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callcorrk.F90 @ 3614

Last change on this file since 3614 was 3613, checked in by afalco, 6 days ago
Pluto: fixes for OpenMP. AF
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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,zzlev,tsurf,fract,dist_star,dtau_aer,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,firstcall,lastcall)
16
17	use mod_phys_lmdz_para, only : is_master
18	use radinc_h, only: L_NSPECTV, L_NSPECTI, naerkind, banddir, corrkdir,&
19	L_LEVELS, L_NGAUSS, L_NLEVRAD, L_NLAYRAD, L_REFVAR
20	use radcommon_h, only: wrefvar, Cmk, fzeroi, fzerov, gasi, gasv, &
21	glat_ig, gweight, pfgasref, pgasmax, pgasmin, &
22	pgasref, tgasmax, tgasmin, tgasref, scalep, &
23	ubari, wnoi, stellarf, glat, dwnv, dwni, tauray
24	use datafile_mod, only: datadir
25	use ioipsl_getin_p_mod, only: getin_p
26	use gases_h, only: ngasmx
27	use radii_mod, only : su_aer_radii, haze_reffrad_fix
28	use aerosol_mod, only : iaero_haze
29	use aeropacity_mod, only: aeropacity
30	use aeroptproperties_mod, only: aeroptproperties
31	use tracer_h, only: igcm_ch4_gas,igcm_n2,mmol
32	use comcstfi_mod, only: pi, mugaz, cpp, r, g
33	use callkeys_mod, only: diurnal,tracer,varfixed,satval, &
34	diagdtau,kastprof,strictboundcorrk,specOLR, &
35	tplanckmin,tplanckmax,global1d, &
36	optichaze,haze_radproffix,&
37	methane,carbox,cooling,nlte,strobel,&
38	ch4fix,vmrch4_proffix,vmrch4fix,&
39	callmufi
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 planetwide_mod, only: planetwide_maxval, planetwide_minval
46	use radcommon_h, only: wavev,wavei
47	use mp2m_diagnostics
48	implicit none
49
50	!==================================================================
51	!
52	! Purpose
53	! -------
54	! Solve the radiative transfer using the correlated-k method for
55	! the gaseous absorption and the Toon et al. (1989) method for
56	! scatttering due to aerosols.
57	!
58	! Authors
59	! -------
60	! Emmanuel 01/2001, Forget 09/2001
61	! Robin Wordsworth (2009)
62	!
63	!==================================================================
64
65	!-----------------------------------------------------------------------
66	! Declaration of the arguments (INPUT - OUTPUT) on the LMD GCM grid
67	! Layer #1 is the layer near the ground.
68	! Layer #nlayer is the layer at the top.
69	!-----------------------------------------------------------------------
70
71
72	! INPUT
73	INTEGER,INTENT(IN) :: ngrid ! Number of atmospheric columns.
74	INTEGER,INTENT(IN) :: nlayer ! Number of atmospheric layers.
75	REAL,INTENT(IN) :: pq(ngrid,nlayer,nq) ! Tracers (kg/kg_of_air).
76	INTEGER,INTENT(IN) :: nq ! Number of tracers.
77	REAL,INTENT(IN) :: qsurf(ngrid,nq) ! Tracers on surface (kg.m-2).
78	REAL,INTENT(IN) :: albedo(ngrid,L_NSPECTV) ! Spectral Short Wavelengths Albedo. By MT2015
79	REAL,INTENT(IN) :: emis(ngrid) ! Long Wave emissivity.
80	REAL,INTENT(IN) :: mu0(ngrid) ! Cosine of sun incident angle.
81	REAL,INTENT(IN) :: pplev(ngrid,nlayer+1) ! Inter-layer pressure (Pa).
82	REAL,INTENT(IN) :: pplay(ngrid,nlayer) ! Mid-layer pressure (Pa).
83	REAL,INTENT(IN) :: pt(ngrid,nlayer) ! Air temperature (K).
84	REAL,INTENT(IN) :: zzlay(ngrid,nlayer) ! Mid-layer altitude
85	REAL,INTENT(IN) :: zzlev(ngrid,nlayer) ! Altitude at the layer boundaries.
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	logical,intent(in) :: firstcall ! Signals first call to physics.
91	logical,intent(in) :: lastcall ! Signals last call to physics.
92
93	! OUTPUT
94	REAL,INTENT(OUT) :: dtau_aer(ngrid,nlayer,naerkind) ! Aerosol tau at reference wavelenght.
95	REAL,INTENT(OUT) :: dtlw(ngrid,nlayer) ! Heating rate (K/s) due to LW radiation.
96	REAL,INTENT(OUT) :: dtsw(ngrid,nlayer) ! Heating rate (K/s) due to SW radiation.
97	REAL,INTENT(OUT) :: fluxsurf_lw(ngrid) ! Incident LW flux to surf (W/m2).
98	REAL,INTENT(OUT) :: fluxsurf_sw(ngrid) ! Incident SW flux to surf (W/m2)
99	REAL,INTENT(OUT) :: fluxsurfabs_sw(ngrid) ! Absorbed SW flux by the surface (W/m2). By MT2015.
100	REAL,INTENT(OUT) :: fluxtop_lw(ngrid) ! Outgoing LW flux to space (W/m2).
101	REAL,INTENT(OUT) :: fluxabs_sw(ngrid) ! SW flux absorbed by the planet (W/m2).
102	REAL,INTENT(OUT) :: fluxtop_dn(ngrid) ! Incident top of atmosphere SW flux (W/m2).
103	REAL,INTENT(OUT) :: OLR_nu(ngrid,L_NSPECTI) ! Outgoing LW radiation in each band (Normalized to the band width (W/m2/cm-1).
104	REAL,INTENT(OUT) :: OSR_nu(ngrid,L_NSPECTV) ! Outgoing SW radiation in each band (Normalized to the band width (W/m2/cm-1).
105	REAL,INTENT(OUT) :: GSR_nu(ngrid,L_NSPECTV) ! Surface SW radiation in each band (Normalized to the band width (W/m2/cm-1).
106	REAL,INTENT(OUT) :: tau_col(ngrid) ! Diagnostic from aeropacity.
107	REAL,INTENT(OUT) :: albedo_equivalent(ngrid) ! Spectrally Integrated Albedo. For Diagnostic. By MT2015
108	REAL,INTENT(OUT) :: int_dtaui(ngrid,nlayer,L_NSPECTI) ! VI optical thickness of layers within narrowbands for diags ().
109	REAL,INTENT(OUT) :: int_dtauv(ngrid,nlayer,L_NSPECTV) ! IR optical thickness of layers within narrowbands for diags ().
110
111
112
113
114
115	! Globally varying aerosol optical properties on GCM grid ; not needed everywhere so not in radcommon_h.
116	! made "save" variables so they are allocated once in for all, not because
117	! the values need be saved from a time step to the next
118	REAL,SAVE,ALLOCATABLE :: QVISsQREF3d(:,:,:,:)
119	REAL,SAVE,ALLOCATABLE :: omegaVIS3d(:,:,:,:)
120	REAL,SAVE,ALLOCATABLE :: gVIS3d(:,:,:,:)
121	!$OMP THREADPRIVATE(QVISsQREF3d,omegaVIS3d,gVIS3d)
122	REAL,SAVE,ALLOCATABLE :: QIRsQREF3d(:,:,:,:)
123	REAL,SAVE,ALLOCATABLE :: omegaIR3d(:,:,:,:)
124	REAL,SAVE,ALLOCATABLE :: gIR3d(:,:,:,:)
125	!$OMP THREADPRIVATE(QIRsQREF3d,omegaIR3d,gIR3d)
126
127	! REAL :: omegaREFvis3d(ngrid,nlayer,naerkind)
128	! REAL :: omegaREFir3d(ngrid,nlayer,naerkind) ! not sure of the point of these...
