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module_mp_morr_two_moment.f90
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module_mp_morr_two_moment.f90
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!WRF:MODEL_LAYER:PHYSICS
!
! THIS MODULE CONTAINS THE TWO-MOMENT MICROPHYSICS CODE DESCRIBED BY
! MORRISON ET AL. (2009, MWR)
! CHANGES FOR V3.2, RELATIVE TO MOST RECENT (BUG-FIX) CODE FOR V3.1
! 1) ADDED ACCELERATED MELTING OF GRAUPEL/SNOW DUE TO COLLISION WITH RAIN, FOLLOWING LIN ET AL. (1983)
! 2) INCREASED MINIMUM LAMBDA FOR RAIN, AND ADDED RAIN DROP BREAKUP FOLLOWING MODIFIED VERSION
! OF VERLINDE AND COTTON (1993)
! 3) CHANGE MINIMUM ALLOWED MIXING RATIOS IN DRY CONDITIONS (RH < 90%), THIS IMPROVES RADAR REFLECTIIVITY
! IN LOW REFLECTIVITY REGIONS
! 4) BUG FIX TO MAXIMUM ALLOWED PARTICLE FALLSPEEDS AS A FUNCTION OF AIR DENSITY
! 5) BUG FIX TO CALCULATION OF LIQUID WATER SATURATION VAPOR PRESSURE (CHANGE IS VERY MINOR)
! 6) INCLUDE WRF CONSTANTS PER SUGGESTION OF JIMY
! bug fix, 5/12/10
! 7) bug fix for saturation vapor pressure in low pressure, to avoid division by zero
! 8) include 'EP2' WRF constant for saturation mixing ratio calculation, instead of hardwire constant
! CHANGES FOR V3.3
! 1) MODIFICATION FOR COUPLING WITH WRF-CHEM (PREDICTED DROPLET NUMBER CONCENTRATION) AS AN OPTION
! 2) MODIFY FALLSPEED BELOW THE LOWEST LEVEL OF PRECIPITATION, WHICH PREVENTS
! POTENTIAL FOR SPURIOUS ACCUMULATION OF PRECIPITATION DURING SUB-STEPPING FOR SEDIMENTATION
! 3) BUG FIX TO LATENT HEAT RELEASE DUE TO COLLISIONS OF CLOUD ICE WITH RAIN
! 4) CLEAN UP OF COMMENTS IN THE CODE
! additional minor bug fixes and small changes, 5/30/2011
! minor revisions by A. Ackerman April 2011:
! 1) replaced kinematic with dynamic viscosity
! 2) replaced scaling by air density for cloud droplet sedimentation
! with viscosity-dependent Stokes expression
! 3) use Ikawa and Saito (1991) air-density scaling for cloud ice
! 4) corrected typo in 2nd digit of ventilation constant F2R
! additional fixes:
! 5) TEMPERATURE FOR ACCELERATED MELTING DUE TO COLLIIONS OF SNOW AND GRAUPEL
! WITH RAIN SHOULD USE CELSIUS, NOT KELVIN (BUG REPORTED BY K. VAN WEVERBERG)
! 6) NPRACS IS NOT SUBTRACTED FROM SNOW NUMBER CONCENTRATION, SINCE
! DECREASE IN SNOW NUMBER IS ALREADY ACCOUNTED FOR BY NSMLTS
! 7) fix for switch for running w/o graupel/hail (cloud ice and snow only)
! hm bug fix 3/16/12
! 1) very minor change to limits on autoconversion source of rain number when cloud water is depleted
! WRFV3.5
! hm/A. Ackerman bug fix 11/08/12
! 1) for accelerated melting from collisions, should use rain mass collected by snow, not snow mass
! collected by rain
! 2) minor changes to some comments
! 3) reduction of maximum-allowed ice concentration from 10 cm-3 to 0.3
! cm-3. This was done to address the problem of excessive and persistent
! anvil cirrus produced by the scheme.
! CHANGES FOR WRFV3.5.1
! 1) added output for snow+cloud ice and graupel time step and accumulated
! surface precipitation
! 2) bug fix to option w/o graupel/hail (IGRAUP = 1), include PRACI, PGSACW,
! and PGRACS as sources for snow instead of graupel/hail, bug reported by
! Hailong Wang (PNNL)
! 3) very minor fix to immersion freezing rate formulation (negligible impact)
! 4) clarifications to code comments
! 5) minor change to shedding of rain, remove limit so that the number of
! collected drops can smaller than number of shed drops
! 6) change of specific heat of liquid water from 4218 to 4187 J/kg/K
! CHANGES FOR WRFV3.6.1
! 1) minor bug fix to melting of snow and graupel, an extra factor of air density (RHO) was removed
! from the calculation of PSMLT and PGMLT
! 2) redundant initialization of PSMLT (non answer-changing)
! CHANGES FOR WRFV3.8.1
! 1) changes and cleanup of code comments
! 2) correction to universal gas constant (very small change)
!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
! THIS SCHEME IS A BULK DOUBLE-MOMENT SCHEME THAT PREDICTS MIXING
! RATIOS AND NUMBER CONCENTRATIONS OF FIVE HYDROMETEOR SPECIES:
! CLOUD DROPLETS, CLOUD (SMALL) ICE, RAIN, SNOW, AND GRAUPEL/HAIL.
#define KVALUE 20
#define JVALUE 11
#define IVALUE 20
#ifdef MARS_MORR_DEBUG
#define CALL_DEBUG(a,b) call debugval(a,b)
#endif
MODULE MODULE_MP_MORR_TWO_MOMENT
USE module_wrf_error
! USE module_utility, ONLY: WRFU_Clock, WRFU_Alarm ! GT
! USE module_domain, ONLY : HISTORY_ALARM, Is_alarm_tstep ! GT
! USE WRF PHYSICS CONSTANTS
use module_model_constants, ONLY: CP, G, R => r_d, RV => r_v, EP_2
#ifdef WRF_MARS
use module_model_constants, only: co2_molmass, co2_molrad, N_avogadro, kboltz => bk, &
mass_h2o, mass_co2, h2o_molrad, PI_S,SQRTPI
use module_planet_utilities, only : esat, tfrost_co2, prep_gaussian_weights
#endif
! USE module_state_description
IMPLICIT NONE
#if ( WRF_MARS == 1 )
REAL, PARAMETER :: PI = PI_S
#else
REAL, PARAMETER :: PI = 3.1415926535897932384626434
#endif
REAL, PARAMETER :: xxx = 0.9189385332046727417803297
PUBLIC :: MP_MORR_TWO_MOMENT
#ifdef WRF_MARS
PUBLIC :: constrain_mars_waterice, constrain_mars_dust, average_mass_of_particle
#endif
PUBLIC :: POLYSVP
PRIVATE :: GAMMA, DERF1
PRIVATE :: PI, xxx
PRIVATE :: MORR_TWO_MOMENT_MICRO
#ifdef WRF_MARS
! set this to true to get error messages if we're getting anything other than
! a vapour<->ice<-cloud system (it shouldn't rain on Mars - at least not today!)
