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Penetration of solar protons into the Earth's magnetosphere on November 22, 1977The low polar-orbiting Cosmos-900 satellite carried a large geometric factor Cerenkov counter to study the particle anisotropy and spectrum near the proton increase peak in solar cosmic rays. The data help understand different temporal behavior of the increases detected at the stations because the whole set of data showed that the angular distribution of solar cosmic ray particles in interplanetary space was narrow throughout the observation time, resulting in a rapid variation of particle intensity near the poles. The power-law index of the solar cosmic ray integral spectrum varied from -2.4 to -5.2 in the 1 to 4 GV rigidity range from 10.31 to 11.25 UT on November 22, 1977. The flare-time data from all orbits indicate an increased radiation intensity on L=3.5 to 4.0.
Document ID
19850026775
Acquisition Source
Legacy CDMS
Document Type
Other
Authors
Gorchakov, E. V.
(Moscow State Univ.)
Afanasyev, V. G.
(Moscow State Univ.)
Afanasyev, K. G.
(Moscow State Univ.)
Ignatyev, P. P.
(Moscow State Univ.)
Iozenas, V. A.
(Moscow State Univ.)
Ternovskaya, M. V.
(Moscow State Univ.)
Zenchev, G. G.
(Moscow State Univ.)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: 19th Intern. Cosmic Ray Conf - Vol. 5
Subject Category
Solar Physics
Report/Patent Number
SH-6.1-15
Accession Number
85N35088
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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