Second-stage acceleration in solar flares

Details Second-stage acceleration in solar flares Second-stage acceleration in solar flares

Oct 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976a%26a....52..305m&link_type=abstract

Astronomy and Astrophysics, vol. 52, no. 2, Oct. 1976, p. 305, 306.

Astronomy and Astrophysics

Astrophysics

8

Solar Cosmic Rays, Solar Flares, Stellar Models, Supernova Remnants, Astronomical Models, Particle Acceleration, Shock Waves, Solar Protons

Scientific paper

A model proposed by Chevalier and Scott (1975) to account for cosmic-ray
acceleration in an expanding supernova remnant is applied to the case of
a shock wave injected into the solar corona by a flare. Certain features
of solar cosmic rays can be explained by this model

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