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Published 2005 | Version Published
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The effect of cosmic ray energy changes in the heliosphere on K-capture

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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.

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56467
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CaltechAUTHORS:20150408-092437734

Related works

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http://adsabs.harvard.edu/abs/2005ICRC....2...85C (URL)

Funding

NSF
ATM-0107181
South African National Research Foundation
UNAM-DGAPA
IN106105

Dates

Created
2015-04-16
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Updated
2019-11-22
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Space Radiation Laboratory
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Space Radiation Laboratory
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2005-22