SCIENTIFIC ABSTRACT GNEUSHEV, M.N. - GNEVYSHEV, M.N.

• Document Type: CREST
• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R000615510012-0
• Release Decision: RIF
• Original Classification: S
• Document Page Count: 100
• Document Creation Date: November 2, 2016
• Document Release Date: September 19, 2001
• Sequence Number: 12
• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT

G11M_TC1V) V. M.
"Semiconductor Heat-sensitive Resistors and the Study of Their 7hermal Cptrating
Conditions as Applied to Cunditions for Mderowave Power Measurement." Cand Tech
Sci Leningrad Inst of Precisicn Wchanics and Optics, Luningr*d, 1954. (RZhFiz,
Un 55)
Survey of Scientific and Technical Dissertaticho Defended at U3,SF Higher
Educational Institutions (12)
SO: Smz~. No. 556, 24 Jun 55

GNEUSHEVI M.N.
An additional video amplifier, Avtom., telem.i Bviss, 6
no.8:38 Ag 162, (KRA l5t8)
1. Nachallnik laboratorii radioavyazi i teleyidenVa Moakovakoy
dorogi.
(Amplifiers (Electronics)) (Railroads--Electronic equipment)

GNEUSHEV, N.M.; OVINNIKOV, A.I., starshiy inzh.
Radio comminicatione for signalman during track maintenen a work.
Avtom., telem.i svias' 6 no.1:31-32 Ja 162. (NIFA 15.3)
I* Nachal-Inik laboratorii radionvyani i tolevideniya Hookovskoy
dorogi~(for Gnewhev).
(Railroads-Commini cation 370tew)

Apr 46
d
oftr,isir achim" - Qualtried ftchinlatej
euvi I No 4
Gtrn`"s Importanoe of varkers-I receivlr4l
'iftquate Instructlon la use. of nev Adnies
-moblnery.

GRUMP Pol.9 inzh.
Introducing new type of roof bolting in developi.,iont mint.ng. Bezop.
truda v prom. 5 n0-4:1-3 AP 161. 140)
1. Institut gornogo dela im. A.A.Skochinakogo Akademli nauk SSSSR.
(Mine roof bolting)

GNKUSHEV, F.I., inah.
Precast reinforced concrete supports for mine vorkings. Ugoll.
prom. no.1240-43 Ja-F 162. (MIRA 15:8)
1e Institut gornogo del& im. A.A.Skochinskogo,
(Nine timbering)

GNEUM-Xt P.I.
Support of workings at the bi ierzhinskii and other Krivoy Ro- Haisin
a
mines. Fiz. mekh. svoiz.,, dav. i razr. gor, pomd, tio,2:207-2-23 t630
(~9RA -17.'l)

I P IIN I 111:1111 1 PI 'N P. Fly 'I In IJP .11 ,1 -11
GNEUSHEV, V.I. LHneushev, V.I.], inzh.-rsokhanik.
Poultry section of the "Zoria komanizmy* Collactire Farm. Makh. all'.
hoop. 9 no.1:25 A 158. (MIRA 11:Z)
(Poultry houses and equipmnt)

GNEUSHEV, V.I., in2h.-mekhanlk CHneuehov, V.I.]
11 ~ -1.1 4
~7-The FW-4 milking machine. Makh. all'. hasp* [91 no-5:25-27 My 158.
(Milking machines) (MIRA 11:6)

ACC NR. AP6036758 SOURCE CODE: UR70620/66/171:/()01/0081-/OO63-7
AUTHOR: Gneunheys VO us; Lyashchenko, B. G.; Matoyarov, V, A,; Novak, L. L;
Sark V V-'..
OAG: none
TI'TLE: Neutron diffraction investigation of radiation-induced orderinA in Xi3j~! and
Xi'3Fj / 2~~I/ 2_'ali~yz
SOURCE: AN SSSR. Doklady, v. 171, no. 1, 1966, 81-83
TOPIC TAGS: neutron diffraction, neutron irradiation, fast neutron, ordered alloy#
nickel alloy, manganese containing alloy
ABSTRACT: The tests were made on polycrystalline aamples irradiated in a type S14 re-
actor in an integral fast-neutron flux 3.5 x 1017 neut/cM2 at a temperature 60 -- 70*-
The neutron diffraction pictures were taken 56, 74, and 87 or more days folloving the
irradiation. Both samples exhibited ordering action of the reactor irradiation, with
(001) and (011) lines appearing for the nickel-iron-manganese compound, and also
smeared (012) and (112) lines for the nickel-manganese alloy. The latter two lines
indicate that long-range atomic order is also produced. The degrees of long-range
order, deterained from the ratios of the intensities of the superstructure lines (001)
and (011) to the intensity of the main line (Ul), differed by almst a factor or twoe
UDCt 539.2.22

ACC NR: AP6036758
This difference is attributed to the anisotropy of the distribution of the radiation
defects. It is concluded from the results that ordering of a previously disordered
N131-b alloy is feasible, and that this phenomenon depends on the conditions under vhich
the experiments vere made. This explains also discrepancies and the results obtained
by others* The authors thank V. I. Klimenkov for valuable advice. This report vas
presented by Acadeuician 0. V. Kurdyumov 2"anuwy 1966. Orig. art. best I figur*
and 1 table.
SUB COW a 20/ SM D=t oTjun65/ ORIG RUt 002/ OTH RV: 005
Card 2 /2

ACC NRi AP6029111 SOURCE CODE: Ult/OO411/60/030/006/0072/0074
I
AIMIOR: Gnoushov V ~y�shchcnko,BoG.; Novok,b.I,; Sarkqyaq., ~V,
.... . ........ .......
ORG: none
TITLE: Multiple component superstructures of variable composition In magnstisaakm
based on N13FO and Ni Mn Z'Report, All-Union Conference on the Physics of-Ferro- and
Antiferromagneti.am hold 2-7 July 1965 in Sverdlovsg_ 1-
SOURCE: AN SSSR. Izvestiya. Seriya fizicheskays, v. 30, no. 6, 1966, 972-974
TOPIC TAGS: neutron diffraction, ordered alloy, iron nickel alloy, nickel alloy'*
manganese alloy, chromium alloy ) /0096?-,0&r1C- -9"O(f
ABSTRACT: Investigations-.of single phase solid solutions of 3d metals have shown that
formation of superstructures of variable composition is characteristic of cross
sections of the phase equilibrix* diagrams of such threo-component alloys N1
(Fe,11n) _J,(Ni,C0)3Fe1ahd others, so that there was reason to assu VaF
1 ,N13 (Fe qr 8:0
ordti-rinj should o'b&in iWthe-superstructures based on N13FOO W13un and FeCoo Ac-
cordingly, in the present work there were investigated by neutron dtffraction analysis
alloys having the compositions X13(Fe0Un)# Ni3(Fo,Cr), NL3(Mn,Cr), WXO)On, snd
(Ni ICO)3 Peo sKno.5. It is feasible to detect formation of long-range order in experi-
ments on polycrystalline specimens of these alloys, About 21 specimens were prepared
by induction furnace melting of technical grade components under slag with latm-
.---A 1/2

SELIVANOV, A.I.p rei.; GNEUSHEV, V.114., InMi., retoorizent; HHOHINKi.'),
G.P., inzh., retRdiizifit
[Album of technological Obarts for a continuous repair of
the KDN-46 a.,a KDM-100 engines in specialized plants]
Allbom tekhnologicheskikh kart dlia potochnogo remotrta dvl-
gatelei KDM-46 i KDM-100 na spetsializirovanrWkh predpriiati-
iakh. Moskva, Mashinostroenie, 1964. 282 p. (MIRA 18,12)
1. Perovo. Gosudarstvennyy vaesoyuznyy nauchno-isslodovatell-
skiy tekhnologicheekly institut remorita i ekspluatntsii ma-
shinr-o-traktornogo parka.

GNEUSS, G.
A modern block steam engine. Wiad naft 6 no.6;133-136 Je.'60.
(Steam engines) (ERAI 9310)

3/1,3,3/62/000/0 1 1/005/OC5
A054/A 1 Ln
AUTHORS: Rakhshtadt, A.G., Docent. Meshcherionova, O.N., Candidates of
Technical Sciences, Gnevko, A.I., Soshnikov, S.A., Engineers-
TITLE: The effect of boron and ti-tanium on the mechanical properties and
ductility of the new 55 xrp (55KhOR) and 55cr2P (55SG2R) spring
steels
PERIODICAL: Stall, no. 11, 1962, 1o4l io47
TEXT: At the MBTY1m. Baumana (MVTU im, Bauman) and TsNIICY4M tests were
carried out to improve the quality of 60 C 2 (6oS2), 55 C 2 (55S2) and 55 x r (55Kha)
spring steelA by the addition of boron (0-003 - 0.01%) and fitanlum (o.o6 - 0.24%).
The new grades were melted in a 50-kg magnesite,lined induction furnace In the
following composition (55KhGR A', A"; 55S2GR - B', 55S2 - C for contzlol):
Card 1/4

"11331621ON10 1 1/005/0C5
The effect of boron and ...... A054/Ai27
"t~,L-
cjlklra(~
G
Mn
S1
Cr
il
11
16;;;~
C
Ain
51
T1
0

