source: LMDZ6/trunk/libf/phylmd/ecrad/radiation/radiation_adding_ica_lw.F90 @ 5423

Last change on this file since 5423 was 4773, checked in by idelkadi, 13 months ago
  • Update of Ecrad in LMDZ The same organization of the Ecrad offline version is retained in order to facilitate the updating of Ecrad in LMDZ and the comparison between online and offline results. version 1.6.1 of Ecrad (https://github.com/lguez/ecrad.git)
  • Implementation of the double call of Ecrad in LMDZ


File size: 12.9 KB
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1! radiation_adding_ica_lw.F90 - Longwave adding method in independent column approximation
2!
3! (C) Copyright 2015- ECMWF.
4!
5! This software is licensed under the terms of the Apache Licence Version 2.0
6! which can be obtained at http://www.apache.org/licenses/LICENSE-2.0.
7!
8! In applying this licence, ECMWF does not waive the privileges and immunities
9! granted to it by virtue of its status as an intergovernmental organisation
10! nor does it submit to any jurisdiction.
11!
12! Author:  Robin Hogan
13! Email:   r.j.hogan@ecmwf.int
14!
15! Modifications
16!   2017-04-11  R. Hogan  Receive emission/albedo rather than planck/emissivity
17!   2017-07-12  R. Hogan  Fast adding method for if only clouds scatter
18!   2017-10-23  R. Hogan  Renamed single-character variables
19
20module radiation_adding_ica_lw
21
22  public
23
24contains
25
26  !---------------------------------------------------------------------
27  ! Use the scalar "adding" method to compute longwave flux profiles,
28  ! including scattering, by successively adding the contribution of
29  ! layers starting from the surface to compute the total albedo and
30  ! total upward emission of the increasingly larger block of
31  ! atmospheric layers.
32  subroutine adding_ica_lw(ncol, nlev, &
33       &  reflectance, transmittance, source_up, source_dn, emission_surf, albedo_surf, &
34       &  flux_up, flux_dn)
35
36    use parkind1, only           : jprb
37    use yomhook,  only           : lhook, dr_hook, jphook
38
39    implicit none
40
41    ! Inputs
42    integer, intent(in) :: ncol ! number of columns (may be spectral intervals)
43    integer, intent(in) :: nlev ! number of levels
44
45    ! Surface emission (W m-2) and albedo
46    real(jprb), intent(in),  dimension(ncol) :: emission_surf, albedo_surf
47
48    ! Diffuse reflectance and transmittance of each layer
49    real(jprb), intent(in),  dimension(ncol, nlev)   :: reflectance, transmittance
50
51    ! Emission from each layer in an upward and downward direction
52    real(jprb), intent(in),  dimension(ncol, nlev)   :: source_up, source_dn
53
54    ! Resulting fluxes (W m-2) at half-levels: diffuse upwelling and
55    ! downwelling
56    real(jprb), intent(out), dimension(ncol, nlev+1) :: flux_up, flux_dn
57   
58    ! Albedo of the entire earth/atmosphere system below each half
59    ! level
60    real(jprb), dimension(ncol, nlev+1) :: albedo
61
62    ! Upwelling radiation at each half-level due to emission below
63    ! that half-level (W m-2)
64    real(jprb), dimension(ncol, nlev+1) :: source
65
66    ! Equal to 1/(1-albedo*reflectance)
67    real(jprb), dimension(ncol, nlev)   :: inv_denominator
68
69    ! Loop index for model level and column
70    integer :: jlev, jcol
71
72    real(jphook) :: hook_handle
73
74    if (lhook) call dr_hook('radiation_adding_ica_lw:adding_ica_lw',0,hook_handle)
75
76    albedo(:,nlev+1) = albedo_surf
77
78    ! At the surface, the source is thermal emission
79    source(:,nlev+1) = emission_surf
80
81    ! Work back up through the atmosphere and compute the albedo of
82    ! the entire earth/atmosphere system below that half-level, and
83    ! also the "source", which is the upwelling flux due to emission
84    ! below that level
85    do jlev = nlev,1,-1
86      ! Next loop over columns. We could do this by indexing the
87      ! entire inner dimension as follows, e.g. for the first line:
88      !   inv_denominator(:,jlev) = 1.0_jprb / (1.0_jprb-albedo(:,jlev+1)*reflectance(:,jlev))
89      ! and similarly for subsequent lines, but this slows down the
90      ! routine by a factor of 2!  Rather, we do it with an explicit
91      ! loop.
