A relation between Balmer and soft X-ray emission in flares

Details A relation between Balmer and soft X-ray emission in flares A relation between Balmer and soft X-ray emission in flares

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...219..317h&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 219, no. 1-2, July 1989, p. 317-319. Research supported by the Lockheed Indepe

Astronomy and Astrophysics

Astrophysics

4

Balmer Series, Solar Flares, Solar X-Rays, Stellar Flares, Goes Satellites, H Alpha Line, Solar Maximum Mission

Scientific paper

Data are presented on 370 solar flares simultaneously observed and
classified in H-alpha and in the GOES (1-8 A) soft X-ray band. SMM
observations corroborate the association of the GOES and the H-alpha
events in all cases. These flares are used to examine the correlation
proposed recently by Butler, Rodono and Foing (1988).

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