129
130	REAL,ALLOCATABLE,SAVE :: reffrad(:,:,:) ! aerosol effective radius (m)
131	REAL,ALLOCATABLE,SAVE :: nueffrad(:,:,:) ! aerosol effective variance
132	!$OMP THREADPRIVATE(reffrad,nueffrad)
133
134	!-----------------------------------------------------------------------
135	! Declaration of the variables required by correlated-k subroutines
136	! Numbered from top to bottom (unlike in the GCM)
137	!-----------------------------------------------------------------------
138
139	REAL*8 tmid(L_LEVELS),pmid(L_LEVELS)
140	REAL*8 tlevrad(L_LEVELS),plevrad(L_LEVELS)
141
142	! Optical values for the optci/cv subroutines
143	REAL*8 stel(L_NSPECTV),stel_fract(L_NSPECTV)
144	! NB: Arrays below are "save" to avoid reallocating them at every call
145	! not because their content needs be reused from call to the next
146	REAL*8,allocatable,save :: dtaui(:,:,:)
147	REAL*8,allocatable,save :: dtauv(:,:,:)
148	REAL*8,allocatable,save :: cosbv(:,:,:)
149	REAL*8,allocatable,save :: cosbi(:,:,:)
150	REAL*8,allocatable,save :: wbari(:,:,:)
151	REAL*8,allocatable,save :: wbarv(:,:,:)
152	!$OMP THREADPRIVATE(dtaui,dtauv,cosbv,cosbi,wbari,wbarv)
153	REAL*8,allocatable,save :: tauv(:,:,:)
154	REAL*8,allocatable,save :: taucumv(:,:,:)
155	REAL*8,allocatable,save :: taucumi(:,:,:)
156	!$OMP THREADPRIVATE(tauv,taucumv,taucumi)
157	REAL*8,allocatable,save :: tauaero(:,:)
158	!$OMP THREADPRIVATE(tauaero)
159	REAL*8 nfluxtopv,nfluxtopi,nfluxtop,fluxtopvdn
160	real*8 nfluxtopv_nu(L_NSPECTV)
161	REAL*8 nfluxoutv_nu(L_NSPECTV) ! Outgoing band-resolved VI flux at TOA (W/m2).
162	REAL*8 nfluxtopi_nu(L_NSPECTI) ! Net band-resolved IR flux at TOA (W/m2).
163	REAL*8 fluxupi_nu(L_NLAYRAD,L_NSPECTI) ! For 1D diagnostic.
164	REAL*8 fmneti(L_NLAYRAD),fmnetv(L_NLAYRAD)
165	real*8 fmneti_nu(L_NLAYRAD,L_NSPECTI) !
166	real*8 fmnetv_nu(L_NLAYRAD,L_NSPECTV) !
167	REAL*8 fluxupv(L_NLAYRAD),fluxupi(L_NLAYRAD)
168	REAL*8 fluxdnv(L_NLAYRAD),fluxdni(L_NLAYRAD)
169	REAL*8 albi,acosz
170	REAL*8 albv(L_NSPECTV) ! Spectral Visible Albedo.
171
172	INTEGER ig,l,k,nw,iaer,iq
173
174	real*8,allocatable,save :: taugsurf(:,:)
175	real*8,allocatable,save :: taugsurfi(:,:)
176	!$OMP THREADPRIVATE(taugsurf,taugsurfi)
177	real*8 qvar(L_LEVELS) ! Mixing ratio of variable component (mol/mol). index 1 is the top of the atmosphere, index L_LEVELS is the bottom
178
179	! Local aerosol optical properties for each column on RADIATIVE grid.
180	real8,save,allocatable :: QXVAER(:,:,:) ! Extinction coeff (QVISsQREFQREFvis)
181	real*8,save,allocatable :: QSVAER(:,:,:)
182	real*8,save,allocatable :: GVAER(:,:,:)
183	real8,save,allocatable :: QXIAER(:,:,:) ! Extinction coeff (QIRsQREFQREFir)
184	real*8,save,allocatable :: QSIAER(:,:,:)
185	real*8,save,allocatable :: GIAER(:,:,:)
186	!$OMP THREADPRIVATE(QXVAER,QSVAER,GVAER,QXIAER,QSIAER,GIAER)
187	real, dimension(:,:,:), save, allocatable :: QREFvis3d
188	real, dimension(:,:,:), save, allocatable :: QREFir3d
189	!$OMP THREADPRIVATE(QREFvis3d,QREFir3d)
190
191	! Miscellaneous :
192	real*8 temp,temp1,temp2,pweight,sig
193	character(len=10) :: tmp1
194	character(len=10) :: tmp2
195	character(len=100) :: message
196	character(len=10),parameter :: subname="callcorrk"
197
198	logical OLRz
199	real*8 NFLUXGNDV_nu(L_NSPECTV)
200
201	! Included by RW for runaway greenhouse 1D study.
202	real vtmp(nlayer)
203	REAL*8 muvarrad(L_LEVELS)
204
205	! Included by MT for albedo calculations.
206	REAL*8 albedo_temp(L_NSPECTV) ! For equivalent albedo calculation.
207	REAL*8 surface_stellar_flux ! Stellar flux reaching the surface. Useful for equivalent albedo calculation.
208
209	! NLTE factor for CH4
210	real eps_nlte_sw23(ngrid,nlayer) ! CH4 NLTE efficiency factor for zdtsw
211	real eps_nlte_sw33(ngrid,nlayer) ! CH4 NLTE efficiency factor for zdtsw
212	real eps_nlte_lw(ngrid,nlayer) ! CH4 NLTE efficiency factor for zdtsw
213	integer Nfine,ifine
214	parameter(Nfine=701)
215	real,save :: levdat(Nfine),vmrdat(Nfine)
216	REAL dtlw_hcn_c2h2(ngrid, nlayer) ! cooling rate (K/s) due to C2H2/HCN (diagnostic)
217	real :: vmrch4(ngrid,nlayer) ! vmr ch4 from vmrch4_proffix
218
219	REAL dtlw_nu(nlayer,L_NSPECTI) ! heating rate (K/s) due to LW in spectral bands
220	REAL dtsw_nu(nlayer,L_NSPECTV) ! heating rate (K/s) due to SW in spectral bands
221
222	! local variable
223	REAL, save :: dpp ! intermediate
224	!$OMP THREADPRIVATE(dpp)
225
226	integer ok ! status (returned by NetCDF functions)
227
228	REAL :: maxvalue,minvalue
229
230	!===============================================================
231	! I.a Initialization on first call
232	!===============================================================
233
234
235	if(firstcall) then
236
237	! test on allocated necessary because of CLFvarying (two calls to callcorrk in physiq)
238	if(.not.allocated(QVISsQREF3d)) then
239	allocate(QVISsQREF3d(ngrid,nlayer,L_NSPECTV,naerkind))
240	endif
241	if(.not.allocated(omegaVIS3d)) then
242	allocate(omegaVIS3d(ngrid,nlayer,L_NSPECTV,naerkind))
243	endif
244	if(.not.allocated(gVIS3d)) then
245	allocate(gVIS3d(ngrid,nlayer,L_NSPECTV,naerkind))
246	endif
247	if (.not.allocated(QIRsQREF3d)) then
248	allocate(QIRsQREF3d(ngrid,nlayer,L_NSPECTI,naerkind))
249	endif
250	if (.not.allocated(omegaIR3d)) then
251	allocate(omegaIR3d(ngrid,nlayer,L_NSPECTI,naerkind))
252	endif
253	if (.not.allocated(gIR3d)) then
254	allocate(gIR3d(ngrid,nlayer,L_NSPECTI,naerkind))
255	endif
256	if (.not.allocated(tauaero)) then
257	allocate(tauaero(L_LEVELS,naerkind))
258	endif
259
260	if(.not.allocated(QXVAER)) then
261	allocate(QXVAER(L_LEVELS,L_NSPECTV,naerkind), stat=ok)
262	if (ok /= 0) then
263	write(,) "memory allocation failed for QXVAER!"