LOGICAL, PARAMETER :: debug = .true.
! should probably have a namelist flag that comes through that allows this code to
! only treat dust for if we're running the two-moment dust but with water off
! - can't do the inverse of this since there is no homogeneous nucleation (i.e.
! homogeneous nuc is so hard in the Mars environment that it probably does not
! happen)
#endif
!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
! SWITCHES FOR MICROPHYSICS SCHEME
! IACT = 1, USE POWER-LAW CCN SPECTRA, NCCN = CS^K
! IACT = 2, USE LOGNORMAL AEROSOL SIZE DIST TO DERIVE CCN SPECTRA
! IACT = 3, ACTIVATION CALCULATED IN MODULE_MIXACTIVATE
INTEGER, PRIVATE :: IACT
! INUM = 0, PREDICT DROPLET CONCENTRATION
! INUM = 1, ASSUME CONSTANT DROPLET CONCENTRATION
! !!!NOTE: PREDICTED DROPLET CONCENTRATION NOT AVAILABLE IN THIS VERSION
! CONTACT HUGH MORRISON (morrison@ucar.edu) FOR FURTHER INFORMATION
INTEGER, PRIVATE :: INUM
! FOR INUM = 1, SET CONSTANT DROPLET CONCENTRATION (CM-3)
REAL, PRIVATE :: NDCNST
! SWITCH FOR LIQUID-ONLY RUN
! ILIQ = 0, INCLUDE ICE
! ILIQ = 1, LIQUID ONLY, NO ICE
INTEGER, PRIVATE :: ILIQ
! SWITCH FOR ICE NUCLEATION
! INUC = 0, USE FORMULA FROM RASMUSSEN ET AL. 2002 (MID-LATITUDE)
! = 1, USE MPACE OBSERVATIONS
#ifdef WRF_MARS
! = 2, USE HETEROGENEOUS NUC ON DUST FOR MARS INC. CZICZO [2013] CONTACT PARAM VAR WITH T
! = 3, pseudo homogeneous ice nucleation following simple water scheme
! = 4, pseudo heterogeneous ice nucleation with growth
! = 5, pseudo heterogeneous ice nucleation requiring dust presence, with growth
! = 6, heterogeneous ice nucleation, omg.
logical, private :: mars_heterogeneous, mars_growth, mars_dust_scavenging, &
nucleation_monolayer, nucleation_surface_diffusion
real, private :: nucleation_m
#endif
INTEGER, PRIVATE :: INUC
! IBASE = 1, NEGLECT DROPLET ACTIVATION AT LATERAL CLOUD EDGES DUE TO
! UNRESOLVED ENTRAINMENT AND MIXING, ACTIVATE
! AT CLOUD BASE OR IN REGION WITH LITTLE CLOUD WATER USING
! NON-EQULIBRIUM SUPERSATURATION,
! IN CLOUD INTERIOR ACTIVATE USING EQUILIBRIUM SUPERSATURATION
! IBASE = 2, ASSUME DROPLET ACTIVATION AT LATERAL CLOUD EDGES DUE TO
! UNRESOLVED ENTRAINMENT AND MIXING DOMINATES,
! ACTIVATE DROPLETS EVERYWHERE IN THE CLOUD USING NON-EQUILIBRIUM
! SUPERSATURATION, BASED ON THE
! LOCAL SUB-GRID AND/OR GRID-SCALE VERTICAL VELOCITY
! AT THE GRID POINT
! NOTE: ONLY USED FOR PREDICTED DROPLET CONCENTRATION (INUM = 0) IN NON-WRF-CHEM VERSION OF CODE
INTEGER, PRIVATE :: IBASE
! INCLUDE SUB-GRID VERTICAL VELOCITY IN DROPLET ACTIVATION
! ISUB = 0, INCLUDE SUB-GRID W (RECOMMENDED FOR LOWER RESOLUTION)
! ISUB = 1, EXCLUDE SUB-GRID W, ONLY USE GRID-SCALE W
! NOTE: ONLY USED FOR PREDICTED DROPLET CONCENTRATION (INUM = 0) IN NON-WRF-CHEM VERSION OF CODE
INTEGER, PRIVATE :: ISUB
! SWITCH FOR GRAUPEL/NO GRAUPEL
! IGRAUP = 0, INCLUDE GRAUPEL
! IGRAUP = 1, NO GRAUPEL
INTEGER, PRIVATE :: IGRAUP
! HM ADDED NEW OPTION FOR HAIL
! SWITCH FOR HAIL/GRAUPEL
! IHAIL = 0, DENSE PRECIPITATING ICE IS GRAUPEL
! IHAIL = 1, DENSE PRECIPITATING GICE IS HAIL
INTEGER, PRIVATE :: IHAIL
! CLOUD MICROPHYSICS CONSTANTS
REAL, PRIVATE :: AI,AC,AS,AR,AG ! 'A' PARAMETER IN FALLSPEED-DIAM RELATIONSHIP
REAL, PRIVATE :: BI,BC,BS,BR,BG ! 'B' PARAMETER IN FALLSPEED-DIAM RELATIONSHIP
! REAL, PRIVATE :: R ! GAS CONSTANT FOR AIR
! REAL, PRIVATE :: RV ! GAS CONSTANT FOR WATER VAPOR
! REAL, PRIVATE :: CP ! SPECIFIC HEAT AT CONSTANT PRESSURE FOR DRY AIR
REAL, PRIVATE :: RHOSU ! STANDARD AIR DENSITY AT 850 MB
REAL, PRIVATE :: RHOW ! DENSITY OF LIQUID WATER
REAL, PRIVATE :: RHOI ! BULK DENSITY OF CLOUD ICE
REAL, PRIVATE :: RHOSN ! BULK DENSITY OF SNOW
REAL, PRIVATE :: RHOG ! BULK DENSITY OF GRAUPEL
REAL, PRIVATE :: AIMM ! PARAMETER IN BIGG IMMERSION FREEZING
REAL, PRIVATE :: BIMM ! PARAMETER IN BIGG IMMERSION FREEZING
REAL, PRIVATE :: ECR ! COLLECTION EFFICIENCY BETWEEN DROPLETS/RAIN AND SNOW/RAIN
REAL, PRIVATE :: DCS ! THRESHOLD SIZE FOR CLOUD ICE AUTOCONVERSION
REAL, PRIVATE :: MI0 ! INITIAL SIZE OF NUCLEATED CRYSTAL
REAL, PRIVATE :: MG0 ! MASS OF EMBRYO GRAUPEL
REAL, PRIVATE :: F1S ! VENTILATION PARAMETER FOR SNOW
REAL, PRIVATE :: F2S ! VENTILATION PARAMETER FOR SNOW
REAL, PRIVATE :: F1R ! VENTILATION PARAMETER FOR RAIN
REAL, PRIVATE :: F2R ! VENTILATION PARAMETER FOR RAIN
