First CCD Observations of a Flare in H_epsilon and Ca-II(H)

Details First CCD Observations of a Flare in H_epsilon and Ca-II(H) First CCD Observations of a Flare in H_epsilon and Ca-II(H)

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994kofu.symp..309r&link_type=abstract

In: Proceedings of Kofu Symposium, Kofu, Japan, Sept. 6-10, 1993, p.309-312.

Physics

Scientific paper

The dynamic evolution of the chromospheric electron density during solar flares is fundamental for the testing of solar flare models. For this purpose we built an imaging spectrograph to observe optically thin Balmerlines below 400 nm with a time resolution of 1 s. On January 5, 1992 we observed a M1 / 1N flare in H_alpha, H_epsilon and Ca-II(H) and determined the temporal evolution of the electron density.

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