Basic Principles and Examples of Solar-type Flare Modelling

Details Basic Principles and Examples of Solar-type Flare Modelling Basic Principles and Examples of Solar-type Flare Modelling

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aspc..289..393s&link_type=abstract

The Proceedings of the IAU 8th Asian-Pacific Regional Meeting, Volume I, held 2-5 July 2002 at National Center of Sciences, Hito

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Scientific paper

We review the fundamental ideas which are under current use to model flares and other non-stationary phenomena in the solar atmosphere. Recent multi-wavelength observations of solar flares allow us to improve a theory of solar-type flares, which can be applied to many astrophysical phenomena accompanied by fast plasma ejection, powerful fluxes of radiation, and the acceleration of electrons and ions to high energies.

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