! REAL, PRIVATE :: G ! GRAVITATIONAL ACCELERATION
REAL, PRIVATE :: QSMALL ! SMALLEST ALLOWED HYDROMETEOR MIXING RATIO
REAL, PRIVATE :: CI,DI,CS,DS,CG,DG ! SIZE DISTRIBUTION PARAMETERS FOR CLOUD ICE, SNOW, GRAUPEL
REAL, PRIVATE :: EII ! COLLECTION EFFICIENCY, ICE-ICE COLLISIONS
REAL, PRIVATE :: ECI ! COLLECTION EFFICIENCY, ICE-DROPLET COLLISIONS
REAL, PRIVATE :: RIN ! RADIUS OF CONTACT NUCLEI (M)
! hm, add for V3.2
REAL, PRIVATE :: CPW ! SPECIFIC HEAT OF LIQUID WATER
! CCN SPECTRA FOR IACT = 1
REAL, PRIVATE :: C1 ! 'C' IN NCCN = CS^K (CM-3)
REAL, PRIVATE :: K1 ! 'K' IN NCCN = CS^K
! AEROSOL PARAMETERS FOR IACT = 2
REAL, PRIVATE :: MW ! MOLECULAR WEIGHT WATER (KG/MOL)
REAL, PRIVATE :: OSM ! OSMOTIC COEFFICIENT
REAL, PRIVATE :: VI ! NUMBER OF ION DISSOCIATED IN SOLUTION
REAL, PRIVATE :: EPSM ! AEROSOL SOLUBLE FRACTION
REAL, PRIVATE :: RHOA ! AEROSOL BULK DENSITY (KG/M3)
REAL, PRIVATE :: MAP ! MOLECULAR WEIGHT AEROSOL (KG/MOL)
REAL, PRIVATE :: MA ! MOLECULAR WEIGHT OF 'AIR' (KG/MOL)
REAL, PRIVATE :: RR ! UNIVERSAL GAS CONSTANT
REAL, PRIVATE :: BACT ! ACTIVATION PARAMETER
REAL, PRIVATE :: RM1 ! GEOMETRIC MEAN RADIUS, MODE 1 (M)
REAL, PRIVATE :: RM2 ! GEOMETRIC MEAN RADIUS, MODE 2 (M)
REAL, PRIVATE :: NANEW1 ! TOTAL AEROSOL CONCENTRATION, MODE 1 (M^-3)
REAL, PRIVATE :: NANEW2 ! TOTAL AEROSOL CONCENTRATION, MODE 2 (M^-3)
REAL, PRIVATE :: SIG1 ! STANDARD DEVIATION OF AEROSOL S.D., MODE 1
REAL, PRIVATE :: SIG2 ! STANDARD DEVIATION OF AEROSOL S.D., MODE 2
REAL, PRIVATE :: F11 ! CORRECTION FACTOR FOR ACTIVATION, MODE 1
REAL, PRIVATE :: F12 ! CORRECTION FACTOR FOR ACTIVATION, MODE 1
REAL, PRIVATE :: F21 ! CORRECTION FACTOR FOR ACTIVATION, MODE 2
REAL, PRIVATE :: F22 ! CORRECTION FACTOR FOR ACTIVATION, MODE 2
REAL, PRIVATE :: MMULT ! MASS OF SPLINTERED ICE PARTICLE
REAL, PRIVATE :: LAMMAXI,LAMMINI,LAMMAXR,LAMMINR,LAMMAXS,LAMMINS,LAMMAXG,LAMMING
#ifdef WRF_MARS
REAL, PRIVATE :: LAMMAXD, LAMMIND, LAMDEFD, LAMD, DUST_CONS0, DUST_CONS1, DUST_CONS2, DUST_CONS3, dust_cons3_a, DUST_MU, &
DUST_CONS_A_SEDIM, DUST_CONS_B_SEDIM, DUST_CONS_E_SEDIM, DUST_PIRHOD, DUST_CONS_RHO, &
DUST_CONS_INV_G1, DUST_CONS_INV_G4, DUST_CONS_G3,&
nfac_lammaxd1, nfac_lammind1, nfac_lammaxd4, nfac_lammind4, &
nfac_lamdefd1, nfac_lamdefd4
real(kind(0.d0)) :: dust_mu_r8
real, private :: ice_consmin_q_n, ice_consmax_q_n, lammind_q_n, lammaxd_q_n, lamdefd_q_n
! real, private :: lamdefi,nfac_lamdefd1, nfac_lamdefd4
integer, private :: DISTRIBUTION_MARS_DUST
real, private :: sigma_squared
real, private :: dust_reff_max, dust_reff_min, dust_reff_default
real, private :: ln_dust_reff_max, ln_dust_reff_min, ln_dust_reff_default
!ice constants
real, private :: ice_mu, ice_cons12, ice_cons11, ice_cons10, ice_cons2
real, private :: ice_cons11min, ice_cons11max, ice_cons10min, ice_cons10max
real, private :: ice_cons_nuc_m0,ice_cons_nuc_m2,ice_cons_nuc_m3
real, private :: ice_cons_nuc_m0p5,ice_cons_nuc_m2p5,ice_cons_nuc_m3p5
real, private :: homogeneous_ice_number_cons1
!nucleation
real, private :: ice_cons_prefactor
real, private :: water_molec_volume, water_molec_radius
real, dimension(:,:), allocatable :: hc_data
integer :: hc_ncolumns, hc_nrows
real :: hc_tmin, hc_deltaT
real :: photolysis_scrit
#endif
! CONSTANTS TO IMPROVE EFFICIENCY
REAL, PRIVATE :: CONS1,CONS2,CONS3,CONS4,CONS5,CONS6,CONS7,CONS8,CONS9,CONS10
REAL, PRIVATE :: CONS11,CONS12,CONS13,CONS14,CONS15,CONS16,CONS17,CONS18,CONS19,CONS20
REAL, PRIVATE :: CONS21,CONS22,CONS23,CONS24,CONS25,CONS26,CONS27,CONS28,CONS29,CONS30
REAL, PRIVATE :: CONS31,CONS32,CONS33,CONS34,CONS35,CONS36,CONS37,CONS38,CONS39,CONS40
REAL, PRIVATE :: CONS41
logical :: iprint, jprint
!bin scheme
integer, parameter :: nbins=6
real(kind(0.d0)), dimension(nbins) :: number, mass
real(kind(0.d0)), dimension(nbins) :: diam, vol, bin_width
real(kind(0.d0)), dimension(2,nbins) :: weights_pos
real(kind(0.d0)), dimension(nbins+1) :: diam_edges
#ifdef MARS_MORR_DEBUG
interface debugval
module procedure debugvaldouble, debugvalsingle, debugvalint,debugvallogical
end interface
#endif
CONTAINS
#ifdef MARS_MORR_DEBUG
subroutine debugvallogical(name, value)
implicit none
character(len=*), intent(in) :: name
logical, intent(in) :: value
if (iprint) write(*,*) name, " = ", value
