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module suphec_m |
module suphec_m |
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use nr_util, only: pi |
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implicit none |
implicit none |
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! A1.0 Fundamental constants |
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real, parameter:: RCLUM = 299792458. ! speed of light, m s-1 |
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real, parameter:: RHPLA = 6.6260755E-34 ! Planck constant, J s |
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real, parameter:: KBOL = 1.380658E-23 ! Boltzmann constant, in J K-1 |
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real, parameter:: NAVO = 6.0221367E23 ! Avogadro number, in mol-1 |
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! A1.1 Astronomical constants |
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REAL RSIYEA, RSIDAY, ROMEGA |
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real, parameter:: RDAY = 86400. |
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real, parameter:: REA = 149597870000. |
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real, parameter:: REPSM = 0.409093 |
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! A1.2 Geoide |
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real, parameter:: RG = 9.80665 ! acceleration of gravity, in m s-2 |
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real, parameter:: RA = 6371229. |
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! A1.3 Radiation |
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REAL, parameter:: rsigma = 2. * pi**5 * (kbol / rhpla)**3 * kbol / rclum**2 & |
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/ 15. |
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! A1.4 Thermodynamic gas phase |
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REAL, parameter:: R = NAVO * KBOL ! ideal gas constant, in J K-1 mol-1 |
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real, parameter:: MV = 18.0153 ! molar mass of water, in g mol-1 |
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real, parameter:: RV = 1e3 * R / MV |
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! specific ideal gas constant for water vapor, in J K-1 kg-1 |
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! (factor 1e3: conversion from g to kg) |
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real, parameter:: MD = 28.9644 ! molar mass of dry air, in g mol-1 |
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real, parameter:: RD = 1e3 * R / MD |
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! specific ideal gas constant for dry air, in J K-1 kg-1 |
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! (factor 1e3: conversion from g to kg) |
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real, save:: RCPV, RCVD, RCVV |
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real, parameter:: RCPD = 7. / 2 * RD |
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! specific heat capacity for dry air, in J K-1 kg-1 |
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real, parameter:: RMO3 = 47.9942 |
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REAL, parameter:: RKAPPA = RD/RCPD |
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real, save:: RETV |
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! A1.5, 6 Thermodynamic liquid, solid phases |
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REAL, save:: RCW, RCS |
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! A1.7 Thermodynamic transition of phase |
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REAL, save:: RLMLT |
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real, parameter:: RTT = 273.16 |
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real, parameter:: RLVTT = 2.5008E+6 |
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real, parameter:: RLSTT = 2.8345E+6 |
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real, parameter:: RATM = 1e5 |
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! A1.8 Curve of saturation |
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REAL, save:: RALPW, RBETW, RGAMW, RALPS, RBETS, RGAMS |
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real, parameter:: RESTT = 611.14 |
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REAL, save:: RALPD, RBETD, RGAMD |
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private pi |
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contains |
contains |
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SUBROUTINE suphec |
SUBROUTINE suphec |
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! From phylmd/suphec.F,v 1.2 2005/06/06 13:16:33 |
