Computer Simulation Overview No.1
Computer Simulation Overview No.1
Interaction of the solar wind with the earth's magnetosphere has
been studied by using a 3-dimensional global MHD model.
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MHD Simulation of Earth's Magnetosphere
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Computer Simulation Overview No.2, Several Examples
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Computer Simulation Overview No.3: 3D magnetic field configuration
of Earth's magnetosphere when the IMF rotates.
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Computer Simulation Overview No.4: 3D magnetic field configuration
of Earth's magnetosphere in a 3 Dimensional view when the IMF rotates.
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Computer Simulation Overview No.5: 3D magnetic field configuration
of Earth's magnetosphere in a view from the sun when the IMF rotates.
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Computer Simulation Overview No.6: Projection of regions of minimum
B and V (perpendicular to B) when the IMF rotates.
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Computer Simulation Overview No.7: Cross sectional patterns on
noon-midnight and equatorial planes and at x=-40Re when the IMF
rotates.
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Computer Simulation Overview No.8: Cross sectional patterns on
noon-midnight and equatorial planes and at x=-100Re when the IMF
rotates.
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Computer Simulation Overview No.9: Integration of density and
energy along z-axis and x-axis in the magnetosphere.
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Computer Simulation Overview No.10: Integration of density and
energy along y-axis and x-axis in the magnetosphere.
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Computer Simulation Overview No.11: Matrix Table.
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