Numerical modeling of the energy storage and release in solar flares

Details Numerical modeling of the energy storage and release in solar flares Numerical modeling of the energy storage and release in solar flares

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993jatp...55..939w&link_type=abstract

Journal of Atmospheric and Terrestrial Physics (ISSN 0021-9169), vol. 55, no. 7, p. 939-945.

Physics

Magnetohydrodynamic Stability, Photosphere, Solar Energy, Solar Flares, Solar Magnetic Field, Data Simulation, Energy Storage

Scientific paper

This paper reports on investigation of the photospheric magnetic field-line footpoint motion (usually referred to as shear motion) and magnetic flux emerging from below the surface in relation to energy storage in a solar flare. These causality relationships are demonstrated by using numerical magnetohydrodynamic simulations. From these results, one may conclude that the energy stored in solar flares is in the form of currents. The dynamic process through which these currents reach a critical value is discussed as well as how these currents lead to energy release, such as the explosive events of solar flares.

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