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callcorrk.F90 @ 2176

Last change on this file since 2176 was 2138, checked in by jvatant, 6 years ago
Correct outptuts of dtaui/v with correct ponderations of weights, but now it is attenuation exp(-tau) --JVO
Property svn:executable set to ``*
File size: 41.4 KB

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1	MODULE callcorrk_mod
2
3	IMPLICIT NONE
4
5	CONTAINS
6
7	subroutine callcorrk(ngrid,nlayer,pq,nq,qsurf, &
8	albedo,albedo_equivalent,emis,mu0,pplev,pplay,pt, &
9	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_nh3, 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	use optcv_mod, only: optcv
36	use optci_mod, only: optci
37	implicit none
38
39	!==================================================================
40	!
41	! Purpose
42	! -------
43	! Solve the radiative transfer using the correlated-k method for
44	! the gaseous absorption and the Toon et al. (1989) method for
45	! scatttering due to aerosols.
46	!
47	! Authors
48	! -------
49	! Emmanuel 01/2001, Forget 09/2001
50	! Robin Wordsworth (2009)
51	!
52	!==================================================================
53
54	!-----------------------------------------------------------------------
55	! Declaration of the arguments (INPUT - OUTPUT) on the LMD GCM grid
56	! Layer #1 is the layer near the ground.
57	! Layer #nlayer is the layer at the top.
58	!-----------------------------------------------------------------------
59
60
61	! INPUT
62	INTEGER,INTENT(IN) :: ngrid ! Number of atmospheric columns.
63	INTEGER,INTENT(IN) :: nlayer ! Number of atmospheric layers.
64	REAL,INTENT(IN) :: pq(ngrid,nlayer,nq) ! Tracers (kg/kg_of_air).
65	INTEGER,INTENT(IN) :: nq ! Number of tracers.
66	REAL,INTENT(IN) :: qsurf(ngrid,nq) ! Tracers on surface (kg.m-2).
67	REAL,INTENT(IN) :: albedo(ngrid,L_NSPECTV) ! Spectral Short Wavelengths Albedo. By MT2015
68	REAL,INTENT(IN) :: emis(ngrid) ! Long Wave emissivity.
69	REAL,INTENT(IN) :: mu0(ngrid) ! Cosine of sun incident angle.
70	REAL,INTENT(IN) :: pplev(ngrid,nlayer+1) ! Inter-layer pressure (Pa).
71	REAL,INTENT(IN) :: pplay(ngrid,nlayer) ! Mid-layer pressure (Pa).
72	REAL,INTENT(IN) :: pt(ngrid,nlayer) ! Air temperature (K).
73	REAL,INTENT(IN) :: tsurf(ngrid) ! Surface temperature (K).
74	REAL,INTENT(IN) :: fract(ngrid) ! Fraction of day.
75	REAL,INTENT(IN) :: dist_star ! Distance star-planet (AU).
76	REAL,INTENT(IN) :: muvar(ngrid,nlayer+1)
77	REAL,INTENT(IN) :: cloudfrac(ngrid,nlayer) ! Fraction of clouds (%).
78	logical,intent(in) :: clearsky
79	logical,intent(in) :: firstcall ! Signals first call to physics.
80	logical,intent(in) :: lastcall ! Signals last call to physics.
81
82	! OUTPUT
83	REAL,INTENT(OUT) :: aerosol(ngrid,nlayer,naerkind) ! Aerosol tau (kg/kg).
84	REAL,INTENT(OUT) :: dtlw(ngrid,nlayer) ! Heating rate (K/s) due to LW radiation.
85	REAL,INTENT(OUT) :: dtsw(ngrid,nlayer) ! Heating rate (K/s) due to SW radiation.
86	REAL,INTENT(OUT) :: fluxsurf_lw(ngrid) ! Incident LW flux to surf (W/m2).
87	REAL,INTENT(OUT) :: fluxsurf_sw(ngrid) ! Incident SW flux to surf (W/m2)
88	REAL,INTENT(OUT) :: fluxsurfabs_sw(ngrid) ! Absorbed SW flux by the surface (W/m2). By MT2015.
89	REAL,INTENT(OUT) :: fluxtop_lw(ngrid) ! Outgoing LW flux to space (W/m2).
90	REAL,INTENT(OUT) :: fluxabs_sw(ngrid) ! SW flux absorbed by the planet (W/m2).
91	REAL,INTENT(OUT) :: fluxtop_dn(ngrid) ! Incident top of atmosphere SW flux (W/m2).
92	REAL,INTENT(OUT) :: OLR_nu(ngrid,L_NSPECTI) ! Outgoing LW radition in each band (Normalized to the band width (W/m2/cm-1).
93	REAL,INTENT(OUT) :: OSR_nu(ngrid,L_NSPECTV) ! Outgoing SW radition in each band (Normalized to the band width (W/m2/cm-1).
94	REAL,INTENT(OUT) :: tau_col(ngrid) ! Diagnostic from aeropacity.
95	REAL,INTENT(OUT) :: albedo_equivalent(ngrid) ! Spectrally Integrated Albedo. For Diagnostic. By MT2015
96	REAL,INTENT(OUT) :: totcloudfrac(ngrid) ! Column Fraction of clouds (%).
97	REAL,INTENT(OUT) :: int_dtaui(ngrid,nlayer,L_NSPECTI) ! VI optical thickness of layers within narrowbands for diags ().
98	REAL,INTENT(OUT) :: int_dtauv(ngrid,nlayer,L_NSPECTV) ! IR optical thickness of layers within narrowbands for diags ().
99
100
101
102
103
104	! Globally varying aerosol optical properties on GCM grid ; not needed everywhere so not in radcommon_h.
105	REAL :: QVISsQREF3d(ngrid,nlayer,L_NSPECTV,naerkind)
106	REAL :: omegaVIS3d(ngrid,nlayer,L_NSPECTV,naerkind)
107	REAL :: gVIS3d(ngrid,nlayer,L_NSPECTV,naerkind)
108	REAL :: QIRsQREF3d(ngrid,nlayer,L_NSPECTI,naerkind)
109	REAL :: omegaIR3d(ngrid,nlayer,L_NSPECTI,naerkind)
110	REAL :: gIR3d(ngrid,nlayer,L_NSPECTI,naerkind)
111
112	! REAL :: omegaREFvis3d(ngrid,nlayer,naerkind)
113	! REAL :: omegaREFir3d(ngrid,nlayer,naerkind) ! not sure of the point of these...
