Nonideal phenomena in the solar plasma. Application of the theory of Coulomb fluids to stellar plasmas

2001 ◽  
Vol 93 (1-3) ◽  
pp. 229-233
Author(s):  
C.-V. Meister
Keyword(s):  
Solar Plasma ◽  
Coulomb Fluids

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

1996 ◽  
Vol 154 ◽  
pp. 149-153
Author(s):  
S. T. Wu ◽  
A. H. Wang ◽  
W. P. Guo
Keyword(s):  
Boundary Conditions ◽  
Method Of Characteristics ◽  
Numerical Solutions ◽  
The Self ◽  
Time Dependent ◽  
Solar Plasma ◽  
The Method Of Characteristics ◽  
Mhd Simulations ◽  
Self Consistent ◽  
Dynamic Structures

AbstractWe 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.

Hydrodynamic Instabilities in Coulomb Fluids

1977 ◽  
Vol 38 (11) ◽  
pp. 599-602
Author(s):  
B. A. Huberman ◽  
W. Streifer
Keyword(s):  
Hydrodynamic Instabilities ◽  
Coulomb Fluids
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