Context Navigation

callcorrk.F90 @ 2470

Last change on this file since 2470 was 2470, checked in by yjaziri, 4 years ago
Generic GCM: global1d and szangle for 1D simulation moved from callcorrk to callkeys to defined a consistent 1D sza in physiq_mod used also in chemistry + typo YJ
Property svn:executable set to ``*
File size: 42.6 KB

Line
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	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, &
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 watercommon_h, only: psat_water, epsi
26	use datafile_mod, only: datadir
27	use ioipsl_getin_p_mod, only: getin_p
28	use gases_h, only: ngasmx
29	use radii_mod, only : su_aer_radii,co2_reffrad,h2o_reffrad,dust_reffrad,h2so4_reffrad,back2lay_reffrad
30	use aerosol_mod, only : iaero_co2,iaero_h2o,iaero_dust,iaero_h2so4, iaero_back2lay, iaero_aurora
31	use tracer_h, only: igcm_h2o_vap, igcm_h2o_ice, igcm_co2_ice
32	use comcstfi_mod, only: pi, mugaz, cpp
33	use callkeys_mod, only: varactive,diurnal,tracer,water,varfixed,satval,diagdtau, &
34	kastprof,strictboundcorrk,specOLR,CLFvarying, &
35	tplanckmin,tplanckmax,global1d
36	use optcv_mod, only: optcv
37	use optci_mod, only: optci
38	implicit none
39
40	!==================================================================
41	!
42	! Purpose
43	! -------
44	! Solve the radiative transfer using the correlated-k method for
45	! the gaseous absorption and the Toon et al. (1989) method for
46	! scatttering due to aerosols.
47	!
48	! Authors
49	! -------
50	! Emmanuel 01/2001, Forget 09/2001
51	! Robin Wordsworth (2009)
52	!
53	!==================================================================
54
55	!-----------------------------------------------------------------------
56	! Declaration of the arguments (INPUT - OUTPUT) on the LMD GCM grid
57	! Layer #1 is the layer near the ground.
58	! Layer #nlayer is the layer at the top.
59	!-----------------------------------------------------------------------
60
61
62	! INPUT
63	INTEGER,INTENT(IN) :: ngrid ! Number of atmospheric columns.
64	INTEGER,INTENT(IN) :: nlayer ! Number of atmospheric layers.
65	REAL,INTENT(IN) :: pq(ngrid,nlayer,nq) ! Tracers (kg/kg_of_air).
66	INTEGER,INTENT(IN) :: nq ! Number of tracers.
67	REAL,INTENT(IN) :: qsurf(ngrid,nq) ! Tracers on surface (kg.m-2).
68	REAL,INTENT(IN) :: albedo(ngrid,L_NSPECTV) ! Spectral Short Wavelengths Albedo. By MT2015
69	REAL,INTENT(IN) :: emis(ngrid) ! Long Wave emissivity.
70	REAL,INTENT(IN) :: mu0(ngrid) ! Cosine of sun incident angle.
71	REAL,INTENT(IN) :: pplev(ngrid,nlayer+1) ! Inter-layer pressure (Pa).
72	REAL,INTENT(IN) :: pplay(ngrid,nlayer) ! Mid-layer pressure (Pa).
73	REAL,INTENT(IN) :: pt(ngrid,nlayer) ! Air temperature (K).
74	REAL,INTENT(IN) :: tsurf(ngrid) ! Surface temperature (K).
75	REAL,INTENT(IN) :: fract(ngrid) ! Fraction of day.
76	REAL,INTENT(IN) :: dist_star ! Distance star-planet (AU).
77	REAL,INTENT(IN) :: muvar(ngrid,nlayer+1)
78	REAL,INTENT(IN) :: cloudfrac(ngrid,nlayer) ! Fraction of clouds (%).
79	logical,intent(in) :: clearsky
80	logical,intent(in) :: firstcall ! Signals first call to physics.
81	logical,intent(in) :: lastcall ! Signals last call to physics.
82
83	! OUTPUT
84	REAL,INTENT(OUT) :: aerosol(ngrid,nlayer,naerkind) ! Aerosol tau at reference wavelenght.
85	REAL,INTENT(OUT) :: dtlw(ngrid,nlayer) ! Heating rate (K/s) due to LW radiation.
86	REAL,INTENT(OUT) :: dtsw(ngrid,nlayer) ! Heating rate (K/s) due to SW radiation.
87	REAL,INTENT(OUT) :: fluxsurf_lw(ngrid) ! Incident LW flux to surf (W/m2).
88	REAL,INTENT(OUT) :: fluxsurf_sw(ngrid) ! Incident SW flux to surf (W/m2)
89	REAL,INTENT(OUT) :: fluxsurfabs_sw(ngrid) ! Absorbed SW flux by the surface (W/m2). By MT2015.
90	REAL,INTENT(OUT) :: fluxtop_lw(ngrid) ! Outgoing LW flux to space (W/m2).
91	REAL,INTENT(OUT) :: fluxabs_sw(ngrid) ! SW flux absorbed by the planet (W/m2).
92	REAL,INTENT(OUT) :: fluxtop_dn(ngrid) ! Incident top of atmosphere SW flux (W/m2).
93	REAL,INTENT(OUT) :: OLR_nu(ngrid,L_NSPECTI) ! Outgoing LW radition in each band (Normalized to the band width (W/m2/cm-1).
94	REAL,INTENT(OUT) :: OSR_nu(ngrid,L_NSPECTV) ! Outgoing SW radition in each band (Normalized to the band width (W/m2/cm-1).
95	REAL,INTENT(OUT) :: tau_col(ngrid) ! Diagnostic from aeropacity.
96	REAL,INTENT(OUT) :: albedo_equivalent(ngrid) ! Spectrally Integrated Albedo. For Diagnostic. By MT2015
97	REAL,INTENT(OUT) :: totcloudfrac(ngrid) ! Column Fraction of clouds (%).
98	REAL,INTENT(OUT) :: int_dtaui(ngrid,nlayer,L_NSPECTI) ! VI optical thickness of layers within narrowbands for diags ().
99	REAL,INTENT(OUT) :: int_dtauv(ngrid,nlayer,L_NSPECTV) ! IR optical thickness of layers within narrowbands for diags ().
100
101
102
103
104
105	! Globally varying aerosol optical properties on GCM grid ; not needed everywhere so not in radcommon_h.
