SCIENTIFIC ABSTRACT BLOKH, R.L. - BLOKH, Y.L.

• Document Type: CREST
• Collection: Scientific Abstracts
• Document Number (FOIA) /ESDN (CREST): CIA-RDP86-00513R000205530005-1
• Release Decision: RIF
• Original Classification: S
• Document Page Count: 100
• Document Creation Date: November 2, 2016
• Document Release Date: August 22, 2000
• Sequence Number: 5
• Publication Date: December 31, 1967
• Content Type: SCIENCEAB

BIOXH.
ClinM signif icance of colloid blood reactions in liver
diseases.
Ter. arkh. 23~no.lt46-51 Ja*-Feb 51. (CIML 20:8)
1. Of the Department of Theraj~eutic Natrition of the Central
Institute
for the Advanced Training of Physicians and of the Clinic of
Therapeutic
%trition (Directo-r-Ronored Worker in Science Prof. H.1.
Pawner) of
the'Institute of Hatrition of the Academy of Hadical Sciences
USSR.

BLOO, R. L.
BLOKH~ R. L. - "The SignificanceAf Colloidal Reactions of the
Blood in
the Clinic Course of Botkin's IDiseasb."' Sub 15 Apr 52,
Central Inst
fot the Advanced.Traintng of Physicians. (Dissertation for the
Degree
of Candidate in Medical Sciences).
SO: Vechernaya Moskva January-December 1952

HAZAROVA, S.A.; SYPCHENKO, O.A.- IIREKKYBV, Yu.N.;
YAKSAHOU,
A.M.; RUBINSKIY, S.I.
Outdoor day naps during the cold season in the
treatment of night
sleep disorders. Vop.kur., fizioter. i lech.fiz.kulit.
22 no 3:
17-21 Hy-Je '57* (MIRA i1:1)
1. Iz P~ratigorakogo klinichaskogo otdoloniya (zav. -
prof. Ye.Ya.
Stavokara) Ballneologicheakogp.inatituta na Kavkazakikh
Minerall-
nVkh Yodakh (dir. - dotsent I.S*SavoBhchenko) i
klinicheekogo
sanatoriya Pyatigorskogo kurorta (glavrqy vrach
O.N.Smolenskaya)
(wSOHNIA) (SLEEP)

)5LOM, R.L.; 7HUTAN, V.A.
Bffectiveness of antipyretic diet in a general therapeutic
complex for chronic gastritis at Pyatigorek. Zhur.ob.biol.
20 no.2:29-34 Nr-Ap 159. (MIRA 12:5)
Is Is kliniki (nauchnyy rukovoditell prof. Te.76.5tavokaya)
Gosudarstyennogo ballneologicheakogo Institnta, Pyatigore~:*
(DIMSP in vare dies.
anti-fever diet in gastritie (Rue))
(USTRITIS, ther.
anti-fever diet (Rua))

BLOXH, R.L., kand.med.nauk; VASIWYEVA, N.K.; SAAKYAN, A.G.
Effect of Won waters of varying concentrations on some indices
of,neurohumoral regulation in chronic gastritis.
Uch.zap.Pyatjgos.
nauch.-issl.balln.inst. 3148-58 160. (MIRA 15:10)
(RADON-THERAPEUTIC USE) .(STOMACH--INFLAMMTION)
(NEUROCHEMISTRY)

BLOKH, R.L*, kand.med.nauk
Nature and significance of compensation and adaptation in the
treatment of chronic diseases of,the-digestive organs under
health resort.conditions. Uch.zap.Pyat.gos.nauch.-issl.balln.inst.*,.
3:219-230 160, (MIRA 15110)
(DIGESTIVE ORGANS-DISEASES) '. (HEALTH RESORTS, WATERING-FLACESJETC.)
(ADAPTATION BIOLOGY))

R~q TBUTAN, VA*i IAWOTA, i1w.
mphowlaulas test as an Index of the Inflammatory process In
abroula gastrItIso Ub.delo 6 no.31:23-26 V.".Te 160.
SallueologlobeekiyAnstitut (dir. doteent LS, Sayeshchanko),
(STONACR--DWAMTION) (DIPMOMMUM)

ELMH, R.L.
--------------
Role of radon radiations and the products of its decopposition
in bringing about the therapwitic action of radon baths in functio-
nal and infle=atory diseases of the stomach. Med.rad. no.9:48--
53 161. (MIRA 1511),
1. Iz GosudaretvannogL; ballneologicheskogo instuituta na Navkas-
skikh Min$val'nykh Vodakh (Pyatigorsk).
(STORACH-DISRASES) (UMN-THERAPEUTIC USE)

ALEKSANDROVAq V,P,; BEREZINAs N,K,; BERNSIITMI, A.I.;'
BFMSHTEYN# S.E.;
ZINKOVETSKAYAp T,S&; IDESISp Ye.S.; SMOLENKOVAp O.N.19
TOSHINSKIY, I.I.; TSARFIS, F.G.; SHABADP Ye.T.; SHEYNBERG9
O.A.
Profesoor B.IA. Stavokaia;.obituary. Vop. kur., fizioter. i
loch.
fis. kultt. 26 no. 2:191 W,;~Ap t61. (KIRA 3J+:,4)
(STAVSDUg svGENiiA iAKovLwn, 1892-196o)

BLOKH, R.L.,- NOGALLER, A.M.
General pr inciples for-the differentiated use of a therapeutic
diet
at a health resort In.diseases of the digestive organs. V .t. 21
M~m. PX
no.1:9-13 Ja-F t62.. 15:2
I..Iz Gosudare.tvennogo nauchno-tvaledovatellskogo
ballneologicheskogo
instituta na Kavkazakikh Mineralln kh Vodalch'Pyatigorsk.
.(DIET IN DLUASE) (rIGESTIVE 6RWS DISEASES)

FRUMIX, SAO ~BLOM,, ROL
Ceramic L-5 flux for the welding of low-carbon steel. Avtom.
evar. 16 no.1204-39 D-163.' (MMA 17:1)
is Leningradsk.iy institut vodpogo tran--porta.

A,U* use of chtwobtateals as aWITOnt train the P(Ant 01
VIOW 431 indubial bygleas. N. 11. RkI41MINIllul. It N
Uk"rfl. N~ Krvmcva, 3, L. diurAmfg. nod 1. V,
harbk I G' * 11 s3wit 12. No. 1. 21-4(1917).'
Z,,W (k=rn"ZQtM Nd ) AW 1 =5-0 --Nutucmv, Imts
;~~ and rabbita & ~W. tfille'dw to'be 20
.A. lot PhCl vapor and 30 mit.P. for fientene ratmor,
E
'PhCf AouM not lie used as a wivetit lit IndualrT it ih~
txmcn. of Its vapor In the atm. irs"Im VAA mg, /I.

S16601611000/0101001/001
D258/D301
AUTHOR: Blokh, S.
TITLE: Thermophysical properties of chamotte refractories
at high temperatures
SOURCE: Akademiya nauk Ukrajinsikoyi RSR. Instytut vykoris-
tannya gazu. Trudy. no. 10, 1961. Teplotekhnika proiz-
vodBtva stekla i keramiki, no. 3, 92 - 99
TEXT: The aim of this work was to supplement data regarding.phy-
sical. changes occurring in chamotte refractories at high tempera-
tures. The information was required for programming of firing ope-
ra-Gions in the glass industry. The tests were performed on brick
specimens, both fired and unfired, manufactured from the same gra-
de of clay containing 50.15 B102; 35.22 A1203 and 1 ~1 % (CaO i MgO)
The loss on iginition was 11o28 %. The burnt specimens were fired
at 14500C. The coefficients c'. thermal expansion and of heat con-
ductivity~ the tensile streng-uh and the modulus of normal elastici--
ty were determined. The coefficient of thermal expansion of a
Card 1/4'

S/66 0/ 61/000/010/001/001
Thermophysical properties of D_2158/D301
fired specimen increased smoothly 2.5 x 10-6deg- 1 at 100'G to 3,5
x 10-6 deg-1 at 900 00. The curve of,P vs. temperature for an unfi.-
red specimen fell from' 2.9 x 10- 6(1000C) to 1.6 x 10-6 -i fpoooc)
deg- k7
increased.to a maximum of 3.9 x 10 at 650-700'C and finally.fell
to 2.8 x 10 -6deg -1 at 9000C. The coefficient of thermal conducti-
vity a was measured by a method.similar to that employed by N.A~
Zakharikov and S.A. Blokh (Ref. 2: Teplotekhnika pro-LzvodeTva ste-
kla (Heat Technology of Glass'Production)p Izd. AN SSSR K~q 195-3)
in producing glass. In this method the temperatures of 3 points at
various depths in a specimen are constantly recorded, while the
specimen is heated at the rate of 300/min. The express-' Lon for The
-.oefficient of heat conductivity a (in m2/hr.) was derived from
the equation of heat conductivity, thus
1 C_ . 1PU + P) /%4)
2 _TT7 1 ~4- (Pp
3
and
Card 2/4
,