264	call abort_physic(subname,'allocation failure for QXVAER',1)
265	endif
266	endif
267	if(.not.allocated(QSVAER)) then
268	allocate(QSVAER(L_LEVELS,L_NSPECTV,naerkind), stat=ok)
269	if (ok /= 0) then
270	write(,) "memory allocation failed for QSVAER!"
271	call abort_physic(subname,'allocation failure for QSVAER',1)
272	endif
273	endif
274	if(.not.allocated(GVAER)) then
275	allocate(GVAER(L_LEVELS,L_NSPECTV,naerkind), stat=ok)
276	if (ok /= 0) then
277	write(,) "memory allocation failed for GVAER!"
278	call abort_physic(subname,'allocation failure for GVAER',1)
279	endif
280	endif
281	if(.not.allocated(QXIAER)) then
282	allocate(QXIAER(L_LEVELS,L_NSPECTI,naerkind), stat=ok)
283	if (ok /= 0) then
284	write(,) "memory allocation failed for QXIAER!"
285	call abort_physic(subname,'allocation failure for QXIAER',1)
286	endif
287	endif
288	if(.not.allocated(QSIAER)) then
289	allocate(QSIAER(L_LEVELS,L_NSPECTI,naerkind), stat=ok)
290	if (ok /= 0) then
291	write(,) "memory allocation failed for QSIAER!"
292	call abort_physic(subname,'allocation failure for QSIAER',1)
293	endif
294	endif
295	if(.not.allocated(GIAER)) then
296	allocate(GIAER(L_LEVELS,L_NSPECTI,naerkind), stat=ok)
297	if (ok /= 0) then
298	write(,) "memory allocation failed for GIAER!"
299	call abort_physic(subname,'allocation failure for GIAER',1)
300	endif
301	endif
302
303	!!! ALLOCATED instances are necessary because of CLFvarying (strategy to call callcorrk twice in physiq...)
304	IF(.not.ALLOCATED(QREFvis3d))THEN
305	ALLOCATE(QREFvis3d(ngrid,nlayer,naerkind), stat=ok)
306	IF (ok/=0) THEN
307	write(,) "memory allocation failed for QREFvis3d!"
308	call abort_physic(subname,'allocation failure for QREFvis3d',1)
309	ENDIF
310	ENDIF
311	IF(.not.ALLOCATED(QREFir3d)) THEN
312	ALLOCATE(QREFir3d(ngrid,nlayer,naerkind), stat=ok)
313	IF (ok/=0) THEN
314	write(,) "memory allocation failed for QREFir3d!"
315	call abort_physic(subname,'allocation failure for QREFir3d',1)
316	ENDIF
317	ENDIF
318	! Effective radius and variance of the aerosols
319	IF(.not.ALLOCATED(reffrad)) THEN
320	allocate(reffrad(ngrid,nlayer,naerkind), stat=ok)
321	IF (ok/=0) THEN
322	write(,) "memory allocation failed for reffrad!"
323	call abort_physic(subname,'allocation failure for reffrad',1)
324	ENDIF
325	ENDIF
326	IF(.not.ALLOCATED(nueffrad)) THEN
327	allocate(nueffrad(ngrid,nlayer,naerkind), stat=ok)
328	IF (ok/=0) THEN
329	write(,) "memory allocation failed for nueffrad!"
330	call abort_physic(subname,'allocation failure for nueffrad',1)
331	ENDIF
332	ENDIF
333
334	if (is_master) call system('rm -f surf_vals_long.out')
335
336	!--------------------------------------------------
337	! Set up correlated k
338	!--------------------------------------------------
339
340	!this block is now done at firstcall of physiq_mod
341	! print*, "callcorrk: Correlated-k data base folder:",trim(datadir)
342	! call getin_p("corrkdir",corrkdir)
343	! print*, "corrkdir = ",corrkdir
344	! write( tmp1, '(i3)' ) L_NSPECTI
345	! write( tmp2, '(i3)' ) L_NSPECTV
346	! banddir=trim(adjustl(tmp1))//'x'//trim(adjustl(tmp2))
347	! banddir=trim(adjustl(corrkdir))//'/'//trim(adjustl(banddir))
348
349	! call setspi ! Basic infrared properties.
350	! call setspv ! Basic visible properties.
351	! call sugas_corrk ! Set up gaseous absorption properties.
352	! call suaer_corrk ! Set up aerosol optical properties.
353
354
355	! now that L_NGAUSS has been initialized (by sugas_corrk)
356	! allocate related arrays
357	if(.not.allocated(dtaui)) then
358	ALLOCATE(dtaui(L_NLAYRAD,L_NSPECTI,L_NGAUSS), stat=ok)
359	if (ok/=0) then
360	write(,) "memory allocation failed for dtaui!"
361	call abort_physic(subname,'allocation failure for dtaui',1)
362	endif
363	endif
364	if(.not.allocated(dtauv)) then
365	ALLOCATE(dtauv(L_NLAYRAD,L_NSPECTV,L_NGAUSS), stat=ok)
366	if (ok/=0) then
367	write(,) "memory allocation failed for dtauv!"
368	call abort_physic(subname,'allocation failure for dtauv',1)
369	endif
370	endif
371	if(.not.allocated(cosbv)) then
372	ALLOCATE(cosbv(L_NLAYRAD,L_NSPECTV,L_NGAUSS), stat=ok)
373	if (ok/=0) then
374	write(,) "memory allocation failed for cosbv!"
375	call abort_physic(subname,'allocation failure for cobsv',1)
376	endif
377	endif
378	if(.not.allocated(cosbi)) then
379	ALLOCATE(cosbi(L_NLAYRAD,L_NSPECTI,L_NGAUSS), stat=ok)
380	if (ok/=0) then
381	write(,) "memory allocation failed for cosbi!"
382	call abort_physic(subname,'allocation failure for cobsi',1)
383	endif
384	endif
385	if(.not.allocated(wbari)) then
386	ALLOCATE(wbari(L_NLAYRAD,L_NSPECTI,L_NGAUSS), stat=ok)
387	if (ok/=0) then
388	write(,) "memory allocation failed for wbari!"
389	call abort_physic(subname,'allocation failure for wbari',1)
390	endif
391	endif
392	if(.not.allocated(wbarv)) then
393	ALLOCATE(wbarv(L_NLAYRAD,L_NSPECTV,L_NGAUSS), stat=ok)
394	if (ok/=0) then
395	write(,) "memory allocation failed for wbarv!"
396	call abort_physic(subname,'allocation failure for wbarv',1)
397	endif
398	endif
399	if(.not.allocated(tauv)) then
400	ALLOCATE(tauv(L_NLEVRAD,L_NSPECTV,L_NGAUSS), stat=ok)
401	if (ok/=0) then
402	write(,) "memory allocation failed for tauv!"
