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.
and Thampi, R.S.: 2013, Geophysical Research Letters 40(12), 2913-2917
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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.