source: trunk/LMDZ.GENERIC/libf/phystd/gfluxi.F @ 603

Last change on this file since 603 was 543, checked in by aslmd, 13 years ago

LMDZ.GENERIC: Temperature grid for Planck calculations can now be refined through the parameter NTfac in radinc_h

File size: 6.7 KB
Line 
1      SUBROUTINE GFLUXI(NLL,TLEV,NW,DW,DTAU,TAUCUM,W0,COSBAR,UBARI,
2     *                  RSF,BTOP,BSURF,FTOPUP,FMIDP,FMIDM)
3
4C  THIS SUBROUTINE TAKES THE OPTICAL CONSTANTS AND BOUNDARY CONDITIONS
5C  FOR THE INFRARED FLUX AT ONE WAVELENGTH AND SOLVES FOR THE FLUXES AT
6C  THE LEVELS. THIS VERSION IS SET UP TO WORK WITH LAYER OPTICAL DEPTHS
7C  MEASURED FROM THE TOP OF EACH LAYER.  THE TOP OF EACH LAYER HAS 
8C  OPTICAL DEPTH ZERO.  IN THIS SUB LEVEL N IS ABOVE LAYER N. THAT IS LAYER N
9C  HAS LEVEL N ON TOP AND LEVEL N+1 ON BOTTOM. OPTICAL DEPTH INCREASES
10C  FROM TOP TO BOTTOM. SEE C.P. MCKAY, TGM NOTES.
11C THE TRI-DIAGONAL MATRIX SOLVER IS DSOLVER AND IS DOUBLE PRECISION SO MANY
12C VARIABLES ARE PASSED AS SINGLE THEN BECOME DOUBLE IN DSOLVER
13C
14C NLL            = NUMBER OF LEVELS (NLAYERS + 1) MUST BE LESS THAT NL (101)
15C TLEV(L_LEVELS) = ARRAY OF TEMPERATURES AT GCM LEVELS
16C WAVEN          = WAVELENGTH FOR THE COMPUTATION
17C DW             = WAVENUMBER INTERVAL
18C DTAU(NLAYER)   = ARRAY OPTICAL DEPTH OF THE LAYERS
19C W0(NLEVEL)     = SINGLE SCATTERING ALBEDO
20C COSBAR(NLEVEL) = ASYMMETRY FACTORS, 0=ISOTROPIC
21C UBARI          = AVERAGE ANGLE, MUST BE EQUAL TO 0.5 IN IR
22C RSF            = SURFACE REFLECTANCE
23C BTOP           = UPPER BOUNDARY CONDITION ON IR INTENSITY (NOT FLUX)
24C BSURF          = SURFACE EMISSION = (1-RSFI)*PLANCK, INTENSITY (NOT FLUX)
25C FP(NLEVEL)     = UPWARD FLUX AT LEVELS
26C FM(NLEVEL)     = DOWNWARD FLUX AT LEVELS
27C FMIDP(NLAYER)  = UPWARD FLUX AT LAYER MIDPOINTS
28C FMIDM(NLAYER)  = DOWNWARD FLUX AT LAYER MIDPOINTS
29C
30C----------------------------------------------------------------------C
31
32      use radinc_h
33      use radcommon_h, only: planckir
34
35      implicit none
36
37#include "comcstfi.h"
38
39      INTEGER NLP
40      PARAMETER (NLP=101) ! MUST BE LARGER THAN NLEVEL
41
42      INTEGER NLL, NLAYER, L, NW, NT, NT2
43      REAL*8  TERM, CPMID, CMMID
44      REAL*8  PLANCK
45      REAL*8  EM,EP
46      REAL*8  COSBAR(L_NLAYRAD), W0(L_NLAYRAD), DTAU(L_NLAYRAD)
47      REAL*8  TAUCUM(L_LEVELS), DTAUK
48      REAL*8  TLEV(L_LEVELS)
