IMF inclusion adds a cyclotron frequency term to the TSI dispersion relation, changing growth rate with velocity, density and B; PIC runs show background electrons shielding solar wind electrons in vortices and some lunar electrons aligning with solar wind flow.
Daniele, and Wurz, Peter: 2009, Current Science 96(4), 526-532
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The two-stream instability generation around Moon: Effect of Interplanetary Magnetic Field during Solar Wind - Lunar Plasma Interaction
IMF inclusion adds a cyclotron frequency term to the TSI dispersion relation, changing growth rate with velocity, density and B; PIC runs show background electrons shielding solar wind electrons in vortices and some lunar electrons aligning with solar wind flow.