mHM
The mesoscale Hydrological Model
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Provides mHM specific constants. More...
Variables | |
real(dp), parameter, public | h2odens = 1000.0_dp |
real(dp), parameter, public | p2_initstatefluxes = 15.00_dp |
real(dp), parameter, public | p3_initstatefluxes = 10.00_dp |
real(dp), parameter, public | p4_initstatefluxes = 75.00_dp |
real(dp), parameter, public | p5_initstatefluxes = 1500.00_dp |
real(dp), parameter, public | c1_initstatesm = 0.25_dp |
integer(i4), parameter, public | noutflxstate = 21_i4 |
real(dp), parameter, public | harsamconst = 17.800_dp |
Hargreaves-Samani ref. | |
real(dp), parameter, public | duffiedr = 0.0330_dp |
real(dp), parameter, public | duffiedelta1 = 0.4090_dp |
real(dp), parameter, public | duffiedelta2 = 1.3900_dp |
real(dp), parameter, public | tetens_c1 = 0.6108_dp |
Tetens's formula to calculate saturated vapour pressure. | |
real(dp), parameter, public | tetens_c2 = 17.270_dp |
real(dp), parameter, public | tetens_c3 = 237.30_dp |
real(dp), parameter, public | satpressureslope1 = 4098.0_dp |
calculation of the slope of the saturation vapour pressure curve following Tetens | |
real(dp), parameter, public | desilets_a0 = 0.0808_dp |
Neutrons and moisture: N0 formula, Desilets et al. | |
real(dp), parameter, public | desilets_a1 = 0.372_dp |
real(dp), parameter, public | desilets_a2 = 0.115_dp |
real(dp), parameter, public | cosmic_n = 348.33_dp |
Neutrons and moisture: COSMIC, Shuttleworth et al. | |
real(dp), parameter, public | cosmic_alpha = 0.2392421548_dp |
real(dp), parameter, public | cosmic_l1 = 161.98621864_dp |
real(dp), parameter, public | cosmic_l2 = 129.14558985_dp |
real(dp), parameter, public | cosmic_l3 = 107.82204562_dp |
real(dp), parameter, public | cosmic_l4 = 3.1627190566_dp |
Provides mHM specific constants.
Provides mHM specific constants such as flood plain elevation.
COPYING
and COPYING.LESSER
provided with this software. The complete GNU license text can also be found at http://www.gnu.org/licenses/. real(dp), parameter, public mo_mhm_constants::c1_initstatesm = 0.25_dp |
Definition at line 30 of file mo_mhm_constants.f90.
real(dp), parameter, public mo_mhm_constants::cosmic_alpha = 0.2392421548_dp |
Definition at line 57 of file mo_mhm_constants.f90.
Referenced by mo_neutrons::cosmic().
real(dp), parameter, public mo_mhm_constants::cosmic_l1 = 161.98621864_dp |
Definition at line 58 of file mo_mhm_constants.f90.
Referenced by mo_neutrons::cosmic().
real(dp), parameter, public mo_mhm_constants::cosmic_l2 = 129.14558985_dp |
Definition at line 59 of file mo_mhm_constants.f90.
Referenced by mo_neutrons::cosmic().
real(dp), parameter, public mo_mhm_constants::cosmic_l3 = 107.82204562_dp |
Definition at line 60 of file mo_mhm_constants.f90.
real(dp), parameter, public mo_mhm_constants::cosmic_l4 = 3.1627190566_dp |
Definition at line 61 of file mo_mhm_constants.f90.
Referenced by mo_neutrons::cosmic().
real(dp), parameter, public mo_mhm_constants::cosmic_n = 348.33_dp |
Neutrons and moisture: COSMIC, Shuttleworth et al.
2013
Definition at line 56 of file mo_mhm_constants.f90.
real(dp), parameter, public mo_mhm_constants::desilets_a0 = 0.0808_dp |
Neutrons and moisture: N0 formula, Desilets et al.
2010
Definition at line 51 of file mo_mhm_constants.f90.
Referenced by mo_neutrons::desiletsn0().
real(dp), parameter, public mo_mhm_constants::desilets_a1 = 0.372_dp |
Definition at line 52 of file mo_mhm_constants.f90.
Referenced by mo_neutrons::desiletsn0().
real(dp), parameter, public mo_mhm_constants::desilets_a2 = 0.115_dp |
Definition at line 53 of file mo_mhm_constants.f90.
Referenced by mo_neutrons::desiletsn0().
real(dp), parameter, public mo_mhm_constants::duffiedelta1 = 0.4090_dp |
Definition at line 40 of file mo_mhm_constants.f90.
Referenced by mo_pet::extraterr_rad_approx().
real(dp), parameter, public mo_mhm_constants::duffiedelta2 = 1.3900_dp |
Definition at line 41 of file mo_mhm_constants.f90.
Referenced by mo_pet::extraterr_rad_approx().
real(dp), parameter, public mo_mhm_constants::duffiedr = 0.0330_dp |
Definition at line 39 of file mo_mhm_constants.f90.
Referenced by mo_pet::extraterr_rad_approx().
real(dp), parameter, public mo_mhm_constants::h2odens = 1000.0_dp |
Definition at line 23 of file mo_mhm_constants.f90.
Referenced by mo_neutrons::cosmic(), and mo_mrm_riv_temp_class::get_e_io().
real(dp), parameter, public mo_mhm_constants::harsamconst = 17.800_dp |
Hargreaves-Samani ref.
ET formula [deg C]
Definition at line 36 of file mo_mhm_constants.f90.
Referenced by mo_meteo_handler::get_corrected_pet().
integer(i4), parameter, public mo_mhm_constants::noutflxstate = 21_i4 |
Definition at line 33 of file mo_mhm_constants.f90.
real(dp), parameter, public mo_mhm_constants::p2_initstatefluxes = 15.00_dp |
Definition at line 26 of file mo_mhm_constants.f90.
real(dp), parameter, public mo_mhm_constants::p3_initstatefluxes = 10.00_dp |
Definition at line 27 of file mo_mhm_constants.f90.
real(dp), parameter, public mo_mhm_constants::p4_initstatefluxes = 75.00_dp |
Definition at line 28 of file mo_mhm_constants.f90.
real(dp), parameter, public mo_mhm_constants::p5_initstatefluxes = 1500.00_dp |
Definition at line 29 of file mo_mhm_constants.f90.
real(dp), parameter, public mo_mhm_constants::satpressureslope1 = 4098.0_dp |
calculation of the slope of the saturation vapour pressure curve following Tetens
Definition at line 48 of file mo_mhm_constants.f90.
Referenced by mo_pet::slope_satpressure().
real(dp), parameter, public mo_mhm_constants::tetens_c1 = 0.6108_dp |
Tetens's formula to calculate saturated vapour pressure.
Definition at line 44 of file mo_mhm_constants.f90.
Referenced by mo_pet::sat_vap_pressure().
real(dp), parameter, public mo_mhm_constants::tetens_c2 = 17.270_dp |
Definition at line 45 of file mo_mhm_constants.f90.
Referenced by mo_pet::sat_vap_pressure().
real(dp), parameter, public mo_mhm_constants::tetens_c3 = 237.30_dp |
Definition at line 46 of file mo_mhm_constants.f90.
Referenced by mo_pet::sat_vap_pressure(), and mo_pet::slope_satpressure().