SCIENTIFIC ABSTRACT FOMENKO, B. A. - FOMENKO, I.A.

• Document Type: CREST
• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R000413420012-4
• Release Decision: RIF
• Original Classification: S
• Document Page Count: 100
• Document Creation Date: November 2, 2016
• Document Release Date: August 23, 2000
• Sequence Number: 12
• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT

:ACCESSION NO: AP3006764 s/019O/63/005/009/1393/1397
AUTHORSt Fomankof D, h,; Volodin, V, Ps; Sidorovioh, A. F.; Xuvehinskiy, Ye. V.
TITLE; Thermomechanical investigations of polyisobutylene by means of dilation and
penetration
SOURCE: Vy*sokomolekulyarny*ye ooyedineniyal Y. 5, no. 9, 1963, 1393-1397
TOPIC TAGS: polymor, thermal oxidation, single axis elongation, polyisobutylene,
amorphoun polymer, thermomechanics
ABSTRACT: The lovr-molecular-weight polymer was prephred by means of thermal
oxidation decomposition of the hich-molecular-weiGht product, heating- the latter
in air -at 160-~70C for 50 hours. The characteristic molecular weights 11W, and MW2
were 0-55 x 10 and 1.86 x 106 respectively. The method of investigation
consisted of single-axis elongation of a film strip under a constant force, and
penetration by a 3-mm cylindrical indentor under a gradual temperature rise. The
results chow behavior of polyisobutylone analogous to other linear polymers. As in
,other amorphous polymer deformations, a sharp branch in the thermomechanical curve
of polyisobutylene shows a"superelastic behavior, Orig. art. has, 4 figures.
Card 1/2

~ACCESSION NO: AP3oo6764
~ASSOCIATIOM Tristitut vy*ookomolokulyarr (Institute of
q*kh soyedinaniy AN SSSR
High-Major,%LLar-Jet X~t Compounds AN SSSR)
DATE ACqt 3Wep63 EXCL: 00
SUB COM CH NO REP SOVt 008 OTWM: 000
Card 2/2

GARCHEV, Petr Ivanovich(Harchev, P.I.1; MALKIYELI, Semen
Veniaminovich [Malkiiell.. S.V.]; LQ,.AA,,,red.;
LIMANOVA, M.I... tekhn. red.
[Lenin Collective Farm in Lebedin DiBtrict of SaW
Province] Kolhosp imeni Lenina Lebedynskoho raionu na
Sumshchyni. Kharkivy Kharkivslke kriyzhkove vyd-vo,
1963. 90 p. (MIRA 17:1)

F01-04KOP B.A.; ORLOV, V.A.1 TARAXANOV, O.G.
Studying the kinetics of polyurethane formatica by the change of
the specific volumetric resistance of the thermosetting(system.
Plast.massy no.lOt47-49 164- MIRA 17310)

L 24116-66 FYJTk 1)/EWPk m)/,EWA(d)/T-2/rWA(1) IJPr%O)
ACC NRs AP6011515 SOME COM. UR/0382/66766676-617667476RZ4
AUTHOR: Vulie,,,L, A.1-Fomen!:00 B. A.
ORG: none
TITLE: Transient conditions of flow in,magnetohydrod mice
yn
SOURCE: Magaitneya gidrodinmika, no. 1, 1966, 74-84
TOPIC TAGS: magnetohydrodynamics, transient flowj conductive fluid, laminar flow#
Reynolds number
ABSTRACT: A discussion is presented of the qualitative (haractbrittles of a conducting
3-iquid flow in a channel In the presence ofa magnetic field In the transient region
of the flow between the laminar and turbulent flows. Interpolation fo-rmulas for the
friction coe ficient as a function of Reynolds and Hartmann numbers are analyzed,
Theoretical data am compared with the experimental results. Orig. art. has:
9 figures and 16 formulas* (Based on authors' abstract] ENrl
Card 1/1- -11al UDC: 538.4
un,~~=
UK 11 F1501-

Faimmu, B.Ij.
Meteorological observations during the solar eclipse of June 30, 1954.
Biul.VAGO no.20:1q-50 '57. (ISTa 10.- 13)
I.StaltrkKradskly pedagogicheekty institut.
(Eclipses, Solar--1954)
(Metecrology-Observations)

