SCIENTIFIC ABSTRACT MADORSKIY, Z.N. - MADYANOV, A.M.
Document Type:
Collection:
Document Number (FOIA) /ESDN (CREST):
CIA-RDP86-00513R001031320016-4
Release Decision:
RIF
Original Classification:
S
Document Page Count:
100
Document Creation Date:
November 2, 2016
Document Release Date:
August 31, 2001
Sequence Number:
16
Case Number:
Publication Date:
December 31, 1967
Content Type:
SCIENTIFIC ABSTRACT
File:
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Body:
TATAUROV, Yi.Ya.0.5 Mev and electrons with energies >40 kev) was registered
by another counter of the same type which was also shielded by copper but had, in
addition, a 1.2 mg + 0.3 mg/cM2 mica and gold sheet forming a small window 0.5 cm in
diameter. The total eometry factor of the counters for the isotropic hard radia-
tion was 2.6 1 0.2 cm . The counting rate was recorded on a logarithmic scale. The
error in transmission of the radiation count data did not exceed 3%. The average
count rate of hard radiation recorded between 31 March and 3 April 1966 was
12.2 1 0.1 particles/Bec, which corresponds to a flux of 4,7 t 0.4 particles/cM2.sec.
The data.indicate that the intensity of primary cosmic radiation is characteristic
Card 1/2 UDC: 537-591+523-165
ACC NR: AP6032854
-PW
4-3W
0 0
Fig. 1. Radiation counting rate as a
function of distance from the Moon.
for the minimum solar activity cycle. Luna-10 was placed in a selenocentric orbit
on 3 April 1966 'with an apogee of 1000 km,a perigee of 350 km, and an angle of
inclination of 72' with respect to the Moon's axis. The counting rate is plotted as
a function of altitude in Fig. 1. Orig. art. has: 1 figure.
SUB CODE:O//,V ~UBM DATE: o4jul66/. ORIG REF: 001/ ATD PRESS: 5099
/ 2
Distance from Moon's surf Ece
MADVID,I, I.I.V.; SIIFV-ISOV, G.A.
Theor7 and design of universal profilometers. Avton.kont.1 JzE7.
takh. no.2:47-59 158. NIRA 11:7)
(Electric measureoents)
-ACC NIZ. AP7007597 SOURCZ ccD'.'; UR/0293/66/004/006/0342/0850
G:`go_-0v, N. L.; V. L. Pizaran.