- ------
---- -------
Card.
ACCESSLOUNK: AT4045616
1250-1230 kv-0: The extol-URI inji of is nill, 60 1; v-~ tdtk* In iol*r
to prevent deterioration ofthe breakdomi voltage. OrIg. mrC. has: i:,1fcpd1cj11S 1104,
11 figures.
ASSOCATION: Vy*aokwrol'Way4 JaborMarlyet Mv4 t VOICq4I
Laboratory of the "ProleWriy" Plant); Viftokovol, Maya labortfort.,M fruIPT (111g1h
Voltage Laboratory of IMPT)
SUBMITTED: 13Mar64
ENCL-
EE
NO REF SOV: 006
OTHE-11: 000
Card 3/6
--ACCENSIOM.N.%.*:~ AT40-15610-i St K,
Ftg. 1. Simplified dlagi!am of a oombined- 500 kv die charger: I'- lighoing arrc4ttv put
(1-multiple spark gap, Z-large aottitnear rosistance, 11--tervitte noitflAeux
OJF4,ca,
JAW Am 1"'T 146v I &Iqi
0 KJ
I ,
YV 44,
Fig. 2. Probability of oporation of a IfghEafij, akrestar and tt MORIChI4, tirminiant
discharger at 500 kv anti coordinatiou of, their perform. amce M: Industrw
voltag-e frequencfea. I-brcakduom probability of lighmaull,* arnifiter..
~~ - t-~ r o;-~ h 1~ frw r, nrf-On ahl I I tv nf qwl tahl n fr ov n r s hq>j t di s v. h.arti va. -. 3 - Dif-chabil I t-
IT:
L 1,;
H 'I
14E
Jill
.7 :1.,
KALTNIN, Ye.V., kand. tokhn. nauk; KARPOVA, O.V., inzh.
Design of flare-type line insulatora and wat discharge potential of
suspension insulator chains. Elek. eta. 36 no.6163-66 A 165.
(MRA 18t?)
;KALININ Ye.V. kand. takhn. nauk
v
Construction of suspension Insulators with wedge-sbaped pins
and methods for testing tbem. Elek. sta. 36 no.2:63-68 F 165.
(KCRA 184)
KALININY YU.1 inzh.
Optical calculating machines. Un.tekh. 6 no.1:26-32 Ja 162.
(HIM 15:2)
(Polarization (Light))
(Magnetic memory (Chloulating machines))
IKALININLYu., inzh.; RYABOV, L., inzh.
Aimed into space. Znan.-sila 37 no.11:12-13 11 162. (MIRA 16W
(Antennas (Electronics))
KALININ, Yu., inzh.
Horse in the wind tunnel. Znanie-sila 38 no.ls8-9 Ja 163.
(MIRA 16:3)
(Wind tunnels)
AZERIIIKOV, V.; ARLAZOROV, M.; ARSKIY, F.; BAKANOV, S.; IJEIOUT.V, I.J;
BILENKIII, D.; VAIELI, I.; VLADDIIHOV, L.; GUO'HWIEN,
YELAGIN, V.; YERESHKO, F.; 7JIURBINA~ S.; KAZARVOVSKAYA, G.;
KALINB; , Yu.; KFIER, V.; KONOVALOV, B.; KREINDLIN, Tu.;
IX,13EDEV, L.; PODGORODNIKOV, M..; RJONOVICII, I.; REPIN, L.;
cNOLYAN ,
G.; TITARENKO, V.; TOPILINA, T.; ADC)OKO, V.;
EYDELINAN, N.; 2-24E, A.; NAUIOV, F.; YAKOVLEEV, N.;
MIKHAYLOV, K., nauchn. red.; LIVAIIOV, A., red.
[Little stories about the great cosmos] Malen41o rnaskavj o
bol'shom Kosmose. Izd.2., Moskva, Molodaia pardlia, 1964.
368 p. (MIRA 18:4)
'It P UIA VI I I fill] Ig I I !111111rim ! I I '!I! I 5if I R [it PII V 1-i I "wal IW,
Al L 2,3112
ACC NRt AF6001853 SOURCS CODS:
URTOR016510001009IM1810048
qUnginear)
AUTHORt uv 1, (Candidate-of technical sciences) n yull;
ORGt None
TITLS: A device for the purification of waste water
SOURCSt Rechnoy transport# no* 9, 1965p 48
TOPIC TAGSt water purification$ fresh water, water puzifl6ation oquiptwnt
ship, ship component
ARSTRACTs The Leningrad Institute 6f Water Transportatioti:(Leniin5lr&clskiy
institut vodnogo transporta) developed a new design of a Statidaril shipborn6'
device for the removal of petroleum products from the Ail)' s wasto wwer. ~ The
device, shown in Fig. I. ii-'designated'16-f-Diosel ships of the Irivix f leet4
The capacity of the unit.is 300 literAr.-,The device vras tested successf ul IV.
on'the motor ship "Sochi" (SZRP). and motor ship "Reshtui".(VDRP)*: Orig* ;exte
hast. 1 figure*
1/2 629,128t628.16,004
Card
113179-66
ACC NO' AP6001853
Figs 1. Block diagrairt of ilia unlfWd. shiptor"
device for the remoVrAl of iietrolowum product) Iro"
waste water (LIVT design).4; -- vmte waterii.-
separated petroleum products; -4 -, air;
outside water; I - pump with a Zt/lhr capao*,
pum dischnigI3
p = 2 kg/cm.2; 2 - water )el. p; 3
air chamber; 15 vaccum taxik; 1; -
valve; 4 kPA.
chambex, 7 - one way vaI6 8 - 'o6vir6a ptwffloa-
LI
tion filter-, 1) - coke Wart-,
10 petftle= layar;:
r
1 11 - ftm Pwffication filbar; 12 - vfvlod chips V6th
sawdust; 13 - purified watbr foftbe ship; 14- ~j
water over the side; 16 ~. witter kcam. over thts:
side; 16 - petroleum collocting ijuik.
it t; j.
-4F
ACCESSION NR: AP5008332 SAII 15165folaotool tooes(00011
A --'0 1: K ~- b;i - E- A I, w a k c.-., A. S. K -ii r, r i ku ii 'V. Kali oi!: Y A.
T- i 1) %f ;.5 1.1
SOUI-ICE: fzmeritel'nalya telcLnika, no. 1, 1765, 5-8
TOPEC TAGS: metrology, quantum radiophpsics
ABS'r"-'-T: A brief generaL revirw of the measuremerit: prohicri-is orcuri-ing in
modern devices based an quanturn-mechaltics phenomem-11 is pitevented. 1,111-6e
LLjp-,C!: --. f C tciuchct' Up-:n p rc,-- Li Lzion radk? apecil t yri' "i pma 1; ~- "i 1-'Aly
r
lu-ninesrence; quantun.,i paramagnetic ampli.fiern, weama ring W' Oiei-r piJim,
P. I a 1 1 pn,x,- (- r P- r, rt s i rnp c r itt i i r t, a -q e r aji d t lh&i: r it, i i f!. -'IIIC:
"'Id, ;j~ V'T' r --I I a. (i I fi el. Al I, Orig. -~.ri lilm -t,:
and no tabie.
Card
Card
F. '~, KA"I'll-,", ',u.A,,, E""MrCii~'V, V.M
..n L - 11
MoaEux-ing the ererej and power of opt-Iral qiiurtum
... 41 Fly 165. U-1:."F-fl, IS,
lzm. tekh. no.5s37 18"
L 22138-66
'ACC NR, AP6012935 SOURCE CODE.- X1R/03J-5/65A1O0/O0~/O01VW4l]
AUTHOR: Valitov,, R. A.; Kaj~j4q Kuzlmichev. V. D1-
ORG: none
TITLE: Measurement of energy and power of optic quantum las
SOURCE: Izmeriteltnaya tekhnika, no. 5, 1965, 37-41
TOPIC TAGS: laser# ruby laser, calorimeter, elastic osalllation,..gaveous stat6.
laser, photoelectric effect, thermal effect
AWTRACT: A survey of presently known method memsuring the
electrical charaoteristios of lasers. 3,easp.rIng deviaes
Types 0v
must vary for measurement of the various types
which vary from low power, continuous operating Ho-Z-HiF gas laser's
to very high power, very short pulse duration ruby lgLsors. T40
effects used in measurement are the thermal, pon6.ermotive and;
,photoelectric effects. A typical calorimeter for pourbi, measx.= '
ment Is described, Its operation and pr~nclple 80urceri, of error
(errors in-calibration of dc or condensor energyp transparency~
of calorimeter sectional degree of "blaolmess" of blsO: bodyf
readout, and energy lose compensation) are dlscussed.~ A drawtng
.of a ponde,rmotor power me.asurin.g device is presented dind Its
Card 1/2 UDC:~ 621.3-75-91
1111iff4vullilmn E111"IfAll Jill Dgul Ira FM
L 22138-66
ACC NR% AP6012935
0 eration briefly outlined.' Main sources of e!rr6r li'sted arei
P
error In measurement of specific moment of rotation of.thread,
and of Inertia of mobile system; Inaccurate bean,41mirigI reado4t
error; radiometric effects; inaccurate determination of an1r.le or fall on.
reflecting surface and of reflecting capacity of the surfa(lef The rormatic"it;
of elastic oscillations and other effects are also noted &4 havi~a been
suggested as bases for measurement of laser power. Orig. ;irts liftet 2 figAres.
