The white-light flare of 1982 June 15 - Observations

Details The white-light flare of 1982 June 15 - Observations The white-light flare of 1982 June 15 - Observations

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apjs...74..609m&link_type=abstract

Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 74, Oct. 1990, p. 609-646.

Other

18

Solar Flares, Solar Radiation, Solar Spectra, Atomic Spectra, Chromosphere, Emission Spectra, H Lines, Photosphere

Scientific paper

This paper presents spectral observations of the continuum as well as the profiles of 29 selected atomic lines for the two continuum-emitting kernels of the June 15 1982 white-light flare, and for the neighboring quiet sun. It is found that one of the kernels does not show enhanced emission in chromospheric lines, particularly in H-alpha, although it presents the same level of white-light emission as the other kernel. This suggests that both kernels have the same thermal structure in the continuum-emitting region, but a different structure in the chromosphere, thus supporting the hypothesis that the continuum emission is of photospheric origin, and due to H(-).

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