The theory of spectral analysis for solar impulsive hard X-ray burst

Details The theory of spectral analysis for solar impulsive hard X-ray burst The theory of spectral analysis for solar impulsive hard X-ray burst

Sep 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979acasn..20..268z&link_type=abstract

Acta Astronomica Sinica, vol. 20, Sept. 1979, p. 268-274. In Chinese, with abstract in English.

Astronomy and Astrophysics

Astronomy

3

Particle Acceleration, Pulsed Radiation, Solar Flares, Solar X-Rays, Spectrum Analysis, X Ray Spectra, Bursts, Energetic Particles, Energy Dissipation, Energy Distribution, Kinetic Equations, Particle Energy, Reaction Kinetics

Scientific paper

In this paper a new analytical method is proposed. Using the kinetic equation and taking into account the energy losses for accelerated particles in solar flare, the time-dependent particle energy distribution is obtained. It is shown that the particle energy distribution in emission region is generally different from that in acceleration region and the deviation from power law spectrum seems to be evident. The results derived from the kinetic equation can be used to analyze the radiation spectrum of the hard pulsed X-ray bursts precisely. Finally, the softening phenomenon of the X-ray spectrum in high energy region is discussed.

Affiliated with

Also associated with

No associations

Rating

The theory of spectral analysis for solar impulsive hard X-ray burst does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The theory of spectral analysis for solar impulsive hard X-ray burst, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The theory of spectral analysis for solar impulsive hard X-ray burst will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1817385