[JPRS3
SUB CODE: 20 SUBM DATE: none 01b MW: 016. oTif REJ?.- 09-0
it
2/2
KALININ p Y'u. D.
Georiagnatic Secular Variations in the USSR and tfto Earth's Internal Structure.
(Geromagnitnyye vekovyye variats'Li v SSSR i vnutrenneye stroyeniye ze%li.)
Vorks of Sci-Res Institutions of the Main Administration of the !~ydro-
mateoroloGical Service USSR9 Series VIp No. 0. i~~droneteorological Presis,
Moscow/Leningrad.- 1940. 48 pp idtn Maps*
(Yeteorologiya i Gidrologiya, N; 6 Nov/Dee 1947)
SOi U-3218~ J Apr 1953
Also: Dok. AN 53, No. 1, 1946
Tnst. of Terrestrial YAgnetism.
A
Ll
u
fez
low mob
00 'S i ortw
a 11! 9l
dw op"M
0 t rdheio"
94)
001 W
'lip
Inst. Pea. in Terrestrial Magnetism.
~
for
L 06 Om lit
- - --- ------
nn-, I.-T
of iego go 0 e 0 o 0 0 0 o o 0 o 0, 4,
so*
no*
we*
Ylj-
U35'111
USSRA100-physion
Msgaetiem, Terrestrial
YAgaetic risids
"Reterogeneity of the Depth of the Zarth and Goom
netic Varlaticne," Yu. D. Kalinin, Soi Res lust of
Terrestrial YAgnetiam, 4 pp
"!"_ Ak Nauk SSW. Bar Geograf i Goof izu Vol XII, No 3
Studies of the fixed gemagnetic field and its secular
variatian led author to tho omGlnsim that imide tb4
earth at depths approximately equal to ba-I of the
earth2s radius there is unequal distribution of elec-
trical conductivity. Question is mcplained on tho
66T63
USM/Geophysles (Ccntd) XV/Jun 2.948
basis of solar-diurnal variations. Submitted by
Academician L. S. Laybenzan 2 Jun 194T.
66T63
KALINY, YU. D.
"Secular Geomagnetic Variations and Fluctuations of the Length of Day,"
by Yu. D. Kalinin, is included in a list of translated titles of articles on
geophysics appearing in Meterologiya i Gidrologiya, No 3, 10419.
0
SO: U-2551, 30 Oct 52.
Ono cl-laractucrirtic of
-.0U.1,hutlo- C,
tM, field ot a im-natic 3Lom. Dokl. A',.' 1;3~~ ~,2,
No - 3, 1952.
T-,jjtjtUt ZeMrj0,-0 '. intoLimma r(-,!. J,,.il-:- YPI
SO: Mont List of Russian Accessionas Library of Congreas,, uncl.
/VW-
KOZ Ie, S.M. professor; AFANASIYXVA, V.I., kandidat fisiko-
matematichaskikh nauk; PSHMIGH. H.S., kandidat fiziko-matematicho-
skikh nauk; GLUSHKOVA. To.?.; KUZENTSOVA, Z.S.; RNLOUSOVI, M.A,;
SOIANZYCHIK, A.A., tokhnicheakiy redaktor
[Manual on variation in the magnetic field of the U-S-S-R-3
Spravochnik po paremennomn magnitnomu polAu SSSR. Pod red. V.I.
Afanes'evoi. leningrad, Gidrometeor.izd-vo, 1954. 265 p. (MLIRA 10.7)
1. Leningrado Nouchno-isslodovatellskiy Inititut semnogo magnotizza,
2. Nauchno-tooledovatellskiy institut samnogo magnottzma (for
Xalinin. Afanaelyeva. Belousova) 1. Tashlwntskays nauchno-iseledova-
tollskaya goofizichookaya observatoriya (for Kozik). 4. Glaynays
Geofizichaskays observatoriye (for Penkovich, G-lushlrovs, XUzuetsova)
(gaguetism, Terrestrial)
AFAUSIYJIVA, V.I.; .K&LININ, Yu.D.
Some problems of magnetic cartography. Trudy KIIZK no.11:33-80 155.
(Nagnetism, Terrestrial)
KALININ Yu. D.
"Forecasting Secular Geomagnatic Variationa."
The International Aesconiation of Geomagnetism and Aeronomy; Abstracts
of the Reports at the XI General Assembly of the International Union of
Geodesy and Geophysics) Moscow, Izd-vo AN $SM , 1957. 46 p.
Abstract: Variation in annual values of geomagnetic elements Is the sumnary
affect of changes in the geomagnatic field caused by internal agents ( ) and by
geomagnetic activity ( ). The lat-ter could be completely elelminated by
taking average values for 10-11 year cycles. The mprphological examination of
such factors leads to the establishment of space-time ralAitionships. The effects
of internal forces in Eurasia are ofa smooth, quasi-periodic character
lastig a few decades and the geomagnetic activity follows an aloven year cycla.
This makes it possible to forecaBt average values for a five year period vitb
sufficient accuracy and to construct magnetic charts for the nearest epoch.
37-11-21/18
AUTHOR: Afanaslyeva, V.I.,Kalinin, Yu. D. _~b nekotorykh
TITLE: Some Problems of Magnetic Mapping
voprosakh magnitnoy kartografii)
PERIODICAL: Trudy Nauchno-issledovatellskogo instituta zemnogo
magnetizma, 1957, Nr 11(21), pp. 33-8o (USSR)
ABSTRACT: The accuracy of collected data and methods of map
mapping are discus6ed. The following authors are men-
tioned: Smirnov, I#N., Tillo, A.N., TrubyatchinBIcly,N.N.,
Penkevich, M.S., Ivanov, M.M., Lazarev, P.P.,
Veynberg, B.P., Rykachev, M.A., Kuchinskiy, Ye-A. There
are 11 figures, 10 tables, 'and 27 references of which
18 are USSR, 1 French, 2 German, 2 Japanese, and 3
English.
AVAILABLE: Library of Congress
Card 1/1
AUTHOR: Kalinin, Yu.D. 49-12-4/16
Petwork of Magnetic Observatories in
TITIE: Organisation )f t
the USSR during the Last 40 Years (Organ-izatsiya seti
magnitnykh observatoriy v SSSR za 40 let)
PE RIODICAL: Izvestiya Akademii Nauk SSSR, Seriya Geofizicheskaya,
No.12, pp. 1469 - 147? (USSR)
ABSTRACT: The history of the organisation of the network of mag-
netic observatories is dealt with from the early beginnings
up to 1957, outlining also the main results achieved. Para. 1
deals with magnetic observatories in Russia prior to 191?.
Para. 2 deals with the network of magnetic observatories
organised between 191? - 1930. Para. 3 deals with the network
of magnetic observatories organised in the period 1931 - 1940.
In 1941, 18 magnetic observatories were in operation in the
Soviet Union. Of these, 5 were subordinated to the Main
Administraticn of the Northern Sea Route (Glavnoye upravleniye
Severnogo Morskogo puti), but tLeir scientific work was con-
trolled by the Arcti6 Research Institute (A~kticheskiy nauchno-
issledovatelskiy Institut); 10 observatories were subordinated
to the Hydro-meteorological Service (GidrometsluzhbA,), etc.
The most important achievement of the Soviet magnetic obser-
Cardl/7 vatories between 191? and 1941 is stated to be the successful
49-12-4/16
Organisation of the Network of Magnetic Observatories in the USISR
during the Last 40 Years.
participation in the Second International Polar Year, partici-
pation in carrying out general magnetic mapping ~about 100
expeditions amounting to about 25% of the total number of such
expeditions) and also supplying data on magnetic variations.