1 ,
4
0'5 1,01 0,35 1.4 0:06 0,003 9S 1 1 0.54 1.7 1,25 0,06 0-003
A' 2 0
t
5 1.10 0.32 1.2 0.06 0 006 ~41 2 0.55 1.65 1.33 0 06 0.0()r,
3 0,55 1,05 0.37 1.3 0,06 0:01 3 0.55 1.7 1.40 0:06 0.0 1
1 0.55 1.08 0.24 1.3 - - 0,003 1 0.54 1.7 1.08 0.06 -
2 .
0,55 1,1 0.30 1.5 0,06 - 2 0.54 1.5 1.05 0.10 0,003
A' 3 0,55 1.04 0.32 1.30 0.09 0 .003 3 0.54 1.6 1.1 0.12 0.003
4 0,55 0,99 0.32 1.35 0,16 0,003 4 0,54 1.65 1,15 0,24 0,003
5 0,55 0.94 0.36 1.30 0,24 0,003
- 0,53 1,0 1,8 0,3 -
Prior to adding boron the steel was reduced by aluminu;m, then titanium was added.
Tests carried out to study the hardenability of the new grades showed that an
addition of 0.003% boron greatly improved this property. Addition of lip to 0.06%
titanium to steels containing 0.003% boron Improves the hardennbiLity still
further. When more than 0.06% titanium was added, however, this property or the
steel deteriorated, most probably due to the crystallizing affect of titanium
compounds leading to the transformation of the supercooled austenite phase. The
addition of more than 0.1% titanium weakens the tendency to grain growth in the
Card 2/4

S/'.33/62/000/01 I /X5/CC5
The effect A' boron and ...... AO 54 /A I 2'r
steel structure, on account of the capping effect of titanitun tompounds that are
not dissolved in theaAstenite phase, not even at high (up to 11500C) temperatures.
The optimum addition both with regard to grain growth and hardening properties
are 0.003% boron and 0.06% titanium. The addition of.0.06 - 0.124% titanium sligkvt,
ly reduces the strength of the test grades. The 55SG2R grade, containing various.
amounts of boron and titanium has a higher ductility than the conventiopal 55S2
grade. The threshold of ductility will be attained with 0.003% boron and 0.1 -
- 0.16% titanium. Optimum ductility for the 55Sd2R grade will be obtained with
annealing at 3500C, whereas for the 55KhGR grade at 3000C. In the 55SQ2R grade
the value of stresses reaches the maximum simultaneously with the maximum val-ue
of ductility; at the same time the microplastic friction starts developing.
Spring steels containing boron and titanium show a lower tendency to decarburiza-
tion (in 5510M grade.- 0.01 mm, in 55SG2R: 0.003 mm, whereas in the 55S2 grade:
0.12 mm). The test grades proved superior to the conventional spring steels'
also in view of relaxation stability, which was tested under uni-nxial extension
at a stress ofcfo = 120 kg1mm2. To obtain a high degree of relaxntion stability,
the steel must coptain sufficient chrome. In general, the optimum amounts of
boron and'titanium added depend on the steel composition. Greater amounts of
Ca it-d 3/4

GNBVXO, D.G..inzh.
,:,- -.1 11 . -
In reference to the article "Organizational problems of dispatcher
control in power systems." Blek.atao 29 ne.11:90-91 N 058.
(KIRA 11: 12)
(Blectric power distribution)

GNEVKOj, D.G.; ZAROZHM,, A.M.
Experience in using a olosed-loop network in a law."Itago,.
power distribution system. Elsk.sta. 33 no.12140-42 D 162. -
(Electric power distribution) (XML l6x2)

FFDOSENKO, R.Ya., kand. tekhn. nauk (Moskva); RFYNVJtLl)_, O.A, (ReinvaldB, 0.1
(Riga); GNEVKO, D.G., inzh. (Minsk); ZAROZENYY, A.M., Inzh. (Minsk);
VOYTKO, A.M., Inzh. (Minsk); FEDOROV, Ye.Ya., inzh. (Minsk);
AYZENBERG, B.L., doktor tekhn. nauk (Leningrad)
Protection of closed-loop networks. Elektrichestvo no.2:
83-89 F 165. (MIRA 180)

GM~;.~,ENNIXO L.I.; RYABOKON', N.A.; GIMKOVSKAYA, T.V.
Determination of epiline in drugs. Med. lwom- 14 no.7:39-42 Je 160.
(MIRA 13:8)
1. Vsesoyuznyy nauchno-iseledovatel'skiy khimiko-farmatsevticheakiy
institut im. S. Ordzhonikidze.
(HAIRv REXOVAL OF)

GREBENJURl L.I.; MMOVSKAYAg T.V.; VFlJKWV0lLljFJ&TAP G.A*
Comparative data an the metabolism of nicotinic and Igionicotinic
acids in the rat 'Organism. Farm, i tol-j. 23 no. 5:/+3&-439 S-0
160a (MIRA 13:12)
Ig Otdel khimioterapii (zav. - prof. G.N. Pershin) Voesoyuznogo
nauchno-issledovateliskogo kbimiko-farmatsevt1cheskogo instituta
imeni S, Ordzhonikidze,
(NICOTINIC ACID) (ISOHICOTINIC ACID)

GREBUINIK, L. 1. ; , ; . M (!. " .
Met,abolism of vanilllr., is a ,) -,.fvriz~~je
med. khIm. 9 no.2:127-135 Mr.-Ip 163. e .~ 17: 8)
1. Otdel kh'--doterapij
khin.ikc-,-farmatsevtich&..-I~..;,-c in.7'Ituts iinx-nl (r-:~zIxn~R'dze i
Inst-itut tuberkuleza ~*!l S".41,

GNNVKOVSKIY. 0., prof. (Praga)
Clinical syvyptom of beginning avascular necrosis of the coxofemoral
joint. Ortop.trava.1 protes. 20 n0-8:32-37 Ag 159. (KIRA 12:11)
,HIP, d1seases)

CNENKOVSKIYY V4G, _ inzli.
Transportation characteristics of wheeled tractoro. Makh.i elek.
sot!).sel'khoz. 19 no.5:52 161. (MIRA 14 dO)
1. Melitopol;skiy Institut mekhanizatsii seltskorgo ld:o--yaystva.
(Tractors)

GNEVUSHEV, M.A.; DANILOCHKINA, L.Te.
Use of black-and-white photography in geologienl documentation
of underground mine workings. Razved. i okh.'nedr 29 no.902-36
S 163. (MIRA 16:10)
1. Vsesoyuznyy nauchno-issladovatellskiy inatitut mtodiki i
tekhniki razvedki.

15-57-7-9361
Translation from: Referativnyy zhurnal, Geologiya, 1957, Nr 7,
p 90 (USSR)
AUTHOR: Gnevushey- M. A
TITLE: The Origin of the Oppositely Oriented Parallel Pits
on the Faces of Diamonds (0 proiskhozhdenii obratno-
parallellnykh treugol'Inykh Ypadin na granyakh almaza)
PERIODICAL': Mineralog. sb. Llvovsk. geol. o-va, 1955, Nr 9,
pp 25-30
ABSTRACT: The author enumerates different observations of tri-
angular pits and projections on the octahedral faces
of a diamond, and he notes that the triangular pro-
jections are always oriented with their edges parallel
to the edges of the octahedral faces, whereas the
triangular pits (most commonly) are disposed in an
oppositely parallel attitude and only occasionally have
Card 1/2 a parallel orientation. He bhows that the'pits are

15-57-7-9361
The Origin of the Oppositely Oriented Parallel Pits (Colit.)
much more widespread than the projections. In explaining the origin
of the oppositely parallel orientation of the triangular pits he
adopts the view that the arrangement is the result of growth. lie
also associates the parallel orientation of the projections with
growth and recognizes'that the pits with parallel orientation are
solution figures. The author sees support for his view in the
experiments on the burning of diamonds, in which triangular pro-
jections with parallel orientation are obtained.
Card 2/2 M. 0. Kliya

15-57-7-9362
Translation from: Referativnvy zhurnal, Geologiya, 1957, Nr 7,
p 90 (USSR)
AUTHOR: Gnevushev, M. A.
TITLE: The Fluorescence of Diamond (0 futolyuminestsentsii
almaza)
PERIODICAL: Mineralog. sb. L'vovsk. geol. o-va pri un-te, 1956,
Nr 10$ PP 325-329
ABSTRACT: A consignment of diamonds was studied with the port-
able apparatus LYuM-1 (PRK-4 lamp, UPS-3 light filter,
voltage of 75 v, current strength of 3.75 amp)* Dif-
ferent fluorescent colors were observed: predominantly
shades of blue and yellow, rarely yellowish red, and
very rarely green. Densely smoky, yellow, and highly
iron-stained crystals did not fluoresce at all and
seemed to be stained in dark violet or velvet-black
colors. After segregating the diamonds of the con-
Gard 1/3 signment according to density of colar, the following

The Fluorescence of Diamond (Cont.)
15-57-7-9362
Well-formed, transparent, and colorless crystals are characterized
by medium blue fluorescence. Distorted forms, the presence of
intergrowths, decrease in transparency, and the appearance of
colors and point inclusions lower the fluorescence to yellows and
red-yellows. Thus the conditions of crystallization of the diamonds
affect their fluorescent properties.
Card 313 V. A. Vorobfyeva

GNZVUSIMV,,M.A,.
Traces of scouring on diamond grains. Z&p.VseM.min.ob-va 85
no-3:401-403 156. (KLU 9:11)
(Diamonds)

