FIP Effect and FIP-Dependent Bias in the Solar Corona

Details FIP Effect and FIP-Dependent Bias in the Solar Corona FIP Effect and FIP-Dependent Bias in the Solar Corona

Jan 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004iaus..219..493d&link_type=abstract

Stars as suns : activity, evolution and planets, Proceedings of the 219th symposium of the International Astronomical Union held

Astronomy and Astrophysics

Astronomy

Scientific paper

Using EUV spectra of an active region observed off the solar disk by SUMER (Solar Ultraviolet Measurements of Emitted Radiation) spectrograph on the SOHO spacecraft we investigate the dependence of the FIP effect on the height above the photosphere and its relation to plasma magnetic structures present in the field of view. We also investigate the possibility of the FIP bias in the low-FIP elements to be FIP-dependent so that different abundance anomalies must be found even within the low-FIP class of elements which can provide important constraints on the FIP effect models.

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