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callcorrk.F90 @ 3444

Last change on this file since 3444 was 3444, checked in by afalco, 2 months ago
Pluto PCM: reffrad not written if not initialized. AF
Property svn:executable set to ``*
File size: 52.8 KB

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1	MODULE callcorrk_mod
2
3	IMPLICIT NONE
4
5	CONTAINS
6
7	subroutine callcorrk(ngrid,nlayer,pq,nq,qsurf, &
8	albedo,albedo_equivalent,emis,mu0,pplev,pplay,pt, &
9	zzlay,tsurf,fract,dist_star,aerosol,muvar, &
10	dtlw,dtsw,fluxsurf_lw, &
11	fluxsurf_sw,fluxsurfabs_sw,fluxtop_lw, &
12	fluxabs_sw,fluxtop_dn, &
13	OLR_nu,OSR_nu,GSR_nu, &
14	int_dtaui,int_dtauv, &
15	tau_col,cloudfrac,totcloudfrac, &
16	clearsky,firstcall,lastcall)
17
18	use mod_phys_lmdz_para, only : is_master
19	use radinc_h, only: L_NSPECTV, L_NSPECTI, naerkind, banddir, corrkdir,&
20	L_LEVELS, L_NGAUSS, L_NLEVRAD, L_NLAYRAD, L_REFVAR
21	use radcommon_h, only: wrefvar, Cmk, fzeroi, fzerov, gasi, gasv, &
22	glat_ig, gweight, pfgasref, pgasmax, pgasmin, &
23	pgasref, tgasmax, tgasmin, tgasref, scalep, &
24	ubari, wnoi, stellarf, glat, dwnv, dwni, tauray
25	use datafile_mod, only: datadir
26	use ioipsl_getin_p_mod, only: getin_p
27	use gases_h, only: ngasmx
28	use radii_mod, only : su_aer_radii, haze_reffrad_fix
29	use aerosol_mod, only : iaero_haze
30	use aeropacity_mod, only: aeropacity
31	use aeroptproperties_mod, only: aeroptproperties
32	use tracer_h, only: constants_epsi_generic,igcm_ch4_gas,igcm_n2,mmol
33	use comcstfi_mod, only: pi, mugaz, cpp, r, g
34	use callkeys_mod, only: varactive,diurnal,tracer,varfixed,satval, &
35	diagdtau,kastprof,strictboundcorrk,specOLR, &
36	tplanckmin,tplanckmax,global1d, &
37	generic_condensation,aerohaze,haze_radproffix,&
38	methane,carbox,cooling,nlte,strobel,&
39	ch4fix,vmrch4_proffix,vmrch4fix
40	use optcv_mod, only: optcv
41	use optci_mod, only: optci
42	use sfluxi_mod, only: sfluxi
43	use sfluxv_mod, only: sfluxv
44	use recombin_corrk_mod, only: corrk_recombin, call_recombin
45	use generic_cloud_common_h, only: Psat_generic, epsi_generic
46	use generic_tracer_index_mod, only: generic_tracer_index
47	use planetwide_mod, only: planetwide_maxval, planetwide_minval
48	use radcommon_h, only: wavev,wavei
49	implicit none
50
51	!==================================================================
52	!
53	! Purpose
54	! -------
55	! Solve the radiative transfer using the correlated-k method for
56	! the gaseous absorption and the Toon et al. (1989) method for
57	! scatttering due to aerosols.
58	!
59	! Authors
60	! -------
61	! Emmanuel 01/2001, Forget 09/2001
62	! Robin Wordsworth (2009)
63	!
64	!==================================================================
65
66	!-----------------------------------------------------------------------
67	! Declaration of the arguments (INPUT - OUTPUT) on the LMD GCM grid
68	! Layer #1 is the layer near the ground.
69	! Layer #nlayer is the layer at the top.
70	!-----------------------------------------------------------------------
71
72
73	! INPUT
74	INTEGER,INTENT(IN) :: ngrid ! Number of atmospheric columns.
75	INTEGER,INTENT(IN) :: nlayer ! Number of atmospheric layers.
76	REAL,INTENT(IN) :: pq(ngrid,nlayer,nq) ! Tracers (kg/kg_of_air).
77	INTEGER,INTENT(IN) :: nq ! Number of tracers.
78	REAL,INTENT(IN) :: qsurf(ngrid,nq) ! Tracers on surface (kg.m-2).
79	REAL,INTENT(IN) :: albedo(ngrid,L_NSPECTV) ! Spectral Short Wavelengths Albedo. By MT2015
80	REAL,INTENT(IN) :: emis(ngrid) ! Long Wave emissivity.
81	REAL,INTENT(IN) :: mu0(ngrid) ! Cosine of sun incident angle.
82	REAL,INTENT(IN) :: pplev(ngrid,nlayer+1) ! Inter-layer pressure (Pa).
83	REAL,INTENT(IN) :: pplay(ngrid,nlayer) ! Mid-layer pressure (Pa).
84	REAL,INTENT(IN) :: pt(ngrid,nlayer) ! Air temperature (K).
85	REAL,INTENT(IN) :: zzlay(ngrid,nlayer) ! Mid-layer altitude
86	REAL,INTENT(IN) :: tsurf(ngrid) ! Surface temperature (K).
87	REAL,INTENT(IN) :: fract(ngrid) ! Fraction of day.
88	REAL,INTENT(IN) :: dist_star ! Distance star-planet (AU).
89	REAL,INTENT(IN) :: muvar(ngrid,nlayer+1)
90	REAL,INTENT(IN) :: cloudfrac(ngrid,nlayer) ! Fraction of clouds (%).
91	logical,intent(in) :: clearsky
92	logical,intent(in) :: firstcall ! Signals first call to physics.
93	logical,intent(in) :: lastcall ! Signals last call to physics.
94
95	! OUTPUT
96	REAL,INTENT(OUT) :: aerosol(ngrid,nlayer,naerkind) ! Aerosol tau at reference wavelenght.
97	REAL,INTENT(OUT) :: dtlw(ngrid,nlayer) ! Heating rate (K/s) due to LW radiation.
98	REAL,INTENT(OUT) :: dtsw(ngrid,nlayer) ! Heating rate (K/s) due to SW radiation.
99	REAL,INTENT(OUT) :: fluxsurf_lw(ngrid) ! Incident LW flux to surf (W/m2).
100	REAL,INTENT(OUT) :: fluxsurf_sw(ngrid) ! Incident SW flux to surf (W/m2)
101	REAL,INTENT(OUT) :: fluxsurfabs_sw(ngrid) ! Absorbed SW flux by the surface (W/m2). By MT2015.
102	REAL,INTENT(OUT) :: fluxtop_lw(ngrid) ! Outgoing LW flux to space (W/m2).
103	REAL,INTENT(OUT) :: fluxabs_sw(ngrid) ! SW flux absorbed by the planet (W/m2).
104	REAL,INTENT(OUT) :: fluxtop_dn(ngrid) ! Incident top of atmosphere SW flux (W/m2).
105	REAL,INTENT(OUT) :: OLR_nu(ngrid,L_NSPECTI) ! Outgoing LW radiation in each band (Normalized to the band width (W/m2/cm-1).
106	REAL,INTENT(OUT) :: OSR_nu(ngrid,L_NSPECTV) ! Outgoing SW radiation in each band (Normalized to the band width (W/m2/cm-1).
107	REAL,INTENT(OUT) :: GSR_nu(ngrid,L_NSPECTV) ! Surface SW radiation in each band (Normalized to the band width (W/m2/cm-1).
108	REAL,INTENT(OUT) :: tau_col(ngrid) ! Diagnostic from aeropacity.
109	REAL,INTENT(OUT) :: albedo_equivalent(ngrid) ! Spectrally Integrated Albedo. For Diagnostic. By MT2015
110	REAL,INTENT(OUT) :: totcloudfrac(ngrid) ! Column Fraction of clouds (%).
111	REAL,INTENT(OUT) :: int_dtaui(ngrid,nlayer,L_NSPECTI) ! VI optical thickness of layers within narrowbands for diags ().
112	REAL,INTENT(OUT) :: int_dtauv(ngrid,nlayer,L_NSPECTV) ! IR optical thickness of layers within narrowbands for diags ().