VI/C
p4milm In &a Amway 440 4-111,AG*44. ifis, jimill:
a ttmc*a Q tbi~ Cl
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Zaftrii Viotayw. MirorA OWWWA4, 41P,049%lom ft
Fkathtc, C.A. 32, pz"Ulaner~ C4 41, i9l.5
Fmm pcecwm X-ft m eats of KdAmed 6rxeo.~ ~i
r4dil of bi,- gnd WvAltwt tottals r" kind)" YI flit W~ei
Fat the Simpta Caid. 0
betwe= 0.740 apd OAM M Irw 91100 .4
0414W 0 - 10420 -fi, 1 ,
gatwo. The ~crr*,jpdi*#,itjm mi,
14 the gTcram1drftc-antdL1e mica to &eti bY the l4w,tial
a4 - 10.605 + 24M r " (for it coast. kv. r', 60 1.01 OX Oat$
0.413 W. -1300 IvIsdons! COA bo~ c"16'-6m1,r0-

formwA 64 $J
V'racts In th
COO as 0 vtzy isr f my 40alhim, IvitO to 4,
--t = x "m b* 1414tvbtkis *f,r,
ScmMey. Further 4d w
and r... with 4*, Add the 49019. 9UPh.
cad tgoosuUtlll Pet= ItIvIl"
-dite. For prigctkaj puiptWo tfit% liNttqr ft 1~
w"a 10 NiNel 11 1
melol, and only tho Aarwimt of hiaO #nd )rA nipy taini'"
about slight dcOmilons. For (he tvka dicilvi Ot!(110 tp
nimben in the gasuet C*p new Wa iaq gi I
W: pyrope - I t.43 ImandRA -~ 11-M. 4 L'A
1"73; PL'Osulmite - I I.Moi.mindrAdite -42MOXV~j N
yite - 12,00. In odda - at glvr4 thom, of "WA t4
MgO.RAASA) - II.Mri; Q T440
00 - 1140S., "Clildelite" (11MU0.11
W
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1 IQ
thtw latter mu pratto t1it rAdil I" 0-&w1;;;;aan4d vv!
WK vFcte cmlcd.

i

i

TATAMKIY. V.B.; FRANK- KARNUTSKI Y, V.A.: BUR[iKOVA. T.N.; IMIDOV, V.V.-,
PHTROV, T.G.; KOURATlYlIVA, V.V.; KAMXNTSXV, 1,Ye.; GRAWITSIL37A,
V.F.; AT-2 SNYIVA, N.P.; ARTSYBAMMVA. T.F.; RARANOVSKAYA. N.I.-,
BUSSU, I.T.; VMUDWSKO, I.A.; GNITUSHIV, M.A.; GOYKO, Ye.A.;
KOKKOV, A.I.; KOTOVICH, V.A.; LITTI NS Xkt~l-' 00P.; milmuVA, I.T.;
MOKITIVSKIYO V.A.; PBTROVA, L.Y.; POPOV, G.M.; SAnONOTA, G.P.;
SCBOIJIVA, V.V.; STUWT, N.N.; TUGARINOVA, T.G.; SHMMANOVSKIY. I'L;
SHTMMAR9, A.A.; YANULOV, K.P.
O.M. Ansheles; obituary. Veet. IW 12 no.18:152-154 '57.(NIBA 110)
(Ansheles, Osip Markovich, 1885-1957)

BOBRIUVICH, A.P., sotrudnik; BOIMAUNIO, M.N., sotrudalk; QliJ;VV44Y, M.A.,
aotrudafk',,"----
sotrudaik; KIND, N.D., sotrudnik; XORASHKOV. B.Ya.,
KURYLEVA, M.A., sotrudnik; NMDOVA. Z.D., sotrudnik-, POPUGAYEVA,
L.A.. sotrudnik; POPOVA. Ye.B., sotrudnik; StULISKIT, V.D.,
votrudnit; SMIRNOV, G.L. sotrudniks, YURNEVICH, R.I., sotrudnik;
TAYNSHINTM, G.9h., sotrudnik; SHCHUKIN. Y.N.. aotrudnik; BUROT.
A.P., nauchny7 redaktor; SOBOIAV. V.S., usuchnyy redektor;
VXRSTAX, G.T., redaktor iziatelletys; KRYNOCHKINA, X.Y.. takhnL-
cheskly redaktor
[Diamonds of Siberia] Almmsy Sibirl. [Moskva] Oos.nouchno-takhn.
lid-vo lit-ry po gaol. i okhrene nedr. 1957. 157 P. (MIRA 10:7)
1. Russia (1923- U.S.S.R.) Mintsterstyo geologii t okhrany nedr.
2. Anakinakays ekspeditelys Glayurelotbgeologit Kinisterstva geolo-
gii t okhrany nedr SSSR (for Bobriyevich, Bondarenko, Gnevushev,
lind, Koreshkov. Kuryleys. Mefedovs. Popugayevs, Pop*ys, Skullskiy.
Smirnov. Turkevich, laynohteyn. Shchukin)
(Siberia-Dissonds)

Gf1ZVUS1MV.,.X.A-~,-BO1JKOV, N.A. [daceased]: BARTOSjjjN,-3yjT. ?,.V.
Etching and dissolving traces on Takutian diAmonds. Hin.abor.
no.11:22-37 157. (MIRA 13:2)
1. Amakinskaya skepeditstya Glavuralsibgsologii Ministerstwo,
goologii okhrektW nedr SSGR.
(Talmtla-Diamond crystals)

BARTOS11I 11 SKIT. Z.V.; qHXr;�11HV. M.A.
Causeu of optical anisotropy in diamonds. 141n.abor. no.12:
57-66 158, (Him 13:2)
1. Amakinskeya skspeditelys, Hinistarstva goologii i okhrany
nedr SSSR.
(Diamonds--Optical properties)

GINEMARV, N.A.; WlKold~YFVA,
OlIvin and pyrope incluRions In Yal-cutian dinmondu. Hin.Bhor.
no.12:440-41w '58- (MIRA 13:2)
1. Amakinakaya okopeditelya Takutskogo geologichookogo
upravInniyo.
(Ya~utla--Chryaollte) (Taktitia-Pyrope)

GYGVUSIW, M.A.; GONON, G.0s; CIMMUKO, A*I*
Iffect of the chromium content of pyropo on tba halght of maximal
curves of spectral absorptioz6 Zap. Toes. min, ob-ya 87 no,10-5.Z9
'58. (KM 1126)
1. Amakinskaya ekspeditsiya, Glavuralsibgsologli, st. Iyurba.
(Chromium--Spectra) (Garnet)

GNEVU5HEV, M. A. Cand Geol-Min Sci -- (dius) "Diennondu of wevtern Yakutiya."
Len, 1958. 15 pp (Min of Geology and Mineml Con ervation USSR. All-Union
i
T k
Sai Res Geol Intt VbYeGYeI. Amakin Expedition of 'akut'*p Gool Adrninistration),
i
100 copies (KL, 11-56, 114)
-31-

-1 5 -
Z i
, i 3 J i S"
a
a u
I Iv
fill
110

BOBRITjIVICII, A.P.; BONDARY,11KO, K.N.; GMVUUH.HV, L.M.-,
SKIRITOV, G.I.; YURKSVICH, R.K.; SOBOLEV, V.S..,"akademik. nailchnyy
red.; VMISTAK, G.V., red.izd-va; GtMOVA, O.A., tekhn.red.
[Diamond deposits of Tabitial Alrwznye mastoroulidealia Ulattii.
Nauchnyi red. V.S.Sobolev. Moskva, Gou.nauchno-tekhn.izd-vo
lit-ry po geologii i okhrana nedr. 1959. 526 p. (MIRA 12:11)
(Taktitia-Diamonds)

ANDRIANOV, Nikolay Ivanovich; BUbNOV, Yevgeniy Sergeyovich;
I - _k 'I
. -Mikh-gil Andreyevich; IOANNESYAN, Rollen Arsenlye-Ach; LITVINCV,
V'ik-61a-j-Nik-o'Ibj;Wab; MEYERSON, Yevj:cniy Grigorlyevlrb; IfXvDLII(,
Yakov Borisovichl ROMANTSEV, Yakov Antonovich; AIWIN# A.G., red.;
JaESHKOVAp S.M.v vedushchiy red.; POLOSINA9 A.S.p tekhn. red,
[DiamFnd drilling] Alwznoe burenie. Moakva, Cos. nimchno-tekbn.
izd-v neft. i gorno-toplivnoi lit-ry, 1961. 170 p. (MIRA 14;9)
(boring) (Diamondsp Industrial)

GliZVUSIM, M.A,; KRASOV, L.M.; DUDOT011NO, Yu.V.; DlYiU:OVA, U.I.
Color of Takutian diamonds. Trudy IAFAN SSSR. Ser h'001.
no.6:87-96 161. iDMU 14:9)
(Yakutia--Diamonds)

GNEVUSHEVY 11I.A,j NIKOLAYEVA, E.S.
Solid inclusions in.diamonds of Yakutian deposits, Trudy
IAFAN SSSR. Ser.geol. no.6:97-105 161. (MIRA 14:9)
(Yakutia-Diamonds)

GNZVUSIEVj, M.A.; BARTOSIIIWoKIYP Z.V.; ZINKOV, A.P.
- .4 11- - i
Diftibution of diamonds in the kimberlite pipes of voltern
Yakutia. Trudy IAFAII SSSR. Ser.pol. no.601&= 161.
FIDA 14:9)
(YaWtia-Diawnds)

,,-----GNEVUdfibYT-MrA,~JEDUROVA, L.Q.
Effect of iBomrphic subetitutionson certain characteristics Of the
infrared spectra of gamet. Dokl. AN SSSR 146 no.3:672-675 S 162.
(141RA 15:10)
1. Vueno"UmVy nauchno-imeledovatellskiy goologichaskiy institut,
(Isomroim) (Garnet-Spectra)

GNEVUSIOV.? V.1khail Andreyevich; KORZINYEV, S.S., st. nauchn.
-,otr., kand. geogr. nauk, retsenzent; KIND, II.V., kand.
geol.-miner. nauk2 reteenzent; VASILIYEV, A.F.p retsenzent;
itODIOZIOVA, F.A., red.; KISELEVA, H.D.) red.kart; YARPOVA,
T.V., takhn. red.
(Yakut diamonds] IAkutakie almazy. Moskvap Uchpedgis, 1963.
102 p. (MIRA 16:12)
1. Institut geografii All SSSR (for Korzliuyev). 2. Yakutskiy
inatitut usoverahenstvovanlya uchiteley (for Vasillyev).
(Yakutia-Diamonft)

GNEVUSHEV, M.A.; GOMON, G.O.; FUTERGENDLER, S.I.
-- - - . , ,
Relation of the luminescence of diamond to some of its other
properties, Min. abor, nool7:82-89 163, (MIRA 17:11)
1. Voesoyuznyy nauchno-inaledovatel'skiy geologicheakiy institut,
Leningrad.

