The flare of 1989 September 9, 09:09 UT: Does coronal loop collision initiate efficient gamma-ray emission

Details The flare of 1989 September 9, 09:09 UT: Does coronal loop collision initiate efficient gamma-ray emission The flare of 1989 September 9, 09:09 UT: Does coronal loop collision initiate efficient gamma-ray emission

Feb 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apjs...90..707a&link_type=abstract

Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 90, no. 2, p. 707-711

Astronomy and Astrophysics

Astrophysics

1

Coronal Loops, Gamma Ray Bursts, Particle Acceleration, Solar Flares, Current Sheets, Faculae, H Alpha Line, Magnetic Field Configurations, Magnetic Signatures, Topology

Scientific paper

Vector magnetogram data and H(alpha) 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 gamma-ray emission.

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