Crazy Coronal Abundances

Details Crazy Coronal Abundances Crazy Coronal Abundances

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003csss...12..869l&link_type=abstract

The Future of Cool-Star Astrophysics: 12th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun (2001 July 30 - August

Astronomy and Astrophysics

Astrophysics

Chromospheres, Coronae, Activity, Magnetic Fields

Scientific paper

Closed magnetic structures in the solar corona show enhanced abundances of elements with first ionization potentials (FIP) less than 10 eV. Analyses of Chandra and XMM-Newton spectra of active stars show an inverse FIP bias in which the low FIP elements are underabundant and some high FIP elements are overabundant. We propose an explanation for both of these abundance anomalies.

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