end subroutine debugvallogical
subroutine debugvalint(name, value)
implicit none
character(len=*), intent(in) :: name
integer, intent(in) :: value
if (iprint) write(*,*) name, " = ", value
end subroutine debugvalint
subroutine debugvaldouble(name, value)
implicit none
character(len=*), intent(in) :: name
real(kind(0.d0)), intent(in) :: value
if (iprint) write(*,*) name, " = ", value
end subroutine debugvaldouble
subroutine debugvalsingle(name, value)
implicit none
character(len=*), intent(in) :: name
real, intent(in) :: value
if (iprint) write(*,*) name, " = ", value
end subroutine debugvalsingle
#endif
!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
SUBROUTINE MORR_TWO_MOMENT_INIT( &
#ifdef WRF_MARS
rho_dust &
,rhod_h2oi &
,reff &
,veff &
,a_dust_sedim &
,b_dust_sedim &
,e_dust_sedim &
,dust_distribution &
,homogeneous_ice_reff &
,mars_ice_nucleation &
,mars_nucleation_surface_diffusion &
,mars_nucleation_monolayer &
,mars_nucleation_m &
,nucleation_filename &
#endif
)
!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
! THIS SUBROUTINE INITIALIZES ALL PHYSICAL CONSTANTS AMND PARAMETERS
! NEEDED BY THE MICROPHYSICS SCHEME.
! NEEDS TO BE CALLED AT FIRST TIME STEP, PRIOR TO CALL TO MAIN MICROPHYSICS INTERFACE
!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
IMPLICIT NONE
#ifdef WRF_MARS
real, intent(in) :: rho_dust, &
rhod_h2oi, &
reff, &
veff, &
a_dust_sedim, &
b_dust_sedim, &
e_dust_sedim
real, intent(in) :: homogeneous_ice_reff
integer, intent(in) :: dust_distribution, mars_ice_nucleation
logical, intent(in) :: mars_nucleation_monolayer, mars_nucleation_surface_diffusion
real, intent(in) :: mars_nucleation_m
character(len=*), intent(in) :: nucleation_filename
real :: volratio, diamratio
real :: bin_min_diam, bin_max_diam, bin_edge_min_diam, bin_edge_max_diam
real(kind(0.d0)), dimension(nbins+1) :: gloc
#endif
integer n,i
real(kind(0.d0)) :: pans, qans, fmin, fmax
!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
! THE FOLLOWING PARAMETERS ARE USER-DEFINED SWITCHES AND NEED TO BE
! SET PRIOR TO CODE COMPILATION
! INUM IS AUTOMATICALLY SET TO 0 FOR WRF-CHEM BELOW,
! ALLOWING PREDICTION OF DROPLET CONCENTRATION
! THUS, THIS PARAMETER SHOULD NOT BE CHANGED HERE
! AND SHOULD BE LEFT TO 1
INUM = 1
! SET CONSTANT DROPLET CONCENTRATION (UNITS OF CM-3)
! IF NO COUPLING WITH WRF-CHEM
NDCNST = 250.
!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
! NOTE, THE FOLLOWING OPTIONS RELATED TO DROPLET ACTIVATION
! (IACT, IBASE, ISUB) ARE NOT AVAILABLE IN CURRENT VERSION
! FOR WRF-CHEM, DROPLET ACTIVATION IS PERFORMED
! IN 'MIX_ACTIVATE', NOT IN MICROPHYSICS SCHEME
! IACT = 1, USE POWER-LAW CCN SPECTRA, NCCN = CS^K
! IACT = 2, USE LOGNORMAL AEROSOL SIZE DIST TO DERIVE CCN SPECTRA
IACT = 2
! IBASE = 1, NEGLECT DROPLET ACTIVATION AT LATERAL CLOUD EDGES DUE TO
! UNRESOLVED ENTRAINMENT AND MIXING, ACTIVATE
! AT CLOUD BASE OR IN REGION WITH LITTLE CLOUD WATER USING
! NON-EQULIBRIUM SUPERSATURATION ASSUMING NO INITIAL CLOUD WATER,
! IN CLOUD INTERIOR ACTIVATE USING EQUILIBRIUM SUPERSATURATION
! IBASE = 2, ASSUME DROPLET ACTIVATION AT LATERAL CLOUD EDGES DUE TO
! UNRESOLVED ENTRAINMENT AND MIXING DOMINATES,
! ACTIVATE DROPLETS EVERYWHERE IN THE CLOUD USING NON-EQUILIBRIUM
! SUPERSATURATION ASSUMING NO INITIAL CLOUD WATER, BASED ON THE
! LOCAL SUB-GRID AND/OR GRID-SCALE VERTICAL VELOCITY
! AT THE GRID POINT
! NOTE: ONLY USED FOR PREDICTED DROPLET CONCENTRATION (INUM = 0)
IBASE = 2
! INCLUDE SUB-GRID VERTICAL VELOCITY (standard deviation of w) IN DROPLET ACTIVATION
! ISUB = 0, INCLUDE SUB-GRID W (RECOMMENDED FOR LOWER RESOLUTION)
! currently, sub-grid w is constant of 0.5 m/s (not coupled with PBL/turbulence scheme)
! ISUB = 1, EXCLUDE SUB-GRID W, ONLY USE GRID-SCALE W
! NOTE: ONLY USED FOR PREDICTED DROPLET CONCENTRATION (INUM = 0)
ISUB = 0
!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
! SWITCH FOR LIQUID-ONLY RUN
! ILIQ = 0, INCLUDE ICE
! ILIQ = 1, LIQUID ONLY, NO ICE
ILIQ = 0
! SWITCH FOR ICE NUCLEATION
! INUC = 0, USE FORMULA FROM RASMUSSEN ET AL. 2002 (MID-LATITUDE)
! = 1, USE MPACE OBSERVATIONS (ARCTIC ONLY)
#ifdef WRF_MARS
! = 2, USE MARS HETERO NUC ON DUST AND CONTACT PARAM TEMPERATURE DEPENDENCE
nucleation_monolayer = .false.
