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The origin of cosmic raysData related to the development of cosmic rays are discussed. The relationship between cosmic ray production and the steady-state Boltzmann equation is analyzed. The importance of the power-law spectrum, the scattering rate, the theory of shock acceleration, anisotropic instabilities, and cosmic ray diffusion in the formation of cosmic rays is described. It is noted that spacecraft observations at the earth's bow shock are useful for studying cosmic rays and that the data support the collisionless shock-wave theory of cosmic ray origin.
Document ID
19870029644
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Eichler, D.
(Maryland, University College Park; Negev, University, Beersheba, Israel)
Date Acquired
August 13, 2013
Publication Date
January 1, 1986
Publication Information
Publication: New York Academy of Sciences, Annals
Volume: 470
ISSN: 0077-8923
Subject Category
Space Radiation
Accession Number
87A16918
Funding Number(s)
CONTRACT_GRANT: NSF AST-83-17755
Distribution Limits
Public
Copyright
Other

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