114
115	REAL,ALLOCATABLE,SAVE :: reffrad(:,:,:) ! aerosol effective radius (m)
116	REAL,ALLOCATABLE,SAVE :: nueffrad(:,:,:) ! aerosol effective variance
117	!$OMP THREADPRIVATE(reffrad,nueffrad)
118
119	!-----------------------------------------------------------------------
120	! Declaration of the variables required by correlated-k subroutines
121	! Numbered from top to bottom (unlike in the GCM)
122	!-----------------------------------------------------------------------
123
124	REAL*8 tmid(L_LEVELS),pmid(L_LEVELS)
125	REAL*8 tlevrad(L_LEVELS),plevrad(L_LEVELS)
126
127	! Optical values for the optci/cv subroutines
128	REAL*8 stel(L_NSPECTV),stel_fract(L_NSPECTV)
129	! NB: Arrays below are "save" to avoid reallocating them at every call
130	! not because their content needs be reused from call to the next
131	REAL*8,allocatable,save :: dtaui(:,:,:)
132	REAL*8,allocatable,save :: dtauv(:,:,:)
133	REAL*8,allocatable,save :: cosbv(:,:,:)
134	REAL*8,allocatable,save :: cosbi(:,:,:)
135	REAL*8,allocatable,save :: wbari(:,:,:)
136	REAL*8,allocatable,save :: wbarv(:,:,:)
137	REAL*8,allocatable,save :: tauv(:,:,:)
138	REAL*8,allocatable,save :: taucumv(:,:,:)
139	REAL*8,allocatable,save :: taucumi(:,:,:)
140
141	REAL*8 tauaero(L_LEVELS,naerkind)
142	REAL*8 nfluxtopv,nfluxtopi,nfluxtop,fluxtopvdn
143	REAL*8 nfluxoutv_nu(L_NSPECTV) ! Outgoing band-resolved VI flux at TOA (W/m2).
144	REAL*8 nfluxtopi_nu(L_NSPECTI) ! Net band-resolved IR flux at TOA (W/m2).
145	REAL*8 fluxupi_nu(L_NLAYRAD,L_NSPECTI) ! For 1D diagnostic.
146	REAL*8 fmneti(L_NLAYRAD),fmnetv(L_NLAYRAD)
147	REAL*8 fluxupv(L_NLAYRAD),fluxupi(L_NLAYRAD)
148	REAL*8 fluxdnv(L_NLAYRAD),fluxdni(L_NLAYRAD)
149	REAL*8 albi,acosz
150	REAL*8 albv(L_NSPECTV) ! Spectral Visible Albedo.
151
152	INTEGER ig,l,k,nw,iaer
153
154	real,save :: szangle
155	logical,save :: global1d
156	!$OMP THREADPRIVATE(szangle,global1d)
157
158	real*8,allocatable,save :: taugsurf(:,:)
159	real*8,allocatable,save :: taugsurfi(:,:)
160	real*8 qvar(L_LEVELS) ! Mixing ratio of variable component (mol/mol).
161
162	! Local aerosol optical properties for each column on RADIATIVE grid.
163	real*8,save,allocatable :: QXVAER(:,:,:)
164	real*8,save,allocatable :: QSVAER(:,:,:)
165	real*8,save,allocatable :: GVAER(:,:,:)
166	real*8,save,allocatable :: QXIAER(:,:,:)
167	real*8,save,allocatable :: QSIAER(:,:,:)
168	real*8,save,allocatable :: GIAER(:,:,:)
169
170	real, dimension(:,:,:), save, allocatable :: QREFvis3d
171	real, dimension(:,:,:), save, allocatable :: QREFir3d
172	!$OMP THREADPRIVATE(QXVAER,QSVAER,GVAER,QXIAER,QSIAER,GIAER,QREFvis3d,QREFir3d)
173
174
175	! Miscellaneous :
176	real*8 temp,temp1,temp2,pweight
177	character(len=10) :: tmp1
178	character(len=10) :: tmp2
179
180	! For fixed water vapour profiles.
181	integer i_var
182	real RH
183	real*8 pq_temp(nlayer)
184	! real(KIND=r8) :: pq_temp(nlayer) ! better F90 way.. DOESNT PORT TO F77!!!
185	real psat,qsat
186
187	logical OLRz
188	real*8 NFLUXGNDV_nu(L_NSPECTV)
189
190	! Included by RW for runaway greenhouse 1D study.
191	real vtmp(nlayer)
192	REAL*8 muvarrad(L_LEVELS)
193
194	! Included by MT for albedo calculations.
195	REAL*8 albedo_temp(L_NSPECTV) ! For equivalent albedo calculation.
196	REAL*8 surface_stellar_flux ! Stellar flux reaching the surface. Useful for equivalent albedo calculation.
197
198
199	!===============================================================
200	! I.a Initialization on first call
201	!===============================================================
202
203
204	if(firstcall) then
205
206	! test on allocated necessary because of CLFvarying (two calls to callcorrk in physiq)
207	if(.not.allocated(QXVAER)) allocate(QXVAER(L_LEVELS,L_NSPECTV,naerkind))
208	if(.not.allocated(QSVAER)) allocate(QSVAER(L_LEVELS,L_NSPECTV,naerkind))
209	if(.not.allocated(GVAER)) allocate(GVAER(L_LEVELS,L_NSPECTV,naerkind))
210	if(.not.allocated(QXIAER)) allocate(QXIAER(L_LEVELS,L_NSPECTI,naerkind))
211	if(.not.allocated(QSIAER)) allocate(QSIAER(L_LEVELS,L_NSPECTI,naerkind))
212	if(.not.allocated(GIAER)) allocate(GIAER(L_LEVELS,L_NSPECTI,naerkind))
213
214	!!! ALLOCATED instances are necessary because of CLFvarying (strategy to call callcorrk twice in physiq...)
