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T. Dum, and M. , 615, Springer Verlag, Heidelberg. Russell, C. , and McPherron, R. , 1973, The magnetotail and substorms, Space Sci. Rev. 15:205–266. Russell, C. , Fedder, J. , Slinker, S. , Luhmann, J. , Fenrich, F. , Chandler, M. , Moore, T. , and Fuselier, S. , 1998a, Entry of the POLAR spacecraft into the polar cusp under northward IMF conditions, Geophys. Res. Lett. 25:3015–3018. Russell, C. , Khurana, K. , Huddleston, D. , and Kivelson, M. , 1998b, Localized reconnection in the near Jovian magnetotail, Science 280:1061–1064.
2002, 3D hybrid simulations of the interaction of the solar wind with a weak comet, Planet. Space Sci. 50(4):403–411. Luhmann, J. , Walker, R. , Russell, C. , Crooker, N. , Spreiter, J. , and Stahara, S. , 1984a, Patterns of potential magnetic field merging sites on the dayside magnetopause, J. Geophys. Res. 89:1739–1742. Luhmann, J. , Walker, R. , Russell, C. , Spreiter, J. , Stahara, S. , and Williams, D. , 1984b, Mapping the magnetosheath field between the magnetopause and bow shock: Implications for magnetospheric particle leakage, J.
Song and Russell (1992) have pointed out that this process also captures any solar wind momentum originally on the reconnected flux tube. This capture also assists in the circulation of plasma and could create the low latitude boundary layer. When the interplanetary magnetic field is southward, reconnection occurs on the closed dayside field lines at low latitudes. This process leads to flow over the polar cap away from the sun. Reconnection of oppositely-directed field lines in the magnetotail completes the circulation by returning magnetic flux from the tail to the night side magnetosphere.
A Computer Simulation Of An Induction Heating System - Magnetics, Ieee Transactions On