106	REAL :: QVISsQREF3d(ngrid,nlayer,L_NSPECTV,naerkind)
107	REAL :: omegaVIS3d(ngrid,nlayer,L_NSPECTV,naerkind)
108	REAL :: gVIS3d(ngrid,nlayer,L_NSPECTV,naerkind)
109	REAL :: QIRsQREF3d(ngrid,nlayer,L_NSPECTI,naerkind)
110	REAL :: omegaIR3d(ngrid,nlayer,L_NSPECTI,naerkind)
111	REAL :: gIR3d(ngrid,nlayer,L_NSPECTI,naerkind)
112
113	! REAL :: omegaREFvis3d(ngrid,nlayer,naerkind)
114	! REAL :: omegaREFir3d(ngrid,nlayer,naerkind) ! not sure of the point of these...
115
116	REAL,ALLOCATABLE,SAVE :: reffrad(:,:,:) ! aerosol effective radius (m)
117	REAL,ALLOCATABLE,SAVE :: nueffrad(:,:,:) ! aerosol effective variance
118	!$OMP THREADPRIVATE(reffrad,nueffrad)
119
120	!-----------------------------------------------------------------------
121	! Declaration of the variables required by correlated-k subroutines
122	! Numbered from top to bottom (unlike in the GCM)
123	!-----------------------------------------------------------------------
124
125	REAL*8 tmid(L_LEVELS),pmid(L_LEVELS)
126	REAL*8 tlevrad(L_LEVELS),plevrad(L_LEVELS)
127
128	! Optical values for the optci/cv subroutines
129	REAL*8 stel(L_NSPECTV),stel_fract(L_NSPECTV)
130	! NB: Arrays below are "save" to avoid reallocating them at every call
131	! not because their content needs be reused from call to the next
132	REAL*8,allocatable,save :: dtaui(:,:,:)
133	REAL*8,allocatable,save :: dtauv(:,:,:)
134	REAL*8,allocatable,save :: cosbv(:,:,:)
135	REAL*8,allocatable,save :: cosbi(:,:,:)
136	REAL*8,allocatable,save :: wbari(:,:,:)
137	REAL*8,allocatable,save :: wbarv(:,:,:)
138	!$OMP THREADPRIVATE(dtaui,dtauv,cosbv,cosbi,wbari,wbarv)
139	REAL*8,allocatable,save :: tauv(:,:,:)
140	REAL*8,allocatable,save :: taucumv(:,:,:)
141	REAL*8,allocatable,save :: taucumi(:,:,:)
142	!$OMP THREADPRIVATE(tauv,taucumv,taucumi)
143	REAL*8 tauaero(L_LEVELS,naerkind)
144	REAL*8 nfluxtopv,nfluxtopi,nfluxtop,fluxtopvdn
145	REAL*8 nfluxoutv_nu(L_NSPECTV) ! Outgoing band-resolved VI flux at TOA (W/m2).
146	REAL*8 nfluxtopi_nu(L_NSPECTI) ! Net band-resolved IR flux at TOA (W/m2).
147	REAL*8 fluxupi_nu(L_NLAYRAD,L_NSPECTI) ! For 1D diagnostic.
148	REAL*8 fmneti(L_NLAYRAD),fmnetv(L_NLAYRAD)
149	REAL*8 fluxupv(L_NLAYRAD),fluxupi(L_NLAYRAD)
150	REAL*8 fluxdnv(L_NLAYRAD),fluxdni(L_NLAYRAD)
151	REAL*8 albi,acosz
152	REAL*8 albv(L_NSPECTV) ! Spectral Visible Albedo.
153
154	INTEGER ig,l,k,nw,iaer
155
156	real*8,allocatable,save :: taugsurf(:,:)
157	real*8,allocatable,save :: taugsurfi(:,:)
158	!$OMP THREADPRIVATE(taugsurf,taugsurfi)
159	real*8 qvar(L_LEVELS) ! Mixing ratio of variable component (mol/mol).
160
161	! Local aerosol optical properties for each column on RADIATIVE grid.
162	real8,save,allocatable :: QXVAER(:,:,:) ! Extinction coeff (QVISsQREFQREFvis)
163	real*8,save,allocatable :: QSVAER(:,:,:)
164	real*8,save,allocatable :: GVAER(:,:,:)
165	real8,save,allocatable :: QXIAER(:,:,:) ! Extinction coeff (QIRsQREFQREFir)
166	real*8,save,allocatable :: QSIAER(:,:,:)
167	real*8,save,allocatable :: GIAER(:,:,:)
168	!$OMP THREADPRIVATE(QXVAER,QSVAER,GVAER,QXIAER,QSIAER,GIAER)
169	real, dimension(:,:,:), save, allocatable :: QREFvis3d
170	real, dimension(:,:,:), save, allocatable :: QREFir3d
171	!$OMP THREADPRIVATE(QREFvis3d,QREFir3d)
172
173
174	! Miscellaneous :
175	real*8 temp,temp1,temp2,pweight
176	character(len=10) :: tmp1
177	character(len=10) :: tmp2
178	character(len=100) :: message
179	character(len=10),parameter :: subname="callcorrk"
180
181	! For fixed water vapour profiles.
182	integer i_var
183	real RH
184	real*8 pq_temp(nlayer)
185	! real(KIND=r8) :: pq_temp(nlayer) ! better F90 way.. DOESNT PORT TO F77!!!
186	real psat,qsat
187
188	logical OLRz
189	real*8 NFLUXGNDV_nu(L_NSPECTV)
190
191	! Included by RW for runaway greenhouse 1D study.
192	real vtmp(nlayer)
193	REAL*8 muvarrad(L_LEVELS)
194
195	! Included by MT for albedo calculations.
196	REAL*8 albedo_temp(L_NSPECTV) ! For equivalent albedo calculation.
197	REAL*8 surface_stellar_flux ! Stellar flux reaching the surface. Useful for equivalent albedo calculation.
198
199
200	!===============================================================
201	! I.a Initialization on first call
202	!===============================================================
203
204
205	if(firstcall) then
206
207	! test on allocated necessary because of CLFvarying (two calls to callcorrk in physiq)
208	if(.not.allocated(QXVAER)) allocate(QXVAER(L_LEVELS,L_NSPECTV,naerkind))
209	if(.not.allocated(QSVAER)) allocate(QSVAER(L_LEVELS,L_NSPECTV,naerkind))
210	if(.not.allocated(GVAER)) allocate(GVAER(L_LEVELS,L_NSPECTV,naerkind))
211	if(.not.allocated(QXIAER)) allocate(QXIAER(L_LEVELS,L_NSPECTI,naerkind))
212	if(.not.allocated(QSIAER)) allocate(QSIAER(L_LEVELS,L_NSPECTI,naerkind))
213	if(.not.allocated(GIAER)) allocate(GIAER(L_LEVELS,L_NSPECTI,naerkind))
214
215	!!! ALLOCATED instances are necessary because of CLFvarying (strategy to call callcorrk twice in physiq...)