Para. 4 deals with the network of magnetic observatories in
existence between 1941 and 195?, enumerating -those damaged by
the war and measures taken after the war to put them back into
operation. The Pavlovo Observatory was completely destroyed
and therefore, it was decided, in 1946, to re-establish the
LeLT;an5rad Magnetic Observatory (Ijeningrads*p9agpitnMa Observat-
or somewhere else, in Voyeykovo. The destroyed observatory
at Aizhnedevitsk was substituted by one in Krasnaya--Pakhra,
where observations started in 1946 in temporary buildings, and
the permanent buildings were completed in 1957. After the war,
the Scientific Research Institute for the Earth's Magnetism
(Nauchno-issledovatelskiy Institut zemnogo magnetisma) started
organising its branch in Murman k. From 1940 o=aards, obser-
vations were resumed in Stepanovka.. Between 1949 and 1952,
the magnetic observatory at L1vov was built and, in 1953, the
fladivostok Magnetic Observatory was moved from May-Tun to
(;ard2/7 voroshilov, where it resumed work in 1952. The work of the
49-12-4/16
Organisation of the network of Magnetic Observatories --":n the USSR
during the Last 40 Years.
reconstructed after the war and, at present, it can be used for
measuging the horizontal componentwith an accuracy of
+ 10-~~' Oe [Ref. 57: v.n. Bobrov tRef.6] investigated the
influence of humildity on the operation of magnetic variometers;
V.1e. Shellting developed a number of designs of magnetic vario-
meters in hic~,the magnet is suspended on quartz tensioning
elements rRef. - in addition, some new designs of magnetic
variometers U magnetic variational stations were evolved.
(B.E. Bryunelli, Ref.8, and B.M. Yanovskiy, Ref.9) and also mag-
netic theodolites (K.G. Bronshteyn et al. Ref.10). The results
of magnetic observations have not been fully published [Ref.lij.
Some of the material has been published in publications of' the
Main Geophysical Observatory and of the Arctic Institute.
After 1940, average hourly values of the magnetic measurements were
not published and only generalised conclusions from such obser-
vations were. Generalised data of observations of almost all
the Soviet observatories between 1938 and 1921-8 are contained
in "Manual on the Variable Magnetic Field of the Soviet Union",
edited by V.I. Afanaslev and published in 1954 [Ref.123. From
1937 o4wards, data on magnetic activity are published systemati-
Card4/7 cally LRef. 13 and A number of works are devoted to the
jr
49-12-4/16
Organisation of the network of Magnetic Observatories in the USSR
during the Last 40 Years.
roblems of the method of operation of magnetic observatories
Reft6 15, 16 and 17], these include:Annual Reviews of the
gnetic Activity (N.P. Ben'kova, MABelousova et al. Ref-18)i
Catalogues of Magnetic Storms (Ref. tatistictidata on the
Magnetic Activity (8.M. Kozik et al. ef.20); Morphology of
Sun-caused Daily Magnetic Variations (N.P. BenIkova., V.B. Mikh-
alkov, Ref,21); Morphology of Long-term Geo-magnetic Variations
Based on Magnetic Observatory Data (P.F. Kokovkin, v.F.Pushkin,
Ref.22); Problems of the Theory of Magnetic Variometers
(n.n. Trubyatdhinskiy et a1.7 Ref.23). The brief review given
in para. 5 does not deal with the numerous theoretical works
which were based on the results of the observations of the
Soviet magnetic observatories. Para. 6 deals with the temporary,
expedition-type maghetic, variational stations. Among these,
the stations organised on drifting ice in the Central Arctic
are of particular importance. In the north of the Asiatic part
of the Soviet Union, an effort was made to organise groups of
variational stations to operate for a season and to supply data
for judging the local nature of the magnetic variations, (I.M.
Card5/7 Pudovkin, Ref.24). A certain number of temporary variational
49-12-4/16
Organisation of the metwork of Magnetic Observatories in the USSR
during the Last 40 Years
stations were organised for shorter durations, for instance,
for investigatint the geo-magnetic effects of the eclipse of
the sun in 1936 Ref 251 and 1952, investigation of magnetic
anomalies, etc. in i95b, a magnetic observatory was established
in the Antarctic and the establishment of several more magnetic
observatories is scheduled. The Scientific Research Institute
for the Earth's Magnetism -.,. (Nauchno-issledovatellskiy
Institut zemnogo magnetizma), created in 1940, is at present a
complex system controlling the work of all the permanent inag-
netic observatories of the Soviet Union, except those in the
Arctic. An original method was evolved of critical analysis
of data gained in observatories and it is claimed that no other
State possesses such a method. This method is based on com-
paring results of observations of a large group of observatories
(Comparison of the changes of the average yearly, average
monthly, average daily and average hourly variations at various
observatories - M.A. Belousova et al.) In recent years, a
tendency has developed to build new types of magnetic apparatus,
the introduction of which will permit, in the near future,
(;ard6/? dispensing with the expensive buildings of observatories without
LL9-12-4/16
Organisation of the Network of Magnetic Observatories in the USSR
during the last 40 Years.
affecting the accuracy of the obtained results. In 1956, a
number of new designs of magneto-metric apparatus have been
passing through the last stages of production (V-F. Shel'ting,
V.H.Bobrov and B.Ye.Bryunelli). It is claimed that the accuracy
of the observations of the main group of permanent,magnetic
observatories is higher than that of numerous non-Russian mag-
netic observatories. There are 25 Slavic references.
ASSOCIATION: Scientific Research Institute: on the Earth's magnetism,
the Ionosphere-anT~~ropagation of Radio:Waves;!i ,
(Nauchno-issledovatellskiy institut zemnogo magnetizma,
ionosfery i rasprostraneniya radiovoln)
SUBMITTED: May 3, 1957.
AVAILABIE: Library of Congress.
Card 7/7
AUTHOR i Kalinin, Yu-D. Profeasor (Maa-3-yw) 1,07-26-58-8-9/51
TITLE., Soviet In-"estigations of Geomagnetism (Sovetskiye issledo-
vaniya PC geomagnetizmu)
PERIODICALt Fr1roda, 1958, N. 8r PP 50-55 (USSR)
ABSTRACT.- Research work into geoma~7,atim is Carried out by magnetic
observatoriesi artificial satellites,, and th-~ only non-mag-
netic ship in -the world ~'Zaxyall- The z,.?sultr3 of these in-
vestigations ara impor-~a-nt not only for navigation, but also
fo:~ aviation ard radio communication. I~ore than 250 magretic
observatories are epexating throughcut the world, half of which
were organized for the IGY. The USSR hao 31 such observatories.
Two are on drifting stations in the Arctic region and 4 in
C,
the Antarctic regions They are nearly all eallipped with
series of magnetostatics magnetic --a-riorieters., and some of
them with fluxmetric devices recording on photopaper. They
ar6 100 times more sensitive than the magretostatic -vario-
meters. on the third sputnik a magnatcmeter is installed
which measures the valuz of the earth:s magnetism. Solar
activity at the present time causes many geomadnet�c dis-
turbances which are espe-~ially inte--,~sting. Tlie sun ejects
Card 1/3 streams of electrically charged rarti~:leu whi-.h affect the
Javiet Investigations of Geomagnetism SoV-26-58-8-9/51
magnetic field of the earth. In the equatorial plane of the
earth an electric ring current moves around the earth at a
height of 10,000 - 20,000 km. The charged particles are then
attracted by the two poles of the earth. The magnetic data
gathered by the artificial satellites show that the electric
conductivity of the ionosphere is distributed among the dif-
ferent layers. The electric currents are supposed to cause
inductive interaction between these layers. The penetiration
of the magnetic lines into the interior of the earth is also
studied during magnetic "storms". The magnetic pulsations
of the magnetic field of the earth are recorded by the flux-
meters. Data gathered on this subject permits the coruiection
of geomagnetism with electro-magnetic processes in interplane-
tary space. The non-magnetic ship "Zaryall measures the mag-
netic field on the ocean. It crossed the Atlantic 6 times
and also conducts research in the Indian Ocean. The Institute
of Earth Magnetism in Moscow is one of the four centere in
Card 2/3 the world in which the results of magnetic investigations
Soviet Investigations off Geomagnetism SOV-26-56-8-9/51
are being gathered during the IGY.
There are 2 maps and 2 diagrams.
1. Te.-zestrial magnetism-Analysis 2. Torreatrial mapretism
---MPaSlZ'(!MaTlt 3. Satelll-",e ;ehicles-Applications
Card 3/3
AFANASIYLVA, V.I.; K4LI11111, Yu.D.
Method of forecasting secalar gemtgnetic variations for the
nearost futurn yearo. Trudy Inat.goofiz,AN Gruz.SS2 171-7-31
158. (MIRA 13:4)
(Magmotiam. Torrestrial-Secular variation)
KALIKINA, Natallya Yevgenlyavna; otv.rod.; BASHCM,
"".4'
V.I., red.; KARABILOVA, S.F., tekhn.red-e-
(Terrestrial magnetio field] Kagnitnoe pole zemli. Moskva,
Gos.izd-vo lit-ry po voprosam aviazi i radio, 1959. 39 p.
