Published 1999
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Basic Properties of Anomalous Cosmic Ray Spectra
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Abstract
The anomalous cosmic ray component is a much more sensitive probe of modulation/acceleration in the heliosphere than galactic cosmic rays. Based on one-dimensional, no-drift solutions of the transport equation, we formulate several properties that govern their acceleration and modulation.
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© University of Utah. Provided by the NASA Astrophysics Data System.Attached Files
Published - 1999-39.pdf
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- 54833
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- CaltechAUTHORS:20150213-110756759
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- http://adsabs.harvard.edu/full/1999ICRC....7..543M (URL)
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2015-02-20Created from EPrint's datestamp field
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2019-10-03Created from EPrint's last_modified field
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- Space Radiation Laboratory
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- 1999-39