403	call abort_physic(subname,'allocation failure for tauv',1)
404	endif
405	endif
406	if(.not.allocated(taucumv)) then
407	ALLOCATE(taucumv(L_LEVELS,L_NSPECTV,L_NGAUSS), stat=ok)
408	if (ok/=0) then
409	write(,) "memory allocation failed for taucumv!"
410	call abort_physic(subname,'allocation failure for taucumv',1)
411	endif
412	endif
413	if(.not.allocated(taucumi)) then
414	ALLOCATE(taucumi(L_LEVELS,L_NSPECTI,L_NGAUSS), stat=ok)
415	if (ok/=0) then
416	write(,) "memory allocation failed for taucumi!"
417	call abort_physic(subname,'allocation failure for taucumi',1)
418	endif
419	endif
420	if(.not.allocated(taugsurf)) then
421	ALLOCATE(taugsurf(L_NSPECTV,L_NGAUSS-1), stat=ok)
422	if (ok/=0) then
423	write(,) "memory allocation failed for taugsurf!"
424	call abort_physic(subname,'allocation failure for taugsurf',1)
425	endif
426	endif
427	if(.not.allocated(taugsurfi)) then
428	ALLOCATE(taugsurfi(L_NSPECTI,L_NGAUSS-1), stat=ok)
429	if (ok/=0) then
430	write(,) "memory allocation failed for taugsurfi!"
431	call abort_physic(subname,'allocation failure for taugsurfi',1)
432	endif
433	endif
434
435	end if ! of if (firstcall)
436
437	!=======================================================================
438	! I.b Initialization on every call
439	!=======================================================================
440
441	qxvaer(:,:,:)=0.0
442	qsvaer(:,:,:)=0.0
443	gvaer(:,:,:) =0.0
444
445	qxiaer(:,:,:)=0.0
446	qsiaer(:,:,:)=0.0
447	giaer(:,:,:) =0.0
448
449	OLR_nu(:,:) = 0.
450	OSR_nu(:,:) = 0.
451	GSR_nu(:,:) = 0.
452
453	!--------------------------------------------------
454	! Effective radius and variance of the aerosols
455	!--------------------------------------------------
456	! Radiative Hazes
457	if (optichaze) then
458	if (callmufi) then
459	! Spherical aerosols
460	sig = 0.2
461	where (mp2m_rc_sph(:,:) > 1e-10)
462	reffrad(:,:,1) = mp2m_rc_sph(:,:) * exp(5.sig*2 / 2.)
463	elsewhere
464	reffrad(:,:,1) = 0d0
465	endwhere
466	if (exp(sig**2) - 1 > 0.1) then
467	nueffrad(:,:,1) = exp(sig**2) - 1
468	else
469	nueffrad(:,:,1) = 0.1
470	endif
471	! Fractal aerosols
472	sig = 0.35
473	where (mp2m_rc_fra(:,:) > 1e-10)
474	reffrad(:,:,2) = mp2m_rc_fra(:,:) * exp(5.sig*2 / 2.)
475	elsewhere
476	reffrad(:,:,2) = 0d0
477	endwhere
478	if (exp(sig**2) - 1 > 0.1) then
479	nueffrad(:,:,2) = exp(sig**2) - 1
480	else
481	nueffrad(:,:,2) = 0.1
482	endif
483
484	else
485	do iaer=1,naerkind
486	if ((iaer.eq.iaero_haze)) then
487	call su_aer_radii(ngrid,nlayer,reffrad(1,1,iaer),nueffrad(1,1,iaer))
488	endif
489	end do ! iaer = 1, naerkind.
490	if (haze_radproffix) then
491	call haze_reffrad_fix(ngrid,nlayer,zzlay,reffrad,nueffrad)
492	if (is_master) print*, 'haze_radproffix=T : fixed profile for haze rad'
493	else
494	if (is_master) print*,'reffrad haze:',reffrad(1,1,iaero_haze)
495	if (is_master) print*,'nueff haze',nueffrad(1,1,iaero_haze)
496	endif ! end haze_radproffix
497	endif ! end callmufi
498	endif ! end radiative haze
499
500	! How much light do we get ?
501	do nw=1,L_NSPECTV
502	stel(nw)=stellarf(nw)/(dist_star**2)
503	end do
504
505	if (optichaze) then
506
507	! Get 3D aerosol optical properties.
508	call aeroptproperties(ngrid,nlayer,reffrad,nueffrad, &
509	QVISsQREF3d,omegaVIS3d,gVIS3d, &
510	QIRsQREF3d,omegaIR3d,gIR3d, &
511	QREFvis3d,QREFir3d)
512
513	! Get aerosol optical depths.
514	call aeropacity(ngrid,nlayer,nq,pplay,pplev,zzlev,pt,pq,dtau_aer, &
515	reffrad,nueffrad,QREFvis3d,QREFir3d, &
516	tau_col)
517	endif
518
519
520	!-----------------------------------------------------------------------
521	! Prepare CH4 mixing ratio for radiative transfer
522	IF (methane) then
523	vmrch4(:,:)=0.
524
525	if (ch4fix) then
526	if (vmrch4_proffix) then
527	!! Interpolate on the model vertical grid
528	do ig=1,ngrid
529	CALL interp_line(levdat,vmrdat,Nfine, &
530	zzlay(ig,:)/1000.,vmrch4(ig,:),nlayer)
531	enddo
532	else
533	vmrch4(:,:)=vmrch4fix
534	endif
535	else
536	vmrch4(:,:)=pq(:,:,igcm_ch4_gas)100. &
537	mmol(igcm_n2)/mmol(igcm_ch4_gas)
538	endif
539	ENDIF
540
541	! Prepare NON LTE correction in Pluto atmosphere
542	IF (nlte) then
543	CALL nlte_ch4(ngrid,nlayer,nq,pplay,pplev,pt,vmrch4,&
544	eps_nlte_sw23,eps_nlte_sw33,eps_nlte_lw)
545	ENDIF
546	! Net atmospheric radiative cooling rate from C2H2 (K.s-1):
547	! ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
548	! dtlw_hcn_c2h2=0.
549	if (cooling) then
550	CALL cooling_hcn_c2h2(ngrid,nlayer,pplay,&
551	pt,dtlw_hcn_c2h2)
552	endif
553
554
555	!-----------------------------------------------------------------------
556	do ig=1,ngrid ! Starting Big Loop over every GCM column
557	!-----------------------------------------------------------------------
558
559
560	!=======================================================================
561	! II. Transformation of the GCM variables
562	!=======================================================================
563
564
565	!-----------------------------------------------------------------------
566	! Aerosol optical properties Qext, Qscat and g.
567	! The transformation in the vertical is the same as for temperature.
568	!-----------------------------------------------------------------------
569
570
571	! AF24: for now only consider one aerosol (=haze)
572	if (optichaze) then
573	do iaer=1,naerkind
574	! Shortwave.