FOMENKO. B.D.
Variations of the coefficient of atmospheric transparency during
the total solar eclipse of June) 30, 1954 [with summary in Frenchl.
Astron. zhur. 34 no.6.-868-882 N-D 57. (MIRA 11:2)
1. Stalingradekly pedagogicheekly institut I Gosudarstvannyy
antronomichankly Inatitut In, PK. Shternberga.
(3clipses, Sblar--1954) (Atmospheric transparenc7)

so) "Change in the
e During the Total
Solar Eclipse of 30 June 1954.1' Mosp 1957. 6 pp 22 cm. (Mos State
Univ im M, V. xxvWMxNvIY Lomonosov, State Astronomical Inst im
P. K. Shternberg), 100 copies (KL, 26-57, lo4)
- 14 -

FOMENKO, B.D.
Aurora borealis In Stalingrad. Astron.tair. no.185:24-25 0 157.
(MIRA 11:4)
(Auroras)

KLIKM 0, 1.7e.; -, FOMMO, B.D.
Some problems in observing artificial earth satellites* Biul.
sta.opt.nabl.isk.sput.Zem. no.6:8-10 159.
(MM 13:6)
1. Stalingradskaya stantsiya nablyadaniya iskusstvonnykh
gputnikov Zemli.
(Artificial satellites-Tracking)

FOMENKO, B.D. (Stalingrad)
Ghanges in the total &4 scattered solar radiation during
the oolar eclipse of June 30, 1954, oboorved in fikhoretsk and
Sal'sk. Biul.VAGO- no.?kn?-W 159, (MM 13:4)
1. Stalingradekoye otdolenlye Yeesoyusnogo astronomoq4o ~821-:-
chaskogo obshchestva.
(Eclipses, Solar--1954)
(Solar radiation-Observations)

SID
PHASE 1 BOOK EXPLO:TATIO-1 f,, V/ 5 5 7 5
Akademiya nauk SSSR. Aatronom-icheakiy sovet.
Byulleten' stantniy opticheikogn nablyudenlya inku3Atvennykh
sputnikov Zemli, no. 6. (Bulletin of the Stationq for Cplieal
Obaervation of Artificial Earth Satellitea. ria. 6) Mlojl:tow,
1959. 23 p. 500 copies printed.
Sponuoring Agency: Astronomiehe:ikiy novot Akadtrilll nauk 333)jR.
Rc3p. Ed. : Ye. 2. G-Indin; Secretary: 0. A. Sc~v6rraya.
PLWOSE : This bullotin is intended for scientists and ergineor,3
ccneerned with optical tracking of artificial ciatellltc3.
COVERAGE : The bulletin contains 9 article3 which prp-3Ent, the
reaults of 3atellite observationa, and dencr-lbe methoda anl
specific equipment used for photographic obs,~rvatirr. of eilrth
natellites. An appendix contains a listing o0 84 Sov-1et satel-
lite observation statlona w1th station number. No perzonalll;leoi
Card 1/0,

13ullptin of the 5tationa (Cont. 07 1-, -Ir /5 c; 7 f;
are mentiencd. There are no referencea.
TABLE OF CONTRIT.").
Panova 0 V T. Yp. SynhzhDnko, D. ~A. Fllrag,;, an! D. 1~
ShchZo**ie~ [GlrvnayP- -~iir-
v-,toriya AN MR - Ma-In ~Ilulkcvo) Aat;ronc----I-.i cf thc
Acadcmy of Sciencez of the USSR]. Ob-ervatlcr.3 cf Vi- S-~c-crd
Artificial Earth Satellite (1957 0) at, Sta--cn No. 039 !F~ilkovol
(Obcervations: B. A. Firago, D. D. Foic --hen t. ~tr;v, V. karova,
N. M. Bronnikova. Measuremenla ard Galcul~t:Lpn,: Y~. ~Y.:;n:'enkc
G. V. Panova, D. Ye. Sh3hagolavj B. A. FIrago, and
leva)
!--ngauer G G. [ Main (Pulkovo) AntroncxIc Gb~lsrvatrry of the
0;-~~of ~-.iences of the ITSSR]. On Methodn for 11reci:3c
graphic Determinations of the Positions of Artificial Earth Zatel-
lites
Cara 2/16