G,'T't",II US HV, M.A.; 'I I V. I.; -, Plk, YF; . 1.
Book reviews Hinoboro 18 no.).361-.367 t,,4# CrIRA 18;3)
1. Vassoyuznyy nauchna-issledovatollokly j_rPologichozUy Instit-at,
Leningrad,

GNr-.VUSHEV,, M.A. 1 FMZRGENDLM, 8.1.
Trucen of magnatic melt in diamonds, Geol. i geofiz. no.2:155-157
165. (MIRA 18:0)
1. Voesoyuznyy nauchno-isoledovateltakly geologicbeekiy inatitutt
Leningrad.

11:11 ~! 7-1 H 111111MI1311041 I I IN MRIMIRII M IMM11 11141111 IMM1111 I IMI Wit, III I INH ;I.Ai III I 4F, 111.111 L'I HIM 11IM111, I
'0
ACC NRi A 0266k_l~_
AUTHOR: GnevuBhev, M.A.; Gomm, G.O.; FuteMendler, S.I.
ORG: none
00
TME: Connection between the luminescence of a dilemond and mcm of its other
properties
SOURCE: Ref. zh. Xhimiya, Abs. 12E3o
BEF SOUXE: Mineralog. sb! LIvovsk. geol. o-va EEi un-te, nof 17, 82-89~
TOPIC TAGS: diamond, luminescence, x ray analysic
TWISTATION: A study was made of the luminescence of more than 100 L d4amondo ri%= t~he
kimberlite shaft "Mir" (West Yakutiya); at the same time a atiidy waS conducted of the
morThological peculiarities of diamonds: coloring and degree of transparency. Sonte
of the samples were subjected to x-ray analysis. For certain S=4ss of the diammois,
a correlation was established between the luminescencent and roentSenostructural spec-
tra and the morphological characteristics. R. Khmellnitskiy.
SUB CODE: 20
Cnrd

GKZVUSIEV, M.V., otv :ed.; PiMINOV, O".V., red.izd-va; tIAKRUSI-11N, IVI.A.,
[Materials on the study of diamonds and diamond-potential
districts in the U.S.S.R.] Materialy po lzucheniiu almazov i
almazonoonykh raionov SSSR, Leningrad, 1960. 186 p. (Leningrad.
Vsesoiuznyi geologichaskii institut. Matorialy, no-40) (MIRA 14:7)
, (Diamonds)

q~EU.Simyj-Yladimir---Grigortypvich; MAGNOV, V.., red.; 141KWIJAWYA, 11.,
tekhne red,
(Pioneers of higher speed) Pionery bollshikh skorostei. Mo-
skva, Izd-vo TsKVLK,%t "Molodaia gvardiia," 1961, 31 p,
(HIM 15:1)
(Tractors)

GNVULMEV, V.V. Csnd 1,1;ed Sci -- (diss ) "Phyniolo6loul brises of the traittmeryt
of &164 contractures of the upper extremitien." St,!vropoll, 19157. 16 pp
(Stavropol! State lied Inst. Stavropollskiy Krny Exerciac-Therniri Dispensary),
200 copies (KL, 14-58, 116)
-100-

V V,
USSR/Iluman and Anirul Physioloay (liormal and Patholq:,,ical). T-10
Nervous Systant Pain,
Abs Jour Ref Zhur - Biolej 4o 16, 19581 75144
Author --,a=yushev, V,V.
Inst : Stavropollsk Medical Institutco
Title : on the PhysioloGioal Machanion of Alan, Contractors*
Orig Pub : Uche zaps Stavropollske mede in-ts 1957t vYPO 10 127-132.
Abstract : 63 patients with algia contractors (AC) were observed
which appeared as a result of fractureso sprains and
bruices of the upper extreLdties and were not accoLVanic-I
by clar-Ce of the nerve trunks. An active (per I.M.
Sechenov) rest showed a favorable effect on the condition
of AC., in the begimin(,? a siC~mificant one (increase of
the work ability and rate of the voluntary contractions,
weakeninG Of force of contractor contraction),, and then
Card 1/2

GNEVUSHEV V.V., dotsent
Need of inserting a correction in the calculation of the
normal vital capacity of the lungs according to lknthonyals
method. Uch. zap. Stavr. gos. mad. inst. 12AI44115 163.
Importance of deep, spaced respiration and sone characteristics
features of the development of fundamental habits furthering it.
Ibid.tll6-U7
Effect of deep, spaced respiration an the state of putmonary
ventilation in elderly persons. Ibid.t120-121
(KIRA 17: 9)
1. Kafedra fizicheskogo vospitaniya, lechebnoy fizulltury
i meditsinskogo kontrolya (zav. dotsent V.V. Gnevushev)
Stavropollskogo gosudarstvennogo meditsinskago institute.

GNEVUSHEV. V.V.. dotsent; PERESYPKIN, V.A.
Effect of deep, spaced respiration on the changes In some
oscillographic indices in elderly and old persons. Uch.
zap. Stavr. gos. med. inst. 12:1.18-119 163. (MIRA l7r9)
1. Kafedra fizicheskogo vdspitaniya, i vrachetmogo kontrolya
(zav. dotBent V.V. Gnevushev) Stavropollskogo goaudarstvennogo
meditsinskogo instituta.

GNEVUSHEV,, V.V., dotsent; KAILkSHUROV, Ye.S., kand. med. ntiuk; KRASNOV, Yu.F.,
a tent
Deep, spaced respiration as a factor iv :(~as-~-Orjrjg the
functional possibiiities of external respiration following
surgery for bronchial asthma. Uch. zap. Stavr. goso med.
inst. 12:258-259 163. (MIRA 17:9)
1. Kafedra obshchey khirurgii (zav. prof. Yu.S. Gilevich)
kafedra lechebnoy fizkulitury i VK (zav. dotsent V.V.
Gnevushev) Stavropollskogo gosudaretvennogo meditainskogo
institutae

GNEVUSHEV, V.V., dolusent; OSMIRKO, G.I., prepodavatell
Deep and spaced respiration as a form of active rest in the
educational process of schoolchildren of the lower grades.
Uch. zap. Stavr. gos. med. inst. 12:404-405 163. (MIRA 17:9)
1. Kafedra fizicheskogo vospitaniyat lechebnoy fizkulltury
i meditsenskogo kontrolya (zav. doteent Gnevushuv VS.)
Stavropol'skogo gosudarstvennogo meditsinakogo instituta.
&"6.d,. --F

GIEVUSEEVA Yelizaveta Ivanovna; GUBM, A.A., otv. red.; GAUUTF,19"
~-M--, ref'-iz-a--va, BERFSUVSKAYA, L.Sh.; teklin. red,
(In the land of throo-thousand islands; Russian sciointiots in
Indonesia]V strane trekh tysiach ostrovov,- rusakie ucherWe v
Indonezii. Moskva, Izd-vo vostochnoi lit-ry., 1962. 221 p.
(Indonesia-Russian exploration) (MnA 1519)

GIfEVUSHEVA, Yelizaveta Ivanovne,; LIPWS, Tu.G.,red.; VILMISKAYA. E.U..tekhn.red-
--- I... (Yorgotten traveler-,. life and travelis of Petr Ivanovich Pashiao)
Rabytyi outeshostvannik: 2hiznl i outeshestvita Petra Ivanovichm
Pashino. Moskva, Goo.. ird-vo geogr. lit-ry, 1958. 110 p-
(MIU 11:12)
(Fashino. Petr Ivenovich, 1838-1891)

Notablishes Ideal cooditions for o'beerysitioms'an Ow
saw corana, d1scuss" mass of the obip"tIOW i
iddah were conducted in 1938, 1941j. wA ~1942. 1, SOU
stated that there we processes wh1ch oa'm:w ii t".
carom& of the ova vhich very closely fljiluu 1 t~*
fission of the Draniva atm. Thwo we low IN":
thearies, however., ftich attempt to wM34iin tie milli.
MM "PhYsIcs (Contd) AL*: 19W
and as yet there: a, me
~siave from the solar carome, :I
derinite solutlaia to these pheiamena.

I.I. S. , GNEVYSHEV, M_. N. , OL A. 1. 1 RUBASIO, L. V.
2. USSR (600)
4. and Mathematics
7. Solar Activity and its Terrestrial Manifestations, M. S. Yeygenson, 11-I. N. Gnevyshev,
A. 1. 011, B. N. Rubashev.
(Moscow-Leningrad, State Technical Press, 1948). Rev!ewel by X. P. barsbushev,
Sov. Kniga, No.j. 1949.
9. M Report U-3081, 16 Jan. 1953s Unclassified.

FA 41T103
Y. N.
Sunspots
Sol" Phonmena
bowl
"The 22-year Cycle of Solar Activity.," M. N. GD&Vys
A. 1. 011, Palkove, Observatory., Acad Sci, USM, 3
"Astr, Zhur" Vol UV, No 1
Discusses the change in polarity of sunspots, and tb*
law of formation of the 22-year cycle frm the II-
year cycle.

