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Flaring Arch Structure of Large Eruptive Phenomena and Rigid Rotation
Published online by Cambridge University Press: 27 September 2017
Abstract
Considering the flaring arch to be the basic element of all flares, we study here the structure of compact flares and double ribbon flares. It is observed that, in the case of compact flares, the flaring arch diverges from a pivot point (rigid rotation), while in the case of double ribbon flares the flaring arches are distributed to either side of the polarity reversal line.
- Type
- Session II: Solar Flares
- Information
- International Astronomical Union Colloquium , Volume 104 , Issue 2: Solar and Stellar Flares , 1989 , pp. 227 - 230
- Copyright
- Copyright © Kluwer 1989