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Pages 77-80

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From page 77...
... 3. It is time to move beyond existing one- and two-dimensional models to threedimensional MHD simulations in order to correctly model the initiation of solar storms (and the associated shocks)
From page 78...
... Mullen, and D.H. Brautigam, "Improved understanding of the earth's radiation belts from the CRRES satellite," IEEE Trans.
From page 79...
... .R. Wygant, "Simulations of radiation belt formation during storm sudden commencements,"
From page 80...
... 28. See note 1.


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