SCIENTIFIC ABSTRACT SKRIPCHINSKIY, V.V. - SKRIPIN. G.V.

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• Collection: Scientific Abstracts
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• Publication Date: December 31, 1967
• Content Type: SCIENTIFIC ABSTRACT

20-118--4-57/61
Certain Rules Holding in the Tillering in Perennial Loose-Tillered Cereals
in Their First Year of Life and in the Subsequent Years, in Comparison to
Related Annual Cereals
their place of origins 1) those formed directly from the
seed embryo, 2) those formed from the buds of the type I
sprouts as long as those sprouts were in the vegetative
(shortened) state or - short sprouts
which had been formed in the respective period, and 3) from
buds of the lower knots of the elongated generative (pro-
bably also vegetative) stalks which upually begin to.grow
during the development of the seeds. The first two types
are morphologioallyequal. For the sprouts of the second type
the author keeps the term "tillering sprouts". The sprouts
of the third type are formed at the perennial cereals after
the harvest. So they are referred to as innovation sprouts,
Thus all type 1 and type.2 sprouts are described as tiller-
in.rr knots, whilst those of the third type are described as
innovation knots. According to the results given above and
to the technical terms the total variety of the cereals in-
vestigated here can be summed up in three characteristic
Card 3/5 groups: I. Annual cereals. Every sprout can live for so-

20-Ila-4-57/61
Certain Rules Holding in the Tillering in Perennial Loose-Tillered Cereals
in Their First Year of Life and in the Subsequent Years, in Comparison to
Related Annual Cereals
order. In the following,year this knot is again replaced by
the innovation knot of the second order, and so on. III. Per-
ennial cereals the short sprouts of which can live for 195 -
- 3 years. These ake: Cock's-foot grass, Bromus erectus,
partly also Festuca elatior. The tillering knot does not
quite die in the first year and works in the following year
besides the'innovation khoi of the first order and in the
year.subsequent to that besides the-innovation knot of the
second order. So in one three-year old'tillering, sprouts of
three morphogenetic types can' be found. There-ard 1 figure,
and .8 reference s, 4 of which are Soviet.,
PRESENTED: October 5, 1957, by A, L Kursanov, Member of the AS USSR
SUBMITTED: June 17, 1957
AVAILABLE: Library of Congress
Card 5/5

The Relation Between the Activity of Organs of 20-U8-5-,57/59
Vegetative, Propagation in Perennial and Arnual
Cereals and the Process of Seed Formation
shoots, in cereals. The author carried out his work with
hertaceows grasses (cereals). Perennial cultivated rye was
chosen as representative of the perennial cereals. The annual
cereals were represented by various sorts of rye, wheat, barley
and oats. Moreover, an amphiploid hybrir! (Nr 927) was included
between the "Alabasskayall winter wheat and the perennial Anatom
lian rye (Secale anatolicum). In each of the incubators which
contained 7 kg of soil-T-Fe-st and coritrol plants were sown. The
first were sterilized-Mainly the forming of new stems was recor=
ded although also the dying of already formed stems was observed.
The number of the living and the dead stems, which had formed
after the forming of the ears, was recorded all phases of deve=
lopment. For this purpose threads of different color were used.
The dynamics of the formation arid dying of the shoots are given
in table 1. The analysis of data shows that 1) the steriliza=
tion of the ears practically did not influence at all the for=
ming of new shoots in the perennial sort. 2) In the case of
annual control plants new shoots were either not formed at all,
or if any, to an extremely limited number. In the case of the
Gard 2/4 operated-.on plants a considerable, although smaller number of

The Relation Between the Activity of organs of 220-1-1&-5-57/59
Veget4tive Propagation in Perennial and knnijal
Cereals and the Process of Seed Formation
sorts., In the case of the latter the innovation shoots
(table 1) which had formed due to sterilization later de=
veloped into reproductive elm of low growth with small ears.
In some cases they also died without having formed new shoots
so that the plant died. The contrary was the case with the
perennial sorts. All these observations may open new ways for
the selecticn of precious annual sorts.
There are 1 table, and l6references, 6 of which are Soviet.
ASSOCIATIONt Stavropol'skiy sel'skokhozyaystyennyy institut
(Agricultural InstituteStavrdioll)
PRESPNTED' . September 9., 1957, by A. L.,KLIrsanov, Academician.
SUBMITTED; June 17, 1957.
Card 4/4

KLOPOVP A.A.; SUIPCHINSKIY. V.V.
Sta-t,-,opol Botanical Garden. Biul. Glav. bot. sada no.39:3-6 260.
(MIRA 14--5)
1. Stavropollskiy botanicheskiy sad, Stavropol' Kavkazskiy.
(Stavropol-Botanical gardens)

SKRIPCHINSKII V.V.
- - .I- ~ I --- _._
Biological fourxiations of the perennial characteristics of tillering
gramineous plants. Biul.glav.bot.sada no-43:34-47 161.
(MMA 15*2)
1. Stavropol'skiy botanicheakiy sad.
(Hybiridization, Vegetable) (Gramineae)

SKRIPCIIINSKIY, VI.V.
Determination of plasmatic permeability as a method for the
evaluation of frost resistance of potatoes. Bot. zhur. 48
no.8.-1168-1172 Ag 163. (MIRA 16:10)
1. Vsesoyuznyy institut rasteniyevodstva, Leningrad.
(Protoplasm)' , (Plants-Frost resistance)
(potatoes)

SKRIPCHINSKIY. VI.V.
Seed germination of some wild ornamental pl-nts under natural con-
ditions. Biul. Glav. bot, sada to.50:78-82 163. (PEFA 17:1)
1. Stavropol'skiy botanicheskiy sad Stavropol'skogo upravleniya lesnogo
khozyaystva i okhrany lesa.

