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PET by Penman method, Kathmandu in February

Short answer

Actual vapour pressure is 7.98 mm Hg; using a = 0.29 cos 28.5° and n/N = 0.588 gives net radiation H_n = 1.780 mm/day and E_a = 2.095 mm/day. Penman's equation gives PET = 1.87 mm/day, about 52 mm for February.

Calculate the potential evapotranspiration for an area over Kathmandu in the month of February by Penman Method. The following data is available.

Mean Monthly Temperature: 12.5∘^\circC Mean RH: 70% Mean Sunshine Hours: 7 h Potential Sunshine Hours: 11.9 h Wind Velocity at 2 m Height = 120 km/day Albedo: 0.15 Upper Terrestrial Solar Radiation: 9 mm of water/day

Other values: Latitude: 28.50 Longitude: 84.50 Saturated Vapor Pressure at 12.5∘^\circC: 11.4 mm of Hg Slope of Saturated Vapor Pressure: 1.24 mm/∘^\circC Psychrometric Constant: 0.49 mm/∘^\circC Boltzman Constant: 2.0×10−92.0 \times 10^{-9} mm/day

Penman's method combines the energy-balance and aerodynamic (mass-transfer) approaches:

PET=AHn+EaγA+γPET = \frac{A H_n + E_a \gamma}{A + \gamma}

where AA = slope of the saturation vapour pressure curve, γ\gamma = psychrometric constant, HnH_n = net radiation (mm of water/day) and EaE_a = drying power of air (mm/day).

Hn=Ha(1−r)(a+bnN)−σTa4(0.56−0.092ea)(0.1+0.9nN),a=0.29cos⁡φ, b=0.52H_n = H_a(1-r)\left(a + b\frac{n}{N}\right) - \sigma T_a^4\left(0.56 - 0.092\sqrt{e_a}\right)\left(0.1 + 0.9\frac{n}{N}\right), \qquad a = 0.29\cos\varphi,\ b = 0.52

Step 1: Vapour pressure

ea=RH×es=0.70×11.4=7.98 mm Hge_a = RH \times e_s = 0.70 \times 11.4 = 7.98\ \text{mm Hg}

Step 2: Net radiation HnH_n

Sunshine ratio n/N=7/11.9=0.588n/N = 7/11.9 = 0.588, and a=0.29cos⁡(28.5∘)=0.2549a = 0.29\cos(28.5^\circ) = 0.2549.

Short-wave part:

9×(1−0.15)×(0.2549+0.52×0.588)=7.65×0.5607=4.290 mm/day9 \times (1-0.15)\times(0.2549 + 0.52\times0.588) = 7.65 \times 0.5607 = 4.290\ \text{mm/day}

Long-wave part, with Ta=12.5+273=285.5T_a = 12.5 + 273 = 285.5 K:

σTa4=2.0×10−9×285.54=13.29 mm/day\sigma T_a^4 = 2.0\times10^{-9}\times 285.5^4 = 13.29\ \text{mm/day} 13.29×(0.56−0.0927.98)×(0.1+0.9×0.588)=13.29×0.3001×0.6294=2.510 mm/day13.29\times(0.56 - 0.092\sqrt{7.98})\times(0.1 + 0.9\times0.588) = 13.29\times0.3001\times0.6294 = 2.510\ \text{mm/day} Hn=4.290−2.510=1.780 mm/dayH_n = 4.290 - 2.510 = 1.780\ \text{mm/day}

Step 3: Drying power of air

Ea=0.35(1+u2160)(es−ea)=0.35×(1+120160)×(11.4−7.98)=2.095 mm/dayE_a = 0.35\left(1 + \frac{u_2}{160}\right)(e_s - e_a) = 0.35\times\left(1+\frac{120}{160}\right)\times(11.4-7.98) = 2.095\ \text{mm/day}

Step 4: PET

PET=1.24×1.780+0.49×2.0951.24+0.49=2.207+1.0271.73=1.87 mm/dayPET = \frac{1.24\times1.780 + 0.49\times2.095}{1.24+0.49} = \frac{2.207+1.027}{1.73} = 1.87\ \text{mm/day}

For February (28 days): 1.869×28≈52.31.869\times28 \approx 52.3 mm.

Answer: PET = 1.87 mm/day, about 52 mm for February.

(The latitude is used only to find a=0.29cos⁡φa = 0.29\cos\varphi; the longitude is not needed. The extraterrestrial radiation is already given.)

✓ Answer checked by Claude Sonnet 5.5

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