215	IF(.not.ALLOCATED(QREFvis3d)) ALLOCATE(QREFvis3d(ngrid,nlayer,naerkind))
216	IF(.not.ALLOCATED(QREFir3d)) ALLOCATE(QREFir3d(ngrid,nlayer,naerkind))
217	! Effective radius and variance of the aerosols
218	IF(.not.ALLOCATED(reffrad)) allocate(reffrad(ngrid,nlayer,naerkind))
219	IF(.not.ALLOCATED(nueffrad)) allocate(nueffrad(ngrid,nlayer,naerkind))
220
221	#ifndef MESOSCALE
222	call system('rm -f surf_vals_long.out')
223	#endif
224
225	if(naerkind.gt.4)then
226	print*,'Code not general enough to deal with naerkind > 4 yet.'
227	call abort
228	endif
229	call su_aer_radii(ngrid,nlayer,reffrad,nueffrad)
230
231
232	!--------------------------------------------------
233	! Set up correlated k
234	!--------------------------------------------------
235
236
237	print*, "callcorrk: Correlated-k data base folder:",trim(datadir)
238	call getin_p("corrkdir",corrkdir)
239	print*, "corrkdir = ",corrkdir
240	write( tmp1, '(i3)' ) L_NSPECTI
241	write( tmp2, '(i3)' ) L_NSPECTV
242	banddir=trim(adjustl(tmp1))//'x'//trim(adjustl(tmp2))
243	banddir=trim(adjustl(corrkdir))//'/'//trim(adjustl(banddir))
244
245	call setspi ! Basic infrared properties.
246	call setspv ! Basic visible properties.
247	call sugas_corrk ! Set up gaseous absorption properties.
248	call suaer_corrk ! Set up aerosol optical properties.
249
250
251	! now that L_NGAUSS has been initialized (by sugas_corrk)
252	! allocate related arrays
253	if(.not.allocated(dtaui)) ALLOCATE(dtaui(L_NLAYRAD,L_NSPECTI,L_NGAUSS))
254	if(.not.allocated(dtauv)) ALLOCATE(dtauv(L_NLAYRAD,L_NSPECTV,L_NGAUSS))
255	if(.not.allocated(cosbv)) ALLOCATE(cosbv(L_NLAYRAD,L_NSPECTV,L_NGAUSS))
256	if(.not.allocated(cosbi)) ALLOCATE(cosbi(L_NLAYRAD,L_NSPECTI,L_NGAUSS))
257	if(.not.allocated(wbari)) ALLOCATE(wbari(L_NLAYRAD,L_NSPECTI,L_NGAUSS))
258	if(.not.allocated(wbarv)) ALLOCATE(wbarv(L_NLAYRAD,L_NSPECTV,L_NGAUSS))
259	if(.not.allocated(tauv)) ALLOCATE(tauv(L_NLEVRAD,L_NSPECTV,L_NGAUSS))
260	if(.not.allocated(taucumv)) ALLOCATE(taucumv(L_LEVELS,L_NSPECTV,L_NGAUSS))
261	if(.not.allocated(taucumi)) ALLOCATE(taucumi(L_LEVELS,L_NSPECTI,L_NGAUSS))
262	if(.not.allocated(taugsurf)) ALLOCATE(taugsurf(L_NSPECTV,L_NGAUSS-1))
263	if(.not.allocated(taugsurfi)) ALLOCATE(taugsurfi(L_NSPECTI,L_NGAUSS-1))
264
265	if((igcm_h2o_vap.eq.0) .and. varactive)then
266	print*,'varactive in callcorrk but no h2o_vap tracer.'
267	stop
268	endif
269
270	OLR_nu(:,:) = 0.
271	OSR_nu(:,:) = 0.
272
273	if (ngrid.eq.1) then
274	PRINT*, 'Simulate global averaged conditions ?'
275	global1d = .false. ! default value
276	call getin_p("global1d",global1d)
277	write(,) "global1d = ",global1d
278
279	! Test of incompatibility : if global1d is true, there should not be any diurnal cycle.
280	if (global1d.and.diurnal) then
281	print*,'if global1d is true, diurnal must be set to false'
282	stop
283	endif
284
285	if (global1d) then
286	PRINT *,'Solar Zenith angle (deg.) ?'
287	PRINT *,'(assumed for averaged solar flux S/4)'
288	szangle=60.0 ! default value
289	call getin_p("szangle",szangle)
290	write(,) "szangle = ",szangle
291	endif
292	endif
293
294	end if ! of if (firstcall)
295
296	!=======================================================================
297	! I.b Initialization on every call
298	!=======================================================================
299
300	qxvaer(:,:,:)=0.0
301	qsvaer(:,:,:)=0.0
302	gvaer(:,:,:) =0.0
303
304	qxiaer(:,:,:)=0.0
305	qsiaer(:,:,:)=0.0
306	giaer(:,:,:) =0.0
307
308	!--------------------------------------------------
309	! Effective radius and variance of the aerosols
310	!--------------------------------------------------
311
312	do iaer=1,naerkind
313
314	if ((iaer.eq.iaero_co2).and.tracer.and.(igcm_co2_ice.gt.0)) then ! Treat condensed co2 particles.
315	call co2_reffrad(ngrid,nlayer,nq,pq,reffrad(1,1,iaero_co2))
316	if (is_master) then
317	print*,'Max. CO2 ice particle size = ',maxval(reffrad(1:ngrid,1:nlayer,iaer))/1.e-6,' um'
318	print*,'Min. CO2 ice particle size = ',minval(reffrad(1:ngrid,1:nlayer,iaer))/1.e-6,' um'
319	end if
320	end if
321
322	if ((iaer.eq.iaero_h2o).and.water) then ! Treat condensed water particles. To be generalized for other aerosols ...
