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The Formation and Evolution of a Ring-filament Associated with Newly-emerging Flux

Published online by Cambridge University Press:  01 November 2006

Suli Ma ,
Yunchun Jiang  and
Huadong Chen
Suli Ma
Affiliation:
National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011, China email: msli@ynao.ac.cn
Yunchun Jiang
Affiliation:
National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011, China email: msli@ynao.ac.cn
Huadong Chen
Affiliation:
National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011, China email: msli@ynao.ac.cn
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Abstract

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Using the data from BBSO, YNAO and SOHO/MDI we studied the formation and evolution of a ring-filament which was located in NOAA AR09470 from May 21 to 24, 2001. We found that: (1) the ring-filament's formation was well associated with newly-emerging flux. (2) all the eruptions of the filament happened during the decay of the emerging bipoles.

Keywords

Sun: ring-filamentmagnetic fluxactivity
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S233: Solar Activity and its Magnetic Origin , March 2006 , pp. 411 - 412
Copyright
© 2006 International Astronomical Union