SKRIPCHINSKIY, V,V., doktor biolog.nauk; NATAL'IN, N.B.,- kapd.sellskokhoz.nauk
Raising rice. Priroda 53 no.1%20-28 164. (MIRA 1732)
1. Stavropollskiy botanicheskiy sad (for Skripchinskiy). 2. Kubanskaya
risovaya opytnaya stantsiya (for Natallin).

Hitfll~xi I Y V- V,
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S Cap Pr -~blem's ~ f 1. .;",. j ~ 1 Z, . A ~ , ~L. _.~ ~', ;j ~ Fil , ,~ , c
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_,. j1 -, ) 11 'A I

Y, V I V~ I I ~ V-EEW!,
;ecphytee
i-~;st renstance of vegetative primorrila of some
cf the Stavropol Territory flora. B1,ul. Glav. bot.
no.c;5;109-114 164.
1. .`7.tavropollsk4ly botanichesk-ly sad.

V
:ua
.6 theory-
b!
02 Ja-F t65.
(MIRA 18:6)

6~1

SPH TTC.711 I i1i's K rf t,r 11
-- *.- 7 - - .- --
Thoor 4nrj..
y of phasic develoMent and Dlalvlt~ breeds , Genetika
no.3:144-160 S 165. (MIRA 18-1-9)
1. Stavropollskiy nauchno-issledovatellskiy institut sellskogo
khO--,VUyctva. SubmitLed July 8, 1965.

";.c),-,nd -encral
--a
clien-Icorre.
--oskovskogo me-

Continvo-as steel -~cstln-- at tho Nlovo-Tullsl ii l' tollur ic 1 1-1, t
Biul.te'- .-e'r-on.inform. no-l-:11-13
12:7)
(Novo-Tullskiy-Continuous Casting)

AUT11ORS: 0. 1., K11"Illni. M- V.- K--M. M-,

TITLE: Cc-tnt3 nn Recirculatic,i -3*,.--'1mc1t'n-'

PERIODICAW
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Stal lir 10, p, zl?,!
ABSTRACT In conparing performance
and 7. o,,e-h--th f 18-, by
m A j 1). ~j M. 0. !. 1). Lhe
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point out that workl,F 11tion. .- not
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nutho
a-L contequently, re-
furnac~s
dt,n
b
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tlc3l lor
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t a '. "a a a S" 'a rG Of tc~ t3 "ealed
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that rocir c" 1.11.. ra,,~Perattv. ur ace e nferlor
In c,pacity ind perfomanc . to at W, 'I ar d ope -hearth
furnace3. There are 2 tablea; and I Sow let rerere-e.

Card 1/1

PASTUKHOV, A.I.; I I It A.L.; ANDREUV, T.V.; MAZUN, A.I.;
Prinimali uchastiye: MARKIN, A.A.; Sj9jE9HUK_, V.S.; MAR TONOV,
Yu.A.; SE=IN, N. P..; GAVRILOVA,, Ye, A,.
GAVRIWVA., YO.A.
Steelmaking from Tanadium cast iron in convertero with a top '
oxygen blow. Stall 21 no*12:1070-1074 D 161. (MIRA 14:12)
(Steel-Metallurgy)
(03cygen-Industrial applications)

REZNICHENKO, V,A.i SIDORFNKO, G.D.; EPSHTEYN, Z.D.; MARKIN, A.A.;
SKRIPCHUK, V.S.
I - __ _ -_ ~ . , -_ - -
Pilot plant investigation of the blowing of titanium-niobium
cast iron. Titan i ego splavy no.8:72-85 162. (M1RA 16:1)
(Cast iron-Analysis) (Slag-Analysis)
-(Oxygen-Industrial applications)

MAZUROV, Ye.F.; GNUCHEV, S.M.; SHRIPGOE, V.S.; IMARKIN, A.A.; LYALIN, Ye.S.
Sponge iron used as a charge material. Metal-lurg 9 no.11:17-19
N 164, (MIRA 18:2)
1. TSentrallnyy nauchno-issledovatellskiy institut chernoy
metallurgii imeni I.P.Bardina.

NAGORNYY, L.Ya.; PEGHUK, V.I.;.-SKR.IPCHUK, V.Yu.; TOPOLEV, V.P.
Methods for reducing the dynamic error of tensometric scales.
Izm. tekh. no.12:15-17 D 163. (MIRA 16:12)

Influence of the --,ane of the experimental body on the shearing strength of
the tjued joints. p. 51- ( --IAR`~--' v'-`7KU" 1. 1, No. 1/2, Jct 1956,
:~ratisln-4, "'ztchos1ov,?Ma)
SO: Vonthly LiSt 3f -:,ast -'-ur-)pean Accessions 7C, Vol. 6, ho. 12, iDec 195?- Uncl.

CZECHOSLOVAKIA/Cheudcal Technology - Chemical Products and fl-L'q
Application. Synthetic Polymers. Plastics.
Abs Jour : Ref Zhur - Xhimiya, No 8, 1958, 27034
Author : Lexa Jaroslav, Skripen Jan
Inst
Title : Effect of Low-temperature Hardening on Bonding Strength
of Phenol-Resorcin'ol-Formldehyde Adhesives.
Orig Pub : Drevexsky vyskum,'1956, i, No 1-2) 147-156
Abstract : The performed teAs of wood (of conifers) bonded with
phenol-resorcinol-formaldehyde adhesive FR-80 (I) at 5,
10 and 150, have shown that final bonding strength does
not depend on temperature of hardening but is determined
by shearing strength of the wood (which, in the conducted
tests, was of approximately 67 kg/cm2)- Determinations
were made of the length of time during which th2 parts,to
be bonded should be maintained under pressure (to
achieve a strength of 70% of ultimate):
Card 1/2

l.: t cl 1 : c, t r,--, c n i i c t r - s -
(Vi ni s t-.,: vc s ~brt c tvi F r;~ h,-,, Vol - 4, P-0 -
S C -,"H -e:7t "-.urcnenn ~.ccet~sjcns List, cf Conc-ress
1. 5, D;:

