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mhd characteristics

International Astronomical Union Colloquium (1)

International Astronomical Union (1)

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Numerical Boundary Conditions for Solar Magnetic Hydrodynamic Flows Using the Method of Characteristics
S. T. Wu, A. H. Wang, W. P. Guo
Journal:

International Astronomical Union Colloquium / Volume 154 / 1996

Published online by Cambridge University Press:

12 April 2016, pp. 149-153

Print publication:

1996
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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.