nucleation_surface_diffusion=.true.
nucleation_m = 0.954
nucleation_monolayer = mars_nucleation_monolayer
nucleation_surface_diffusion = mars_nucleation_surface_diffusion
nucleation_surface_diffusion = mars_nucleation_surface_diffusion
nucleation_m = mars_nucleation_m
INUC = mars_ice_nucleation
mars_heterogeneous = .false.
mars_growth=.false.
mars_dust_scavenging = .true.
if(inuc.ge.4) then
mars_growth=.true.
endif
if (inuc.eq.6 .or. inuc.eq.7) then
mars_heterogeneous = .true.
if(inuc .eq. 7) mars_dust_scavenging = .false.
!call load_heterogeneous_coefficients(nucleation_filename)
endif
#else
INUC = 0
#endif
! SWITCH FOR GRAUPEL/HAIL NO GRAUPEL/HAIL
! IGRAUP = 0, INCLUDE GRAUPEL/HAIL
! IGRAUP = 1, NO GRAUPEL/HAIL
#ifdef WRF_MARS
IGRAUP=1
#else
IGRAUP = 0
#endif
! HM ADDED 11/7/07
! SWITCH FOR HAIL/GRAUPEL
! IHAIL = 0, DENSE PRECIPITATING ICE IS GRAUPEL
! IHAIL = 1, DENSE PRECIPITATING ICE IS HAIL
! NOTE ---> RECOMMEND IHAIL = 1 FOR CONTINENTAL DEEP CONVECTION
IHAIL = 0
!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
! SET PHYSICAL CONSTANTS
! FALLSPEED PARAMETERS (V=AD^B)
AI = 700.
AC = 3.E7
AS = 11.72
AR = 841.99667
BI = 1.
BC = 2.
BS = 0.41
BR = 0.8
IF (IHAIL.EQ.0) THEN
AG = 19.3
BG = 0.37
ELSE ! (MATSUN AND HUGGINS 1980)
AG = 114.5
BG = 0.5
END IF
! CONSTANTS AND PARAMETERS
! R = 287.15
! RV = 461.5
! CP = 1005.
RHOSU = 85000./(287.15*273.15)
RHOW = 997.
#ifdef WRF_MARS
RHOI = rhod_h2oi
#else
RHOI = 500.
#endif
RHOSN = 100.
IF (IHAIL.EQ.0) THEN
RHOG = 400.
ELSE
RHOG = 900.
END IF
AIMM = 0.66
BIMM = 100.
ECR = 1.
#ifdef WRF_MARS
! Need to think about what cutoff size for ice vs. clouds. This must
! surely be something we estimate from the stokes-cunnigham to make it
! general - which means we need some cutoff fall speed above which we
! say it is snow
DCS = 125.E-6 ! cutoff or transition diameter (ice-snow) in meters
MI0 = 4./3.*PI*RHOI*(10.E-6)**3 ! initial nucleated ice particle mass
#else
DCS = 125.E-6
MI0 = 4./3.*PI*RHOI*(10.E-6)**3
#endif
MG0 = 1.6E-10
F1S = 0.86
F2S = 0.28
F1R = 0.78
! F2R = 0.32
! fix 053011
F2R = 0.308
! G = 9.806
QSMALL = 1.E-14
EII = 0.1
ECI = 0.7
! HM, ADD FOR V3.2
! hm, 7/23/13
! CPW = 4218.
CPW = 4187.
! SIZE DISTRIBUTION PARAMETERS
CI = RHOI*PI/6.
DI = 3.
CS = RHOSN*PI/6.
DS = 3.
CG = RHOG*PI/6.
DG = 3.
! RADIUS OF CONTACT NUCLEI
RIN = 0.1E-6
MMULT = 4./3.*PI*RHOI*(5.E-6)**3
! SIZE LIMITS FOR LAMBDA
#ifdef WRF_MARS
LAMMAXI = 1./5.E-7
LAMMINI = 1./(2.*DCS+100.E-6)
LAMMAXR = 1./1.E-6
! LAMMINR = 1./500.E-6
LAMMINR = 1./2800.E-6
#else
LAMMAXI = 1./1.E-6
LAMMINI = 1./(2.*DCS+100.E-6)
LAMMAXR = 1./20.E-6
! LAMMINR = 1./500.E-6
LAMMINR = 1./2800.E-6
#endif
LAMMAXS = 1./10.E-6
LAMMINS = 1./2000.E-6
LAMMAXG = 1./20.E-6
LAMMING = 1./2000.E-6
!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
! note: these parameters only used by the non-wrf-chem version of the
! scheme with predicted droplet number
! CCN SPECTRA FOR IACT = 1
! MARITIME
! MODIFIED FROM RASMUSSEN ET AL. 2002
! NCCN = C*S^K, NCCN IS IN CM-3, S IS SUPERSATURATION RATIO IN %
K1 = 0.4
C1 = 120.
! CONTINENTAL
! K1 = 0.5
! C1 = 1000.
! AEROSOL ACTIVATION PARAMETERS FOR IACT = 2
! PARAMETERS CURRENTLY SET FOR AMMONIUM SULFATE
MW = 0.018
OSM = 1.
VI = 3.
EPSM = 0.7
RHOA = 1777.
