The ratio of impulsive to thermal X-ray flux as a function of solar flare position

Details The ratio of impulsive to thermal X-ray flux as a function of solar flare position The ratio of impulsive to thermal X-ray flux as a function of solar flare position

Apr 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975aero.reptq....m&link_type=abstract

Interim Report Aerospace Corp., El Segundo, CA. Lab. Operations.

Physics

Solar Flares, Solar Flux, Solar X-Rays, Bremsstrahlung, Oso-7, Photosphere, Solar Corona

Scientific paper

A study of 119 flares observed by OSO-7 shows no evident correlation
between the ratio of the maximum 20 keV impulsive flux to the maximum 5
keV thermal flux and the flare location.

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