Luliu'.In of tile "'tationa (Con'..)
Klimenko, I. Ye., and B. D. Fomazlko (Stalingradnkaya .3tantzllya
I -oil
nablyudeniya 1SZ - Stall-n-gr-a-T-S-ae.11itc Tracking Station]
Some Froblcmz in the Methcd of Satellite Obcc--vat'-on 8
K,husainov, S. Kh., and Sh. Karatayev (Stantulya nablyt,&-niya 2:SZ
pri Kzyj - Ordinskom Soz. pcdinzt!',,ate - Satell-Ita '4ra~klng
Station at the Kzy3. - Orda State Pcda2p&~_cal inat-f%ute). Table
of the Conversion of Horizontal Coordinates Into Equatorial Co-
ordinates io
Eynasto, Ya., and U. Veyamann (Inatitut fizilci i actrcilomti
P11 E33R - 3tantaiya nablyudeniya spixtnlkov pr! Tartuckom go3-
dar3tvenno"m universitate - Institute of Fhynics and of
the Academy of Sciences of the Eutonian Solilat Sociai-IL;. Republic.
Satellite Tracking Station at Tartu Stat3 Univeraityj. Pic-elim-
inary Results of Using Automatic Recording in Theodolite Satel-
lite Observations 11
Zatsiorakiy, L. M. [Main (Pulkovo) Astronomic. Observatory). Modift-
Card 3/6
IT
-1 --, ~*,6.Ai.~~ft-;.~A,2~-J~z a .
pji

.S/169/62/000/004/01 8/103
D228/D302
AUTHORS: Pariyskiy, N. N., Hu Jen-Chlao, Pomenklo, B. D. and
Gindilis, L. M.
TITL'-';A: Chano-es in the ozone
0 layer during the annular solar
eclipse of April 19, 1958, on Hainan Island
PERIODICAL:. Referativnyy zhurnal, Geofizika, no. 4, 19062, 7, ab-
stract 4B68 (Acta geo phys. 31nica, 10, no. 1, 1961,
1-16)
TEXT: A Sino-Soviet group ihvestigated the ozone content from so-
lar-ecliuse observations during the annular solar eclipse of April
19, 1958 $ on Hainan island. A spectrograph, which was employed to
-he counter-radiance,
observe simultaneously -the zodiacal light and t
was used in the observations. The observational procedure and the
processing of the resulting data are described. The results show
1hat the content of atmospheric ozone changes conspicuously during
a solar eclipse. It is noted that the concentration rises up to
moment half an hour after the middle of the eclipse; the lay-
Ca rd 1/2

S/169/62/000/004/018/103~
Changes in the ozone ... D228/D302
-e:
yer's thickness thensubsequently decreases. Z-Abstracter's not
Complete translation. j
Card 2/2

39090
S/169/62/000/006/071/093
D228/D304
Fomenko
A.VTHOR: ._D__
121TLE': The synoptic relation of solar activity to processes
in the troposphere
D-".HODICAL: Referativnyy(zhurnal, Geofizika, no. 6, 1962, 8, ab-
st.ract 6G40 Solnechnyye dannyye, no. 9, 196117 _78)
T.','~'XT: Local high-temperature coronal areas over the sun's active
regiono generate high-energy corpuscles, ensuring the high elec-
0 LD
zron temperature of coronal -as at the distance of the earth's
pmen %
orbit (Chapman (Che I model of an extended curona). The solu-
Uion of the heat-conductivity equation shows that the ionosphere's-
heo-zino- in a comoaratively short time and the development of syn-
op-~ c-type tropospheric disturbances, associated with this heating,
can be guaranteed only by high-speed flows of corpuscles. Such a LY
mechanism leads to tropospheric disturbances only in years o~
high solar activity; in years of minimum activity there are no lo-
C)
cal areas of heating, since local high-temperature coronal areas
Card 1/2

