Computer Science
Scientific paper
Sep 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..528..119r&link_type=abstract
ACCELERATION AND TRANSPORT OF ENERGETIC PARTICLES OBSERVED IN THE HELIOSPHERE: ACE 2000 Symposium. AIP Conference Proceedings, V
Computer Science
Particle Acceleration
Scientific paper
We briefly review the gamma-ray data of the 1991 June 1 flare and the analysis which provide evidence that the accelerated ion composition is that observed from impulsive flares and that the heavy ion enrichment, characteristic of impulsive flares, increased during the course of the flare as the gamma-ray fluxes decreased. We propose that this anti correlation is due to acceleration by cascading Alfvén turbulence. We also show that a large behind-the-limb flare, such as the June 1 event, could produce detectable gamma-ray line emission as the radioactive patch which it creates rotates onto the visible solar disk. .
Lenters Geoffrey
Mandzhavidze Natalie
Miller Aaron J.
Ramaty Reuven
No associations
LandOfFree
Gamma-ray evidence for time-dependent heavy ion enhancement in a solar flare 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 Gamma-ray evidence for time-dependent heavy ion enhancement in a solar flare, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gamma-ray evidence for time-dependent heavy ion enhancement in a solar flare will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1523573