Publisher: Elsevier

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Volume 28, Number 12, 2001

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Preface
pp. 1683-1683(1)
Authors: Pulkkinen, T.; Wolf, R.

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Comparison of global MHD simulation results with actual storm and substorm events
pp. 1701-1706(6)
Authors: Lopez, R.E.; Lyon, J.G.; Wiltberger, M.J.; Goodrich, C.C.

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The accuracy of present models of the high altitude polar magnetosphere
pp. 1707-1716(10)
Authors: Russell, C.T.; Luhmann, J.G.; Fenrich, F.R.

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How to address the accuracy of empirical magnetic field models?
pp. 1717-1726(10)
Author: Pulkkinen, T.I.

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Comparing two models of the Earth's magnetosphere
pp. 1727-1732(6)
Author: Wodnicka, E.B.

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The model of turbulent plasma sheet during IMF Bz > 0
pp. 1747-1752(6)
Authors: Antonova, E.E.; Ovchinnikov, I.L.

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Solar-proton polar-cap intensity structures as a test of magnetic field models
pp. 1753-1757(5)
Authors: Blake, J.B.; McNab, M.C.; Mazur, J.E.

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FEM code simulation of the magnetospheric proton fluxes
pp. 1759-1762(4)
Authors: Pugacheva, G.I.; Gusev, A.A.; Jayanthi, U.B.; Martin, I.M.; Spjeldvik, W.N.

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Global MHD simulations for southward IMF: a pair of wings in the flanks
pp. 1763-1771(9)
Authors: Song, P.; DeZeeuw, D.L.; Gombosi, T.I.; Kozyra, J.U.; Powell, K.G.

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Author index
pp. 1775-1775(1)

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