Converging motions of solar flare ribbons

Details Converging motions of solar flare ribbons Converging motions of solar flare ribbons

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agusmsp23b..03j&link_type=abstract

American Geophysical Union, Spring Meeting 2005, abstract #SP23B-03

Other

7524 Magnetic Fields

Scientific paper

We present a number of examples of solar flares, in which conjugate
ribbons move toward each other during the impulsive phase. Meanwhile,
HXR coronal sources move down. Normal separation motions occur only
after the impulsive phase. This phenomena may pose a new topic to flare
reconnection theory.

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