Post-flare coronal arches observed with the SMM/XRP flat crystal spectrometer

Details Post-flare coronal arches observed with the SMM/XRP flat crystal spectrometer Post-flare coronal arches observed with the SMM/XRP flat crystal spectrometer

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987soph..114..329h&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 114, no. 2, 1987, p. 329-345. Research supported by the Lockheed Independent Research Progr

Physics

19

Coronal Loops, Solar Flares, Solar Spectra, Brightness, Chromosphere, Solar Activity, Solar Maximum Mission, Spectrometers, X Ray Spectra

Scientific paper

Postflare coronal arch observations made with the SMM Flat Crystal Spectrometer on January 20-23, 1985 are discussed. Results suggest that the arch revival following the dynamic flare of 23:50 UT on January 1 was of the type noted on November 6-8 and June 4, 1980 by the SMM Hard X-ray Imaging Spectrometer (HXIS). Activity different from that of the HXIS observations was found starting at about 23 UT on January 22, with no trigger of the revival being identified, and with the activity being restricted to the coronal regions (without any related disturbance in the chromosphere). The development of the arch enhancement in the corona was shown to be slower than is expected for a flare-associated revival.

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