575	do nw=1,L_NSPECTV
576
577	do l=1,nlayer
578
579	temp1=QVISsQREF3d(ig,nlayer+1-l,nw,iaer) &
580	*QREFvis3d(ig,nlayer+1-l,iaer)
581
582	temp2=QVISsQREF3d(ig,max(nlayer-l,1),nw,iaer) &
583	*QREFvis3d(ig,max(nlayer-l,1),iaer)
584
585	qxvaer(2*l,nw,iaer) = temp1
586	qxvaer(2*l+1,nw,iaer)=(temp1+temp2)/2
587
588	temp1=temp1*omegavis3d(ig,nlayer+1-l,nw,iaer)
589	temp2=temp2*omegavis3d(ig,max(nlayer-l,1),nw,iaer)
590
591	qsvaer(2*l,nw,iaer) = temp1
592	qsvaer(2*l+1,nw,iaer)=(temp1+temp2)/2
593
594	temp1=gvis3d(ig,nlayer+1-l,nw,iaer)
595	temp2=gvis3d(ig,max(nlayer-l,1),nw,iaer)
596
597	gvaer(2*l,nw,iaer) = temp1
598	gvaer(2*l+1,nw,iaer)=(temp1+temp2)/2
599
600	end do ! nlayer
601
602	qxvaer(1,nw,iaer)=qxvaer(2,nw,iaer)
603	qxvaer(2*nlayer+1,nw,iaer)=0.
604
605	qsvaer(1,nw,iaer)=qsvaer(2,nw,iaer)
606	qsvaer(2*nlayer+1,nw,iaer)=0.
607
608	gvaer(1,nw,iaer)=gvaer(2,nw,iaer)
609	gvaer(2*nlayer+1,nw,iaer)=0.
610
611	end do ! L_NSPECTV
612
613	do nw=1,L_NSPECTI
614	! Longwave
615	do l=1,nlayer
616
617	temp1=QIRsQREF3d(ig,nlayer+1-l,nw,iaer) &
618	*QREFir3d(ig,nlayer+1-l,iaer)
619
620	temp2=QIRsQREF3d(ig,max(nlayer-l,1),nw,iaer) &
621	*QREFir3d(ig,max(nlayer-l,1),iaer)
622
623	qxiaer(2*l,nw,iaer) = temp1
624	qxiaer(2*l+1,nw,iaer)=(temp1+temp2)/2
625
626	temp1=temp1*omegair3d(ig,nlayer+1-l,nw,iaer)
627	temp2=temp2*omegair3d(ig,max(nlayer-l,1),nw,iaer)
628
629	qsiaer(2*l,nw,iaer) = temp1
630	qsiaer(2*l+1,nw,iaer)=(temp1+temp2)/2
631
632	temp1=gir3d(ig,nlayer+1-l,nw,iaer)
633	temp2=gir3d(ig,max(nlayer-l,1),nw,iaer)
634
635	giaer(2*l,nw,iaer) = temp1
636	giaer(2*l+1,nw,iaer)=(temp1+temp2)/2
637
638	end do ! nlayer
639
640	qxiaer(1,nw,iaer)=qxiaer(2,nw,iaer)
641	qxiaer(2*nlayer+1,nw,iaer)=0.
642
643	qsiaer(1,nw,iaer)=qsiaer(2,nw,iaer)
644	qsiaer(2*nlayer+1,nw,iaer)=0.
645
646	giaer(1,nw,iaer)=giaer(2,nw,iaer)
647	giaer(2*nlayer+1,nw,iaer)=0.
648
649	end do ! L_NSPECTI
650
651	end do ! naerkind
652
653	! Test / Correct for freaky s. s. albedo values.
654	do iaer=1,naerkind
655	do k=1,L_LEVELS
656
657	do nw=1,L_NSPECTV
658	if(qsvaer(k,nw,iaer).gt.1.05*qxvaer(k,nw,iaer))then
659	message='Serious problems with qsvaer values'
660	call abort_physic(subname,message,1)
661	endif
662	if(qsvaer(k,nw,iaer).gt.qxvaer(k,nw,iaer))then
663	qsvaer(k,nw,iaer)=qxvaer(k,nw,iaer)
664	endif
665	end do
666
667	do nw=1,L_NSPECTI
668	if(qsiaer(k,nw,iaer).gt.1.05*qxiaer(k,nw,iaer))then
669	message='Serious problems with qsvaer values'
670	call abort_physic(subname,message,1)
671	endif
672	if(qsiaer(k,nw,iaer).gt.qxiaer(k,nw,iaer))then
673	qsiaer(k,nw,iaer)=qxiaer(k,nw,iaer)
674	endif
675	end do
676
677	end do ! L_LEVELS
678	end do ! naerkind
679	end if ! optichaze
680
681	!-----------------------------------------------------------------------
682	! Aerosol optical depths
683	!-----------------------------------------------------------------------
684	if (optichaze) then
685	do iaer=1,naerkind ! a bug was here
686	do k=0,nlayer-1
687
688	pweight=(pplay(ig,L_NLAYRAD-k)-pplev(ig,L_NLAYRAD-k+1))/ &
689	(pplev(ig,L_NLAYRAD-k)-pplev(ig,L_NLAYRAD-k+1))
690	! As 'dtau_aer' is at reference (visible) wavelenght we scale it as
691	! it will be multplied by qxi/v in optci/v
692	temp=dtau_aer(ig,L_NLAYRAD-k,iaer)/QREFvis3d(ig,L_NLAYRAD-k,iaer)
693	tauaero(2k+2,iaer)=max(temppweight,0.d0)
694	tauaero(2k+3,iaer)=max(temp-tauaero(2k+2,iaer),0.d0)
695
696	end do
697	! boundary conditions
698	tauaero(1,iaer) = tauaero(2,iaer)
699	!tauaero(1,iaer) = 0.
700	!JL18 at time of testing, the two above conditions gave the same results bit for bit.
701
702	end do ! naerkind
703	else
704	tauaero(:,:)=0
705	end if ! optichaze
706
707	! Albedo and Emissivity.
708	albi=1-emis(ig) ! Long Wave.
709	DO nw=1,L_NSPECTV ! Short Wave loop.
710	albv(nw)=albedo(ig,nw)
711	ENDDO
712
713	acosz=mu0(ig) ! Cosine of sun incident angle : 3D simulations or local 1D simulations using latitude.
714
715	!-----------------------------------------------------------------------
716	! Methane Vapor
717	!-----------------------------------------------------------------------
718	if (methane) then
719	do l=1,nlayer
720	qvar(2l) = vmrch4(ig,nlayer+1-l)/100. &
721	mmol(igcm_ch4_gas)/mmol(igcm_n2)
722	qvar(2*l+1) = ((vmrch4(ig,nlayer+1-l)+vmrch4(ig, &
723	max(nlayer-l,1)))/2.)/100.* &
724	mmol(igcm_ch4_gas)/mmol(igcm_n2)
725	end do
726	qvar(1)=qvar(2)
727
728	else
729	do k=1,L_LEVELS
730	qvar(k) = 1.0D-7
731	end do
732	end if ! end methane
733
734	!-----------------------------------------------------------------------
735	! kcm mode only !
736	!-----------------------------------------------------------------------
737
738	DO l=1,nlayer
739	muvarrad(2*l) = muvar(ig,nlayer+2-l)
740	muvarrad(2*l+1) = (muvar(ig,nlayer+2-l)+muvar(ig,max(nlayer+1-l,1)))/2
741	END DO
742
743	muvarrad(1) = muvarrad(2)
744	muvarrad(2*nlayer+1)=muvar(ig,1)
745
746	! Keep values inside limits for which we have radiative transfer coefficients !!!