SIMSON, A.E., knnd.tekhn.nnuk; NASTROV, R.A., knnd.tekhri.nRuk; SKRIPETS, N.F.,
inzhener; FAVOROV, Yu.L., aspirant.
Dynamic characteristics of two-cycle diesel engines with diverging
pistons. Vest.TSKII MPS 16 no.6:39-44 S '57. (MIRA 10:10)
1. Khar'kovskiy teplovozostroitellnyy zavod im. V.A.Malysheva,
Vsesoyuznyy nauchno-issledovatellskiy institut zheleznodorozhnogo
transporta i rnarlkovskiy institut inzhenerov zheleznodorozhnogo
transporta im. S.M.Kirova.
(Diesel locomotives)

BALASH j R.; SKRIPETS, R.---[Skrypets', R.]., starshiy inzh,; TIMHENKO, 0.
[Tymc-fiiiiikop 0j, tekhni
Glazing bricks made of raw materials with a high moisture contert.
Sill,bud. 11 no*6:20-21 Je 161. (MM 14:7)
19 Nachallatk budivelinoi dillnitai Bilokurakinslkoi mizhkolgospnoi
budivelinoi organizataii Luganslkoi oblasti (for Balash). 2. Viddil
geologorozviduvalinikh robit i tekhdopomogi "UkrsIl'gosptekbnJkJ*
(for Skripets, Timchenko).
(Brickmakin

SMIPEETS, V. [Skrypetss, Vd, iInzh,
------- --.- .,
Letis observe exactly the techniques for vibrating brick.
Sills bad. 11 no.8:22-23 Ag 161. (MIRA 14:9)
(Brick induBtry) (Vibrators)

SKRIPETS, V. [Skrypets'. V.], inzli.
Heat blocking of kilns and c1riers. Sill.bud. 13 no.5:14-15 14y'63.
(MA -17-3)

SOIPILI) V.I.
Some problems relative to the genesis of the Gay
deposit. Mat. po geol. i pol. iskop. IUzh. Urals.
16o.
(Ural Mountains--Chalcopyrite)
copper pyrite
no.2;76-80
(MIRA 14:3)

SKRIPILI,, V.I.,- NEDOZHOGIN, M.S.; SIBIRSIrJIYA, N.A.
Rasic geological characteristics of the Gay copper pyrite
deposit in the Southern Urals. Mat. po geol. i pol iskop.
IUzh. Urala no.2:81-93 160. ~MIRA 14:3)
(Ural Mountains-Geology)

SKRIPILI . V.I.; MDO'17,HOGIN., M.S.
Geological and structural position of the Gay copper pyrite deposit.
Razved. i*ol-h. nedr 26 no.4*~10 Ap 160. (141RA .15:7)
1. Gayskaya geologorazvedochnaya ekspeditsiya.
(Gay -'legion (Orenburg Province)--Chalco-o *',e'j
.yrit

S KIUPIL I Y, V. I a
8tructure of volcanic formations in the'Gay ore province and
distribution of pyrites in them. Geol. rud. mestorozh. no.l:
80-91 Ja-F 161. (MIRA 1434)
1. Kompleksrlaya teinaticheskaya ekspeditsiya Yuzhnourallsko'go
geologicheskogo upravleniya, UEa.
. (Magnitogorsk-Geology)

VODOREZOV, G.I.; DEPLIPIK, A.I.; LAZAREV, P.V.; SKRIPIL' V.I.
Ivan Vasillevich Lennylkh;.1901-19610 obituary, Mat. po geol.
i pol. iskop. Illzh. Urala no. 3:3-4 162.
- I
I
I
f
I

NOVIKCIV, M.F.; V.1.
Yelenovskoye capperz-Mol-~tdPtIUM dc-P2it- Xa-, PrI k,ecll, 1. Pcl~
iskop. Illzh, Urain no. 3-.171-17:', 164' ti~IHA i7--,)

. - . 7 1 '1 -, 1, - -, ,
: I -~:~ I . 41 . I ! "- Je ~ 1 :" ~ !, -
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- , I " -
no , , 4 -I - - 1 -, -') r! C. ~ . I

KUZ "Iff N, A. I . -, SKRI PI N, f1r. V.
Gorrf!lation of apmidiurnal variations in the intensity of the
hard component of cosmic rays with semidiurnal fluctuations of
barometric pressure. Trudy lAk.fil. AN SSSR. Ser. fiz. no.l:
23-26 l5s. (KLHA 9;10)
(Cosmic rays) (Atmospheric pressure)

KUZI~QN, lk.l. ; SYRIPIN, G-V-
".. ...
Monthl3r-iid('T,-S-'~"~imont~ily variations in the intpnsity of cosmic
rays. Trudy lAk.fil. AN SSSR. Ser. fiz. no.1:27-32 '55.
OILRA 9:10)
(Cosmic rays)

