On the Total Emissivity in Chromospheric Lines in the 17th May 2002 Flare

Details On the Total Emissivity in Chromospheric Lines in the 17th May 2002 Flare On the Total Emissivity in Chromospheric Lines in the 17th May 2002 Flare

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008espm...12.2.63p&link_type=abstract

"12th European Solar Physics Meeting, Freiburg, Germany, held September, 8-12, 2008. Online at http://espm.kis.uni-freiburg.de/,

Physics

Scientific paper

Energy balance in the 17th May 2002 flare was studied. Chromospheric lines observed by the Ondrejov spectrograph were analysed taking into account the HXR data from RHESSI. Positions of the HXR sources were identified at the H-alpha slit-jaw images and the corresponding flare spectra were processed. Total emissivity in H-alpha and H-beta lines was derived and the net energy emitted in these lines during various phases of the flare was estimated. The results were compared with evolution of HXR flux and plasma parameters obtained from the HXR spectra.

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