Energy build-up, transport, and release in solar flares

Details Energy build-up, transport, and release in solar flares Energy build-up, transport, and release in solar flares

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992esasp.344...73s&link_type=abstract

In ESA, Solar Physics and Astrophysics at Interferometric Resolution p 73-80 (SEE N93-10901 01-90)

Astronomy and Astrophysics

Astrophysics

Energy Transfer, Solar Flares, Solar Protons, Ionization, Solar Corona, Solar Electrons, Solar Wind

Scientific paper

With the advent of the new observatories, it is becoming more evident that the solar flare is a more global phenomenon than previously thought. It is only the high temperature/high density manifestations that are confined to a small part of an active region. The overall question of the energy buildup, transport, and release is examined from a global perspective. The case of transporting the flare energy via energetic charged particles is discussed. Out of the two possibilities, protons or electrons, it is found that the protons give the more satisfactory account for the observations.

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