fig01.htm

Figure 1. Profiles of the plasma density calculated for the stationary state versus the length of the magnetic field line given in the nightside auroral magnetosphere. The solid and dotted (dashed and dash-dot) lines are shown for the thermal (auroral) protons and electrons, respectively. The curves are shown for the case where Drperp=100  km, Eperp=10 mV m-1, and W/(nkBT2)=1times 10-3 at s=0. Besides, n1/n3=10 at the top of the given magnetic field line (s=sm) for t=0.


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