323	call h2o_reffrad(ngrid,nlayer,pq(1,1,igcm_h2o_ice),pt, &
324	reffrad(1,1,iaero_h2o),nueffrad(1,1,iaero_h2o))
325	if (is_master) then
326	print*,'Max. H2O cloud particle size = ',maxval(reffrad(1:ngrid,1:nlayer,iaer))/1.e-6,' um'
327	print*,'Min. H2O cloud particle size = ',minval(reffrad(1:ngrid,1:nlayer,iaer))/1.e-6,' um'
328	end if
329	endif
330
331	if(iaer.eq.iaero_dust)then
332	call dust_reffrad(ngrid,nlayer,reffrad(1,1,iaero_dust))
333	if (is_master) then
334	print*,'Dust particle size = ',reffrad(1,1,iaer)/1.e-6,' um'
335	end if
336	endif
337
338	if(iaer.eq.iaero_h2so4)then
339	call h2so4_reffrad(ngrid,nlayer,reffrad(1,1,iaero_h2so4))
340	if (is_master) then
341	print*,'H2SO4 particle size =',reffrad(1,1,iaer)/1.e-6,' um'
342	end if
343	endif
344
345	if(iaer.eq.iaero_back2lay)then
346	call back2lay_reffrad(ngrid,reffrad(1,1,iaero_back2lay),nlayer,pplev)
347	endif
348	! if(iaer.eq.iaero_nh3)then
349	! call nh3_reffrad(ngrid,nlayer,reffrad(1,1,iaero_nh3))
350	! endif
351	! if(iaer.eq.iaero_aurora)then
352	! call aurora_reffrad(ngrid,nlayer,reffrad(1,1,iaero_aurora))
353	! endif
354
355	end do !iaer=1,naerkind.
356
357
358	! How much light do we get ?
359	do nw=1,L_NSPECTV
360	stel(nw)=stellarf(nw)/(dist_star**2)
361	end do
362
363	! Get 3D aerosol optical properties.
364	call aeroptproperties(ngrid,nlayer,reffrad,nueffrad, &
365	QVISsQREF3d,omegaVIS3d,gVIS3d, &
366	QIRsQREF3d,omegaIR3d,gIR3d, &
367	QREFvis3d,QREFir3d)
368
369	! Get aerosol optical depths.
370	call aeropacity(ngrid,nlayer,nq,pplay,pplev,pq,aerosol, &
371	reffrad,QREFvis3d,QREFir3d, &
372	tau_col,cloudfrac,totcloudfrac,clearsky)
373
374
375
376	!-----------------------------------------------------------------------
377	do ig=1,ngrid ! Starting Big Loop over every GCM column
378	!-----------------------------------------------------------------------
379
380
381	!=======================================================================
382	! II. Transformation of the GCM variables
383	!=======================================================================
384
385
386	!-----------------------------------------------------------------------
387	! Aerosol optical properties Qext, Qscat and g.
388	! The transformation in the vertical is the same as for temperature.
389	!-----------------------------------------------------------------------
390
391
392	do iaer=1,naerkind
393	! Shortwave.
394	do nw=1,L_NSPECTV
395
396	do l=1,nlayer
397
398	temp1=QVISsQREF3d(ig,nlayer+1-l,nw,iaer) &
399	*QREFvis3d(ig,nlayer+1-l,iaer)
400
401	temp2=QVISsQREF3d(ig,max(nlayer-l,1),nw,iaer) &
402	*QREFvis3d(ig,max(nlayer-l,1),iaer)
403
404	qxvaer(2*l,nw,iaer) = temp1
405	qxvaer(2*l+1,nw,iaer)=(temp1+temp2)/2
406
407	temp1=temp1*omegavis3d(ig,nlayer+1-l,nw,iaer)
408	temp2=temp2*omegavis3d(ig,max(nlayer-l,1),nw,iaer)
409
410	qsvaer(2*l,nw,iaer) = temp1
411	qsvaer(2*l+1,nw,iaer)=(temp1+temp2)/2
412
413	temp1=gvis3d(ig,nlayer+1-l,nw,iaer)
414	temp2=gvis3d(ig,max(nlayer-l,1),nw,iaer)
415
416	gvaer(2*l,nw,iaer) = temp1
417	gvaer(2*l+1,nw,iaer)=(temp1+temp2)/2
418
419	end do ! nlayer
420
421	qxvaer(1,nw,iaer)=qxvaer(2,nw,iaer)
422	qxvaer(2*nlayer+1,nw,iaer)=0.
423
424	qsvaer(1,nw,iaer)=qsvaer(2,nw,iaer)
425	qsvaer(2*nlayer+1,nw,iaer)=0.
426
427	gvaer(1,nw,iaer)=gvaer(2,nw,iaer)
428	gvaer(2*nlayer+1,nw,iaer)=0.
429
430	end do ! L_NSPECTV
431
432	do nw=1,L_NSPECTI
433	! Longwave
434	do l=1,nlayer
435
436	temp1=QIRsQREF3d(ig,nlayer+1-l,nw,iaer) &
437	*QREFir3d(ig,nlayer+1-l,iaer)
438
439	temp2=QIRsQREF3d(ig,max(nlayer-l,1),nw,iaer) &
440	*QREFir3d(ig,max(nlayer-l,1),iaer)
441
442	qxiaer(2*l,nw,iaer) = temp1
443	qxiaer(2*l+1,nw,iaer)=(temp1+temp2)/2
444
445	temp1=temp1*omegair3d(ig,nlayer+1-l,nw,iaer)
446	temp2=temp2*omegair3d(ig,max(nlayer-l,1),nw,iaer)
447
448	qsiaer(2*l,nw,iaer) = temp1
449	qsiaer(2*l+1,nw,iaer)=(temp1+temp2)/2
450
451	temp1=gir3d(ig,nlayer+1-l,nw,iaer)
452	temp2=gir3d(ig,max(nlayer-l,1),nw,iaer)
453
454	giaer(2*l,nw,iaer) = temp1
455	giaer(2*l+1,nw,iaer)=(temp1+temp2)/2
456
457	end do ! nlayer
458
459	qxiaer(1,nw,iaer)=qxiaer(2,nw,iaer)
460	qxiaer(2*nlayer+1,nw,iaer)=0.
461
462	qsiaer(1,nw,iaer)=qsiaer(2,nw,iaer)
463	qsiaer(2*nlayer+1,nw,iaer)=0.