113
114
115
116
117
118	! Globally varying aerosol optical properties on GCM grid ; not needed everywhere so not in radcommon_h.
119	! made "save" variables so they are allocated once in for all, not because
120	! the values need be saved from a time step to the next
121	REAL,SAVE,ALLOCATABLE :: QVISsQREF3d(:,:,:,:)
122	REAL,SAVE,ALLOCATABLE :: omegaVIS3d(:,:,:,:)
123	REAL,SAVE,ALLOCATABLE :: gVIS3d(:,:,:,:)
124	!$OMP THREADPRIVATE(QVISsQREF3d,omegaVIS3d,gVIS3d)
125	REAL,SAVE,ALLOCATABLE :: QIRsQREF3d(:,:,:,:)
126	REAL,SAVE,ALLOCATABLE :: omegaIR3d(:,:,:,:)
127	REAL,SAVE,ALLOCATABLE :: gIR3d(:,:,:,:)
128	!$OMP THREADPRIVATE(QIRsQREF3d,omegaIR3d,gIR3d)
129
130	! REAL :: omegaREFvis3d(ngrid,nlayer,naerkind)
131	! REAL :: omegaREFir3d(ngrid,nlayer,naerkind) ! not sure of the point of these...
132
133	REAL,ALLOCATABLE,SAVE :: reffrad(:,:,:) ! aerosol effective radius (m)
134	REAL,ALLOCATABLE,SAVE :: nueffrad(:,:,:) ! aerosol effective variance
135	!$OMP THREADPRIVATE(reffrad,nueffrad)
136
137	!-----------------------------------------------------------------------
138	! Declaration of the variables required by correlated-k subroutines
139	! Numbered from top to bottom (unlike in the GCM)
140	!-----------------------------------------------------------------------
141
142	REAL*8 tmid(L_LEVELS),pmid(L_LEVELS)
143	REAL*8 tlevrad(L_LEVELS),plevrad(L_LEVELS)
144
145	! Optical values for the optci/cv subroutines
146	REAL*8 stel(L_NSPECTV),stel_fract(L_NSPECTV)
147	! NB: Arrays below are "save" to avoid reallocating them at every call
148	! not because their content needs be reused from call to the next
149	REAL*8,allocatable,save :: dtaui(:,:,:)
150	REAL*8,allocatable,save :: dtauv(:,:,:)
151	REAL*8,allocatable,save :: cosbv(:,:,:)
152	REAL*8,allocatable,save :: cosbi(:,:,:)
153	REAL*8,allocatable,save :: wbari(:,:,:)
154	REAL*8,allocatable,save :: wbarv(:,:,:)
155	!$OMP THREADPRIVATE(dtaui,dtauv,cosbv,cosbi,wbari,wbarv)
156	REAL*8,allocatable,save :: tauv(:,:,:)
157	REAL*8,allocatable,save :: taucumv(:,:,:)
158	REAL*8,allocatable,save :: taucumi(:,:,:)
159	!$OMP THREADPRIVATE(tauv,taucumv,taucumi)
160	REAL*8,allocatable,save :: tauaero(:,:)
161	!$OMP THREADPRIVATE(tauaero)
162	REAL*8 nfluxtopv,nfluxtopi,nfluxtop,fluxtopvdn
163	real*8 nfluxtopv_nu(L_NSPECTV)
164	REAL*8 nfluxoutv_nu(L_NSPECTV) ! Outgoing band-resolved VI flux at TOA (W/m2).
165	REAL*8 nfluxtopi_nu(L_NSPECTI) ! Net band-resolved IR flux at TOA (W/m2).
166	REAL*8 fluxupi_nu(L_NLAYRAD,L_NSPECTI) ! For 1D diagnostic.
167	REAL*8 fmneti(L_NLAYRAD),fmnetv(L_NLAYRAD)
168	real*8 fmneti_nu(L_NLAYRAD,L_NSPECTI) !
169	real*8 fmnetv_nu(L_NLAYRAD,L_NSPECTV) !
170	REAL*8 fluxupv(L_NLAYRAD),fluxupi(L_NLAYRAD)
171	REAL*8 fluxdnv(L_NLAYRAD),fluxdni(L_NLAYRAD)
172	REAL*8 albi,acosz
173	REAL*8 albv(L_NSPECTV) ! Spectral Visible Albedo.
174
175	INTEGER ig,l,k,nw,iaer,iq
176
177	real*8,allocatable,save :: taugsurf(:,:)
178	real*8,allocatable,save :: taugsurfi(:,:)
179	!$OMP THREADPRIVATE(taugsurf,taugsurfi)
180	real*8 qvar(L_LEVELS) ! Mixing ratio of variable component (mol/mol). index 1 is the top of the atmosphere, index L_LEVELS is the bottom
181
182	! Local aerosol optical properties for each column on RADIATIVE grid.
183	real8,save,allocatable :: QXVAER(:,:,:) ! Extinction coeff (QVISsQREFQREFvis)
184	real*8,save,allocatable :: QSVAER(:,:,:)
185	real*8,save,allocatable :: GVAER(:,:,:)
186	real8,save,allocatable :: QXIAER(:,:,:) ! Extinction coeff (QIRsQREFQREFir)
187	real*8,save,allocatable :: QSIAER(:,:,:)
188	real*8,save,allocatable :: GIAER(:,:,:)
189	!$OMP THREADPRIVATE(QXVAER,QSVAER,GVAER,QXIAER,QSIAER,GIAER)
190	real, dimension(:,:,:), save, allocatable :: QREFvis3d
191	real, dimension(:,:,:), save, allocatable :: QREFir3d
192	!$OMP THREADPRIVATE(QREFvis3d,QREFir3d)
193
194
195	! Miscellaneous :
196	real*8 temp,temp1,temp2,pweight
197	character(len=10) :: tmp1
198	character(len=10) :: tmp2
199	character(len=100) :: message
200	character(len=10),parameter :: subname="callcorrk"
201
202	! For fixed water vapour profiles.
203	integer i_var
204	real RH
205	real*8 pq_temp(nlayer)
206	! real(KIND=r8) :: pq_temp(nlayer) ! better F90 way.. DOESNT PORT TO F77!!!
207	real psat,qsat
208
209	logical OLRz
210	real*8 NFLUXGNDV_nu(L_NSPECTV)
211
212	! Included by RW for runaway greenhouse 1D study.
213	real vtmp(nlayer)
214	REAL*8 muvarrad(L_LEVELS)
215
216	! Included by MT for albedo calculations.
