Analysis of high-temporal-resolution spectra of the 1991 Oct. 24 white-light flare.

Details Analysis of high-temporal-resolution spectra of the 1991 Oct. 24 white-light flare. Analysis of high-temporal-resolution spectra of the 1991 Oct. 24 white-light flare.

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996acaps..16..401x&link_type=abstract

Acta Astrophys. Sin., Vol. 16, No. 4, p. 401 - 407

Astronomy and Astrophysics

Astrophysics

Solar Flares: Spectra

Scientific paper

The authors analyse the spectra of a 2N/X2.1 white-light flare (WLF) by comparing the line profiles and the continuum emission with X-ray and radio data. This WLF was simultaneously observed in five wavelength-bands. The measurement indicates that this flare was a Type I WLF and the characteristics are given. They find that the theories of electron-beam bombardment, chromospheric evaporation and condensation can provide a good qualitative interpretation of the energy storage and release of this WLF.

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