747	if(L_REFVAR.gt.1)then ! (there was a bug here)
748	do k=1,L_LEVELS
749	if(qvar(k).lt.wrefvar(1))then
750	qvar(k)=wrefvar(1)+1.0e-8
751	elseif(qvar(k).gt.wrefvar(L_REFVAR))then
752	qvar(k)=wrefvar(L_REFVAR)-1.0e-8
753	endif
754	end do
755	endif
756
757	!-----------------------------------------------------------------------
758	! Pressure and temperature
759	!-----------------------------------------------------------------------
760
761	DO l=1,nlayer
762	plevrad(2*l) = pplay(ig,nlayer+1-l)/scalep
763	plevrad(2*l+1) = pplev(ig,nlayer+1-l)/scalep
764	tlevrad(2*l) = pt(ig,nlayer+1-l)
765	tlevrad(2*l+1) = (pt(ig,nlayer+1-l)+pt(ig,max(nlayer-l,1)))/2
766	END DO
767
768	plevrad(1) = 0.
769	!!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.
770
771	tlevrad(1) = tlevrad(2)
772	tlevrad(2*nlayer+1)=tsurf(ig)
773
774	pmid(1) = pplay(ig,nlayer)/scalep
775	pmid(2) = pmid(1)
776
777	tmid(1) = tlevrad(2)
778	tmid(2) = tmid(1)
779
780	DO l=1,L_NLAYRAD-1
781	tmid(2l+1) = tlevrad(2l+1)
782	tmid(2l+2) = tlevrad(2l+1)
783	pmid(2l+1) = plevrad(2l+1)
784	pmid(2l+2) = plevrad(2l+1)
785	END DO
786	pmid(L_LEVELS) = plevrad(L_LEVELS)
787	tmid(L_LEVELS) = tlevrad(L_LEVELS)
788
789	!!Alternative interpolation:
790	! pmid(3) = pmid(1)
791	! pmid(4) = pmid(1)
792	! tmid(3) = tmid(1)
793	! tmid(4) = tmid(1)
794	! DO l=2,L_NLAYRAD-1
795	! tmid(2l+1) = tlevrad(2l)
796	! tmid(2l+2) = tlevrad(2l)
797	! pmid(2l+1) = plevrad(2l)
798	! pmid(2l+2) = plevrad(2l)
799	! END DO
800	! pmid(L_LEVELS) = plevrad(L_LEVELS-1)
801	! tmid(L_LEVELS) = tlevrad(L_LEVELS-1)
802
803	! Test for out-of-bounds pressure.
804	if(plevrad(3).lt.pgasmin)then
805	print*,'Warning: minimum pressure is outside the radiative'
806	print*,'transfer kmatrix bounds, exiting.'
807	print*,'Pressure:', plevrad(3), 'Pa'
808	message="Minimum pressure outside of kmatrix bounds"
809	!call abort_physic(subname,message,1)
810	elseif(plevrad(L_LEVELS).gt.pgasmax)then
811	print*,'Maximum pressure is outside the radiative'
812	print*,'transfer kmatrix bounds, exiting.'
813	message="Minimum pressure outside of kmatrix bounds"
814	call abort_physic(subname,message,1)
815	endif
816
817	! Test for out-of-bounds temperature.
818	! -- JVO 20 : Also add a sanity test checking that tlevrad is
819	! within Planck function temperature boundaries,
820	! which would cause gfluxi/sfluxi to crash.
821	do k=1,L_LEVELS
822
823	if(tlevrad(k).lt.tgasmin)then
824	print*,'Minimum temperature is outside the radiative'
825	print*,'transfer kmatrix bounds'
826	print*,"k=",k," tlevrad(k)=",tlevrad(k)
827	print*,"tgasmin=",tgasmin
828	if (strictboundcorrk) then
829	message="Minimum temperature outside of kmatrix bounds"
830	call abort_physic(subname,message,1)
831	else
832	print,'**********************************************'
833	print*,'we allow model to continue with tlevrad<tgasmin'
834	print*,' ... we assume we know what you are doing ... '
835	print*,' ... but do not let this happen too often ... '
836	print,'**********************************************'
837	!tlevrad(k)=tgasmin ! Used in the source function !
838	endif
839	elseif(tlevrad(k).gt.tgasmax)then
840	print*,'Maximum temperature is outside the radiative'
841	print*,'transfer kmatrix bounds, exiting.'
842	print*,"k=",k," tlevrad(k)=",tlevrad(k)
843	print*,"tgasmax=",tgasmax
844	if (strictboundcorrk) then
845	message="Maximum temperature outside of kmatrix bounds"
846	call abort_physic(subname,message,1)
847	else
848	print,'**********************************************'
849	print*,'we allow model to continue with tlevrad>tgasmax'
850	print*,' ... we assume we know what you are doing ... '
851	print*,' ... but do not let this happen too often ... '
852	print,'**********************************************'
853	!tlevrad(k)=tgasmax ! Used in the source function !
854	endif
855	endif
856
857	if (tlevrad(k).lt.tplanckmin) then
858	print*,'Minimum temperature is outside the boundaries for'
859	print*,'Planck function integration set in callphys.def, aborting.'
860	print*,"k=",k," tlevrad(k)=",tlevrad(k)
861	print*,"tplanckmin=",tplanckmin
862	message="Minimum temperature outside Planck function bounds - Change tplanckmin in callphys.def"
863	call abort_physic(subname,message,1)
864	else if (tlevrad(k).gt.tplanckmax) then
865	print*,'Maximum temperature is outside the boundaries for'
866	print*,'Planck function integration set in callphys.def, aborting.'
867	print*,"k=",k," tlevrad(k)=",tlevrad(k)
868	print*,"tplanckmax=",tplanckmax
869	message="Maximum temperature outside Planck function bounds - Change tplanckmax in callphys.def"
870	call abort_physic(subname,message,1)
871	endif
872
873	enddo
874
875	do k=1,L_NLAYRAD+1
876	if(tmid(k).lt.tgasmin)then
877	print*,'Minimum temperature is outside the radiative'
878	print*,'transfer kmatrix bounds, exiting.'
879	print*,"k=",k," tmid(k)=",tmid(k)
880	print*,"tgasmin=",tgasmin
881	if (strictboundcorrk) then
882	message="Minimum temperature outside of kmatrix bounds"
883	call abort_physic(subname,message,1)
884	else
885	print,'**********************************************'
886	print*,'we allow model to continue but with tmid=tgasmin'
887	print*,' ... we assume we know what you are doing ... '
888	print*,' ... but do not let this happen too often ... '
889	print,'**********************************************'
890	tmid(k)=tgasmin
891	endif
892	elseif(tmid(k).gt.tgasmax)then
893	print*,'Maximum temperature is outside the radiative'
894	print*,'transfer kmatrix bounds, exiting.'
895	print*,"k=",k," tmid(k)=",tmid(k)
896	print*,"tgasmax=",tgasmax
897	if (strictboundcorrk) then
898	message="Maximum temperature outside of kmatrix bounds"
899	call abort_physic(subname,message,1)
900	else
901	print,'**********************************************'
902	print*,'we allow model to continue but with tmid=tgasmax'
903	print*,' ... we assume we know what you are doing ... '
904	print*,' ... but do not let this happen too often ... '
905	print,'**********************************************'
906	tmid(k)=tgasmax
907	endif
908	endif
909	enddo
910
911	!=======================================================================
912	! III. Calling the main radiative transfer subroutines
913	!=======================================================================
914
915	! ----------------------------------------------------------------
916	! Recombine reference corrk tables if needed - Added by JVO, 2020.
