Transition Region: First Ionization Potential Effect

Details Transition Region: First Ionization Potential Effect Transition Region: First Ionization Potential Effect

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000eaa..booke2265v&link_type=abstract

"Encyclopedia of Astronomy and Astrophysics, Edited by Paul Murdin, article 2265. Bristol: Institute of Physics Publishing, 2001

Astronomy and Astrophysics

Astrophysics

Sun, Solar Atmosphere

Scientific paper

The first ionization potential (FIP) effect causes a fractionation, i.e. a change of the relative abundances, of elements with a low FIP in the corona and solar wind as compared with the SOLAR PHOTOSPHERE. These elements (specifically Mg, Si and Fe) are becoming enriched somewhere in the solar atmosphere by an average factor of 2-5 relative to the high-FIP elements (specifically oxygen). The proc...

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