217	REAL*8 albedo_temp(L_NSPECTV) ! For equivalent albedo calculation.
218	REAL*8 surface_stellar_flux ! Stellar flux reaching the surface. Useful for equivalent albedo calculation.
219
220	! NLTE factor for CH4
221	real eps_nlte_sw23(ngrid,nlayer) ! CH4 NLTE efficiency factor for zdtsw
222	real eps_nlte_sw33(ngrid,nlayer) ! CH4 NLTE efficiency factor for zdtsw
223	real eps_nlte_lw(ngrid,nlayer) ! CH4 NLTE efficiency factor for zdtsw
224	integer Nfine,ifine
225	parameter(Nfine=701)
226	real,save :: levdat(Nfine),vmrdat(Nfine)
227	REAL dtlw_hcn_c2h2(ngrid, nlayer) ! cooling rate (K/s) due to C2H2/HCN (diagnostic)
228	real :: vmrch4(ngrid,nlayer) ! vmr ch4 from vmrch4_proffix
229
230	REAL dtlw_nu(nlayer,L_NSPECTI) ! heating rate (K/s) due to LW in spectral bands
231	REAL dtsw_nu(nlayer,L_NSPECTV) ! heating rate (K/s) due to SW in spectral bands
232
233	! local variable
234	REAL dpp ! intermediate
235
236	integer ok ! status (returned by NetCDF functions)
237
238	integer igcm_generic_gas, igcm_generic_ice! index of the vap and ice of generic_tracer
239	logical call_ice_gas_generic ! to call only one time the ice/vap pair of a tracer
240	real, save :: metallicity ! metallicity of planet --- is not used here, but necessary to call function Psat_generic
241	!$OMP THREADPRIVATE(metallicity)
242	REAL, SAVE :: qvap_deep ! deep mixing ratio of water vapor when simulating bottom less planets
243	!$OMP THREADPRIVATE(qvap_deep)
244
245	REAL :: maxvalue,minvalue
246
247	!===============================================================
248	! I.a Initialization on first call
249	!===============================================================
250
251
252	if(firstcall) then
253
254	! test on allocated necessary because of CLFvarying (two calls to callcorrk in physiq)
255	if(.not.allocated(QVISsQREF3d)) then
256	allocate(QVISsQREF3d(ngrid,nlayer,L_NSPECTV,naerkind))
257	endif
258	if(.not.allocated(omegaVIS3d)) then
259	allocate(omegaVIS3d(ngrid,nlayer,L_NSPECTV,naerkind))
260	endif
261	if(.not.allocated(gVIS3d)) then
262	allocate(gVIS3d(ngrid,nlayer,L_NSPECTV,naerkind))
263	endif
264	if (.not.allocated(QIRsQREF3d)) then
265	allocate(QIRsQREF3d(ngrid,nlayer,L_NSPECTI,naerkind))
266	endif
267	if (.not.allocated(omegaIR3d)) then
268	allocate(omegaIR3d(ngrid,nlayer,L_NSPECTI,naerkind))
269	endif
270	if (.not.allocated(gIR3d)) then
271	allocate(gIR3d(ngrid,nlayer,L_NSPECTI,naerkind))
272	endif
273	if (.not.allocated(tauaero)) then
274	allocate(tauaero(L_LEVELS,naerkind))
275	endif
276
277	if(.not.allocated(QXVAER)) then
278	allocate(QXVAER(L_LEVELS,L_NSPECTV,naerkind), stat=ok)
279	if (ok /= 0) then
280	write(,) "memory allocation failed for QXVAER!"
281	call abort_physic(subname,'allocation failure for QXVAER',1)
282	endif
283	endif
284	if(.not.allocated(QSVAER)) then
285	allocate(QSVAER(L_LEVELS,L_NSPECTV,naerkind), stat=ok)
286	if (ok /= 0) then
287	write(,) "memory allocation failed for QSVAER!"
288	call abort_physic(subname,'allocation failure for QSVAER',1)
289	endif
290	endif
291	if(.not.allocated(GVAER)) then
292	allocate(GVAER(L_LEVELS,L_NSPECTV,naerkind), stat=ok)
293	if (ok /= 0) then
294	write(,) "memory allocation failed for GVAER!"
295	call abort_physic(subname,'allocation failure for GVAER',1)
296	endif
297	endif
298	if(.not.allocated(QXIAER)) then
299	allocate(QXIAER(L_LEVELS,L_NSPECTI,naerkind), stat=ok)
300	if (ok /= 0) then
301	write(,) "memory allocation failed for QXIAER!"
302	call abort_physic(subname,'allocation failure for QXIAER',1)
303	endif
304	endif
305	if(.not.allocated(QSIAER)) then
306	allocate(QSIAER(L_LEVELS,L_NSPECTI,naerkind), stat=ok)
307	if (ok /= 0) then
308	write(,) "memory allocation failed for QSIAER!"
309	call abort_physic(subname,'allocation failure for QSIAER',1)
310	endif
311	endif
312	if(.not.allocated(GIAER)) then
313	allocate(GIAER(L_LEVELS,L_NSPECTI,naerkind), stat=ok)
314	if (ok /= 0) then
315	write(,) "memory allocation failed for GIAER!"
316	call abort_physic(subname,'allocation failure for GIAER',1)
317	endif
318	endif
319
320	!!! ALLOCATED instances are necessary because of CLFvarying (strategy to call callcorrk twice in physiq...)
321	IF(.not.ALLOCATED(QREFvis3d))THEN
322	ALLOCATE(QREFvis3d(ngrid,nlayer,naerkind), stat=ok)
323	IF (ok/=0) THEN
324	write(,) "memory allocation failed for QREFvis3d!"
325	call abort_physic(subname,'allocation failure for QREFvis3d',1)
326	ENDIF
327	ENDIF
328	IF(.not.ALLOCATED(QREFir3d)) THEN
329	ALLOCATE(QREFir3d(ngrid,nlayer,naerkind), stat=ok)
330	IF (ok/=0) THEN
331	write(,) "memory allocation failed for QREFir3d!"
332	call abort_physic(subname,'allocation failure for QREFir3d',1)
333	ENDIF
334	ENDIF
335	! Effective radius and variance of the aerosols
336	IF(.not.ALLOCATED(reffrad)) THEN
337	allocate(reffrad(ngrid,nlayer,naerkind), stat=ok)
338	IF (ok/=0) THEN
339	write(,) "memory allocation failed for reffrad!"
340	call abort_physic(subname,'allocation failure for reffrad',1)
341	ENDIF
342	ENDIF
343	IF(.not.ALLOCATED(nueffrad)) THEN
344	allocate(nueffrad(ngrid,nlayer,naerkind), stat=ok)
345	IF (ok/=0) THEN
346	write(,) "memory allocation failed for nueffrad!"
347	call abort_physic(subname,'allocation failure for nueffrad',1)
348	ENDIF
349	ENDIF
350
351	if (is_master) call system('rm -f surf_vals_long.out')
352
353	call su_aer_radii(ngrid,nlayer,reffrad,nueffrad)
354
355
356	!--------------------------------------------------
357	! Set up correlated k
358	!--------------------------------------------------
359
360	!this block is now done at firstcall of physiq_mod
361	! print*, "callcorrk: Correlated-k data base folder:",trim(datadir)
362	! call getin_p("corrkdir",corrkdir)
363	! print*, "corrkdir = ",corrkdir
364	! write( tmp1, '(i3)' ) L_NSPECTI
365	! write( tmp2, '(i3)' ) L_NSPECTV
366	! banddir=trim(adjustl(tmp1))//'x'//trim(adjustl(tmp2))
367	! banddir=trim(adjustl(corrkdir))//'/'//trim(adjustl(banddir))
368
369	! call setspi ! Basic infrared properties.
370	! call setspv ! Basic visible properties.
371	! call sugas_corrk ! Set up gaseous absorption properties.
372	! call suaer_corrk ! Set up aerosol optical properties.
373
374
375	! now that L_NGAUSS has been initialized (by sugas_corrk)
376	! allocate related arrays
377	if(.not.allocated(dtaui)) then
378	ALLOCATE(dtaui(L_NLAYRAD,L_NSPECTI,L_NGAUSS), stat=ok)
379	if (ok/=0) then
380	write(,) "memory allocation failed for dtaui!"
381	call abort_physic(subname,'allocation failure for dtaui',1)
382	endif
383	endif
384	if(.not.allocated(dtauv)) then
385	ALLOCATE(dtauv(L_NLAYRAD,L_NSPECTV,L_NGAUSS), stat=ok)
386	if (ok/=0) then
387	write(,) "memory allocation failed for dtauv!"
388	call abort_physic(subname,'allocation failure for dtauv',1)
389	endif
390	endif
391	if(.not.allocated(cosbv)) then
392	ALLOCATE(cosbv(L_NLAYRAD,L_NSPECTV,L_NGAUSS), stat=ok)
393	if (ok/=0) then
394	write(,) "memory allocation failed for cosbv!"
395	call abort_physic(subname,'allocation failure for cobsv',1)
396	endif
397	endif
398	if(.not.allocated(cosbi)) then
399	ALLOCATE(cosbi(L_NLAYRAD,L_NSPECTI,L_NGAUSS), stat=ok)
400	if (ok/=0) then
401	write(,) "memory allocation failed for cosbi!"
402	call abort_physic(subname,'allocation failure for cobsi',1)
403	endif
404	endif
405	if(.not.allocated(wbari)) then
406	ALLOCATE(wbari(L_NLAYRAD,L_NSPECTI,L_NGAUSS), stat=ok)
407	if (ok/=0) then
408	write(,) "memory allocation failed for wbari!"