13/660/61/000/010/001/001
Thermophysical properties of ... D258/D301
tl,- t2 t1
T3 - t2
where C is the rateof heating (OC/hr.); t1, t2 and t 3 the tempera-
tures measured at 3 fixed points and 1 and p are the distances bet-
ween the points t t and t - t respectively (in meters). The
calculated thickn;s-s, ?.ee th; ciroh-sectional distancet between
the point corres onding to tj to that having the lowest temperatu-
re s (in meterZ is needed for the determination of the mean tem-
perature 7, defined by
S TP(21 + p) + 12 (3)
1 2 1 + (Pp
and t + 1 + P [S 1 (1 + P) 1+ (5)
1(1 2S 1 3
In the case of fired specimens the relationship between a and Fis
linear from~.11.8 x 1o-3 at 2000C to 2.0 x jo-3deg-1 at 90000. The
Card 3/4

S/66 61/000/010/001/001
Thermophysical properties of D258%301
corresponding curve for unfired specimens starts at 1.8 x
10_3dee~,
at 200uC. In the latter caset there is no change in a up to
4500C
from where it decreases to 1.4 x jo-3 at 7000C. The tensile
strepg1h
determined at a heating rate'of 30C/min.t rose slowly from 1
kg/ci2
at room temperature to 6.5 kg/OM2 at 700OC; it then rose sharply
to 15 kg/cm2 at 90000. Fired specimens showed a constant value
of
36 kg/cm2 throughout the whole temperature range. The modulus of
normal elasticity of unfired specimens was Wo4 kg/cm2 up to
80ooC
and rose to about 6.104 kg/cm2, at 9000C, while that of fired
spe-
cimens was 2.105 kg/CM2 throughout. There are 5 figures and 3
So-
viet-bloo references.

S/169/61/000/005/027/049
AO05/A13O
AUTHORS, Blokhp* Ya:*L.p Glokoval Ye,S.q Kaminerp X.S.
TITLEt On the barometric effect of cosmic rays
PERIODICALs Referativnyy zhurnal. Geofizikaj no- 59 1961, 12,
abstract
5 G 9~. (Tra Yakutakogo fil, AN SSSR. Ser. fiz., 1960p no- 39
74-77-
TEXTt The authors discuss a method of taking into account the
baro-
metric effect in-recording theu-meson.and neutron components of
cosmic
rays which was used in a practical worki It follows from the
analysisi
1) in recording the hard component of cosmic raysp-the barometric
effect
can be determined-with sufficient accuracy on the assumption of
a-linear
connection between variations in barometric pressure and the
intensity
of-oosmic rayal 2) in order to determine the barometric-effect in
record-
ing the neutron component , the' linear 'approximation -is~ no
longer suf f ioient,
and the exponential-dependence of Cosmic ray intensity on
atmospheric-
pressure has to be taken into account, The authors briefly
consider a
Gard 1/2

ViOJ61/000/005/027/049.
On the baromettic effect of cosmic iaya- k005/kI3O
method of introducing barometric correo~ions, which is based on a
logarithmic representation of cosmic ray'intensity data.
EAbstraotor's notet Complete translation.]
Card 2/2

ZATHARTEDY, N.A., kandidat tekbuicheskikh nauk; BIOIM, S.A., inzhener.
Increasing the productivity of glass pot &=aaling furnaces and
improving their quality.,frud Insteisp.gasa AN UM 1:44-56 153.
(Glass. manufacture) (Fwnaces~ (MLU 9:6)

ZAMW=V, N.A., kandidat takhnichookikh nauk; BLOIM, S.A., inshener.
Design analysis and performance data on glass pot annealing furnacos
using recirculated combustion proauots. TrvAjv Inst.lep.gaza AN UM
1257-68 153. Mu 9:6)
(Purnaces) (Olass manufacture)

ZAKWINOV, N.A., kandidat tskbMobsskikb naak-. BLOKH, S.A..
inzhener.
-
Therma'1 stresses, in sheet glass and glass tubes. Trudy'Inst,
isp. gaza AN MW 2:64-82 154. (WIM 9: 10)
(Glass manufacture) (Thermal analy-sis) (Strains and stresses)
M

BLOKH S. A. Cand Tech Sci (diaa) "Study of the themal processes
o0ouring
during the kilning of Vr-eT~raoory ~oham~oe materials for tIze It
glass."
Minsk, 1957. 18 pp (Min of Higher Education USSR. Belorussian
Polytechnic Inat),
100 copies (KL, 3-58, 97)

MAUMIT. A. L; BICKH' S.A.; ZAKHARI]MV, N.A.
k
Qarb4rizing the gas torch In glass furnaces, Trudy Inet.
Isp. gaza
AN URSA no.5:68-76 158. (miRAn:i2)
(Glass furnaces) (Gas torches)

MM. S.A.
Conditions for firing grog floater bars. Trudy Inst.
isp. gaza
AN URSR no.5:109-126 158. (MIRA 11:22)
(Glass furnaces) (Refractory materials)

BWKH, S.A.: MAYXVSKIY. Ye.]R.: SHEYKINA, K.A.
Investigating the operation.of kilns for firing grog floater bars.
Tiudy Inst. isp. gaza,AN UOR no.5:1.27-134 '58. (MIRA n: 12)
(Refractory materials) (Kilns)

AUTHORS:
Zakharikov, N. A-,_J~g~ ~., Sen', Z. P., SOV/72-58-9-9/20

Lesovoy, IT. Vop Yarmak, 0. F.
TITLE:
Non-Recurrent Baking of
Porcelaini~'~, (Skorostnoy odnokratnyy

obzhig farfora)

PERIODICAL:
Steklo i keramika, 1c546r 9, pp 20 - 24 (USSR)
ABSTRACT:
This is an
investigation of the influence of the rate of

heating,of the products
upon their quality, if they are

baked by,a non-recurrent process
without casing. The

tests were carried out with porcelaine cups,
sizes.'B -53

and "Kiyevskaya". The ingredients of the batch are given

intable 1 and the results for the chemical analysis

( in percent) are
given in table 2. The molecular formula

for the batch is also
presented. Por increasing the

mechanical strength of the semi-finished
porcelaine product

O,3%_of oarboxy-methyl cellulose were added to the

batch. 0,2% of fluid glass and 0,1% of soda were used

in the
preparation of the electrolyte. The porcelaine

cups were cast in
plaster molds at fashioned to give a
Card 1/4
wall strength of 1,5-2,5
mm. Moisture is driven off to

Non-Recurrent Baking of PorcelaiO
Card 2/4
SOV/72-58-9-9/2o
a content'of 1% under natural conditions. The ware is then
glaz'ed with a 0-45VZPX hand operated atomizer. The raw
materials for the glaze are listed in table 1, their
chemical analysis is detailed in table 2. The molecular
formula ofthe glaze is also given. The glazed cups were
dried to a humidity of 0,5% and then baked in the
laboratory furnace (Pig 1). The maximum temperature in the
furnace was 13200. The cups were placed on the bottom
of the furnace without a casing and were cooled according
to a schedule specified by the diagram in figure 2. The
heating and baking period at this temperature varied
between 2-5 hours. Data concerning the baking conditions
are presented in t able 3. The degree of rhiteness of
the body was determined by, means of a ,FKI photometer,
wher6as the water absorption and the hZat resistance
of the'test products was checked according to GOST 7591-55.
The best whiteness was obtained with combustion gases
with a CO content of 3-4% (Pig 3). The rate of heating
varied between 60 and 3000 per hour. At this rate the
quality of the products obtained is by no means inferior

Non-Recurrent Baking of Fortelain SOV/72-518-9-5/20
to that of the products from the Baranovka an".7'KiYev
Works. Their water absorption does not excee(~ 0,39% -
The specimens corresponded to the requirements imposed upon
them-inthe-checking of thermal and chemical resistivity.
The glaze. also exhibited a customary qualit,-T. Inves-
tigations of the mi-crostructure of the body were carried
out with a ;'Hp -3 microscope and X-ray, structural analyses
were made an the!.D'H~-70 instrument. In table 4 the
structures'of customary and of test products are portrayed.
As can be seen they do not differ at all. Figures 4 to 8
contain micrographs of polished porcelaine sections made aftea
different baking.periods. They do not indicate any
e'asential variations in structure. The duration of baking
is therefore not determined by the physical and chemical
transformations in the porcelaine but only by the heating
facilities of the furnaces. The cooling process has
hitherto not been the object of minute research. Preliminary
,experiments showed that a cooling of porcelaine cups from
13200 to 100*.is possible within 8 - 10 minutes without
impairing the quality of the product. The experiments
Card 3/4 showed that a non-recurrent burning without casing

Non-Recurrent Baking of.*.Pero.elain SOV/72--58-9-9/2*
of porcelaine produc ts in short autouatic continuous
car tunnel furnaces"As possible. There are 8 figures,and
4 tablesO
,,a A.N UkrainskDy SSR ( Institute of
ASSOCIATION: Institut-.ispoltzovan iya gaq
Gas Utilization AS Ukr SSR)
Nauchno-issledovatel'skaya laboratoriya Kiyevskoge
sovmarkhoza ( Scientific Research Institute of the Kiyev
Council of Natiohal Econox~y)
Card 4/4