-)'K'R I V
USSR/Nuclear Physics - Cosmic rays fluctuation FD-2207
Card 1/1 Pub. 146-12/25
Author Kuzlmin, A. I., and Skripin, G. V.
Title Letter to the editor. Influence of lunar tidal fluctuations of the atmos-
pheve upon the intensity of the hard component of cosmic rays
Periodical Zhur. eksp. i teor. fiz. 28, 6o8-6og, May 1955
Abstract Theauthors state that a consideration of the influence of lunar tidal
fluctuations in the atmosphere upon the intensity of the hard"Component
of cosmic rays 6'1 is of interest both for the study of the nature of
the half-daily rariations in the cosmic rays and for the stuay of the
nature of the dail-v fluctuations of the temperature in the upper layers
of the atmosphere (Ye. S. Selezneva, Izv. AN SSSR, ser. geogr., 9, 82y
1945). In connection w1th the fact that the period of the main lunar
tidal fluctuation of the atmosphere equals one half of the lunar day
(N. Ye. Kochin, Sobraniye sochineniy [Collected works], 1,1949), they
expect the appearances of the effect of the fluctuations in the regular
half-daily variations in the intensity of cosmic rays, but that these
regular variations can be masked by statistical fluctuations of the cosmic
ray particles. They thank Professor Ye. L. Feynberg. Five References
Institution Yakutsk Affiliate, Academy of Sciences USSR
Submitted January 19, 1954

Category USSR/Nuclear Physics - Cosmic rays
Abs Jour Ref Zhur - Fizika, No 1, 10,57., tio 622
Author Kuz)min, AI., Skrypin, G.V., Tyanutova, G.V., Shafer, Yu.G.
Inst Yukutsk Branch Acad. of Sciendes USSR.
Title Unique Flare of Intensity of Cosmic Rays.
Orig Pub Dokl. AN SSSR, 1956, loB, No 1, 66-68
Abstract Report on the results of measurements of intensities of cosmic rays during
the time of the great flare of solar activity on 23 February 1956. The
measurements were made in Yukutsk (elevation 101 meters, 510 northern
latitude, 1290 eastern longitude) with the aid of ionization chambers
shielded with 12 cm of lead and aimed with a telescopic system made of
Geiger-Mueller counters. The maximum by which the intensity exceeded the
usual value occurred at S.40 -- 4 hours Greenwich mean time and amounts to
165 -- 20Yp, depending on the type of recording apparatus. Apparatus re-
cording extensive showers with a density of 25 and 50 particles per square
meter did not detect any increase in Intensity.
C-7
Card 1/1

SKRIPIN, GeV*
Mffect of radioactive ervinations on the observable diurnal variations
in the intensitv of ionization produced by cosmic rays. Uch. zap.
IAI--. tin. no.1:2~-321 1117. (MIRA 110)
(Cosmic rays)

89791
S/169/61/000/GO3/008/022
AC)(j5/AW:z
o 7
Translation from. Referativnyy zhurnalk, Geoflzlka, 1961, No, 3, P. 10, # -,G79
A UB 10 R: __ariPLnj__1L_
TITLE. On the Star-Diurnal Variation of lnten~slty of the Stablo Component of
Cosmic Rays
PERIODICAL. "Nauchn. soobshch. Yakutskiy fil. Sibirsk. otd, AN SSSR", 1958, No. 4
pp~ 72-74
TEXT. The star-diu-nnal variation Is studied from da-~a of contl=:aouz record-
Ing of the Intensity of the stable component of cosmic rays at Yakutsk in 1954.
it is shown that 'he observed star-diumal variation with a-n amplitade of 0.06 +
0.002% and with a time of mayimum at 22.9 � 0.5 o'--lock of local star time occ-'s
as a result of seascnal variations of the amolitude of the slwn-diurnal variation.
With respect to the dls-~or-.ion effect of zhe sLm-diur-nal %ariatfor., -the star-
diurnal-variation of intensity of the itable ~ompcr.`ent vanishes.
N. K.
Treunslator'_- not-e; This is the ftill translation of 7ne original, Russian abstract.
Card 1/1

PHASE I BOOK EXPLOITATION 881
Akademiya nauk SSSR. Yakutskly filial
Variatsii intensivnosti kosmicheskikh luchey (Variations of the
Intensity of Cosmic Rays) Moscow, Izd-vo AN SSSR, 1958. 168 p.
(Series: Its: Trudy, seriya fizicheakaya, vyp. 2) 1,500 copies
printed. -
Resp. Ed.: Shafer, Yu.G., Candidate of Physical and Mathematical
Sciences; Ed. of Publishing House: Fradkin, M.I.; Tech. Ed.:
Pavlovskiy, A.
PURPOSE% This collection of articles is for scientists and students
of cosmic rays and meteorology.
COVERAGE: This issue contains articles on experimental methods In the
continuous registration of cosmic rays, the investigation of
meteorological effects of the different components of cosmic rays,
and the connection between variations in cosmic ray intensity and
solar and magnetic activity. Part I describes apparatus used in
Card 1/6

Variations of the Intensity of Cosmic Rays 881
measuring cosmic ray intensity on and under the earth's surface and
in the upper layers of the atmosphere, and specifically discusses
the ASK automatic ionization chamber. Part II discusses the theory,
methods and results of the investigation of meteorological effects
of the various components of cosmic rays. Part III discusses the
characteristics of daily variations in cosmic ray activity. The
following scientists are mentioned in the introduction: S.N.Vernov,
Corresponding Member of the AS USSR, Professor Ye.L.Feynberg, and
N.L.Grigorov, Doctor of Physical and Mathematical Sciences. The
articles are accompanied by diagrams, tables, and bibliographic
references.
TABIZ OF CONTENTS:
Preface
3
Card 2/6

Variations of the Intensity of Cosmic Rays 881
PART I. APPARATUS FOR MEASURING VARIATIONS
OF INTENSITY OF COSMIC RAYS
Shafer, Yu.G. Continuous Registration of Variations in the Intensity
of Cosmic Rays by an Ionization Chamber With Automatic Control 7
Shafer, Yu.G. Further Improvements in Automatic Cosmic Ray Stations 23
Kuzlmin, A.I., S$~,ripin, G.B., Yarygin, A.V., Installation for
Studying the Ene-r-gy-r?mTa-c~eristics of Cosmic Ray Variations 34
Kuzlmin, A.I., Yarygin, A.V. Apparatus for Subsurface Measurement
of Variations in Cosmic Ray Intensity 36
Belomestnykh, V.A., Shafer, Yu.G. Methods of Registration and
Study of Cosmic Ray Intensity Variations in the Stratosphere 47
Card 3/6

