source: trunk/LMDZ.MARS/libf/phymars/dimradmars_mod.F90 @ 1747

Last change on this file since 1747 was 1266, checked in by aslmd, 11 years ago

LMDZ.MARS
IMPORTANT CHANGE

  • Remove all reference/use of nlayermx and dimphys.h
  • Made use of automatic arrays whenever arrays are needed with dimension nlayer
  • Remove lots of obsolete reference to dimensions.h
  • Converted iono.h and param_v4.h into corresponding modules

(with embedded subroutine to allocate arrays)
(no arrays allocated if thermosphere not used)

  • Deleted param.h and put contents into module param_v4_h
  • Adapted testphys1d, newstart, etc...
  • Made DATA arrays in param_read to be initialized by subroutine

fill_data_thermos in module param_v4_h

  • Optimized computations in paramfoto_compact (twice less dlog10 calculations)
  • Checked consistency before/after modification in debug mode
  • Checked performance is not impacted (same as before)
File size: 7.7 KB
Line 
1module dimradmars_mod
2!   Declaration and settings for radiative transfer calculations
3!   Initializations and allocations are done in phys_state_var_init
4implicit none
5  ! nflev: number of vertical layer
6  ! ndlon,ndlo2: number of horizontal points
7  ! Splitting of horizontal grid
8  ! NDLO2 and ndomainsz for the splitting in the physics call
9  ! WARNING:  One must have  1 < ndomainsz =< ngrid
10  integer,save :: NFLEV !=nlayer   ! with splitting
11  integer,save :: ndomainsz !=(ngrid-1)/20 + 1
12  integer,save :: NDLON !=ndomainsz  ! with splitting
13  integer,save :: NDLO2 !=NDLON
14
15
16! Number of kind of tracer radiative properties
17! ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
18! naerkind is set by reading callphys.def
19! -- see conf_phys
20! -- value of nsizemax below is comfortably high
21!    but beware in case you add a lot of scatterers
22  INTEGER, SAVE :: naerkind
23
24  ! AS: previously in aerkind.h
25  character*20, SAVE, ALLOCATABLE :: name_iaer(:)  ! name of the scatterers
26  integer iaer_dust_conrath ! Typical dust profiles using a
27                            ! Conrath type analytical equation
28  integer iaer_dust_doubleq ! Dust profile is given by the
29                            ! mass mixing ratio of the two-
30                            ! moment scheme method (doubleq)
31  integer iaer_dust_submicron ! Dust profile is given by a
32                              ! submicron population of dust
33                              ! particles
34  integer iaer_h2o_ice ! Water ice particles
35
36  ! AS: was in aeropacity
37  INTEGER,SAVE,ALLOCATABLE :: iaerdust(:)
38
39  ! AS: was in suaer
40  CHARACTER(LEN=30), SAVE, ALLOCATABLE :: file_id(:,:)
41
42! Reference wavelengths used to compute reference optical depth (m)
43! ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
44  REAL,SAVE,ALLOCATABLE :: longrefir(:),longrefvis(:)
45 
46! Definition of spectral intervals at thermal infrared wavelengths (LW)
47! ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
48  integer,parameter :: nir=4 ! Total number of thermal IR bands
49  integer,parameter :: nuco2=2 ! number of bands in CO2 bands
50  real,parameter :: long1ir=5.E-6 , long2ir=200.E-6
51  real,parameter :: long1co2=1.E+0 / 865.E+2 , long2co2=1.E+0 / 500.E+2
52
53!  Warning : the "nir" thermal IR bands are not ordered by wavelength:
54!      iir=1 : central 15um CO2 bands     
55!      iir=2 : CO2 band wings    [long1co2-long2co2] MINUS central band
56!      iir=3 : 9 um band [long1ir - long1co2]
57!      iir=4 : Far IR    [long2co2 - long2ir]
58   
59!  Definition of spectral interval at solar wavelengths (SW)
60!  ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
61  integer,parameter :: NSUN=2   ! do not change that !
62!  Boundaries of spectral intervals (m) :
63  real,parameter :: long1vis=0.1E-6 , long2vis=0.5E-6 , long3vis=5.E-6
64!  Fraction of solar energy in solar band #1 [long1vis-long2vis] : 0.274490
65!  Fraction of solar energy in solar band #2 [long2vis-long3vis] : 0.725509
66  real,save :: sunfr(2) = (/ 0.274490 , 0.725509 /)
67
68! Maximum number of grain size classes
69! ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
70! This parameter has to be set to the maximum number of particle
71!   sizes contained in the optical parameter database; For example,
72!   if only one grain size is used to describe dust, and 30 are used
73!   to describe water-ice crystals in the visible and 15 in the IR,
74!   nsizemax has to be set to 30.
75! If only one grain size is considered for all the aerosols, set
76!   this parameter to 1 and convolution will be turned off during
77!   the radiative calculations.
78
79  integer, parameter :: nsizemax = 60
80! integer, parameter :: nsizemax = 1