- ' I BWXH, S. A.
-, w It
Efficient methods for kilning firebricks, Stek.i ker.
17 no.7:35-38 JI 160 (MM 13:7)
(Glass furnaceO (firebrick)

S/081162/000/020/016/049
B158/B101
AUTHOR: Blokh, S. A.
TITLE: Thermo-physical properties of fireclay refractories at high
temperatures
PERIODICAL: Referativnyy zhurnal. Khimiya$ no. 20, 1962, 348,
abstract
20K178 (Tr* In-t ispol'zova4iya gaze AN USSR9 no. 10f 1961#
92-99)
TEXT: Descriptions are given of methods for determining: the
coefficient
of thermal expansion of refractory products (RP) using the
dilatometer of
V. G. Permyakov; the coefficient of temperature conductivity by a
method
of calculation using data on temperatureg through the
croan-aectiQn.of
RP whilst being hedted; the limit of tensile strength and the
modulus of
normal elasticity of RP whilst being heated. It is established that:
the coefficient of thermal, expansion of RP decreases when the
dried brick
clay is heated to 20OPC as a result of shrinkage in the temperature
range
100-2000C1 it increases with a further rise in temperature to
700oC, but
vhen the temperature reaches >70000 it falls off again as a result
of
Card 1/2

5/081/62/000/020/016/040
Thermo-physical properties B158/.BIOI
a glass phase forming in the specimen; the thermal diffusivity of
RP in
the range 450_6oooC falls sharply as a result of the constitution
vater
being rapidly removed. [Abstracter's note: Complete translation.]
Card 2/12

ZAKHARIKOV, N.A., doktor tekhn.nauk; BLOKH. S.A.
'Rapid drying of porcelain. Stek. i ker. 18 no.11925-28 N 161.
(MIRA 1-5:3)
(Drying apparatus) (Porcelain)

ZAKHARIKOV, II.A.; NAYDENOV V.V.i BLOKH, S.A.; SOLDATOV, G.A.;
LEVITSKIY,
V.K.; KUZNETSOV, V.V.; SPEKTORp M.F.-
Radiation gas drying of structural ceramic products. Stek. i
ker. 19 -no.7:21-25 J1 162. (MIRA 15:7)
(Tiles-Drying)

MOM, S. A. (Institute of use of gas of Academy of Sciences of Ukrainian SSR)
ItResultIs of investigations in the processes of radiation drying"
Report presented at the Section on Heat and Mass Transfer, Scientific Session,
Council of Acad. Sci. Ukr SSR on High Memperature Physics, Kiev, 2-4 Apr 1963-
Reported in Thplofizika Vysokikh temperatur, No. 2, Sep-Oct 1963, p. 321, JPRS
24,651.
19 May 1964.

BL OKH-, S J6 kand.~-. t6kha. nauk
Quiok-dr7ing method for pottez7 wares. Stek. i ker,
20 no.7:
26-28 J3. A63. -(MM 17:2)
L-InBtitiit iBpollsovaniya gaza AN UkrSSR*
11.1 -4W

BLOM S.A. hand. tekhn. nauk; VOLOVIK) inzh.; SOLDATOV,
G.A.P inzh,;
-MEVITSHY, V.K.., inzh.
li-1,gli temperature gas spray drying of ceramic
suspensions* Stek.
I ker. 22 no.8:21-23 Ag 165. (MIRA 18.9)
1. Institut gaz-a AN McrSSP (for Bloldi., Voiov-1k). 2.
Khartkovskly
plitochn7y zavod (for Soldatovp Levitskiy).

kand.tekhn.nauk; GUZ, D.B., inzh.; RUBASHEVSKIY, I.Ya.,
BAUMAN, A.Zh., inzh.; SENI, Z.F., kand.tekhn.nauk;
IgUITON, Ya.G. , inzh.
Conveyor kiln with a wallcing hearth for rapid saggerless
firing of poreelain. Stek. I ker. 23 no.lt29-32 Ja 166.
(MIRA 19:1)
1. Institut gaza. AN UkrGSR (for Blokh). 2. Konstruktorskoye
byi= Ukralnskogo soveta, narodnogo khozyaystva (for Rubashavskiy,
Bayman). 3. Ukrainskiy institut stskollnoy i farforo-fayansovoy
promyshlonnosti (for Sen', Khariton).

BLOKH, S. I., Gand of A,,-,ri Sci (dies)
"Efi'ectf~-e-n-e--s--s--of---Ye-a-t
on Various Types of Rations,," Kharlkov, 1959, 17 pp (Njarikov
Veterinary institute)
(KL, 8-60, 117)

BLOKH, S.I., kand. sellkhoa.' nauk; BORZOV, ViV.0-kand. sellkhoz.
naux; TMHENKO, GJ.-[IUrchenko, H.T.], inzh.-mekhanik;
VOLOSOZHAR, V.'A.9-kand. ekon. naukj GERTSENv Ye.l.[Iiertsen,
IE.I.1, kand. sellkhoz,' -nauk; DANWKOI.A*-jDuq4m*koI.Aj red.;
SMIRNOV, O.V.[Smymov, 03.1, red.; MYCHENKO, I.Tu.,
[Niamehenko, LIU.], tekhn. red.
[Advanced work practices on cattle farms] Peredovi metody
raboty na fermakh velykoi rohatol khudoby. 2., vypraviene i
dop. vyd. Za red. I.A.Danylenka. Kyiv, Derzhailthospvydav
URSRI 1963. 203 P. (HIRA 16slO)
1. Chlen-korrespondent Vaesoyuznoy akademii sel'skokhozyay-
stvennykh nauk imeni V .I.Lenina (for Danilenko).
(Wrying)

BLOKTIO S. me
2o3.62 BLom, s. me
P4!ofilaktika likhoradochnykh poslerodovykh zabolevanii. Vracheb. delo.,
1949'. Noe 6.
stb. 531-34.
SO: LETOPIS ZHURM STATE.Y. Vol. 27, Mosk7a, 1949.

BERNSHT&N, M.A.j BLOKH, S.S ; HUAV, V.I.
Certain results of deep-well-investigations of gas we:Lis with
MGG-2u and DGM-4/2 man=etera. Gaz. prom. 9 no,40-10 161,.
(MIRA 17:8)

KUTU OV, A.I., red.; ZAYTSET, A.P., red.; DROGALIN, G.V., red.; POLESIN,
Ya.L., red.; KOSTYUKOV, U.N., redo; XUBAZ, DaHat red.; LU2MIKOT,
A.H.p red.; RODIONOV, I.S., .red*;-_NLOKHL S,$,_,_red,; SULTANOT9
D,X,, red,; BIBILUROV, V.P.0 red,; MROV, A.I., red.;
XWCHEVNIKOV, NX, red.; ANDRIANOV, K.I., red.; GADZHINSKATA, M.,.
red.izd-va; BMSLAVSKAYA, L.Sh., tekhn.red.
[Safety regulations for petroleum and gas producing industries]
rravila bazopasnosti v n8ft6gE12odobyvaiuahchei promyshlennostia
Moskva. Gou.nauchno-takhn.izd-vo lit-ry po gornoma delu, 1960.
123 p. (MM.14:3)
1. Russia (1917- R.S.F.S.R..) GosudaretvenW komitet po nad2orri
2a bezopasnym, veder-tiem robot v promyshlennosti i gornomu nadsora.;
2. TSentralln" apparat Goegortakhnadzore RSFSR (for Kutukovp
Zoytoev,.Drogalin. Poleain. Kostyukov, X-aras, Luzhnikov, Rodionov,
Blokh). 3..Vseso~uznyy nauchno-isoledovateltskiy institut po
tekhniks-bezopasnosti (for Sultanov). 4. UprovIeniya ukrugov
Goegortekhuadsora RSFSR (for Bibilurov, Petrov, Kharchevnikov).
5. TSontrallnyy komitet profsoyuza rabochikh neftyanoy i khimi-
chaskoy promyshlennosti (for Andrianov).
(Oil fields--Safety measures)
(Gas izxdustry--Safety measures)

.I-IL"Ai:t stsel inzho
U:,,in!- li,Tulfiod :fasos. Dozoi).ill-ad-a v pron. 5 no.1:17-19 Ja 'a.-
1- -
Mquef iod r,otrull oulm

B
.PIPE BUCHIN, A.N.; KRYUCHKOV B.N.; REYTENBAKH G.R.;
SINYAVSKAYA'- N.P*:
Certain features of the technological process in the
development of the Western-Tebuk oil field in t~p Kqmi
A.S.S.R. Nauch-tekh'm.~.a~DT* po dob, nefti. n6.21t
54-58 163-0 (MIRA 17%5)
1. Voesoyuznyy neftegazovyy nauchno-isaledovatellskiy
Instiftt i Fechorokly nauchno-iosledovatellskiy
ugolInyy
institut.

