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A simulation of high energy cosmic ray propagation 2The cosmic ray propagation in the Galactic arm is simulated. The Galactic magnetic fields are known to go along with so called Galactic arms as a main structure with turbulences of the scale about 30pc. The distribution of cosmic ray in Galactic arm is studied. The escape time and the possible anisotropies caused by the arm structure are discussed.
Document ID
19850025766
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Honda, M. (Tokyo Univ.)
Kamata, K. (Tokyo Univ.)
Kifune, T. (Tokyo Univ.)
Matsubara, Y. (Kyoto Univ.)
Mori, M. (Kyoto Univ.)
Nishijima, K. (Kobe Univ.)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: 19th Intern. Cosmic Ray Conf - Vol. 2
Subject Category
Space Radiation
Report/Patent Number
OG-5.4-2
Accession Number
85N34079
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle19850025693Collected WorksNinteenth International Cosmic Ray Conference. OG Sessions, Volume 2
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