39090
S/169/62/000/006/071/093
The sy.n.optic relation ... D228/ff3O4
are absent over the active regions. The coefficients of correla-
t4or bQ-,,vieen the level of solar activity, characterized by the
~~rea )f suns-00ts and the change in the atmospheric pressure (the
at-mos-)here's local heating must lead to airmass movement and con-
4,,jqu,n-cly -11o pressure changes) were calculated from the data of
Mleteorologic stations near Volgograd in order to verify these con-
siderati-ons. Very low values for the coefficients, when there is
practu-ically no relation, are also found in addition to high values.
7C-L.e Coefficients are of different signs. It is supposed that for
t-"--.e earth's local areas the simultaneous effect of two types of
soia_-, ac-uivi-'Uy influence on the troposphere may hamper the ex-
posure of this correlation. On the whole the correlative dependence
bears a pulsatory character, reflecting the pulsatory nature of-
~.he solar activity itself. Abstracter's note: Complete transla-
tion.-7
C~_.vd e2/2

S/16 62/000/009/079/120
D228YD307
AUTHOR: Fomenko, B. D.
TITLE: Variation in the atmospheric transparency factor in
the spb tral sections 2900-5250, 5250-6250, and 6250-'
20,000 R during'a solar eclipse
PERIODICAL: Referativnyy zhurnal, Geofizikaj no. 9, 1962f 29, ab-
stract 9B175 (Uch zap. Stalingr. gos. ped. in-ta,
no. 11, 1959, 61-i9)
TEXT: Measurements were made on an actinometer with Schott (Shott)
filters near Tikhoretsk during the solar fflalips6 of June 30, 1954..
The transparency factors were computed from the formula of Bouguer.
Using the distribution of solar energy at the atM08phere's upper
.boundary (So,,0, the values df So,,6x were calculated for three cho-,
sen spectral sections and for the eclipse's different phases. The -
tranapaxency factors for the eclipse's different phases were deter-
_Mined from the measurement data and the calculated values of S
BRr jhj/�rounds,of the relations obtained the author. supposes the

'S/169/62/000/009/079/'120
Variation in the atmospheric D228/D307
increase in the transparency factor in the short-wave spectral sea
tion, when the eclipse's phases are ~0.95, to be connected with
the fact that the amount of ozone,decreaBed by 1/3 during the
eclipse. This occurs in consequence of the effect whereby the so-,
lar disc is' da'tkOied from the center.towards the edge, when the
share of the intensity of ozone-forming radiation diminishes as
compared with.*that''of ozone-diBintegrating radiation. The result-
ing increase in the transparency.factor,during the eclipse in the
ldng-wave spectral section is related to the increase in.the abso-,-
lute humidity that occurred as a result.-of-the-ohanged synoptic
:conditions. ~_Abstraoterle note: Gomplete translation,_7
Card.2/2

FOMENKO, B.D.
Meteorological observations during the total solar eclipse'of
February 15, 1961, in Volgograd Province. Biul.VAGO no-321
32-34 162. (KRA 15sll)
1. Volgogradskoye otdeleniye Vsesoyuznogo astronomo-geodezicheskogo
obshchestva.
(Eclipses, Solar-1961)
(Volgograd Province-Moteorology,-Observations)

7-
S/886
0 W
i/62/000/600/0 2/0
D207/D308
AALWHORS:, I'ariybltiy, 'N.N., HU Jen-chlao, Fomenka,B
D.,and
~ITLL
Measurements of the ozone layer during the annular
solar eclipse on April 19, 1958, on'Hainan Island
SOURCE: Sbornik trudov XGU po Nezhdunarodnomu geofizicheskoml
Zodu; astronomiya. Gloscow) Izd-vo Mosk. univ., 1962'9
31-53
TZXT-. The observations during the eclipse were carried ouV
by a joint Soviet-Chinese expedition led on behalf of the USSR Acad-!
emy of Sciences by A.11. Holchanov, and on behalf of the Chinese
Academy of Sciences by Chleng Fang-yung. The expedition was organ-
ized by the Chairman of the ikstronomicheskiy sovet LUI SSSR (Astron-
omical Council, AS USSR) A.A. Milthaylov and his deputy B.V. Kukarkin.
On the Chinese side there was a special committee led by the Vice- i
President of the Chinese Academy of Sciences Vh, Yu-hsiung. The opti"
:cal group included N.N. Pariyskiy of the Inatitut fiziki Zemli AN
C ard 1/:5