BLOKII, S.S.; VOINOV, V.V.; THUSHINA, K.G.
Certain geological features of the Middle-Devonia
producting
layers in the Western Tebuk oil field.
Nauch.-tekh.sbor.
po dob. nefti no. 21:13-19 163. (141RA 17-5)
1. Pechorskiy naur-lino-issledovatellskiy ugolInyy
institut i
Vses--.izr,yy neftegazovyf naitchno-issledovatellskly
institut.

REYTENBAKH, G.R.
ResultB of the experimental exploitation of the Western-
Tebukakoye oil field. Nafteprom. delo no. 9:3-6 163.
(MIRA 17W
1. Neftegazovyy otdal Nehorskogo nauohno-issladovateltakogo
ugollnogo instituta.

BLOKH ~ S. S.
~- rmining the parameters of producing strata forming an
edge-
water region in the Western TebWk oil field. 110ftepwom.
delo. no.
90-7 164. - (MIRA 17:10)
1. Ukhtinskiy neftegazovyy otdal Vsasoyuznogo
nauchno-issledovatell-
skogo instituta prirodnogo gaza.

BLOKH S S.1 VASSEMNP V.0.
Using electronic computers for processing well
data ty the
built-up pressure method. Nefteprom.delo
no.10.-40-41 165.
(MIRA lgtl)
LUWtinskly nefte-gazovyy otdal Vsesoyuznogo
nauchno-
iseledovatellskogo instituta, prirodnogo gaza i
UkhtinskAy
nefte-gazovyy kombinat.

B-IDKR- Samull T %XJAXjObp4GRKIU, Samall L'vovIcb;
DANILVIGH, Te.P.;
ONMYOk, To.. red.; IMBEDIff, A., tokhn.red.
CH&ndbook of prices for building materials and equipmout
approved
during the period from Julr 1, 1955 to January 1, 1958]
Spravocbnik
teen na strottelinye materialy i oborudovanie,
utverzhdannykh v
period a 1 iiulia 1955 g. po 1 lanvaria, 1958 g. Moskva.
Goafin-
izdat. PtA. 1958. 1182 p. (HIRL 12:1)
(Building matorials--Prices)

DANILSVICH, Te.F.; GOLOYNINA, Te. red.;
IMIURVI A,', teiQ.red,
[Price manual for materials and equipment approved for the
period January 1,*1958 to January 1. 19591 Spravochnik
tsen
na materialy i oboradovanie, utvarshdenxxykh v period a 1
isn-
varia. 1958 g. po I ianvaria 1959 g. Moskva. Goefinizdat.
Pt-5- 1959. 672P. (MIRA 12:9)
(Industrial equipment--Prices)

t .1mW&
Al
15
MAE-
Ng
ILI
taw u.11
lu* 7i
tog
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lot
llj
a M
-o r. Zee
4 ni
4:413
jrz
j "eta
l...
N r 2e , *19
11 A
e v - HE 1
Rl t to
u t- RA
o.9 -*q
o a NoNs ':*I
. i -. :
ire ~ - ll,;
o
3 - .7 R
5 9 ESE
Va IFR
ov
P4
npq
I p -
-o3

L o r\
V
J7
PMSR I BOOK MMOITATio sov/546o
LepinLlradokiy metallio"Iesk-ly zavod. Otdal takhnichookoy
Infor-=atall.
NexotoryY0 voprony to'chnoloall pro.Uvodntva turbin (Certain Problems
In tho Manufactura of Turbines) Roncola, 1',anhr,,iz, 1960. 398 P.
Errata slip inserted. 2,100 copies
Its: Trudy, vYP. 7)
7.iinted.
Spoasoring, Aceneyt RUM. Sovot narad-noro lzhozyay;3tva L--ninrrad-
,ho!:o ekonomichesIzo,!3o admini3trativilogo rixyoia, Upravlonlya
wj*-r~-icloZp mnohinootroyonlya, and Leningradskly dvazhdy ordcna
Lonina metallichouldy zavod. Otdol telchniolieskoy informatail.
.f Ed, (T tle page): 0. A. Drobilkoj Editorial Board: RezP. Ed. : 0.
A.
D.-N131w, B1, A. Glebov, A. V.. tlayzoll, and 11. Kh. Mcrnikj Tech.
Ed.: A. I. Kontorovioh; ManaGing Ed. for laterature on M-chine-
BullcUnS Technology% Ye. P. Naumov, Engineer, "Leningrad Depart-
PMUICZE: - Zftis collection of articles In Intended for technical
p--nn'Onnel in turbino plantap Inetitutesp planning organizations,
-r, wall as fo?? production innovators.

Certain Problems (Cont.) SOV/5460
COVERAGE: The experience of the LMZ (Leningradakiy metallicheakly
zavod Leningrad Metalworking Plant) In the manufacture of modern
large-capacity turbines is presented. Methods for the rationali-
zation of basic manufacturing processes and for thelmeebahizatiori
and
automation of manual operations are given. Descriptions of attaoh-
ments and tools designed by UIZ for Improving labor productivity'
and product quality are provided, - and advanced inspection methods
discussed. References accompany some articles. 'No personalities
are mention2d. There are 26 referenaeat 25 Soviet and 1 English.
TABU OF 6ONTEms
Foreword
M FROGESSING IMMODS IN MACHINING
PM AS&TOMY
M. [Engineer). -The Organization,, Mathods,and Trends In.
Efforts for Improving the:Easy Manufaoturability of Designs for
Large Hydraulic Turbines... 5
Card_2Ae-

Certain Problems (Cont.) SOV/5460
Surface of Turbine Blades on a Lathe 224
Tsimmerman, A. I. [Engineer]. Fixtures With Universal Pneu-
matic Actuation 230
Martlyanov, G. I. [Engineer]. Surfacing the Leading Edges of
Turbine Blades With Stellite- [Type] Hard Alloy 234
Blokh, V. A. [Engineer]. Moment Recording Scales for Weighing
bine Blades 237
IV. PROGRESSIVE METHODS FOR WELDINGs CASTING, PARTS
HEATINGsAND ELECTROCHEMICAL TREATING
Averin,, V, D, [Engineer], and B. A. Rabotnov [Engineer]. The
Application of Automatic Welding in the Manufacture of Hydraulic
and Steam Turbines 24o
Sukach, S. A. [Engineer]. The Welding of Steam-Turbine Cylin-
ders Made of Types 20KhNFL and 15KhlMlFL Perlitic Steels 248
Card 7A2

2376-110000 1 Z/O W/o 42
A004/A101
AUTHOR: Blbkh;'V. A
'kMki Moment s'eales for the-'weigl%ing. of turbihe -blades
Pmowdkt ReferativW zhurnal, ftshinoitroyeniye,,no. 12, 1961, 3,
abstract
12Zh13 (V ob. "Nekotoryyi V60r. 'tekhnoV. prolz-va, turbin".'[Tr.
Leningr. metallich. z-da,lno. 7]. Mosoow-Lehingrad, 19.60,
237-239)
Twt. The author-desaribei'moment scales making it Possible
to,match tur-
blni,bladei 'according to: thelr~ we(ght iind moment(of Inertia),
which elim~inates
any unbalance of thi turbine~'dll3k after the blades have-been
fitted. "The moment
scales consist of.the,stand 'carrying a packing of khives by
yhich the('knife;-edge
bearings of the balano6 arm. are. bom*.!. The 4nd:' of, the-
right*.balance arm carries
a'clampipg,device with'interchangeable pih stopa,.which is
intended for,the
setting and olainping ot-the-tall part'of the'.blad:6 being
weighed. The length
of this-arm from the knife-edge'bearing'tothe pin stops-is equal
to the,radius
of the turbine -disX. sungnit on'whioh~ the- blade being'weighed
is fastened. On the
leiftlbalanbe' arm .oo~nter,*,weighte are mounted, The soales are
fixed with the aid
an k6reelt"located'unde thebl -arm,
f r. alanae Under the lower oreW of th ~olbAping
0
"Card'T/2

8/-123-/61/WD/012/C)30/042
moyiiht scal6e for the weighing of -turbine blades A004/A.161
,aevice,,tfie, Plate, of", a''oomercial- di'al, scales is placed
on which'r6sts'the- -,r~ht
b&Ihnce 'arm d'ths' momaht"'soal6s'.,~ith'the fastened- blade
being vieighed. -:-Th
'MitfiWgli6i aii- aocount'of thei- a-aalia-- operation. There are
2 figures.
R. Skulk6v&
[Abstracter's note: "Complete translailon]
Cardm~2/2

BLOIUI, V.A,, inzh.j BYEKIN,V.S.,, inzh.
Automatio rotation of the rotor of a turbine unit. Llnergomashino-
stroanie 10 noollt36-36 N 164 (MIRA 18:2)