409	call abort_physic(subname,'allocation failure for wbari',1)
410	endif
411	endif
412	if(.not.allocated(wbarv)) then
413	ALLOCATE(wbarv(L_NLAYRAD,L_NSPECTV,L_NGAUSS), stat=ok)
414	if (ok/=0) then
415	write(,) "memory allocation failed for wbarv!"
416	call abort_physic(subname,'allocation failure for wbarv',1)
417	endif
418	endif
419	if(.not.allocated(tauv)) then
420	ALLOCATE(tauv(L_NLEVRAD,L_NSPECTV,L_NGAUSS), stat=ok)
421	if (ok/=0) then
422	write(,) "memory allocation failed for tauv!"
423	call abort_physic(subname,'allocation failure for tauv',1)
424	endif
425	endif
426	if(.not.allocated(taucumv)) then
427	ALLOCATE(taucumv(L_LEVELS,L_NSPECTV,L_NGAUSS), stat=ok)
428	if (ok/=0) then
429	write(,) "memory allocation failed for taucumv!"
430	call abort_physic(subname,'allocation failure for taucumv',1)
431	endif
432	endif
433	if(.not.allocated(taucumi)) then
434	ALLOCATE(taucumi(L_LEVELS,L_NSPECTI,L_NGAUSS), stat=ok)
435	if (ok/=0) then
436	write(,) "memory allocation failed for taucumi!"
437	call abort_physic(subname,'allocation failure for taucumi',1)
438	endif
439	endif
440	if(.not.allocated(taugsurf)) then
441	ALLOCATE(taugsurf(L_NSPECTV,L_NGAUSS-1), stat=ok)
442	if (ok/=0) then
443	write(,) "memory allocation failed for taugsurf!"
444	call abort_physic(subname,'allocation failure for taugsurf',1)
445	endif
446	endif
447	if(.not.allocated(taugsurfi)) then
448	ALLOCATE(taugsurfi(L_NSPECTI,L_NGAUSS-1), stat=ok)
449	if (ok/=0) then
450	write(,) "memory allocation failed for taugsurfi!"
451	call abort_physic(subname,'allocation failure for taugsurfi',1)
452	endif
453	endif
454
455
456	if(varfixed .and. (generic_condensation .or. methane .or. carbox))then
457	write(,) "Deep generic tracer vapor mixing ratio ? (no effect if negative) "
458	qvap_deep=-1. ! default value
459	call getin_p("qvap_deep",qvap_deep)
460	write(,) " qvap_deep = ",qvap_deep
461
462	metallicity=0.0 ! default value --- is not used here but necessary to call function Psat_generic
463	call getin_p("metallicity",metallicity) ! --- is not used here but necessary to call function Psat_generic
464	endif
465
466	end if ! of if (firstcall)
467
468	!=======================================================================
469	! I.b Initialization on every call
470	!=======================================================================
471
472	qxvaer(:,:,:)=0.0
473	qsvaer(:,:,:)=0.0
474	gvaer(:,:,:) =0.0
475
476	qxiaer(:,:,:)=0.0
477	qsiaer(:,:,:)=0.0
478	giaer(:,:,:) =0.0
479
480	OLR_nu(:,:) = 0.
481	OSR_nu(:,:) = 0.
482	GSR_nu(:,:) = 0.
483
484	!--------------------------------------------------
485	! Effective radius and variance of the aerosols
486	!--------------------------------------------------
487	if (aerohaze) then
488	do iaer=1,naerkind
489	if ((iaer.eq.iaero_haze)) then
490	call su_aer_radii(ngrid,nlayer,reffrad(1,1,iaer), &
491	nueffrad(1,1,iaer))
492	endif
493	end do !iaer=1,naerkind.
494	if (haze_radproffix) then
495	if (haze_radproffix) then
496	call haze_reffrad_fix(ngrid,nlayer,zzlay,&
497	reffrad,nueffrad)
498	endif
499
500	print*, 'haze_radproffix=T : fixed profile for haze rad'
501	else
502	print*,'reffrad haze:',reffrad(1,1,iaero_haze)
503	print*,'nueff haze',nueffrad(1,1,iaero_haze)
504	endif
505	endif
506
507
508	! How much light do we get ?
509	do nw=1,L_NSPECTV
510	stel(nw)=stellarf(nw)/(dist_star**2)
511	end do
512
513	if (aerohaze) then
514
515	! Get 3D aerosol optical properties.
516	call aeroptproperties(ngrid,nlayer,reffrad,nueffrad, &
517	QVISsQREF3d,omegaVIS3d,gVIS3d, &
518	QIRsQREF3d,omegaIR3d,gIR3d, &
519	QREFvis3d,QREFir3d)
520
521	! Get aerosol optical depths.
522	call aeropacity(ngrid,nlayer,nq,pplay,pplev, pt,pq,aerosol, &
523	reffrad,nueffrad,QREFvis3d,QREFir3d, &
524	tau_col,cloudfrac,totcloudfrac,clearsky)
525	endif
526
527
528	!-----------------------------------------------------------------------
529	! Prepare CH4 mixing ratio for radiative transfer
530	IF (methane) then
531	vmrch4(:,:)=0.
532
533	if (ch4fix) then
534	if (vmrch4_proffix) then
535	!! Interpolate on the model vertical grid
536	do ig=1,ngrid
537	CALL interp_line(levdat,vmrdat,Nfine, &
538	zzlay(ig,:)/1000.,vmrch4(ig,:),nlayer)
539	enddo
540	else
541	vmrch4(:,:)=vmrch4fix
542	endif
543	else
544	vmrch4(:,:)=pq(:,:,igcm_ch4_gas)100. &
545	mmol(igcm_n2)/mmol(igcm_ch4_gas)
546	endif
547	ENDIF
548
549	! Prepare NON LTE correction in Pluto atmosphere
550	IF (nlte) then
551	CALL nlte_ch4(ngrid,nlayer,nq,pplay,pplev,pt,vmrch4,&
552	eps_nlte_sw23,eps_nlte_sw33,eps_nlte_lw)
553	ENDIF
554	! Net atmospheric radiative cooling rate from C2H2 (K.s-1):
555	! ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
556	! dtlw_hcn_c2h2=0.
557	if (cooling) then
558	CALL cooling_hcn_c2h2(ngrid,nlayer,pplay,&
559	pt,dtlw_hcn_c2h2)
560	endif
561
562
563	!-----------------------------------------------------------------------
564	do ig=1,ngrid ! Starting Big Loop over every GCM column
565	!-----------------------------------------------------------------------
566
567
568	!=======================================================================
569	! II. Transformation of the GCM variables
570	!=======================================================================
571
572
573	!-----------------------------------------------------------------------
574	! Aerosol optical properties Qext, Qscat and g.
575	! The transformation in the vertical is the same as for temperature.
576	!-----------------------------------------------------------------------
577
578
579	! AF24: for now only consider one aerosol (=haze)
580	if (aerohaze) then
581	do iaer=1,naerkind
582	! Shortwave.
583	do nw=1,L_NSPECTV
584
585	do l=1,nlayer
586
587	temp1=QVISsQREF3d(ig,nlayer+1-l,nw,iaer) &
588	*QREFvis3d(ig,nlayer+1-l,iaer)
589
590	temp2=QVISsQREF3d(ig,max(nlayer-l,1),nw,iaer) &
591	*QREFvis3d(ig,max(nlayer-l,1),iaer)
592
593	qxvaer(2*l,nw,iaer) = temp1
594	qxvaer(2*l+1,nw,iaer)=(temp1+temp2)/2
595
596	temp1=temp1*omegavis3d(ig,nlayer+1-l,nw,iaer)
597	temp2=temp2*omegavis3d(ig,max(nlayer-l,1),nw,iaer)
598
599	qsvaer(2*l,nw,iaer) = temp1
600	qsvaer(2*l+1,nw,iaer)=(temp1+temp2)/2
601
602	temp1=gvis3d(ig,nlayer+1-l,nw,iaer)
603	temp2=gvis3d(ig,max(nlayer-l,1),nw,iaer)
604
605	gvaer(2*l,nw,iaer) = temp1
606	gvaer(2*l+1,nw,iaer)=(temp1+temp2)/2
607
608	end do ! nlayer
609
610	qxvaer(1,nw,iaer)=qxvaer(2,nw,iaer)
611	qxvaer(2*nlayer+1,nw,iaer)=0.