S/886/62/000/000 002/003
-Measurements of the ozone D207/D308
SSSR (Institute of Physics of the Earth, AS USSR) and the Gosudarst-ii
vennyy astronomicheskiy iiastitut im. P.K. Shternberga (State Aatron-~
omical Institute imeni P.K. Shternberg), L.M. Gindilis of the State
As-ronomical Institute itueni P.K. Shternberg, Eu Jen-chlao, and Yu
jen, 6oth-of the Peking Geophysical Institute of the Academy of';
Hal
Sciences of the Chinese People's 111epublic. The optical group was
led by N.N. Pariysltiy. The results were analyzed by B.D. Fomenko
of the Stalingradskiy pedagogicheskiy institut im. A.S. Serafimovi-
cha (Stalingrad Pedagogical Institute imeni A.S. Serafimovich) under'
the direction of N.N. Pariyskiy. The time service was provided by
the Chinese scientists Chleng Fang-yung and Wang Shou-1cuan. The
observations were carried out at the south extremity of Hainan Is-
land at a latitude of about + 180.3. The varic.tions in the ozone
layer thickness during 'the eclipse were observed together vrith the
gegenschein using a very-high-speed nebular spectrograph HKC WKS)
with quartz-lithiura fluoride optical parts; the spectrograph is A
described in detail in the article of N.N. Pariyskiy and L.M. Gindi-
lis. Since the NKS spectrograph was designed primarily for observa--
of the gegenschein and zodiacal ligri~ C ~j
ht, a special photometri
Card-
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, 7-. . --- - - - --
.
I ~.4 - r - .
-, .", q, " , ; ~': .. .I ~ j..
-~I- -
w-, -~ 'A M, I a ~~ -,- I ".

4149o
S/033/62/039/005/003/011
3 E032/E314
A~THOR:
Pomenico., B.D.
TITLE- Properties of type-M solar corpuscular streams as
deduced from an analysis of their influence on the
troposphere
PERIODICAL: Astronomicheskiyzhurnal, v. .39, no. 5, 1962,
833 - 839
TEXT: A statistical analysts is reported of the correlation
between plages and tropospheric disturbances for the descending
branch of solar activity when the relative Wolf number is in
the range 15 < R < 75- 719 plages were includeO in the analysis
covering the period 1906. - 1952. The obs ervatiomml material was
taken from the data on the passage of'plages through the solar
centre, as reported by the Sluthba Solntsa-SSSR (Solar Service,
SSSR),Meudon, Coimbrei Guadalcanal and Mount Wilson observatories.
A full list of -the data is given in the papers of E.R. Mustel I
(Astron.zh., 38, 28, 1961; 39, 813, 1962).' The analysis also
includes meteorological data on atmospheric pressure for
Ooscow, Tbilisi, Volgogradj Archangel and Omak. The superimposed
Card 1/3

S/033/62/039/005/003/011
Properties of .... E032/E314
epoch method is used to analyse the data. Inspection of the
statistical curves shows that they all have a maximum at about
d
Zt = 6 and this suggests that the maximum disturbances in the
lower layers o~ the EarthIs atmosphere occur six days af'ter the
passage of the plages through the centre of the solar disc.
There are further secondary maxima to the left of the principal
maximum at Z\t = 6 but these are ascribed to the longitudinal
distribution of plages on the Sun. It is argued that these
curves indicate that type-M 6orpuscular streams arq responsible
for an increase in the pressure in the lower layers of the
terrestrial atmosphere. The fact that this effect occurs in the
entire atmosphere is indicated by Fig. 3, in which the statis-
tical curves for the seven points mentioned above are given
(curves 1-7, respectively)* Curves 5-7 refer to night obser-
vations. In all cases, the maximum occurs at.L t = 6 days. The
general conclusion 15 that there is a definite correlation
between atmospheric disturbance and plagea, that the atmospheric
disturbances reach a maximum after an average interval of six
Card 2/3

S/033/62/039/005/003/011
Properties of .... E032/E3i4
days after the passage of the plages through the.centre of
the disc, that the atmospheric disturbances in the lower layers
of the atmosphere are accompanied by an increase in the
atmospheric pressure and that the plages are the main sourcea
of corpuscular streams. There are 3 figures and Itable.
ASSOCIATION: Volgogradskiy pedagogicheskiy institut
(Volgograd Pedagogical Institute)
SUBMITTED: October 15, 1961
Card 3/3

