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Plasma flow boundaries in the high latitude ionosphere

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Figure

Figure 1.2: A sketch showing the motion of a charged particle in a converging magneticfield.
Figure 1.11: An example of the daytime height profile of the parallel, Pedersen andHall conductivities, respectively
Figure 1.12: A sketch looking down on the northern hemisphere high latitude iono-sphere
Figure 1.13: A sketch taken adapted from Cowley et al. (1991) to show how theIMF By introduces asymmetries on the dayside convection pattern in the northernhemisphere
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