464
465	giaer(1,nw,iaer)=giaer(2,nw,iaer)
466	giaer(2*nlayer+1,nw,iaer)=0.
467
468	end do ! L_NSPECTI
469
470	end do ! naerkind
471
472	! Test / Correct for freaky s. s. albedo values.
473	do iaer=1,naerkind
474	do k=1,L_LEVELS
475
476	do nw=1,L_NSPECTV
477	if(qsvaer(k,nw,iaer).gt.1.05*qxvaer(k,nw,iaer))then
478	print*,'Serious problems with qsvaer values'
479	print*,'in callcorrk'
480	call abort
481	endif
482	if(qsvaer(k,nw,iaer).gt.qxvaer(k,nw,iaer))then
483	qsvaer(k,nw,iaer)=qxvaer(k,nw,iaer)
484	endif
485	end do
486
487	do nw=1,L_NSPECTI
488	if(qsiaer(k,nw,iaer).gt.1.05*qxiaer(k,nw,iaer))then
489	print*,'Serious problems with qsiaer values'
490	print*,'in callcorrk'
491	call abort
492	endif
493	if(qsiaer(k,nw,iaer).gt.qxiaer(k,nw,iaer))then
494	qsiaer(k,nw,iaer)=qxiaer(k,nw,iaer)
495	endif
496	end do
497
498	end do ! L_LEVELS
499	end do ! naerkind
500
501	!-----------------------------------------------------------------------
502	! Aerosol optical depths
503	!-----------------------------------------------------------------------
504
505	do iaer=1,naerkind ! a bug was here
506	do k=0,nlayer-1
507
508	pweight=(pplay(ig,L_NLAYRAD-k)-pplev(ig,L_NLAYRAD-k+1))/ &
509	(pplev(ig,L_NLAYRAD-k)-pplev(ig,L_NLAYRAD-k+1))
510	temp=aerosol(ig,L_NLAYRAD-k,iaer)/QREFvis3d(ig,L_NLAYRAD-k,iaer)
511	tauaero(2k+2,iaer)=max(temppweight,0.d0)
512	tauaero(2k+3,iaer)=max(temp-tauaero(2k+2,iaer),0.d0)
513
514	end do
515	! boundary conditions
516	tauaero(1,iaer) = tauaero(2,iaer)
517	!tauaero(1,iaer) = 0.
518	!JL18 at time of testing, the two above conditions gave the same results bit for bit.
519
520	end do ! naerkind
521
522	! Albedo and Emissivity.
523	albi=1-emis(ig) ! Long Wave.
524	DO nw=1,L_NSPECTV ! Short Wave loop.
525	albv(nw)=albedo(ig,nw)
526	ENDDO
527
528	if ((ngrid.eq.1).and.(global1d)) then ! Fixed zenith angle 'szangle' in 1D simulations w/ globally-averaged sunlight.
529	acosz = cos(pi*szangle/180.0)
530	print*,'acosz=',acosz,', szangle=',szangle
531	else
532	acosz=mu0(ig) ! Cosine of sun incident angle : 3D simulations or local 1D simulations using latitude.
533	endif
534
535	!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
536	!!! Note by JL13 : In the following, some indices were changed in the interpolations,
537	!!! so that the model results are less dependent on the number of layers !
538	!!!
539	!!! --- The older versions are commented with the comment !JL13index ---
540	!!!
541	!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
542
543
544	!-----------------------------------------------------------------------
545	! Water vapour (to be generalised for other gases eventually ...)
546	!-----------------------------------------------------------------------
547
548	if(varactive)then
549
550	i_var=igcm_h2o_vap
551	do l=1,nlayer
552	qvar(2*l) = pq(ig,nlayer+1-l,i_var)
553	qvar(2*l+1) = pq(ig,nlayer+1-l,i_var)
554	!JL13index qvar(2*l+1) = (pq(ig,nlayer+1-l,i_var)+pq(ig,max(nlayer-l,1),i_var))/2
555	!JL13index ! Average approximation as for temperature...
556	end do
557	qvar(1)=qvar(2)
558
559	elseif(varfixed)then
560
561	do l=1,nlayer ! Here we will assign fixed water vapour profiles globally.
562	RH = satval * ((pplay(ig,l)/pplev(ig,1) - 0.02) / 0.98)
563	if(RH.lt.0.0) RH=0.0
564
565	call Psat_water(pt(ig,l),pplay(ig,l),psat,qsat)
566
567	!pq_temp(l) = qsat ! fully saturated everywhere
568	pq_temp(l) = RH * qsat ! ~realistic profile (e.g. 80% saturation at ground)
569	end do
570
571	do l=1,nlayer
572	qvar(2*l) = pq_temp(nlayer+1-l)
573	qvar(2*l+1) = (pq_temp(nlayer+1-l)+pq_temp(max(nlayer-l,1)))/2
574	end do
575
576	qvar(1)=qvar(2)
577
578	! Lowest layer of atmosphere
579	RH = satval * (1 - 0.02) / 0.98
580	if(RH.lt.0.0) RH=0.0
581
582	qvar(2nlayer+1)= RH qsat ! ~realistic profile (e.g. 80% saturation at ground)
583
584	else
585	do k=1,L_LEVELS
586	qvar(k) = 1.0D-7
587	end do
588	end if ! varactive/varfixed
589
590	if(.not.kastprof)then
591	! IMPORTANT: Now convert from kg/kg to mol/mol.
592	do k=1,L_LEVELS
593	qvar(k) = qvar(k)/(epsi+qvar(k)*(1.-epsi))
594	end do
595	end if
596
597	!-----------------------------------------------------------------------
598	! kcm mode only !
599	!-----------------------------------------------------------------------
600
601	if(kastprof)then
602
603	if(.not.global1d)then ! garde-fou/safeguard added by MT (to be removed in the future)
604	write(,) 'You have to fix mu0, '
605	write(,) 'the cosinus of the solar angle'
606	stop
607	endif
608
609	! Initial values equivalent to mugaz.