917	if (corrk_recombin) then
918	call call_recombin(ig,nlayer,pq(ig,:,:),pplay(ig,:),pt(ig,:),qvar(:),tmid(:),pmid(:))
919	endif
920	! ----------------------------------------------------------------
921
922	Cmk= 0.01 * 1.0 / (glat(ig) * mugaz * 1.672621e-27) ! q_main=1.0 assumed.
923	glat_ig=glat(ig)
924
925	!-----------------------------------------------------------------------
926	! Short Wave Part
927	!-----------------------------------------------------------------------
928
929	if(fract(ig) .ge. 1.0e-4) then ! Only during daylight.
930	if((ngrid.eq.1).and.(global1d))then
931	do nw=1,L_NSPECTV
932	stel_fract(nw)= stel(nw)* 0.25 / acosz ! globally averaged = divide by 4, and we correct for solar zenith angle
933	end do
934	else
935	do nw=1,L_NSPECTV
936	stel_fract(nw)= stel(nw) * fract(ig)
937	end do
938	endif
939
940	call optcv(dtauv,tauv,taucumv,plevrad, &
941	qxvaer,qsvaer,gvaer,wbarv,cosbv,tauray,tauaero, &
942	tmid,pmid,taugsurf,qvar,muvarrad)
943
944	call sfluxv(dtauv,tauv,taucumv,albv,dwnv,wbarv,cosbv, &
945	acosz,stel_fract,nfluxtopv,fluxtopvdn,nfluxoutv_nu,&
946	nfluxgndv_nu,nfluxtopv_nu, &
947	fmnetv,fmnetv_nu,fluxupv,fluxdnv,fzerov,taugsurf)
948
949	else ! During the night, fluxes = 0.
950	nfluxtopv = 0.0d0
951	fluxtopvdn = 0.0d0
952	nfluxtopv_nu(:) = 0.0d0
953	nfluxoutv_nu(:) = 0.0d0
954	nfluxgndv_nu(:) = 0.0d0
955	fmnetv_nu(:,:)=0.0
956	do l=1,L_NLAYRAD
957	fmnetv(l)=0.0d0
958	fluxupv(l)=0.0d0
959	fluxdnv(l)=0.0d0
960	end do
961	end if
962
963
964	! Equivalent Albedo Calculation (for OUTPUT). MT2015
965	if(fract(ig) .ge. 1.0e-4) then ! equivalent albedo makes sense only during daylight.
966	surface_stellar_flux=sum(nfluxgndv_nu(1:L_NSPECTV))
967	if(surface_stellar_flux .gt. 1.0e-3) then ! equivalent albedo makes sense only if the stellar flux received by the surface is positive.
968	DO nw=1,L_NSPECTV
969	albedo_temp(nw)=albedo(ig,nw)*nfluxgndv_nu(nw)
970	ENDDO
971	albedo_temp(1:L_NSPECTV)=albedo_temp(1:L_NSPECTV)/surface_stellar_flux
972	albedo_equivalent(ig)=sum(albedo_temp(1:L_NSPECTV))
973	else
974	albedo_equivalent(ig)=0.0 ! Spectrally Integrated Albedo not defined for non-irradiated grid points. So we arbitrary set the equivalent albedo to 0.
975	endif
976	else
977	albedo_equivalent(ig)=0.0 ! Spectrally Integrated Albedo not defined for non-irradiated grid points. So we arbitrary set the equivalent albedo to 0.
978	endif
979
980
981	!-----------------------------------------------------------------------
982	! Long Wave Part
983	!-----------------------------------------------------------------------
984
985	call optci(plevrad,tlevrad,dtaui,taucumi, &
986	qxiaer,qsiaer,giaer,cosbi,wbari,tauaero,tmid,pmid, &
987	taugsurfi,qvar,muvarrad)
988
989	call sfluxi(plevrad,tlevrad,dtaui,taucumi,ubari,albi, &
990	wnoi,dwni,cosbi,wbari,nfluxtopi,nfluxtopi_nu, &
991	fmneti,fmneti_nu,fluxupi,fluxdni,fluxupi_nu,fzeroi,taugsurfi)
992
993	!-----------------------------------------------------------------------
994	! Transformation of the correlated-k code outputs
995	! (into dtlw, dtsw, fluxsurf_lw, fluxsurf_sw, fluxtop_lw, fluxtop_sw)
996
997	! Flux incident at the top of the atmosphere
998	fluxtop_dn(ig)=fluxtopvdn
999
1000	fluxtop_lw(ig) = real(nfluxtopi)
1001	fluxabs_sw(ig) = real(-nfluxtopv)
1002	fluxsurf_lw(ig) = real(fluxdni(L_NLAYRAD))
1003	fluxsurf_sw(ig) = real(fluxdnv(L_NLAYRAD))
1004
1005	! Flux absorbed by the surface. By MT2015.
1006	fluxsurfabs_sw(ig) = fluxsurf_sw(ig)*(1.-albedo_equivalent(ig))
1007
1008	if(fluxtop_dn(ig).lt.0.0)then
1009	print*,'Achtung! fluxtop_dn has lost the plot!'
1010	print*,'fluxtop_dn=',fluxtop_dn(ig)
1011	print*,'acosz=',acosz
1012	print*,'dtau_aer=',dtau_aer(ig,:,:)
1013	print*,'temp= ',pt(ig,:)
1014	print*,'pplay= ',pplay(ig,:)
1015	message="Achtung! fluxtop_dn has lost the plot!"
1016	call abort_physic(subname,message,1)
1017	endif
1018
1019	! Spectral output, for exoplanet observational comparison
1020	if(specOLR)then
1021	do nw=1,L_NSPECTI
1022	OLR_nu(ig,nw)=nfluxtopi_nu(nw)/DWNI(nw) !JL Normalize to the bandwidth
1023	end do
1024	do nw=1,L_NSPECTV
1025	GSR_nu(ig,nw)=nfluxgndv_nu(nw)/DWNV(nw)
1026	OSR_nu(ig,nw)=nfluxoutv_nu(nw)/DWNV(nw) !JL Normalize to the bandwidth
1027	end do
1028	endif
1029
1030	! Finally, the heating rates
1031	DO l=2,L_NLAYRAD
1032	! dtsw(ig,L_NLAYRAD+1-l)=(fmnetv(l)-fmnetv(l-1)) &
1033	! glat(ig)/(cppscalep(plevrad(2l+1)-plevrad(2*l-1)))
1034	dpp = glat(ig)/(cppscalep(plevrad(2l+1)-plevrad(2l-1)))
1035	do nw=1,L_NSPECTV
1036	dtsw_nu(L_NLAYRAD+1-l,nw)= &
1037	(fmnetv_nu(l,nw)-fmnetv_nu(l-1,nw))*dpp
1038	end do
1039
1040	! dtlw(ig,L_NLAYRAD+1-l)=(fmneti(l)-fmneti(l-1)) &
1041	! glat(ig)/(cppscalep(plevrad(2l+1)-plevrad(2*l-1)))
1042	do nw=1,L_NSPECTI
1043	dtlw_nu(L_NLAYRAD+1-l,nw)= &
1044	(fmneti_nu(l,nw)-fmneti_nu(l-1,nw))*dpp
1045	end do
1046	END DO
1047
1048	! These are values at top of atmosphere
1049	! dtsw(ig,L_NLAYRAD)=(fmnetv(1)-nfluxtopv) &
1050	! glat(ig)/(cppscalep*(plevrad(3)-plevrad(2)))
1051	! dtlw(ig,L_NLAYRAD)=(fmneti(1)-nfluxtopi) &
1052	! glat(ig)/(cppscalep*(plevrad(3)-plevrad(2)))
1053	dpp = g/(cppscalep(plevrad(3)-plevrad(1)))
1054	do nw=1,L_NSPECTV
1055	dtsw_nu(L_NLAYRAD,nw)= &
1056	(fmnetv_nu(1,nw)-nfluxtopv_nu(nw))*dpp
1057	end do
1058	do nw=1,L_NSPECTI
1059	dtlw_nu(L_NLAYRAD,nw)= &
1060	(fmneti_nu(1,nw)-nfluxtopi_nu(nw))*dpp
1061	end do
1062
1063	! Optical thickness diagnostics (added by JVO)
1064	if (diagdtau) then
1065	do l=1,L_NLAYRAD
1066	do nw=1,L_NSPECTV
1067	int_dtauv(ig,l,nw) = 0.0d0
1068	DO k=1,L_NGAUSS
1069	! Output exp(-tau) because gweight ponderates exp and not tau itself
1070	int_dtauv(ig,l,nw)= int_dtauv(ig,l,nw) + exp(-dtauv(l,nw,k))*gweight(k)
1071	ENDDO
1072	enddo
1073	do nw=1,L_NSPECTI
1074	int_dtaui(ig,l,nw) = 0.0d0
1075	DO k=1,L_NGAUSS
1076	! Output exp(-tau) because gweight ponderates exp and not tau itself
1077	int_dtaui(ig,l,nw)= int_dtaui(ig,l,nw) + exp(-dtaui(l,nw,k))*gweight(k)
1078	ENDDO
1079	enddo
1080	enddo
1081	endif
1082
1083	! **********************************************************
1084	! NON NLTE correction in Pluto atmosphere
1085	! And conversion of LW spectral heating rates to total rates
1086	! **********************************************************
1087
1088	if (.not.nlte) then
1089	eps_nlte_sw23(ig,:) =1. ! IF no NLTE
1090	eps_nlte_sw33(ig,:) =1. ! IF no NLTE
1091	eps_nlte_lw(ig,:) =1. ! IF no NLTE
1092	endif
1093
1094	do l=1,nlayer
1095
1096	!LW
1097	dtlw(ig,l) =0.