612
613	qsvaer(1,nw,iaer)=qsvaer(2,nw,iaer)
614	qsvaer(2*nlayer+1,nw,iaer)=0.
615
616	gvaer(1,nw,iaer)=gvaer(2,nw,iaer)
617	gvaer(2*nlayer+1,nw,iaer)=0.
618
619	end do ! L_NSPECTV
620
621	do nw=1,L_NSPECTI
622	! Longwave
623	do l=1,nlayer
624
625	temp1=QIRsQREF3d(ig,nlayer+1-l,nw,iaer) &
626	*QREFir3d(ig,nlayer+1-l,iaer)
627
628	temp2=QIRsQREF3d(ig,max(nlayer-l,1),nw,iaer) &
629	*QREFir3d(ig,max(nlayer-l,1),iaer)
630
631	qxiaer(2*l,nw,iaer) = temp1
632	qxiaer(2*l+1,nw,iaer)=(temp1+temp2)/2
633
634	temp1=temp1*omegair3d(ig,nlayer+1-l,nw,iaer)
635	temp2=temp2*omegair3d(ig,max(nlayer-l,1),nw,iaer)
636
637	qsiaer(2*l,nw,iaer) = temp1
638	qsiaer(2*l+1,nw,iaer)=(temp1+temp2)/2
639
640	temp1=gir3d(ig,nlayer+1-l,nw,iaer)
641	temp2=gir3d(ig,max(nlayer-l,1),nw,iaer)
642
643	giaer(2*l,nw,iaer) = temp1
644	giaer(2*l+1,nw,iaer)=(temp1+temp2)/2
645
646	end do ! nlayer
647
648	qxiaer(1,nw,iaer)=qxiaer(2,nw,iaer)
649	qxiaer(2*nlayer+1,nw,iaer)=0.
650
651	qsiaer(1,nw,iaer)=qsiaer(2,nw,iaer)
652	qsiaer(2*nlayer+1,nw,iaer)=0.
653
654	giaer(1,nw,iaer)=giaer(2,nw,iaer)
655	giaer(2*nlayer+1,nw,iaer)=0.
656
657	end do ! L_NSPECTI
658
659	end do ! naerkind
660
661	! Test / Correct for freaky s. s. albedo values.
662	do iaer=1,naerkind
663	do k=1,L_LEVELS
664
665	do nw=1,L_NSPECTV
666	if(qsvaer(k,nw,iaer).gt.1.05*qxvaer(k,nw,iaer))then
667	message='Serious problems with qsvaer values'
668	call abort_physic(subname,message,1)
669	endif
670	if(qsvaer(k,nw,iaer).gt.qxvaer(k,nw,iaer))then
671	qsvaer(k,nw,iaer)=qxvaer(k,nw,iaer)
672	endif
673	end do
674
675	do nw=1,L_NSPECTI
676	if(qsiaer(k,nw,iaer).gt.1.05*qxiaer(k,nw,iaer))then
677	message='Serious problems with qsvaer values'
678	call abort_physic(subname,message,1)
679	endif
680	if(qsiaer(k,nw,iaer).gt.qxiaer(k,nw,iaer))then
681	qsiaer(k,nw,iaer)=qxiaer(k,nw,iaer)
682	endif
683	end do
684
685	end do ! L_LEVELS
686	end do ! naerkind
687	end if ! aerohaze
688
689	!-----------------------------------------------------------------------
690	! Aerosol optical depths
691	!-----------------------------------------------------------------------
692	if (aerohaze) then
693	do iaer=1,naerkind ! a bug was here
694	do k=0,nlayer-1
695
696	pweight=(pplay(ig,L_NLAYRAD-k)-pplev(ig,L_NLAYRAD-k+1))/ &
697	(pplev(ig,L_NLAYRAD-k)-pplev(ig,L_NLAYRAD-k+1))
698	! As 'aerosol' is at reference (visible) wavelenght we scale it as
699	! it will be multplied by qxi/v in optci/v
700	temp=aerosol(ig,L_NLAYRAD-k,iaer)/QREFvis3d(ig,L_NLAYRAD-k,iaer)
701	tauaero(2k+2,iaer)=max(temppweight,0.d0)
702	tauaero(2k+3,iaer)=max(temp-tauaero(2k+2,iaer),0.d0)
703
704	end do
705	! boundary conditions
706	tauaero(1,iaer) = tauaero(2,iaer)
707	!tauaero(1,iaer) = 0.
708	!JL18 at time of testing, the two above conditions gave the same results bit for bit.
709
710	end do ! naerkind
711	else
712	tauaero(:,:)=0
713	end if ! aerohaze
714
715	! Albedo and Emissivity.
716	albi=1-emis(ig) ! Long Wave.
717	DO nw=1,L_NSPECTV ! Short Wave loop.
718	albv(nw)=albedo(ig,nw)
719	ENDDO
720
721	acosz=mu0(ig) ! Cosine of sun incident angle : 3D simulations or local 1D simulations using latitude.
722
723
724	!-----------------------------------------------------------------------
725	! GCS (Generic Condensable Specie) Vapor
726	! If you have GCS tracers and they are : variable & radiatively active
727	!
728	! NC22
729	!-----------------------------------------------------------------------
730
731	if (generic_condensation .or. methane .or. carbox) then
732
733	! IF (methane) then
734
735	! do l=1,nlayer
736	! qvar(2l) = vmrch4(ig,nlayer+1-l)/100. &
737	! mmol(igcm_ch4_gas)/mmol(igcm_n2)
738	! qvar(2*l+1) = ((vmrch4(ig,nlayer+1-l)+vmrch4(ig, &
739	! max(nlayer-l,1)))/2.)/100.* &
740	! mmol(igcm_ch4_gas)/mmol(igcm_n2)
741	! end do
742	! qvar(1)=qvar(2)
743
744	! ELSE
745
746	! For now, only one GCS tracer can be both variable and radiatively active
747	! If you set two GCS tracers, that are variable and radiatively active,
748	! the last one in tracer.def will be chosen as the one that will be vadiatively active
749
750	do iq=1,nq
751
752	call generic_tracer_index(nq,iq,igcm_generic_gas,igcm_generic_ice,call_ice_gas_generic)
753
754	if (call_ice_gas_generic) then ! to call only one time the ice/vap pair of a tracer
755
756	if(varactive)then
757
758	i_var=igcm_generic_gas
759	do l=1,nlayer
760	qvar(2*l) = pq(ig,nlayer+1-l,i_var)
761	qvar(2*l+1) = pq(ig,nlayer+1-l,i_var)
762	!JL13index qvar(2*l+1) = (pq(ig,nlayer+1-l,i_var)+pq(ig,max(nlayer-l,1),i_var))/2
763	!JL13index ! Average approximation as for temperature...
764	end do
765	qvar(1)=qvar(2)
766
767	elseif(varfixed .and. (qvap_deep .ge. 0))then
768
769	do l=1,nlayer ! Here we will assign fixed water vapour profiles globally.
770
771	call Psat_generic(pt(ig,l),pplay(ig,l),metallicity,psat,qsat)
772
773	if (qsat .lt. qvap_deep) then
774	pq_temp(l) = qsat ! fully saturated everywhere
775	else
776	pq_temp(l) = qvap_deep
777	end if
778
779	end do
780
781	do l=1,nlayer
782	qvar(2*l) = pq_temp(nlayer+1-l)
783	qvar(2*l+1) = (pq_temp(nlayer+1-l)+pq_temp(max(nlayer-l,1)))/2
784	end do
785
786	qvar(1)=qvar(2)
787
788	else
789	do k=1,L_LEVELS
790	qvar(k) = 1.0D-7
791	end do
792	end if ! varactive/varfixed
793
794	endif
795
796	end do ! do iq=1,nq loop on tracers
797
798	end if ! if (generic_condensation)
799
800	!-----------------------------------------------------------------------
801	! No Water vapor and No GCS (Generic Condensable Specie) vapor
802	!-----------------------------------------------------------------------
803
804	if (.not. (generic_condensation .or. methane .or. carbox)) then
805	do k=1,L_LEVELS
806	qvar(k) = 1.0D-7
807	end do
808	end if ! if (.not. generic_condensation)
809
810
811	if(.not.kastprof)then
812	! IMPORTANT: Now convert from kg/kg to mol/mol.