92      do jcol = 1,ncol
93        ! Lacis and Hansen (1974) Eq 33, Shonk & Hogan (2008) Eq 10:
94        inv_denominator(jcol,jlev) = 1.0_jprb &
95             &  / (1.0_jprb-albedo(jcol,jlev+1)*reflectance(jcol,jlev))
96        ! Shonk & Hogan (2008) Eq 9, Petty (2006) Eq 13.81:
97        albedo(jcol,jlev) = reflectance(jcol,jlev) + transmittance(jcol,jlev)*transmittance(jcol,jlev) &
98             &  * albedo(jcol,jlev+1) * inv_denominator(jcol,jlev)
99        ! Shonk & Hogan (2008) Eq 11:
100        source(jcol,jlev) = source_up(jcol,jlev) &
101             &  + transmittance(jcol,jlev) * (source(jcol,jlev+1) &
102             &                    + albedo(jcol,jlev+1)*source_dn(jcol,jlev)) &
103             &                   * inv_denominator(jcol,jlev)
104      end do
105    end do
106
107    ! At top-of-atmosphere there is no diffuse downwelling radiation
108    flux_dn(:,1) = 0.0_jprb
109
110    ! At top-of-atmosphere, all upwelling radiation is due to emission
111    ! below that level
112    flux_up(:,1) = source(:,1)
113
114    ! Work back down through the atmosphere computing the fluxes at
115    ! each half-level
116    do jlev = 1,nlev
117      do jcol = 1,ncol
118        ! Shonk & Hogan (2008) Eq 14 (after simplification):
119        flux_dn(jcol,jlev+1) &
120             &  = (transmittance(jcol,jlev)*flux_dn(jcol,jlev) &
121             &     + reflectance(jcol,jlev)*source(jcol,jlev+1) &
122             &     + source_dn(jcol,jlev)) * inv_denominator(jcol,jlev)
123        ! Shonk & Hogan (2008) Eq 12:
124        flux_up(jcol,jlev+1) = albedo(jcol,jlev+1)*flux_dn(jcol,jlev+1) &
125             &            + source(jcol,jlev+1)
126      end do
127    end do
128
129    if (lhook) call dr_hook('radiation_adding_ica_lw:adding_ica_lw',1,hook_handle)
130
131  end subroutine adding_ica_lw
132
133
134  !---------------------------------------------------------------------
135  ! Use the scalar "adding" method to compute longwave flux profiles,
136  ! including scattering in cloudy layers only.
137  subroutine fast_adding_ica_lw(ncol, nlev, &
138       &  reflectance, transmittance, source_up, source_dn, emission_surf, albedo_surf, &
139       &  is_clear_sky_layer, i_cloud_top, flux_dn_clear, &
140       &  flux_up, flux_dn)
141
142    use parkind1, only           : jprb
143    use yomhook,  only           : lhook, dr_hook, jphook
144
145    implicit none
146
147    ! Inputs
148    integer, intent(in) :: ncol ! number of columns (may be spectral intervals)
149    integer, intent(in) :: nlev ! number of levels
150
151    ! Surface emission (W m-2) and albedo
152    real(jprb), intent(in),  dimension(ncol) :: emission_surf, albedo_surf
153
154    ! Diffuse reflectance and transmittance of each layer
155    real(jprb), intent(in),  dimension(ncol, nlev)   :: reflectance, transmittance
156
157    ! Emission from each layer in an upward and downward direction
158    real(jprb), intent(in),  dimension(ncol, nlev)   :: source_up, source_dn
159
160    ! Determine which layers are cloud-free
161    logical, intent(in) :: is_clear_sky_layer(nlev)
162
163    ! Index to highest cloudy layer
164    integer, intent(in) :: i_cloud_top
165
166    ! Pre-computed clear-sky downwelling fluxes (W m-2) at half-levels
167    real(jprb), intent(in), dimension(ncol, nlev+1)  :: flux_dn_clear
168
169    ! Resulting fluxes (W m-2) at half-levels: diffuse upwelling and
170    ! downwelling
171    real(jprb), intent(out), dimension(ncol, nlev+1) :: flux_up, flux_dn
