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- W2017017057 abstract "There are important geomagnetic implications whenever the interplanetary magnetic field (IMF) turns northward or southward. This paper addresses only the initial turning when the solar events' shock signals first reach 1 AU. A three-dimensional (3D), time-dependent, MHD model [Han et al., 1988] of disturbances' propagation through the solar wind and interplanetary magnetic field (IMF) has been used by Wu (1993) to develop a “recipe” for the initial north- or south-turning of the IMF's polarity. Its temporal behavior thereafter is not addressed in this paper. Four independent data sets have been used [Wu et al., 1996a, b, c] in a study currently underway to test this idea. A fifth data set [Gosling et al., 1990] is used in this paper to examine, via this idea, the initial Bz polarity's change at 1 AU caused by shocks associated with interplanetary/coronal mass ejection events and large geomagnetic storms during the period of August 1978 to October 1982. Twenty-five events from this fifth data set are studied; the prediction model is in agreement with twenty-one of them. Our results suggest that the initial IMF Bz polarity's change at 1 AU may be associated with a simple relationship between the location of the solar disturbance, the relative position of the heliospheric current sheet, and the initial toward or away polarity of the IMF at Earth." @default.
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- W2017017057 title "predicting the initial IMF B<sub><i>z</i></sub>polarity's change at 1 AU caused by shocks that precede coronal mass ejections" @default.
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- W2017017057 doi "https://doi.org/10.1029/96gl01721" @default.
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