Published 1990
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Energy Spectra Between 10 and Several Hundred GeV/Nucleon for Elements from _(18)Ar to _(23)V: Results from HEAO-3
Abstract
We report updates of recently published results on cosmic ray energy spectra of the sub-iron nuclei. This paper is based on the following analysis and improvements : a) a better analysis of the charge resolution of the instrument, b) availability of more recent charge-changing cross sections necessary to correct the abundances for interactions inside the detector, and c) a recent revision of the results from the French-Danish C2 experiment on HEA0-3 that were included in our analysis.
Additional Information
© Organizing Committee of the 21st Int. Cosmic Ray Conf. Provided by the NASA Astrophysics Data System. This research was supported in part by NASA grants NAG8- 498, 500, 502 and NGR 05-002-160, 24-005-050 and 26-008-001. The assistance of E. C. Stone is gratefully acknowledged.Attached Files
Published - 1989-06.pdf
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1989-06.pdf
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Additional details
- Eprint ID
- 45415
- Resolver ID
- CaltechAUTHORS:20140501-111300538
- NASA
- NAG8-498
- NASA
- NAG8-500
- NASA
- NAG8-502
- NASA
- NGR 05-002-160
- NASA
- NGR 24-005-050
- NASA
- NGR 26-008-001
- Created
-
2014-05-07Created from EPrint's datestamp field
- Updated
-
2020-03-09Created from EPrint's last_modified field
- Caltech groups
- Space Radiation Laboratory
- Other Numbering System Name
- Space Radiation Laboratory
- Other Numbering System Identifier
- 1989-06