A Clarification on the invariable point in the power-law energy spectra of non-thermal electrons of solar flares

Details A Clarification on the invariable point in the power-law energy spectra of non-thermal electrons of solar flares A Clarification on the invariable point in the power-law energy spectra of non-thermal electrons of solar flares

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ap%26ss.288..451g&link_type=abstract

Astrophysics and Space Science, v. 288, Issue 4, p. 451-455 (2003).

Astronomy and Astrophysics

Astrophysics

Scientific paper

The invariable point of non-thermal electrons was proposed two years ago, based on analyzing the two intense gamma-ray line flares observed with the X2 detector on GRS/SMM. Due to too strong hard X-ray flux in those two flares, the influence of pile-up effect might not be fully excluded. In this paper, we check the invariable point by using some medium hard X-ray events observed with HXRBS/SMM and BATSE/CGRO. It is found that the invariable point could indeed appear in some weaker hard X-ray events, in which the pile-up effect cannot play a role. Further refinement should be based on the observations with a high energy resolution.

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