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- W2330487633 abstract "Using a 3-D hybrid pa rticle-in-cell (PIC) model we have presented h ere the interaction o f a plasma stream with an inflated magnetic bubble. When h igh-density thermal plasma is injected into a dipole magnetic field, the plasma gets trapped in the closed magnetic field lines. When the plasma pressures exceeds the local magnetic pressure, the expanding plasma inflates the magnetic field forming a magnetic bubble. Plasma stream resembling solar wind interacts with the magnetic bubble thereby forming a bow-shock structure at t he interaction zone. Plasma stream particles are accumulated at the interaction zone and some of them are reflected also. Eventually, the magnetic inflation comes to a halt and a standoff shock is formed. The original dipole magnetic field, which falls as 3 R , is inflated to the extent that it falls as 1 R ." @default.
- W2330487633 created "2016-06-24" @default.
- W2330487633 creator A5058607685 @default.
- W2330487633 creator A5084384156 @default.
- W2330487633 date "2003-06-26" @default.
- W2330487633 modified "2023-09-27" @default.
- W2330487633 title "Simulation of Mini-Magnetospheric Plasma Propulsion (M2P2)" @default.
- W2330487633 cites W1982430569 @default.
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- W2330487633 doi "https://doi.org/10.2514/6.2003-4886" @default.
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