Variations of the Intensity of Cosmic Rays 881
PART II. METEOROLOGICAL EFFECTS
Dorman, L.I. Concerning the Theory of Meteorological Effects of
the General Ionizing and the Soft Components of Cosmic Rays 59
Dorman, L.I. Concerning the Theory of Temperature Effect of
the Neutron Component in Cosmic Rays 68
Kaminer, N.S. Problem of Temperature Extrapolation
in the Lower Stratosphere Region 73
Sokolov, V.D. Methodology of Applying Temperature Corrections
in the Intensity Measurements of the Hard Component Cosmic Rays
Using the Atmospheric Temperature Profile up to Elevationsof 5-6 km 78
Tyanutova, G.V. Preliminary Results of Comparing Data or,
Measurement of Global Intensity Variation of the Hard Component of
Cosmic Rays with Instruments ASK-1 and S-2 81
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Variations of the Intensity of Cosmic Rays 881
Koval'skaya, A.I. Problem of Seasonal Variability of the Barometric
Coefficient of the Hard Component of Cosmic Rays 85
Kovallskaya, A.I., Krasillnikov, D.D., Nikollskiy, S.I. Preliminary
Results in Determining the Barometric and Temperature Effects of
Extensive Torrential Rains Near the Sea Devel 88
PART III. NATURE OF VARIATIONS IN COSMIC RAY INTENSITY
Glokova, E.S., Kaminer, N.S., Mishina, N.A. Cyclic and Seasonal
Variations of Diurnal Wave of Intensity of Cosmic Rays 95
Kuzlmin, A I Skripin, G- V Relation of the Diurnal Effect of
Cosmic Ray IA-eln:5~Hy-~=magnetic and Solar Activity 107
F~ks, L.A., Shvartsman,B'.F. Temperature Effect in Seaeonal-anid
Diurnal Variations of the Hard Component of Cosmic Rays From the
Data Collected on Shmidt's Promontory Station 118
Card 5/6

SKRIPIN, G.V.
--l-
Diurnal variation in the irtensily of the hard =-np~-nent of cosmic
rays. Nauch. soob. IAFAN SSSR no.l.-72-74 158. (MM 1721)

jp
09000 SOJ106f-~9-4-4061
Translation from% Referativnyy zhurnal, Geofizika, 1959, Nr 4, p 126 (USSR)
AUTHORS,- Sokolov, V,.D,, Skrigin, G V
htt__
TITLE. In the Yakut Laboratory of Cosmic Radiation
Nr 5, pp 40 - 42
PERIODICAL. Mezhdunar, geofiz. god. Inform. byul., 1958,
A&STRACT: The collaboration of the Yakutskiy filial AN SSSR (Yakut Branch
of the AS USSR) in the investigation of cosmic-_ray.;/ kn accordance
with the IGY program is described. The stations of the world-
wide network were supplied with standard equipment of two types
in accordance with recommendations of the Central Committee for
the- IGY2 a telescope counter of charged particles and a
neutron monitor. The observation of the cosmic radiation in
the stratosphere permits the investigation of the stratosphere
variations of cosmic rays, their variation with the altitude
of the atmosphere, the connection between the variations in the
stratosphere and the variations at great altitudes, and the
obtaining of information on the transformation mechanism of
Card l/ 2 primary particles in proportion to their penetration into the
LIK

80404
In the Yakut Laborator-j of Cosmic Radiation SOV/169-59-4-4o6i
atmosphere. The equipment for stratosphere investigations comprises a
telescope counter for measuring the intensity of the cosmic rays and a set
for measuring the temperature and the pressure in the flight altitude. The
equipment is carried to the stratosphere by sour-ding balloons, For in-
vestigating the intensity variations of cosmic rays beneath the earth's
surface, a counter equipment of crossed telescopes has been developed, con-
sisting of a device placed on the earth's surface and devices placed below
the earth's surface in depths of 7, 20, and 60 m of water equivalent. The
main purpose of this work is the investigation of the energy spectrum
variation of the primary particles on the basis of the observations at
various levels below the earth's surface, and the study of the alteration
of the intensity variations of the t-meson component in dependence on the
thickness variation of the absorber, The time frequency variations of extensive
atmospheric showers of cosmic r s were also investigated in the range of the
ultra-high energies (1013 - jolyev), which has been studied relatively little.
By means of a standard neutron monitor placed on the earth's surface, the
Intensity of the neutron component of the cosmis rays Iz recorded, which is
Most sensitive to variations in the low energy range of the primary spectrum.
Card 2/2 L,V. Terent'yeva VK

29664
S/16g/61/000/005/023/049
3, AO05/A13O
AUTHORS: Danilov, A.A., Druzhinin, S.N.~ Kapustin. I.N., Skripin, G.V.
TITLE: A counter telescope f3r measuring the hard oomponent of
cosmic rays below the grou:ad
PERIODICALt Referativnyy zhurnal, Ge._~fizika, no. 5, 1961i 11, abstract 5
G 93. (Tr. Yakutsk. fii. AN SSSR. Ser. fiz... 1960, no. 3,
40-45)
TEXT: The authors desoribe the deeign of a cosmic ray counter tele-
scope produced in Yakutsk. The telescope :~oneists of three single blocks
with a total area of about 0.9 M2. To :Lnerease the efficiency of the
equipment, a quenching circuit is introduced, counter end effects are ex-
cluded and automatic control of the stability of the high voltage supplying
the counters is effected. The teleszops of triple ~;oincidence, installed
at a depth of 60 m of water equivalent, allows the re~zording of the hard
component of cosmic rays with an accurarq- of i-4% per heur. The device
has been in operation since February, 1956. X
[Abstractor's notei Complete transla,,ionl
Card 1/1