--LCKUKPs,_D.D-.---
Calculating relative changes tyrthe atmospheric transparency
coefficient during a solar eclipse, Biul, VAGO no.33:3.6-18
163. (MIRA 1614)
L Volgogradskoye otdalaniya Voesoyuznogo astronomo-geodezi-
cheskojo Obahchestva.
Eclipses, Solar)
~Atmoapheric transparency)

ACCESSIONNR: AT4016594 B/2556/63/000/034/0003/0004
AUTHOR: Fomenko, B. D.
TITLE: Solar corpuscular streams of active regions and atmospheric disturbances
SOURCE: Vsesoyuznoye astronomo-geodezicheskoye obBhchestvo. Byulletin', no. 34,
1963, 3-4
TOPIC TAGS: corpuscular stream, solar active region, sun, astronomy, M-disturbanco.
calcium flocculus, flocculus, geomagnetic disturbance, atmospheric pressure, frozen-in
magnetic field, upper atmosphere, stratosphere
ABSTRACT: Mustell has demonstrated that geomagnetic M-disturbances are caused by
solar corpuscular streams asbociated with calcium flocculae. A geomagnetic, M-dis-
turbance sets in 4 t = 6d after a. flocculus crosses the central meridian. Disturbances
in the lower layers of the atmosphere set in after the same time. M-disturbances cause
an increase of atmospheric pressure with a maximum atL t = A It is postulated that
the frozen-in magnetic field of the stream is broken up in the upper atmosphere ~nd the
latter experiences considerable heating and expansion, leading to the name effects in the
lower layers. A study has been made to test this mechanism. Radiosonde data for Volgo-
grad and Moscow were used; data on flocculae were furnished by Mustell. The super-
Card

ACCI~SSION NR: AT4016594
posed epochs method was used to determine the relationship between disturbances at
different atmospheric heights and solar corpuscular streams from active regions. The
"zero phase" corresponds to passage of a floccalus across the central meridian. Statis-
tical curves for Moscow and Volgograd for the heights 0, 5, 10 and 15 km are shown In
Enclosures. There is a lag of 0. 5-1d in the surface layer in comparison with the event
in the stratosphere. The character of the maximum and Its distance from the "zero
phase" indicates that the mean velocity of corpuscular streams is 370-400 km, in good
agreement with other determinations. The stable maximum of disturbances atAt = 6d
for all heights in the troposphere and stratosphere indicated correctness of the postulated
mechanism. Orig. art. has: 2 figures.
ASSOCIATION: Volgogradskiy pedinstitut, Volgogradskoye otdolonlye VAGO (Volgograd
Teachers Institute, Volgograd Division VAGO)
SUBMITTED: 00 DATE ACQ: 24Feb64 ENCL: 02
SUB CODE: AS NO REF SOV: 004 OTHER: 001
Card 2 $
V

ACCEOSION NR: AT4016595 S/2556/63/000/034/0005/0007
AUTHOR: Fomenko, B. D.; Bonells, I.. V.
TITLE: The relationship between calcium flocculae and disturbances of the lower layers of
the earth's atmosphere in 1950
SOURCE: Vsesoyuznoye astronomo-goodezichoskoye obshchestvo. Byulleten%, no. 34,
1963, 5-7
TOPV,' TAGS: astronomy, sun, calcium flocculus, geomagnetic disturbance, corpuscular
stream, M-disturbance, solar activity, sunspot, atmospheric pressure, superposed epoch,
flocculus, solar active region
ABSTRACT: A study has been made of the relationship between solar calcium flocculae and.
disturbances in the earth's atmosphere for a period of solar activity when 65 < R .4 125,
where R is the smoothed sunspot number. Synoptic charts for solar rotations 1291-1299,
prepared at the Meudon Observatory, were used, together with atmospheric pressure data
for Thilisi, Volgograd and Arkhangellsk. The superposed epochs method was used for
determining the relationship between disturbances in the lower atmosphere and corpuscular
streams associated with calcium flocculae. Forty-six flocculae observed during March-
November 1950 were used. The number of flocculae crossing the central meridian with
Card 11AI_

