Statistics and investigation of white light solar flares

Details Statistics and investigation of white light solar flares Statistics and investigation of white light solar flares

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984acasn..25..127c&link_type=abstract

(Acta Astronomica Sinica, vol. 25, no. 2, 1984, p. 127-135) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 8, Dec. 19

Astronomy and Astrophysics

Astrophysics

1

Solar Flares, Statistical Analysis, Continuous Radiation, Convection Currents, Energetic Particles, H Alpha Line, Ionospheric Disturbances, Solar Radio Bursts, Solar X-Rays

Scientific paper

The properties of white-light flares are discussed on the basis of the published accounts of these events, together with the associated H-alpha flares, radio bursts, X-ray bursts, proton events, and ionospheric disturbances. In addition, spectral plates taken at Purple Mountain Observatory since 1962 have been examined. It is found that 5 percent of the spectrograms of solar flares show variable white-light emission. A minority of the white-light flares are associated with H-alpha flares of small importance classes, which may be caused by perturbations originating in the convective zone below; the majority, accompanied by high-energy events, are caused by the bombardment of energetic particles from above.

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