! From phylmd/suphec.F, version 1.2 2005/06/06 13:16:33 |
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! Initialise certaines constantes et certains paramètres physiques. |
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! Initialise certaines constantes et parametres physiques. |
!------------------------------------------ |
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use YOMCST, only: rpi, rclum, rhpla, rkbol, rnavo, rday, rea, repsm, & |
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rsiyea, rsiday,romega, rg, ra, r1sa, rsigma, r, rmd, rmo3, rmv, rd, & |
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rv, rcpd, rcvd, rcpv, rcvv, rkappa, retv, rcw, rcs, rtt, rlvtt, & |
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rlstt, rlmlt, ratm, restt, rgamw, rbetw, ralpw, rgams, rbets, ralps, & |
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rgamd, rbetd, ralpd |
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use yoethf |
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LOGICAL:: firstcall = .TRUE. |
PRINT *, 'Call sequence information: suphec' |
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!------------------------------------------ |
! 2. DEFINE ASTRONOMICAL CONSTANTS |
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IF (firstcall) THEN |
RSIYEA = 365.25*RDAY*2.*PI/6.283076 |
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PRINT *, 'suphec initialise les constantes du GCM' |
RSIDAY = RDAY/(1.+RDAY/RSIYEA) |
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firstcall = .FALSE. |
ROMEGA = 2.*PI/RSIDAY |
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!* 1. DEFINE FUNDAMENTAL CONSTANTS. |
print *, 'Astronomical constants ' |
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print '('' day = '', E13.7, '' s'')', RDAY |
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WRITE(UNIT=6,FMT='(''0*** Constants of the ICM ***'')') |
print '('' half g. axis = '', E13.7, '' m'')', REA |
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RPI=2.*ASIN(1.) |
print '('' mean anomaly = '', E13.7, '' -'')', REPSM |
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RCLUM=299792458. |
print '('' sideral year = '', E13.7, '' s'')', RSIYEA |
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RHPLA=6.6260755E-34 |
print '('' sideral day = '', E13.7, '' s'')', RSIDAY |
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RKBOL=1.380658E-23 |
print '('' omega = '', E13.7, '' s-1'')', ROMEGA |
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RNAVO=6.0221367E+23 |
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WRITE(UNIT=6,FMT='('' *** Fundamental constants ***'')') |
! 3. DEFINE GEOIDE. |
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WRITE(UNIT=6,FMT='('' PI = '',E13.7,'' -'')')RPI |
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WRITE(UNIT=6,FMT='('' c = '',E13.7,''m s-1'')') & |
print *, ' Geoide ' |
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RCLUM |
print '('' Gravity = '', E13.7, '' m s-2'')', RG |
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WRITE(UNIT=6,FMT='('' h = '',E13.7,''J s'')') & |
print '('' Earth radius = '', E13.7, '' m'')', RA |
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RHPLA |
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WRITE(UNIT=6,FMT='('' K = '',E13.7,''J K-1'')') & |
! 4. DEFINE RADIATION CONSTANTS. |
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RKBOL |
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WRITE(UNIT=6,FMT='('' N = '',E13.7,''mol-1'')') & |
print *, ' Radiation ' |
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RNAVO |
print '('' Stefan-Bol. = '', E13.7, '' W m-2 K-4'')', RSIGMA |
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!* 2. DEFINE ASTRONOMICAL CONSTANTS. |
! 5. DEFINE THERMODYNAMIC CONSTANTS, GAS PHASE. |
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RDAY=86400. |
RCVD = RCPD-RD |
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REA=149597870000. |
RCPV = 4. * RV |
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REPSM=0.409093 |
RCVV = RCPV-RV |
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RETV = RV / RD - 1. |
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RSIYEA=365.25*RDAY*2.*RPI/6.283076 |
print *, 'Thermodynamics, gas' |
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RSIDAY=RDAY/(1.+RDAY/RSIYEA) |
print '('' Ozone mass = '', e13.7)', RMO3 |
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ROMEGA=2.*RPI/RSIDAY |
print *, "rd = ", RD, "J K-1 kg-1" |
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print *, "rv = ", RV, "J K-1 kg-1" |
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WRITE(UNIT=6,FMT='('' *** Astronomical constants ***'')') |
print '('' Cpd = '', e13.7)', RCPD |