MAP = 0.132
MA = 0.0284
! hm fix 6/23/16
! RR = 8.3187
RR = 8.3145
BACT = VI*OSM*EPSM*MW*RHOA/(MAP*RHOW)
! AEROSOL SIZE DISTRIBUTION PARAMETERS CURRENTLY SET FOR MPACE
! (see morrison et al. 2007, JGR)
! MODE 1
RM1 = 0.052E-6
SIG1 = 2.04
NANEW1 = 72.2E6
F11 = 0.5*EXP(2.5*(LOG(SIG1))**2)
F21 = 1.+0.25*LOG(SIG1)
! MODE 2
RM2 = 1.3E-6
SIG2 = 2.5
NANEW2 = 1.8E6
F12 = 0.5*EXP(2.5*(LOG(SIG2))**2)
F22 = 1.+0.25*LOG(SIG2)
!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
! CONSTANTS FOR EFFICIENCY
CONS1=GAMMA(1.+DS)*CS
CONS2=GAMMA(1.+DG)*CG
CONS3=GAMMA(4.+BS)/6.
CONS4=GAMMA(4.+BR)/6.
CONS5=GAMMA(1.+BS)
CONS6=GAMMA(1.+BR)
CONS7=GAMMA(4.+BG)/6.
CONS8=GAMMA(1.+BG)
CONS9=GAMMA(5./2.+BR/2.)
CONS10=GAMMA(5./2.+BS/2.)
CONS11=GAMMA(5./2.+BG/2.)
CONS12=GAMMA(1.+DI)*CI
CONS13=GAMMA(BS+3.)*PI/4.*ECI
CONS14=GAMMA(BG+3.)*PI/4.*ECI
CONS15=-1108.*EII*PI**((1.-BS)/3.)*RHOSN**((-2.-BS)/3.)/(4.*720.)
CONS16=GAMMA(BI+3.)*PI/4.*ECI
CONS17=4.*2.*3.*RHOSU*PI*ECI*ECI*GAMMA(2.*BS+2.)/(8.*(RHOG-RHOSN))
CONS18=RHOSN*RHOSN
CONS19=RHOW*RHOW
CONS20=20.*PI*PI*RHOW*BIMM
CONS21=4./(DCS*RHOI)
CONS22=PI*RHOI*DCS**3/6.
CONS23=PI/4.*EII*GAMMA(BS+3.)
CONS24=PI/4.*ECR*GAMMA(BR+3.)
CONS25=PI*PI/24.*RHOW*ECR*GAMMA(BR+6.)
CONS26=PI/6.*RHOW
CONS27=GAMMA(1.+BI)
CONS28=GAMMA(4.+BI)/6.
CONS29=4./3.*PI*RHOW*(25.E-6)**3
CONS30=4./3.*PI*RHOW
CONS31=PI*PI*ECR*RHOSN
CONS32=PI/2.*ECR
CONS33=PI*PI*ECR*RHOG
CONS34=5./2.+BR/2.
CONS35=5./2.+BS/2.
CONS36=5./2.+BG/2.
CONS37=4.*PI*1.38E-23/(6.*PI*RIN)
CONS38=PI*PI/3.*RHOW
CONS39=PI*PI/36.*RHOW*BIMM
CONS40=PI/6.*BIMM
CONS41=PI*PI*ECR*RHOW
#ifdef WRF_MARS
DUST_PIRHOD = pi * rho_dust
DUST_CONS_RHO = rho_dust
!compiler issues with dust_cons3
dust_cons3_a = N_avogadro * co2_molrad * co2_molrad
DUST_CONS3 = 1./ (4. * sqrt(2.) * pi) * co2_molmass / (dust_cons3_a)
dust_reff_max = 25.e-6
dust_reff_min = 0.1e-6
dust_reff_default = reff
if(dust_distribution == 0) then !GAMMA function
DUST_MU = (1-3*veff)/veff !mu_dust
dust_mu_r8 = dust_mu
DUST_CONS0 = GAMMA(DUST_MU + 4.) * DUST_PIRHOD / (6.)
DUST_CONS1 = DUST_CONS0 / GAMMA(DUST_MU+1.)
DUST_CONS2 = GAMMA(DUST_MU + 4.) / (2*GAMMA(DUST_MU + 3.))
DUST_CONS_INV_G1 = 1./ GAMMA(DUST_MU + 1.)
DUST_CONS_INV_G4 = 1./ GAMMA(DUST_MU + 4.)
DUST_CONS_G3 = GAMMA(DUST_MU + 3.)
DUST_CONS_A_SEDIM = a_dust_sedim
DUST_CONS_B_SEDIM = b_dust_sedim
DUST_CONS_E_SEDIM = e_dust_sedim
LAMMIND = DUST_CONS2/dust_reff_max !25 micron
LAMMAXD = DUST_CONS2/dust_reff_min !0.1 micron
LAMDEFD = DUST_CONS2/dust_reff_default !2.0 micron
!nfac_LAMMIND1 = GAMMA(DUST_MU+1.) * exp(-(DUST_MU+1.)*log(LAMMIND))
!nfac_LAMMAXD1 = GAMMA(DUST_MU+1.) * exp(-(DUST_MU+1.)*log(LAMMAXD))
!nfac_LAMMIND4 = exp((DUST_MU+4.)*log(LAMMIND)) / dust_cons0
!nfac_LAMMAXD4 = exp((DUST_MU+4.)*log(LAMMAXD)) / dust_cons0
!nfac_LAMDEFD1 = GAMMA(DUST_MU+1.) * exp(-(DUST_MU+1.)*log(LAMDEFD))
!nfac_LAMDEFD4 = exp((DUST_MU+4.)*log(LAMDEFD)) / dust_cons0
LAMMIND_Q_N = exp((3.)*log(LAMMIND)) / dust_cons1
LAMMAXD_Q_N = exp((3.)*log(LAMMAXD)) / dust_cons1
LAMDEFD_Q_N = exp((3.)*log(LAMDEFD)) / dust_cons1
! Bins Gauss Legendre
gloc=0.
call prep_gaussian_weights(nbins,.false.,weights_pos) !these are the fractions. yay.
