Numerical Boundary Conditions for Solar Magnetic Hydrodynamic Flows Using the Method of Characteristics

Details Numerical Boundary Conditions for Solar Magnetic Hydrodynamic Flows Using the Method of Characteristics Numerical Boundary Conditions for Solar Magnetic Hydrodynamic Flows Using the Method of Characteristics

Mar 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ap%26ss.243..149w&link_type=abstract

Solar and Interplanetary Transients, proceedings of IAU Colloquium 154, held in Pune, India, January 23-27, 1995. ASTROPHYSICS A

Astronomy and Astrophysics

Astrophysics

7

Mhd Simulation, Mhd Characteristics, Corona

Scientific paper

We discuss the self-consistent time-dependent numerical boundary conditions on the basis of theory of characteristics for magnetohydrodynamics (MHD) simulations of solar plasma flows. The importance of using self-consistent boundary conditions is demonstrated by using an example of modeling coronal dynamic structures. This example demonstrates that the self-consistent boundary conditions assure the correctness of the numerical solutions. Otherwise, erroneous numerical solutions will appear.

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