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Three Dimensional image Reconstruction of an Hα Flare

Published online by Cambridge University Press:  13 May 2016

Z. Q. Qu ,
Y. C. Jiang ,
T. Luan  and
Z. Xu
Z. Q. Qu
Affiliation:
Yunnan Astronomical Observatory, Chinese Academy of Sciences, Kunming 650011, China National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
Y. C. Jiang
Affiliation:
Yunnan Astronomical Observatory, Chinese Academy of Sciences, Kunming 650011, China National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
T. Luan
Affiliation:
Yunnan Astronomical Observatory, Chinese Academy of Sciences, Kunming 650011, China National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
Z. Xu
Affiliation:
Yunnan Astronomical Observatory, Chinese Academy of Sciences, Kunming 650011, China National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China

Abstract

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The three-dimensional (3D) image of an Hα flare is reconstructed from its line-center and seriary off-center filtergrams. The reconstruction is based on the principle of the line formation theory that the contribution function (CF) of emergent specific line intensity describes the escape photon distribution from stellar atmospheric layers. Thus the reconstruction depends on the model atmosphere accepted which determines the CF. An Hα flare taking place on April 22, 1992 is utilized to illustrate the process.

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. 303 - 306
Copyright
Copyright © Astronomical Society of the Pacific 2001 

References

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