Garrard, T. L. and Stone, E. C. (1993) New SEP-Based Solar Abundances. In: 23rd International Cosmic Ray Conference. University of Calgary , Calgary, Canada, pp. 384-387. https://resolver.caltech.edu/CaltechAUTHORS:20140212-100928259
Full text is not posted in this repository. Consult Related URLs below.
Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20140212-100928259
Abstract
The relative abundances of various elements in the solar photosphere and the solar corona are re-determined from relative abundances of solar energetic particles (SEP) in the light of revised solar spectroscopic abundances. We find excellent correlation between SEP-based abundances and spectroscopic abundances, after correcting for fractionation due to ionic charge-to-mass ratio and first ionization potential.
| Item Type: | Book Section | ||||||
|---|---|---|---|---|---|---|---|
| Related URLs: |
| ||||||
| ORCID: |
| ||||||
| Additional Information: | © 1993 University of Calgary. This work has been partially supported by NASA under NAS7-918. We acknowledge excellent assistance from M. Looper in data analysis and presentation. | ||||||
| Group: | Space Radiation Laboratory | ||||||
| Funders: |
| ||||||
| Record Number: | CaltechAUTHORS:20140212-100928259 | ||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20140212-100928259 | ||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | ||||||
| ID Code: | 43793 | ||||||
| Collection: | CaltechAUTHORS | ||||||
| Deposited By: | Tony Diaz | ||||||
| Deposited On: | 24 Feb 2014 19:27 | ||||||
| Last Modified: | 20 Feb 2020 14:33 |
Repository Staff Only: item control page