49      REAL*8  WAVEN, DW, UBARI, RSF
50      REAL*8  BTOP, BSURF, FMIDP(L_NLAYRAD), FMIDM(L_NLAYRAD)
51      REAL*8  B0(NLP),B1(NLP),ALPHA(NLP),LAMDA(NLP),XK1(NLP),XK2(NLP)
52      REAL*8  GAMA(NLP),CP(NLP),CM(NLP),CPM1(NLP),CMM1(NLP),E1(NLP)
53      REAL*8  E2(NLP),E3(NLP),E4(NLP)
54
55      REAL*8  FTOPUP, FLUXUP, FLUXDN
56
57      real*8 :: TAUMAX = L_TAUMAX
58
59C======================================================================C
60 
61C     WE GO WITH THE HEMISPHERIC CONSTANT APPROACH IN THE INFRARED
62 
63
64      IF (NLL .GT. NLP) STOP 'PARAMETER NL TOO SMALL IN GFLUXI'
65
66      NLAYER = L_NLAYRAD
67
68      DO L=1,L_NLAYRAD-1
69        ALPHA(L) = SQRT( (1.0-W0(L))/(1.0-W0(L)*COSBAR(L)) )
70        LAMDA(L) = ALPHA(L)*(1.0-W0(L)*COSBAR(L))/UBARI
71
72        !NT2   = TLEV(2*L+2)*10.0D0-499
73        !NT    = TLEV(2*L)*10.0D0-499
74        NT    = int(TLEV(2*L)*NTfac)   - NTstar+1
75        NT2   = int(TLEV(2*L+2)*NTfac) - NTstar+1
76
77        B1(L) = (PLANCKIR(NW,NT2)-PLANCKIR(NW,NT))/DTAU(L)
78        B0(L) = PLANCKIR(NW,NT)
79      END DO
80
81C     Take care of special lower layer
82
83      L        = L_NLAYRAD
84      ALPHA(L) = SQRT( (1.0-W0(L))/(1.0-W0(L)*COSBAR(L)) )
85      LAMDA(L) = ALPHA(L)*(1.0-W0(L)*COSBAR(L))/UBARI
86
87      !NT    = TLEV(2*L+1)*10.0D0-499
88      !NT2   = TLEV(2*L)*10.0D0-499
89      NT    = int(TLEV(2*L+1)*NTfac) - NTstar+1
90      NT2   = int(TLEV(2*L)*NTfac)   - NTstar+1
91      B1(L) = (PLANCKIR(NW,NT)-PLANCKIR(NW,NT2))/DTAU(L)
92      B0(L) = PLANCKIR(NW,NT2)
93
94      DO L=1,L_NLAYRAD
95        GAMA(L) = (1.0-ALPHA(L))/(1.0+ALPHA(L))
96        TERM    = UBARI/(1.0-W0(L)*COSBAR(L))
97
98C       CP AND CM ARE THE CPLUS AND CMINUS TERMS EVALUATED AT THE
99C       BOTTOM OF THE LAYER.  THAT IS AT DTAU OPTICAL DEPTH
100
101        CP(L) = B0(L)+B1(L)*DTAU(L) +B1(L)*TERM
102        CM(L) = B0(L)+B1(L)*DTAU(L) -B1(L)*TERM
103
104C       CPM1 AND CMM1 ARE THE CPLUS AND CMINUS TERMS EVALUATED
105C       AT THE TOP OF THE LAYER, THAT IS ZERO OPTICAL DEPTH
106
107        CPM1(L) = B0(L)+B1(L)*TERM
108        CMM1(L) = B0(L)-B1(L)*TERM
109      END DO
110 
111C     NOW CALCULATE THE EXPONENTIAL TERMS NEEDED
112C     FOR THE TRIDIAGONAL ROTATED LAYERED METHOD
113C     WARNING IF DTAU(J) IS GREATER THAN ABOUT 35 (VAX)
114C     WE CLIP IT TO AVOID OVERFLOW.
115
116      DO L=1,L_NLAYRAD
117
118C       CLIP THE EXPONENTIAL HERE.
