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A first generation numerical geomagnetic storm prediction scheme
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Simulation of three-dimensional solar wind disturbances and resulting geomagnetic storms
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Evaluation of solar Type-II radio burst estimates of initial solar wind shock speed using a kinematic model of the solar wind on April 2001 solar event swarm
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(in press). Sun W., Dryer M., Fry C.D., Deehr C.S., Smith Z., Akasofu S.-I., Kartaleval M.D., and Grigokov K.G. Evaluation of solar Type-II radio burst estimates of initial solar wind shock speed using a kinematic model of the solar wind on April 2001 solar event swarm. Geophys. Res. Lett. (2001)
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Origin of interplanetary southward magnetic fields responsible for major magnetic storms near solar maximum (1978-79)
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Tsurutani B.T., Gonzalez W.D., Tang F., Akasofu S.-I., and Smith E.J. Origin of interplanetary southward magnetic fields responsible for major magnetic storms near solar maximum (1978-79). J. Geophys. Res. 93 (1988) 8519
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