Red Asymmetries of Optical Lines at the Impulsive Phase of Solar Flares

Details Red Asymmetries of Optical Lines at the Impulsive Phase of Solar Flares Red Asymmetries of Optical Lines at the Impulsive Phase of Solar Flares

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994kofu.symp..409s&link_type=abstract

In: Proceedings of Kofu Symposium, Kofu, Japan, Sept. 6-10, 1993, p.409-411.

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Scientific paper

Impulsive phase spectra of two chromospheric flares were obtained with
high temporal resolution. H_alpha, Ca II K, He I D_3, and other metallic
lines were observed simultaneously and their red asymmetries were
studied. Velocities derived from K and D_3 line emissions are found to
be as large as H_alpha velocity, contrary to the previous works.

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