'ACCESSION NR: AT4016595
d d d
longitude intervals & L of 1 2 3 . ..... days is shown in-Enclosure. In construct-
Sol
ing statistical curves for flocculae with identicalA L the following values were combined:
Sol
AIJ 3-4d I &L 5-6d, &L 8 j-10d ... 8tatistical
Sol Sol 01 curves obtained by the super-
posed epochs method are shown as Figures 1, 2 and 3 in Enclosure. On these curves there'
Is only one peak, falling at At A The peak shows that for th~. r"post part the disturbance
maximum in the lower atmosphere appears At = 6d after a calci* flocculus crosses the i
solar central meridian. Calcium flocculae determine the boundaries of active regions.
Therefore, corpuscular streams emanating from active regions are responsible for the re-
I current geomagnetic disturbances causing disturbances in the earth's atmosphere. "The
author wishes to thank S. D. Nikolayev for assistance in collection of the nleteorological
data". Orig. art. has. 3 figures.
ASSOCIATION: Volgogradsldy pedinstitut, Volgogradskoye otdeleniye VAGO (Volgograd
i Teachers Institute, Volgograd Division VAGO)
SUBMITTED: 00 DATE ACQ: 24Feb64 ENCL: 04
SUB CODE: AS NO REF SOV: 003 OTHER: 000
2/j
card
~;i-I Ki-X zl

ACCESSION NR: AP3004325 S/0033/63/040/004/0700/0702
AUTHOR: Fomenko,- B.-Dv; Bonelis, 1. V.; Kuby*shkin, V, V.
TITLE: The latitude and height dependence of atmospheric disturbances
due to type M solar corpuscular streams
SOURCE: Astronomicheskiy zhurnal, v. 40, no. 4, 1963, 700-702
TOPIC TAGS: atmospheric disturbance, atmospheric disturbance latitude
dependence, atmospheric disturbance height dependence, corpuscular
stream, solar corpuscular stream, type M solar corpuscular stream,
radio sounding
ABSTRACT: The latitude dependence of atmospheric disturbances has
been detected from a study of data. in addition to that used previously
(B. D. Foluenko, Astron. zh., v. 39, 833, 1962). It is found that the
amplitude of atmospheric disturbances increases with geomagnetic
latitude. Radio sounding data show that the disturbance occurs in the
atmosphere. Orig. art. has: 4 figures and 1 table.
Card 2
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ACCESSION NR: AP3004325
ASSOCIATION: Volgogradskiy pedagogicheakiy inaticut (Volgograd
Pedagogic Institute)
SUBHITTED: 07Feb63 DATE ACQ: 20Au963. ENCL: 00
SUB CODE: 00 NO REF SOVt 005 OTHER: 000
Card 2 2

FOMENKO, B.D.
Urrelation of the secular intensity variation of cosmic rays in
the stratosphere with solar activity. Geomag. i aer. 4 no.2:402
Mr-Ap 64. (MIRA 17:4)
1. Volgogradskiy gosudarstvennyy pedagogichaskiy institut.

1 ACC NRt AR603211a SOURCE CODE: uR/ol6q/66/ooo/oo6/AOl5/AOl5
AUTHOR: Fome~ko, B. D.,
TITLE: Influence of solar corpuscular streams on the lower layers of the terrestrial
atmosphere
SOURCE: Ref. zh. Geofizika, Abs. 6A91
REF SOURCE: Sb. Solnechn. aktivnost 1. No. 2. M. I Nauka, 1965, 53-84
TOPIC TAGS: atmospheric pressure, corpuscular stream, active solar region,
chromospheric flare, geomagnetic latitude, solar corpuscular stream Sot-4fZ
C,4 #20 In 0 :3 l2we'e e- 0 4 1. ig W f *,4,9 a e-scia -e - 00,?,0()S0V4J1,e 'eR,PMr,->4)
ABSTRACT: The correlation between 'Variations of atmospheric pressure in the lower
atmospheric layers and corpusular streams has been studied. Streams from active -..
regions generating recurr ent geomagnetic perturbations and also streams ejected from
chromospheric flares are discussed. Investigations are made by superposition of
epochs. Atmospheric pressure in the lower layers reaches maximum approximately
si.r days after the passage of the active regiori through the central meridian. The
perturbation amplitude of atmospheric pressure increases with geomagnetic latitude
and diminishes with the altitude above the earth Is surface; the effect of disturbed
atmospheric pressure vanishes totally at the height fo 20-25 km. The highest
pressure, caused by corpuscular streams, occurs three days after the.chromospheric
9 1

