Doppler shifts of metallic lines for a white-light flare

Details Doppler shifts of metallic lines for a white-light flare Doppler shifts of metallic lines for a white-light flare

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994soph..149..143d&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 149, no. 1, p. 143-148

Astronomy and Astrophysics

Astronomy

9

Asymmetry, Calcium, Doppler Effect, Emission Spectra, K Lines, Metal Ions, Solar Flares, Solar Radio Emission, Coronagraphs, Photosphere, Radio Astronomy, Spectrograms

Scientific paper

In this paper we investigated the Doppler shifts of the metallic lines
for a 3B white-light flare on September 19, 1979. The results show that
there is no systematic shift at the line center, while there may appear
some asymmetry at the line wing. A possible heating process of this
flare is proposed to interpret the observed spectral features.

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