Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

First-order fermi acceleration in solar flares as a mechanism for the second-step acceleration of prompt protons and relativistic electrons

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/160881· OSTI ID:5915344
We find that for two of the hard X-ray bursts of an energetic flare on 1980 June 27, the time profile of the hard X-rays above 235 keV is delayed by 3 s with respect to the time profiles of the lower energy X-rays and that the high energy spectrum becomes flatter with time during each of these bursts. From these findings we argue that during this flare a second-step mechanism accelerated further some of the high-energy tail population of the first-step electrons. By noticing that all of the flares with second-step delays produced interplanetary energetic protons, and that gamma-ray lines were detected from all of these flares except one that was not observed by any gamma-ray detector, we conclude that the second-step mechanism accelerates not only (mildly) relativistic electrons but also protons and heavy nuclei. Small delays of the nuclear gamma-ray time profiles with respect to the hard X-ray time profiles observed by SMM from the 1980 June 7 and 21 flares are consistent with this conclusion. After estimating the acceleration rate, we conclude that first-order Fermi acceleration operating in a closed flare loop is a very likely mechanism for the second-step acceleration.
Research Organization:
Center for Astrophysics and Space Sciences, University of California, San Diego
OSTI ID:
5915344
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 267:1; ISSN ASJOA
Country of Publication:
United States
Language:
English