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The cause of high intensity long-duration continuous AE activity (HILDCAAs): Interplanetary AlfVen trains
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The efficiency of “viscous interaction” between the solar wind and the magnetosphere during intense northward IMF events
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Origin of interplanetary southward magnetic fields responsible for major magnetic storms near solar maximum (1978-1979)
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50
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Interplanetary origin of geomagnetic activity in the declining phase of the solar cycle
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51
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The interplanetary causes of magnetic storms: A review
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Plasma properties of driver gas following interplanetary shocks observed by ISEE-3
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Zwickl, R.D., J.R. Ashbridge, S.J. Bame, W.C. Feldman, J.T. Gosling, and E.J. Smith, Plasma properties of driver gas following interplanetary shocks observed by ISEE-3, in Solar Wind Five, NASA Conf. Publ. CP-2280, 711, 1983.
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