172   
173    ! Albedo of the entire earth/atmosphere system below each half
174    ! level
175    real(jprb), dimension(ncol, nlev+1) :: albedo
176
177    ! Upwelling radiation at each half-level due to emission below
178    ! that half-level (W m-2)
179    real(jprb), dimension(ncol, nlev+1) :: source
180
181    ! Equal to 1/(1-albedo*reflectance)
182    real(jprb), dimension(ncol, nlev)   :: inv_denominator
183
184    ! Loop index for model level and column
185    integer :: jlev, jcol
186
187    real(jphook) :: hook_handle
188
189    if (lhook) call dr_hook('radiation_adding_ica_lw:fast_adding_ica_lw',0,hook_handle)
190
191    ! Copy over downwelling fluxes above cloud from clear sky
192    flux_dn(:,1:i_cloud_top) = flux_dn_clear(:,1:i_cloud_top)
193
194    albedo(:,nlev+1) = albedo_surf
195   
196    ! At the surface, the source is thermal emission
197    source(:,nlev+1) = emission_surf
198
199    ! Work back up through the atmosphere and compute the albedo of
200    ! the entire earth/atmosphere system below that half-level, and
201    ! also the "source", which is the upwelling flux due to emission
202    ! below that level
203    do jlev = nlev,i_cloud_top,-1
204      if (is_clear_sky_layer(jlev)) then
205        ! Reflectance of this layer is zero, simplifying the expression
206        do jcol = 1,ncol
207          albedo(jcol,jlev) = transmittance(jcol,jlev)*transmittance(jcol,jlev)*albedo(jcol,jlev+1)
208          source(jcol,jlev) = source_up(jcol,jlev) &
209               &  + transmittance(jcol,jlev) * (source(jcol,jlev+1) &
210               &                    + albedo(jcol,jlev+1)*source_dn(jcol,jlev))
211        end do
212      else
213        ! Loop over columns; explicit loop seems to be faster
214        do jcol = 1,ncol
215          ! Lacis and Hansen (1974) Eq 33, Shonk & Hogan (2008) Eq 10:
216          inv_denominator(jcol,jlev) = 1.0_jprb &
217               &  / (1.0_jprb-albedo(jcol,jlev+1)*reflectance(jcol,jlev))
218          ! Shonk & Hogan (2008) Eq 9, Petty (2006) Eq 13.81:
219          albedo(jcol,jlev) = reflectance(jcol,jlev) + transmittance(jcol,jlev)*transmittance(jcol,jlev) &
220               &  * albedo(jcol,jlev+1) * inv_denominator(jcol,jlev)
221          ! Shonk & Hogan (2008) Eq 11:
222          source(jcol,jlev) = source_up(jcol,jlev) &
223               &  + transmittance(jcol,jlev) * (source(jcol,jlev+1) &
224               &                    + albedo(jcol,jlev+1)*source_dn(jcol,jlev)) &
225               &                   * inv_denominator(jcol,jlev)
226        end do
227      end if
228    end do
229
230    ! Compute the fluxes above the highest cloud
231    flux_up(:,i_cloud_top) = source(:,i_cloud_top) &
232         &                 + albedo(:,i_cloud_top)*flux_dn(:,i_cloud_top)
233    do jlev = i_cloud_top-1,1,-1
234      flux_up(:,jlev) = transmittance(:,jlev)*flux_up(:,jlev+1) + source_up(:,jlev)
235    end do
236
237    ! Work back down through the atmosphere from cloud top computing
238    ! the fluxes at each half-level
239    do jlev = i_cloud_top,nlev
240      if (is_clear_sky_layer(jlev)) then
241        do jcol = 1,ncol
242          flux_dn(jcol,jlev+1) = transmittance(jcol,jlev)*flux_dn(jcol,jlev) &
243               &               + source_dn(jcol,jlev)
244          flux_up(jcol,jlev+1) = albedo(jcol,jlev+1)*flux_dn(jcol,jlev+1) &
245               &               + source(jcol,jlev+1)
246        end do
247      else
248        do jcol = 1,ncol
