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callcorrk.F90 @ 3094

Last change on this file since 3094 was 3090, checked in by slebonnois, 15 months ago
BdeBatz? : Cleans microphysics and makes few corrections for physics
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1	subroutine callcorrk(ngrid,nlayer,pq,nq,qsurf,zday, &
2	albedo,albedo_equivalent,emis,mu0,pplev,pplay,zzlev, &
3	pt,tsurf,fract,dist_star, &
4	dtlw,dtsw,fluxsurf_lw, &
5	fluxsurf_sw,fluxsurfabs_sw,fluxtop_lw, &
6	fluxabs_sw,fluxtop_dn, &
7	OLR_nu,OSR_nu, &
8	int_dtaui,int_dtauv,popthi,popthv,poptci,poptcv, &
9	lastcall)
10
11	use mod_phys_lmdz_para, only : is_master
12	use radinc_h
13	use radcommon_h
14	use gases_h
15	USE tracer_h
16	use callkeys_mod, only: global1d, szangle
17	use comcstfi_mod, only: pi, mugaz, cpp
18	use callkeys_mod, only: diurnal,tracer,seashaze,corrk_recombin, &
19	strictboundcorrk,specOLR,diagdtau, &
20	tplanckmin,tplanckmax,callclouds,Fcloudy
21	use geometry_mod, only: latitude
22
23	implicit none
24
25	!==================================================================
26	!
27	! Purpose
28	! -------
29	! Solve the radiative transfer using the correlated-k method for
30	! the gaseous absorption and the Toon et al. (1989) method for
31	! scatttering due to aerosols.
32	!
33	! Authors
34	! -------
35	! Emmanuel 01/2001, Forget 09/2001
36	! Robin Wordsworth (2009)
37	!
38	! Modified
39	! --------
40	! Jan Vatant d'Ollone (2018)
41	! --> corrk recombining case
42	! B. de Batz de Trenquelléon (2023)
43	! --> Titan's haze and could optics
44	! --> clear/dark columns method
45	! --> optical diagnostics
46	!
47	!==================================================================
48
49	!-----------------------------------------------------------------------
50	! Declaration of the arguments (INPUT - OUTPUT) on the LMD GCM grid
51	! Layer #1 is the layer near the ground.
52	! Layer #nlayer is the layer at the top.
53	!-----------------------------------------------------------------------
54
55
56	! INPUT
57	INTEGER,INTENT(IN) :: ngrid ! Number of atmospheric columns.
58	INTEGER,INTENT(IN) :: nlayer ! Number of atmospheric layers.
59	REAL,INTENT(IN) :: pq(ngrid,nlayer,nq) ! Tracers (X/kg).
60	INTEGER,INTENT(IN) :: nq ! Number of tracers.
61	REAL,INTENT(IN) :: qsurf(ngrid,nq) ! Tracers on surface (kg.m-2).
62	REAL,INTENT(IN) :: zday ! Time elapsed since Ls=0 (sols).
63	REAL,INTENT(IN) :: albedo(ngrid,L_NSPECTV) ! Spectral Short Wavelengths Albedo. By MT2015
64	REAL,INTENT(IN) :: emis(ngrid) ! Long Wave emissivity.
65	REAL,INTENT(IN) :: mu0(ngrid) ! Cosine of sun incident angle.
66	REAL,INTENT(IN) :: pplev(ngrid,nlayer+1) ! Inter-layer pressure (Pa).
67	REAL,INTENT(IN) :: pplay(ngrid,nlayer) ! Mid-layer pressure (Pa).
68	REAL,INTENT(IN) :: zzlev(ngrid,nlayer+1) ! Altitude at the atmospheric layer boundaries (ref : local surf).
69	REAL,INTENT(IN) :: pt(ngrid,nlayer) ! Air temperature (K).
70	REAL,INTENT(IN) :: tsurf(ngrid) ! Surface temperature (K).
71	REAL,INTENT(IN) :: fract(ngrid) ! Fraction of day.
72	REAL,INTENT(IN) :: dist_star ! Distance star-planet (AU).
73	logical,intent(in) :: lastcall ! Signals last call to physics.
74
75	! OUTPUT
76	REAL,INTENT(OUT) :: dtlw(ngrid,nlayer) ! Heating rate (K/s) due to LW radiation.
77	REAL,INTENT(OUT) :: dtsw(ngrid,nlayer) ! Heating rate (K/s) due to SW radiation.
78	REAL,INTENT(OUT) :: fluxsurf_lw(ngrid) ! Incident LW flux to surf (W/m2).
79	REAL,INTENT(OUT) :: fluxsurf_sw(ngrid) ! Incident SW flux to surf (W/m2)
80	REAL,INTENT(OUT) :: fluxsurfabs_sw(ngrid) ! Absorbed SW flux by the surface (W/m2). By MT2015.
81	REAL,INTENT(OUT) :: fluxtop_lw(ngrid) ! Outgoing LW flux to space (W/m2).
82	REAL,INTENT(OUT) :: fluxabs_sw(ngrid) ! SW flux absorbed by the planet (W/m2).
83	REAL,INTENT(OUT) :: fluxtop_dn(ngrid) ! Incident top of atmosphere SW flux (W/m2).
84	REAL,INTENT(OUT) :: OLR_nu(ngrid,L_NSPECTI) ! Outgoing LW radition in each band (Normalized to the band width (W/m2/cm-1).
85	REAL,INTENT(OUT) :: OSR_nu(ngrid,L_NSPECTV) ! Outgoing SW radition in each band (Normalized to the band width (W/m2/cm-1).
86	REAL,INTENT(OUT) :: albedo_equivalent(ngrid) ! Spectrally Integrated Albedo. For Diagnostic. By MT2015
87	REAL,INTENT(OUT) :: int_dtaui(ngrid,nlayer,L_NSPECTI) ! IR optical thickness of layers within narrowbands for diags ().
88	REAL,INTENT(OUT) :: int_dtauv(ngrid,nlayer,L_NSPECTV) ! VI optical thickness of layers within narrowbands for diags ().
89	! Diagnostics
90	REAL,INTENT(OUT) :: popthi(ngrid,nlayer,L_NSPECTI,5) ! IR optical properties of haze within narrowbands (dtau,tau,k,w,g).
91	REAL,INTENT(OUT) :: popthv(ngrid,nlayer,L_NSPECTV,5) ! VI optical properties of haze within narrowbands (dtau,tau,k,w,g).
92	REAL,INTENT(OUT) :: poptci(ngrid,nlayer,L_NSPECTI,5) ! IR optical properties of haze and clouds within narrowbands (dtau,tau,k,w,g).
93	REAL,INTENT(OUT) :: poptcv(ngrid,nlayer,L_NSPECTV,5) ! VI optical properties of haze and clouds within narrowbands (dtau,tau,k,w,g).