(KM 12:8)
(Magnetism, Terrestrial)
- ULININ-,.-Tu.D-.; -doktor fiziko-mat. nauk, otv. red.; KURIKOVA, H.F.,
red.; NOVICHKOVA, N.D.9 tekhno redo
(CoLlection of artioles]Sbornik statei. Moskva., lzd-vo Akad,,
nauk SSSR. No.l.[Magnotic and ionospheric dicturbances)l-lagn.Ano-
ionosfernye vozmushcheniia. 1959. 72 p. (14IRA 15: .10)
1. AkademAya. nauk SSSR. MozbduvedomBtvennyy komitet po prove-
deniyu Mezbdunarodnogo geofizichookogo goda. III i V razdal-
programmy MGG: Zemnoi magnetizm. i zemvyo toki, iorLoefera.
(Magnetic storms) (Ionosphere)
KALIN .14, doktor f1Z.-mn"lum. nauk , otv. red . ; ViTt -,'I AJK
--94-lu
G.V. , red.
(collection of articles] Sbornik statei. Mu~ilom, Izdvvo
All SSSR. No.4. ~eomagnitriye vozmshcheniia. 1960. 51 P.
(I,JRA 28:11)
I, Akademiya nauk SSSR. I,'ezhduvedorrstvenrryv kcrdtat po
provedeniyu Mezhduriarodtiogo goofiziche.3kogo razpdel
programmy MGG. Zemnoy mgnetimi.
KALININ, TV.D.. doktor fiziko-mi3tem.nauk, otv.rod.-. KWIUOVA. K.F.,
red.; MAKUNI, Te.T., tekhn.red.
(Disturbances of the earth's electromagnetic field; collectioa
of articles] Tozmushcheniia elektromagnitnogo polls zemli;
abornik statei. III razdel programmy MOO (gemnoi wgnetizm i
semaye toki). Moskva. No.2. 1960. 68 p. (KIRA 13:12)
1. Akademiya nauk SSSR. Mezhduvadomatvennyy komitet po provedeniyu
Mezhdunarodnogo geofizichaBkogo goda.
(Magnetism, Terrestrial) (Earth currents)
297214
8/169/61/boo/008/045/053
AoD6/A101
AUTHORS: Afanas yeva,
Ti~ixl Very strong and strong geomagnetic storms and some problems of their
.theory
PMODICAL: Referativnyy zhurnal. Geofizika, no 8, 1961, 36, abstract 8CI251
(V sb. "Oeomagn. vozmushcheniy&, no:'4", Moscow, AN SSSR, 19C0, 5-
14,-English summary~
7m: During the period from 1878 to 1959 a classification was mado of
1603 magnetic storms, divided into three classes according to their forcej (mo-
derateP strong, very strong). For these three classes changes in the number (N)
of storms from year to year are analyzed. Besides changes in the 11-year cycle,
secular changes were revealed, which are synchronous with secular changes of
solar activity, estimated by the relative number of sunspots (W). The authors
discuss the problem pertaining to the cause of delay of the maximum N epoch from
maximum W in the 11-year cycle. This is explained by the previously known la-
titudinal shift of.the spot forming zone and by an increase In density of the
Interplanetary medium during the years of W-maximum. The density of this medium
card.. 1/2
2904
S/169/61/000/008/045/053
Very strong and strong,.geomagnatio stoma ... A006/A101
is from 1 to 100 protons per 1 cm3. In oQrpunoular stream interacting with the
interplanetary medium, an external turbulent zone is formed where a magnetic
field is developed because of the hundredfold amplification of the interplane-
tary field in the path from the Sun to -the Earth. Active periods of storms
correspond to the entrance of the Earth into the basio axial part of the stream.
V. Afanas'yeva
[Abstracter's notei Complete translation]
Card 2/2
N, Tu. D.
An attempt to explain magnetic anomalies of the world. Izv.
AN SSSR.Ser.geofiz. no.6.-906-908 Je 160. (MIRA 13:6)
lo Akademiya nAu SSSR. Institut zemnogo magnetizma, ionoefery
I rasprostraneniya radiovolue
(magnetic anomalies)
NALrNrN*..,Tu..D.
Oeomagnetism. Nezhdnnar. geofiz. god no.8.-19-21 160.
(MTI?A 13:6)
(Kagnetism, Terrestrial)
KUD121,1j). D. (Prof.)
IlMeenetic Observations by Artificial Sputnikfj and Rockets in Connection -with the
World Magnetic Survey."
report tmx_kmxV*mIt presented at the Co=d&HP51, an Space Research,- 2nd Intl.
Sympoalwa arO~Tlenary Meetine, 7-13 April 1961, Florence Italy.
8/030/61/000/003/008/013
B1051B215
AUTHORs Kalinin, Yu.B.
TITLEt Examination of the alternating magnetic field of the earth
FERIODICALt Vestnik Akademii nauk SSSR# no. 3, 19619 109
TEXTt This is a report on a conference held by representatives of the
USSR institutions concentrating on the examination of the alternating gea-
magnetic field. The conference was held in Moscow from December 8, to 12,
1960, and had been organized by the Mezhduvedomstvennyy komitet po
provedeniyu Mezhdunarodnogo geofizicheskogo gods, (Interdepartmental Commit-
tee for the International Geophysical Year). It was attended by represen-
tatives of academic and departmental scientific research and training in-
stitutes. L summary was given on the research results collected in accor-
dance with the program of the International Geophysical Year (IGY) and
during the International Geophysical Cooperation in 1959. After their
first evaluation, the majority of observations were submitted to the World
Center of Data of the IGY in Moscow* The following reports were mentioneds
Card 1/3
Examination of the alternating ...
S/030/61/000/003/008/013
B105/B215
L*I. Borman on the physics of cosmic radiation and the relation between its
variations and the geometry of the approach between the earth and the cor-
Puacular stream of the Bunj BeI. Mogilevskiy on solar physics# the depen-
dence of the flow of corpuscular streams of the sun on elootromagnetic
phenomena on the sunj T.A.. Troitskaya on the examination of short-period
oscillations of the electromagnetic field of the earthl R.0, Lfonina gavt
a survey an the geomagnetic activity for the years 1952 - 1960; L.G, Man-
surova gave general comparisons of the standards of USSR observatories for
magnetism by a field magnetometer, and thus found that in 9one observato-
ries corrections should be madej- N.K. Osipov reported on programs for the
calculation of electric currents,in the ionosphere on the basis of obser-
vations made by observatories; M.1. Pudovking on the results obtained by
Gomparing geomagnetic storms with ionoopheric drifts. All reports which
were heard. at the conference will be published in a special edition of the
series *Annaly MGGOO, Some comprehensive monographs on various problems of
magnetic activity are planned. Collaborators of the Institut zemnogo mag-
netizmaq ionoefery i rasprostraneniya radiovoln (Institute of Terrestrial
Magmetisal,lonosphere and Wave Propagation)q and the Arkticheskiy i ant-
arkticheskiy nauchno-issledovatel'skiy ins titut (Arctic and Antaratia
Card 2/3
ILI L)
Jt-~~
AUTHOR:
TITLE:
PERIODICAL:
24601
S/004/61/000/009,,/001/003
D264/D304
Kalinin, Yu., Engineer
Training of the brave. "Room" flight
Znaniye sila, no. 9, 1961, 9-11
TEXT: The article describes the purpose and applications of
flight trainers for simulating all the normal and abnormal features
of actual flight. A brief account of Yuriy Gagarin's training in
preparation for space flight is also given. Gagarin was accustomed
to weightlessness in planes and was subjected on a centrifuge to
stresses equal to those encountered in rocket take-off and braking.
He parachuted onto land and into water and spent long periods alone
in a soundproof chamber. He was subjected to vibration on a test
stand and to prolonged exposure to cold and heat in hot and vacuum
chambers. Gagarin learned to drink, eat and write in a space suit.
His preparation also included instruction in a special trainer com-
Dlete with instruments and controls and a computer to set the
ilight route. The author believes that such trainers will play a
Card 1/2
24601
S/004/61/000/009/001/005
Training of the brave. "Room" flight D264/D304
due part in space technique. They will be used for studying satel-
lite communications in space, for simulating the meeting of satel-
lites in orbit, for compiling "interplanetary stations" and for sim-
ulating landings on various planets, etc. There are 3 figures.
Card 2/2
31658
S/570/6',/000/018/002/004
Bl16/BlO8
AUTHORS: Afanaslyeva, V. I~, Kaliniri--Y[u. D.
TITLE: Geomapnetic storms in the years 1878-1959 and the solar
activity
SOURCE: Akademiya nauk SSSR. Institut zemnogo magnetizma, ionosfery
i rasprostraneniya radiovoln. Trudy, no. 18(28), -1961, 27-41
TEXT: The authors give results of studying the list of all geomagnetic
storms in the years 1878-1959. This list is a compilation of data from the
Leningradskaya magnitnaya observatoriya (b~ Pavlovskaya, ili Slutskaya)
(Leningrad Magnetic Observatory (previously Pavlovsk or Slutsk))
(N. P. Benikova i Yu. D. Kalinin, Katalog magnitnykh burl Slutskoy
magnitnoy observatorii. Kosmicheskiye dannyye, no, 125-128, 1941) for
1876-19409 the data from the Spravochnik po peremennomu magnitnomu polyu
SSSR (Reference book on the variable magnetic field of the USSR).