119
120        EP    = EXP( MIN((LAMDA(L)*DTAU(L)),TAUMAX))
121        EM    = 1.0/EP
122        E1(L) = EP+GAMA(L)*EM
123        E2(L) = EP-GAMA(L)*EM
124        E3(L) = GAMA(L)*EP+EM
125        E4(L) = GAMA(L)*EP-EM
126      END DO
127 
128c     B81=BTOP  ! RENAME BEFORE CALLING DSOLVER - used to be to set
129c     B82=BSURF ! them to real*8 - but now everything is real*8
130c     R81=RSF   ! so this may not be necessary
131
132C     Double precision tridiagonal solver
133
134      CALL DSOLVER(NLAYER,GAMA,CP,CM,CPM1,CMM1,E1,E2,E3,E4,BTOP,
135     *             BSURF,RSF,XK1,XK2)
136 
137
138C     NOW WE CALCULATE THE FLUXES AT THE MIDPOINTS OF THE LAYERS.
139 
140      DO L=1,L_NLAYRAD-1
141        DTAUK = TAUCUM(2*L+1)-TAUCUM(2*L)
142        EP    = EXP(MIN(LAMDA(L)*DTAUK,TAUMAX)) ! CLIPPED EXPONENTIAL
143        EM    = 1.0/EP
144        TERM  = UBARI/(1.-W0(L)*COSBAR(L))
145
146C       CP AND CM ARE THE CPLUS AND CMINUS TERMS EVALUATED AT THE
147C       BOTTOM OF THE LAYER.  THAT IS AT DTAU  OPTICAL DEPTH
148
149        CPMID    = B0(L)+B1(L)*DTAUK +B1(L)*TERM
150        CMMID    = B0(L)+B1(L)*DTAUK -B1(L)*TERM
151        FMIDP(L) = XK1(L)*EP + GAMA(L)*XK2(L)*EM + CPMID
152        FMIDM(L) = XK1(L)*EP*GAMA(L) + XK2(L)*EM + CMMID
153
154C       FOR FLUX WE INTEGRATE OVER THE HEMISPHERE TREATING INTENSITY CONSTANT
155
156        FMIDP(L) = FMIDP(L)*PI
157        FMIDM(L) = FMIDM(L)*PI
158      END DO
159 
160C     And now, for the special bottom layer
161
162      L    = L_NLAYRAD
163
164      EP   = EXP(MIN((LAMDA(L)*DTAU(L)),TAUMAX)) ! CLIPPED EXPONENTIAL
165      EM   = 1.0/EP
166      TERM = UBARI/(1.-W0(L)*COSBAR(L))
167
168C     CP AND CM ARE THE CPLUS AND CMINUS TERMS EVALUATED AT THE
169C     BOTTOM OF THE LAYER.  THAT IS AT DTAU  OPTICAL DEPTH
170
171      CPMID    = B0(L)+B1(L)*DTAU(L) +B1(L)*TERM
172      CMMID    = B0(L)+B1(L)*DTAU(L) -B1(L)*TERM
173      FMIDP(L) = XK1(L)*EP + GAMA(L)*XK2(L)*EM + CPMID
174      FMIDM(L) = XK1(L)*EP*GAMA(L) + XK2(L)*EM + CMMID
175 
176C     FOR FLUX WE INTEGRATE OVER THE HEMISPHERE TREATING INTENSITY CONSTANT
177
178      FMIDP(L) = FMIDP(L)*PI
179      FMIDM(L) = FMIDM(L)*PI
180
181C     FLUX AT THE PTOP LEVEL
182
183      EP   = 1.0
184      EM   = 1.0
185      TERM = UBARI/(1.0-W0(1)*COSBAR(1))
186
187C     CP AND CM ARE THE CPLUS AND CMINUS TERMS EVALUATED AT THE
188C     BOTTOM OF THE LAYER.  THAT IS AT DTAU  OPTICAL DEPTH
189
190      CPMID  = B0(1)+B1(1)*TERM
191      CMMID  = B0(1)-B1(1)*TERM
192
193      FLUXUP = XK1(1)*EP + GAMA(1)*XK2(1)*EM + CPMID
194      FLUXDN = XK1(1)*EP*GAMA(1) + XK2(1)*EM + CMMID
195 
196C     FOR FLUX WE INTEGRATE OVER THE HEMISPHERE TREATING INTENSITY CONSTANT
197
198      FTOPUP = (FLUXUP-FLUXDN)*PI
199
200
201      RETURN
202      END
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