94
95
96
97	!-----------------------------------------------------------------------
98	! Declaration of the variables required by correlated-k subroutines
99	! Numbered from top to bottom (unlike in the GCM)
100	!-----------------------------------------------------------------------
101
102	REAL*8 tmid(L_LEVELS),pmid(L_LEVELS)
103	REAL*8 tlevrad(L_LEVELS),plevrad(L_LEVELS)
104
105	! Optical values for the optci/cv subroutines
106	REAL*8 stel(L_NSPECTV),stel_fract(L_NSPECTV)
107	! IR
108	REAL*8 dtaui(L_NLAYRAD,L_NSPECTI,L_NGAUSS)
109	REAL*8 taucumi(L_LEVELS,L_NSPECTI,L_NGAUSS)
110	REAL*8 wbari(L_NLAYRAD,L_NSPECTI,L_NGAUSS)
111	REAL*8 cosbi(L_NLAYRAD,L_NSPECTI,L_NGAUSS)
112	! VI
113	REAL*8 dtauv(L_NLAYRAD,L_NSPECTV,L_NGAUSS)
114	REAL*8 tauv(L_NLEVRAD,L_NSPECTV,L_NGAUSS)
115	REAL*8 taucumv(L_LEVELS,L_NSPECTV,L_NGAUSS)
116	REAL*8 wbarv(L_NLAYRAD,L_NSPECTV,L_NGAUSS)
117	REAL*8 cosbv(L_NLAYRAD,L_NSPECTV,L_NGAUSS)
118
119	! Temporary optical values for the optci/cv subroutines (clear column)
120	REAL*8 dtaui_cc(L_NLAYRAD,L_NSPECTI,L_NGAUSS)
121	REAL*8 dtauv_cc(L_NLAYRAD,L_NSPECTV,L_NGAUSS)
122	REAL*8 tauv_cc(L_NLEVRAD,L_NSPECTV,L_NGAUSS)
123	REAL*8 taucumi_cc(L_LEVELS,L_NSPECTI,L_NGAUSS)
124	REAL*8 taucumv_cc(L_LEVELS,L_NSPECTV,L_NGAUSS)
125	REAL*8 wbari_cc(L_NLAYRAD,L_NSPECTI,L_NGAUSS)
126	REAL*8 wbarv_cc(L_NLAYRAD,L_NSPECTV,L_NGAUSS)
127	REAL*8 cosbi_cc(L_NLAYRAD,L_NSPECTI,L_NGAUSS)
128	REAL*8 cosbv_cc(L_NLAYRAD,L_NSPECTV,L_NGAUSS)
129	! Temporary optical values for the optci/cv subroutines (dark column)
130	REAL*8 dtaui_dc(L_NLAYRAD,L_NSPECTI,L_NGAUSS)
131	REAL*8 dtauv_dc(L_NLAYRAD,L_NSPECTV,L_NGAUSS)
132	REAL*8 tauv_dc(L_NLEVRAD,L_NSPECTV,L_NGAUSS)
133	REAL*8 taucumi_dc(L_LEVELS,L_NSPECTI,L_NGAUSS)
134	REAL*8 taucumv_dc(L_LEVELS,L_NSPECTV,L_NGAUSS)
135	REAL*8 wbari_dc(L_NLAYRAD,L_NSPECTI,L_NGAUSS)
136	REAL*8 wbarv_dc(L_NLAYRAD,L_NSPECTV,L_NGAUSS)
137	REAL*8 cosbi_dc(L_NLAYRAD,L_NSPECTI,L_NGAUSS)
138	REAL*8 cosbv_dc(L_NLAYRAD,L_NSPECTV,L_NGAUSS)
139
140	! Optical diagnostics
141	REAL*8 popt_hazei(L_LEVELS,L_NSPECTI,3)
142	REAL*8 popt_hazev(L_LEVELS,L_NSPECTV,3)
143	REAL*8 popt_cloudsi(L_LEVELS,L_NSPECTI,3)
144	REAL*8 popt_cloudsv(L_LEVELS,L_NSPECTV,3)
145	! Temporary optical diagnostics (clear column)
146	REAL*8 popt_hazei_cc(L_LEVELS,L_NSPECTI,3)
147	REAL*8 popt_hazev_cc(L_LEVELS,L_NSPECTV,3)
148	REAL*8 popt_cloudsi_cc(L_LEVELS,L_NSPECTI,3)
149	REAL*8 popt_cloudsv_cc(L_LEVELS,L_NSPECTV,3)
150	! Temporary optical diagnostics (dark column)
151	REAL*8 popt_hazei_dc(L_LEVELS,L_NSPECTI,3)
152	REAL*8 popt_hazev_dc(L_LEVELS,L_NSPECTV,3)
153	REAL*8 popt_cloudsi_dc(L_LEVELS,L_NSPECTI,3)
154	REAL*8 popt_cloudsv_dc(L_LEVELS,L_NSPECTV,3)
155
156
157	REAL*8 nfluxtopv,nfluxtopi,nfluxtop,fluxtopvdn
158	REAL*8 nfluxoutv_nu(L_NSPECTV) ! Outgoing band-resolved VI flux at TOA (W/m2).
159	REAL*8 nfluxtopi_nu(L_NSPECTI) ! Net band-resolved IR flux at TOA (W/m2).
160	REAL*8 fluxupi_nu(L_NLAYRAD,L_NSPECTI) ! For 1D diagnostic.
161	REAL*8 fmneti(L_NLAYRAD),fmnetv(L_NLAYRAD)
162	REAL*8 fluxupv(L_NLAYRAD),fluxupi(L_NLAYRAD)
163	REAL*8 fluxdnv(L_NLAYRAD),fluxdni(L_NLAYRAD)
164	REAL*8 albi,acosz
165	REAL*8 albv(L_NSPECTV) ! Spectral Visible Albedo.
166
167	INTEGER ig,l,k,nw,iq,ip,ilay,it,lev2lay,cdcolumn,ng
168
169	LOGICAL found
170
171	real*8 taugsurf(L_NSPECTV,L_NGAUSS-1)
172	real*8 taugsurfi(L_NSPECTI,L_NGAUSS-1)
173
174	! Miscellaneous :
175	character(len=100) :: message
176	character(len=10),parameter :: subname="callcorrk"
177
178	logical OLRz
179	real*8 NFLUXGNDV_nu(L_NSPECTV)
180
181	! Included by MT for albedo calculations.