216	IF(.not.ALLOCATED(QREFvis3d)) ALLOCATE(QREFvis3d(ngrid,nlayer,naerkind))
217	IF(.not.ALLOCATED(QREFir3d)) ALLOCATE(QREFir3d(ngrid,nlayer,naerkind))
218	! Effective radius and variance of the aerosols
219	IF(.not.ALLOCATED(reffrad)) allocate(reffrad(ngrid,nlayer,naerkind))
220	IF(.not.ALLOCATED(nueffrad)) allocate(nueffrad(ngrid,nlayer,naerkind))
221
222	#ifndef MESOSCALE
223	call system('rm -f surf_vals_long.out')
224	#endif
225
226	if(naerkind.gt.4)then
227	message='Code not general enough to deal with naerkind > 4 yet.'
228	call abort_physic(subname,message,1)
229	endif
230	call su_aer_radii(ngrid,nlayer,reffrad,nueffrad)
231
232
233	!--------------------------------------------------
234	! Set up correlated k
235	!--------------------------------------------------
236
237
238	print*, "callcorrk: Correlated-k data base folder:",trim(datadir)
239	call getin_p("corrkdir",corrkdir)
240	print*, "corrkdir = ",corrkdir
241	write( tmp1, '(i3)' ) L_NSPECTI
242	write( tmp2, '(i3)' ) L_NSPECTV
243	banddir=trim(adjustl(tmp1))//'x'//trim(adjustl(tmp2))
244	banddir=trim(adjustl(corrkdir))//'/'//trim(adjustl(banddir))
245
246	call setspi ! Basic infrared properties.
247	call setspv ! Basic visible properties.
248	call sugas_corrk ! Set up gaseous absorption properties.
249	call suaer_corrk ! Set up aerosol optical properties.
250
251
252	! now that L_NGAUSS has been initialized (by sugas_corrk)
253	! allocate related arrays
254	if(.not.allocated(dtaui)) ALLOCATE(dtaui(L_NLAYRAD,L_NSPECTI,L_NGAUSS))
255	if(.not.allocated(dtauv)) ALLOCATE(dtauv(L_NLAYRAD,L_NSPECTV,L_NGAUSS))
256	if(.not.allocated(cosbv)) ALLOCATE(cosbv(L_NLAYRAD,L_NSPECTV,L_NGAUSS))
257	if(.not.allocated(cosbi)) ALLOCATE(cosbi(L_NLAYRAD,L_NSPECTI,L_NGAUSS))
258	if(.not.allocated(wbari)) ALLOCATE(wbari(L_NLAYRAD,L_NSPECTI,L_NGAUSS))
259	if(.not.allocated(wbarv)) ALLOCATE(wbarv(L_NLAYRAD,L_NSPECTV,L_NGAUSS))
260	if(.not.allocated(tauv)) ALLOCATE(tauv(L_NLEVRAD,L_NSPECTV,L_NGAUSS))
261	if(.not.allocated(taucumv)) ALLOCATE(taucumv(L_LEVELS,L_NSPECTV,L_NGAUSS))
262	if(.not.allocated(taucumi)) ALLOCATE(taucumi(L_LEVELS,L_NSPECTI,L_NGAUSS))
263	if(.not.allocated(taugsurf)) ALLOCATE(taugsurf(L_NSPECTV,L_NGAUSS-1))
264	if(.not.allocated(taugsurfi)) ALLOCATE(taugsurfi(L_NSPECTI,L_NGAUSS-1))
265
266	if((igcm_h2o_vap.eq.0) .and. varactive)then
267	message='varactive in callcorrk but no h2o_vap tracer.'
268	call abort_physic(subname,message,1)
269	endif
270
271	end if ! of if (firstcall)
272
273	!=======================================================================
274	! I.b Initialization on every call
275	!=======================================================================
276
277	qxvaer(:,:,:)=0.0
278	qsvaer(:,:,:)=0.0
279	gvaer(:,:,:) =0.0
280
281	qxiaer(:,:,:)=0.0
282	qsiaer(:,:,:)=0.0
283	giaer(:,:,:) =0.0
284
285	OLR_nu(:,:) = 0.
286	OSR_nu(:,:) = 0.
287
288	!--------------------------------------------------
289	! Effective radius and variance of the aerosols
290	!--------------------------------------------------
291
292	do iaer=1,naerkind
293
294	if ((iaer.eq.iaero_co2).and.tracer.and.(igcm_co2_ice.gt.0)) then ! Treat condensed co2 particles.
295	call co2_reffrad(ngrid,nlayer,nq,pq,reffrad(1,1,iaero_co2))
296	if (is_master) then
297	print*,'Max. CO2 ice particle size = ',maxval(reffrad(1:ngrid,1:nlayer,iaer))/1.e-6,' um'
298	print*,'Min. CO2 ice particle size = ',minval(reffrad(1:ngrid,1:nlayer,iaer))/1.e-6,' um'
299	end if
300	end if
301
302	if ((iaer.eq.iaero_h2o).and.water) then ! Treat condensed water particles. To be generalized for other aerosols ...
