Mewaldt, R. A. and Stone, E. C.
(1987)
Isotope Abundances of Solar Coronal Material Derived from Solar Energetic Particle Measurements.
In:
Proceedings of the 21st International Cosmic Ray Conference.
Vol.3.
, Nakau, Russia, pp. 255-258.
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Abstract
Coronal isotopic abundances for the elements He, C, N, 0, Ne, and Mg are derived
from previously published measurements of solar energetic particles by first measuring,
and then correcting for the charge-to-mass-dependent fractionation due to solar flare
acceleration and propagation processes. The resulting coronal composition generally
agrees with that of other samples of solar system material, but the previously noted
difference between the solar flare and solar wind ^(22)Ne/^(26)Ne ratios remains unresolved.
Item Type: | Book Section |
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Additional Information: | © INR. Provided by the NASA Astrophysics Data System.
We are grateful to R. E. Vogt and J. D. Spalding for their
contributions to the HIST program. This work was supported in part by NASA grants
NAG5-722 and NGR 05-001-160. |
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Group: | Space Radiation Laboratory |
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Funders: | Funding Agency | Grant Number |
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NASA | NAG5-722 | NASA | NGR 05-001-160 |
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Other Numbering System: | Other Numbering System Name | Other Numbering System ID |
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Space Radiation Laboratory | 1987-09 |
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Record Number: | CaltechAUTHORS:20140512-141332323 |
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Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20140512-141332323 |
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Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. |
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ID Code: | 45698 |
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Collection: | CaltechAUTHORS |
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Deposited By: |
Joy Painter
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Deposited On: | 12 May 2014 21:18 |
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Last Modified: | 20 Feb 2020 14:33 |
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