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SCHRIFTENREIHE Institut für Pflanzenernährung und Bodenkunde ...

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Simulations of soil water and heat flow were performed with HYDRUS-1D<br />

(Šimůnek et al., 1998). HYDRUS-1D is a finite element model for simulating the<br />

one-dimensional movement of water, heat, and multiple solutes in variably<br />

saturated media. The program numerically solves the Richards’ equation for<br />

saturated and unsaturated water flow and Fickian-based advection dispersion<br />

equations for heat and solute transport. Variably saturated water flow is<br />

described by the modified Richards’ equation:<br />

∂h<br />

∂T<br />

[ ( h)<br />

+ K ( h)<br />

+ K ( h)<br />

S<br />

∂ ( h)<br />

∂ = K ∂t<br />

∂z<br />

h ∂z<br />

h<br />

T ∂z<br />

θ w ] −<br />

[1]<br />

where θw is the volumetric liquid water content, t is time, z is the spatial<br />

coordinate positive upward, h is the pressure head, T is the temperature, and S<br />

is a sink term usually accounting for root water uptake. Kh and KT donate<br />

hydraulic conductivity due to a gradient in h and T, respectively. Soil hydraulic<br />

properties are described by the following expressions (van Genuchten, 1980):<br />

S ( h)<br />

e<br />

θ ( h)<br />

−θ<br />

1<br />

w r = =<br />

[2]<br />

n m<br />

θs<br />

−θ<br />

r [ 1+<br />

αh<br />

]<br />

K ( h)<br />

−<br />

h<br />

l<br />

1/<br />

m m 2<br />

= K s × Se<br />

( 1−<br />

( 1 Se<br />

) )<br />

[3]<br />

where Se is the effective saturation, θs and θr are the saturated and residual<br />

water contents (L 3 L -3 ), respectively; the symbols α (L -1 ), n, and m=1-1/n are<br />

empirical shape parameters, and the inverse of α is often referred to as the air<br />

entry value or bubbling pressure; Ks is the saturated hydraulic conductivity (L<br />

T -1 ), and L is a pore connectivity parameter which normally is set to 0.5. The Eq.<br />

[2] was fitted to the measured water retention data (drying branch) using the<br />

RETC code (van Genuchten et al., 1991).<br />

The soil thermal regime is modeled with the conduction–convection heat<br />

flow equation (e.g., Nassar et al., 1992):<br />

∂T<br />

∂T<br />

[ λ(<br />

] − C q C ST<br />

∂ T ∂ C( ) = θ<br />

t z w)<br />

z w −<br />

∂ ∂<br />

∂<br />

∂z<br />

w<br />

θ [4]<br />

where C(θ) and Cw denote the volumetric heat capacity of the bulk soil and<br />

liquid phase, respectively. C(θ) is determined according to De Vries (1963):<br />

90<br />

C( θ ×<br />

6<br />

θ ) ≈ ( 1.<br />

92θ<br />

m + 2.<br />

51θ<br />

o + 4.<br />

18 w ) 10<br />

[5]

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