Published by V. I. Afanaslyeva L., Gidrometeoizdat, 19511 for 1938-1948 and
of the catalogue for 1949-1959, compiled by one of the authors of this
study on the basis of data in the periodical "Kosmicheskiye dannyye". The
Card 1/3
1658
S/570)61/000/018/'002/004
Geomagnetic storms in the years.. B116/B108
investigation is restricted to the cyclic (11 years) and secular variations
of the number of geomagnetic storms as well as to the relationship between
these variations and the corresponding fluctuations of the solar activity.
It was tried to consider the possible effect of the variable donsity of
interplanetary matter during an 11-year cycle. It is pointed out that the
secular variations of the magnetic activity correspond to the secular
variations of the solar activity. The authors considered the Interplanetary
matter. This made it possible to determine from the delay of the
geomagnetic phenomena the velocities at which the corpuscular fluxes are
emitted from the surface of the sun as well as the density of interplanetary
matter. These velocities amount to 4'102_8.102 km/sec, the density varies
from 1 to 60 units of measurement. Both quantities vary periodically,
corresponding to the cyclic variations of solar processes.. The corpuscular
fluxes are assumed to increase the density of interplanetary matter. The
investigation showed that the cyclic variations of the delay of geomagnetic
storms are mainly caused by the cyclic variations of the initial corpuscle
velocities, and only partly by the density change of interplanetary matter.
The shift of -the maximum in the geomagnetic cycle, relative to the maximum
in the solar cycle, is connected with the cyclic variation of' the
Card 2/3
31658
S/570/61/000/018/002/004
Geomagnetic storms in the years,_ B116/B108
heliographic latitude of the active formations on the sun at a relatively
small solid angle of the corpuscular fluxes. The corpuscular flows seem
to be connected with the flocculi, The authors thank A. K, Bychkov,
A. V. Seleznev and V, M. Treshchetkin for calculations and A, K Bychkova
for graphs. E. R. Mustell and 0. n. Mitropollskaya (Astron, zh, )5, 1958
and ~.6, 1959) are mentioned.. There are 6 figures, 7 tables, and _
24 references: 20 Soviet and 4 non-Soviet. The four references to
English-language publications read as follows; S. Chapman and J- Bartels.
Geomagnetism, 337, 1940; W. H. Bennet and E. 0, Hulburt. Theory of the
aurora based on magnetic self-focusing of solar ion stroams.. Phys. Rev.
J.~, no. 2, 315-319, 1954; W. H. Bennet and E. 0.. Hulburt. Magnetic
self-focussed solar ion streams as the cause of aurora. J, AtmosDh, Terr,
Phys., 5, 211-216, 1954; W~ H, Bennet.. Auroral and magnetic-storm theory.
Astroph., J., 127, No. 3, 731-742, 1958.
Card 3/3
KALINIII, Yu.D,
Conference on geomagnetism. Geomag. i aer. I no.12128-129
Ja-F 161, (141U 14:7)
(Magnetism., Teriestrial-Congrasses)
I
t~ILIKIL Yu.
I
".econd Inteniational Sympositua on the Exploration of the Cosmic
'i
~.,pacrj. Geomrg. i aer. I n0-3:1,46-450 MY-Je t6l. (14MA 11': 9)
(Outar space--Exploration)
KALITTIN, Yu.D.
-_-.KC6_0t_,c observations from artificial satellites and rockets in
connection with the world-wide magnetic surv-ey. Georag. i aer.
I no.4:618-619 J1-Ag 161. (ItilitA 14!1.2)
1. Institut zemnogo magnetizma, ionosfery i rasprostraneniya
radiovoln AN SSSR.
(14agnetism, Terrestrial) (Artificial satellites)
KALININ,-Yu.D.
Secular geomagnetic variatione, irregularitioa of the earth's rota-
tiont and radiation zones of the carth. Geomag. i aer. 1 no.5:
795-802 S-0 061. (MIRA 15:1)
1. Institut zemnogo magnetizma, ionosfery i rasprostraneniya
radiovoln AN SSSR.
(Magnetism, Terrestrial--Secular variation)
(Eartb--Rotationx)
KALINII, Yu-,.D. , -
Observations of the magnetiq field from the American satellite
"Explorer X.11 Geomaly. i aer. 1 no.5:844 5-0 161. MRA 15:1)
(Magnetism, Terrestrial)
KAMM, Yu,D,
Fifth Conference of the Special Comaittee for Antarc tic Research.
Geomag. i aer,1 no.6tlOl8-1019 N-r 161, (MM 15s2)
(Antarctic regions-Geophysical t4fsearch-Congresses)
KALININ, Yu.D.
,r--.. Anniversary of the Kazan Magnetic Observatory. Goomag. i aer.
2 no.2:370 Mr-Ap 162. (XIM 15:6)
(Kazan--Geophysical observatories)
42145
S/203/62/002/004/006/018
1046/1242
A UT r 1 OX-S Afanaslyova, V..T., Mogilevskiy, E.I.. Pnd Kalinin,
Yu. D.
TITLE: lnber~nl ctriictiire of solar oorpuseblar streams from
g6o-.aqgnetJ.(- dsta
PER I ODI"AL Geotmigns3fizri I aoronomlya, v.2, no.4, 1962, 659-662
TEXT: According to 1W. 1 (E.I.Mogilevskiy. Goomagn. i seronomiya,
1962, 2, No. 1, 48-55), the steady geoeffectiveolylar corpuscular
stroam is a soquence of plssna clouds of/%) 5.1 - :.012 cm in
diameter moving away frorri tho sun. The geomagnetic d-sturbances
result from the internetion between thQ t6rrestrial imignetosphere
and the magnetic field (definitely not the plasma) of the stream
which is forceloss ( H-roti =0) and essentially reazricted to the
.surf,ice of the plasm Flo,idF: the field of the Gorpuscular stream,
rioving vi'th % suporsonic velocit-y with respect to the magnetosphere
tosphe-
(M>- 10), generotes magnotoacou3tle shook waves In the magne
L~
Card 1/2
S/203/62/002/004/006/018
1046/1242
internal structuro of aoiar...
ric plasma. The anergy trnn:!ported by these low-frequenc7 (T-?, 0.1-
10 see) waves (-2.10 Org/cm`.soc) provides ra)onero fliLx suf-
ficient to produce mmgnetic disturbances (-~~-'10 , ergl~ec),. The
earth passing through t1ne corpuscular stream twice crosses i+u*s tr. F-
R.,
netic field, and since .--Ithlri the stream the rragnatic field 'Is
almost zero, each major inngnatic storm should have two intensity
maxima .-Iith a relatIve 2.1ill In between. From tho way geomr-ignetic
disturbances are generntod, the time dependence of theIr Intensity
should vary with tho geornngnatic latitude. Experimental results
for moderate, lnrge tind vary large storms confirm these theoretical
c one lus Ions .
ASSOCIATIO', institut zcmnoi-
,o tmgnetizma, lonosfery i raspross-
trananiya radiovoln AN SSSR (Institu'Ll-le of Terrestrial
10,'agnetism, the Ionosphere and Propagation of Radio
Waves, .11.!~
SIM MITTED: April 26, 1962
Card '2/2
1~kLIIIJIN, Yu.D.
Siberian conference on geoma&netism and aeronomy. Geomag.i aer.
2 ro.1:182-183 Ja-F 162. OURA 15: 11)
(Siberia-Geophysical research--Congresses)
KALININ, Yu.D.
Expression in spherical coordinates of the magnetic dipole potential
situated at any point in space and having a magnetic moment of any
direction. Geomag. i aer. 3 no.6tlO89-1093 R-D, 163.
(MIRA 16:12)
1. Institut zemnogo magnetizma, ionosfery i rasproatraneniy&
radiovoln AN SSSR. .
AFtlil I V.Sl lyll"VA, V ~, 1 . , ZHU I' I if) I A. ; K A Ll,'! fl, 't i. o. ;H.V, j',. I.
,y oC g,~~omagnetic dist-~rbanc~. ~ rt-r. ~ ric,.E:* 7-113()
Ene rg I ~., L.L2
w
I TD 1 4,.