249          ! Shonk & Hogan (2008) Eq 14 (after simplification):
250          flux_dn(jcol,jlev+1) &
251               &  = (transmittance(jcol,jlev)*flux_dn(jcol,jlev) &
252               &     + reflectance(jcol,jlev)*source(jcol,jlev+1) &
253               &     + source_dn(jcol,jlev)) * inv_denominator(jcol,jlev)
254          ! Shonk & Hogan (2008) Eq 12:
255          flux_up(jcol,jlev+1) = albedo(jcol,jlev+1)*flux_dn(jcol,jlev+1) &
256               &               + source(jcol,jlev+1)
257        end do
258      end if
259    end do
260
261    if (lhook) call dr_hook('radiation_adding_ica_lw:fast_adding_ica_lw',1,hook_handle)
262
263  end subroutine fast_adding_ica_lw
264
265
266  !---------------------------------------------------------------------
267  ! If there is no scattering then fluxes may be computed simply by
268  ! passing down through the atmosphere computing the downwelling
269  ! fluxes from the transmission and emission of each layer, and then
270  ! passing back up through the atmosphere to compute the upwelling
271  ! fluxes in the same way.
272  subroutine calc_fluxes_no_scattering_lw(ncol, nlev, &
273       &  transmittance, source_up, source_dn, emission_surf, albedo_surf, flux_up, flux_dn)
274
275    use parkind1, only           : jprb
276    use yomhook,  only           : lhook, dr_hook, jphook
277
278    implicit none
279
280    ! Inputs
281    integer, intent(in) :: ncol ! number of columns (may be spectral intervals)
282    integer, intent(in) :: nlev ! number of levels
283
284    ! Surface emission (W m-2) and albedo
285    real(jprb), intent(in),  dimension(ncol) :: emission_surf, albedo_surf
286
287    ! Diffuse reflectance and transmittance of each layer
288    real(jprb), intent(in),  dimension(ncol, nlev)   :: transmittance
289
290    ! Emission from each layer in an upward and downward direction
291    real(jprb), intent(in),  dimension(ncol, nlev)   :: source_up, source_dn
292
293    ! Resulting fluxes (W m-2) at half-levels: diffuse upwelling and
294    ! downwelling
295    real(jprb), intent(out), dimension(ncol, nlev+1) :: flux_up, flux_dn
296   
297    ! Loop index for model level
298    integer :: jlev, jcol
299
300    real(jphook) :: hook_handle
301
302    if (lhook) call dr_hook('radiation_adding_ica_lw:calc_fluxes_no_scattering_lw',0,hook_handle)
303
304    ! At top-of-atmosphere there is no diffuse downwelling radiation
305    flux_dn(:,1) = 0.0_jprb
306
307    ! Work down through the atmosphere computing the downward fluxes
308    ! at each half-level
309! Added for DWD (2020)
310!NEC$ outerloop_unroll(8)
311    do jlev = 1,nlev
312      do jcol = 1,ncol
313        flux_dn(jcol,jlev+1) = transmittance(jcol,jlev)*flux_dn(jcol,jlev) + source_dn(jcol,jlev)
314      end do
315    end do
316
317    ! Surface reflection and emission
318    flux_up(:,nlev+1) = emission_surf + albedo_surf * flux_dn(:,nlev+1)
319
320    ! Work back up through the atmosphere computing the upward fluxes
321    ! at each half-level
322! Added for DWD (2020)
323!NEC$ outerloop_unroll(8)
324    do jlev = nlev,1,-1
325      do jcol = 1,ncol
326        flux_up(jcol,jlev) = transmittance(jcol,jlev)*flux_up(jcol,jlev+1) + source_up(jcol,jlev)
327      end do
328    end do
329   
330    if (lhook) call dr_hook('radiation_adding_ica_lw:calc_fluxes_no_scattering_lw',1,hook_handle)
331
332  end subroutine calc_fluxes_no_scattering_lw
333
334end module radiation_adding_ica_lw
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