Temperature structure of spatially resolved hard X-ray flares

Details Temperature structure of spatially resolved hard X-ray flares Temperature structure of spatially resolved hard X-ray flares

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983soph...86..289s&link_type=abstract

(Japan Society for the Promotion of Science and National Science Foundation, U.S.-Japan Seminar on the Recent Advances in the Un

Astronomy and Astrophysics

Astronomy

13

Plasma Temperature, Solar Flares, Solar X-Rays, X Ray Astronomy, Chromosphere, Coronal Loops, Energy Sources, High Resolution, Solar Maximum Mission

Scientific paper

High resolution X-ray images are used to study the temperature structure and evolution of two spatially resolved, but compact, solar flares. Both flares developed within a magnetic loop whose footpoints were separated by typically 15000 km, and involved primary energy release at one footpoint. This was followed by transfer of chromospheric material into and around the loop. The flares involved total energies differing by over an order of magnitude, and they follow different evolutionary paths because of this.

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