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The Flare of 1989 September 9, 09:09 UT: Does Coronal Loop Collision Initiate Efficient Gamma-Ray Emission?
Published online by Cambridge University Press: 12 April 2016
Abstract
Vector magnetogram data and Hα pictures together with data published by Chupp et al. lead us to conjecture that in the presented case a contact between the rising two-ribbon flare current sheet and a coronal loop connecting two nearby plage regions initiates efficient high-energy γ-ray emission.
Subject headings: Sun: corona — Sun: flares — Sun: X-rays, gamma rays
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- Copyright © The American Astronomical Society 1994