3 W/o
e00 (101//, oy6)
AUTHORSs
TITLEt
29671
3/169/61/000/005/034/049
A005/A139
Kuzlmin, A.I., Skripin, G.V.
On the decrease effect of cosmic ray intensity during magnetic
storms
PERIODICAL: Referativnyy zhurnal, Geofizika, no- 5, 1961, 13, abstract
5 G 104- (Tr. Yakutskogo fil. AN SSSR. Ser. fiz., 1960,
no. 3, 121-139)
TEXTt The authors investigated the upper limit and shape of the
energy spectrum of primary particles of cosmic rays subjected to the action
of the mechanism responsible for magnetic storms. For the analysis they
used data obtained from continuous recording of intensity at Yakutsk by a
neutron monitor, an ionization chamber and counter telescopes placed at
depths of 0-7, 20 and 60 m of water equivalent. The data were corrected
for the barometric and temperature effects. The presence of effects of
intensity decrease at depths of up to 60 m w.e. shows that the mechanism
which modifies cosmic ray intensity during magnetic storms affects par-
ticles with energies up to 400 Bev. This being the case, the energy
Card 1/2

DOW-!AN I L.I.; KUZ1111IN, A.I.; _MMKIN, G.V.
Sounding electromagnetic conditions in the interplanetary space
and in the vicinizy of the earth by high-energy cosmic rays.
Goomag. i aur, 1 noj-'333-345 MY-Je '61. (MIRA 14:9)
1,, Nagnitnaya laboratoriya AN SSSR i Laboratoriya fizicheskikh
problem Yallcutskogo fili4la S'birskogo otdeleniya AN SSSR.
(Wsmic rays)

~-:tdzdly 1-,f the ...
SIC --5- 8/6 P/OCO/OC6/018/136
A06 I/A 10 1
particle--z. The values of the barcm.,etric. coeff-fo.4-i-n of different components
ar~ iridic-ated, as Twell. as the principal rez~u!+13 ot a-n inv,?s+].gatlon of 27-day and
~:c,iar day variations of intensity, Plienomena obs ~~r7~-d djring magnetl'.c storms
Trv-.~ int-err--lation factors u~tw~en variations of intensity
nrlmar~; rid secondary coswic ray componerits up t.,, :nergle,- :,f ~j'00 Ee-.r are
'11res-~ fact.-)rs are litilized Cor -'the ana-Iyz;.;s of some types of varia-
of intensity.
0. Kaiminer
note: Complete trzanslation]

5-1 7- 741.5~) S/169/62/000/004/075/103
D218/D302
AUTHORS: Kuzlmin, A.I.0 Danilovt A.A.j Krymskiyq G.F., and
Skripin, G.V.
TITLE: Energy characteristics of cosmic-ray variations
during magnetic disturbances
PERIODICAL: Referativnyy zhurnal. Geofizika, no. 4, 19620 14, ab-
stract 4G74 (V. sb. Kosmicheskiye luchit no. 4, M-t
AN SSSR, 1961t 16-24)
TE'~'T: The data obtained with a number of surface and underground
instruments at Yakutsk are used to analyze the energy characteris-
tics of cosmic-ray intensity variations during magnetic storms. It
is shown that the intensity recovery period after the Forbush-effect
minimu.-.q decreases with increasing depth of the recording device. 1br
some Forbush-type reductions there is a noticeable North-South ani-
sotropy in this effect. The method of coupling coefficients is used
to determine the energy spectrum of the Drimary radiation during
Forbush effects. Best agreement between experimental data and theo-
retical predictions is obtained with the following primary differen-
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S/16 62/000/004/075/103
Energy characteristics of D218YD302
tial spectrum
C, 0.7
offjE a F_ at E
1
D at F_1
Further analysis shows that the effective width of the corpuscular
stream should depend on the energy of the scattered particles. It
is surrr-*ested that the regular field of the stream carries with it
magnetic irregularities which give rise to scattering and diffusion
of moderate-energy particles. The parameters of the streams, and
the ma-netic irregularities carried by them, are estimated. [Ab-
stractor's note: Complete translationi.
Card 2/2

AUTHOR: Skripin, G.V.
TITLE: On som-- properties of
(based on directional
cosmic-rays)
) 7-'A 1-Y-i
S/169/62/000/004/088/103
D218/D302
the solar-diurnal variation
underground measurements on
PERIODICAL: Referativnyy zhurnal. Geofizika, no. 4, 1962, 16, ab-
stract 4G87 (B 8b. Kosmicheskiye luchi, no. 4, 1-4.1
AN SSSR, 1961, 229-236)
TEi"7,T: A study is reported of the solar diurnal variation in the
cosmic-ray intensity, based on experimental data obtained with di-
rectional t 'elescopes at depths of 7, 20 and 60 m at Yakutsk in 1958
- 1959. It is shown that the phase difference between the southern
and northern telescopes located on the earth's surface is also pre-
sent in measurements with underground telescopes. The source of the
diurnal varlation lies at an angle of 830 east of the sun-earth li-
ne in the plane of the exliptic. The energy spectrum of the diurnal
variat4 on is of the form
Card 1/2

S/16 62/000/004/088/103
On some properties of the ... D218YD302
5D(E) r 0.16 E-1 , (E -;-- 13 Bev) V~
D(z:) ~_ t - 0, (E 13 Bev).
Data on the anomalous characteristics of the solar-diurnal varia-
tion during the period of minimum solar activity (1954-1955) are gi-
ven. EAbstractor's note: Complete translation].
Card 2/2

