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FIP Effect and FIP-Dependent Bias in the Solar Corona

Published online by Cambridge University Press:  26 May 2016

B.N. Dwivedi ,
A. Mohan  and
E. Landi
B.N. Dwivedi
Affiliation:
Department of Applied Physics, Institute of Technology, Banaras Hindu University, Varanasi-221 005, India
A. Mohan
Affiliation:
Department of Applied Physics, Institute of Technology, Banaras Hindu University, Varanasi-221 005, India
E. Landi
Affiliation:
Artep, Inc. at Naval Research Laboratory, Washington, DC 20375, USA

Abstract

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Using EUV spectra of an active region observed off the solar disk by the SOHO/SUMER 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.

Information

Type
Part 9: Heating of Solar and Stellar Coronae
Information
Symposium - International Astronomical Union , Volume 219: Stars as Suns : Activity, Evolution and Planets , 2004 , pp. 493 - 497
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

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