Solar Coronal Abundance Variations

Details Solar Coronal Abundance Variations Solar Coronal Abundance Variations

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003agufmsh11a..01k&link_type=abstract

American Geophysical Union, Fall Meeting 2003, abstract #SH11A-01

Astronomy and Astrophysics

Astrophysics

7500 Solar Physics, Astrophysics, And Astronomy, 7509 Corona, 7549 Ultraviolet Emissions

Scientific paper

Coronal abundances are found to vary among different coronal structures, within streamers, and along heliocentric heights. Characterizing its variations is essential in understanding the underlying fractionation mechanisms and the coronal origin of the solar wind. We will review recent measurements in solar coronal abundance and its variations with time and among coronal structures. In particular, we will present SOHO observations of abundances in active regions with a broad range of age and activity levels. Results that compare coronal abundances with in-situ measurements will also be reviewed.

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