610	DO l=1,nlayer
611	muvarrad(2*l) = mugaz
612	muvarrad(2*l+1) = mugaz
613	END DO
614
615	if(ngasmx.gt.1)then
616
617	DO l=1,nlayer
618	muvarrad(2*l) = muvar(ig,nlayer+2-l)
619	muvarrad(2*l+1) = (muvar(ig,nlayer+2-l) + &
620	muvar(ig,max(nlayer+1-l,1)))/2
621	END DO
622
623	muvarrad(1) = muvarrad(2)
624	muvarrad(2*nlayer+1) = muvar(ig,1)
625
626	print*,'Recalculating qvar with VARIABLE epsi for kastprof'
627	print*,'Assumes that the variable gas is H2O!!!'
628	print*,'Assumes that there is only one tracer'
629
630	!i_var=igcm_h2o_vap
631	i_var=1
632
633	if(nq.gt.1)then
634	print*,'Need 1 tracer only to run kcm1d.e'
635	stop
636	endif
637
638	do l=1,nlayer
639	vtmp(l)=pq(ig,l,i_var)/(epsi+pq(ig,l,i_var)*(1.-epsi))
640	!vtmp(l)=pq(ig,l,i_var)*muvar(ig,l+1)/mH2O !JL to be changed
641	end do
642
643	do l=1,nlayer
644	qvar(2*l) = vtmp(nlayer+1-l)
645	qvar(2*l+1) = vtmp(nlayer+1-l)
646	! qvar(2*l+1) = ( vtmp(nlayer+1-l) + vtmp(max(nlayer-l,1)) )/2
647	end do
648	qvar(1)=qvar(2)
649
650	print*,'Warning: reducing qvar in callcorrk.'
651	print*,'Temperature profile no longer consistent ', &
652	'with saturated H2O. qsat=',satval
653
654	do k=1,L_LEVELS
655	qvar(k) = qvar(k)*satval
656	end do
657
658	endif
659	else ! if kastprof
660	DO l=1,nlayer
661	muvarrad(2*l) = muvar(ig,nlayer+2-l)
662	muvarrad(2*l+1) = (muvar(ig,nlayer+2-l)+muvar(ig,max(nlayer+1-l,1)))/2
663	END DO
664
665	muvarrad(1) = muvarrad(2)
666	muvarrad(2*nlayer+1)=muvar(ig,1)
667	endif ! if kastprof
668
669	! Keep values inside limits for which we have radiative transfer coefficients !!!
670	if(L_REFVAR.gt.1)then ! (there was a bug here)
671	do k=1,L_LEVELS
672	if(qvar(k).lt.wrefvar(1))then
673	qvar(k)=wrefvar(1)+1.0e-8
674	elseif(qvar(k).gt.wrefvar(L_REFVAR))then
675	qvar(k)=wrefvar(L_REFVAR)-1.0e-8
676	endif
677	end do
678	endif
679
680	!-----------------------------------------------------------------------
681	! Pressure and temperature
682	!-----------------------------------------------------------------------
683
684	DO l=1,nlayer
685	plevrad(2*l) = pplay(ig,nlayer+1-l)/scalep
686	plevrad(2*l+1) = pplev(ig,nlayer+1-l)/scalep
687	tlevrad(2*l) = pt(ig,nlayer+1-l)
688	tlevrad(2*l+1) = (pt(ig,nlayer+1-l)+pt(ig,max(nlayer-l,1)))/2
689	END DO
690
691	plevrad(1) = 0.
692	! 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.
693
694	tlevrad(1) = tlevrad(2)
695	tlevrad(2*nlayer+1)=tsurf(ig)
696
697	pmid(1) = pplay(ig,nlayer)/scalep
698	pmid(2) = pmid(1)
699
700	tmid(1) = tlevrad(2)
701	tmid(2) = tmid(1)
702
703	DO l=1,L_NLAYRAD-1
704	tmid(2l+1) = tlevrad(2l+1)
705	tmid(2l+2) = tlevrad(2l+1)
706	pmid(2l+1) = plevrad(2l+1)
707	pmid(2l+2) = plevrad(2l+1)
708	END DO
709	pmid(L_LEVELS) = plevrad(L_LEVELS)
710	tmid(L_LEVELS) = tlevrad(L_LEVELS)
711
712	!!Alternative interpolation:
713	! pmid(3) = pmid(1)
714	! pmid(4) = pmid(1)
715	! tmid(3) = tmid(1)
716	! tmid(4) = tmid(1)
717	! DO l=2,L_NLAYRAD-1
718	! tmid(2l+1) = tlevrad(2l)
719	! tmid(2l+2) = tlevrad(2l)
720	! pmid(2l+1) = plevrad(2l)
721	! pmid(2l+2) = plevrad(2l)
722	! END DO
723	! pmid(L_LEVELS) = plevrad(L_LEVELS-1)
724	! tmid(L_LEVELS) = tlevrad(L_LEVELS-1)
725
726	! Test for out-of-bounds pressure.
727	if(plevrad(3).lt.pgasmin)then
728	print*,'Minimum pressure is outside the radiative'
729	print*,'transfer kmatrix bounds, exiting.'
730	call abort
731	elseif(plevrad(L_LEVELS).gt.pgasmax)then
732	print*,'Maximum pressure is outside the radiative'
733	print*,'transfer kmatrix bounds, exiting.'
734	call abort
735	endif
736
737	! Test for out-of-bounds temperature.
738	do k=1,L_LEVELS
739	if(tlevrad(k).lt.tgasmin)then
740	print*,'Minimum temperature is outside the radiative'
741	print*,'transfer kmatrix bounds'
742	print*,"k=",k," tlevrad(k)=",tlevrad(k)
743	print*,"tgasmin=",tgasmin
744	if (strictboundcorrk) then
745	call abort
746	else
747	print,'**********************************************'
748	print*,'we allow model to continue with tlevrad<tgasmin'
749	print*,' ... we assume we know what you are doing ... '
750	print*,' ... but do not let this happen too often ... '
751	print,'**********************************************'
752	!tlevrad(k)=tgasmin ! Used in the source function !