303	call h2o_reffrad(ngrid,nlayer,pq(1,1,igcm_h2o_ice),pt, &
304	reffrad(1,1,iaero_h2o),nueffrad(1,1,iaero_h2o))
305	if (is_master) then
306	print*,'Max. H2O cloud particle size = ',maxval(reffrad(1:ngrid,1:nlayer,iaer))/1.e-6,' um'
307	print*,'Min. H2O cloud particle size = ',minval(reffrad(1:ngrid,1:nlayer,iaer))/1.e-6,' um'
308	end if
309	endif
310
311	if(iaer.eq.iaero_dust)then
312	call dust_reffrad(ngrid,nlayer,reffrad(1,1,iaero_dust))
313	if (is_master) then
314	print*,'Dust particle size = ',reffrad(1,1,iaer)/1.e-6,' um'
315	end if
316	endif
317
318	if(iaer.eq.iaero_h2so4)then
319	call h2so4_reffrad(ngrid,nlayer,reffrad(1,1,iaero_h2so4))
320	if (is_master) then
321	print*,'H2SO4 particle size =',reffrad(1,1,iaer)/1.e-6,' um'
322	end if
323	endif
324
325	if(iaer.eq.iaero_back2lay)then
326	call back2lay_reffrad(ngrid,reffrad(1,1,iaero_back2lay),nlayer,pplev)
327	endif
328
329	! For n-layer aerosol size set once for all at firstcall in su_aer_radii
330
331	! if(iaer.eq.iaero_aurora)then
332	! call aurora_reffrad(ngrid,nlayer,reffrad(1,1,iaero_aurora))
333	! endif
334
335	end do !iaer=1,naerkind.
336
337
338	! How much light do we get ?
339	do nw=1,L_NSPECTV
340	stel(nw)=stellarf(nw)/(dist_star**2)
341	end do
342
343	! Get 3D aerosol optical properties.
344	call aeroptproperties(ngrid,nlayer,reffrad,nueffrad, &
345	QVISsQREF3d,omegaVIS3d,gVIS3d, &
346	QIRsQREF3d,omegaIR3d,gIR3d, &
347	QREFvis3d,QREFir3d)
348
349	! Get aerosol optical depths.
350	call aeropacity(ngrid,nlayer,nq,pplay,pplev,pq,aerosol, &
351	reffrad,QREFvis3d,QREFir3d, &
352	tau_col,cloudfrac,totcloudfrac,clearsky)
353
354
355
356	!-----------------------------------------------------------------------
357	do ig=1,ngrid ! Starting Big Loop over every GCM column
358	!-----------------------------------------------------------------------
359
360
361	!=======================================================================
362	! II. Transformation of the GCM variables
363	!=======================================================================
364
365
366	!-----------------------------------------------------------------------
367	! Aerosol optical properties Qext, Qscat and g.
368	! The transformation in the vertical is the same as for temperature.
369	!-----------------------------------------------------------------------
370
371
372	do iaer=1,naerkind
373	! Shortwave.
374	do nw=1,L_NSPECTV
375
376	do l=1,nlayer
377
378	temp1=QVISsQREF3d(ig,nlayer+1-l,nw,iaer) &
379	*QREFvis3d(ig,nlayer+1-l,iaer)
380
381	temp2=QVISsQREF3d(ig,max(nlayer-l,1),nw,iaer) &
382	*QREFvis3d(ig,max(nlayer-l,1),iaer)
383
384	qxvaer(2*l,nw,iaer) = temp1
385	qxvaer(2*l+1,nw,iaer)=(temp1+temp2)/2
386
387	temp1=temp1*omegavis3d(ig,nlayer+1-l,nw,iaer)
388	temp2=temp2*omegavis3d(ig,max(nlayer-l,1),nw,iaer)
389
390	qsvaer(2*l,nw,iaer) = temp1
391	qsvaer(2*l+1,nw,iaer)=(temp1+temp2)/2
392
393	temp1=gvis3d(ig,nlayer+1-l,nw,iaer)
394	temp2=gvis3d(ig,max(nlayer-l,1),nw,iaer)
395
396	gvaer(2*l,nw,iaer) = temp1
397	gvaer(2*l+1,nw,iaer)=(temp1+temp2)/2
398
399	end do ! nlayer
400
401	qxvaer(1,nw,iaer)=qxvaer(2,nw,iaer)
402	qxvaer(2*nlayer+1,nw,iaer)=0.
403
404	qsvaer(1,nw,iaer)=qsvaer(2,nw,iaer)
405	qsvaer(2*nlayer+1,nw,iaer)=0.
406
407	gvaer(1,nw,iaer)=gvaer(2,nw,iaer)
408	gvaer(2*nlayer+1,nw,iaer)=0.
409
410	end do ! L_NSPECTV
411
412	do nw=1,L_NSPECTI
413	! Longwave
414	do l=1,nlayer
415
416	temp1=QIRsQREF3d(ig,nlayer+1-l,nw,iaer) &
417	*QREFir3d(ig,nlayer+1-l,iaer)
418
419	temp2=QIRsQREF3d(ig,max(nlayer-l,1),nw,iaer) &
420	*QREFir3d(ig,max(nlayer-l,1),iaer)
421
422	qxiaer(2*l,nw,iaer) = temp1
423	qxiaer(2*l+1,nw,iaer)=(temp1+temp2)/2
424
425	temp1=temp1*omegair3d(ig,nlayer+1-l,nw,iaer)
426	temp2=temp2*omegair3d(ig,max(nlayer-l,1),nw,iaer)
427
428	qsiaer(2*l,nw,iaer) = temp1
429	qsiaer(2*l+1,nw,iaer)=(temp1+temp2)/2
430
431	temp1=gir3d(ig,nlayer+1-l,nw,iaer)
432	temp2=gir3d(ig,max(nlayer-l,1),nw,iaer)
433
434	giaer(2*l,nw,iaer) = temp1
435	giaer(2*l+1,nw,iaer)=(temp1+temp2)/2
436
437	end do ! nlayer
438
439	qxiaer(1,nw,iaer)=qxiaer(2,nw,iaer)
440	qxiaer(2*nlayer+1,nw,iaer)=0.
441
442	qsiaer(1,nw,iaer)=qsiaer(2,nw,iaer)
443	qsiaer(2*nlayer+1,nw,iaer)=0.
444
445	giaer(1,nw,iaer)=giaer(2,nw,iaer)
446	giaer(2*nlayer+1,nw,iaer)=0.
447
448	end do ! L_NSPECTI
449
450	end do ! naerkind
451
452	! Test / Correct for freaky s. s. albedo values.
