fig05.htm

Figure 5. Profiles of the coefficient of thermal conductivity of plasma calculated for the stationary state versus the length of the magnetic field line given in the nightside auroral magnetosphere. The solid and dotted lines indicate thermal protons and electrons, respectively. The curves are shown for the case where Drperp=100  km, Eperp=10  mV m-1, and W/(nkBT2)=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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