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Your run results will be published online under your Run Registration Number (FirstName_LastName_MMDDYY_ModelType_RunNumber) e.g. John_Smith_032511_SH_1.
vo( fs, Θb ) = a1 + a2 / (1 + fs) 1/a3 ( a4 - a5 e- (( Θb/a6 ) a7 ) ) a8 km s -1
v = min ( max ( v0, a9 ), a10 )
where fs is the rate at which a magnetic flux tube at rssexpands compared to a purely radial expansion and Θb is the minimum angular separation at the photosphere between an open field foot-point and the nearest coronal hole boundary [Owens,M.J., et al, (2008), Space Weather, Vol. 6, S08001, doi:10.1029/2007SW000380].
Values for each parameter can be between: 0.1 - 999.9
ONLY if you require a customized simulation setup not provided by the standard submission options. Unlike the standard runs that are automatically processed, special requests are reviewed and manually modified by the CCMC staff. Please note that special requests are reviewed and manually modified by the CCMC staff and are executed only if resources are available.
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