182	REAL*8 albedo_temp(L_NSPECTV) ! For equivalent albedo calculation.
183	REAL*8 surface_stellar_flux ! Stellar flux reaching the surface. Useful for equivalent albedo calculation.
184
185	! For variable haze
186	REAL*8 seashazefact(L_LEVELS)
187
188	! For muphys optics
189	REAL*8 pqmo(ngrid,nlayer,nmicro) ! Tracers for microphysics optics (X/m2).
190	REAL*8 i2e(ngrid,nlayer) ! int 2 ext factor ( X.kg-1 -> X.m-2 for optics )
191
192	! For corr-k recombining
193	REAL*8 pqr(ngrid,L_PINT,L_REFVAR) ! Tracers for corr-k recombining (mol/mol).
194	REAL*8 fact, tmin, tmax
195
196	LOGICAL usept(L_PINT,L_NTREF) ! mask if pfref grid point will be used
197	INTEGER inflay(L_PINT) ! nearest inferior GCM layer for pfgasref grid points
198
199	!=======================================================================
200	! I. Initialization on every call
201	!=======================================================================
202
203
204	! How much light do we get ?
205	do nw=1,L_NSPECTV
206	stel(nw)=stellarf(nw)/(dist_star**2)
207	end do
208
209	! Convert (microphysical) tracers for optics: X.kg-1 --> X.m-2
210	! NOTE: it should be moved somewhere else: calmufi performs the same kind of
211	! computations... waste of time...
212	i2e(:,1:nlayer) = ( pplev(:,1:nlayer)-pplev(:,2:nlayer+1) ) / gzlat(:,1:nlayer)
213	pqmo(:,:,:) = 0.0
214	DO iq=1,nmicro
215	pqmo(:,:,iq) = pq(:,:,iq)*i2e(:,:)
216	ENDDO
217
218	! Default value for fixed species for whom vmr has been taken
219	! into account while computing high-resolution spectra
220	if (corrk_recombin) pqr(:,:,:) = 1.0
221
222	!-----------------------------------------------------------------------
223	do ig=1,ngrid ! Starting Big Loop over every GCM column
224	!-----------------------------------------------------------------------
225
226	! Recombine reference corr-k if needed
227	if (corrk_recombin) then
228
229	! NB : To have decent CPU time recombining is not done on all gridpoints and wavelenghts but we
230	! calculate a gasi/v_recomb variable on the reference corrk-k T,P grid (only for T,P values
231	! who match the atmospheric conditions ) which is then processed as a standard pre-mix in
232	! optci/v routines, but updated every time tracers on the ref P grid have varied > 1%.
233
234	! Extract tracers for variable radiative species
235	! Also find the nearest GCM layer under each ref pressure
236	do ip=1,L_PINT
237
238	ilay=0
239	found = .false.
240	do l=1,nlayer
241	if ( pplay(ig,l) .gt. 10.0**(pfgasref(ip)+2.0) ) then ! pfgasref=log(p[mbar])
242	found=.true.
243	ilay=l
244	endif
245	enddo
246
247	if (.not. found ) then ! set to min
248	do iq=1,L_REFVAR
249	if ( radvar_mask(iq) ) then
250	pqr(ig,ip,iq) = pq(ig,1,radvar_indx(iq)) / rat_mmol(radvar_indx(iq)-nmicro) ! mol/mol
251	endif
252	enddo
253	else
254	if (ilay==nlayer) then ! set to max
255	do iq=1,L_REFVAR
256	if ( radvar_mask(iq) ) then
257	pqr(ig,ip,iq) = pq(ig,nlayer,radvar_indx(iq)) / rat_mmol(radvar_indx(iq)-nmicro) ! mol/mol
258	endif
259	enddo
260	else ! standard
261	fact = ( 10.0**(pfgasref(ip)+2.0) - pplay(ig,ilay+1) ) / ( pplay(ig,ilay) - pplay(ig,ilay+1) ) ! pfgasref=log(p[mbar])
262	do iq=1,L_REFVAR
263	if ( radvar_mask(iq) ) then
264	pqr(ig,ip,iq) = pq(ig,ilay,radvar_indx(iq))*fact pq(ig,ilay+1,radvar_indx(iq))**(1.0-fact)
265	pqr(ig,ip,iq) = pqr(ig,ip,iq) / rat_mmol(radvar_indx(iq)-nmicro) ! mol/mol
266	endif
267	enddo
268	endif ! if ilay==nlayer
269	endif ! if not found
270
271	inflay(ip) = ilay
272
273	enddo ! ip=1,L_PINT
274
275	! NB : The following usept is a trick to call recombine only for the reference T-P
276	! grid points that are useful given the temperature range at this altitude
277	! It saves a looot of time - JVO 18
278	usept(:,:) = .true.
279	do ip=1,L_PINT-1
280	if ( inflay(ip+1)==nlayer ) then
281	usept(ip,:) = .false.
282	endif
283	if ( inflay(ip) == 0 ) then
284	usept(ip+1:,:) = .false.
285	endif
286	if ( usept(ip,1) ) then ! if not all false
287	tmin = minval(pt(ig,max(inflay(ip+1)+1,1):min(inflay(ip)+1,nlayer)))
288	tmax = maxval(pt(ig,max(inflay(ip+1)+1,1):min(inflay(ip)+1,nlayer)))
289	do it=1,L_NTREF-1
290	if ( tgasref(it+1) .lt. tmin ) then
291	usept(ip,it) = .false.
292	endif
293	enddo
294	do it=2,L_NTREF
295	if ( tgasref(it-1) .gt. tmax ) then
296	usept(ip,it) = .false.
297	endif
298	enddo
299	! in case of out-of-bounds
300	if ( tgasref(1) .lt. tmin ) usept(ip,1) = .true.
301	if ( tgasref(L_NTREF) .gt. tmax ) usept(ip,L_NTREF) = .true.
302	endif
303	enddo ! ip=1,L_PINT-1
304	! deal with last bound
305	if ( inflay(L_PINT-1).ne.0 ) usept(L_PINT,:) = usept(L_PINT-1,:)
306
307
308	do ip=1,L_PINT
309
310	! Recombine k at (useful only!) reference T-P values if tracers or T have enough varied
311	do it=1,L_NTREF
312
313	if ( usept(ip,it) .eqv. .false. ) cycle
314
315	do l=1,L_REFVAR
316	if ( abs( (pqr(ig,ip,l) - pqrold(ip,l)) / max(1.0e-30,pqrold(ip,l))) .GT. 0.01 & ! +- 1%
317	.or. ( useptold(ip,it) .eqv. .false. ) ) then ! in case T change but not the tracers
318	call recombin_corrk( pqr(ig,ip,:),ip,it )
319	exit ! one is enough to trigger the update
320	endif
321	enddo
322
323	enddo
324
325	enddo ! ip=1,L_PINT
326
327	useptold(:,:)=usept(:,:)
328
329	endif ! if corrk_recombin
330
331	!=======================================================================
332	! II. Transformation of the GCM variables
333	!=======================================================================
334
335
336	! Albedo and Emissivity.
