Magnetohydrodynamic simulations of dynamic phenomena in the solar atmosphere

Details Magnetohydrodynamic simulations of dynamic phenomena in the solar atmosphere Magnetohydrodynamic simulations of dynamic phenomena in the solar atmosphere

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003asthe..96..530y&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 96, No. 10, p. 530 - 533 (2003)

Physics

1

Solar Atmosphere, Magnetohydrodynamics

Scientific paper

The magnetic field is the energy source of solar atmospheric activities.
The interaction between the magnetic fields and the ionized plasma cause
various dynamic phenomena such as explosions, brightenings, bulk motions
and so on. Several topics are picked up from recent studies by MHD
simulations in the solar physics.

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