Other
Scientific paper
Nov 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..598..113k&link_type=abstract
SOLAR AND GALACTIC COMPOSITION: A Joint SOHO/ACE Workshop. AIP Conference Proceedings, Volume 598, pp. 113-119 (2001).
Other
6
Composition, Particle Emission, Solar Wind, Solar Instruments
Scientific paper
The Sun is the largest reservoir representing the matter of the early solar nebula. Its isotopic composition for the elements N, Ne, Mg, Si, Ar, and Fe has been determined by measuring solar wind abundances with the CELIAS experiment on board SOHO and other spacecraft instruments. These measurements and theoretical considerations indicate that the solar wind, in particular the coronal-hole type solar wind, is much less isotopically fractionated than solar energetic particles. The data give evidence that the isotopic abundance ratios typically vary by only ~1-2% per amu in different solar wind regimes such as coronal-hole type and streamer-belt associated solar wind, ejecta of coronal mass ejections (CMEs), or so-called ``blobs''. .
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