753	endif
754	elseif(tlevrad(k).gt.tgasmax)then
755	print*,'Maximum temperature is outside the radiative'
756	print*,'transfer kmatrix bounds, exiting.'
757	print*,"k=",k," tlevrad(k)=",tlevrad(k)
758	print*,"tgasmax=",tgasmax
759	if (strictboundcorrk) then
760	call abort
761	else
762	print,'**********************************************'
763	print*,'we allow model to continue with tlevrad<tgasmax'
764	print*,' ... we assume we know what you are doing ... '
765	print*,' ... but do not let this happen too often ... '
766	print,'**********************************************'
767	!tlevrad(k)=tgasmax ! Used in the source function !
768	endif
769	endif
770	enddo
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	call abort
779	else
780	print,'**********************************************'
781	print*,'we allow model to continue but with tmid=tgasmin'
782	print*,' ... we assume we know what you are doing ... '
783	print*,' ... but do not let this happen too often ... '
784	print,'**********************************************'
785	tmid(k)=tgasmin
786	endif
787	elseif(tmid(k).gt.tgasmax)then
788	print*,'Maximum temperature is outside the radiative'
789	print*,'transfer kmatrix bounds, exiting.'
790	print*,"k=",k," tmid(k)=",tmid(k)
791	print*,"tgasmax=",tgasmax
792	if (strictboundcorrk) then
793	call abort
794	else
795	print,'**********************************************'
796	print*,'we allow model to continue but with tmid=tgasmin'
797	print*,' ... we assume we know what you are doing ... '
798	print*,' ... but do not let this happen too often ... '
799	print,'**********************************************'
800	tmid(k)=tgasmax
801	endif
802	endif
803	enddo
804
805	!=======================================================================
806	! III. Calling the main radiative transfer subroutines
807	!=======================================================================
808
809
810	Cmk= 0.01 * 1.0 / (glat(ig) * mugaz * 1.672621e-27) ! q_main=1.0 assumed.
811	glat_ig=glat(ig)
812
813	!-----------------------------------------------------------------------
814	! Short Wave Part
815	!-----------------------------------------------------------------------
816
817	if(fract(ig) .ge. 1.0e-4) then ! Only during daylight.
818	if((ngrid.eq.1).and.(global1d))then
819	do nw=1,L_NSPECTV
820	stel_fract(nw)= stel(nw)* 0.25 / acosz ! globally averaged = divide by 4, and we correct for solar zenith angle
821	end do
822	else
823	do nw=1,L_NSPECTV
824	stel_fract(nw)= stel(nw) * fract(ig)
825	end do
826	endif
827
828	call optcv(dtauv,tauv,taucumv,plevrad, &
829	qxvaer,qsvaer,gvaer,wbarv,cosbv,tauray,tauaero, &
830	tmid,pmid,taugsurf,qvar,muvarrad)
831
832	call sfluxv(dtauv,tauv,taucumv,albv,dwnv,wbarv,cosbv, &
833	acosz,stel_fract, &
834	nfluxtopv,fluxtopvdn,nfluxoutv_nu,nfluxgndv_nu, &
835	fmnetv,fluxupv,fluxdnv,fzerov,taugsurf)
836
837	else ! During the night, fluxes = 0.
838	nfluxtopv = 0.0d0
839	fluxtopvdn = 0.0d0
840	nfluxoutv_nu(:) = 0.0d0
841	nfluxgndv_nu(:) = 0.0d0
842	do l=1,L_NLAYRAD
843	fmnetv(l)=0.0d0
844	fluxupv(l)=0.0d0
845	fluxdnv(l)=0.0d0
846	end do
847	end if
848
849
850	! Equivalent Albedo Calculation (for OUTPUT). MT2015
851	if(fract(ig) .ge. 1.0e-4) then ! equivalent albedo makes sense only during daylight.
852	surface_stellar_flux=sum(nfluxgndv_nu(1:L_NSPECTV))
853	if(surface_stellar_flux .gt. 1.0e-3) then ! equivalent albedo makes sense only if the stellar flux received by the surface is positive.
854	DO nw=1,L_NSPECTV
855	albedo_temp(nw)=albedo(ig,nw)*nfluxgndv_nu(nw)
856	ENDDO
857	albedo_temp(1:L_NSPECTV)=albedo_temp(1:L_NSPECTV)/surface_stellar_flux
858	albedo_equivalent(ig)=sum(albedo_temp(1:L_NSPECTV))
859	else
860	albedo_equivalent(ig)=0.0 ! Spectrally Integrated Albedo not defined for non-irradiated grid points. So we arbitrary set the equivalent albedo to 0.
861	endif
862	else
863	albedo_equivalent(ig)=0.0 ! Spectrally Integrated Albedo not defined for non-irradiated grid points. So we arbitrary set the equivalent albedo to 0.
864	endif
865
866
867	!-----------------------------------------------------------------------
868	! Long Wave Part
869	!-----------------------------------------------------------------------
870
871	call optci(plevrad,tlevrad,dtaui,taucumi, &
872	qxiaer,qsiaer,giaer,cosbi,wbari,tauaero,tmid,pmid, &
873	taugsurfi,qvar,muvarrad)
874
875	call sfluxi(plevrad,tlevrad,dtaui,taucumi,ubari,albi, &
876	wnoi,dwni,cosbi,wbari,nfluxtopi,nfluxtopi_nu, &
877	fmneti,fluxupi,fluxdni,fluxupi_nu,fzeroi,taugsurfi)
878
879	!-----------------------------------------------------------------------
880	! Transformation of the correlated-k code outputs
881	! (into dtlw, dtsw, fluxsurf_lw, fluxsurf_sw, fluxtop_lw, fluxtop_sw)
882
883	! Flux incident at the top of the atmosphere
884	fluxtop_dn(ig)=fluxtopvdn
885
886	fluxtop_lw(ig) = real(nfluxtopi)
887	fluxabs_sw(ig) = real(-nfluxtopv)
888	fluxsurf_lw(ig) = real(fluxdni(L_NLAYRAD))
889	fluxsurf_sw(ig) = real(fluxdnv(L_NLAYRAD))
890
891	! Flux absorbed by the surface. By MT2015.
