[414] | 1 | c*********************************************************************** |
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| 2 | c tcrco2_subrut.f |
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| 3 | c |
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| 4 | c jan 98 malv version for mz1d. copied from solar10/mz4sub.f |
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| 5 | c jul 2011 malv+fgg adapted to LMD-MGCM |
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| 6 | c*********************************************************************** |
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| 7 | |
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| 8 | ************************************************************************ |
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| 9 | |
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| 10 | subroutine dinterconnection ( v, vt ) |
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| 11 | |
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| 12 | * input: vib. temp. from che*.for programs, vt(nl) |
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| 13 | * output: test vibrational temp. for other che*.for, v(nl) |
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| 14 | ! iconex_smooth=1 ==> with smoothing |
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| 15 | ! iconex_smooth=0 ==> without smoothing |
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| 16 | ! iconex_tk=40 ==> with forced lte up to 40 km |
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| 17 | ! iconex_tk=20 ==> with forced lte up to 20 km |
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| 18 | ************************************************************************ |
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| 19 | |
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| 20 | implicit none |
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| 21 | include 'nltedefs.h' |
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| 22 | |
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| 23 | c argumentos |
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| 24 | real*8 vt(nl), v(nl) |
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| 25 | |
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| 26 | c local variables |
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| 27 | integer i |
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| 28 | |
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| 29 | c ************* |
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| 30 | |
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| 31 | do i=1,nl |
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| 32 | v(i) = vt(i) |
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| 33 | end do |
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| 34 | |
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| 35 | ! lo siguiente se utilizaba en solar10, pero es mejor introducirlo en |
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| 36 | ! la driver. por ahora no lo uso todavia. |
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| 37 | ! call fluctua(v,iconex_fluctua) |
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| 38 | ! call smooth_nl(v,iconex_smooth,nl) |
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| 39 | ! call forzar_tk(v,iconex_tk) |
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| 40 | |
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| 41 | return |
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| 42 | end |
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| 43 | |
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| 44 | c*********************************************************************** |
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| 45 | subroutine smooth_nl(y,nlx,nl) |
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| 46 | |
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| 47 | c returns smoothed y |
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| 48 | c*********************************************************************** |
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| 49 | |
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| 50 | implicit none |
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| 51 | |
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| 52 | c arguments |
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| 53 | integer nl ! Dimension of vectors |
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| 54 | integer nlx ! i. =0 ==> no smoothing |
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| 55 | ! =m ==> smoothing from point m up to nl |
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| 56 | real*8 y(nl) ! o. is returned after smoothed |
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| 57 | |
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| 58 | c local variables and constants |
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| 59 | integer i , nlmax |
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| 60 | parameter ( nlmax=250 ) ! Llevarse esto al mz1d.par ! |
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| 61 | real*8 x(nlmax) |
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| 62 | |
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| 63 | c *************** |
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| 64 | |
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| 65 | if (nlx.eq.0) return |
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| 66 | |
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| 67 | do i=nlx,nl |
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| 68 | x(i)=y(i) |
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| 69 | y(i)=0. |
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| 70 | end do |
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| 71 | |
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| 72 | do i=nlx,nl |
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| 73 | if(i.eq.nlx)then |
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| 74 | y(i)=x(i) |
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| 75 | elseif(i.eq.nl)then |
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| 76 | y(i)=2.*y(i-1)-y(i-2) |
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| 77 | else |
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| 78 | y(i)=(x(i+1)/2.+x(i)+x(i-1)/2.)/2. |
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| 79 | end if |
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| 80 | end do |
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| 81 | |
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| 82 | return |
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| 83 | end |
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| 84 | |
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| 85 | c*********************************************************************** |
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| 86 | function planckdp(tp,xnu) |
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| 87 | c returns the black body function at wavenumber xnu and temperature t. |
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| 88 | c*********************************************************************** |
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| 89 | |
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| 90 | implicit none |
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| 91 | |
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| 92 | include 'nltedefs.h' |
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| 93 | include 'nlte_data.h' |
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| 94 | ! common/datis/ pi, vlight, ee, hplanck, gamma, ab, |
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| 95 | ! @ n_avog, GG, R0, cte_sb, kboltzman, raddeg |
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| 96 | ! real*8 pi, vlight, ee, hplanck, gamma, ab, |
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| 97 | ! @ n_avog, GG, R0, cte_sb, kboltzman, raddeg |
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| 98 | |
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| 99 | real*8 planckdp |
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| 100 | real*8 xnu |
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| 101 | real tp |
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| 102 | |
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| 103 | planckdp = gamma*xnu**3.0 / exp( ee*xnu/dble(tp) ) |
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| 104 | !erg cm-2.sr-1/cm-1. |
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| 105 | |
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| 106 | return |
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| 107 | end |
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| 108 | c*********************************************************************** |
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| 109 | function planckdpdp(tp,xnu) |
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| 110 | c returns the black body function at wavenumber xnu and temperature t. |
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| 111 | c*********************************************************************** |
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| 112 | |
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| 113 | implicit none |
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| 114 | |
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| 115 | include 'nltedefs.h' |
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| 116 | include 'nlte_data.h' |
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| 117 | ! common/datis/ pi, vlight, ee, hplanck, gamma, ab, |
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| 118 | ! @ n_avog, GG, R0, cte_sb, kboltzman, raddeg |
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| 119 | ! real*8 pi, vlight, ee, hplanck, gamma, ab, |
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| 120 | ! @ n_avog, GG, R0, cte_sb, kboltzman, raddeg |
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| 121 | |
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| 122 | real*8 planckdpdp |
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| 123 | real*8 xnu |
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| 124 | real*8 tp |
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| 125 | |
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| 126 | planckdpdp = gamma*xnu**3.0 / exp( ee*xnu/dble(tp) ) |
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| 127 | !erg cm-2.sr-1/cm-1. |
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| 128 | |
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| 129 | return |
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| 130 | end |
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| 131 | c **************************************************************** |
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| 132 | function bandid (ib) |
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| 133 | c returns the 2 character code of the band |
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| 134 | c **************************************************************** |
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| 135 | implicit none |
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| 136 | |
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| 137 | integer ib |
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| 138 | character*2 bandid |
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| 139 | |
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| 140 | 132 format(i2) |
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| 141 | ! encode (2,132,bandid) ib |
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| 142 | write ( bandid, 132) ib |
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| 143 | |
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| 144 | if ( ib .eq. 1 ) bandid = '01' |
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| 145 | if ( ib .eq. 2 ) bandid = '02' |
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| 146 | if ( ib .eq. 3 ) bandid = '03' |
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| 147 | if ( ib .eq. 4 ) bandid = '04' |
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| 148 | if ( ib .eq. 5 ) bandid = '05' |
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| 149 | if ( ib .eq. 6 ) bandid = '06' |
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| 150 | if ( ib .eq. 7 ) bandid = '07' |
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| 151 | if ( ib .eq. 8 ) bandid = '08' |
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| 152 | if ( ib .eq. 9 ) bandid = '09' |
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| 153 | if ( ib .eq. 0 ) bandid = '00' |
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| 154 | |
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| 155 | c end |
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| 156 | return |
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| 157 | end |
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