813	do k=1,L_LEVELS
814	if (generic_condensation .or. methane .or. carbox) then
815	do iq=1,nq
816	call generic_tracer_index(nq,iq,igcm_generic_gas,igcm_generic_ice,call_ice_gas_generic)
817	if (call_ice_gas_generic) then ! to call only one time the ice/vap pair of a tracer
818	if(.not. varactive .or. i_var.eq.iq)then
819
820	epsi_generic=constants_epsi_generic(iq)
821
822	qvar(k) = qvar(k)/(epsi_generic+qvar(k)*(1.-epsi_generic))
823	endif
824
825	endif
826	end do ! do iq=1,nq loop on tracers
827	endif
828	end do
829	end if
830
831	!-----------------------------------------------------------------------
832	! kcm mode only !
833	!-----------------------------------------------------------------------
834
835	DO l=1,nlayer
836	muvarrad(2*l) = muvar(ig,nlayer+2-l)
837	muvarrad(2*l+1) = (muvar(ig,nlayer+2-l)+muvar(ig,max(nlayer+1-l,1)))/2
838	END DO
839
840	muvarrad(1) = muvarrad(2)
841	muvarrad(2*nlayer+1)=muvar(ig,1)
842
843	! Keep values inside limits for which we have radiative transfer coefficients !!!
844	if(L_REFVAR.gt.1)then ! (there was a bug here)
845	do k=1,L_LEVELS
846	if(qvar(k).lt.wrefvar(1))then
847	qvar(k)=wrefvar(1)+1.0e-8
848	elseif(qvar(k).gt.wrefvar(L_REFVAR))then
849	qvar(k)=wrefvar(L_REFVAR)-1.0e-8
850	endif
851	end do
852	endif
853
854	!-----------------------------------------------------------------------
855	! Pressure and temperature
856	!-----------------------------------------------------------------------
857
858	DO l=1,nlayer
859	plevrad(2*l) = pplay(ig,nlayer+1-l)/scalep
860	plevrad(2*l+1) = pplev(ig,nlayer+1-l)/scalep
861	tlevrad(2*l) = pt(ig,nlayer+1-l)
862	tlevrad(2*l+1) = (pt(ig,nlayer+1-l)+pt(ig,max(nlayer-l,1)))/2
863	END DO
864
865	plevrad(1) = 0.
866	!!plevrad(2) = 0. !! JL18 enabling this line puts the radiative top at p=0 which was the idea before, but does not seem to perform best after all.
867
868	tlevrad(1) = tlevrad(2)
869	tlevrad(2*nlayer+1)=tsurf(ig)
870
871	pmid(1) = pplay(ig,nlayer)/scalep
872	pmid(2) = pmid(1)
873
874	tmid(1) = tlevrad(2)
875	tmid(2) = tmid(1)
876
877	DO l=1,L_NLAYRAD-1
878	tmid(2l+1) = tlevrad(2l+1)
879	tmid(2l+2) = tlevrad(2l+1)
880	pmid(2l+1) = plevrad(2l+1)
881	pmid(2l+2) = plevrad(2l+1)
882	END DO
883	pmid(L_LEVELS) = plevrad(L_LEVELS)
884	tmid(L_LEVELS) = tlevrad(L_LEVELS)
885
886	!!Alternative interpolation:
887	! pmid(3) = pmid(1)
888	! pmid(4) = pmid(1)
889	! tmid(3) = tmid(1)
890	! tmid(4) = tmid(1)
891	! DO l=2,L_NLAYRAD-1
892	! tmid(2l+1) = tlevrad(2l)
893	! tmid(2l+2) = tlevrad(2l)
894	! pmid(2l+1) = plevrad(2l)
895	! pmid(2l+2) = plevrad(2l)
896	! END DO
897	! pmid(L_LEVELS) = plevrad(L_LEVELS-1)
898	! tmid(L_LEVELS) = tlevrad(L_LEVELS-1)
899
900	! Test for out-of-bounds pressure.
901	if(plevrad(3).lt.pgasmin)then
902	print*,'Minimum pressure is outside the radiative'
903	print*,'transfer kmatrix bounds, exiting.'
904	message="Minimum pressure outside of kmatrix bounds"
905	call abort_physic(subname,message,1)
906	elseif(plevrad(L_LEVELS).gt.pgasmax)then
907	print*,'Maximum pressure is outside the radiative'
908	print*,'transfer kmatrix bounds, exiting.'
909	message="Minimum pressure outside of kmatrix bounds"
910	call abort_physic(subname,message,1)
911	endif
912
913	! Test for out-of-bounds temperature.
914	! -- JVO 20 : Also add a sanity test checking that tlevrad is
915	! within Planck function temperature boundaries,
916	! which would cause gfluxi/sfluxi to crash.
917	do k=1,L_LEVELS
918
919	if(tlevrad(k).lt.tgasmin)then
920	print*,'Minimum temperature is outside the radiative'
921	print*,'transfer kmatrix bounds'
922	print*,"k=",k," tlevrad(k)=",tlevrad(k)
923	print*,"tgasmin=",tgasmin
924	if (strictboundcorrk) then
925	message="Minimum temperature outside of kmatrix bounds"
926	call abort_physic(subname,message,1)
927	else
928	print,'**********************************************'
929	print*,'we allow model to continue with tlevrad<tgasmin'
930	print*,' ... we assume we know what you are doing ... '
931	print*,' ... but do not let this happen too often ... '
932	print,'**********************************************'
933	!tlevrad(k)=tgasmin ! Used in the source function !
934	endif
935	elseif(tlevrad(k).gt.tgasmax)then
936	print*,'Maximum temperature is outside the radiative'
937	print*,'transfer kmatrix bounds, exiting.'
938	print*,"k=",k," tlevrad(k)=",tlevrad(k)
939	print*,"tgasmax=",tgasmax
940	if (strictboundcorrk) then
941	message="Maximum temperature outside of kmatrix bounds"
942	call abort_physic(subname,message,1)
943	else
944	print,'**********************************************'
945	print*,'we allow model to continue with tlevrad>tgasmax'
946	print*,' ... we assume we know what you are doing ... '
947	print*,' ... but do not let this happen too often ... '
948	print,'**********************************************'
949	!tlevrad(k)=tgasmax ! Used in the source function !
950	endif
951	endif
952
953	if (tlevrad(k).lt.tplanckmin) then
954	print*,'Minimum temperature is outside the boundaries for'
955	print*,'Planck function integration set in callphys.def, aborting.'
956	print*,"k=",k," tlevrad(k)=",tlevrad(k)
957	print*,"tplanckmin=",tplanckmin
958	message="Minimum temperature outside Planck function bounds - Change tplanckmin in callphys.def"
959	call abort_physic(subname,message,1)
960	else if (tlevrad(k).gt.tplanckmax) then
961	print*,'Maximum temperature is outside the boundaries for'
962	print*,'Planck function integration set in callphys.def, aborting.'
963	print*,"k=",k," tlevrad(k)=",tlevrad(k)
964	print*,"tplanckmax=",tplanckmax
965	message="Maximum temperature outside Planck function bounds - Change tplanckmax in callphys.def"
966	call abort_physic(subname,message,1)
967	endif
968
969	enddo
970
971	do k=1,L_NLAYRAD+1
972	if(tmid(k).lt.tgasmin)then
973	print*,'Minimum temperature is outside the radiative'
974	print*,'transfer kmatrix bounds, exiting.'
975	print*,"k=",k," tmid(k)=",tmid(k)
976	print*,"tgasmin=",tgasmin
977	if (strictboundcorrk) then
978	message="Minimum temperature outside of kmatrix bounds"
979	call abort_physic(subname,message,1)
980	else
981	print,'**********************************************'
982	print*,'we allow model to continue but with tmid=tgasmin'
983	print*,' ... we assume we know what you are doing ... '
984	print*,' ... but do not let this happen too often ... '
985	print,'**********************************************'
986	tmid(k)=tgasmin
987	endif
988	elseif(tmid(k).gt.tgasmax)then
989	print*,'Maximum temperature is outside the radiative'
990	print*,'transfer kmatrix bounds, exiting.'
