Published October 1994
| public
Book Section - Chapter
Composition of energetic particles from solar flares
- Creators
- Garrard, T. L.
-
Stone, E. C.
- Other:
- Horneck, G.
Abstract
We present a model for composition of heavy ions in the solar energetic particles (SEP). The SEP composition in a typical large solar particle event reflects the composition of the Sun, with adjustments due to fractionation effects which depend on the first ionization potential (FIP) of the ion and on the ratio of ionic charge to mass (Q/M). Flare-to-flare variations in composition are represented by parameters describing these fractionation effects and the distributions of these parameters are presented.
Additional Information
© 1994 COSPAR. This work was supported in part by NAS7-918 and NAGW-1919. The data analysis work done by Caltech student Todd Rope was invaluable. The following people were generous with their time and copy machines in assisting us to collect and evaluate the literature reviewed here, and we appreciate it: J. Feynman, S. Kahler, G. Mason, J. Mazur, R. McGuire, R. Mewaldt, E. Moebius, D. Reames, and G. Spitale.Additional details
- Eprint ID
- 43800
- Resolver ID
- CaltechAUTHORS:20140212-144700326
- NASA
- NAS7-918
- NASA
- NAGW-1919
- Created
-
2014-02-21Created from EPrint's datestamp field
- Updated
-
2021-11-10Created from EPrint's last_modified field
- Caltech groups
- Space Radiation Laboratory
- Series Name
- Advances in Space Research
- Series Volume or Issue Number
- 14