The Inverse Compton Effect as a Possible Cause of the X-ray Radiation of Solar Flares

Details The Inverse Compton Effect as a Possible Cause of the X-ray Radiation of Solar Flares The Inverse Compton Effect as a Possible Cause of the X-ray Radiation of Solar Flares

Apr 1964

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1964natur.202..275s&link_type=abstract

Nature, Volume 202, Issue 4929, pp. 275-276 (1964).

Computer Science

10

Scientific paper

THE X-ray radiation of the Sun in the spectral range 60 Å < λ < 0.1 Å has been investigated since 1948. A wealth of data has been obtained on the radiation of both the quiet Sun (60 > λ > 5 Å) and of solar flares (down to λ ~ 0.01 Å) (refs. 2-4). Theoretical calculations are based on the assumption that the X-ray radiation of the Sun is of thermal origin and may be caused by the recombination radiation, bremsstrahlung, and radiation in selected lines of a very hot and optically thin plasma. The most complete calculations have been made by Elwert5,6.

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