Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apjs...73..253c&link_type=abstract
(NASA and University of New Hampshire, Workshop on Impulsive Solar Flares, 2nd, Durham, NH, Sept. 26-28, 1988) Astrophysical Jou
Astronomy and Astrophysics
Astrophysics
13
Energetic Particles, Particle Acceleration, Solar Flares, Gamma Ray Spectra, H Alpha Line, Solar X-Rays, Type 3 Bursts, Type 4 Bursts
Scientific paper
The impulsive mode of particle acceleration is studied by searching for 0.2-2 MeV electron increases associated with intense type III/V bursts. It is found that the presence of a type III/V burst in association with a relatively intense flare event indicates the acceleration and escape of greater than 100 KeV electrons. A list of type III/V electron events is compiled, showing that the majority included greater than 10 MeV proton increases, although they were not followed by a type II burst. The results suggest that there are two different modes of proton acceleration with the second mode becoming significant only for larger, gradual flares.
Cane Hilary V.
Reames Donald. V.
No associations
LandOfFree
The relationship between energetic particles and flare properties for impulsive 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 The relationship between energetic particles and flare properties for impulsive solar flares, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The relationship between energetic particles and flare properties for impulsive solar flares will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-982409