Published July 15, 1979
| Published
Journal Article
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The isotopic composition of solar flare accelerated neon
Chicago
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Abstract
The individual isotopes of neon in energetic solar flare particles have been clearly resolved with arms mass resolution of 0.20 amu. We find ^(20)Ne/^(22)Ne = 7.6 (+2.0, -1.8) and ^(21)Ne/^(22)Ne ≾ 0.11 in the 11-26 MeV per nucleon interval. This isotopic composition is essentially the same as that of meteoritic planetary neon-A and is significantly different from that of the solar wind.
Additional Information
© 1979 American Astronomical Society. Received 1979 March 12; accepted 1979 April 6. W. E. Althouse, A. C. Cummings, and T. L. Garrard made significant contributions to the design and development of the HIST instrument. This work was supported in part by NASA under contract NAS5-20721 and grant NGR 05-002-160.Attached Files
Published - 1979ApJ___231L__97M.pdf
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Additional details
- Eprint ID
- 43738
- Resolver ID
- CaltechAUTHORS:20140210-110925110
- NASA
- NAS5-20721
- NASA
- NGR 05-002-160
- Created
-
2014-02-10Created from EPrint's datestamp field
- Updated
-
2021-11-10Created from EPrint's last_modified field
- Caltech groups
- Space Radiation Laboratory
- Other Numbering System Name
- Space Radiation Laboratory
- Other Numbering System Identifier
- 1979-01