453	do iaer=1,naerkind
454	do k=1,L_LEVELS
455
456	do nw=1,L_NSPECTV
457	if(qsvaer(k,nw,iaer).gt.1.05*qxvaer(k,nw,iaer))then
458	message='Serious problems with qsvaer values'
459	call abort_physic(subname,message,1)
460	endif
461	if(qsvaer(k,nw,iaer).gt.qxvaer(k,nw,iaer))then
462	qsvaer(k,nw,iaer)=qxvaer(k,nw,iaer)
463	endif
464	end do
465
466	do nw=1,L_NSPECTI
467	if(qsiaer(k,nw,iaer).gt.1.05*qxiaer(k,nw,iaer))then
468	message='Serious problems with qsvaer values'
469	call abort_physic(subname,message,1)
470	endif
471	if(qsiaer(k,nw,iaer).gt.qxiaer(k,nw,iaer))then
472	qsiaer(k,nw,iaer)=qxiaer(k,nw,iaer)
473	endif
474	end do
475
476	end do ! L_LEVELS
477	end do ! naerkind
478
479	!-----------------------------------------------------------------------
480	! Aerosol optical depths
481	!-----------------------------------------------------------------------
482
483	do iaer=1,naerkind ! a bug was here
484	do k=0,nlayer-1
485
486	pweight=(pplay(ig,L_NLAYRAD-k)-pplev(ig,L_NLAYRAD-k+1))/ &
487	(pplev(ig,L_NLAYRAD-k)-pplev(ig,L_NLAYRAD-k+1))
488	! As 'aerosol' is at reference (visible) wavelenght we scale it as
489	! it will be multplied by qxi/v in optci/v
490	temp=aerosol(ig,L_NLAYRAD-k,iaer)/QREFvis3d(ig,L_NLAYRAD-k,iaer)
491	tauaero(2k+2,iaer)=max(temppweight,0.d0)
492	tauaero(2k+3,iaer)=max(temp-tauaero(2k+2,iaer),0.d0)
493
494	end do
495	! boundary conditions
496	tauaero(1,iaer) = tauaero(2,iaer)
497	!tauaero(1,iaer) = 0.
498	!JL18 at time of testing, the two above conditions gave the same results bit for bit.
499
500	end do ! naerkind
501
502	! Albedo and Emissivity.
503	albi=1-emis(ig) ! Long Wave.
504	DO nw=1,L_NSPECTV ! Short Wave loop.
505	albv(nw)=albedo(ig,nw)
506	ENDDO
507
508	acosz=mu0(ig) ! Cosine of sun incident angle : 3D simulations or local 1D simulations using latitude.
509
510	!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
511	!!! Note by JL13 : In the following, some indices were changed in the interpolations,
512	!!! so that the model results are less dependent on the number of layers !
513	!!!
514	!!! --- The older versions are commented with the comment !JL13index ---
515	!!!
516	!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
517
518
519	!-----------------------------------------------------------------------
520	! Water vapour (to be generalised for other gases eventually ...)
521	!-----------------------------------------------------------------------
522
523	if(varactive)then
524
525	i_var=igcm_h2o_vap
526	do l=1,nlayer
527	qvar(2*l) = pq(ig,nlayer+1-l,i_var)
528	qvar(2*l+1) = pq(ig,nlayer+1-l,i_var)
529	!JL13index qvar(2*l+1) = (pq(ig,nlayer+1-l,i_var)+pq(ig,max(nlayer-l,1),i_var))/2
530	!JL13index ! Average approximation as for temperature...
531	end do
532	qvar(1)=qvar(2)
533
534	elseif(varfixed)then
535
536	do l=1,nlayer ! Here we will assign fixed water vapour profiles globally.
537	RH = satval * ((pplay(ig,l)/pplev(ig,1) - 0.02) / 0.98)
538	if(RH.lt.0.0) RH=0.0
539
540	call Psat_water(pt(ig,l),pplay(ig,l),psat,qsat)
541
542	!pq_temp(l) = qsat ! fully saturated everywhere
543	pq_temp(l) = RH * qsat ! ~realistic profile (e.g. 80% saturation at ground)
544	end do
545
546	do l=1,nlayer
547	qvar(2*l) = pq_temp(nlayer+1-l)
548	qvar(2*l+1) = (pq_temp(nlayer+1-l)+pq_temp(max(nlayer-l,1)))/2
549	end do
550
551	qvar(1)=qvar(2)
552
553	! Lowest layer of atmosphere
554	RH = satval * (1 - 0.02) / 0.98
555	if(RH.lt.0.0) RH=0.0
556
557	qvar(2nlayer+1)= RH qsat ! ~realistic profile (e.g. 80% saturation at ground)
558
559	else
560	do k=1,L_LEVELS
561	qvar(k) = 1.0D-7
562	end do
563	end if ! varactive/varfixed
564
565	if(.not.kastprof)then
566	! IMPORTANT: Now convert from kg/kg to mol/mol.
567	do k=1,L_LEVELS
568	qvar(k) = qvar(k)/(epsi+qvar(k)*(1.-epsi))
569	end do
570	end if
571
572	!-----------------------------------------------------------------------
573	! kcm mode only !
574	!-----------------------------------------------------------------------
575
576	if(kastprof)then
577
578	if(.not.global1d)then ! garde-fou/safeguard added by MT (to be removed in the future)
579	message='You have to fix mu0, the cosinus of the solar angle'
580	call abort_physic(subname,message,1)
581	endif
582
583	! Initial values equivalent to mugaz.
584	DO l=1,nlayer
585	muvarrad(2*l) = mugaz
586	muvarrad(2*l+1) = mugaz
587	END DO
588
589	if(ngasmx.gt.1)then
590
591	DO l=1,nlayer
592	muvarrad(2*l) = muvar(ig,nlayer+2-l)
593	muvarrad(2*l+1) = (muvar(ig,nlayer+2-l) + &
594	muvar(ig,max(nlayer+1-l,1)))/2
595	END DO
596
597	muvarrad(1) = muvarrad(2)
598	muvarrad(2*nlayer+1) = muvar(ig,1)
599
600	print*,'Recalculating qvar with VARIABLE epsi for kastprof'
601	print*,'Assumes that the variable gas is H2O!!!'
602	print*,'Assumes that there is only one tracer'
603
604	!i_var=igcm_h2o_vap
605	i_var=1
606
607	if(nq.gt.1)then
608	message='Need 1 tracer only to run kcm1d.e'
609	call abort_physic(subname,message,1)
610	endif
611
612	do l=1,nlayer
613	vtmp(l)=pq(ig,l,i_var)/(epsi+pq(ig,l,i_var)*(1.-epsi))
614	!vtmp(l)=pq(ig,l,i_var)*muvar(ig,l+1)/mH2O !JL to be changed
615	end do
616
617	do l=1,nlayer
618	qvar(2*l) = vtmp(nlayer+1-l)
619	qvar(2*l+1) = vtmp(nlayer+1-l)
620	! qvar(2*l+1) = ( vtmp(nlayer+1-l) + vtmp(max(nlayer-l,1)) )/2
621	end do
622	qvar(1)=qvar(2)
623
624	write(,)trim(subname),' :Warning: reducing qvar in callcorrk.'