337	albi=1-emis(ig) ! Long Wave.
338	DO nw=1,L_NSPECTV ! Short Wave loop.
339	albv(nw)=albedo(ig,nw)
340	ENDDO
341
342	if ((ngrid.eq.1).and.(global1d)) then ! Fixed zenith angle 'szangle' in 1D simulations w/ globally-averaged sunlight.
343	acosz = cos(pi*szangle/180.0)
344	print*,'acosz=',acosz,', szangle=',szangle
345	else
346	acosz=mu0(ig) ! Cosine of sun incident angle : 3D simulations or local 1D simulations using latitude.
347	endif
348
349	!-----------------------------------------------------------------------
350	! Pressure and temperature
351	!-----------------------------------------------------------------------
352
353	DO l=1,nlayer
354	plevrad(2*l) = pplay(ig,nlayer+1-l)/scalep
355	plevrad(2*l+1) = pplev(ig,nlayer+1-l)/scalep
356	tlevrad(2*l) = pt(ig,nlayer+1-l)
357	tlevrad(2*l+1) = (pt(ig,nlayer+1-l)+pt(ig,max(nlayer-l,1)))/2
358	END DO
359
360	plevrad(1) = 0.
361	plevrad(2) = 0. !! Trick to have correct calculations of fluxes in gflux(i/v).F, but the pmid levels are not impacted by this change.
362
363	tlevrad(1) = tlevrad(2)
364	tlevrad(2*nlayer+1)=tsurf(ig)
365
366	pmid(1) = max(pgasmin,0.0001*plevrad(3))
367	pmid(2) = pmid(1)
368
369	tmid(1) = tlevrad(2)
370	tmid(2) = tmid(1)
371
372	DO l=1,L_NLAYRAD-1
373	tmid(2l+1) = tlevrad(2l+1)
374	tmid(2l+2) = tlevrad(2l+1)
375	pmid(2l+1) = plevrad(2l+1)
376	pmid(2l+2) = plevrad(2l+1)
377	END DO
378	pmid(L_LEVELS) = plevrad(L_LEVELS)
379	tmid(L_LEVELS) = tlevrad(L_LEVELS)
380
381	!!Alternative interpolation:
382	! pmid(3) = pmid(1)
383	! pmid(4) = pmid(1)
384	! tmid(3) = tmid(1)
385	! tmid(4) = tmid(1)
386	! DO l=2,L_NLAYRAD-1
387	! tmid(2l+1) = tlevrad(2l)
388	! tmid(2l+2) = tlevrad(2l)
389	! pmid(2l+1) = plevrad(2l)
390	! pmid(2l+2) = plevrad(2l)
391	! END DO
392	! pmid(L_LEVELS) = plevrad(L_LEVELS-1)
393	! tmid(L_LEVELS) = tlevrad(L_LEVELS-1)
394
395	! Test for out-of-bounds pressure.
396	if(plevrad(3).lt.pgasmin)then
397	print*,'Minimum pressure is outside the radiative'
398	print*,'transfer kmatrix bounds, exiting.'
399	call abort
400	elseif(plevrad(L_LEVELS).gt.pgasmax)then
401	print*,'Maximum pressure is outside the radiative'
402	print*,'transfer kmatrix bounds, exiting.'
403	call abort
404	endif
405
406	! Test for out-of-bounds temperature.
407	do k=1,L_LEVELS
408	if(tlevrad(k).lt.tgasmin)then
409	print*,'Minimum temperature is outside the radiative'
410	print*,'transfer kmatrix bounds'
411	print*,"k=",k," tlevrad(k)=",tlevrad(k)
412	print*,"tgasmin=",tgasmin
413	if (strictboundcorrk) then
414	call abort
415	else
416	print,'**********************************************'
417	print*,'we allow model to continue with tlevrad=tgasmin'
418	print*,' ... we assume we know what you are doing ... '
419	print*,' ... but do not let this happen too often ... '
420	print,'**********************************************'
421	!tlevrad(k)=tgasmin
422	endif
423	elseif(tlevrad(k).gt.tgasmax)then
424	! print*,'Maximum temperature is outside the radiative'
425	! print*,'transfer kmatrix bounds, exiting.'
426	! print*,"k=",k," tlevrad(k)=",tlevrad(k)
427	! print*,"tgasmax=",tgasmax
428	if (strictboundcorrk) then
429	call abort
430	else
431	! print,'**********************************************'
432	! print*,'we allow model to continue with tlevrad=tgasmax'
433	! print*,' ... we assume we know what you are doing ... '
434	! print*,' ... but do not let this happen too often ... '
435	! print,'**********************************************'
436	!tlevrad(k)=tgasmax
437	endif
438	endif
439
440	if (tlevrad(k).lt.tplanckmin) then
441	print*,'Minimum temperature is outside the boundaries for'
442	print*,'Planck function integration set in callphys.def, aborting.'
443	print*,"k=",k," tlevrad(k)=",tlevrad(k)
444	print*,"tplanckmin=",tplanckmin
445	message="Minimum temperature outside Planck function bounds - Change tplanckmin in callphys.def"
446	call abort_physic(subname,message,1)
447	else if (tlevrad(k).gt.tplanckmax) then
448	print*,'Maximum temperature is outside the boundaries for'
449	print*,'Planck function integration set in callphys.def, aborting.'
450	print*,"k=",k," tlevrad(k)=",tlevrad(k)
451	print*,"tplanckmax=",tplanckmax
452	message="Maximum temperature outside Planck function bounds - Change tplanckmax in callphys.def"
453	call abort_physic(subname,message,1)
454	endif
455
456	enddo
457
458	do k=1,L_NLAYRAD+1
459	if(tmid(k).lt.tgasmin)then
460	print*,'Minimum temperature is outside the radiative'
461	print*,'transfer kmatrix bounds, exiting.'
462	print*,"k=",k," tmid(k)=",tmid(k)
463	print*,"tgasmin=",tgasmin
464	if (strictboundcorrk) then
465	call abort
466	else
467	print,'**********************************************'
468	print*,'we allow model to continue with tmid=tgasmin'
469	print*,' ... we assume we know what you are doing ... '
470	print*,' ... but do not let this happen too often ... '
471	print,'**********************************************'
472	tmid(k)=tgasmin
473	endif
474	elseif(tmid(k).gt.tgasmax)then
475	! print*,'Maximum temperature is outside the radiative'
476	! print*,'transfer kmatrix bounds, exiting.'
