Coronal explosions as a signature of current loop coalescence in solar flares

Details Coronal explosions as a signature of current loop coalescence in solar flares Coronal explosions as a signature of current loop coalescence in solar flares

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989soph..123..393s&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 123, no. 2, 1989, p. 393-396.

Physics

13

Coalescing, Coronal Loops, Solar Flares, Chromosphere, Magnetohydrodynamic Flow, Plasma Jets, Solar X-Rays, Type 2 Bursts

Scientific paper

The coronal explosions interpreted by De Jaeger and Boelee (1984) as masnifestations of plasma streaming out of flare kernels are presently reinterpreted as signatures of current loop coalescence in the flaring region. This interpretation can quantitatively explain the various characteristics of the observed coronal explosions. The present model is expected to be very directly addressed by the soft X-ray imaging instrument that will be carried by the Solar-A mission spacecraft due for launch during the next solar maximum.

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