Numerical simulation of solar flares

Details Numerical simulation of solar flares Numerical simulation of solar flares

Nov 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996r%26qe...39..912p&link_type=abstract

Radiophysics and Quantum Electronics, Volume 39, Issue 11-12, pp. 912-915

Physics

Scientific paper

We have developed the Peresvet program for numerical simulation of
energy accumulation above active regions. This program solves 3D MHD
equations for the compressible plasma with allowance for the dissipative
terms. It is shown that the energy can be stored in a layer of current
by focusing the photospheric disturbances.

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