0 '%IIIRA a8-J),
1. Institut zeinnogo migneutzma, I rw~;prostranenl.ya ruelovoln
Ali
L5
Peb
ACCESM0"NNIL- AT50(19973
TITLE: Results of Lnvestigatle-nig of magnetic activity during the ICY
SOURCE: AN SSSR. Mezhduve,domstventW gooffAche-n-Tcly Imimitat.. OwfizicNeeldly
byulletx-.n', no. 14, 1966, 15-541
TOPIC TAG3.- IGY ~6~ ctivity, Antaxotiolmagneltle
tt~_r_esearch, Arctic nls,%netic a
activity, magn ~tic gtorm, geioE,7wl)A--lv fFe-ld, 13012X C01-PUSCUlaT cv-rrent, rmil ation belle
ABSTRACT- Aftor presenting 2-wioraJ information about the lmt;ej-natj,jjn.IL: one-p-ritcifir
I 1,j! f dl I' ALI 011) T c~n-eijt.- ;te t,!
'g ILI I
ACCESSION Nb: AT50C99713
ASSOCIATION- none
SUBMITTED- CO ENC U 00
NO REF SOV-. ooo crrTmi.- 000
&T.TEl OODII,'.: ES
L 3283-66 it4T
ACCESSION MR.i AT5023606
AUTHOR: Kalini~, Yu. D.; Mogilevskiy, C. 1.
TITIX: -1-tructure of the solar corpuscular stream and Interi'actiort of this a1ream;
with the eArth's magnetosphere
uznava konferent e3koaa IL03i:
SOURCE Ysesov ajyd 20 fizike kosmieb P
1965, Issledovaniya kosmicheskogo prostranstva (Space reie-i;ca t, trudy konf erelltsifo.i
Moscow, Izd-vo Nauka, 1965, 368-381
TOPIC TAGS: geomagnetic field, solar plasma, solar radlatfon, s0lar wind, satellite
data analysis
structure of wuscu!3r q; Mar.
ABSTRACT: A model is proposed for the the -vjar--Qp in
an attempt to determine the mechanism by which energy is transfe.1pred from this
stream to the magnetospheN of our planet. The theory proposed in the papbi~. is,;
ba0ed on magnetic vector ob;,16rvations made by "Mariner-2,11.. "IKP,"jlll and other! satel-
1*fea and rockets. Itjs assumed that the magnetic'-field 6nd probably the~pjzd;ma)
of,the corpuscular stream corresponds to a Plow model conalating cifseveral,dis4'xete
laige-scale plasmoids (I'M-elements") which have an intrinsic quaol-forceleDiri-A,
C*d
-2-
L;3283-66
ACCESSION MR: AT5023606
s
magnetic field. This structure is a direct consequence of the whrrietic field ob-
served on -the sun, and of the mechanism responsible for emiiision of the corpuscular
~stream in -the active regions. Present theories for the interacilon between the ~o-
examineJ in the light of
the-earth's magnetosphere
are
Lar corpustular stream and
Isounding" observations of the-fliagnetic vector at the periphery of.,the magnetosphe
ind close -to the earth, which show that the magnertic field Of thod, solar Istream play
i considerable (if not decisive) part.in the ene~rg3* transfer between the stream ~nd
:he magnetDaphere. A comparison of "sounding" and surface observ4tions shmis that
there is a direct relation3hip between D-variations in the ':geomqgnetic field and
I
rariations in the field beyond the eartPs magnetosphere. in i6nClusion, the au-
thors are sincerelygrateful to V4,,I. Afanaslyeva who directed *~e 'preparation of
nuch of the information from surface magnetic observatori a., Used 'in this pat*r, and
iho was also responsible for'oeveral Of the illustrations u;~Ang these data atid d4ita
-1.11 Orig. Art. hash 11 figures 0 2 formulasi
From "IMP tl4j
WSOCIATIM: none
3UBMITTED: 02Sep6s EMCG: 00 UQ CODE:~M M
10 RU SOVt 6 OTHERt 018, ATD 8:.
... .......... fill 1041111 [lilt [its, U53.40 le".11111. 1111 1-
L .112g2-66
-XC-C' NRff AP6002756 SOURCE CODE: UR/020316511105/00611098/1099
AUTHOR: Afanaslyeva, V. 1.1K.41inlirl. YU.
ORG., Institu:e of Terrestrial Magnet ism,jonosehere and
Auwama's 41
Waves, AN SSSR (Institut zemnogo magnetizma, lonoefery i rasprobtrapp-miya radio.
voln SSSR)
TITLE: Diurnal changes I title rokaWi
n the velocity of the ear and,passLbla reasoas
for changes
SOURCE: Geomagnetizm I aeronomiya, v. 5, no. 6, 1965, 1098-1099
TOPIC TAGS; earth rotation, velocity vector, magnetic field,
magnetic momeat, AkjL14-Z4m,
ABSTRACT: Data of the International Time Service on the Irregular rotation of
the earth is not an accurate enough source for judging the cNinge Lit rotation
from day to day. V. I.. Afanas'yeva, Yu. D. Kalinin, and E. I. Mogilevakly made an~
attempt to. find the real source causing this Irregular rotation. They imagined a
metallic ball. hanging on a thread. A magnet moves along this ball horizontally at
a steady speed. Its magnetic moment coincides with the velacit :y vackor. Tha 01an1je
in the magnetic field caused by the moving magnet forces the ball to rotate. The
rotation is stopped by the torsion of the thread. The direct:k)n of-the ball's
rotation depends upon the side along which the magnet. moves. Solar
_Sorpuscular
Card 1/2 UDC., _5256.3~__
lit 1; .--M,
HIM 1
L 1125?--46
NRs' AP6002-756
streams pass the earth either traveling In the opposite direction or orvertaift it. Whan
the corpuscular stream and the earth pass each other in opposite directions, tj~is
creates forces which decelerate the earth's rotation. In contrasttl0lor cOrputictilar
streams overtaking the earth initiate forces Which accelerate the eakth's rotatl~,n.
The experiment with the ball was applied to the earth with ita Magnetosphere. The
experimenters developed a formula for computing the acceleration and deceleration of
the earth's rotation when a corpuscular stream passea the eartli at willected dimtancea.
OrIg. art. has:; 4 formulae.
SUB CODE:OIP3/ SUBM DATEI 12Aug6S/ ORIG REPI 005/ OTH ROVI 0021 ATD PREM
40
Card 2/9-
11411IM111111111MR I 'TRIll I
IBM
0)7142 SOURCE COOBs UR/3148/60/000/004/0005/0014
AUT11OAs Afanafilyovaa V# If YaI1212~ X?, hl~ Poctor of Phlysico-mthomatical sciences)
..... . ...
ORG r None
TITLEs Very large and large geomagnetic storms, and some topicsof their theory
SOURCE: AN SSSR. Mezbduvedomstvennyy geofizicheskiv komitet.111 razdel programy
NGG: Geomagrietizm i zemnyye toki. Sbornik statey, no. 4, 1960,. 5-14
TOPIC TAGS: xnxn -Xiantrq solar activity, magnetic storm, -solar
corpuscular radiation,.. interplanetary magnetic field, tnta p1xxff1xrxxxx0UHmXd&XXi4
sunspot 0-
ABSTRACT: This paper del 'yes into thenature and theory of significftnt_&~~.!&nttic
storms. The statistical basis was prbvided by observations of 1603 magnetic .storms
over a period of 82 years, - 1878 to 1959. Included were atoms with at least one of
the three elements exceeding 150 gammas (or 351). Amplitudes to 300-gammas weve cla-,
ssed as moderate, 300'- 500 as large, and those over 500 gammas as very large. Be-
sides the well-known 11 year cycle, a 30 year cycle of summary duration of moderate
storms has been detected. The time series of mr.gnetic storm activity is found related
with the sunspot activity, as shown in Fig. 1. The displacement of the maximum of a
storm number withfespect to the maximum of the relative number of sun spots, -;- aa a
function of j&jjL\bpots zone displacement along the latitudep is connected with the
time variations of the density of the interplanetary medium. Corpuscular sun stre 3
-card 1/2
ACC NRs A76CP07142
Time series of the Sun and ge(aag.
Pttic activities from 1878 to 1959-
W - av. yearly rel. mmbers of sun-
spot$. 1947
N-.numberz of atorms per, year
'1937 1 59;
W 1893 1 17 1928
I
.1 83
883
perturb. the interplanetary mediumt and the magnetic.storu field (which is to a con-
sidekable extent an;AntexplaneftEy magnetic field) is intensified ten hundred times
by the -turbulent movement caused by the strew$. orig. art. has: 11 figures, 4 tables,
SUB.'CWE: 00, 03/ SUB DATE: None/ ORIG REP a W4/ OW PMP: 002
3(6) PHASE I BOOK EXPLOITATION SOV/1934
Leningrad. Nauchno-issledovatellakly institut zemnogo magnet~izma,
ionosfery i rasprostraneniya radiovoln
Trudy, Vyp. 13. (Transactions of the Institute of Scientific
Research on Terrestrial Magnetiam, the Ionoopheret and Radio
Wave Pro agation. Nr. 13) Moscow, Gidrometeoizdat (Otd-nie),
1957. 119 p. 1,120 copies printed.