bin_width=weights_pos(1,:)
gloc(:nbins) = weights_pos(2,:)
! write(*,*) "loc", gloc
! write(*,*) "bw", bin_width
call gamma_inc_inv_calc(dust_mu_r8,gloc(:nbins),diam,nbins,"diam")
gloc(1)=0.0
do i=2, nbins+1
gloc(i) = gloc(i-1) + bin_width(i-1)
end do
fmin=1e-9
fmax=1-fmin
gloc(1) = fmin
gloc(nbins+1)=fmax
!write(*,*) "edges", gloc
call gamma_inc_inv_calc(dust_mu_r8,gloc(:),diam_edges,nbins+1,"diam_edges")
call calc_weights(dust_mu_r8,diam_edges, number, nbins) !fraction of total number between edges
call calc_weights(dust_mu_r8+3,diam_edges, mass, nbins) !fraction of total mass between edges
!done bin calculation
!debug bins
!write(*,*) bin_width
!write(*,*) diam
!write(*,*) diam_edges
! do i=1, nbins
! write(*,*) "bin ", i,": ",diam_edges(i), diam(i), diam_edges(i+1), bin_width(i), number(i),mass(i)
! end do
else if (dust_distribution == 1) then !lognormal
sigma_squared = alog(veff+1)
dust_cons1 = (DUST_PIRHOD / 6. )
!exp(-sigma**2 / 2)
dust_cons2 = exp(-sigma_squared/2)
!Cunningham factors, B and E is not used in lognormal
DUST_CONS_A_SEDIM = a_dust_sedim
ln_dust_reff_max = alog(dust_reff_max)
ln_dust_reff_min = alog(dust_reff_min)
ln_dust_reff_default = alog(dust_reff_default)
endif
DISTRIBUTION_MARS_DUST=dust_distribution
!ice constants
ice_mu = dust_mu
ice_cons2 = GAMMA(1.+DI+ice_mu) / (2.*GAMMA(ice_mu+DI)) !replaces dust_cons2 for ice on Mars
LAMMINI = ICE_CONS2/100e-6 !100 micron
LAMMAXI = ICE_CONS2/.1e-6 !.1 micron
! LAMDEFI = ICE_CONS2/dust_reff_default !2.0 micron
! DI is the shape parameter for ice that scale size to mass
! alternatively, it is describes how density changes with diameter*(1/3), or makes
! ice particles behave less spherical if DI != 3.
ice_cons10 = GAMMA(1+ice_mu)
!ice_cons10min = GAMMA(1+ice_mu) / exp((1+ice_mu)*log(lammini)) ! gamma(mu+1) / lam**(mu+1)
!ice_cons10max = GAMMA(1+ice_mu) / exp((1+ice_mu)*log(lammaxi)) ! gamma(mu+1) / lam**(mu+1)
ice_cons11 = 1./(ci * GAMMA(1+ice_mu+DI))
!ice_cons11min = ice_cons11 * exp((1+ice_mu+DI)*log(lammini))
!ice_cons11max = ice_cons11 * exp((1+ice_mu+DI)*log(lammaxi))
ice_cons12 = GAMMA(1.+DI+ice_mu) * ci / GAMMA(1+ice_mu) !replaces cons12 for Mars
ice_consmin_Q_N = exp(DI*log(lammini)) / ice_cons12
ice_consmax_Q_N = exp(DI*log(lammaxi)) / ice_cons12
homogeneous_ice_number_cons1 = (1./8) * (1./ci) * (1./homogeneous_ice_reff**3) &
* GAMMA(ice_mu+1) * (ice_mu+DI)**3 / gamma(ice_mu+DI+1) !that's horrible
!For DI ==3:
!(6/8) * (1./pi*rho) * (1./reff**3) * (mu+3)*(mu+3)/((mu+2)*(mu+1))
!The '6' is already folded in 'ci'
water_molec_volume = 3.22e-29 !m^3
water_molec_radius = ((3./(4*pi)) * water_molec_volume)**(1./3)
ice_cons_prefactor = sqrt(3./(8*pi*pi*water_molec_radius*rhoi)) * (1./kboltz)
ice_cons_nuc_m0 = 1. !ice_cons10
ice_cons_nuc_m2 = 1. ! GAMMA(3 + ice_mu)
ice_cons_nuc_m3 = 1. ! GAMMA(DI + 1 + ice_mu)
ice_cons_nuc_m0p5 = GAMMA(1.5 + ice_mu) / GAMMA(1. + ice_mu) ! GAMMA(1.5+ ice_mu)
ice_cons_nuc_m2p5 = GAMMA(3.5 + ice_mu) / GAMMA(3 + ice_mu)
ice_cons_nuc_m3p5 = GAMMA(DI + 1.5 + ice_mu) / GAMMA(DI + 1. + ice_mu)
photolysis_scrit = 10.
#endif
END SUBROUTINE MORR_TWO_MOMENT_INIT
!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
! THIS SUBROUTINE IS MAIN INTERFACE WITH THE TWO-MOMENT MICROPHYSICS SCHEME
! THIS INTERFACE TAKES IN 3D VARIABLES FROM DRIVER MODEL, CONVERTS TO 1D FOR
! CALL TO THE MAIN MICROPHYSICS SUBROUTINE (SUBROUTINE MORR_TWO_MOMENT_MICRO)
! WHICH OPERATES ON 1D VERTICAL COLUMNS.
! 1D VARIABLES FROM THE MAIN MICROPHYSICS SUBROUTINE ARE THEN REASSIGNED BACK TO 3D FOR OUTPUT
! BACK TO DRIVER MODEL USING THIS INTERFACE.
! MICROPHYSICS TENDENCIES ARE ADDED TO VARIABLES HERE BEFORE BEING PASSED BACK TO DRIVER MODEL.
! THIS CODE WAS WRITTEN BY HUGH MORRISON (NCAR) AND SLAVA TATARSKII (GEORGIA TECH).
! FOR QUESTIONS, CONTACT: HUGH MORRISON, E-MAIL: MORRISON@UCAR.EDU, PHONE:303-497-8916
!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
SUBROUTINE MP_MORR_TWO_MOMENT(ITIMESTEP, &
TH, QV, QC, QR, QI, QS, QG, NI, NS, NR, NG, &
RHO, PII, P, DT_IN, DZ, HT, W, &
RAINNC, RAINNCV, SR, &
SNOWNC,SNOWNCV,GRAUPELNC,GRAUPELNCV, & ! hm added 7/13/13
qrcuten, qscuten, qicuten, mu & ! hm added
,F_QNDROP, qndrop & ! hm added, wrf-chem
,IDS,IDE, JDS,JDE, KDS,KDE & ! domain dims
,IMS,IME, JMS,JME, KMS,KME & ! memory dims
,ITS,ITE, JTS,JTE, KTS,KTE & ! tile dims )
!jdf ,C2PREC3D,CSED3D,ISED3D,SSED3D,GSED3D,RSED3D & ! HM ADD, WRF-CHEM
,QLSINK,PRECR,PRECI,PRECS,PRECG & ! HM ADD, WRF-CHEM
#ifdef WRF_MARS
,qdust,ndust &
,dustnc, dustncv &
,qice_core &
,corenc, corencv &
,reff_dust,effi &
,do_water &
,DUSTQ_MICRO, DUSTQ_SED &
,DUSTN_MICRO, DUSTN_SED &
,COREQ_MICRO, COREQ_SED &
,ICEQ_MICRO, ICEQ_SED &
,ICEN_MICRO, ICEN_SED &
,dsed1, dsed2 &
#endif
)
! QV - water vapor mixing ratio (kg/kg)
! QC - cloud water mixing ratio (kg/kg)
! QR - rain water mixing ratio (kg/kg)
! QI - cloud ice mixing ratio (kg/kg)
! QS - snow mixing ratio (kg/kg)
! QG - graupel mixing ratio (KG/KG)
! NI - cloud ice number concentration (1/kg)
! NS - Snow Number concentration (1/kg)
! NR - Rain Number concentration (1/kg)
! NG - Graupel number concentration (1/kg)
#ifdef WRF_MARS
! QDUST - dust mixing ratio (kg/kg)
! NDUST - dust Number concentration (1/kg)
! PRECD - SEDIMENTATION FLUXES (KG/M^2/S) FOR DUST
! QICE_CORE - dust core mixing ratio (kg/kg)
#endif
! NOTE: RHO AND HT NOT USED BY THIS SCHEME AND DO NOT NEED TO BE PASSED INTO SCHEME!!!!
