Hostname: page-component-586b7cd67f-l7hp2 Total loading time: 0 Render date: 2024-11-27T04:52:15.545Z Has data issue: false hasContentIssue false
  • English
  • Français

Pre-Eruption Disturbance of an Active Filament

Published online by Cambridge University Press:  12 April 2016

Jingxiu Wang  and
Zhongxian Shi
Jingxiu Wang
Affiliation:
Beijing Astronomical Observatory, Chinese Academy of Sciences
Zhongxian Shi
Affiliation:
Beijing Astronomical Observatory, Chinese Academy of Sciences

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

A pre-eruption disturbance of an active filament has been observed. The disturbance is characterized by untwisting rotation and vigorous upward motion. It starts at the site where microflares took place, and appears in the late phase of magnetic flux cancellation beneath the central part of the filament, when more than 1020 Mx flux had disappeared.

Type
Session 6. Flares and Transients
Information
International Astronomical Union Colloquium , Volume 141: The Magnetic and Velocity Fields of Solar Active Regions , 1993 , pp. 397 - 400
Copyright
Copyright © Astronomical Society of the Pacific 1993

References

Schmieder, B., Raadu, M.A., and Malherbe, J.M. 1985, A &A, 142, 249.Google Scholar
Schmieder, B. 1991, A & A (preprint)Google Scholar