625	write(,)trim(subname),' :Temperature profile no longer consistent ', &
626	'with saturated H2O. qsat=',satval
627
628	do k=1,L_LEVELS
629	qvar(k) = qvar(k)*satval
630	end do
631
632	endif
633	else ! if kastprof
634	DO l=1,nlayer
635	muvarrad(2*l) = muvar(ig,nlayer+2-l)
636	muvarrad(2*l+1) = (muvar(ig,nlayer+2-l)+muvar(ig,max(nlayer+1-l,1)))/2
637	END DO
638
639	muvarrad(1) = muvarrad(2)
640	muvarrad(2*nlayer+1)=muvar(ig,1)
641	endif ! if kastprof
642
643	! Keep values inside limits for which we have radiative transfer coefficients !!!
644	if(L_REFVAR.gt.1)then ! (there was a bug here)
645	do k=1,L_LEVELS
646	if(qvar(k).lt.wrefvar(1))then
647	qvar(k)=wrefvar(1)+1.0e-8
648	elseif(qvar(k).gt.wrefvar(L_REFVAR))then
649	qvar(k)=wrefvar(L_REFVAR)-1.0e-8
650	endif
651	end do
652	endif
653
654	!-----------------------------------------------------------------------
655	! Pressure and temperature
656	!-----------------------------------------------------------------------
657
658	DO l=1,nlayer
659	plevrad(2*l) = pplay(ig,nlayer+1-l)/scalep
660	plevrad(2*l+1) = pplev(ig,nlayer+1-l)/scalep
661	tlevrad(2*l) = pt(ig,nlayer+1-l)
662	tlevrad(2*l+1) = (pt(ig,nlayer+1-l)+pt(ig,max(nlayer-l,1)))/2
663	END DO
664
665	plevrad(1) = 0.
666	! 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.
667
668	tlevrad(1) = tlevrad(2)
669	tlevrad(2*nlayer+1)=tsurf(ig)
670
671	pmid(1) = pplay(ig,nlayer)/scalep
672	pmid(2) = pmid(1)
673
674	tmid(1) = tlevrad(2)
675	tmid(2) = tmid(1)
676
677	DO l=1,L_NLAYRAD-1
678	tmid(2l+1) = tlevrad(2l+1)
679	tmid(2l+2) = tlevrad(2l+1)
680	pmid(2l+1) = plevrad(2l+1)
681	pmid(2l+2) = plevrad(2l+1)
682	END DO
683	pmid(L_LEVELS) = plevrad(L_LEVELS)
684	tmid(L_LEVELS) = tlevrad(L_LEVELS)
685
686	!!Alternative interpolation:
687	! pmid(3) = pmid(1)
688	! pmid(4) = pmid(1)
689	! tmid(3) = tmid(1)
690	! tmid(4) = tmid(1)
691	! DO l=2,L_NLAYRAD-1
692	! tmid(2l+1) = tlevrad(2l)
693	! tmid(2l+2) = tlevrad(2l)
694	! pmid(2l+1) = plevrad(2l)
695	! pmid(2l+2) = plevrad(2l)
696	! END DO
697	! pmid(L_LEVELS) = plevrad(L_LEVELS-1)
698	! tmid(L_LEVELS) = tlevrad(L_LEVELS-1)
699
700	! Test for out-of-bounds pressure.
701	if(plevrad(3).lt.pgasmin)then
702	print*,'Minimum pressure is outside the radiative'
703	print*,'transfer kmatrix bounds, exiting.'
704	message="Minimum pressure outside of kmatrix bounds"
705	call abort_physic(subname,message,1)
706	elseif(plevrad(L_LEVELS).gt.pgasmax)then
707	print*,'Maximum pressure is outside the radiative'
708	print*,'transfer kmatrix bounds, exiting.'
709	message="Minimum pressure outside of kmatrix bounds"
710	call abort_physic(subname,message,1)
711	endif
712
713	! Test for out-of-bounds temperature.
714	! -- JVO 20 : Also add a sanity test checking that tlevrad is
715	! within Planck function temperature boundaries,
716	! which would cause gfluxi/sfluxi to crash.
717	do k=1,L_LEVELS
718
719	if(tlevrad(k).lt.tgasmin)then
720	print*,'Minimum temperature is outside the radiative'
721	print*,'transfer kmatrix bounds'
722	print*,"k=",k," tlevrad(k)=",tlevrad(k)
723	print*,"tgasmin=",tgasmin
724	if (strictboundcorrk) then
725	message="Minimum temperature outside of kmatrix bounds"
726	call abort_physic(subname,message,1)
727	else
728	print,'**********************************************'
729	print*,'we allow model to continue with tlevrad<tgasmin'
730	print*,' ... we assume we know what you are doing ... '
731	print*,' ... but do not let this happen too often ... '
732	print,'**********************************************'
733	!tlevrad(k)=tgasmin ! Used in the source function !
734	endif
735	elseif(tlevrad(k).gt.tgasmax)then
736	print*,'Maximum temperature is outside the radiative'
737	print*,'transfer kmatrix bounds, exiting.'
738	print*,"k=",k," tlevrad(k)=",tlevrad(k)
739	print*,"tgasmax=",tgasmax
740	if (strictboundcorrk) then
741	message="Maximum temperature outside of kmatrix bounds"
742	call abort_physic(subname,message,1)
743	else
744	print,'**********************************************'
745	print*,'we allow model to continue with tlevrad>tgasmax'
746	print*,' ... we assume we know what you are doing ... '
747	print*,' ... but do not let this happen too often ... '
748	print,'**********************************************'
749	!tlevrad(k)=tgasmax ! Used in the source function !
750	endif
751	endif
752
753	if (tlevrad(k).lt.tplanckmin) then
754	print*,'Minimum temperature is outside the boundaries for'
755	print*,'Planck function integration set in callphys.def, aborting.'
756	print*,"k=",k," tlevrad(k)=",tlevrad(k)
757	print*,"tplanckmin=",tplanckmin
758	message="Minimum temperature outside Planck function bounds - Change tplanckmin in callphys.def"
759	call abort_physic(subname,message,1)
760	else if (tlevrad(k).gt.tplanckmax) then
761	print*,'Maximum temperature is outside the boundaries for'
762	print*,'Planck function integration set in callphys.def, aborting.'