892	fluxsurfabs_sw(ig) = fluxsurf_sw(ig)*(1.-albedo_equivalent(ig))
893
894	if(fluxtop_dn(ig).lt.0.0)then
895	print*,'Achtung! fluxtop_dn has lost the plot!'
896	print*,'fluxtop_dn=',fluxtop_dn(ig)
897	print*,'acosz=',acosz
898	print*,'aerosol=',aerosol(ig,:,:)
899	print*,'temp= ',pt(ig,:)
900	print*,'pplay= ',pplay(ig,:)
901	call abort
902	endif
903
904	! Spectral output, for exoplanet observational comparison
905	if(specOLR)then
906	do nw=1,L_NSPECTI
907	OLR_nu(ig,nw)=nfluxtopi_nu(nw)/DWNI(nw) !JL Normalize to the bandwidth
908	end do
909	do nw=1,L_NSPECTV
910	!GSR_nu(ig,nw)=nfluxgndv_nu(nw)
911	OSR_nu(ig,nw)=nfluxoutv_nu(nw)/DWNV(nw) !JL Normalize to the bandwidth
912	end do
913	endif
914
915	! Finally, the heating rates
916
917	DO l=2,L_NLAYRAD
918	dtsw(ig,L_NLAYRAD+1-l)=(fmnetv(l)-fmnetv(l-1)) &
919	glat(ig)/(cppscalep(plevrad(2l+1)-plevrad(2*l-1)))
920	dtlw(ig,L_NLAYRAD+1-l)=(fmneti(l)-fmneti(l-1)) &
921	glat(ig)/(cppscalep(plevrad(2l+1)-plevrad(2*l-1)))
922	END DO
923
924	! These are values at top of atmosphere
925	dtsw(ig,L_NLAYRAD)=(fmnetv(1)-nfluxtopv) &
926	glat(ig)/(cppscalep*(plevrad(3)-plevrad(2)))
927	dtlw(ig,L_NLAYRAD)=(fmneti(1)-nfluxtopi) &
928	glat(ig)/(cppscalep*(plevrad(3)-plevrad(2)))
929
930	! Optical thickness diagnostics (added by JVO)
931	if (diagdtau) then
932	do l=1,L_NLAYRAD
933	do nw=1,L_NSPECTV
934	int_dtauv(ig,l,nw) = 0.0d0
935	DO k=1,L_NGAUSS
936	! Output exp(-tau) because gweight ponderates exp and not tau itself
937	int_dtauv(ig,l,nw)= int_dtauv(ig,l,nw) + exp(-dtauv(l,nw,k))*gweight(k)
938	ENDDO
939	enddo
940	do nw=1,L_NSPECTI
941	int_dtaui(ig,l,nw) = 0.0d0
942	DO k=1,L_NGAUSS
943	! Output exp(-tau) because gweight ponderates exp and not tau itself
944	int_dtaui(ig,l,nw)= int_dtaui(ig,l,nw) + exp(-dtaui(l,nw,k))*gweight(k)
945	ENDDO
946	enddo
947	enddo
948	endif
949
950
951	!-----------------------------------------------------------------------
952	end do ! End of big loop over every GCM column.
953	!-----------------------------------------------------------------------
954
955
956
957	!-----------------------------------------------------------------------
958	! Additional diagnostics
959	!-----------------------------------------------------------------------
960
961	! IR spectral output, for exoplanet observational comparison
962	if(lastcall.and.(ngrid.eq.1))then ! could disable the 1D output, they are in the diagfi and diagspec... JL12
963
964	print*,'Saving scalar quantities in surf_vals.out...'
965	print*,'psurf = ', pplev(1,1),' Pa'
966	open(116,file='surf_vals.out')
967	write(116,*) tsurf(1),pplev(1,1),fluxtop_dn(1), &
968	real(-nfluxtopv),real(nfluxtopi)
969	close(116)
970
971
972	! USEFUL COMMENT - Do Not Remove.
973	!
974	! if(specOLR)then
975	! open(117,file='OLRnu.out')
976	! do nw=1,L_NSPECTI
977	! write(117,*) OLR_nu(1,nw)
978	! enddo
979	! close(117)
980	!
981	! open(127,file='OSRnu.out')
982	! do nw=1,L_NSPECTV
983	! write(127,*) OSR_nu(1,nw)
984	! enddo
985	! close(127)
986	! endif
987
988	! OLR vs altitude: do it as a .txt file.
989	OLRz=.false.
990	if(OLRz)then
991	print*,'saving IR vertical flux for OLRz...'
992	open(118,file='OLRz_plevs.out')
993	open(119,file='OLRz.out')
994	do l=1,L_NLAYRAD
995	write(118,) plevrad(2l)
996	do nw=1,L_NSPECTI
997	write(119,*) fluxupi_nu(l,nw)
998	enddo
999	enddo
1000	close(118)
1001	close(119)
1002	endif
1003
1004	endif
1005
1006	! See physiq.F for explanations about CLFvarying. This is temporary.
1007	if (lastcall .and. .not.CLFvarying) then
1008	IF( ALLOCATED( gasi ) ) DEALLOCATE( gasi )
1009	IF( ALLOCATED( gasv ) ) DEALLOCATE( gasv )
1010	!$OMP BARRIER
1011	!$OMP MASTER
1012	IF( ALLOCATED( pgasref ) ) DEALLOCATE( pgasref )
1013	IF( ALLOCATED( tgasref ) ) DEALLOCATE( tgasref )
1014	IF( ALLOCATED( wrefvar ) ) DEALLOCATE( wrefvar )
1015	IF( ALLOCATED( pfgasref ) ) DEALLOCATE( pfgasref )
1016	IF( ALLOCATED( gweight ) ) DEALLOCATE( gweight )
1017	!$OMP END MASTER
1018	!$OMP BARRIER
1019	IF ( ALLOCATED(reffrad)) DEALLOCATE(reffrad)
1020	IF ( ALLOCATED(nueffrad)) DEALLOCATE(nueffrad)
1021	endif
1022
1023
1024	end subroutine callcorrk
1025
1026	END MODULE callcorrk_mod

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