81
82! Various initialisation for LW radiative code
83! ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~
84! npademx : number of Pade coefficients
85! nabsmx : ?
86! nt_pademx : number of temperature intervals for Pade
87
88  integer,parameter :: npademx=4
89  integer,parameter :: nabsmx=2
90  integer,parameter :: nt_pademx=19
91
92!!
93!! variables
94!!
95  REAL,SAVE,ALLOCATABLE :: dtrad(:,:) ! Net atm. radiative heating rate (K.s-1)
96  REAL,SAVE,ALLOCATABLE :: fluxrad_sky(:) ! rad. flux from sky absorbed by surface (W.m-2)
97  REAL,SAVE,ALLOCATABLE :: fluxrad(:) ! Net radiative surface flux (W.m-2)
98  REAL,SAVE,ALLOCATABLE :: albedo(:,:) ! Surface albedo in each solar band
99  REAL,SAVE,ALLOCATABLE :: tauscaling(:)   ! Convertion factor for qdust and Ndust
100! aerosol (dust or ice) extinction optical depth  at reference wavelength
101! "longrefvis" set in dimradmars_mod , for one of the "naerkind"  kind of
102! aerosol optical properties  :
103  REAL,SAVE,ALLOCATABLE :: aerosol(:,:,:)
104  REAL,SAVE,ALLOCATABLE :: nueffdust(:,:) ! Dust effective variance
105
106!! ------------------------------------------------------
107!! AS: what was previously in yomaer
108!   Shortwave
109!   ~~~~~~~~~
110!
111! tauvis: dust optical depth at reference wavelength  ("longrefvis" set
112! in dimradmars_mod : typically longrefvis = 0.67E-6 m, as measured by Viking )
113
114! For the "naerkind" kind of aerosol radiative properties :
115! QVISsQREF  :  Qext / Qext("longrefvis")   <--- For both solar bands
116! omegavis   :  sinle scattering albedo     <--- For both solar bands
117! gvis       :  assymetry factor            <--- For both solar bands
118!
119!   Longwave
120!   ~~~~~~~~
121!
122! For the "naerkind" kind of aerosol radiative properties :
123! QIRsQREF :  Qext / Qext("longrefvis")     <--- For the nir bandes IR
124! omegaIR  :  mean single scattering albedo <--- For the nir bandes IR
125! gIR      :  mean assymetry factor         <--- For the nir bandes IR
126!
127  real,save :: tauvis
128  real,save,allocatable :: QVISsQREF(:,:,:)
129  real,save,allocatable :: omegavis(:,:,:)
130  real,save,allocatable :: gvis(:,:,:)
131  real,save,allocatable :: QIRsQREF(:,:,:)
132  real,save,allocatable :: omegaIR(:,:,:)
133  real,save,allocatable :: gIR(:,:,:)
134! Actual number of grain size classes in each domain for a
135!   given aerosol:
136  integer,save,allocatable :: nsize(:,:)
137! Particle size axis (depend on the kind of aerosol and the
138!   radiation domain)
139  real,save,allocatable :: radiustab(:,:,:)
140! Extinction coefficient at reference wavelengths;
141!   These wavelengths are defined in dimradmars_mod, and called
142!   longrefvis and longrefir.
143  real,save,allocatable :: QREFvis(:,:)
144  real,save,allocatable :: QREFir(:,:)
145  real,save,allocatable :: omegaREFvis(:,:)
146  real,save,allocatable :: omegaREFir(:,:)
147!! ------------------------------------------------------
148
149contains
150
151  subroutine ini_dimradmars_mod(ngrid,nlayer)
152 
153  implicit none
154 
155  integer,intent(in) :: ngrid ! number of atmospheric columns
156  integer,intent(in) :: nlayer ! number of atmospheric layers
157
158   nflev=nlayer
159!  ndomainsz=ngrid
160   ndomainsz=(ngrid-1)/20 + 1
161!  ndomainsz=(ngrid-1)/5 + 1
162   ndlon=ndomainsz
163   ndlo2=ndlon
164
165   allocate(albedo(ngrid,2))
166   allocate(dtrad(ngrid,nlayer))
167   allocate(fluxrad_sky(ngrid))
168   allocate(fluxrad(ngrid))
169   allocate(tauscaling(ngrid))
170   allocate(nueffdust(ngrid,nlayer))
171
172  end subroutine ini_dimradmars_mod
173 
174  subroutine ini_scatterers(ngrid,nlayer)
175
176  implicit none
177
178  integer,intent(in) :: ngrid ! number of atmospheric columns
179  integer,intent(in) :: nlayer ! number of atmospheric layers
180
181   allocate(name_iaer(naerkind))
182   allocate(aerosol(ngrid,nlayer,naerkind))
183   allocate(longrefir(naerkind))
184   allocate(longrefvis(naerkind))
185   allocate(iaerdust(naerkind))
186   allocate(file_id(naerkind,2))
187
188   allocate(QVISsQREF(nsun,naerkind,nsizemax))
189   allocate(omegavis(nsun,naerkind,nsizemax))
190   allocate(gvis(nsun,naerkind,nsizemax))
191   allocate(QIRsQREF(nir,naerkind,nsizemax))
192   allocate(omegaIR(nir,naerkind,nsizemax))
193   allocate(gIR(nir,naerkind,nsizemax))
194   allocate(nsize(naerkind,2))
195   allocate(radiustab(naerkind,2,nsizemax))
196   allocate(QREFvis(naerkind,nsizemax))
197   allocate(QREFir(naerkind,nsizemax))
198   allocate(omegaREFvis(naerkind,nsizemax))
199   allocate(omegaREFir(naerkind,nsizemax))
200
201  end subroutine ini_scatterers
202
203end module dimradmars_mod
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