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WRITE(UNIT=6,FMT='('' day = '',E13.7,'' s'')')RDAY |
print '('' Cvd = '', e13.7)', RCVD |
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WRITE(UNIT=6,FMT='('' half g. axis = '',E13.7,'' m'')')REA |
print '('' Cpv = '', e13.7)', RCPV |
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WRITE(UNIT=6,FMT='('' mean anomaly = '',E13.7,'' -'')')REPSM |
print '('' Cvv = '', e13.7)', RCVV |
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WRITE(UNIT=6,FMT='('' sideral year = '',E13.7,'' s'')')RSIYEA |
print '('' Rd/Cpd = '', e13.7)', RKAPPA |
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WRITE(UNIT=6,FMT='('' sideral day = '',E13.7,'' s'')')RSIDAY |
print '('' Rv / Rd - 1 = '', e13.7)', RETV |
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WRITE(UNIT=6,FMT='('' omega = '',E13.7,'' s-1'')') & |
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ROMEGA |
! 6. DEFINE THERMODYNAMIC CONSTANTS, LIQUID PHASE. |
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!* 3. DEFINE GEOIDE. |
RCW = RCPV |
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print *, 'Thermodynamic, liquid ' |
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RG=9.80665 |
print '('' Cw = '', E13.7)', RCW |
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RA=6371229. |
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R1SA=SNGL(1.D0/DBLE(RA)) |
! 7. DEFINE THERMODYNAMIC CONSTANTS, SOLID PHASE. |
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WRITE(UNIT=6,FMT='('' *** Geoide ***'')') |
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WRITE(UNIT=6,FMT='('' Gravity = '',E13.7,'' m s-2'')') & |
RCS = RCPV |
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RG |
print *, 'thermodynamic, solid' |
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WRITE(UNIT=6,FMT='('' Earth radius = '',E13.7,'' m'')')RA |
print '('' Cs = '', E13.7)', RCS |
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WRITE(UNIT=6,FMT='('' Inverse E.R. = '',E13.7,'' m'')')R1SA |
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! 8. DEFINE THERMODYNAMIC CONSTANTS, TRANSITION OF PHASE. |
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!* 4. DEFINE RADIATION CONSTANTS. |
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RLMLT = RLSTT-RLVTT |
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rsigma = 2.*rpi**5 * (rkbol/rhpla)**3 * rkbol/rclum/rclum/15. |
print *, 'Thermodynamic, transition of phase:' |
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!IM init. dans conf_phys.F90 RI0=1365. |
print '('' Fusion point = '', E13.7)', RTT |
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WRITE(UNIT=6,FMT='('' *** Radiation ***'')') |
print '('' RLvTt = '', E13.7)', RLVTT |
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WRITE(UNIT=6,FMT='('' Stefan-Bol. = '',E13.7,'' W m-2 K-4'')') RSIGMA |
print '('' RLsTt = '', E13.7)', RLSTT |
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print '('' RLMlt = '', E13.7)', RLMLT |
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!* 5. DEFINE THERMODYNAMIC CONSTANTS, GAS PHASE. |
print '('' Normal pressure = '', E13.7)', RATM |
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R=RNAVO*RKBOL |
! 9. SATURATED VAPOUR PRESSURE. |
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RMD=28.9644 |
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RMO3=47.9942 |
RGAMW = (RCW-RCPV)/RV |
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RMV=18.0153 |
RBETW = RLVTT/RV+RGAMW*RTT |
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RD=1000.*R/RMD |
RALPW = LOG(RESTT)+RBETW/RTT+RGAMW*LOG(RTT) |
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RV=1000.*R/RMV |
RGAMS = (RCS-RCPV)/RV |
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RCPD=3.5*RD |
RBETS = RLSTT/RV+RGAMS*RTT |
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RCVD=RCPD-RD |
RALPS = LOG(RESTT)+RBETS/RTT+RGAMS*LOG(RTT) |
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RCPV=4. *RV |
RGAMD = RGAMS-RGAMW |
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RCVV=RCPV-RV |
RBETD = RBETS-RBETW |
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RKAPPA=RD/RCPD |
RALPD = RALPS-RALPW |
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RETV=RV/RD-1. |
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WRITE(UNIT=6,FMT='('' *** Thermodynamic, gas ***'')') |
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WRITE(UNIT=6,FMT='('' Perfect gas = '',e13.7)') R |
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WRITE(UNIT=6,FMT='('' Dry air mass = '',e13.7)') RMD |
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WRITE(UNIT=6,FMT='('' Ozone mass = '',e13.7)') RMO3 |
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WRITE(UNIT=6,FMT='('' Vapour mass = '',e13.7)') RMV |
