Energetic (HXR/GR) Emission from Flares: Implications for Particle Acceleration and Transport

Details Energetic (HXR/GR) Emission from Flares: Implications for Particle Acceleration and Transport Energetic (HXR/GR) Emission from Flares: Implications for Particle Acceleration and Transport

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999spro.proc..335v&link_type=abstract

Solar Physics with Radio Observations, Proceedings of the Nobeyama Symposium, held in Kiyosato, Japan, Oct. 27-30, 1998, Edited

Physics

Scientific paper

This paper reviews a selection of observations in hard X-rays (HXR) and gamma-rays (GR) that allow us to derive quantitative constraints on the energetic electrons and ions accelerated during solar flares. We shall focus on the results obtained for the relative energy contents in electrons and ions in strong gamma-ray line (GRL) eventsas well as on the chemical composition of accelerated ions. We shall discuss new estimates of the upper limit of the energy contained in ions for electron-dominated eventsand briefly summarize new results concerning the relationship found between centimetric-millimetric emitting electrons and HXR/GR bremsstrahlung emitting ones.

Affiliated with

Also associated with

No associations

Rating

Energetic (HXR/GR) Emission from Flares: Implications for Particle Acceleration and Transport 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 Energetic (HXR/GR) Emission from Flares: Implications for Particle Acceleration and Transport, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Energetic (HXR/GR) Emission from Flares: Implications for Particle Acceleration and Transport will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1062333