991	print*,"k=",k," tmid(k)=",tmid(k)
992	print*,"tgasmax=",tgasmax
993	if (strictboundcorrk) then
994	message="Maximum temperature outside of kmatrix bounds"
995	call abort_physic(subname,message,1)
996	else
997	print,'**********************************************'
998	print*,'we allow model to continue but with tmid=tgasmax'
999	print*,' ... we assume we know what you are doing ... '
1000	print*,' ... but do not let this happen too often ... '
1001	print,'**********************************************'
1002	tmid(k)=tgasmax
1003	endif
1004	endif
1005	enddo
1006
1007	!=======================================================================
1008	! III. Calling the main radiative transfer subroutines
1009	!=======================================================================
1010
1011	! ----------------------------------------------------------------
1012	! Recombine reference corrk tables if needed - Added by JVO, 2020.
1013	if (corrk_recombin) then
1014	call call_recombin(ig,nlayer,pq(ig,:,:),pplay(ig,:),pt(ig,:),qvar(:),tmid(:),pmid(:))
1015	endif
1016	! ----------------------------------------------------------------
1017
1018	Cmk= 0.01 * 1.0 / (glat(ig) * mugaz * 1.672621e-27) ! q_main=1.0 assumed.
1019	glat_ig=glat(ig)
1020
1021	!-----------------------------------------------------------------------
1022	! Short Wave Part
1023	!-----------------------------------------------------------------------
1024
1025	if(fract(ig) .ge. 1.0e-4) then ! Only during daylight.
1026	if((ngrid.eq.1).and.(global1d))then
1027	do nw=1,L_NSPECTV
1028	stel_fract(nw)= stel(nw)* 0.25 / acosz ! globally averaged = divide by 4, and we correct for solar zenith angle
1029	end do
1030	else
1031	do nw=1,L_NSPECTV
1032	stel_fract(nw)= stel(nw) * fract(ig)
1033	end do
1034	endif
1035
1036	call optcv(dtauv,tauv,taucumv,plevrad, &
1037	qxvaer,qsvaer,gvaer,wbarv,cosbv,tauray,tauaero, &
1038	tmid,pmid,taugsurf,qvar,muvarrad)
1039
1040	call sfluxv(dtauv,tauv,taucumv,albv,dwnv,wbarv,cosbv, &
1041	acosz,stel_fract,nfluxtopv,fluxtopvdn,nfluxoutv_nu,&
1042	nfluxgndv_nu,nfluxtopv_nu, &
1043	fmnetv,fmnetv_nu,fluxupv,fluxdnv,fzerov,taugsurf)
1044
1045	else ! During the night, fluxes = 0.
1046	nfluxtopv = 0.0d0
1047	fluxtopvdn = 0.0d0
1048	nfluxoutv_nu(:) = 0.0d0
1049	nfluxgndv_nu(:) = 0.0d0
1050	do l=1,L_NLAYRAD
1051	fmnetv(l)=0.0d0
1052	fmnetv_nu(l,:)=0.0d0
1053	fluxupv(l)=0.0d0
1054	fluxdnv(l)=0.0d0
1055	end do
1056	end if
1057
1058
1059	! Equivalent Albedo Calculation (for OUTPUT). MT2015
1060	if(fract(ig) .ge. 1.0e-4) then ! equivalent albedo makes sense only during daylight.
1061	surface_stellar_flux=sum(nfluxgndv_nu(1:L_NSPECTV))
1062	if(surface_stellar_flux .gt. 1.0e-3) then ! equivalent albedo makes sense only if the stellar flux received by the surface is positive.
1063	DO nw=1,L_NSPECTV
1064	albedo_temp(nw)=albedo(ig,nw)*nfluxgndv_nu(nw)
1065	ENDDO
1066	albedo_temp(1:L_NSPECTV)=albedo_temp(1:L_NSPECTV)/surface_stellar_flux
1067	albedo_equivalent(ig)=sum(albedo_temp(1:L_NSPECTV))
1068	else
1069	albedo_equivalent(ig)=0.0 ! Spectrally Integrated Albedo not defined for non-irradiated grid points. So we arbitrary set the equivalent albedo to 0.
1070	endif
1071	else
1072	albedo_equivalent(ig)=0.0 ! Spectrally Integrated Albedo not defined for non-irradiated grid points. So we arbitrary set the equivalent albedo to 0.
1073	endif
1074
1075
1076	!-----------------------------------------------------------------------
1077	! Long Wave Part
1078	!-----------------------------------------------------------------------
1079
1080	call optci(plevrad,tlevrad,dtaui,taucumi, &
1081	qxiaer,qsiaer,giaer,cosbi,wbari,tauaero,tmid,pmid, &
1082	taugsurfi,qvar,muvarrad)
1083
1084	call sfluxi(plevrad,tlevrad,dtaui,taucumi,ubari,albi, &
1085	wnoi,dwni,cosbi,wbari,nfluxtopi,nfluxtopi_nu, &
1086	fmneti,fmneti_nu,fluxupi,fluxdni,fluxupi_nu,fzeroi,taugsurfi)
1087
1088	!-----------------------------------------------------------------------
1089	! Transformation of the correlated-k code outputs
1090	! (into dtlw, dtsw, fluxsurf_lw, fluxsurf_sw, fluxtop_lw, fluxtop_sw)
1091
1092	! Flux incident at the top of the atmosphere
1093	fluxtop_dn(ig)=fluxtopvdn
1094
1095	fluxtop_lw(ig) = real(nfluxtopi)
1096	fluxabs_sw(ig) = real(-nfluxtopv)
1097	fluxsurf_lw(ig) = real(fluxdni(L_NLAYRAD))
1098	fluxsurf_sw(ig) = real(fluxdnv(L_NLAYRAD))
1099
1100	! Flux absorbed by the surface. By MT2015.
1101	fluxsurfabs_sw(ig) = fluxsurf_sw(ig)*(1.-albedo_equivalent(ig))
1102
1103	if(fluxtop_dn(ig).lt.0.0)then
1104	print*,'Achtung! fluxtop_dn has lost the plot!'
1105	print*,'fluxtop_dn=',fluxtop_dn(ig)
1106	print*,'acosz=',acosz
1107	print*,'aerosol=',aerosol(ig,:,:)
1108	print*,'temp= ',pt(ig,:)
1109	print*,'pplay= ',pplay(ig,:)
1110	message="Achtung! fluxtop_dn has lost the plot!"