477	! print*,"k=",k," tmid(k)=",tmid(k)
478	! print*,"tgasmax=",tgasmax
479	if (strictboundcorrk) then
480	call abort
481	else
482	! print,'**********************************************'
483	! print*,'we allow model to continue with tmid=tgasmin'
484	! print*,' ... we assume we know what you are doing ... '
485	! print*,' ... but do not let this happen too often ... '
486	! print,'**********************************************'
487	tmid(k)=tgasmax
488	endif
489	endif
490	enddo
491
492	!=======================================================================
493	! III. Calling the main radiative transfer subroutines
494	!=======================================================================
495
496	Cmk(:) = 0.01 * 1.0 / (gzlat(ig,:) * mugaz * 1.672621e-27) ! q_main=1.0 assumed.
497	gzlat_ig(:) = gzlat(ig,:)
498
499	! Compute the haze seasonal modulation factor
500	if (seashaze) call season_haze(zday,latitude(ig),plevrad,seashazefact)
501
502	!-----------------------------------------------------------------------
503	! Short Wave Part
504	!-----------------------------------------------------------------------
505
506	! Clear column :
507	cdcolumn = 0
508	call optcv(pqmo(ig,:,:),nlayer,zzlev(ig,:),plevrad,tmid,pmid, &
509	dtauv_cc,tauv_cc,taucumv_cc,wbarv_cc,cosbv_cc,tauray,taugsurf,seashazefact,&
510	popt_hazev_cc,popt_cloudsv_cc,cdcolumn)
511	! Dark column :
512	cdcolumn = 1
513	call optcv(pqmo(ig,:,:),nlayer,zzlev(ig,:),plevrad,tmid,pmid, &
514	dtauv_dc,tauv_dc,taucumv_dc,wbarv_dc,cosbv_dc,tauray,taugsurf,seashazefact,&
515	popt_hazev_dc,popt_cloudsv_dc,cdcolumn)
516
517	! Mean opacity, ssa and asf :
518	where ((exp(-dtauv_cc(:,:,:)).ge.1.d-40) .and. (exp(-dtauv_dc(:,:,:)).ge.1.d-40))
519	dtauv(:,:,:) = -log((1-Fcloudy)exp(-dtauv_cc(:,:,:)) + Fcloudyexp(-dtauv_dc(:,:,:)))
520	elsewhere
521	dtauv(:,:,:) = dtauv_dc(:,:,:) ! No need to average...
522	endwhere
523	do ng = 1, L_NGAUSS
524	do nw = 1, L_NSPECTV
525	taucumv(1,nw,ng) = 0.0d0
526	do k = 2, L_LEVELS
527	if ((exp(-taucumv_cc(k,nw,ng)).ge.1.d-40) .and. (exp(-taucumv_dc(k,nw,ng)).ge.1.d-40)) then
528	taucumv(k,nw,ng) = taucumv(k-1,nw,ng) - log((1-Fcloudy)exp(-taucumv_cc(k,nw,ng)) + Fcloudyexp(-taucumv_dc(k,nw,ng)))
529	else
530	taucumv(k,nw,ng) = taucumv(k-1,nw,ng) + taucumv_dc(k,nw,ng) ! No need to average...
531	end if
532	end do
533	do l = 1, L_NLAYRAD
534	tauv(l,nw,ng) = taucumv(2*l,nw,ng)
535	end do
536	tauv(l,nw,ng) = taucumv(2*L_NLAYRAD+1,nw,ng)
537	end do
538	end do
539	wbarv = (dtauv_ccwbarv_cc + dtauv_dcwbarv_dc) / (dtauv_cc + dtauv_dc)
540	cosbv = (dtauv_ccwbarv_cccosbv_cc + dtauv_dcwbarv_dccosbv_dc) / (dtauv_ccwbarv_cc + dtauv_dcwbarv_dc)
541
542	! Diagnostics for haze :
543	where (popt_hazev_cc(:,:,1) .lt. 1.d-30)
544	popt_hazev_cc(:,:,1) = 1.d-30
545	endwhere
546	where (popt_hazev_dc(:,:,1) .lt. 1.d-30)
547	popt_hazev_dc(:,:,1) = 1.d-30
548	endwhere
549	popt_hazev(:,:,1) = -log( (1-Fcloudy)exp(-popt_hazev_cc(:,:,1)) + Fcloudyexp(-popt_hazev_dc(:,:,1)) )
550	popt_hazev(:,:,2) = ((popt_hazev_cc(:,:,1)popt_hazev_cc(:,:,2) + popt_hazev_dc(:,:,1)popt_hazev_dc(:,:,2)) &
551	/ (popt_hazev_cc(:,:,1) + popt_hazev_dc(:,:,1)))
552	where ((popt_hazev_cc(:,:,2).gt.0.0D0) .or. (popt_hazev_dc(:,:,2).gt.0.0D0))
553	popt_hazev(:,:,3) = (popt_hazev_cc(:,:,1)popt_hazev_cc(:,:,2)popt_hazev_cc(:,:,3) + popt_hazev_dc(:,:,1)popt_hazev_dc(:,:,2)popt_hazev_dc(:,:,3)) &
554	/ (popt_hazev_cc(:,:,1)popt_hazev_cc(:,:,2) + popt_hazev_dc(:,:,1)popt_hazev_dc(:,:,2))
555	elsewhere
556	popt_hazev(:,:,3) = 0.0D0
557	endwhere
558	! Diagnostics for clouds :
559	if (callclouds) then
560	where (popt_cloudsv_cc(:,:,1) .lt. 1.d-30)
561	popt_cloudsv_cc(:,:,1) = 1.d-30
562	endwhere
563	where (popt_cloudsv_dc(:,:,1) .lt. 1.d-30)
564	popt_cloudsv_dc(:,:,1) = 1.d-30
565	endwhere
566	popt_cloudsv(:,:,1) = -log( (1-Fcloudy)exp(-popt_cloudsv_cc(:,:,1)) + Fcloudyexp(-popt_cloudsv_dc(:,:,1)) )
567	popt_cloudsv(:,:,2) = ((popt_cloudsv_cc(:,:,1)popt_cloudsv_cc(:,:,2) + popt_cloudsv_dc(:,:,1)popt_cloudsv_dc(:,:,2)) &
568	/ (popt_cloudsv_cc(:,:,1) + popt_cloudsv_dc(:,:,1)))
569	where ((popt_cloudsv_cc(:,:,2).gt.0.0D0) .or. (popt_cloudsv_dc(:,:,2).gt.0.0D0))
570	popt_cloudsv(:,:,3) = (popt_cloudsv_cc(:,:,1)popt_cloudsv_cc(:,:,2)popt_cloudsv_cc(:,:,3) + popt_cloudsv_dc(:,:,1)popt_cloudsv_dc(:,:,2)popt_cloudsv_dc(:,:,3)) &
571	/ (popt_cloudsv_cc(:,:,1)popt_cloudsv_cc(:,:,2) + popt_cloudsv_dc(:,:,1)popt_cloudsv_dc(:,:,2))
572	elsewhere
573	popt_cloudsv(:,:,3) = 0.0D0
574	endwhere
575	endif
576
577	if(fract(ig) .ge. 1.0e-4) then ! Only during daylight.
