Published November 21, 2001
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Measuring Solar Abundances
Abstract
This is the rapporteur paper of Working Group 2 on Measuring Solar Abundances. The working group presented and discussed the different observations and methods for obtaining the elemental and isotopic composition of the Sun, and critically reviewed their results and the accuracies thereof. Furthermore, a few important yet unanswered questions were identified, and the potential of future missions to provide answers was assessed.
Additional Information
© 2001 American Institute of Physics. Issue Date: 21 November 2001. We gratefully acknowledge the effort of the scientific and local organisation committees, in particular of Robert F. Wimmer-Schweingruber, in making this workshop happen. We also thank Sylvie Vauclair and Robert F. Wimmer-Schweingruber for useful comments on the manuscript. JML was supported by NRL/ONR Solar Magnetism and the Earth's Environment 6.1 Research Option and by NASA Contracts W19473 and S137836.Attached Files
Published - STEaipcp01.pdf
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STEaipcp01.pdf
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Additional details
- Eprint ID
- 27840
- Resolver ID
- CaltechAUTHORS:20111117-145415835
- NRL/ONR Solar Magnetism and the Earth's Environment 6.1 Research Option
- NASA
- W19473
- NASA
- S137836
- Created
-
2011-11-21Created from EPrint's datestamp field
- Updated
-
2021-11-09Created from EPrint's last_modified field
- Caltech groups
- Space Radiation Laboratory
- Series Name
- AIP Conference Proceedings
- Series Volume or Issue Number
- 598