Development of shoulders and plumes in the frame of the interchange instability mechanism for plasmapause formation

Physics

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Magnetospheric Physics: Magnetosphere-Inner, Magnetospheric Physics: Plasma Convection, Magnetospheric Physics: Numerical Modeling, Magnetospheric Physics: Plasmasphere, Magnetospheric Physics: Storms And Substorms

Scientific paper

The mechanism of plasmapause formation based on interchange instability and a Kp-dependent magnetospheric electric field model, enables us to determine the position of the plasmapause as a function of Kp and local time. We illustrate here how this physical mechanism is able to account for the formation of shoulders like those observed by EUV on IMAGE. A wide variety of other structures observed by IMAGE like tails (also called plumes), and notches are also obtained with this mechanism for the formation of a ``knee'' in the high altitude cross-L distribution of the cold plasma density distribution.

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