FIP Effect Measurements in the Solar Corona and in Flares

Details FIP Effect Measurements in the Solar Corona and in Flares FIP Effect Measurements in the Solar Corona and in Flares

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agusm..sh52c04f&link_type=abstract

American Geophysical Union, Spring Meeting 2001, abstract #SH52C-04 INVITED

Astronomy and Astrophysics

Astrophysics

7500 Solar Physics, Astrophysics, And Astronomy, 7509 Corona, 7519 Flares

Scientific paper

The compositions of solar upper atmosphere plasmas were studied from spectra obtained by instruments aboard all major solar observatories that were launched into space in the last three decades. During my talk I will review FIP effect results that were obtained from instruments on some of the observatories as they relate to coronal holes, quiet regions, active regions and flares. I will shaw that although the derived compositions vary considerably with the type of plasma observed some regularities in their behavior begin to emerge.

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