Published 1999
| Published
Book Section - Chapter
Open
Basic Properties of Anomalous Cosmic Ray Spectra
- Creators
- Moraal, H.
- Steenberg, C. D.
- Others:
- Kieda, D.
- Salamon, M.
- Dingus, B.
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.
Additional Information
© University of Utah. Provided by the NASA Astrophysics Data System.Attached Files
Published - 1999-39.pdf
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Additional details
- Eprint ID
- 54833
- Resolver ID
- CaltechAUTHORS:20150213-110756759
- Created
-
2015-02-20Created from EPrint's datestamp field
- Updated
-
2019-10-03Created from EPrint's last_modified field
- Caltech groups
- Space Radiation Laboratory
- Other Numbering System Name
- Space Radiation Laboratory
- Other Numbering System Identifier
- 1999-39