1098	! dtlw_co(ig,l) =0. ! only for diagnostic
1099	do nw=1,L_NSPECTI
1100	! wewei : wavelength in micrometer
1101	if ((wavei(nw).gt.6.).and.(wavei(nw).lt.9)) then
1102	dtlw_nu(l,nw)=dtlw_nu(l,nw)*eps_nlte_lw(ig,l)
1103	else
1104	!dtlw_nu(l,nw)=1.*dtlw_nu(l,nw) ! no CO correction (Strobbel 1996)
1105	dtlw_nu(l,nw)=0.33*dtlw_nu(l,nw) ! CO correction (Strobbel 1996)
1106	! dtlw_co(ig,l)=dtlw_co(ig,l)+ dtlw_nu(l,nw) ! diagnostic
1107	end if
1108	dtlw(ig,l)=dtlw(ig,l)+ dtlw_nu(l,nw) !average now on each wavelength
1109	end do
1110	! adding c2h2 if cooling active
1111	dtlw(ig,l)=dtlw(ig,l)+dtlw_hcn_c2h2(ig,l)
1112
1113	!SW
1114	dtsw(ig,l) =0.
1115
1116	if (strobel) then
1117
1118	do nw=1,L_NSPECTV
1119	if ((wavev(nw).gt.2).and.(wavev(nw).lt.2.6)) then
1120	dtsw_nu(l,nw)=dtsw_nu(l,nw)*eps_nlte_sw23(ig,l)
1121	elseif ((wavev(nw).gt.3).and.(wavev(nw).lt.3.6)) then
1122	dtsw_nu(l,nw)=dtsw_nu(l,nw)*eps_nlte_sw33(ig,l)
1123	else
1124	dtsw_nu(l,nw)=dtsw_nu(l,nw)
1125	end if
1126	dtsw(ig,l)=dtsw(ig,l)+ dtsw_nu(l,nw)
1127	end do
1128
1129	else ! total heating rates multiplied by nlte coef
1130
1131	do nw=1,L_NSPECTV
1132	dtsw_nu(l,nw)=dtsw_nu(l,nw)*eps_nlte_sw23(ig,l)
1133	dtsw(ig,l)=dtsw(ig,l)+ dtsw_nu(l,nw)
1134	enddo
1135
1136	endif
1137
1138
1139	end do
1140	! **********************************************************
1141
1142
1143	!-----------------------------------------------------------------------
1144	end do ! End of big loop over every GCM column.
1145	!-----------------------------------------------------------------------
1146
1147
1148	!-----------------------------------------------------------------------
1149	! Additional diagnostics
1150	!-----------------------------------------------------------------------
1151
1152	! IR spectral output, for exoplanet observational comparison
1153	if(lastcall.and.(ngrid.eq.1))then ! could disable the 1D output, they are in the diagfi and diagspec... JL12
1154
1155	print*,'Saving scalar quantities in surf_vals.out...'
1156	print*,'psurf = ', pplev(1,1),' Pa'
1157	open(116,file='surf_vals.out')
1158	write(116,*) tsurf(1),pplev(1,1),fluxtop_dn(1), &
1159	real(-nfluxtopv),real(nfluxtopi)
1160	close(116)
1161
1162
1163	! USEFUL COMMENT - Do Not Remove.
1164	!
1165	! if(specOLR)then
1166	! open(117,file='OLRnu.out')
1167	! do nw=1,L_NSPECTI
1168	! write(117,*) OLR_nu(1,nw)
1169	! enddo
1170	! close(117)
1171	!
1172	! open(127,file='OSRnu.out')
1173	! do nw=1,L_NSPECTV
1174	! write(127,*) OSR_nu(1,nw)
1175	! enddo
1176	! close(127)
1177	! endif
1178
1179	! OLR vs altitude: do it as a .txt file.
1180	OLRz=.false.
1181	if(OLRz)then
1182	print*,'saving IR vertical flux for OLRz...'
1183	open(118,file='OLRz_plevs.out')
1184	open(119,file='OLRz.out')
1185	do l=1,L_NLAYRAD
1186	write(118,) plevrad(2l)
1187	do nw=1,L_NSPECTI
1188	write(119,*) fluxupi_nu(l,nw)
1189	enddo
1190	enddo
1191	close(118)
1192	close(119)
1193	endif
1194
1195	endif
1196
1197	! See physiq.F for explanations about CLFvarying. This is temporary.
1198	if (lastcall) then
1199	IF( ALLOCATED( gasi ) ) DEALLOCATE( gasi )
1200	IF( ALLOCATED( gasv ) ) DEALLOCATE( gasv )
1201	!$OMP BARRIER
1202	!$OMP MASTER
1203	IF( ALLOCATED( pgasref ) ) DEALLOCATE( pgasref )
1204	IF( ALLOCATED( tgasref ) ) DEALLOCATE( tgasref )
1205	IF( ALLOCATED( wrefvar ) ) DEALLOCATE( wrefvar )
1206	IF( ALLOCATED( pfgasref ) ) DEALLOCATE( pfgasref )
1207	IF( ALLOCATED( gweight ) ) DEALLOCATE( gweight )
1208	!$OMP END MASTER
1209	!$OMP BARRIER
1210	IF ( ALLOCATED(reffrad)) DEALLOCATE(reffrad)
1211	IF ( ALLOCATED(nueffrad)) DEALLOCATE(nueffrad)
1212	endif
1213
1214
1215	end subroutine callcorrk
1216
1217	END MODULE callcorrk_mod

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