763	print*,"k=",k," tlevrad(k)=",tlevrad(k)
764	print*,"tplanckmax=",tplanckmax
765	message="Maximum temperature outside Planck function bounds - Change tplanckmax in callphys.def"
766	call abort_physic(subname,message,1)
767	endif
768
769	enddo
770
771	do k=1,L_NLAYRAD+1
772	if(tmid(k).lt.tgasmin)then
773	print*,'Minimum temperature is outside the radiative'
774	print*,'transfer kmatrix bounds, exiting.'
775	print*,"k=",k," tmid(k)=",tmid(k)
776	print*,"tgasmin=",tgasmin
777	if (strictboundcorrk) then
778	message="Minimum temperature outside of kmatrix bounds"
779	call abort_physic(subname,message,1)
780	else
781	print,'**********************************************'
782	print*,'we allow model to continue but with tmid=tgasmin'
783	print*,' ... we assume we know what you are doing ... '
784	print*,' ... but do not let this happen too often ... '
785	print,'**********************************************'
786	tmid(k)=tgasmin
787	endif
788	elseif(tmid(k).gt.tgasmax)then
789	print*,'Maximum temperature is outside the radiative'
790	print*,'transfer kmatrix bounds, exiting.'
791	print*,"k=",k," tmid(k)=",tmid(k)
792	print*,"tgasmax=",tgasmax
793	if (strictboundcorrk) then
794	message="Maximum temperature outside of kmatrix bounds"
795	call abort_physic(subname,message,1)
796	else
797	print,'**********************************************'
798	print*,'we allow model to continue but with tmid=tgasmax'
799	print*,' ... we assume we know what you are doing ... '
800	print*,' ... but do not let this happen too often ... '
801	print,'**********************************************'
802	tmid(k)=tgasmax
803	endif
804	endif
805	enddo
806
807	!=======================================================================
808	! III. Calling the main radiative transfer subroutines
809	!=======================================================================
810
811
812	Cmk= 0.01 * 1.0 / (glat(ig) * mugaz * 1.672621e-27) ! q_main=1.0 assumed.
813	glat_ig=glat(ig)
814
815	!-----------------------------------------------------------------------
816	! Short Wave Part
817	!-----------------------------------------------------------------------
818
819	if(fract(ig) .ge. 1.0e-4) then ! Only during daylight.
820	if((ngrid.eq.1).and.(global1d))then
821	do nw=1,L_NSPECTV
822	stel_fract(nw)= stel(nw)* 0.25 / acosz ! globally averaged = divide by 4, and we correct for solar zenith angle
823	end do
824	else
825	do nw=1,L_NSPECTV
826	stel_fract(nw)= stel(nw) * fract(ig)
827	end do
828	endif
829
830	call optcv(dtauv,tauv,taucumv,plevrad, &
831	qxvaer,qsvaer,gvaer,wbarv,cosbv,tauray,tauaero, &
832	tmid,pmid,taugsurf,qvar,muvarrad)
833
834	call sfluxv(dtauv,tauv,taucumv,albv,dwnv,wbarv,cosbv, &
835	acosz,stel_fract, &
836	nfluxtopv,fluxtopvdn,nfluxoutv_nu,nfluxgndv_nu, &
837	fmnetv,fluxupv,fluxdnv,fzerov,taugsurf)
838
839	else ! During the night, fluxes = 0.
840	nfluxtopv = 0.0d0
841	fluxtopvdn = 0.0d0
842	nfluxoutv_nu(:) = 0.0d0
843	nfluxgndv_nu(:) = 0.0d0
844	do l=1,L_NLAYRAD
845	fmnetv(l)=0.0d0
846	fluxupv(l)=0.0d0
847	fluxdnv(l)=0.0d0
848	end do
849	end if
850
851
852	! Equivalent Albedo Calculation (for OUTPUT). MT2015
853	if(fract(ig) .ge. 1.0e-4) then ! equivalent albedo makes sense only during daylight.
854	surface_stellar_flux=sum(nfluxgndv_nu(1:L_NSPECTV))
855	if(surface_stellar_flux .gt. 1.0e-3) then ! equivalent albedo makes sense only if the stellar flux received by the surface is positive.
856	DO nw=1,L_NSPECTV
857	albedo_temp(nw)=albedo(ig,nw)*nfluxgndv_nu(nw)
858	ENDDO
859	albedo_temp(1:L_NSPECTV)=albedo_temp(1:L_NSPECTV)/surface_stellar_flux
860	albedo_equivalent(ig)=sum(albedo_temp(1:L_NSPECTV))
861	else
862	albedo_equivalent(ig)=0.0 ! Spectrally Integrated Albedo not defined for non-irradiated grid points. So we arbitrary set the equivalent albedo to 0.
863	endif
864	else
865	albedo_equivalent(ig)=0.0 ! Spectrally Integrated Albedo not defined for non-irradiated grid points. So we arbitrary set the equivalent albedo to 0.
866	endif
867
868
869	!-----------------------------------------------------------------------
870	! Long Wave Part
871	!-----------------------------------------------------------------------
872
873	call optci(plevrad,tlevrad,dtaui,taucumi, &
874	qxiaer,qsiaer,giaer,cosbi,wbari,tauaero,tmid,pmid, &
875	taugsurfi,qvar,muvarrad)
876
877	call sfluxi(plevrad,tlevrad,dtaui,taucumi,ubari,albi, &
878	wnoi,dwni,cosbi,wbari,nfluxtopi,nfluxtopi_nu, &
879	fmneti,fluxupi,fluxdni,fluxupi_nu,fzeroi,taugsurfi)
880
881	!-----------------------------------------------------------------------
882	! Transformation of the correlated-k code outputs
883	! (into dtlw, dtsw, fluxsurf_lw, fluxsurf_sw, fluxtop_lw, fluxtop_sw)
884
885	! Flux incident at the top of the atmosphere
886	fluxtop_dn(ig)=fluxtopvdn
887
888	fluxtop_lw(ig) = real(nfluxtopi)
889	fluxabs_sw(ig) = real(-nfluxtopv)
890	fluxsurf_lw(ig) = real(fluxdni(L_NLAYRAD))
891	fluxsurf_sw(ig) = real(fluxdnv(L_NLAYRAD))
892
893	! Flux absorbed by the surface. By MT2015.
