2:2.2.2 Priestley-Taylor Method

Priestley and Taylor (1972) developed a simplified version of the combination equation for use when surface areas are wet. The aerodynamic component was removed and the energy component was multiplied by a coefficient, αpet\alpha_{pet} = 1.28, when the general surroundings are wet or under humid conditions

λEo=αpetΔΔ+γ(HnetG)\lambda E_o=\alpha_{pet}*\frac{\Delta}{\Delta+\gamma}*(H_{net}-G) 2:2.2.23

where λ\lambda is the latent heat of vaporization (MJ kg1^{-1}), EoE_o is the potential evapotranspiration (mm d1^{-1}), αpet\alpha_{pet} is a coefficient, Δ\Delta is the slope of the saturation vapor pressure-temperature curve, de/dTde/dT (kPa ˚C1^{-1}), γ\gamma is the psychrometric constant (kPa ˚C1^{-1}), HnetH_{net} is the net radiation (MJ m2^{-2} d1^{-1}), and GG is the heat flux density to the ground (MJ m2^{-2} d1^{-1}).

The Priestley-Taylor equation provides potential evapotranspiration estimates for low advective conditions. In semiarid or arid areas where the advection component of the energy balance is significant, the Priestley-Taylor equation will underestimate potential evapotranspiration.

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