BL=.,.-.%Vjaamjr.GeorgVevloh; HIMMMICHO Owl., otvatstvenn)7 rs&,; MKIN,
[Reorganization of the mm%agemint of a6 factory] Cjqt perestroild
wravienila, savoiLon. lenitkrad,, Goe. soiusnoe izd-vo sudestroito
prowshl... 1958. 65 P.' (MIRA 320
(Industrial managemant)

BLOKH Vladimir_qV_QrgXyeyioh; HISHMICH, G.I.. otv.red.; LEVOCHKINA,
JJ,10, tokhn.re 0
.(A plant without workshops; practice in reorganizing production
management] Zavod bez tsekhov; opyt perestroiki upravlaniia
proizvodstvom. Izd*2.t dopeA perer. Leningrad, Goo.soiusnoo
izd-vo sudostroit.promyshl., 1959. 89 po (MIRA 12:12)
(Industrial organization)

141LI)DDV. X.: BBOXH, V.; AMICHINKO, M.
Toward a radioalroorganization of mnagement.
Sots.trud
4 no,7;106-115 J1 159o (KRA 13 -.4)
It Nachallnik otdala truds t xarabotnoy, platy
Karel'skogo
sovnarkhova (for Millkov). 2* Direktor Mookovskogo
zavoda
evototekhnicbeakikb isdeliv (for Blokb), 3.
Nacbal'nik otdola.
truds i zarabotnoy platy Upravlaniya
motallurgicbesko7 pronV-
ablennosti.
(Industrial organization)

PrOKII) V. K.
K voproau ob usilenii provoznol sporobnosti Kazalinsko[-.2
nar-ravleniia.
Zheleznodorozhnala liniia Kinel-Kazelinsk-Tashkent. On ihe question
of raising
.2 trarspprt capacity of Kazalinsk direction. Railway line
Kinel-Kazoinsk-
th
Tashken.d/ (Trars~ortonow troitelletvo. 1935, no. 11 p. 28-31,
sketch).
11. C: HE7.T7
SO:
Soviet Transportation 6 nd Co'=unica tions. A Bibliography, Library
of Congress
Reference Department, Washington, 1952, Unclassified.

SAXIN. A.A.; BLOKH. Ya.L.-. DUBROVIN* M6K,
Prol;ng*ju,g.ttje.j,jfA of.jaelf-quenohing counters using ra4io engi7
neering methods. Prib. i t-Ich. skep n0.1158-59 J-a-7 15?.
(Geiger-ftller counters) Ruclear counters) (MU lot6)

AUTHOR: Blokh, Ya. L. and Dorman, L. 120-2-1V37
TITIS: Meteorological Coefficients for 47tand 21r"ounter
Telescopes. (Mete orologiehe skiye KoeffitBiyentydlya
Kubicheskogo i Polukubicheskogo Teleskopov.)
PERIODICAL: 11~ribory i Telchnilra -Eksperimenta, 1957, No.2,
pp. 46 - 48, (USSR).
A13STRACT: Complex telescopes for continuous registration of the
cosmic rays-intensity will be extensively used during the
coming I.G.Y. The author determines the theoretical values
of the barometric pressure coefficient and of the tempera-
ture coefficient which can be used with cubical telescopes
at the sea level and to the semi-cubical telescopes under
the surface of the earth, at depths of 25 and 55m of the
water equivalent. The use of these coefficients will free
experimental data from the distorting influence of the
varying meteorological conditions. According to the theorj
(Ref. 1) the relative change
h
6NtL/X 11 abarbho + Wt(h).6T(h)dh,
of ~L-mesons intensity due to a relative barometric.change
Card 113 6ho at the observation level and the relative temperature

120-2-13/37
Meteorological coefficients for 4Trand 2frCounter Telescopes.
change 6T (h) is given by eq.(l). This expression has
two coefficients a bar atmospheric pressure coefficient
in %/millibar and W T(h) density of the temperature
coefficient in %/10C atift. Both coefficients can be
determined from the two equations (2), where
WT(h,e) and m bar(e) are the meteoroloGical
coefficients for directed intensities. The values of
W (h,E) for subterranean measurements were obtained in
iWf.2 and for the sea level measurements in Ref.3.
Results of a calculation of abar(e) are given in the
form of a graph (Fig.2) for various assumed values of the
effective index n of the differential spectrum of
Jr-meson production. Using abar(e) and WT(h,e) as
defined in eq.(2), the required coefficients are
presented graphically in Figs. 3 and 4 (cf. Ref.2). The
meteorological coefficients should not depend in practice
on the latitude of the observation point, nor on the
Card 2/3 local climatic conditions. ,Six graphs of numerical

120-2-13/37
,Meteorological coefficients for Or and 2Tr Counter Telescopes.
reference are given. There are 7 references, 5 of which
are Slavic.
SUMITTED: November 3, 1956.
ASSOCIATION: Scientific and Research Institute of Terrestrial
Magnetism, of the Ionosphere and of Radiowave Propagations.
(NauchnO-IBsledovatellskiy Institut Zemnogo Magnetizua,
'Ionosfery i Rasprostraneniya Radiovoln.)
AVAJUBLE: Library of Congress.
Card 3/3

XD
AUTHORS: Blokh, Ya.L. and Korablev, L.N. 120-5-13/35
TITLE: Automatic Recording of Cosmic Ray Ovtburst (Avtomaticheskaya
registratsiya vspyshek kosmicheskogo izlucheniya)
PERIODICAL: Fribory i Tekhnika Eksperimenta, 195?, No-5,
pp. 58 - 59 (USSR).
ABSTRACT: Studies of major solar outbursts in the intensity of
cosmic radiation (Ref.1) are of major interest in the solution
of the problem of the mechanism of production of cosmic rays
on the sun. To solve the theoretical problem it is necessary
not only to detect the presence of an increase in the intensity
but also to know the moment at which the intensity begins to
increase (to within a minute), the rate of growth up to the
maximum, and the rate of fall to the normal level thereaTter.
In accordance with the recommendation of the International
Committee for the IGY (15.'9.56) it is necessary to record
increases in the intensity of cosmic rays of the order of IV%
and their beginning to + 0-5 min. A method for an automatic
recording of the beginning of an increase in the intensity of
the hard component of cosmic radiation is now described.
Increases greater than or equal to 5% can be measured with an
accuracy of less than 0.5 min. The device includes a fast
Uardl/3 recorder of the number of coincidences seen by a cubic telescope

Automatic Recording of Cosmic Ray Outburst. 120-5-13/35
which is also used for the continuous recording of cosmic
radiation during the IGY. This telescope consists of three rows
of counters with a 10 cm lead screen between the second and
the third row. The instrument consists of two independent
systems (2 cubes). Coincidences between pulses from the first,
second and third rows are produced by the hard component.
Apart from the triple coincidences, double coincidences between
the first and the second and the second and the third rows are
also recorded. These coincidences are produced by the general
and the hard component in a wide solid angle and can be used
to determine the soft component. The beginning of the solar
outburst is determined from the double coincidences (first and
second row) which record the general component. This increases
the statistical accuracy and the accuracy of fixing of the
beginning of an outburst since the number of coincidences 1-2
is larger by a factor of 2.4 than the number of coincidences
1-2-3. In addition, the coincidences 1-2 record the general
component which in itself is more sensitive to solar outbursts
than the hard component (Ref.2). In summing up the number of
double coincidences 1-2 the total number of pulses increases
Gard2/3 to 240 000 per hour which in half-a-minute gives the
statistical

Automatic Recording of Cosmic Ray Outburst. 120-5-13/35
accuracy of + 2.2%. In order to increase the stability of the
working thre7hold, the recorded radiation is compvared with the
frequency of the standard oscillator urhich is stable to
0.1 - 0.01%. The comparison is carried out by means of a
discrete count of the radiation pul-ses and the pulses from the
oscillator using the counter circuit shovin in Fig.l. There
are 1 fiaure and 3 Slavic references.
ASSOCIATION: Scientific Research Institute for Geomagnetism of
the Ionosphere and Radio-wave Propagation
(Nau-,hno-issledovatellskiy Institut zemnogo magnetizma
lonosfery i rasprostraneniya radiovoln)
SUBMITTED: January 14, 195?.
AVAIIABIE: Library of uongress
Uard 3/3

BLOKH, YA.L.
"ELECTROMAG=C-CONDITIONS IN IN~ NETARY SPACE ACCORDING TO COS14IC
RAY VARIATION DATA FROM AUGUST, 20 TO SEPTEKER 10, 195711
Ya.L. Blokh, E.S. Glokova,,~L*'I* Dorman
Using correlation coefficients to.analyze the data on cosmic ray variation
provided by the-World International Network of Statifts for the period from
August
20 to September 10, 1957 (the period which witnessed several magnetic
stoma), It is
-shown that these variations could be explained by assuming the following
picture for
.the state-of interplanetary space during that period. We assumed that for a
long
time there.existed in interplanetary space a comparatively extensive, slow
corpuscular
stream with a "frozed" magnetic field of 10-5 gauss, Wit n the extensive
stream
a narrow fast stream with a 11frozed" magnetic -field of 10!~Igauss was
ejected from
the Sun and captured the Earth with its front edge at a distance of
approximately one
fourth of the stream's width from thr front,edge. A shock wave originated In
frontc-,
of that stream and caused an increase in cosmic ray intensity several- hours
before the
onset of the magnetic storm. Several days later. the Earth was captured by
another
stream with magnetic field perpendicular to the direction of propagation. In
this
stream the moving "frozed" magnetid field Induced a large electrical field,
which,
in turn, had evoked a substantial anistropy of cosmic rays.
report presented at the International Cowde Ray Conference, Moscow, 6-11
July 1959-