ACC NR. AR6032141
flare. The correlation between the variation of atmosheric pressure and solar
corpuscular stream is proved statistically.
SUB CODE; 04/ SUBM DATE: none
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ACC Ni". ARG032353 SOURCE CODE: UR/O 16 9/66 /000 /007/A020/AO20
AUTHOR: Fomenko, B. D.; Kubyshkin, V. V.
TITLE: Temperature fluctuations in atmospheric disturbances as a function of
recurrent solar corpuscular streams
SOURCE: Ref. zh. Geofiziha, Abs. 7A116
R*ZF SOURCE: Sb. Solnechn. aktivnost'. No. 2. M., Nauka, 1965, 85-87
TOPIC TAGS: atmospheric disturbance, solar corpuscular radiation, solar
corpuscular stream, solar corpuscular temperature fluctuation, flocculus
ABSTRACT: Data on center flocculi, i. e., floculli having a heliographic width of
not more than 6* and situated in the solar hemisphere disposed to affect the earth,
were selected for subsidence curves of the 18th and I Oth solar activity cycles, when
the Wolf number was between 15 and 75. At the same time an analysis was made of
flocculi having a heliographic width greater than 6* and situated in the solar hemi-
sphere not producing geophysical effects on the Earth. Data obtained in high alti-
tude temperature soundings made at Tbilisi, Volgograd, Moscow, Arkhangel'sk
and Murmansk were used as the geophysical index. The method of superimposed
1/2 UDC: 551.5:523.745
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ACC NR'
AR6032353
epochs was used. Data obtained in high-altitude temperature soundings were
analyzed simultaneously with disturbances in atmospheric pressure as a function
of active solar regions. It was found that the temperature maximum in the 0-20-km
layer occurs 7 days after the passage of the active region through the central solar
meridian. B. Rubashev. [Translation of abstract]
SUB CODE: 03, 04/
,2/2
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24

ACC NRt AR6020768 SOURCE CODE: UR/0269/66/000/006/0063/0064
AUT HOR: Fomenko, B. D.
TITLE: Effect of solar cor*puscular fluxes on the lower layers of the earth's atmo-
sphere
SOURCE: Ref. zh. Astronomiya, Abs.,*6.51.487
REF SOURCE: Sb. Solnechn. aktivnost". Ho. 2. M., Nauka, 1965, 53-84
;TOPIC TAGS: solar corpuscular radiation, solar flare, lower atmosphere
;TRANSLATION: The relationship between variations in atmospheric pressure in the lower
11layers of the earth Is atmosphere and the' corpuscular fluxes was examined. Fluxes fromn
I
:active areas causing recurrent geomagnetic disturbances, as well as fluxes related to
the chromospheric flares were considered. It is found that the atmospheric pressure
.reaches its maximum value approximately six days after the passage of the active area
:through the center of the visible solar disc. The amplitude of the disturbances grows
~With increasing geomagnetic latitude, and decreases with the altitude. At altitudes of
ithe order of 20 to 25 Xm, there is no disturbance of the atmospheric pressure. The max-
imum growth of the pressure caused by corpuscular fluxes from flar.,Js takes place three
;days after the flare. 35 references. -B. Rubashev.
I
SUB CODE: 03 UDC: 523,75:525.23
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ACC NRi AR6028769 SOURCE CODE., L)R/0269/66/000/006/0064/0064
'AUTHOR- Fomenko, B. D.; Kubyshkin, V. V.
TITLE: Temperature changes in atmospheric disturbances caused by recurrent corpuscula
!solar fluxes
,SOURCE: Ref. zh. Astronomiya, Abs. 6.51.488
~REF SOURCE: Sb. Solnechn. aktivnost'. No. 2. M., Nauka, 1965, 85-87
TOPIC TAGS: solar activity, solar corpuscular radiation, sunspot cycle
*NSLATION: To determine the effect of corpuscular fluxes upon temperature variations,
Idata on the flocculi for the descending branches of the 18th and 19th cycles of solar
iactivity were selected; the selection was made at a heliographic latitude of