! P - AIR PRESSURE (PA)
! W - VERTICAL AIR VELOCITY (M/S)
! TH - POTENTIAL TEMPERATURE (K)
! PII - exner function - used to convert potential temp to temp
! DZ - difference in height over interface (m)
! DT_IN - model time step (sec)
! ITIMESTEP - time step counter
! RAINNC - accumulated grid-scale precipitation (mm)
! RAINNCV - one time step grid scale precipitation (mm/time step)
! SNOWNC - accumulated grid-scale snow plus cloud ice (mm)
! SNOWNCV - one time step grid scale snow plus cloud ice (mm/time step)
! GRAUPELNC - accumulated grid-scale graupel (mm)
! GRAUPELNCV - one time step grid scale graupel (mm/time step)
! SR - one time step mass ratio of snow to total precip
! qrcuten, rain tendency from parameterized cumulus convection
! qscuten, snow tendency from parameterized cumulus convection
! qicuten, cloud ice tendency from parameterized cumulus convection
! variables below currently not in use, not coupled to PBL or radiation codes
! TKE - turbulence kinetic energy (m^2 s-2), NEEDED FOR DROPLET ACTIVATION (SEE CODE BELOW)
! NCTEND - droplet concentration tendency from pbl (kg-1 s-1)
! NCTEND - CLOUD ICE concentration tendency from pbl (kg-1 s-1)
! KZH - heat eddy diffusion coefficient from YSU scheme (M^2 S-1), NEEDED FOR DROPLET ACTIVATION (SEE CODE BELOW)
! EFFCS - CLOUD DROPLET EFFECTIVE RADIUS OUTPUT TO RADIATION CODE (micron)
! EFFIS - CLOUD DROPLET EFFECTIVE RADIUS OUTPUT TO RADIATION CODE (micron)
! HM, ADDED FOR WRF-CHEM COUPLING
! QLSINK - TENDENCY OF CLOUD WATER TO RAIN, SNOW, GRAUPEL (KG/KG/S)
! CSED,ISED,SSED,GSED,RSED - SEDIMENTATION FLUXES (KG/M^2/S) FOR CLOUD WATER, ICE, SNOW, GRAUPEL, RAIN
! PRECI,PRECS,PRECG,PRECR - SEDIMENTATION FLUXES (KG/M^2/S) FOR ICE, SNOW, GRAUPEL, RAIN
!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
! reflectivity currently not included!!!!
! REFL_10CM - CALCULATED RADAR REFLECTIVITY AT 10 CM (DBZ)
!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!
! EFFC - DROPLET EFFECTIVE RADIUS (MICRON)
! EFFR - RAIN EFFECTIVE RADIUS (MICRON)
! EFFS - SNOW EFFECTIVE RADIUS (MICRON)
! EFFI - CLOUD ICE EFFECTIVE RADIUS (MICRON)
! ADDITIONAL OUTPUT FROM MICRO - SEDIMENTATION TENDENCIES, NEEDED FOR LIQUID-ICE STATIC ENERGY
! QGSTEN - GRAUPEL SEDIMENTATION TEND (KG/KG/S)
! QRSTEN - RAIN SEDIMENTATION TEND (KG/KG/S)
! QISTEN - CLOUD ICE SEDIMENTATION TEND (KG/KG/S)
! QNISTEN - SNOW SEDIMENTATION TEND (KG/KG/S)
! QCSTEN - CLOUD WATER SEDIMENTATION TEND (KG/KG/S)
! WVAR - STANDARD DEVIATION OF SUB-GRID VERTICAL VELOCITY (M/S)
IMPLICIT NONE
INTEGER, INTENT(IN ) :: ids, ide, jds, jde, kds, kde , &
ims, ime, jms, jme, kms, kme , &
its, ite, jts, jte, kts, kte
! Temporary changed from INOUT to IN
#ifdef WRF_PLANET
REAL, DIMENSION(ims:ime, kms:kme, jms:jme), INTENT(INOUT):: &
TH
REAL, DIMENSION(ims:ime, kms:kme, jms:jme), INTENT(INOUT), optional:: &
qv, qc, qr, qi, qs, qg, ni, ns, nr, NG
#else
REAL, DIMENSION(ims:ime, kms:kme, jms:jme), INTENT(INOUT):: &
qv, qc, qr, qi, qs, qg, ni, ns, nr, TH, NG
#endif
#ifdef WRF_MARS
logical, intent(in),optional :: do_water
logical :: use_water
REAL, DIMENSION(ims:ime, kms:kme, jms:jme), INTENT(INOUT):: &
qdust, ndust, qice_core
! REAL, DIMENSION(ims:ime, kms:kme, jms:jme), optional,INTENT(INOUT):: PRECD
REAL, DIMENSION(ims:ime, jms:jme), INTENT(INOUT):: &
DUSTNC, DUSTNCV, &
CORENC, CORENCV
REAL, DIMENSION(ims:ime, kms:kme, jms:jme), intent(out):: &
reff_dust, effi !effective radius for dust
real, dimension(ims:ime, kms:kme, jms:jme), intent(inout), optional :: &
DUSTQ_MICRO, DUSTQ_SED &
,DUSTN_MICRO, DUSTN_SED &
,COREQ_MICRO, COREQ_SED &