subroutine rrtmg_sw::setcoef ( real (kind=kind_phys), dimension(:), intent(in)  pavel, real (kind=kind_phys), dimension(:), intent(in)  tavel, real (kind=kind_phys), dimension(:), intent(in)  h2ovmr, integer, intent(in)  nlay, integer, intent(in)  nlp1, integer, intent(out)  laytrop, integer, dimension(nlay), intent(out)  jp, integer, dimension(nlay), intent(out)  jt, integer, dimension(nlay), intent(out)  jt1, real (kind=kind_phys), dimension(nlay), intent(out)  fac00, real (kind=kind_phys), dimension(nlay), intent(out)  fac01, real (kind=kind_phys), dimension(nlay), intent(out)  fac10, real (kind=kind_phys), dimension(nlay), intent(out)  fac11, real (kind=kind_phys), dimension(nlay), intent(out)  selffac, real (kind=kind_phys), dimension(nlay), intent(out)  selffrac, integer, dimension(nlay), intent(out)  indself, real (kind=kind_phys), dimension(nlay), intent(out)  forfac, real (kind=kind_phys), dimension(nlay), intent(out)  forfrac, integer, dimension(nlay), intent(out)  indfor  )

private

Parameters

pavel	layer pressure (mb)
tavel	layer temperature (k)
h2ovmr	layer w.v. volumn mixing ratio (kg/kg)
nlay	total number of vertical layers
nlp1	total number of vertical levels
laytrop	tropopause layer index (unitless)
jp	indices of lower reference pressure
jt,jt1	indices of lower reference temperatures at levels of jp and jp+1
fac00,fac01,fac10,fac11	factors mltiply the reference ks,i,j=0/1 for lower/higher of the 2 appropriate temperature and altitudes.
selffac	scale factor for w. v. self-continuum equals (w.v. density)/(atmospheric density at 296k and 1013 mb)
selffrac	factor for temperature interpolation of reference w.v. self-continuum data
indself	index of lower ref temp for selffac
forfac	scale factor for w. v. foreign-continuum
forfrac	factor for temperature interpolation of reference w.v. foreign-continuum data
indfor	index of lower ref temp for forfac

setcoef General Algorithm

1. Find the two reference pressures on either side of the layer pressure. store them in jp and jp1. store in fp the fraction of the difference (in ln(pressure)) between these two values that the layer pressure lies.
2. Determine, for each reference pressure (jp and jp1), which reference temperature (these are different for each reference pressure) is nearest the layer temperature but does not exceed it. store these indices in jt and jt1, resp. store in ft (resp. ft1) the fraction of the way between jt (jt1) and the next highest reference temperature that the layer temperature falls.
3. We have now isolated the layer ln pressure and temperature, between two reference pressures and two reference temperatures (for each reference pressure). we multiply the pressure fraction fp with the appropriate temperature fractions to get the factors that will be needed for the interpolation that yields the optical depths (performed in routines taugbn for band n).
4. If the pressure is less than ~100mb, perform a different set of species interpolations.
5. Set up factors needed to separately include the water vapor foreign-continuum in the calculation of absorption coefficient.
6. Set up factors needed to separately include the water vapor self-continuum in the calculation of absorption coefficient.

References f_one, f_zero, module_radsw_ref::preflog, stpfac, and module_radsw_ref::tref.

Referenced by rrtmg_sw_run().