The significance of invariable point in the energy spectra of non-thermal electrons of solar flares.

Details The significance of invariable point in the energy spectra of non-thermal electrons of solar flares. The significance of invariable point in the energy spectra of non-thermal electrons of solar flares.

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ppmto..18..125g&link_type=abstract

Publ. Purple Mt. Obs., Vol. 18, No. 2, p. 125 - 127

Physics

Solar Flares: Electrons, Solar Flares: Energy Spectra, Solar Flares: X-Ray Spectra

Scientific paper

By using the data of GRS/SMM, it has been discovered that for some
flares, the power-law energy spectra of non-thermal electrons present a
roughly fixed crossing point. The authors believe that the "crossing
point" may be a reflection of a flux saturation at the low-energy cutoff
in the process of electron acceleration.

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