Dynamics of a supersonic plume moving along a magnetized plasma.
A particle-in-cell code is used to investigate the evolution of a density plume moving through a background plasma with supersonic speed directed along the confinement magnetic field. For scale lengths representative of laboratory and auroral phenomena, the major nonlinear effects identified by the present simulations are the formation of a bipolar current system from the ballistic electrons, the appearance of transient potential layers, and the carving of deep density cavities. A 3D magnetic topology is generated by the self-consistent ballistic and diamagnetic currents that accompany highly localized potential layers.
Tsung
F S
FS
Department of Physics and Astronomy, University of California-Los Angeles, 90095, USA.
Morales
G J
GJ
Leboeuf
J N
JN