Published 2005
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The effect of cosmic ray energy changes in the heliosphere on K-capture
Abstract
In an accompanying paper we give a re-assessment of cosmic ray energy changes in the heliosphere to determine the effects of acceleration at the solar wind termination shock and modulation in the heliosheath beyond that. In this paper we show that these effects have important consequences for the interpretation of secondary to primary ratios of cosmic rays at energies below 1 GeV, i.e. in the region where they are strongly modulated
Additional Information
Copyright TATA Institute of Fundamental Research. This work was supported by NSF Grant ATM 0107181 and the South African National Research Foundation. RCL was supported by UNAM-DGAPA grant IN106105.Attached Files
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Additional details
- Eprint ID
- 56467
- Resolver ID
- CaltechAUTHORS:20150408-092437734
- ATM-0107181
- NSF
- South African National Research Foundation
- IN106105
- UNAM-DGAPA
- Created
-
2015-04-16Created from EPrint's datestamp field
- Updated
-
2019-11-22Created from EPrint's last_modified field
- Caltech groups
- Space Radiation Laboratory
- Other Numbering System Name
- Space Radiation Laboratory
- Other Numbering System Identifier
- 2005-22