Solar Flare Peculiarities: A Hypothesis for a New Phenomenological Model

Details Solar Flare Peculiarities: A Hypothesis for a New Phenomenological Model Solar Flare Peculiarities: A Hypothesis for a New Phenomenological Model

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000cosre..38..579l&link_type=abstract

Cosmic Research, v. 38, Issue 6, p. 579-583 (2000).

Physics

Scientific paper

An intensity time-profile of the hard X-ray emission in two cores of a small impulsive solar flare is analyzed. The emission in the cores proved to evolve in the opposite phases. The phases of growth and decay are also shown to be modulated by the slower oscillatory variations. It is suggested that acceleration processes may be oscillating and a collapsing acceleration process may occur above and below the photosphere.

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