RICHARDS Mode¶
Governing Equations¶
RICHARDS
mode applies to single phase, variably saturated, isothermal
systems. The governing mass conservation equation is given by
with Darcy flux \({\boldsymbol{q}}\) defined as
Here, \(\porosity\) denotes porosity [-], \(s\) saturation [m\(^3\) m\(^{-3}\)], \(\eta\) molar water density [kmol m\(^{-3}\)], \(\density\) mass water density [kg m\(^{-3}\)], \({\boldsymbol{q}}\) Darcy flux [m s\(^{-1}\)], \(k\) intrinsic permeability [m\(^2\)], \(k_r\) relative permeability [-], \(\mu\) viscosity [Pa s], \(P\) pressure [Pa], \({\boldsymbol{g}}\) gravity [m s\(^{-2}\)]. Supported relative permeability functions \(k_r\) for Richards’ equation include van Genuchten, Books-Corey and Thomeer-Corey, while the saturation functions include Burdine and Mualem. Water density and viscosity are computed as a function of temperature and pressure through an equation of state for water. The source/sink term \(Q_w\) [kmol m\(^{-3}\) s\(^{-1}\)] has the form
where \(q_M\) denotes a mass rate in kg/m\(^{3}\)/s, and \({\boldsymbol{r}}_{ss}\) denotes the location of the source/sink.