A
111 1
a A
Sea
i Oka .111mis
UA 6 b. V 0 0
41 Q 0 GAS
39c. on the Nature of Uw Solar Particle* (0 Pr1rodo WmebrAych KorruaW)
17 2 m cam 100-422 (2948) 1k"1W (I& Itusplam)
The knows foots an polar sureres sad p~gatic aborm are best explained:
tr the "thesis of particle strewn origloating to the reglo" or
So 81 activity on the am's forfames Fm "m latitude distrIbution of the
go 4 1 intensities of the magnotle disturbuces, ON muthor ocacludes that a see
31 ,`~, vertical stream mists, 14be horlsoatal section of which can to evaluated
Is enob partioular saw. For strong mgmatic stem, the electric
current thus dotomimd roadwo 0o6 x 105 amp. Studies of the age
fluctuations In the goomigs"Is field show that the particle strewn

'a should be wismaUaW as elouis which, due to voloelty dispersion,
arth
assume an elongated shop while traveling from the mima to the
AssVele of the velocity distrilbotion gives as Ols at ymbable value
2696/11
TU
ti
d t
b
Th
2
I
f
10
t
5
3
3
/ COO
ra
oom
e
x
x
0ce
o o
A
s
o
e moo
.
.
#
pmbable empmaltion of solar streams would thus be a mIxturs of
at-parill4olos and &uW laMs" bellum allow. The voloally given
above closely approambes that ofek4ortiallse witted during thorime
disintegration (1020 x 10%W"). in this connection the author
A I 4I LOit~f (1) the fbdiag Ot tberilso 21soal. IN the poldrun of ow active
a

ee
regione on the am a mrfoem V C a mom mad A a KIM$ (IkkLAASM
00 Is AK bLM 36 (290) ad (2) Us Wpolbotled picture of nuclear 40 a
U a Ireas
.
tions In the sams, famated br K 1 Saba (In BAS Int S&I
O

1
-
141MULA (1942), ftes PZ
&M(L*'Aoa) dU 271
(1945)).

ur-n-ISHE'v, Y. -.
QuQvvahey, 14, fi. and Gnevysheva, R. S. - "The conrect ion Nitueen the Igws of Chnbe-
Wolf and of Sperrer", Byidleten' Komissil po Issledovanlyu SoIntua. (Aked. muk SM)
No. 1, 1949, p. 1-8
SO: U-4631, 16 Sept. 53, (Letopis Invkh Statey, No. 24, 1949).

-4-w-
4
y to Mis a 11 Is If M S

so A f 0."16
lor 1,04
11
000 FICKIIIII Aw #111,01st'll
.. - .- . 1...., .1
Sig.

00: see

goo
Coe
~
00. IJdMdw O
AM
h
k
A
r O 160
w
o
w o
z pm
p
Wa
dwAiiisu No 9 101 A 4N ft adw soma whhw an 7 voo
d"M
of
by wan
a Oweesswo inewbi is see
MOMAM C8880M 2 030 0 dWO Nii bOW.
P. Wwato coo
Joe
t gee
lies
I 8I L AGIVAMOLK&L L611414TWI CLOSWICAVOGIS
Sao., 11.10849.
19#adv 0.1 a.- .. ...... ....
-.-P, q --- --
u It I to a I IN tw a I IN, a Ip M 0 3
p
0 49 0 0 Ole 0 0 0 0 0 0 0 0 0 0 0 0 o oo 0 o 1* 0 o o go 0

G)E"SHKV, M. N.
21 J6* 51
am/Aptroapay - 8=
"ObsIrvations of the Solar Corons. Without EcIAP"s
in 6374-5-A%m*tmXA7* and Of Prominences In
6562.8-Angstrem Rays," M'. If. Onevyishey p H - 0 #
Gnavysheva, Ift Astr SU of Main Astr Obs, A~M
Sci USSR
"Dok A Nauk SM" Vol LXM., No 31 sfp 375;, 376.
Explains how subject photographo were succosofully
made, without eclipse., with quartz Uterferamee
polarization'filter designed by A. 18. Gultrars,
Inst of Cryst, A6&d Sci USSR. Aublaitted 24 NOY 50
by Aced S. 1. Vayflov.
17,322

sat
GriellihtV, Wjj' 00malit astrozarrilthilliala stantollia. r$ mcijni~jlfl 44tronrink2l I
tatidirl No. 9:47-12, Sept. 1033. .1 figs., tjkl 1111,~'-A V111nd
U S S ldescrip4ort of physical properties oftolarcurom and brki otitllneil INtop"ro-P-6
4C
Methods and results obtained. Tlie author qives s rather dcallni repert Ott 011 froAltht!"'ns
and operation of the. mcently orpniged Mutintain Atilroneintical Station stwo 10#10VMsk
(Caucasus 2130m)attached tothe hiaini'trstf'olll)lllir'iilObl,4lvntai'Y4(l~ull',O~'.)~c(fthtAcidt'MY I
of Sciences. FIgures thow thr. in%trum(nti and Wat! S)Wngraphli (A colows and spectr4
registered. Points out that the combiriation of inatniments mitl IV this Migio" Permit
simultaneous investigation (W Physical ronditic4ti in the d4tur1w I 1,11cri of tie .1gr at-
mosphere and individual formations in coitutction with all t~c othtt phenetit-tirt. The im-
portance o(simultaneous and rombined soidyis stlei,-*A anti trOverull TIIULk
of fruitless work when trying to investigate tolar phenriniann ~eliw!ji&tly fi,11111 41tho dow). ii
a&wjatedphenorneri.i. N1 uch at ten Con Is paid to t lie t mi III ng o4 900 111 Ific Pal. 111wel (lituiletits
of graduate coorseA from Leningrad and Kiev universitick). Svl'jea 4(roditsf-_ 1.
2.9uril3sorona J. Asttoomical observatories

GNEVTSHEV, M. N. and GNMSHEVA, R. S.
"Start of Regul&r Solar Corona Obsorvations Without Eclipse~oll.
Byul Komis. 22 issled. Solntea. AN SSSM, No. l0j, pp 60-620 1954.
The solar spectrograph of the Peak Astronomical Station of Kisloyodsk
mounted in 1952 is described. The spectrograph was basically intended for
the line 5303 A observation. The diameters of the mirror and the collimator
are 50 mm, the diffraction grating of Geraaimoyta work; the photographic
exposure is a few secondne (RZhAstrj No. 1s 1956)
SO: Sum No 884, 9 Apr 1956

ONEVYSHEV, M.N.; GNEYYSHgVA, R.S.
Characteristics of the solar corona and prominenceg, Dokl.AN SSSR 94
no.4:6)9-641 Y 054. kkhRA 7:2)
1. Gornaya astronomichaskaya stantelya Glavnoy astranoutcheekoy
observatorii Akadexii nauk SSSR. (Sun)

-;III' 1~'VV I I I 11111FIlm dh WHIM 1111
vt
awco
El 0 CAWXU IN tut
As %PA
I. F6 w!
hrl4f JIUMOVY Of tfi* OVfdhW* ~t# WJOMMMI*##~ Air$" I'la 1
1953 SA tb* emislobs (~Gcm *.G,cceoh*, ideadInad Iful li4,~
Wt M 4114A A ta apt4mad with Abi ?qVt4h4slA d It
(1948). 04
4v

i I - It - I 1~ ilt"Vit - I M. A11111 W1 LAIIIIIIHI FITAM 14jouqu I millRA1. 1 111; 1 It 1~ 11 1 -1 'It "j,
USER/Astro"nomy - Sun chromosphere
Card 1/1 Pub. 22 - 11/52
Authors j Gnevyshev, H. N., and GnevysheVa. R* Be
Title Brightness of the cronona line) 5302.8 in!1he a6lar chromosphere
Periodical t Dok. AN SSSR 101A, page 627j, Apr 1l 1953
Abstraot j Spectrograms are presented in an attempt to Orovoilthat the sun's
chromosphere consists of a mass of prominenc4)s and that the b~ace;between
them is filled with a corona, substance. The: coromit line, 5309 - 19 R, is
2). ~hto USSR references
clearly seen on the apectrograms (fig. 1 and:
(1950-1953). Illustrations.
Institution Acad. of Sc,O USSR., the Mountain Station of the Maiv Observa4~ry
Presented by: Academician G. A. Shayng January 1? 1955

.I V '1' m 14
I I P I M111 it MIAT M 11141111 gje~11;1 I!- q~mwljnl. I rii pI
USSR,/ Astronomy - Solar corona
Card 1/1 Pub. 22 - 10/47
Authors i Onevysh&'P-V, It. N. Iand Gneyvsheval R. S.
Title I Some results of the observations of the solar cavma 6utsido the, 6clijbse
Periodical I Dok. AN SSSR 101/6, 1017 - 1018v Apr. 21p 1955
Abstract I Some statements, expressed by the authors, concegnin~,Ithe Intensity Varia-
tions of the green, 5302.A, and the red, 6374.5X, Fpipctral linlels! in the
solar corona are presented. The phenomenon waviobserved by the:Wjthdrs
outside the eclipse. The g-reen line was widor 6bserytition sinceOelat-
ter part of 1952, and the red line since the b(,'41 Iinninj.11 -of 1953. !~ Pour' re-
ferences: 1 Germ. and 3 USSR (1950-1954). Graiihs; i1lustratio46.
Institution Acad. of Sc., USSR, the Main Astronomical Observatory;
*'resented by: Academician G. A. ShcWn, January 6, 1955

GNLFVYSHKV, M.N.; GIIMSHLVA, R.S.
New date on the solar corons. Ixv.Krym.astrofiz.obser. 16:
212-215 '56. (WRA 13:4)
1. (;ornaya aFitronomicheskaya stantalya Glavmy astranomichookoy
observatorii AN SSSR.
(Sun-Corona)

