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• W1978686234 abstract "Disk‐shaped current distributions are useful tools in modeling the magnetospheres of Earth and other planets and have also been adapted for modeling the geotail. Such models usually start with an axisymmetric vector potential but may be modified to account for observed asymmetries, variable thickness, and warping in response to an inclined orientation of the planetary dipole axis. Models of this type until now either have lacked the ability to simulate a sharp inner edge of the current and to control accurately its falloff with distance or did not allow a simple analytical representation. Here existing methods will be reviewed, after which a new class of models which overcomes the above deficiencies and also allows the modeling of current disks of finite thickness flanked by current‐free regions will be presented." @default.
• W1978686234 created "2016-06-24" @default.
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• W1978686234 date "1994-01-01" @default.
• W1978686234 modified "2023-10-16" @default.
• W1978686234 title "Analytical models of the magnetic field of disk‐shaped current sheets" @default.
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• W1978686234 doi "https://doi.org/10.1029/93ja02768" @default.
• W1978686234 hasPublicationYear "1994" @default.
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