1111	call abort_physic(subname,message,1)
1112	endif
1113
1114	! Spectral output, for exoplanet observational comparison
1115	if(specOLR)then
1116	do nw=1,L_NSPECTI
1117	OLR_nu(ig,nw)=nfluxtopi_nu(nw)/DWNI(nw) !JL Normalize to the bandwidth
1118	end do
1119	do nw=1,L_NSPECTV
1120	GSR_nu(ig,nw)=nfluxgndv_nu(nw)/DWNV(nw)
1121	OSR_nu(ig,nw)=nfluxoutv_nu(nw)/DWNV(nw) !JL Normalize to the bandwidth
1122	end do
1123	endif
1124
1125	! Finally, the heating rates
1126	DO l=2,L_NLAYRAD
1127	! dtsw(ig,L_NLAYRAD+1-l)=(fmnetv(l)-fmnetv(l-1)) &
1128	! glat(ig)/(cppscalep(plevrad(2l+1)-plevrad(2*l-1)))
1129	dpp = glat(ig)/(cppscalep(plevrad(2l+1)-plevrad(2l-1)))
1130	do nw=1,L_NSPECTV
1131	dtsw_nu(L_NLAYRAD+1-l,nw)= &
1132	(fmnetv_nu(l,nw)-fmnetv_nu(l-1,nw))*dpp
1133	end do
1134
1135	! dtlw(ig,L_NLAYRAD+1-l)=(fmneti(l)-fmneti(l-1)) &
1136	! glat(ig)/(cppscalep(plevrad(2l+1)-plevrad(2*l-1)))
1137	do nw=1,L_NSPECTI
1138	dtlw_nu(L_NLAYRAD+1-l,nw)= &
1139	(fmneti_nu(l,nw)-fmneti_nu(l-1,nw))*dpp
1140	end do
1141	END DO
1142
1143	! These are values at top of atmosphere
1144	! dtsw(ig,L_NLAYRAD)=(fmnetv(1)-nfluxtopv) &
1145	! glat(ig)/(cppscalep*(plevrad(3)-plevrad(2)))
1146	! dtlw(ig,L_NLAYRAD)=(fmneti(1)-nfluxtopi) &
1147	! glat(ig)/(cppscalep*(plevrad(3)-plevrad(2)))
1148	dpp = g/(cppscalep(plevrad(3)-plevrad(1)))
1149	do nw=1,L_NSPECTV
1150	dtsw_nu(L_NLAYRAD,nw)= &
1151	(fmnetv_nu(1,nw)-nfluxtopv_nu(nw))*dpp
1152	end do
1153	do nw=1,L_NSPECTI
1154	dtlw_nu(L_NLAYRAD,nw)= &
1155	(fmneti_nu(1,nw)-nfluxtopi_nu(nw))*dpp
1156	end do
1157
1158	! Optical thickness diagnostics (added by JVO)
1159	if (diagdtau) then
1160	do l=1,L_NLAYRAD
1161	do nw=1,L_NSPECTV
1162	int_dtauv(ig,l,nw) = 0.0d0
1163	DO k=1,L_NGAUSS
1164	! Output exp(-tau) because gweight ponderates exp and not tau itself
1165	int_dtauv(ig,l,nw)= int_dtauv(ig,l,nw) + exp(-dtauv(l,nw,k))*gweight(k)
1166	ENDDO
1167	enddo
1168	do nw=1,L_NSPECTI
1169	int_dtaui(ig,l,nw) = 0.0d0
1170	DO k=1,L_NGAUSS
1171	! Output exp(-tau) because gweight ponderates exp and not tau itself
1172	int_dtaui(ig,l,nw)= int_dtaui(ig,l,nw) + exp(-dtaui(l,nw,k))*gweight(k)
1173	ENDDO
1174	enddo
1175	enddo
1176	endif
1177
1178	! **********************************************************
1179	! NON NLTE correction in Pluto atmosphere
1180	! And conversion of LW spectral heating rates to total rates
1181	! **********************************************************
1182
1183	if (.not.nlte) then
1184	eps_nlte_sw23(ig,:) =1. ! IF no NLTE
1185	eps_nlte_sw33(ig,:) =1. ! IF no NLTE
1186	eps_nlte_lw(ig,:) =1. ! IF no NLTE
1187	endif
1188
1189	do l=1,nlayer
1190
1191	!LW
1192	dtlw(ig,l) =0.
1193	! dtlw_co(ig,l) =0. ! only for diagnostic
1194	do nw=1,L_NSPECTI
1195	! wewei : wavelength in micrometer
1196	if ((wavei(nw).gt.6.).and.(wavei(nw).lt.9)) then
1197	dtlw_nu(l,nw)=dtlw_nu(l,nw)*eps_nlte_lw(ig,l)
1198	else
1199	!dtlw_nu(l,nw)=1.*dtlw_nu(l,nw) ! no CO correction (Strobbel 1996)
1200	dtlw_nu(l,nw)=0.33*dtlw_nu(l,nw) ! CO correction (Strobbel 1996)
1201	! dtlw_co(ig,l)=dtlw_co(ig,l)+ dtlw_nu(l,nw) ! diagnostic
1202	end if
1203	dtlw(ig,l)=dtlw(ig,l)+ dtlw_nu(l,nw) !average now on each wavelength
1204	end do
1205	! adding c2h2 if cooling active
1206	! dtlw(ig,l)=dtlw(ig,l)+dtlw_hcn_c2h2(ig,l)
1207
1208	!SW
1209	dtsw(ig,l) =0.
1210
1211	if (strobel) then
1212
1213	do nw=1,L_NSPECTV
1214	if ((wavev(nw).gt.2).and.(wavev(nw).lt.2.6)) then
1215	dtsw_nu(l,nw)=dtsw_nu(l,nw)*eps_nlte_sw23(ig,l)
1216	elseif ((wavev(nw).gt.3).and.(wavev(nw).lt.3.6)) then
1217	dtsw_nu(l,nw)=dtsw_nu(l,nw)*eps_nlte_sw33(ig,l)
1218	else
1219	dtsw_nu(l,nw)=dtsw_nu(l,nw)
1220	end if
1221	dtsw(ig,l)=dtsw(ig,l)+ dtsw_nu(l,nw)
1222	end do
1223
1224	else ! total heating rates multiplied by nlte coef
1225
1226	do nw=1,L_NSPECTV
1227	dtsw_nu(l,nw)=dtsw_nu(l,nw)*eps_nlte_sw23(ig,l)
1228	dtsw(ig,l)=dtsw(ig,l)+ dtsw_nu(l,nw)
1229	enddo
1230
1231	endif
1232
1233
1234	end do
1235	! **********************************************************
1236
1237
1238	!-----------------------------------------------------------------------
1239	end do ! End of big loop over every GCM column.
1240	!-----------------------------------------------------------------------
1241
1242
1243	!-----------------------------------------------------------------------
1244	! Additional diagnostics
1245	!-----------------------------------------------------------------------
1246
1247	! IR spectral output, for exoplanet observational comparison
1248	if(lastcall.and.(ngrid.eq.1))then ! could disable the 1D output, they are in the diagfi and diagspec... JL12
1249
1250	print*,'Saving scalar quantities in surf_vals.out...'
1251	print*,'psurf = ', pplev(1,1),' Pa'
1252	open(116,file='surf_vals.out')
1253	write(116,*) tsurf(1),pplev(1,1),fluxtop_dn(1), &
1254	real(-nfluxtopv),real(nfluxtopi)
1255	close(116)
1256
1257
1258	! USEFUL COMMENT - Do Not Remove.
1259	!
1260	! if(specOLR)then
1261	! open(117,file='OLRnu.out')
1262	! do nw=1,L_NSPECTI
1263	! write(117,*) OLR_nu(1,nw)
1264	! enddo
1265	! close(117)
1266	!
1267	! open(127,file='OSRnu.out')
1268	! do nw=1,L_NSPECTV
1269	! write(127,*) OSR_nu(1,nw)
1270	! enddo
1271	! close(127)
1272	! endif
1273
1274	! OLR vs altitude: do it as a .txt file.
1275	OLRz=.false.
1276	if(OLRz)then
1277	print*,'saving IR vertical flux for OLRz...'
1278	open(118,file='OLRz_plevs.out')
1279	open(119,file='OLRz.out')
1280	do l=1,L_NLAYRAD
1281	write(118,) plevrad(2l)
1282	do nw=1,L_NSPECTI
1283	write(119,*) fluxupi_nu(l,nw)
1284	enddo
1285	enddo
1286	close(118)
1287	close(119)
1288	endif
1289
1290	endif
1291
1292	! See physiq.F for explanations about CLFvarying. This is temporary.
1293	if (lastcall) then
1294	IF( ALLOCATED( gasi ) ) DEALLOCATE( gasi )
1295	IF( ALLOCATED( gasv ) ) DEALLOCATE( gasv )
1296	!$OMP BARRIER
1297	!$OMP MASTER
1298	IF( ALLOCATED( pgasref ) ) DEALLOCATE( pgasref )
1299	IF( ALLOCATED( tgasref ) ) DEALLOCATE( tgasref )
1300	IF( ALLOCATED( wrefvar ) ) DEALLOCATE( wrefvar )
1301	IF( ALLOCATED( pfgasref ) ) DEALLOCATE( pfgasref )
1302	IF( ALLOCATED( gweight ) ) DEALLOCATE( gweight )
1303	!$OMP END MASTER
1304	!$OMP BARRIER
1305	IF ( ALLOCATED(reffrad)) DEALLOCATE(reffrad)
1306	IF ( ALLOCATED(nueffrad)) DEALLOCATE(nueffrad)
1307	endif
1308
1309
1310	end subroutine callcorrk
1311
1312	END MODULE callcorrk_mod

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