GNEVYSH171, M.N. I ArNEVYSHEVA, R.S.
0
Observations of line 5694
no.169:6-7 '56.
in the solar corona. Astron.tairk.
(NLRA 9:10)
1.GornWa astronomich*skaym stantsiya Glavnov astronomicheskoy
obsorvatoril A)mdmil muk SSSR,
(Sun-Corona)

-4-1?/19
..AUTHOR: Gnevyshev, M. N., Gnevysheva, R. S. and Kurt, V.G.
TITLE; Obser%-Ations of the infrared coronal lines 1(Y747 R and
10798 X. (0 nablyuden I infrakrasnykh koronallnykh
liniy 10?47 R i 10798E)
PERIODICAL: Astronomicheskiy Zhunial, 195?, Vol-34, No.4, pp.67-1-6 4
ABSTRACT: A method is described whereby the infrared lines of-the
corona. 1074? and 10798 R may be studied using an electron-
optical converter. This was developed at the Pulkovo
observatory in co-operation with theShternberg State
Astronomical Institute., Systematic observations are
being carried out at present using this method. In
addit . the helium lines 1OB30, and the hydrogen lines
10938iflof the Paschen series are being obtained during
the exposures. A preliminary comparison of 'the distribu-
tions of intensity in the inf rared lines rawd the mm
among themselvest anA also with the distribution of the
lines 5303 and 6374 X, has shown similarities in the
behaviour of the lines 1(Y?98, 1074? and 5303,R. This
may be explained by the near-equality of the~*.r ionisation
potentials. The behaviour of the line 6374 X differs
markedly from'the behaviour of the above three lines.
Curd 1/2 This in turn may be explained by a considemble difference

observations of the infrared coronal lines 101?4r/ and 10798
in the ionisation potentials of the line 63?4 R, and
confirms the correctness of the identification of the
lines. Iatest observations confirm thQ presence of the
luminescence in the helium line 10830 X at certain
places in the corona.
There are 3 figures, 2 tables and 4 references, all of
which are Slavic.
SUBMITTED: April, 10, 1957.
ASSOCIATION: The Mountain Astronomical Station of the Main
Astronomical Observatory of tile Aeademy of Sciences of
the USSR. rTheShternberg State Astronomical Institute.
(Gornaya Astronomicheskays Stantsiya Glavnoy Astronomi-
cheskoy Observatorii Akademii Wauk SSSR, Gos. Astronomi-
cheskiy In-T im. P. K. Shternberga).
AVAILABLE: Library of Congress
Card 2/2

A',JTH ':I:
Gnevy3hc.,v, A. 11' 7!10 - 5 6 - 9 - 113,'4 3
TITLE: The Astronomical Mountain Station Near Kisluvoffsk (?ia gornoy
astronomicheskoy stnntsii pod Xialovo:inko-i)
PEHIuDICAL: Vestnik Akademii nauk SSSR, 1958, Er n, pp. 10'T-109 (USSR)
AB4RACT: This mountain station which is affiliated to the Astronomi-
cal Central Observatory A'j j33H operates now for 10 years
(Fig 1). It was built for the observation of the sun corona.
The station is located 50 kilometres from Kislovodsk on a
mountain peak at an altitude of 2130 meters. The surrounding
low-topped mountain ranges anJ the absence of turbulent air
currents facilitate the photographic work in the observatory.
The station is also equipped with apparatus for the observa-
tion of the chromo- and the photosphere. Apart from the
coronograph the station is equipped with a photoheliograph,
with a chromosphere telescope, with a large diffraction opec-
trograph and with a radio interferometer for a wave length of
1,7 m. There is also a laboratory equipped with apparatus for
geo- and photometric measurements. The results of the obser-
Card 113 vations provide a rounded-off picture of proces;es in the sun.

The Astronomical Mountain Station Near Kinlovodak _t~V/30-58-8-18/43
Part of the equipment was built by the : Mt#ff IM. 3f the
Pulkovo observatory, the rest under the direction of P.V.
Dobychin and in the optical workshop of the Pulkovo observa-
tory under the supervision of V.G. Shroyber. The speotro-
graphs are equipped with diffraction gratings by F.M.
Gera imov. Interference-polarization filters by A.B. Gillvarg
and S.B. Ioffe were used. This work is supervised by the
Romissiya po iseledovaniyu Solntsa Akademii nauk SSSR (com-
mission of Solar Research,,AS USSR). The research program of
this mountain station incorporates systematic observations of
the sun spots, of sun eruptions, of floccull, of the magnetic
fields of the sun spots, of the "fibers", of the protuberances
and of the distribution of luminous intensity in the corona.
In 1954 it was found that at certain times helium lines can be
observed in the corons The observation of the infrared corona
lines 10747 and 10798 It was begun with the assistance of the
Gosudarstvennyy astronomicheskiy inatitut i-m. P.K. Shternberga
(state Astronomical Institute imeni P.K. Shternberg). Graduate
Stulents from the universities in :,Irj:ncow, Leningrad, Kiyev an't
Llvov as well as collaborators of the observatories in Chine,
Card 2/3 (Kitay), RoumEtnia (Rumyniya), Hungary (Vengriya) ana

The Antrunumical .'I'lountain :~tntion :.%ar r.inlovo4sk -";
-1
Czechoslowikia ( :flukho-ilovnki,,,a')' are oorAtinur-ovlv train(A in
ttli3 ntation.
'.'hora are 0l figuren.
Card 3/3

,/61/CW/005/023/042
S/0Y
A0OI/A101
AUTHOR: Gnevyshev, M.N.
TITIE: Technology and methods of coronal observations
PERIODICAL:- Referativnyy zhurnal. Astronomiya i Geodeziya, no. 5, 1961, 55, ab-
stract 5A361 (V sb. "Nablyudeniya Solntsa", Moscow, AN SSSR, 1959,
36 - 38, Engi. summary)
TEXT; The author points out that observations of the solar corona carried
oUt at various stations by different methods do not provide continuous series of
coronal data. He describes the methods of observations and processing employed
at the Gormaya stantaiya (Mountainous station) of the Pulkovo Observatory (Kis-
lovodsk). The experience of this station operation can be used to work out the
.most efficient methods for all coronal stations. The observational results of the
Mountadnous station at Kislovodsk and at the Pic-du-Midi Observatory are in good
agreement. A. 1),
(Abstracter's note: Complete translation]
Card 1/1

3 ( I )

AUTHOR: I , 'r
Gnevyshev, M. N., Candidate of 30100-59-5-"!311
Physical and Mathematical Sciences
TITLE: In the Astronomical Mountain Station (Zirt Gornoy
astronomicheskoy stantsii)
PERIODICAL: Vastnik Akademii nauk SSSR, 1959, Nr 51 PP 99-1C0 (US-11)
ABSTRACT: A photograph of a sodium cloud, ejected. by a. Soviet conmi-~
rocket "rias taken on JanuarY 3, 1959 In the mountain station
of the Pulkovo Main Observatory of the Academ,., of Scieno-~,s
of the USSR, situated near Kislovodsk at an altitude of
2000 m above sea level. The formation of' such a cloud had been
planned in order to determine optically the coorlinatos of
the rocket. I. S. Shklovskiy calculated thnt by the rlispersion
of about I'kg sodium a cloud of 100 km in diazzaeter forms
within several seconds; it is possible to record suc!i a rloijd
with the usual instruments. The photoirraph was taken by no!an-
abq
of special cameras mounted on tho toleacopi? of Fin . once-cf-
eclipse coronograph (Fig 1). Figure 2 shows I;he photograph
of such a sodium cloud In 80-fold magnification. Twenty iour
photographs were taken with a time of exponure of 20 second3
Card 1/1 each. There are 2 figures.
Card 1/1

S/033/60/037/02/004/01."'
E032/8914
AUTHOR: GnevypheY. M, N.
TITLE: The Connection Between Optical and Radio Emisaion of tae
Solar orona.
PERIODICAL: Astronomicheskiy.zhu:rnal, Vol 37, Nr 2, pp 227-235 (USSR)
,1960.
ABSTRACT: High quality and comprehensive non-eclipse observations
of the solar corona were carried out dizing the IGY. This
enabled more detailed comparisons to be carried out be-
tween the coronal radiation at X 5303 and meter waves,
and also geomagnetic disturbances. The present paper
reports on the heliographic distribution of intensity at
X 5303, the solid angle of radio emission in the meter
range vis a vis the optical emission of the corona. and
the connection between radio emission and geomagnetic
storms. All the results indicate that the optical, radio
and geomagnetic phenomena can be looked upon as a single
complex. A corpuscular stream having a solid. angle o1 the
order of 80 passes through the corona and causes the
emission. of the line X 5303 and a strong emission having
Cardl/3 a frequency of 200 Mc/s. The radio emission is excited lnt,'/13

S/033/60/037/02/004/013
E032/E911-
The Connection Between Optical and Radio Emission of the Solar
Corona
a cone which has the same solid angle as the geomagnati-
cally active corpuscular stream. A noise storm on meter
waves is usually observed 2-4 days before a geomagnetic,
storm. This is due to the fact that the corpuscular stream
is delayed by this interval of time before it, reachea the
Earth ~as compared with the radio emission). The intenoaty
V of the coronal line X 5303 has a maximum above sunspots.
Fig 1 shows the intensity distribution for this line with
latitude relative to spots. The apparent mwcimum of in-
tensity of coronal formations uccurs a day after their
Card 2/3

S/033/60/03?/02/004/Oi2
E032/E914
The Connection Between Optical and Radio Emission of the SoLryj-
Corona
passage through the East limb of the sun, or a (lay before
they cross the West limb. There are 5 figiLres and 18
neferences, of which 3 are French, 1 is Dutchi I is Swiss~
3 are Soviet and the rest are English.
ASSOCIATION: Glavnaya astronomicheskaya observatoriya Akademii nauk
SSSR (Main Astronomical Observatory, AcadeuV of Sciences USSR)
SUBMITTED: August 13, 1959.
Card 3/3

. N.
GtIMSIMY, M. 0.
"On the connection of coronal emission in optical wid radio spectrwa."
report to be sukimitted for the IAU Symposium on the Corona, Cloudcroft, Ntw
Mexico, 28-30 Aug 1961.

