Line intensities of chromospheric and photospheric spectra of a flare

Details Line intensities of chromospheric and photospheric spectra of a flare Line intensities of chromospheric and photospheric spectra of a flare

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.506..557b&link_type=abstract

In: Solar variability: from core to outer frontiers. The 10th European Solar Physics Meeting, 9 - 14 September 2002, Prague, Cze

Physics

1

Solar Spectral Lines, Photosphere, Chromosphere, Flare

Scientific paper

In this work we present the intensities of spectral lines determined from the time series of high resolution spectra obtained during the relaxing phase of subflare. The spectra were taken in the core of chromospheric Ca II K line and in two photospheric Fe I 522.5 nm and Fe I 557.6 nm lines. It is shown, that the energy of the flaring chromosphere slightly affects the underlying photospheric layers by heating a small area right under the core of the subflare.

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