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WRITE(UNIT=6,FMT='('' Dry air cst. = '',e13.7)') RD |
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WRITE(UNIT=6,FMT='('' Vapour cst. = '',e13.7)') RV |
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WRITE(UNIT=6,FMT='('' Cpd = '',e13.7)') RCPD |
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WRITE(UNIT=6,FMT='('' Cvd = '',e13.7)') RCVD |
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WRITE(UNIT=6,FMT='('' Cpv = '',e13.7)') RCPV |
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WRITE(UNIT=6,FMT='('' Cvv = '',e13.7)') RCVV |
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WRITE(UNIT=6,FMT='('' Rd/Cpd = '',e13.7)') RKAPPA |
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WRITE(UNIT=6,FMT='('' Rv/Rd-1 = '',e13.7)') RETV |
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!* 6. DEFINE THERMODYNAMIC CONSTANTS, LIQUID PHASE. |
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RCW=RCPV |
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WRITE(UNIT=6,FMT='('' *** Thermodynamic, liquid ***'')') |
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WRITE(UNIT=6,FMT='('' Cw = '',E13.7)') RCW |
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!* 7. DEFINE THERMODYNAMIC CONSTANTS, SOLID PHASE. |
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RCS=RCPV |
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WRITE(UNIT=6,FMT='('' *** thermodynamic, solid ***'')') |
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WRITE(UNIT=6,FMT='('' Cs = '',E13.7)') RCS |
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!* 8. DEFINE THERMODYNAMIC CONSTANTS, TRANSITION OF PHASE. |
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RTT=273.16 |
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RLVTT=2.5008E+6 |
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RLSTT=2.8345E+6 |
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RLMLT=RLSTT-RLVTT |
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RATM=100000. |
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WRITE(UNIT=6,FMT='('' *** Thermodynamic, trans. ***'')') |
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WRITE(UNIT=6,FMT='('' Fusion point = '',E13.7)') RTT |
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WRITE(UNIT=6,FMT='('' RLvTt = '',E13.7)') RLVTT |
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WRITE(UNIT=6,FMT='('' RLsTt = '',E13.7)') RLSTT |
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WRITE(UNIT=6,FMT='('' RLMlt = '',E13.7)') RLMLT |
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WRITE(UNIT=6,FMT='('' Normal press. = '',E13.7)') RATM |
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WRITE(UNIT=6,FMT='('' Latent heat : '')') |
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!* 9. SATURATED VAPOUR PRESSURE. |
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RESTT=611.14 |
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RGAMW=(RCW-RCPV)/RV |
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RBETW=RLVTT/RV+RGAMW*RTT |
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RALPW=LOG(RESTT)+RBETW/RTT+RGAMW*LOG(RTT) |
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RGAMS=(RCS-RCPV)/RV |
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RBETS=RLSTT/RV+RGAMS*RTT |
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RALPS=LOG(RESTT)+RBETS/RTT+RGAMS*LOG(RTT) |
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RGAMD=RGAMS-RGAMW |
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RBETD=RBETS-RBETW |
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RALPD=RALPS-RALPW |
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! calculer les constantes pour les fonctions thermodynamiques |
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RVTMP2=RCPV/RCPD-1. |
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RHOH2O=RATM/100. |
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R2ES=RESTT*RD/RV |
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R3LES=17.269 |
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R3IES=21.875 |
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R4LES=35.86 |
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R4IES=7.66 |
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R5LES=R3LES*(RTT-R4LES) |
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R5IES=R3IES*(RTT-R4IES) |
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ELSE |
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PRINT *, 'suphec DEJA APPELE ' |
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ENDIF |
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END SUBROUTINE suphec |
END SUBROUTINE suphec |
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