578	if((ngrid.eq.1).and.(global1d))then
579	do nw=1,L_NSPECTV
580	stel_fract(nw)= stel(nw)* 0.25 / acosz ! globally averaged = divide by 4, and we correct for solar zenith angle
581	end do
582	else
583	do nw=1,L_NSPECTV
584	stel_fract(nw)= stel(nw) * fract(ig)
585	end do
586	endif
587	call sfluxv(dtauv,tauv,taucumv,albv,dwnv,wbarv,cosbv, &
588	acosz,stel_fract, &
589	nfluxtopv,fluxtopvdn,nfluxoutv_nu,nfluxgndv_nu, &
590	fmnetv,fluxupv,fluxdnv,fzerov,taugsurf)
591
592	else ! During the night, fluxes = 0.
593	nfluxtopv = 0.0d0
594	fluxtopvdn = 0.0d0
595	nfluxoutv_nu(:) = 0.0d0
596	nfluxgndv_nu(:) = 0.0d0
597	do l=1,L_NLAYRAD
598	fmnetv(l)=0.0d0
599	fluxupv(l)=0.0d0
600	fluxdnv(l)=0.0d0
601	end do
602	end if
603
604
605	! Equivalent Albedo Calculation (for OUTPUT). MT2015
606	if(fract(ig) .ge. 1.0e-4) then ! equivalent albedo makes sense only during daylight.
607	surface_stellar_flux=sum(nfluxgndv_nu(1:L_NSPECTV))
608	if(surface_stellar_flux .gt. 1.0e-3) then ! equivalent albedo makes sense only if the stellar flux received by the surface is positive.
609	DO nw=1,L_NSPECTV
610	albedo_temp(nw)=albedo(ig,nw)*nfluxgndv_nu(nw)
611	ENDDO
612	albedo_temp(1:L_NSPECTV)=albedo_temp(1:L_NSPECTV)/surface_stellar_flux
613	albedo_equivalent(ig)=sum(albedo_temp(1:L_NSPECTV))
614	else
615	albedo_equivalent(ig)=0.0 ! Spectrally Integrated Albedo not defined for non-irradiated grid points. So we arbitrary set the equivalent albedo to 0.
616	endif
617	else
618	albedo_equivalent(ig)=0.0 ! Spectrally Integrated Albedo not defined for non-irradiated grid points. So we arbitrary set the equivalent albedo to 0.
619	endif
620
621
622	!-----------------------------------------------------------------------
623	! Long Wave Part
624	!-----------------------------------------------------------------------
625
626
627	! Clear column :
628	cdcolumn = 0
629	call optci(pqmo(ig,:,:),nlayer,zzlev(ig,:),plevrad,tlevrad,tmid,pmid,&
630	dtaui_cc,taucumi_cc,cosbi_cc,wbari_cc,taugsurfi,seashazefact, &
631	popt_hazei_cc,popt_cloudsi_cc,cdcolumn)
632	! Dark column :
633	cdcolumn = 1
634	call optci(pqmo(ig,:,:),nlayer,zzlev(ig,:),plevrad,tlevrad,tmid,pmid,&
635	dtaui_dc,taucumi_dc,cosbi_dc,wbari_dc,taugsurfi,seashazefact, &
636	popt_hazei_dc,popt_cloudsi_dc,cdcolumn)
637
638	! Mean opacity, ssa and asf :
639	where ((exp(-dtaui_cc(:,:,:)).ge.1.d-40) .and. (exp(-dtaui_dc(:,:,:)).ge.1.d-40))
640	dtaui(:,:,:) = -log((1-Fcloudy)exp(-dtaui_cc(:,:,:)) + Fcloudyexp(-dtaui_dc(:,:,:)))
641	elsewhere
642	dtaui(:,:,:) = dtaui_dc(:,:,:) ! No need to average...
643	endwhere
644	do ng = 1, L_NGAUSS
645	do nw = 1, L_NSPECTI
646	taucumi(1,nw,ng) = 0.0d0
647	do k = 2, L_LEVELS
648	if ((exp(-taucumi_cc(k,nw,ng)).ge.1.d-40) .and. (exp(-taucumi_dc(k,nw,ng)).ge.1.d-40)) then
649	taucumi(k,nw,ng) = taucumi(k-1,nw,ng) - log((1-Fcloudy)exp(-taucumi_cc(k,nw,ng)) + Fcloudyexp(-taucumi_dc(k,nw,ng)))
650	else
651	taucumi(k,nw,ng) = taucumi(k-1,nw,ng) + taucumi_dc(k,nw,ng) ! No need to average...
652	end if
653	end do
654	end do
655	end do
656	where ((wbari_cc.gt.0.0D0) .or. (wbari_dc.gt.0.0D0))
657	wbari = (dtaui_ccwbari_cc + dtaui_dcwbari_dc) / (dtaui_cc + dtaui_dc)
658	cosbi = (dtaui_ccwbari_cccosbi_cc + dtaui_dcwbari_dccosbi_dc) / (dtaui_ccwbari_cc + dtaui_dcwbari_dc)
659	elsewhere
660	wbari = 0.0D0
661	cosbi = 0.0D0
662	endwhere
663
664	! Diagnostics for haze :
665	where (popt_hazei_cc(:,:,1) .lt. 1.d-30)
666	popt_hazei_cc(:,:,1) = 1.d-30
667	endwhere
668	where (popt_hazei_dc(:,:,1) .lt. 1.d-30)
669	popt_hazei_dc(:,:,1) = 1.d-30
670	endwhere
671	popt_hazei(:,:,1) = -log( (1-Fcloudy)exp(-popt_hazei_cc(:,:,1)) + Fcloudyexp(-popt_hazei_dc(:,:,1)) )
672	popt_hazei(:,:,2) = (popt_hazei_cc(:,:,1)popt_hazei_cc(:,:,2) + popt_hazei_dc(:,:,1)popt_hazei_dc(:,:,2)) &
673	/ (popt_hazei_cc(:,:,1) + popt_hazei_dc(:,:,1))
674	where ((popt_hazei_cc(:,:,2).gt.0.0D0) .or. (popt_hazei_dc(:,:,2).gt.0.0D0))
675	popt_hazei(:,:,3) = (popt_hazei_cc(:,:,1)popt_hazei_cc(:,:,2)popt_hazei_cc(:,:,3) + popt_hazei_dc(:,:,1)popt_hazei_dc(:,:,2)popt_hazei_dc(:,:,3)) &
676	/ (popt_hazei_cc(:,:,1)popt_hazei_cc(:,:,2) + popt_hazei_dc(:,:,1)popt_hazei_dc(:,:,2))
677	elsewhere
678	popt_hazei(:,:,3) = 0.0D0
679	endwhere
680	! Diagnostics for clouds :