"'. 2 2 63
S/845/6Z/000/004/0o6/oi5
E032/E314
Kuz'min, ~G. V
AUTHORS: A.I. and ~kri i
In
TITLE: Underground variations in the intensity of cosmic
rays during 1957-1959
SOURCE': Akademiya nauk .9.55R. Yakutskiy filial. Trudy. Seriya
fizicheskaya. no. 4.. 1962. Variatsii intens.ivnosti
kosmicheskikh luchey, 66 - 82
TP_XT: The intensity of the ~L-meson component was measured
with a system of counter-telescopes at different-depths below sea-
level (7, 20 and 60 m of water equivalent). Variations in the
intensity of the ~L-meson component at sea-level could b8 Investi-
gated with this apparatus for an energy range of 2 x 10 to
2 x 1010 eV, which corresponded roughly to average primary-pakicle
energies between 40 and 2oo-400 BeV. The vertical intensity in a
solid angle of ~-l and the intensity from the southern and northern
directions at 30 0 to the zenith were recorded at each level with
triple-coincidence telescopes. The accuracy was sufficient for the
detection of fine effects provided the recording was extended over
a period of some months or more. It was found that meteorological
Card 1/4

S/845/62/Ooo/oo4/oo6/oi3
Underground variations .... E032/E314
effects in the intensity of the hard component at sea-level and
the above three depths were in agreement with the 1~~meson scheme
for the generation of the hard component in the atmosphere,
suggested by L.I. Dorman (Variatsii kosmicheskilch luchey
(Variation in cosmic rays), Gostelchizdat, Moscow, 1957). The best
agreement between experiment and theory is found to occur for the
following values of the exponent y in the effective integral
IL-meson spectrum:
s ea 1 ev e1 -Y = 0.3
7 m w.e. - Y = 0.5
20 m w.e. - Y = 0.8
60 m w.e. - Y = 1.
The meteorological effects at different depths below sea-level are
in good agreement with Dorman's theory (mentioned above). This is
confirmed by the fact that observed seasonal variations in the
,i-meson intensity at different depths and the expected changes due
to temperature effectswere identical to within experimental and
computational error. itnalysis of solar-diurnal variations at a
fixed point again confirmed Dorman's theory of the modulation of
Card 2/4

s/845/62/ooo/Oo4/oO6/015
Underground variations E032/E3i4
the prilnZLry cosmic-ray intensity by the electric fields of solar
corpuscular streams. The lower energy limit for particles . ..
modulated by these streams is 12 BeV and the effective source of
these variations lies to the left of the Earth-Sun line at an
0
angle of 66 +- 11 . The ratio of the amplitudes of 27-day varia-
tions and the reduction in intensity during magnetic storms are
the same within a wide primary-~particle energy range
(2 x 109 - 4 x lo 11 eV)so that it is suggested that they are due
to a common mechanism. The energy spectrum of primary variations
is of the form:
6D(O b < C
D(E) aca e El
where C1 = 7 + 2 BeV, a = -0.7 + 0-3, a 0.22 and b = 0.11
for the magnetic-storm effects and a =-0.06, b = 0.03 in the
case of the 27-day variations. This spectrum is consistent with
that expected on the Dorman theory due to the scattering of
particles by the frozen-in magnetic field of a stream with an
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S/845/62/000/004/oo6/ol5
Underground 'variations E032/E3i4
4
intensity of 10- gauss at the Earth's orbit but appreciably
disturbed by the interaction between the stream and the inter-
planetary medium. The considerable change in the energy spectrum
of particles with E: -,, 30 BeV in the primary stream during
magnetic storms suggests the presence of irreguiarities in
the regular magnetic field of the stream and the importance of
the influence of electric fields. There are 5 figures and 5 tables.
Card 4/4

C)
4?2'L,
S/845/62/ooo/oWoo/o13
E032/E314
31
AUTHOR: Skripin, G.V.
TITLE: Main properties of solar-diurnal variations according
to directional cosmic-ray measurements
SOURCE: Akademiya nauk SSSR. Yakutskiy filial. Trudy. Seriya
fizicheskaya. no., If.. 1962. Variatsii intensivnosti
Rosmicheskilch luchey, 83 - 90
TEIXT; It is noted that there is a lack of information about the
nature of the diurnal variations in the intensity of cosmic rays
arriving from different directions with energies in excess of 20
Bev. It is also not clear to what extent the mechanism proposed
by Dorman (Variatsii kosmicheskikh luchey-(Variations in cosmic
rays), Gostekhizdat, Moscow, 1957) ~xplainsthe observed anLso-
tropy in the high-energy range.. _.. . The present-paper
reports-the results of directional measurement of-the diurnal vari-
dtion obtained at Yakutsk at the Earth'asurface and at 7, 20 and
60 m of *water equivalent in 1958-1959. The measurements showed
that the observed difference in the ounting rates of telescopes
pointing north and south of the zenith at the Earth'asurface was
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S/845/62/000/004/007/013
"lain properties .... E032/E314
also observed at the above three depths below it. This is inter-
preted as being due to the effiact of the Earth's magnetic field on
the trajectories of the incoming particles. Using these data, a
determination was made of the direction of the source of 0diurnal
variations in 1958-1959 which was found to lie at 83 � 4 to the
E,arth-Sun line in the plane of the ecliptic. A determination was
olso made of the strength distribution of the source of these
diurnal variations in the plane perpendicular to the plane of the
ecliptic. Finally, data are also reported for the intensity at
60 m water equivalent in Yakutsk during the 1954-1955 minimum. The
apparatus employed has been described in previous papers (the
author et al - Tr. YaFAN 353R, ser. fizich., no. 2, 34, 1958;
-do-, no. 3, 40, 1959). The energy spectrum of the diurnal varia-
tions was obtained with the aid of the data provided by a neutron
monitor. The spectrum was found to be
61)(c) o.16.E:-' e > 13 BeV
D(E) 0, c < 13 BeV
Card 2/3