/0 t
AUTHOR t M.N.
TITLE: Sclar Eclipse on Februnry 15,
PERIODICAL; Akademiya nauk SSSR.. Veo "r, ~,k 31) K0, :5r X-r-s*? 141.
TEM The author teacribas the prepnr.,ttioit, mt,ie for t"~tl ob.~4(,rva-,Ion Df
the total solar eclipse made by the Astrorcmicheskiy jovet Akademi,. nauk
(Astronomical Council of the Academy of Sciences) as %YeLl as the observa-
tions themselves. For th,.s purpose it spee-tal zormawtosion headed by M, N.,
Gnevyshev was formed,, The calculation of datik of the solar VCliD'Se which
3 he preliminary
had been made by A A, 'Mikhaylov, the ma-p (Fig. 1). rn.1 t-,
data were sent to the astronomical radio and getjph,ysical ins"itutions and
published in the "Astronomicheskiy zhurn-Al" In the U85R the to-.7ns of
Yevpatoriya. Rostov-na-Donu, Novocherkassk. and Belebey -i.,erc- in the' center
of the zone of the total solar eclipse The maximum height of the sun and
the longest duration of the total phase wore observed at Rostov-na-Donu
and at the Krymskaya astrofizicheskaya observatorlya Akndemii nauk SSSR
(Crimean Astrophysical. Observatory of ft:i US.3H) The main
Card 1A

2
Solar Eclipse on Pebruary 15, 1961 31.0-5/11202
task wits the stud:,, of the outer solar ccrun-i E::P--t_ vori-- sent into
the zone of the total solar eclipse it oeri~,iz of geophysi-
cal rockets viere launched into this zone from which tho corona land the
changes in the earth's atmosphere during tho solar t~IOILPSe studied~ The
follov:irig obsQrvatioris are mentionodi ') Opt-.~.,ttlk ohierVIh-.I0n* The following
institutions took part in the observations;: institut A4111,
P, K, Shternberga (Astronomical Institu'e imi-,ni P K 3-_-it,~rn`,erg
Astrofizicheskaya observatoriya Akadeniii nat.~k Kztzak?,~jk,)J- iSSH ~'As trophy sical.
Observatory of the Academy of Sciences of the Kazakh3k~iy!_-t SSE *),
Astronomicheskaya oboervatoriya Leningradskogo iinilier;~It-ta (Astronomical
Observatory of Leningrad University), Inotitut fizLki. Akademii
nauk SSSR (Instit-ate of Physics of the Atrcsphere of' tho Acniiemy of Sciences
USSR), lnsti.tuL prikiladnoy geofiziki Akademii- nnuk SSSR (Institute of
Applied Geophysicj of the Academy of Sciences USSIO, lni5t_,tut -emnogo
magnetizma, ionosfQry i rasprostraneniya radiovoln Akadf~_-Iii nalik SSSR
(Instittite of Terrestrial 'Magnetism, Ionosphere Lind Rallo '.-datie Propagation
of the Academy of Sciences USSR). Ob!3ervations ,;ere mriile alicard a plane of
type TY - 104 (TU- 10.,') at a height of 10 k%i 'i!ie pl~iria was -.-~it at the
disposal of the Couri.,il "y the
Card 21

3/0'A0/%1/000/005/006/O!2
Solar Eclipse on February 15, 1961 B105/B202
institut greubdanskogo vozdushnogo flots, (Scientific Research Institute of
the Civil Air Fleet). Measures were taken to remove the clouds above the
Crimean Astrophysical Observatory, the Dzhankoy and Rostov-im-Donu. At the
Abastumanskaya observatoriya (Abastumpin, Observatory), Sveralovsk, and
Belebey, scientists succeeded in making observations after removal of the
clouds. Important preparative work was done at Lhe Gornaya astronomiches-
kaya. stantsiya (Astronamical Mountain Station) (Kislovodak). 2) Radio-
astronomical observations. They were made at 6 atation4i in Pulkovo. The
Krymakaya nauchnaya stantsiya (Crimean Scientific Stations) of the
Fizicheskiy institut im. P. N. Lebedeva. Akademii nauk SSSR (Mysics Insti-
tute imeni P. N. Lebedev of the Academy of Sciences USSR) made observations
1n.thetrange of the 20 and 80-cm waves and of the 1.45 aad 1,,63-m waves
(see Table). At the station of the Physics Institute al. Serpukhov observe-
tions were made by means of a giant radioteleacope of a diameter of 22 m.
.The Hail chn a -issl edovatel I skiy radiofizicheakiy institut (Radiophysical.
Scientific Research Institute) of the Gorlkovskiy univexsitet (Gorlkiy
University).made observations at Gorlkiy by means of a airror of I m dia-
meter. In Yalta observations were made by means or radloteloacopea with
a mirror diameter of 1.5 and 4 m. The Astrofiziclieskaya laboratoriya
Card 3/

L 11194-6 1)/FCC(w)/BDS/EEC-2/E;S(v)--AFFTC/E'D-3--ili-4/
ZWT(
Fe-4
AGGNs)?i�-Nftt AP3001233 S/0033/63/040/01))/0401/0412
AUTHOR: Gneyy*shey. ZA-A.
TITLE. Corona and the eleven-year cycle of solar activi,
SOURCE: Astronoxicheskiy zhurnal, v. 40, no. 3, 1963, 4,01-412
TOPIC TAGS: solar activity, solar corona, 11-year cycle, stin sp6tu, solar pivni~
nences, solar latitude effect
ABSTRACT: The author employs systematic data published in Clio QOhl,6terly Bull.etixi
on Solar ActVvity on measurements of the 5303-angstrom coroi3al-11no intensity per-
formed at the Kislovodsk, Pic-du-Midi, Mt. Norikura, ClImuix,, and Sacramento Peak
(New Mexico) solar observatories. Existing U.S. and French. comparisons, shoiring
that the measurements of Kislovodsk and Pic-du-Midi stationp araytrtually identi.-
cal, are confirmed. The present paper is fundamentally ba w4 n , correlationt; of
m and the Pio-du~-
the data of the other three stations with those of Kisloyo4j!e-
Midi (P). The data scatter on the correlation graph betwoen the U.S, -and Japanetie
stations against K and P is interpreted in terms of errors Ln photometric measuro-
ment, errors in the alignment of the spectrograph slit on the preseribed position
angle (especially in the presence of sharply delimited coronal rays), errors in the
Card 1/3
. . . . . . . . ...

L 11194-63
ACCESSION NR: AP3001233
determination of the distance from the photosphere at whit~h mmtsurseents of thil
coronal intensity are made, and lack of simultaneity in U, io met%surments. ~~ 'Yea' to-
year variations of the ratio of the 5303-angstrom line bellmeen the P and X 'Ns. Ahe
U.S. and the Mt. Norikurs stations are interpreted in te;mts of iinfortunate solec-
tions of observation days at Norikura which inadvertently,must bave fallen on days
with weak intensities of the coronal line, and In termts of lntens,u varlatio~s ot
the photometric system of the U.S. stations. The intensill~v of Ilib coronal amistsion
and the appearance of prominences and sunspots in the aurrimit 11 '--year cycle~are~
found to exhibit 2 maxima, equivalent in the total energy tuititted by the coivna~ 'and
the prominences; One during 1956-57, the other during 195!'11-60. t)uring tho1lrtt
maximum the emission intensity increased at all solar latitudes botween tho equator
and the poles, attaining a maximum at latitude 25 degrees. The tiecond max4mum -was
characterized by increases in emission intensity in the aqwitox-iiiI zone only, wi:th
a maximum attained at latitude 10-150. In either maximum did tho 9unspot activity
attain a maximum development one year before that of -the ma4inal,coronal enlosion,
so that tha latter occurred during the period of greatest dii,~.reano in the speit.
formation activity. It is noted that the second emission mitwimuta had remalji~,d U-
detected to date, because until now the characteristics of Alie spot-formation
activity, in the examination of the 11-year emission cycle, had been obtain04 by
summation over the entire disk of the sun. The following avguments are adduc 4d in
Card 2/3
---------------------- _- .................................
................................ -,--1 --------_--

L 11194-63
ACCESSION NR: AP3001233
favor of the applicability of the findings of the current cycls! to antecedaht 11-
year cycles:. (a) During all solar eclipses occurring in via:Idm%~i--i:LcUv3ty y'"rs of
various cycles, an increase in the coronal emission was inmrialil;V observed around
the entire solar disk, whereas In years close to a minimiatt intonaLva enission kiks
noted in the equatorial zone alone. (b) In all observed J."I.-year cycles theL lal""-
tudes of maximum emission decreases to a latitude of approx1mat0ly 10c) at nid-qycle
and remains essentially unchanged during the second half of the qycle. Tbelre a:re
5 tables and 11 figures.
ASSOCIATION: Gornaya astronomicheskaya. stantsiya Glavnoy Astronamicheskoy ibsewva-
torii Akademii nauk SSSR. Kislovodsk (bt Wd,jqjj_4ftjQA,
ical ount _Min Ai~
A
nomical Observatory, Acadwy !pf Scippoes. 5 R)
SUEMITTED: 28Feb63 IATE AOQD-. Oljul63 EM 00
SUB COM. AS, PH NO REP SOV: GOO OTHER: 000
Card 3/3

