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Solar Flares and Related Coronal Magnetic Field Structures in NOAA 8100

Published online by Cambridge University Press:  13 May 2016

Y. Yan
Y. Yan*
Affiliation:
Beijing Astronomical Observatory/National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China

Abstract

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In this paper we describe the available methods for the non-constant-α force-free field reconstruction and study the associations between reconstructed 3-d coronal fields by a new technique and the 2B/X2 flare process from observations in AR 8100 on 4 November 1997.

Type
Session III: Active Region Structure and Dynamics
Information
Symposium - International Astronomical Union , Volume 203: Recent Insights into the Physics of the Sun and Heliosphere: Highlights from Soho and Other Space Missions , 2001 , pp. 341 - 343
Copyright
Copyright © Astronomical Society of the Pacific 2001 

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