S/845/62/000/004/007/013
Nain properties ... E032/E314
It is found that the effects due to the geomagnetic fields are
sufficient to explain the differences in the phases of the
diurnal variation of cosmic rays arising from different azimuths.
Analysis of the diurnal variations during 1958-1959 showed that
they exhibited no seasonal effects. This *means that the source
of the diurnal variation partic *ipates together -with the
Earth-Sun. line in the annual revolution about the Sun and
remains to the left of this line all th-e*time. All these effects
are found to be in agreement with the theoretical results of
ljor.;ian referred to above. According to Dorman's theory, solar-
corpuscular streams carrying frozen-in regular magnetic fields
are the sources of mean solar-diurnal variations and the present
results forin a new experimental confirmation of this theory in the
high-energy range. Finally, a considerable change was found-in
the diurnetl variation during the period of minimum solar activity
(1958-1959) and this is ascribed to a reduction in the frequency of
ejection of solar corpuscular streams and the return of a large
number of such streams to the Sun. There are 3 figures. and
3 tables.
Card 3/3

AUTHORS: Kuzlmin, p,.I.
TITLE: On some basic
variations in
S/845/62/000/004/oO8/013
E032/E3i4
and sl~~ ~pi-IG-1.1-
I _~: L
Properties of disturbed diurnal
tile intensity Of cosmic rays
S UIR?c I': Akademiya nauk SSSR. Yalcutslciy filial. Trudy. Scriya.
fizicheskaya. no. 4.. 1962. Variatsii intensivnosti
kosmicheskikh luchey, 91 - 102
T "I' ~X' T: J. Sek�do.and.S~Joshido (Rep. lonos Res. Japan, 4, 37,
1950)t aiad-the present authors (Tr.YaFAN SSSR, ser. fizich., no. 2,
107, 1958) have found that there is an increase in the amplitude
of tile solar-diurnal variation and a shifi of the maximum towards
earlier hours during and after magnetic storms. According to the
theory of Dorman (Variatsii kosmicheskilch luchey (Variation in
cosmic rays), Gostel-,hizdar, Moscour, 1957), this is due to the fact
that during such storms the Earth enters a corpuscular stream
carrying a large frozen-in magnetic field. The source of the solar-
diurnal variation is then displaced towards the Earth-Sun line and
the amplitude of tile variations increases with the energy of the
recorded particles. This theory has not so far been satisfactorily
er~fl?q- The aim of this work was to use the data obtained at
r
U

5/845/62/000/004/008/013
On some'basic properties .... E032/E314
Yakutsk to determine the main properties of disturbed solar-diurnal
variations and to compare Dorman's theory with experiment. 'The
analy--iis is based on 1957-1959 observations with the apparatus des-
cribed in an earlier paper (the present authors and A.V.Yarvg in,
Tr. YaFAN SSSR, ser. fizich., no. 2, 34, 1958). The apparatus
consists of counter arrays and telescopes at the Earth surface and
at 7, 20 and 60 m of water equivalent. All the data were corrected
for meteorological effects. Magnetic data were taken from the pub-
lications of IZMIPIi.N. The analysis covers only those cases whe:
the reduction in -the measured *~i-meson intensity at the Earth surf-
ace was not less than These data show that magnetic distur-
bances are associated with considerable changes in the solar-
diurnal variations of cosmic rays. The degree of disturbance in
the amplitude and in the position of the maximilffi diurnal variations
is greater at higher energies of the recorded particles. The
maxii,,)um change in the diurnal variations during magnetic storms
at all the four levels mentioned above i4as recorded by the telescope
pointing in the direction parallel to the plane of the ecliptic
and at 300 south of the zenith at a geographic latitude of 600.
t was found th-t; the experimental data on the disturbed diurnal
~
ard 2/q

-z-/645/62/000/004/008/013
on some basic properties .... E032/E314
variations during magnetic storms were consistent.with a spectrum
of tile form
6D(c) 0, C E:
0
OL
D(E:) ~,ac C C
a = -0.5 10 15 BeV A
isrh or e and c0 = Moreover, the experimental
data are also in agreement (to within experimental error) with the
variation spectrum accepted in Dorman's theory
r> -C,
2
6D(c) f 2 -1 C E
1 1 <
+ sin
D(C) C 2e 4 2
0, C El
where f = 0.30 and c 80 - 108 BeV. The source of these
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s/8115/62/000/004/00il/013
On some basic properties .... EOWE314
variations is found to lie at 35 + 5 0 to the left of the Earth-Sun
line. The soiirce of diurnal vari"~tions during magnetic distur-
bances is associated with a mechanism whose position in space
varies continuously. A large number of considerable disturbances
in the solar-dilirnal variation was noted during 1957-1959, during
before and after magnetic storms. The general conclusion is that
the main characteristics of disturbed diurnal variations are in
good agreement with Dorman's theory, which explains them as the
effect of the electric and magnetic fields of solar corpuscular
streams reaching the Earth. There are 3 figures and 6 tables.
Card 4/4

L2266
S/845/62/Ooj/oo4/oo9/013
E032/E314
AUTHORS: Kuz'min, A.I. and Skripin, G.V.
TITLE: On the coefficient of absorption of- cosmic rays wbich are
responsible for solar-diurnal variation
S OURC E' - nauk SSSR. Yakutskiy filial. Trudy. Seriya
fizicheskaya. no. h. 1962. Variatsii intensivnosti
kosmicheskikh luchey, 103 - 107
TF',XT Results of a comparison of diurnal variations in the
~i-meson component of cosmic rays at the Earth'ssurface with measure-
ments obtained with similar apparatus und *er different absorbers are
reported. The A(_~