894	fluxsurfabs_sw(ig) = fluxsurf_sw(ig)*(1.-albedo_equivalent(ig))
895
896	if(fluxtop_dn(ig).lt.0.0)then
897	print*,'Achtung! fluxtop_dn has lost the plot!'
898	print*,'fluxtop_dn=',fluxtop_dn(ig)
899	print*,'acosz=',acosz
900	print*,'aerosol=',aerosol(ig,:,:)
901	print*,'temp= ',pt(ig,:)
902	print*,'pplay= ',pplay(ig,:)
903	message="Achtung! fluxtop_dn has lost the plot!"
904	call abort_physic(subname,message,1)
905	endif
906
907	! Spectral output, for exoplanet observational comparison
908	if(specOLR)then
909	do nw=1,L_NSPECTI
910	OLR_nu(ig,nw)=nfluxtopi_nu(nw)/DWNI(nw) !JL Normalize to the bandwidth
911	end do
912	do nw=1,L_NSPECTV
913	!GSR_nu(ig,nw)=nfluxgndv_nu(nw)
914	OSR_nu(ig,nw)=nfluxoutv_nu(nw)/DWNV(nw) !JL Normalize to the bandwidth
915	end do
916	endif
917
918	! Finally, the heating rates
919
920	DO l=2,L_NLAYRAD
921	dtsw(ig,L_NLAYRAD+1-l)=(fmnetv(l)-fmnetv(l-1)) &
922	glat(ig)/(cppscalep(plevrad(2l+1)-plevrad(2*l-1)))
923	dtlw(ig,L_NLAYRAD+1-l)=(fmneti(l)-fmneti(l-1)) &
924	glat(ig)/(cppscalep(plevrad(2l+1)-plevrad(2*l-1)))
925	END DO
926
927	! These are values at top of atmosphere
928	dtsw(ig,L_NLAYRAD)=(fmnetv(1)-nfluxtopv) &
929	glat(ig)/(cppscalep*(plevrad(3)-plevrad(2)))
930	dtlw(ig,L_NLAYRAD)=(fmneti(1)-nfluxtopi) &
931	glat(ig)/(cppscalep*(plevrad(3)-plevrad(2)))
932
933	! Optical thickness diagnostics (added by JVO)
934	if (diagdtau) then
935	do l=1,L_NLAYRAD
936	do nw=1,L_NSPECTV
937	int_dtauv(ig,l,nw) = 0.0d0
938	DO k=1,L_NGAUSS
939	! Output exp(-tau) because gweight ponderates exp and not tau itself
940	int_dtauv(ig,l,nw)= int_dtauv(ig,l,nw) + exp(-dtauv(l,nw,k))*gweight(k)
941	ENDDO
942	enddo
943	do nw=1,L_NSPECTI
944	int_dtaui(ig,l,nw) = 0.0d0
945	DO k=1,L_NGAUSS
946	! Output exp(-tau) because gweight ponderates exp and not tau itself
947	int_dtaui(ig,l,nw)= int_dtaui(ig,l,nw) + exp(-dtaui(l,nw,k))*gweight(k)
948	ENDDO
949	enddo
950	enddo
951	endif
952
953
954	!-----------------------------------------------------------------------
955	end do ! End of big loop over every GCM column.
956	!-----------------------------------------------------------------------
957
958
959
960	!-----------------------------------------------------------------------
961	! Additional diagnostics
962	!-----------------------------------------------------------------------
963
964	! IR spectral output, for exoplanet observational comparison
965	if(lastcall.and.(ngrid.eq.1))then ! could disable the 1D output, they are in the diagfi and diagspec... JL12
966
967	print*,'Saving scalar quantities in surf_vals.out...'
968	print*,'psurf = ', pplev(1,1),' Pa'
969	open(116,file='surf_vals.out')
970	write(116,*) tsurf(1),pplev(1,1),fluxtop_dn(1), &
971	real(-nfluxtopv),real(nfluxtopi)
972	close(116)
973
974
975	! USEFUL COMMENT - Do Not Remove.
976	!
977	! if(specOLR)then
978	! open(117,file='OLRnu.out')
979	! do nw=1,L_NSPECTI
980	! write(117,*) OLR_nu(1,nw)
981	! enddo
982	! close(117)
983	!
984	! open(127,file='OSRnu.out')
985	! do nw=1,L_NSPECTV
986	! write(127,*) OSR_nu(1,nw)
987	! enddo
988	! close(127)
989	! endif
990
991	! OLR vs altitude: do it as a .txt file.
992	OLRz=.false.
993	if(OLRz)then
994	print*,'saving IR vertical flux for OLRz...'
995	open(118,file='OLRz_plevs.out')
996	open(119,file='OLRz.out')
997	do l=1,L_NLAYRAD
998	write(118,) plevrad(2l)
999	do nw=1,L_NSPECTI
1000	write(119,*) fluxupi_nu(l,nw)
1001	enddo
1002	enddo
1003	close(118)
1004	close(119)
1005	endif
1006
1007	endif
1008
1009	! See physiq.F for explanations about CLFvarying. This is temporary.
1010	if (lastcall .and. .not.CLFvarying) then
1011	IF( ALLOCATED( gasi ) ) DEALLOCATE( gasi )
1012	IF( ALLOCATED( gasv ) ) DEALLOCATE( gasv )
1013	!$OMP BARRIER
1014	!$OMP MASTER
1015	IF( ALLOCATED( pgasref ) ) DEALLOCATE( pgasref )
1016	IF( ALLOCATED( tgasref ) ) DEALLOCATE( tgasref )
1017	IF( ALLOCATED( wrefvar ) ) DEALLOCATE( wrefvar )
1018	IF( ALLOCATED( pfgasref ) ) DEALLOCATE( pfgasref )
1019	IF( ALLOCATED( gweight ) ) DEALLOCATE( gweight )
1020	!$OMP END MASTER
1021	!$OMP BARRIER
1022	IF ( ALLOCATED(reffrad)) DEALLOCATE(reffrad)
1023	IF ( ALLOCATED(nueffrad)) DEALLOCATE(nueffrad)
1024	endif
1025
1026
1027	end subroutine callcorrk
1028
1029	END MODULE callcorrk_mod

Note: See TracBrowser for help on using the repository browser.

Download in other formats:

Original Format