681	if (callclouds) then
682	where (popt_cloudsi_cc(:,:,1) .lt. 1.d-30)
683	popt_cloudsi_cc(:,:,1) = 1.d-30
684	endwhere
685	where (popt_cloudsi_dc(:,:,1) .lt. 1.d-30)
686	popt_cloudsi_dc(:,:,1) = 1.d-30
687	endwhere
688	popt_cloudsi(:,:,1) = -log( (1-Fcloudy)exp(-popt_cloudsi_cc(:,:,1)) + Fcloudyexp(-popt_cloudsi_dc(:,:,1)) )
689	popt_cloudsi(:,:,2) = ((popt_cloudsi_cc(:,:,1)popt_cloudsi_cc(:,:,2) + popt_cloudsi_dc(:,:,1)popt_cloudsi_dc(:,:,2)) &
690	/ (popt_cloudsi_cc(:,:,1) + popt_cloudsi_dc(:,:,1)))
691	where ((popt_cloudsi_cc(:,:,2).gt.0.0D0) .or. (popt_cloudsi_dc(:,:,2).gt.0.0D0))
692	popt_cloudsi(:,:,3) = (popt_cloudsi_cc(:,:,1)popt_cloudsi_cc(:,:,2)popt_cloudsi_cc(:,:,3) + popt_cloudsi_dc(:,:,1)popt_cloudsi_dc(:,:,2)popt_cloudsi_dc(:,:,3)) &
693	/ (popt_cloudsi_cc(:,:,1)popt_cloudsi_cc(:,:,2) + popt_cloudsi_dc(:,:,1)popt_cloudsi_dc(:,:,2))
694	elsewhere
695	popt_cloudsi(:,:,3) = 0.0D0
696	endwhere
697	endif
698
699	call sfluxi(plevrad,tlevrad,dtaui,taucumi,ubari,albi, &
700	wnoi,dwni,cosbi,wbari,nfluxtopi,nfluxtopi_nu, &
701	fmneti,fluxupi,fluxdni,fluxupi_nu,fzeroi,taugsurfi)
702
703	!-----------------------------------------------------------------------
704	! Transformation of the correlated-k code outputs
705	! (into dtlw, dtsw, fluxsurf_lw, fluxsurf_sw, fluxtop_lw, fluxtop_sw)
706
707	! Flux incident at the top of the atmosphere
708	fluxtop_dn(ig)=fluxtopvdn
709
710	fluxtop_lw(ig) = real(nfluxtopi)
711	fluxabs_sw(ig) = real(-nfluxtopv)
712	fluxsurf_lw(ig) = real(fluxdni(L_NLAYRAD))
713	fluxsurf_sw(ig) = real(fluxdnv(L_NLAYRAD))
714
715	! Flux absorbed by the surface. By MT2015.
716	fluxsurfabs_sw(ig) = fluxsurf_sw(ig)*(1.-albedo_equivalent(ig))
717
718	if(fluxtop_dn(ig).lt.0.0)then
719	print*,'Achtung! fluxtop_dn has lost the plot!'
720	print*,'fluxtop_dn=',fluxtop_dn(ig)
721	print*,'acosz=',acosz
722	print*,'temp= ',pt(ig,:)
723	print*,'pplay= ',pplay(ig,:)
724	call abort
725	endif
726
727	! Spectral output, for exoplanet observational comparison
728	if(specOLR)then
729	do nw=1,L_NSPECTI
730	OLR_nu(ig,nw)=nfluxtopi_nu(nw)/DWNI(nw) !JL Normalize to the bandwidth
731	end do
732	do nw=1,L_NSPECTV
733	!GSR_nu(ig,nw)=nfluxgndv_nu(nw)
734	OSR_nu(ig,nw)=nfluxoutv_nu(nw)/DWNV(nw) !JL Normalize to the bandwidth
735	end do
736	endif
737
738	! Finally, the heating rates
739
740	DO l=2,L_NLAYRAD
741	dtsw(ig,L_NLAYRAD+1-l)=(fmnetv(l)-fmnetv(l-1)) &
742	gzlat(ig,L_NLAYRAD+1-l)/(cppscalep(plevrad(2l+1)-plevrad(2*l-1)))
743	dtlw(ig,L_NLAYRAD+1-l)=(fmneti(l)-fmneti(l-1)) &
744	gzlat(ig,L_NLAYRAD+1-l)/(cppscalep(plevrad(2l+1)-plevrad(2*l-1)))
745	END DO
746
747	! These are values at top of atmosphere
748	dtsw(ig,L_NLAYRAD)=(fmnetv(1)-nfluxtopv) &
749	gzlat(ig,L_NLAYRAD)/(cppscalep*(plevrad(3)-plevrad(1)))
750	dtlw(ig,L_NLAYRAD)=(fmneti(1)-nfluxtopi) &
751	gzlat(ig,L_NLAYRAD)/(cppscalep*(plevrad(3)-plevrad(1)))
752
753
754	! Optical thickness diagnostics (added by JVO)
755	if (diagdtau) then
756	do l=1,L_NLAYRAD
757	do nw=1,L_NSPECTV
758	int_dtauv(ig,l,nw) = 0.0d0
759	DO k=1,L_NGAUSS
760	! Output exp(-tau) because gweight ponderates exp and not tau itself
761	int_dtauv(ig,l,nw)= int_dtauv(ig,l,nw) + exp(-dtauv(l,nw,k))*gweight(k)
762	ENDDO
763	enddo
764	do nw=1,L_NSPECTI
765	int_dtaui(ig,l,nw) = 0.0d0
766	DO k=1,L_NGAUSS
767	! Output exp(-tau) because gweight ponderates exp and not tau itself
768	int_dtaui(ig,l,nw)= int_dtaui(ig,l,nw) + exp(-dtaui(l,nw,k))*gweight(k)
769	ENDDO
770	enddo
771	enddo
772	endif
773
774
775	! Diagnostics : optical properties of haze and clouds (dtau, tau, k, w, g) :
776	do l = 2, L_LEVELS, 2
777	lev2lay = L_NLAYRAD+1 - l/2
778	! Visible :
779	do nw = 1, L_NSPECTV
780	popthv(ig,lev2lay,nw,:) = 0.0d0
781	poptcv(ig,lev2lay,nw,:) = 0.0d0
782	! Optical thickness (dtau) :
783	popthv(ig,lev2lay,nw,1) = (popt_hazev(l,nw,1) + popt_hazev(l+1,nw,1)) / 2.0
784	if (callclouds) then
785	poptcv(ig,lev2lay,nw,1) = (popt_cloudsv(l,nw,1) + popt_cloudsv(l+1,nw,1)) / 2.0
786	endif
787	! Opacity (tau) :
788	do k = L_NLAYRAD, lev2lay, -1
789	popthv(ig,lev2lay,nw,2) = popthv(ig,lev2lay,nw,2) + popthv(ig,k,nw,1)
790	if (callclouds) then
791	poptcv(ig,lev2lay,nw,2) = poptcv(ig,lev2lay,nw,2) + poptcv(ig,k,nw,1)
792	endif
793	enddo
794	! Extinction (k) :
