From "Simulations of Radiation Belt Formation During Storm Sudden
Commencements" by Hudson et. al., JGR, 102, 14,087, 1997.
See also "Radiation
Belt Formation During Storm Sudden Commencements and Loss During Main
Phase" by Hudson et. al., Adv. Space Res., 1997 (in press).
Plate 6b -Flux vs. energy and L shell after 500 seconds using solar
proton source population with W-2 power law weighting plus
inner zone and MHD fields, for southward IMF case, with a solar wind
shock speed of 1000 km/s.
Plate 6c - Southward IMF case for a solar wind shock speed of 1400 km/s
and W0.3 solar proton power law weighting, appropriate for
the March 1991 event [Hudson et al., 1995]. Energy axis has been
extended to 100 MeV for this case to coincide with the full range of
the Protel instrument on CRRES.
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