H_alpha and X-ray Signatures of Chromospheric Heating Observed in Solar Flares

Details H_alpha and X-ray Signatures of Chromospheric Heating Observed in Solar Flares H_alpha and X-ray Signatures of Chromospheric Heating Observed in Solar Flares

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994kofu.symp..195w&link_type=abstract

In: Proceedings of Kofu Symposium, Kofu, Japan, Sept. 6-10, 1993, p.195-198.

Physics

Scientific paper

We have studied the spatial and temporal relationship between thermal and non-thermal energy transport, and the chromospheric response in solar flares. H_alpha imaging spectra from Mees Solar Observatory provided the information on the heating and dynamics in the chromosphere, soft X-ray images from Yohkoh provided the conditions of the thermal plasma in the corona, and hard X-ray data from Yohkoh provided the diagnostics of the non-thermal particles. We present some preliminary results for several large flares, and discuss their implications for the chromospheric flare heating mechanism.

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