CaltechAUTHORS
Published 1990 | Version Published
Book Section - Chapter Open

Energy Spectra Between 10 and Several Hundred GeV/Nucleon for Elements from _(18)Ar to _(23)V: Results from HEAO-3

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Contributors

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.

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Published - 1989-06.pdf

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Eprint ID
45415
Resolver ID
CaltechAUTHORS:20140501-111300538

Related works

Describes
http://adsabs.harvard.edu/full/1990ICRC....3...19V (URL)

Funding

NASA
NAG8-498
NASA
NAG8-500
NASA
NAG8-502
NASA
NGR 05-002-160
NASA
NGR 24-005-050
NASA
NGR 26-008-001

Dates

Created
2014-05-07
Created from EPrint's datestamp field
Updated
2020-03-09
Created from EPrint's last_modified field

Caltech Custom Metadata

Caltech groups
Space Radiation Laboratory
Other Numbering System Name
Space Radiation Laboratory
Other Numbering System Identifier
1989-06