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Structures of Chromospheric Magnetic Fields in Active Regions

Published online by Cambridge University Press:  12 April 2016

Hongqi Zhang
Affiliation:
Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing 100080, China
Guoxiang Ai
Affiliation:
Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing 100080, China
Wei Li
Affiliation:
Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing 100080, China
Jimin Chen
Affiliation:
Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing 100080, China

Abstract

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In this paper, we study the distribution of chromospheric magnetic fields and analyze reversed polarity structures on chromospheric magnetograms in active regions.

Type
Session 5. Fields in the Chromosphere and Corona
Copyright
Copyright © Astronomical Society of the Pacific 1993

References

Chen, J., Ai, G., Zhang, H., and Jiang, S. 1989, Suppl. Publ. Yunnan Obser., 108CrossRefGoogle Scholar
Li, W. 1992, personal communicationGoogle Scholar
Livingston, W.C. 1973, World Data Center A for Solar-Terrestrial Physics Report Collected Data Report on August 1972 Solar-Terrestrial Events, ed. Coffey, H.E., 95 Google Scholar
Stenflo, J.O., Harvey, J.W., Brault, J.W., Solanki, S.K. 1984, A&A, 131, 333 Google Scholar
Wang, J. and Shi, Z. 1992, Acta Astronomica Sinica, 33, 95 Google Scholar
Zhang, H. 1991, presented at The First China-Japan Seminar on Solar Physics Workshop, Kunming, China.Google Scholar
Zhang, H., Ai, G., Sakurai, T., and Kurokawa, H. 1991, Solar Phys., 136, 269 CrossRefGoogle Scholar