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New SEP-Based Solar Abundances

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

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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:
URLURL TypeDescription
http://adsabs.harvard.edu/abs/1993ICRC....3..384GADSArticle
ORCID:
AuthorORCID
Stone, E. C.0000-0002-2010-5462
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:
Funding AgencyGrant Number
NASANAS7-918
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

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