Physics
Scientific paper
May 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agusmsp42a..01s&link_type=abstract
American Geophysical Union, Spring Meeting 2005, abstract #SP42A-01
Physics
7514 Energetic Particles (2114), 7519 Flares, 7554 X Rays, Gamma Rays, And Neutrinos
Scientific paper
The Reuven Ramaty High-Energy Solar Spectroscopic Imager (RHESSI) has detected nuclear gamma-ray line emission from at least eleven solar flares over the past three years. These gamma-ray lines are produced when flare-accelerated ions collide with the ambient solar medium. In this paper, we concentrate on the energy content and time profiles of accelerated ions and electrons. Ion spectral information is derived from suitable line ratios. We also compare the fluxes and timing of gamma-ray emission and high-energy electron bremsstrahlung emission. Finally, for the larger flares, we investigate the temporal variability of the nuclear de-excitation lines as well.
Lin Robert P.
Murphy Ronald J.
Schwartz Richard A.
Share Gerald H.
Shih Albert Y.
No associations
LandOfFree
Energetics and Temporal Variability in RHESSI Gamma-Ray 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 Energetics and Temporal Variability in RHESSI Gamma-Ray Flares, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Energetics and Temporal Variability in RHESSI Gamma-Ray Flares will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1699242