Published 1983
| Published
Book Section - Chapter
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A Search for ^2H, ^3H, and ^3He in Large Solar Flares
- Creators
-
Mewaldt, R. A.
-
Stone, E. C.
- Other:
- Durgaprasad, N.
Abstract
The results of a new study of solar flare H and He isotopes imply that earlier observations have significantly overestimated the abundances of ^2H, ^3H, and ^3He in large solar flares. We find no evidence that solar flare nuclei have suffered any significant amount of fragmentation before escaping from the Sun.
Additional Information
We thank R. Ramaty and R. McGuire for instructive discussions, and R. Vogt and G. Hurford for their many contributions to our IMP program. This work was supported in part by NASA under contract NAS5-25789 and grant NGR 05-002-160.Attached Files
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Additional details
- Eprint ID
- 45152
- Resolver ID
- CaltechAUTHORS:20140423-133130136
- NAS5-25789
- NASA
- NGR 05-002-160
- NASA
- Created
-
2014-04-24Created from EPrint's datestamp field
- Updated
-
2020-02-20Created from EPrint's last_modified field
- Caltech groups
- Space Radiation Laboratory
- Other Numbering System Name
- Space Radiation Laboratory
- Other Numbering System Identifier
- 1983-06