Magnetohydrodynamics of solar coronal plasmas in cylindrical geometry.

Details Magnetohydrodynamics of solar coronal plasmas in cylindrical geometry. Magnetohydrodynamics of solar coronal plasmas in cylindrical geometry.

Feb 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998jcoph.140..172l&link_type=abstract

Journal of Computational Physics, Vol. 140, No. 1, p. 172 - 201

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Solar Corona: Plasma, Solar Corona: Magnetohydrodynamics

Scientific paper

The authors describe a three-dimensional algorithm for the advancement
of the resistive MHD equations in cylindrical geometry with line-tied
boundary conditions. This code has been developed to simulate the
behavior of solar coronal plasmas.

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