Computer Simulation Overview No.9
Rotation of Interplanetary Magnetic Field
3D Magnetic Field Configuration of Magnetosphere
Integration of Density and Energy in Magnetosphere
Interaction of the solar wind with the earth's magnetosphere has
been studied by using a 3-dimensional global MHD model.
Rotation of IMF in the north-south and dawn-dusk plane with a
period of 6 hours, where B=5nT.
Counterclockwise rotation of IMF starting from the quasi-steady
magnetospheric configuration for northward IMF.
- t=390m, theta= 90degrees
- t=600m, theta=300degrees
- t=615m, theta=315degrees
- t=630m, theta=330degrees
- t=645m, theta=345degrees
- t=660m, theta= 0degrees
- t=675m, theta= 15degrees
- t=690m, theta= 30degrees
- t=705m, theta= 45degrees
- t=720m, theta= 60degrees
- t=735m, theta= 75degrees
- t=750m, theta= 90degrees
- t=765m, theta=105degrees
Counterclockwise rotation of IMF starting from the quasi-steady
magnetospheric configuration for southward IMF.
- t=390m, theta=270degrees
- t=600m, theta=120degrees
- t=615m, theta=135degrees
- t=630m, theta=150degrees
- t=645m, theta=165degrees
- t=660m, theta=180degrees
- t=675m, theta=195degrees
- t=690m, theta=210degrees
- t=705m, theta=225degrees
- t=709m, theta=240degrees
- t=712m, theta=240degrees
- t=716m, theta=240degrees
- t=720m, theta=240degrees
- t=735m, theta=255degrees
- t=750m, theta=270degrees
- t=765m, theta=285degrees
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