1101M. YA.L.
"CONCERNING THE MEMROLOGICAI EFnCT OF THE COSMC RAY SOFT COMPONENT"
Y-A.L. Blokh
By means of th Ie data cbtained~at Krasnan Pakhra (Moscow) through
continuous
recording o-r the cosmic ray soft component with the cubic telescope
counter designed
for the Soviet network of stations by the author, the variations of
atmospheric.origin
were studied. It is shown that these consist of barometric and sea
level temperature
..effects,and also of the temperature effect throughout the
atmosphere. The obtained
results are analysed from the point of view of Dorman's theory of
-.reteorological effects
of the soft component.
report presented at the International Cosmic Ray Conference, Moscow
6-11 July 1959

BLOO
"COSMIC RAY INTENSITYJNCWSE EFFECT PFOEDING MAG=C STOPMO
Ya.Lj Blokh, L. T9'D6rman,-R.-S-.''Xaminer
BY means of the experimental data obtained through continuous recording of
cosmic ray intensities by an international network of stations, a detailed
study is
made of the cosmic rky intenf3ity Increase-effect preceding magnetic storms. A
,statistical relationship is established between this effect and storms.of
different
types; with sudden and gradual beginning; effective and ineffective (in
relation
to the.decrease in cosmic ray Intensity); vez7 large-, large and
moderatestorm-s, etc.
On the basis of the data on different cosmic ray components, the energy
spectrum of
the particles-which determine the increase effect preceding the onset of
magnetic
storms Is determined. An estimate is made of the dependence of duration-and
aju
plitude
6f the affect upon the primary particle'energy. A possible interpretation. of
the
obtained results is given.
report presented at the International Cosmic Ray Conference, Moscow, 6_11
July 1959

EIDKH, YA'.L.
'ODEISFDMATIOWOF~M-WATURE OF THE* EARTHIS CAPTUFLE BT CORPUSCWJR
STRUM
AND THE STRUM VEMITY BY COSMIC RAY VAKATIONS DUUNG DIPMENT MAGNETIC
STORMS"
Ya. L. Blokh, L. 1:~.Dorman, N. S. Kaminer
The cbserved cosmi-a ray intensity variation' dw7ing different
magnetic storms is"
compared Vith those predicted under different suppositions
regarding the velocity.of
corpuscular streams having "frozed" magnetic fields and as to the
nature of the Earth's
capture by the streams (side or front edge nt different distances
from the axis of
the stream, etc). The stream velocity is obtained and a
determination is made of the
nature of the.Flarth's capture by the stream In different cases.
The obtained results
are compared with date on solarand magnetic activ,-ty, and
statistic regularities
are obtained for the stream velocity ard the nature of the Earth's
capture for magnetic
storms of different types and intensities.
report presented at the.Int arnational Cosmic Ray Conference,
Moscow, &11 July 1939

87h67
s/16q/6o/6oo/bi2/bo5/b1o
91 9 AOO5/AOOj
Translation from: Referativnyy zhurnal, Geofizika, 1960, No. 12,
p. 219, 16268
AUTHORS: Blokh, Ya Glokova, Ye. S., Doman, L. I.
TITLE: Investigation of the Nature of the Cosmic Ray Effect
During the
Magnetic Storm on August 29, 1957, on the Basis of Materials From
the
International Station Network of the IGY
PERIODICAL: V sb.: Variatsii kosmich. luchey pod zemley, na
urovne morya i v
stratosfere, No. 1, Moscow, AN SSSR, 1959, pp. 7-36
TEXT: The analysis is given of the great intensity decrease of
the cosmic
rays which began on August 29, 1957. The investigation was
performed on the basis
of the materials of the international network embracing 50
observation points
(77 recording devices). It was stated that the energy spectrum of
variation of
the primary cosmic rays, which caused the intensity decrease
effect, has the form-
SD (WD(E) = 0.17 A,
where A = -1 for F- < min/4, A - -(2/%) are sin (F-min/A-1) for
&min/4z- f
,i,/2, and A 0 for E < 9-mir/2 and P-min 90 Bev. The analysis
results allow
Card 1/2

87467
S/169/60/000/01P,/005/010
A005/AO01
Investigation of the Nature of the Cosmic Ray Effect During the
Magnetic Storm on
August 29, 1957, on the Basis of Materials From the
International Station Network
of the IGY
the following interpretation of the observed phenomena. A wide
corpuscular stream
containing the frozen-in regular magnetic field (H o-- jo-5 Gs)
hit the Earth with
its leading front on August 29. The scattering of the cosmic
rays by this field
led to the observed intensity decrease. The absence of
solar-diurnal variations
during this period points out that the direction of the
magnetic field In the
stream coincided apparently with the ecliptic plane. On
September 2, the Earth
was hit by the second corpuscular stream having caused a very
intense magnetic
storm and a new decrease in the cosmic ray intensity. The
analysis of the
diurnal variations, observed during this period, points out
that the magnetic
field frozen-in in the stream was oriented perpendicular to the
ecliptic plane.
The Investigation of some phenomena is presented, which
accompanied the main effect
of intensity decrease: a soft decrease and following increase
in intensity before
the beginning of the main effect, the alteration of the
variation spectrum with
time, and others. - There are 16 references. N. S, Kaminer
Translator's,note: This is the full translation of the original
Russian abstract.
Card 2/2

87h69
3, apo 00411,106.zi Ila) S/169/6o/ooo/ol2/Oo7/o1o
AOO5/AOO1
Translation from: Referativnyy zhumal,.Geofizika, 1960, No. 12, P.
219, # 16270
AUTFORS: Blokh, Ya. L., Ve Irnov, S. N., Dorman, L. I., Dubrovin,
M. M.
TITLE: Preliminary Results of an Investigation of the Underground
Variations
of Cosmic Rays
PERIODICAL::. V sb.: Variatsii kosmich. luchey pod zemley, na
urovne morya i v
stratosfere. No. 1, Moscow, AN SSSR,195.9, PP. 37-47
TEXT: The variations of the cosmic ray intensity are investigated
on the
basis of data obtained from acounter telescope of triple
coincidences, which was
located-under the earthis surface at the depth of 40 m of water
equivalent. By
the simple-correlation method the value of the barometric
coefficient /3 - (0.021 +
0.008) %/mb was obtained. The diurnal variation of the underground
intensity
amounts to about 0.05%. By averaging the data it is shown that the
average effect
at the depth of 40 m of water equivalent amounts to 0.3% during 11
events of
decreases of the Forbush type. The investigation of the disturbed
diurnal varzia-
tions in the cosmic ray intensity was also carried out. N. K.
Translator's note: This is the full translation of the original
Russian abstract.
Card 1/1

28833 0/169/61/0W/004/010~~
3.1-Y SO AOO5/AI3G
AUTHORS: Blokh, -Ya.L,i Dorman, L.I.; Kaminer, N.S.
TIM: Determination of the nature of earth's capture by streams, and
the
properties of-corpus6ular streams from cosmic ray variations during
sundry magnetic storms
MMIODICAL: Referativnyy zhurnal. Geofizika, no, 4, 1961, 17, abstract
4 0 160.
(Tr. Mezhdunar. konferentaii po kosmich. lucham, 1959, v. 4. Moscow,
AN SSSR, ig6o,'154 - 171)
TEXT: The authors atudy the variations in intensity of neutron and
hard
emission components of cosmic rays during.magnetio storms for the
period 1954
1959. The intensity variation profile was determined for each
individual in-
stance of Forbush effect and was compared with the theoretical
expectancy for
different assumptions regarding the velocity of solar corpuscular
streams, the
nature of earth's capture by streams and the struolure of the
magnetic field
frozen in the stream. The results of analysis are compared with the
nature of
the geomagnetic disturbances on the earth and the properties of the
active area
of the sun that corresponds to these disturbances. The authors show
that two
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21133 8/169/61/000/004/010/026
Determination of the nature of earth% capture by.... A005/A130
types of stream exist; 1) long-term extensive streams that capture
the earth by
their lateral face, and 2) narrow short-term streams oarrying
Intense frozen mag-
netic fields. Often the narrow streams move within the wide
streams. The field
intensity in the lateral outstripping section of the stream is on
an average .
twice as great as in the lagging section. The density of kinetic
e4ergy in the
stream decreases markedly for transition to the lagging lateral
section of the
stream. In the front section of the stream, substantial compression
(by a factor
of 6 - 10) of plasma and increase of the frozen magnetic field
occur,
N.K.
[Abstracter's note: Complete translation'..]
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28834 5/169/61/000/004/012/026-
AOO5/A13O
AUTHORS% Dorman, L.Lj Kaminer, N.S.
TITIEt The effect of cosmic ray Intensity increase preceding magnetic stma
PERIODICALs Referativnyy zhurnal~ Geofizika, no. 4, 1961, 17, abstract 4 a
101.
(Tr. Mezhdunar. konferentsii po koamioh. lucham, 1959, v. 4. Moscow,
AN SSSR, 178 - 191)
TRUi The authors study the effect of cosmic ray intensity increase pre-
ceding magnetic storms that is due to acceleration of charged particles
incident
to their collision with the front of the oorpusoular stream traveling from
the
sun. It is shown that this effect occurred prior to the magnetic storms of
July
8, 1998, and August 29, 1957. The longitudinal distributions of the
magnitude
and of the time of onset of the effect are elucidated. The authors'study
the en-
ergy spectrum of the emission responsible for anisotropio increase of
intensity.
Analysis of the increase In cosmic ray Intensity In the stratosphere on
July 8,
1958, suggests to the authors that a magnetic trap may exist in the
magnetized
frontal section of the corpusoular stream. This trap may carry particles
with
energies of some hundreds of Mev that have been accelerated in the active
region
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A