795	popthv(ig,lev2lay,nw,3) = popthv(ig,lev2lay,nw,1) / (zzlev(ig,lev2lay+1) - zzlev(ig,lev2lay))
796	if (callclouds) then
797	poptcv(ig,lev2lay,nw,3) = poptcv(ig,lev2lay,nw,1) / (zzlev(ig,lev2lay+1) - zzlev(ig,lev2lay))
798	endif
799	! Simple Scattering Albedo (w) and Asymmetry Parameter (g) :
800	popthv(ig,lev2lay,nw,4) = (popt_hazev(l,nw,2) + popt_hazev(l+1,nw,2)) / 2.0
801	popthv(ig,lev2lay,nw,5) = (popt_hazev(l,nw,3) + popt_hazev(l+1,nw,3)) / 2.0
802	if (callclouds) then
803	poptcv(ig,lev2lay,nw,4) = (popt_cloudsv(l,nw,2) + popt_cloudsv(l+1,nw,2)) / 2.0
804	poptcv(ig,lev2lay,nw,5) = (popt_cloudsv(l,nw,3) + popt_cloudsv(l+1,nw,3)) / 2.0
805	endif
806	enddo
807	! Infra-Red
808	do nw=1,L_NSPECTI
809	popthi(ig,lev2lay,nw,:) = 0.0d0
810	poptci(ig,lev2lay,nw,:) = 0.0d0
811	! Optical thickness (dtau) :
812	popthi(ig,lev2lay,nw,1) = (popt_hazei(l,nw,1) + popt_hazei(l+1,nw,1)) / 2.0
813	if (callclouds) then
814	poptci(ig,lev2lay,nw,1) = (popt_cloudsi(l,nw,1) + popt_cloudsi(l+1,nw,1)) / 2.0
815	endif
816	! Opacity (tau) :
817	do k = L_NLAYRAD, lev2lay, -1
818	popthi(ig,lev2lay,nw,2) = popthi(ig,lev2lay,nw,2) + popthi(ig,k,nw,1)
819	if (callclouds) then
820	poptci(ig,lev2lay,nw,2) = poptci(ig,lev2lay,nw,2) + poptci(ig,k,nw,1)
821	endif
822	enddo
823	! Extinction (k) :
824	popthi(ig,lev2lay,nw,3) = popthi(ig,lev2lay,nw,1) / (zzlev(ig,lev2lay+1) - zzlev(ig,lev2lay))
825	if (callclouds) then
826	poptci(ig,lev2lay,nw,3) = poptci(ig,lev2lay,nw,1) / (zzlev(ig,lev2lay+1) - zzlev(ig,lev2lay))
827	endif
828	! Simple Scattering Albedo (w) and Asymmetry Parameter (g) :
829	popthi(ig,lev2lay,nw,4) = (popt_hazei(l,nw,2) + popt_hazei(l+1,nw,2)) / 2.0
830	popthi(ig,lev2lay,nw,5) = (popt_hazei(l,nw,3) + popt_hazei(l+1,nw,3)) / 2.0
831	if (callclouds) then
832	poptci(ig,lev2lay,nw,4) = (popt_cloudsi(l,nw,2) + popt_cloudsi(l+1,nw,2)) / 2.0
833	poptci(ig,lev2lay,nw,5) = (popt_cloudsi(l,nw,3) + popt_cloudsi(l+1,nw,3)) / 2.0
834	endif
835	enddo
836	enddo
837
838
839	!-----------------------------------------------------------------------
840	end do ! End of big loop over every GCM column.
841	!-----------------------------------------------------------------------
842
843
844	!-----------------------------------------------------------------------
845	! Additional diagnostics
846	!-----------------------------------------------------------------------
847
848	! IR spectral output, for exoplanet observational comparison
849	if(lastcall.and.(ngrid.eq.1))then ! could disable the 1D output, they are in the diagfi and diagspec... JL12
850
851	print*,'Saving scalar quantities in surf_vals.out...'
852	print*,'psurf = ', pplev(1,1),' Pa'
853	open(116,file='surf_vals.out')
854	write(116,*) tsurf(1),pplev(1,1),fluxtop_dn(1), &
855	real(-nfluxtopv),real(nfluxtopi)
856	close(116)
857
858	! USEFUL COMMENT - Do Not Remove.
859	!
860	! if(specOLR)then
861	! open(117,file='OLRnu.out')
862	! do nw=1,L_NSPECTI
863	! write(117,*) OLR_nu(1,nw)
864	! enddo
865	! close(117)
866	!
867	! open(127,file='OSRnu.out')
868	! do nw=1,L_NSPECTV
869	! write(127,*) OSR_nu(1,nw)
870	! enddo
871	! close(127)
872	! endif
873
874	! OLR vs altitude: do it as a .txt file.
875	OLRz=.false.
876	if(OLRz)then
877	print*,'saving IR vertical flux for OLRz...'
878	open(118,file='OLRz_plevs.out')
879	open(119,file='OLRz.out')
880	do l=1,L_NLAYRAD
881	write(118,) plevrad(2l)
882	do nw=1,L_NSPECTI
883	write(119,*) fluxupi_nu(l,nw)
884	enddo
885	enddo
886	close(118)
887	close(119)
888	endif
889
890	endif
891
892	if (lastcall) then
893	IF( ALLOCATED( gasi ) ) DEALLOCATE( gasi )
894	IF( ALLOCATED( gasv ) ) DEALLOCATE( gasv )
895	IF( ALLOCATED( gasi_recomb ) ) DEALLOCATE( gasi_recomb )
896	IF( ALLOCATED( gasv_recomb ) ) DEALLOCATE( gasv_recomb )
897	IF( ALLOCATED( pqrold ) ) DEALLOCATE( pqrold )
898	IF( ALLOCATED( useptold ) ) DEALLOCATE( useptold )
899	!$OMP BARRIER
900	!$OMP MASTER
901	IF( ALLOCATED( pgasref ) ) DEALLOCATE( pgasref )
902	IF( ALLOCATED( tgasref ) ) DEALLOCATE( tgasref )
903	IF( ALLOCATED( pfgasref ) ) DEALLOCATE( pfgasref )
904	IF( ALLOCATED( gweight ) ) DEALLOCATE( gweight )
905	!$OMP END MASTER
906	!$OMP BARRIER
907	endif
908
909
910	end subroutine callcorrk

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