Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990esasp.311....7s&link_type=abstract
In ESA, Plasma Astrophysics p 7-12 (SEE N91-15046 06-90)
Astronomy and Astrophysics
Astrophysics
Electrons, Implosions, Particle Acceleration, Protons, Solar Flares, Coalescing, Mathematical Models, Neutral Currents, Three Dimensional Models
Scientific paper
A model for high energy solar flares is presented to explain prompt proton and electron acceleration within one second to relativistic energies. It is shown that both protons and electrons can be promptly (within than one second) accelerated to approximately 100 GeV and approximately 100 MeV, respectively during the implosion driven by a three dimensional X-type current loop coalescence. The fact that a well developed high energy flare has three phases of particle acceleration is accentuated. The present acceleration mechanism can explain the first phase.
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