Additional Sponsoring Agency: USSR. Ministerstvo xvyazi.
Ed. (Title page): Ya.L. Allpert; Ed. (Inside book): V.I. Tarkhunova:;
.Tech. Ed.: V.V. Mayorov.
PURPOSE: This issue of the Institute's Tgansactions is intended
for geophysicists and technical persohnel working in research
organizations as well as for advanced students at universities
and technical vuzes. It is also of interest to communications
personnel.
Card 1/3
Transactions of the institute (Cont.) SOV/1934
Kushnerevskiy, Yu,V, An Experimental Set-Up for Studying the
Homogeneous and Non-Stationary Structure of Ionosphere 7"?
Kalinin Yu,K. The Problem of Phase Velocity and Direction
Fth'e Kal Toward the Front of the Radio Waves Above
a Non-homogeneous Surface
Lopatina, G,B. The Changeability of the Signal Strength of Long-
Wave Stations 110
AVATTART : Idbrary of Congress
M
/lob
6-22-59
Card 3/3
30V-10)-3-4-16/23
AUTHORL: Kalinin, Yu..K.
TITIE: Perturbation of the Field of a Plane Radio Wave b3r the
Ir:i~e,,_;Ularities of the Earth's Surface (Vozinushcheniye
polya ploskoy radiovolny neodnorodnostyami zenr,'Moy poverhh-
nosti)
PERIODICAL: Radintelchnilm i Elektronika, 1953, Vol 3 , Nr 4,
PP 557-561 (USSR)
ABSTIUCT: It is assumed (Ref.1) that the perturbed field E can
be expressed by:
E = E0 +~Iy) (3)
where Ax is expressed by Eq.(4); A y is given by a
similar equation, Y. (9) is the Sommerfeld attenuation
f unction and E0 is the field in the absence of the
irregularities of the Earth's surface. If En '.(4) is inte-
-rated with respect to y -the expresoic-)ns for the perturb-
Card 1/3
30V-10)-5-4-16/2'a
Perturbation of the Field of a Plane Radio Wave by the Irregularities
of the Earth's Surface
ation due to the profile of the surface and due to the
nature of the soil are given by Bqs.(5) and (6) respect-
ively, in which the x A is the distance from the point
of observation to the boundary of the irregularity, H(l)
0
is the Hankel function of the first Icind of the zero order,
and s = k(x A - x)cos 9 ; h(x) and g(x) in expressions
5 and 6 describe the electrical and the geometrical proper-
ties of the Earth's surface respectively. B(Is.(5) and (6)
were used to evaluate the perturbation for a "slight slope'l-
type of irregularity and for a "sea-dryland-3ea" discontin-
uity; the results are shown graphically in Figs.1 and 2
Card 2/3
SOV-10()-3-4-16/28
Perturbation of the Field of a Plane Radio 'Wave by -tile Irregalari-
ties of the Earth's Surface
respectively. The paper contains 2 figures and 2 Sovio-t
references.
ASSOCIATION: Nauchno-issle(tovatellskiy institut zemnogo inagaetizma,
ionosfery i rasprostraneniya radi.ovoln (Scientific Research
Institute of Terrestfial Magnetism, Ionosphere and Radio ivave
Propa,r,-ation)
SUB"'AITTED: June 1, 1956
1. Radio waves 2. Earth-Electrical properties 3. Earth-Reflective
properties 4. Mathematics-Applications
Card 3/3
;jv*/ lo )..3 ~20
AUTHORS:Kalini4,Yu. K. and Feynber-, Ye. L.
TITLG,: Propagation of the Ground Wave over a Non-Uniform Spherical
Earth Surface (11asprostranenlyo zelanoy volny nad noodnorodnoy
sfericheskoy poverld-inosb,yu zemli)
PER'IODICAL: Rad--;ote'tthnika i elektronika, 1958, Vol 3, k;r c),
pp 1122-1132 (USSR)
AB13TRACT: For the purpose of analysis it is assLuned that the field
is .;roduced by a vertical dipole situated on the surface of
the Barth. The vertical comoonent of the electrical field
En satisfies:
(0) + E v~ dS
En ~ '~a n - - (1)
4Tr On On
Where E(0) is the volume integral of the source function
n
multiplied by v n is the normal to the surface
(directed toviards the centre of the Earth) and v is the
Green function which can be expressed by Eq.(2) where 0 is
the are an-le of a great circle connecting two points, k is
Card, 1/4 Ulie wave number, a is the radius of the Earth and z is
1/ j V C)
P!ropa-ati~n of tlae Gr-)und Iffave over a Non-UniforTa Srherical Ea, r t h
Surface
the vertical co-ordi-iote; the coefficierit (10
where A = (1/2 ka)1/3 ; on the other hand, V (t9-" z0 q0)
denotes the attenuation function. F:)r L"Ollic case of z 0
tiie function V cmi b~,, ~)xprc:3sod 10y Eq.(3), where w(Q is
t~ie Airy function of a complex ar-LuLient. For this easel the
C-1
boundary conditions are expressed by Bcjs.(4), so that :43n is
in U"he form of Eq.(5). The soluLiou for E 11 is in the form
Df Eq.(6) where W is a slowly chaogin- a'-tenuatian fanction,
u
This can be written in the form of Eq.(5a) or in the form of
e
Eq-M. The integral in Eq.(7) is ta'~en along the great
0 -
circle connecting the points of transmission and roception.
If the transmission route consists of N se,,:--gients which
e i,. at,
are uniform Eq.(?) can be writ Eq (8) w1lere
1 1 j is
the au-ular length of the j th se-ment and qj is a U
0 0
parameter describin- its characteristics. For a route
Card 2/4
jJV/1'))-3-9-2/20
Propal-ation of the Gr-,)Luid V'Iave over a Non-Uniform Spherical Earth
3 L
Surface
c,-)r,sistin,,- of two sc -~,aeats the a~tenue.U,J.on function is ex-
I ~j
.iressed by Eq.(9) or Eq.(10'). can also 'be -ariLten as
L
Eq.(12). For a rou'c consistins o' 3 Scj~..mezits Ulie attenua
ZJ
tion function 1013 can be written as Eq.(15). It is of in-
terest to define the attenuation of various senvients Of ~L
transmission route; this can be done by emplo.1-ring Eq.(18).
This was used to determine the attenuation of a number of
systems. The results are shown in Fi,-s.1 and 2; the atten-
uation functions W are plotted for sea-land-sea and land-
sea-land systems as a function of their relative angular
T,Adthl ~ . Similar results are shown in FiSs-3 and 4;
Fi,-,.3 shows the field as a function of distance D over a
land-sea system, while Fig.4 gives the field for a sea-land
system; the crosses and circles in the fir,ures denote the
experimental points (taken from Ref.?). For systems in which
q = q, and q = (12 , the so-called boundary refraction
Dhenomenon is observed (see Fi-.5). The attenuation function
~or this case can be written as:' Eq.(21) or Eq.(22), from
wnich the differential attenuation can be ex-oressed by
R"U/ 1
Prop,a:,-,-Lion of Llie Gx,,:)und Wave over a Non-Unifor.'-l Spherical Earth
Surface
Eq.(23). The paper contaills 5 fi,-ures and 8 roference:3;
5 of the references are, English and 3 Soviet.
IISSOCIATION: NII zemno-o ma-netizma ionosfery i rasprostraneniya
0 0 ?
radiovoln i Fizicheskiy institut im. Y. '-I. Lebedeva, AN
;3,~SR) The Scientific Research Institute for Barth Map-netism,
lonosi)here and Radio Wave Propagation and the Physics
Institute im. P. 14. Lebedev of the Soviet Academy of Sciences)
SUBI'~iITTED: June 26, 1957.
AUVOMR: Kalinin, Yu.K. SOV/109-3-10-6/12 -unif orm,
-TITLE: ~MM~c ion of Radio Waves Over a non
Earth surface (K voprosu o difraktsii radiovoln nad
neodnorodnoy sfericheskoy poverkhnostlyu zemli)
PERIODICAL: Radiotekhnika. i Elektronika, 1958, Vol 3, Nr 10,
pp 12?4 - 12?9 (USSR)
ABSTRACT: A theory of the propagation of pround waves over a spherical,
non-uniform Earth surface was developed by Furutsu and
the author (Refs 1 and 2). In particular, it was found that
for a route consisting of two sections which are cl-aracter-
ised by parameters q, and q 2 1 the attenuation fuzict.-ion
is given by Eq.(l), where .6, e1 and A % are anCular
measures of the two sections; 49 1 + AG~ 2 ~ QA nhile
ti(qi) is the i-th root of the equation: wl(t) q67,(t4j)
where w(t) is the Airy function of ta complex arEurient;
a is the radius of the Earth,
A = (ka/2) 1/2 and q, = iA/ t T-*ne attenuation function
~e T,
41
Gardl/4 for a route consistinG of 3 seg,.ients VMS P.1.6.0 found in luhlc
SOVI0?-Z-lC-6/12
P�oblem of Diffraction of Radio Waves Over a von-uniform, SartlL
.Gurfoce
above works (Fcj.(2)) and it was indicntled how the function
could be derived for a larger number of se:~*ments. Hcre I
the author shows the attenuation function for n se.gLients;
W is given by:
n n-l
1~ o a A
Wn r IA "Am ~Clj - CIj+j)X
j=l
00 -XP iA ita.(qj)
X
af~-t (q.) _
aj a CIj tccj(qj) - tUj+j(qj+j)j~
The proof of Eq.(3) is done by induction; thus, it is
proved that if W nis expressed by E(-).(3)) 11711+1 is iii
Card2/4
SOV/109-3-10-6/12
Problem of Diffraction of Radio Waves over a rion-uniforra EfirL.