11134 8/169/61/000/004/011/026
The effect of cosmic ray intensity inorease4**. A005/A130
of the sun. Incident to collision of the stream with the earth the trap
breaks
up and the particles arrive in the high-latitude regions of the earth via
the
lines of force of the magnetic field. It is shown.in agreement with theory
that
incident to capture of the earth by the lateral face of the stream the
effect in-
crease of intensity prior to a magnetic storm does not occur. Capture of the
earth by the front section of the stream (storms with sudden onset), on the
other
hand, is always accompanied by the effect. No effects of acceleration of
cosmic
ray.,particles by the shocle wave generated by the front of the corpuscular
stream
was'detected.
VK
N. Kaminer
[Abstracter's note: Complete translation.]
;Card 2/2

_37932
S/035/6VbW/005/026/098
;Z or) A055/A101
AUTHORS; Blokh, Ya. L., Doman, L. I., Kaminer, N. S.
TITLE; Individual cases of the influence of magnetic storms on
cosmic rays
and their interpretation
PERIODICAL: Referativnyy zhunnal, Astronomiya I Geodeziya, no.
5, 1962, 31,
abstract'5A252 (V sb. "Variyatsii. kosmich'. luchey I solnechn.
korpuskulyarn. potoki. no. 2", Moscow, AN SSSR,1960, 5-57,
English'&)
TEXT: Approximately 40 cases of the Forbush effect (for the
years.1954-
1959) are investigated upon the b&sis of the available data on
the hard and the
neutron components of.cosmic rays. In the analysis of individual
Forbush effects,
it Is assumed that the profile of the effect In the Intensity of
cosmic rays is
determined by the manner i:n which the Earth comes acrosathe
corpuscular stream;
the front at different distances from the edge of the stream or
a lateral side
of the stream. Calculations and a comparison of the intensity
variations with
the magnetic disturbances and phenomena ori the Sun permit the
determination of
the parameters of the corpuscular streams conditioning the
magnetic storms and
the Forbush effects, i.e. the width of the streams, the
Intensity of the frozen-
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S/035/62/000/005/1026/098
Individual cases of the Influence ... A0551A101.
in.magnetic field and its configuration, the density of the
~stream. Although
a considerable spread of these,parameters was observed, It
proved possible to
detect the average.regularities. The intensity of the field is
considerably
higher in the leading lateral part of the corpuscular streams
than in the
lagging part. Therefore, when the Earth comes acrossa lateral
part of the streaiq
the drop of the intensity of cosmic rays occurs more rapidly
than the return to
the normal level. The kinetic energy density also decreases from
the front
lateral edge to the rear edge of the stream, which explains the
shorter duration
of geomagnetic storms in comparison with the Forbush effects
duration. The
front of,the stream has'a greater density, and the magnetic
field intensity is
here several times higher than in the rest of the stream.
Therefore, when the
Earth comes across the front of the stream, a magnetic storm
with sudden
commencement is observed, as well as a sharp drop of the cosmic
rays intensity..
A few hours before the Earth comes across the front of the
stream, an increase
in intensity I$ observed on the morning-side of the Earth, this
increase being
conditioned by the reflection of cosmic radiation particles from
the moving
front of-the stream. No such intensity increase is observed when
the Earth comes
across ?.oflateral side of the stream.
[~bstracterls notet Complete translation] N. Xaminer
Cird-2/2

c'/169/62/060/004/061/1'03*
G
D228/D302
AUTHOR: Blokh, Ya.L.
TITLE: Standard cubic telescope
PERIODICAL: Referativnyy zhurnalp Geofizika, no. 4, 1962v 3t ab-
stract 4.G17 (V ab. Kosmicheskiye luchi, no. 3, Met
AN SSSR9 1961t 80-104)
TEXT: A description is given of a standard cubic telescope, produ,
ced at the Institut zemnogo magnetizma i rasprostraneniya radiovoln
AN SSSR (Institute of Terrestrial Magnetism and Radiowave Propaga-
tion, Academy of Sciences, USSR) for investigating cosmic rays in
accordance with the IGY program* [Abstractor's note: Complete trans-
lation.l.
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37286
D/186Y62/000/004/071/103
3, )~Y/o (:X;z4g, 21 D302
AUTHOR.S: Blokht Ya.L._t Dormang Lelet and Dubrovin, It.M.
TITLE: Meteorological effects of cosmic rays under the
earth's surface
PERIODICAL: Referativnyy zh~urnal. Geofizika, no. 4, 1962t 13,
ab-
stract 4G70 (V. sb. Kosmicheskiye luchip no, 3# Dl-t
AN SSSR, 1961, 166-169)
TEXT: A study is reported of meteorological effects in the
ji-meson
component of cosmi abased on underground recordings in Moscow
ic rays
(40 m) and Yakutsk (60 m~ in 1957 - 1956. The
triple-correlation
method was used to determine-the partial and total correlatiqn
and
regression coefficients a and P between the observed
cosmic-ray in-
tensity variationsp the barometric pressure and the
temperature of
the atmosphereg (P is the barometric coefficient and a is the
tem-
perature coefficient_representing atmospheric temperature
variatiors
up to heights of 12 20 km). Although the values of a and P
obtai-
;-ned for separate months exhibit a large spreadt their
average values.
are quite reliable and are in good agreement with the
theoretical

B/16 62/000/004/071/103
Meteorological effects of cosmic ... D218YD302
results. For Moscow (40 m) P = (-0.050 t 0.007) %/mb and for Ya-
kutsk (60 m): 0 = (-0.029 0.006) %/mb. Comparison of the values
of a shows that the upper layers of the atmosphere play an impor-
tant role in producing the temperature effect in the hard components
[Abstractor's note: Complete translation].
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S/169/62/000/004/074/103
fao I)218/D302
3, 2. Y/0 ' )-
AUTHORS: Dorman L.Ief Blokh, Ya.L., and Kaminer, N.S.
TITLE: The character of the increase in the cosmic-ray inten-
sity at the Forbush-effect minimum
PERIODICAL: Referativnyy zhurnal, Geofizikaj no. 4, 1962p 14t ab-
stract 4G73 (V.-sb. Kosmicheskiye luchil no. 4, M.,
AN SSSR, 1961p 5-15)
TEXT: The method of coupling coefficients is used to investigate
the increase in cosmic-ray intensity during the principal phase
of
geomagnetic storms which is due to a reduction in the H-component
~of the magnetic field, and the compression of the volume of the
geo-
magnetic field by a corpuscular stream. A theoretical calculation
is given of the effects expected in the various secondary compo-
nents of cosmic rays at sea level and in the mountains. The
results
of these calculations are compared with experimental data
obtained
by the world station network during the magnetic storms of
Septem-
ber 13, 1957 and February 11, 1958. It follows from the analysis
of
these two cases that the observed increase in the cosmic-ray
intens-
ard(112`1

B/169/62/000/004/074/103
The character of the increase in the ... D218/D302
ity is in fact associated with a reduction in the geomagnetio cut-
off threshold during the principal phase of a magnetic storm. It is
noted that in the case of the hard component the effect is only
par-
tly due to the change in the geomagnetic threshold. A part of the
effect is due to a disturbed solar-diurnal variation. It was found
that there is not only a latitudep but also a longitude dependence
of the amplitude of the increase, and hence it follows that the ca-
vity which appears as a result of the flow of the corpuscular stTWm
round the geomagnetic field is not axially symmetric in form. It is
concluded that geomagnetic storms with sudden commencement are pro-
duced as a result of the capture of the earth by the leading front
of a solar corpuscular stream which flows round the geomagnetic
field with ultrasonic velocity. [Abstractorlq note: Complete trans-
lation].
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:3 0 (2,;.0s- '-2'7'0r' ;-e6s)- S/169/62/000/004/076/103
D218/D302
3,V-),0
AUTHORS: Blokh, Ya.L.t Kaminert N,S.? and Dormant L.I.
TITLE: Cosmic-ray effects preceding a magnetic storm
PERIOM CAL: Referativnyy zhurnal, Geofizika, no. 41 1962y 14p
ab-
stract 4G75 (V ab. Kosmicheskiye luchi, no. 4. Ides
AN SSBRI 1961p 25-30)
TEXT: Discusses the interaction of the magnetized front of a
cor-
puscular stL-am with cosmic rays which may give rise to the
appear-
ance of certain effects just before the onset of a magnetic
storm.
A corpuscular stream produces a shock wave in the interplanetary
space, and the magnetic field of this wave interacts with
cosmic-
ray particles. Reflection of the particles from the wave front
gi-
ves rise to their acceleration, and therefore the intensity of
the
radiation should increase before a magnetic storm. The expected
spectrum of this variation is relatively soft. After the earth
has
entered the disturbed medium behind the shock wave front, where
the
magnetized interplanetary plasma is compressed and the field is
correqRgndingly enhanced, the cosmic-ray intensity should
decrease.

