Hard X-ray emission processes in solar flares

Details Hard X-ray emission processes in solar flares Hard X-ray emission processes in solar flares

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987soph..111..207v&link_type=abstract

(Observatoire de Paris, CNRS, CNES, et al., CESRA Workshop on Particle Acceleration and Trapping in Solar Flares, 2nd, Aubigny-s

Physics

29

Energetic Particles, Solar Flares, Solar X-Rays, X Ray Spectra, Bremsstrahlung, Elementary Particle Interactions, Polarized Electromagnetic Radiation, Temporal Distribution

Scientific paper

Solar hard X-ray emission is one of the most direct diagnostics of accelerated particles during solar flares. In this review, the current understanding of hard X-ray emission processes is discussed: first the different emission mechanisms (in particular inverse Compton radiation, energetic ion or electron bremsstrahlung) are presented and the plausibility of each of these mechanisms is discussed. Then, different types of hard X-ray models (thermal or non-thermal, homogeneous or inhomogeneous emission regions) are presented together with the comparison of their predictions with X-ray observations (spectral, spatial and temporal informations - directivity and polarization).

Affiliated with

Also associated with

No associations

Rating

Hard X-ray emission processes in solar flares 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 Hard X-ray emission processes in solar flares, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Hard X-ray emission processes in solar flares will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1599989