MAGNETOHYDRODYNAMIC MODELING OF SOLAR SYSTEM PROCESSES ON GEODESIC GRIDS
- Department of Physics, University of Alabama, Huntsville, AL 35899 (United States)
- Center for Space Plasma and Aeronomic Research, University of Alabama, Huntsville, AL 35899 (United States)
- Department of Physics, University of Notre Dame, Notre Dame, IN 46556 (United States)
This report describes a new magnetohydrodynamic numerical model based on a hexagonal spherical geodesic grid. The model is designed to simulate astrophysical flows of partially ionized plasmas around a central compact object, such as a star or a planet with a magnetic field. The geodesic grid, produced by a recursive subdivision of a base platonic solid (an icosahedron), is free from control volume singularities inherent in spherical polar grids. Multiple populations of plasma and neutral particles, coupled via charge-exchange interactions, can be simulated simultaneously with this model. Our numerical scheme uses piecewise linear reconstruction on a surface of a sphere in a local two-dimensional 'Cartesian' frame. The code employs Haarten-Lax-van-Leer-type approximate Riemann solvers and includes facilities to control the divergence of the magnetic field and maintain pressure positivity. Several test solutions are discussed, including a problem of an interaction between the solar wind and the local interstellar medium, and a simulation of Earth's magnetosphere.
- OSTI ID:
- 22156556
- Journal Information:
- Astrophysical Journal, Supplement Series, Vol. 205, Issue 2; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 0067-0049
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
COSMOLOGY AND ASTRONOMY
ASTROPHYSICS
CHARGE-EXCHANGE INTERACTIONS
COMPUTERIZED SIMULATION
EARTH MAGNETOSPHERE
GEODESICS
GRIDS
MAGNETIC FIELDS
MAGNETOHYDRODYNAMICS
NEUTRAL PARTICLES
PLANETS
PLASMA
SATELLITES
SOLAR SYSTEM
SOLAR WIND
SPHERICAL CONFIGURATION
STARS
TWO-DIMENSIONAL CALCULATIONS