16 USE mo_kind,
ONLY : i4, dp
23 real(dp),
public,
parameter ::
h2odens = 1000.0_dp
39 real(dp),
public,
parameter ::
duffiedr = 0.0330_dp
44 real(dp),
public,
parameter ::
tetens_c1 = 0.6108_dp
45 real(dp),
public,
parameter ::
tetens_c2 = 17.270_dp
46 real(dp),
public,
parameter ::
tetens_c3 = 237.30_dp
56 real(dp),
public,
parameter ::
cosmic_n = 348.33_dp
58 real(dp),
public,
parameter ::
cosmic_l1 = 161.98621864_dp
59 real(dp),
public,
parameter ::
cosmic_l2 = 129.14558985_dp
60 real(dp),
public,
parameter ::
cosmic_l3 = 107.82204562_dp
61 real(dp),
public,
parameter ::
cosmic_l4 = 3.1627190566_dp
Provides mHM specific constants.
real(dp), parameter, public desilets_a0
Neutrons and moisture: N0 formula, Desilets et al.
real(dp), parameter, public desilets_a2
real(dp), parameter, public cosmic_n
Neutrons and moisture: COSMIC, Shuttleworth et al.
real(dp), parameter, public cosmic_l4
real(dp), parameter, public harsamconst
Hargreaves-Samani ref.
real(dp), parameter, public duffiedelta1
real(dp), parameter, public cosmic_l1
real(dp), parameter, public tetens_c3
real(dp), parameter, public h2odens
real(dp), parameter, public tetens_c1
Tetens's formula to calculate saturated vapour pressure.
real(dp), parameter, public cosmic_l3
real(dp), parameter, public cosmic_l2
real(dp), parameter, public tetens_c2
real(dp), parameter, public p3_initstatefluxes
real(dp), parameter, public satpressureslope1
calculation of the slope of the saturation vapour pressure curve following Tetens
real(dp), parameter, public p2_initstatefluxes
integer(i4), parameter, public noutflxstate
real(dp), parameter, public desilets_a1
real(dp), parameter, public duffiedr
real(dp), parameter, public cosmic_alpha
real(dp), parameter, public c1_initstatesm
real(dp), parameter, public p5_initstatefluxes
real(dp), parameter, public p4_initstatefluxes
real(dp), parameter, public duffiedelta2