Hi Cathy,
You can change the spectral distribution of solar radiation fairly
easily by altering the first nine elements of the frcsol array
in radsw.F90.
This is the fraction of solar radiation within a spectral band.
The wavmin and wavmax variables contain the spectral
boundaries (in microns) to guide your re-allocation.
Bands 1-7 are UV and 8 and 9 are visible.
You can reapportion energy among these bands as you wish so long as the net change is zero.
Good luck,
Charlie