B/169/62/000/004/076/103
Cosmic-ray effects preceding a ... D218/D302
This effect is aniBotropic and the character,of the anisotropy de-
pends on the direction of the interplanetary magnetic field. Reflec-
tion of cosmic-ray particles directly from the magnetized front of
the moving,,.orpuscular stream should lead to an anisotropic inerea::,)
se in the iatensityt a few hours prior to the beginning of the Seo
~.magnetic storm. This type,of increase in the intensity has in fact
been observ..Bd before a number of geomagnetic storms accompanied by
large Forbush effects. [Abstractor's note: Complete translation].
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37280
S1169 62/000/004/065/103
D228/D302
AUTHORS: Kaminer, N.S.9 Blokh, Ya.L., and* Dormang L.I.
TITLE: The emission duration and the angular width of solar
corpuscular flows
PERIODICAL: Referativnyy zhurnal Geofizika, no. 4, 1962, 10, ab-
stract 4G53 (V sb. Kosmich. luchi, no. 4, M.p AN SSSRp
1961,'31 - 34)
TEXT: The width of solar corpuscular flows is determined from the
profile of Forbuoh-effects in cosmic rays; this is then compared
with the angular width (the longitudinal extent) of the active re-
gions on the sun that have caused the generation of these corpuscu-
lar flows# A positive correlation with a correlation coefficient of
^j 0.9 and a regression coefficient of jl was discovered between
these two parameters. The estimation of the angular flow width
acocr-
ding to geomagnetic disturbances gives a considerably smaller angu-,
lar width. The possible causes of the divergences in the estimation
of the flow.width by these two methods are briefly discussed, A
number of arguments are cited in favor of the fact that geoeffecti-.
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S/169/62/000/004/065/103
The emission duration and the ... D228/D302
ve corpuscular flows are continuously emitted by active regions
du--
ring long intervals of time (several revolutions of the sun). At
the same time it is possible that plasma clouds are ejected from
an
active region when the.emission of a corpuscular flow haB'Yet to
be
completed. [Abstractor-a note: Complete translation].
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37293
S/169/62/000/004/078/103
70 r/ D218/D302
AUTHORS: Dormano L.I.t Kaminert N.S.v and Blokhj Ya-L.
TITLE: On the nature of the preliminary reduction in the
cosmic-ray intensity before a magnetic storm
PERIODICAL: Referativnyy zhurnal. Geofizika, no. 4, 1962t 14-15,
abstract 4G77 (V sb. Kosmicheskiye luchip no, 4, Met
AN SSSR, 1961, 49-58)
,TEXT: A discussion is given of the nature of the preliminary reduc-
tion in the cosmic-ray intensity which is observed before the onset
of many magnetic storms accompanied by the Forbush effect. The mo-.
tion of a corpuscular stream with a velocity of esjioa cm/sec
through interplanetary medium containing a weak magnetic field,
should lead to the appearance of a shock wave moving towards the
earth with a velocity equal to 4/3 of the velocity of the stream. i
The magnetic field of the medium behind the shock wave front is en-,
hanced. Hence, the arrival of the shock wave at the earth should be~.
accompanied by a reduction in the cosmic-ray intensity. If the in-
terplanetary magnetic field is regularp and is directed at right
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S/169/62/000/004/078/103
On the nature of the preliminary ... D218/D302
angles to the plane of the ecliptic in the same sense as the
earth's
field, then the maximum reduction in the intensity should be
obser-
ved for particle streams arriving from the West relative to the
sun
-earth line. In order to confirm these conclusions on the basis of
the world station network data, an analysis was carried out of the
cosmic-ray intensity variations during periods preceding major
geo-
magnetic disturbances and Forbush effects. A.study of the longitu-
de and latitude dependence of the preliminary reduction in the in-
tensity,shows that the effect is particularly appreciable for
those
groups of stations for which the particles arrive preferentially
from the direction of the sun, or from a direction west of the
earth-sun line. The spectrum of the preliminary reduction effect
is.
close to the Forbush decrease spectrumt although it is slightly
sof-
ter than the latter. LAbstractor's note; Complete translation].
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S/169/62/000/005/071/093
D228/D307
AUT',:ORS.- Kaminer, N". S., Dorman, L. I. and Blokh, Ya.
TI TLE: The magnetic storm in mid-May 1959 and cosmic ray
variations
PERIODICAL: Referativnyy zhurnal, Geofizika, no. 5, 1962, 10, ab-
stract 5GS3 (V sb. Kosmich. luchi, no. 4, M., AN SSSR,
1961, 59-83)
TEXT: The intricate complex.of phenomena, ob5erved in co5mic rays
in connection with the solar chromospheric flare of 10/V/19599 is
being studied from the data of the world station network. These
Dhenomena include: the large increase in the intensity of soft
cosmic rays o,f a solar origin in the stratosphere in high lati-
tudes, the Forbush-effect, the intensity increase befo~re th6.be_'-"I-,'~
ginning of the geomagnetic storm, etc. A marked increase in.the.
intensity of cosmic rays was noted for several days before the
start of the 'Forbush-ef0fect. The peculiarities of this phenomenon
compel one to assume that it is due to the arrival of an additio-
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0
S/169/62/000/005/071/093
The magnetic storm D228/D307
nal radiation flow, generated on the sun and coming tourards the
earth as a result of diffusion in magnetic irregularities with a.
-L-eld intensity of -3 x 10-4 -3
i _ 10 gauos. The beginning of the
Forbush effect of May 11 occurred simultaneously throughout the
world. In the first place the reduction's effect started at sta-
tions where particles, coming from westwards directions in rela-
tion to the line sun-earth, were recorded. At these stations the
reduction's effects began three hours before the outbreak of the
geomagnetic storm. For particles arriving from eastwards direc-
tions in relation to the line sun-earth, the efffect commenced
2 - 3 hours after the beginning of the storm. The epigenetic spec-
t1rurn of the primary radiation's variation during the Forbush ef-
.Lect- was determined. This spectrum agrees with the supposition
that cosmic rays are scattered by the regular magnetic field fro-
zen into'the flow. The parameters of the corpuscular flow and of
the magnetic field.frozen into it were ascertained from the'pro-
file of t-he Forbush effect. The flow's width amounts to x jo13
-cm, the mean intensity of the field in it being -,6 x 1079 gauss.
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S/169/62/000/005/671/093
D228/D307
The nature o--,' the increase in the intensity in the minimum of
the
Forbush effect, observed an May 12-14, is discussed. It is shown
that only a small part of the effect of the intensity's increase
is explained by the change in the geomagnetic trimming threshold;
the main cause of this phenomenon may be the anisotropic screening
of the earth by the corpuscular flow. Z-Abstracter's note: Com-
Dlete translation.-7
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37294
8/169/62/000/004/079/103
D218/D302
AUTHORS: Blokhj, Ya.L#j Dormanp L#I., and Kaminer, N.S.
TITLE: On the superposition of Forbush effects in July 1959
PBRIODIOAL; Referativnyy zhurnal. Geofizika, no. 4, 1962t 15t ab-
stract 4G78 (V ab. Kosmicheakiye luchip no. 4, 11-t
AN SSSRt 1961,64-9?)
TEXT: A detailed study is reported of the character of the super-
position of Forbush effects in July 1959. Analysis of world station
network data shovied that the observed phenomena may be explained by
assuming that the modulation of cosmic rays is due to regular magne-
tic fields frozen-into corpuscular streams. The second and third
Forbush decreaseB occurred as a result of the simultaneous capture
of the earth by two or even three corpu8cular streams. The proper-
ties of these streamsp their dimensions and the intensity of the
frozen-in magnetic fields are determined. The energy spectrum of
the increase in the cosmic-ray intensity observed on July 17 is de-
termined. Analysis of this effect is used to estimate the intensity~
of the magnetio field of the stream which is found to be in good
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