Uses the equation developed by Priestley and Taylor (1972) for ET0 calculation from temperature and solar radiation.
"The Priestley-Taylor equation was developed as a substitute to the Penman-Monteith equation to remove dependence on observations. For Priestley-Taylor, only radiation (irradiance) observations are required. This is done by removing the aerodynamic terms from the Penman-Monteith equation and adding an empirically derived constant factor, \alpha. (source: Wikipedia)
Priestley, C.H.B., Taylor, R.J., 1972. On the Assessment of Surface Heat Flux and Evaporation Using Large-Scale Parameters. Monthly Weather Review 100, 81-92. doi:10.1175/1520-0493(1972)100<0081:OTAOSH>2.3.CO;2
Content Type | Name | Description | Data Type | Unit | Min Value | Max Value | Default Value |
---|---|---|---|---|---|---|---|
constant | cAlphaPT | Priestley-Taylor coefficient | DOUBLE | 1 | 0.0 | - | 1.26 |
constant | cAltitude | altitude | DOUBLE | m | - | - | 0.0 |
input | iNetRadiation | net radiation | DOUBLE | MJ/(m2 d) | - | - | 0.0 |
input | iTMax | maximum daily temperature | DOUBLE | °C | - | - | 0.0 |
input | iTMin | minimum daily temperature | DOUBLE | °C | - | - | 0.0 |
out | ReferenceCropEvapotranspiration | reference evapotranspiration (ET0) | DOUBLE | mm/d | - | - | 0.0 |