I I I iR I I i it I I i I H1 7; 1111 11111141; 1 W11, IR It 14ji 'Ij~fj S., I IF 4111-P 1111F.111 11:
IP J`1-
v6A~'-.4;49 'W -apq~ pt~. '()j/
-65 F
24525 IF /EwG(v)'/f'CC DIA~d)/FEC-,4~~,W
~T
M-4 SOW b)/,9,SD/" 40 /AFFTR
ACCESSION NR 046553 BOOK EXPLO
V. pe Dobrovoll0kiy'. 04 AE I I rk
tg*n, -All Ve i
A. V.1 MOIChanov A. F.; Sobolev V. H .8haranov
dn4,
A course in astrophysics and hUUar antroncmyo 3 Mwmll~mtrbeimikl I z
astranonii. to 3)j Roscowt fa-d-vo "Wauka"P.1964, )75 114ip "blio..
indices, 2,150 copiao printed*
TO)FIN TAGSt a3troptUmatical, staUar astronmy
It
TABLE OF CONTEMS (abridgedli
F ord -- 7
P=1 * The Sun
Ch, Is Introduction
Ch. II. Linear spectrm of the wm -'24
Ch, III. Structure of the phatospherej granulatlians "1116 1w; Is i! 41
Ch. IV. Chromosphere 69
Ch, Ve Protuberances 108
Ch, VI. Chrowsphere flares 130
Cho.VII, Solar corona - 144
Card

I WIR'N If 4 1 HIM HIP:
L.24525-65
ACCESSION NR AMkO40598
Ch, VIM Solar service 164
Ch. IX, Solar radio emission - 176
Part 2. Plans systen

6 226
Ch. X.
Ch* XI. Physics of the planets 250
Ch. XII, Description of the nature of asper;Ltq 0=11~
Ch. XIII. 'Mysical, properties of 4MkJJj" A* " 309:
Che XIV, 9gm0s ms teore
,and 11odiaggl llg bf~rji&
,
Index of nwassT-
Subject indez 373
SUB CODBt AA
MM 1 107
card 2P

L1078,*,-65 W(1)/&1G(v)/EEC_h/ M,, M/Fcc "Apiul IVES: t I) vil
ACCESSION NR: AP4047157 Wom/e#041/005/09,37)
AUTHOR: S-a1rA*13hLy! M, 1. Sazomv
low
TITLE: Influence of solu activity an Proc%ses In the earthfill
SOURCE: Aetrowailobeakty zhurua, v. 41, no, S. 1D04, 931-041'
TOPH', TAGS: solar activiW lower atmouphere, solar corposoubli iradt, prosal a
t Of JetiVe ProeegoeS c11 tljo eft i 'C~Iiom 'I'lli: ~4b- y theI
ABSTRACT: The developmen
emission of solar ultraviolet radiation, corpuscular radiation town Was I j~ W ilia rat 6
range, These roAlations, upon roaching the carth"hi atmoophere.; 4088'~ fill '041 in 11 .01
are manifested most strongly in the upper layers of the atmoisphe~ t hi 1g, Iarent(i tbol
60-70 km. Their influence on thei lower atmosphere Is lans PrOO dh
which have been made on this subject are contrs&dtory In thmir,000 'avid g0a
Oft. 0 th
authors have concluded Umt solar activity has Awo effro n
present authora attributer these negalive conclusions to or ffs"t 1~01111 it 111 51"1 1 ;1
an effort to find universal relatioashilps En different geograplao rol I ins I) I ei IF thil 1:
0 proo I !J
taking Into account the great complexity of tropospherl ess6A 1:1 Lre highl'). Ia-'
pandont on. the properties of the anderlying surftc6f, wagon., UM~3' I'd irjkJ;WflPhI!
card 1/3

jI, I if )I I) Jill q I! w I
'L 10763-6co-'
ACCESSION NR: AP4047167
position and initial conditions' dO~
causing the effect of golar actlvitk~ti i~e 1~1
ferently in different regions; 2) In most casen, theae axithorm lkav!a~!i~Js nolices
Cf s,,1j11r,*
activity (such as Wolf numbers or sunspot area) wlttcjli are n I thu'lv L
of the energy of that solar radiation which to of Im Nrtnice flir proi 11ascif OR tho onrtlrs
lower atmosphere. This article Is essentiaUyat;ynopsloof.ceittil~i:ari,,ijcnii~nt-swhici!i!
demonstrate the influence of soltu.- activity onthe lower atmospli6ro, :projmt~,ied oarli(ii~, by
azonov, Vy* sotny*ye baxichesklye obraz 1~jyaifl; 3 so)[ iv ~hilr . -11
the authors (D. 1. S,
"vnostf,. Gidrometeolzdat, 1064; M. N. GneWahev, Antron 04, ~ 401! PjAA12, 11196).
In the first of these studies, on the basis of an mialysis. of 12, ~111;h-jrr IfI111 IntsBurof
charts of the northern hemisphere, Sammov drew ImporUnt touttilgonai jd6ceraing We
occurrence of regions with the most frequent extreme deviallons oil:1 i~req~, 4i-e: from 0,~
norm. It was found that &.e regions of maximum frequency of noullhaun), I' )j,*cse*rc Ailf`n
ring-like zone similar to the attroral zono; a sinillar ring-like, z", 1115 101-ji0cil for 011-
tremely low pressure values. It waa shown that with
he pao4salgol, il,r, larl o lqppt grouj)o,
across the sun's central meridirLa thoro in a pressure Incre.Ase ijill.,he i ititwi-a foridallon 1
of the first zone and a pressure decroade Lit (lie second, It Is cone
evidence that the agent stimulating the development of PressUre atli 441 i~ 1ho atlr~Lto-
ophere'and upper troposphere Is solar oorpuscular radiation, L WJJ6 I" 1 8!
determined by the earth's magnetic field. The reoction of the la ,4i 11,I,,. ab'lf ollphore Iviijibavi
a different sigu, depending,on Ute region. Although this regloft 1A 63fine, l(Parly 1~ ~he
2/3
Card
37 1TJM7"_
77) 777 7 KITITiMIT T=TJ11777"77 I
'k
Ewa
I

stratoal0tere and upper trope spbere, it becomes n;itich less 61alu t 40fh imli 0 W, Yr
a of Ile
layers due to the influence of the thermal, mochakilcal mid tod]JA pe~', ~11~j
undorlybig surface.
coronal line N 53-03 demonstrates that solar activity to tinklad 411illijoly 16 ~1111.1111;oq in ~thqf
,~111 a
)oar
earth's lower atmosphere. The distribution of prolsou.ro fovill"it"s0t) iw till! li- is Afix
cycle has two maxima which coftiolde with the IntenattY rawdtnidRj~il~)F thil.1 doearl I 1111L
ax
The behavior of both the line and the pressure formattoas 16 dxRrjjjLjj
iinch lj~, nol c6ipuo~
cular radiatiou. Orig. art. hav.- 2 figuras.
10SR stro Rile I
ASSOCIATIO14: Glavnaya astronomicheskaya obsbrvatortyi, Mj'i I , -
Glavneya gooffticheskayg obtjvrvatoflyjx~~l J14
(Mein Geophysical Observatoull
L
SM3MITTED: 10AprG4 FNCL-. 00;, Ail,
A
NO REP SOV. 004 OTHER. 000 1
T
3/3
'I Card

I ~ -j , cii. ".1 11 lli.jll" Lr)k , A. '~ . , , ;Av.
- ~ ~; L -' ; ! :, ." , , " ., ~-, t
i f X , ..
4 1
red. ;
LFKislovr,dsk Launt.--An Astronomical Ob-ooninioryl KAjilovoil.~kmia
gornaia notrozion.1ch,3kaia otantoiia. Mookwi, Vftuli.fi, 1965.
47 p. (MLU 18:8)

- l7l-
A
-6
j&7
%4100:,
ACCESSION NR 5
AM dtiiM
HOR: Gnevyshev, M. N.(Candidate of physidowathematic ii ceai)
N
TITLE: New data un solar activity and its influience:on th I
SOURCE: AN SSSR. Vestnik, no. 5, 19652 67-T1
TOPIC TAGS: solar activity, solar terrestrial relation j Bois'. cya') e dullspots
bicastronautics, coronal emission
ABSTRACT: On the basis of coronal investigations conducted 41'. the !I i0ovodsk
Mountain Station of the Main Aztroncmical Observatory of the j,de:ii), r':Seienale 1
USSR during the IGY, IGC, and IQSY, it has been established ~ th d; t1j( 11-ormiLl 11 Rea~
solar cycle has two, essentially different, maxima. During, th Pei'. 6d. of the ~f Lr.,:jt
naximun the intensity-of coronal radiation increases unitbrul~, Iove~, t" ~e entire
s t e
solar disk, shoving maximal intensity at a solar: latitude of*6ut
first maximum diminishes, a second maximum appears 6 the'eqi[cilbri4j..; Iregion,
exhibiting maximal intensity at a solar latitude orabouii 10 EVI(ii: il,.hough t~e
second maximum ia restricted to the equatorial regi6n, it ini l'i'les i, i,.14! (Une =0 Int
of radiation as the first maximum. The.establishment,of the 6o a >le I jc~ iirity m4x,
"Ln the 11-yqar solar cycle clarifies certain diderebancidis.rAptfll il ;C ~rrelati 9
ard 1/2
Ic
t lf!-~ F I' I q ifl 1. 11 "'1111j'JU, it; I i;