Surface
the form of Eq.(4).
It is shovon that if all the segments are large, i.e.
-A ~~l , the attenuation function is in the form of
15q.(8). At lono waves, Eq.(8) can be written as Eq.(9),
while for the short vaves, it is in the form of -Wq.~10).
If one of the segments is small, the attenuation function
is given by Eq.(11)- in particular, for a = 2 1 Eq.(11)
can be written as Eqs.(12) or (13). The attenuation
function for a route with continuously variable parameters
can be found by solving the integral equation expressed
by Eq.(14). This can be represented in the form of two
integrals, as shown on p 12?8, so that the final expression,
for the attenuation is written as Eq.(16), where V M is
the volume of an m-dimensional wedge whose an6les between
its sides are equal to J'r/4 . It is shown that the
series expressed by Eq.(16) is uniforr-aly converi-ent,
provided the following condition is fulfilled:
Gard3/4
SOV/100-3-10-6/12
Problem of Diffraction of Radio Vloves Over a llon-u_niforr~ Earth
Surface
2Aq iA ()A<
The author thanks Ye.L. Feynber6 and Y-a-L. Al'pert for
discussing the results of this wor1k.
There are 4 references, 3 of r-,,hich are Soviet and 1
English.
ASSOCIATION: N.-i. in-t zemnogo magnetizma, ionosfery i
rasprostraneniya radiovoln (Scientific-research
Institute of Earth Magnetism, the Ionosphere and
Radio-viave Propagation)
SUBMITTED: June 26, 195?
Card 4/4 1. Radio waves--Diffraction
0 0
S/141/60/003/01/001/020
E032/Elli4
AUTHORS: Borodina, S.V., Kalininj Yu.K.. 16likhay.Lova, G.A. and
1~11gell, D.S.
TITLE: A Review of the Present State of Research into the
Propagation of VerX Low Frequency ElectromaEnetic Waves
PERIODICAL% Izvestiya vysshikh uchebnvkh zavedeniy, Radiofizika,
1960, Vol 3, Nr 1, pp 5-32 (USSR)
ABSTRACT: This is a review paper treating both theoretical and
experimental problems,, In the first part a review is
given of calculations on the propagation of electro-
magnetic waves taking into account irregtilarities in the
ionosphere, the finite conductivity and the spheroidicity
of the earth, In the second part a review ir. given of
experimental studies in the frequency range 10 cps to
50 Kc/s. Above 3 Kc/s there is good agreement between
experimental and theoretical data,, It is pointed out
that it is necessary to develop a gelieral theory of
propagation of very low frequency electromagnetic waves
Card 1/2 taking into account both the spheroidicity and the finite.
s/141/60/003/01/oc)1/020
E032/E4-0
A Review of the Present State of Research into the Propagation of
Very Low Frequency Electromagnetic Waves
conductivity of the earth, particularly above .3 kc/s.
The review is based on 109 published papers,
Acknowledgement is made to Ya.L.Allpert, Yu,G.Ishchuk
and G.M.Sosnovskaya for their help, There are .14 figures,
and 2 tables and 1.09 references~ 1i of which are Soviet
and 98 Western.
ASSOCIATION:Institut zemnogo magnetizma, ionosfery i rasprostraneaiya
radiovoln AN SSSR (Institute of Ter-res i!H1 Ma timm,
Ionosphere and the Propagation of Radio Waves, AS USSR)
SUBMITTED: September 19, 1959
Card 2/2
S/194/61/000/008/084/092
POO 0 OV6, /3'7) D201/L)304
jUJT11OR:
TITLE: Certaii,. problems oif radiowave. propagation over -the
inhomol-'r one ous, spherical surface of the Barth
P M-10DICAL: Referativzyyy zhurnal., Atitomatika i radioelelktronika,
110. 8, 3.961, 70, iim3tract 6 1476 (Tr. In-ta zemn.
wagn, ionosfer-y i x-asprostr, radiovoln. AN SS'Sa,
1960, no. 17 (27), 50-129)
TEXT: The rcl.,Mlt is given of various inve stigat ions into
the scoDe of problems concerned with the r,idiowave propagation over
a spherical inhonio-encous carth, In solvin8 t1w.. problem the transi-
tion is rriadc from the diffnrential to irtegral fonu of Ilam,7ell's
equations by applyinff, the Green functions so that the ancilysis is
rcduced to solvin 'f the integral equation for calculating the elec-
tric field E. The itcritiye mothod of- soluti.on is possible for a
x-ride range of functions fl(?n)) where El - the complex dielectric
earth constant, P and rr, aro the coordiuates. Ls, a result, the
Card 1/3
20524
S/1914/61/000/008/084/092
Certain i)roblcmr,. D201/L)304
solutions is found to be proportional to the att.,_Inuatio functio
W as datermincd from the 1TILOfral ellitation,, From the proof of con-
vergence the required numb~x of teimis 1) is de-telmlacd mich that the
first p tems I)c grrcatcr than thEi remaining temus by a givei-i number
of times n. SoDitions may be ol-_)tain(~d fox, 1) = I and n = 0, p = 4_5
and n = 20~ The analysis is rdven of various particular cases of
the attenuation function. The cases are coiisidered of boundary
refraction of dif-ferent earth radii. at differeat sectio-,,,; of the
propagation path, of local field inhomogerize i tier, of -,,mtvcs propaga-
ting along the boundary and of statistical itihomogeneity of the
path. The use is considered of the double Fourier integral for
the solution o-f certain problems together i-rith obtaining the attenu-
ation function fror,.i the parabolic equation. The use of the theory
given above is considercd in view of many experimental results pub-
lished in litcrature, Of special interest is the cffect of increa-
sing field amplitude, when the wave crosses fro[,-l one section of the
path into mother, whose conductivity is grcater - the so-called
recovei-y effect along, short soctions of the propa~,ration path,
Card 2/3
I .cl,I,
?14
S /1113 It 8 84/092
1) /61/000/00 /0
Certain 201/U304
Theoretical calculations are in good ag'l-cemcut ul.-th exPerimental
data. The rccovcny-cf L',.-'Ct IL3 itut o.-Oservc(I alow-t Iong sections of
the :-,ath and if ouc scctimi is m:mIL mid Lhe other long, this effect
is much less -noticeable., I'liasc. re-latiormships giv-n- satisfactory
agreement betircei thoury anicl practice. The thoory shous that the
Process of Propagation han flip propo:.-ty of ,;Ij.divqr ad.ong the earth's
wirfacc, (AfFrac!:inLf into !;Ihadm, rcngio-as. 45 refercuces.
Z7,\I)str,nctor*s notc: c'cmp~-ctr- t:rmir>lation---7
c, W-cl 3/13
30934
1~a 00 S/57o/60/000/017/004/012
~/v 0 E032/EI14
AUTHORS2 Borodina, S.V., Kalinin, Yu.K., Mikhaylova, G.A.,
and Fligell, D.~S.
TITLE3 A review of the present state of research into the
propagation of ultra-long elettromagnetic, waves
SOURCE: Akademiya nauk SSSR. Institut zemnogo magnetizma,
ionosfery i rasprostraneniya radiovoln~ Trudy,
no.17(27). Moscow~ 196o. Rasprostraneniye radiovoin
i ionosfera. 130-172
TEXT- Long and ultra-long electromagnetic waves are defined
as those with wavelengths between '2~ - 5 and some tens of
thousands of kilometres. Part I of this paper is concerned with
a review of the theory of propagation of ultra-long radio waves,
beginning with G.N. Watson's paper (Ref.l: The transmission of
electric waves round the earth. Proc6 Roy. Socal "r-95, 546, igig).
It is indicated how the various equations formulated to describe
the propagation of elec-tromagneti-t waves in the earth-uniform-
ionospheric wa-re-guide can be evaluated. This is followed by a
summary of the methods which can be used to take into actount the
Card 1/6