1:3.4.2 Generated Values

The daily generated values are determined by multiplying the residual elements generated with equation 1:3.4.1 by the monthly standard deviation and adding the monthly average value.

Tmx=μmxmon+χi(1)σmxmonT_{mx}=\mu mx_{mon} + \chi_i(1)*\sigma mx_{mon} 1:3.4.10

Tmn=μmnmon+χi(2)σmnmonT_{mn}=\mu mn_{mon} + \chi_i(2)*\sigma mn_{mon} 1:3.4.11

Hday=μradmon+χi(3)σradmonH_{day}=\mu rad_{mon} + \chi_i(3)*\sigma rad_{mon} 1:3.4.12

where TmxT_{mx} is the maximum temperature for the day (°C\degree C), μmxmon\mu mx_{mon} is the average daily maximum temperature for the month (°C\degree C), χi(1)\chi_i(1) is the residual for maximum temperature on the given day, σmxmon\sigma mx_{mon} is the standard deviation for daily maximum temperature during the month (°C\degree C), TmnT_{mn} is the minimum temperature for the day (°C\degree C), μmnmon\mu mn_{mon} is the average daily minimum temperature for the month (°C\degree C), χi(2)\chi_i(2) is the residual for minimum temperature on the given day, σmnmon\sigma mn_{mon} is the standard deviation for daily minimum temperature during the month (°C\degree C), HdayH_{day} is the solar radiation for the day (MJ m2^{-2}), μradmon\mu rad_{mon} is the average daily solar radiation for the month (MJ m2^{-2}), χi(3)\chi_i(3) is the residual for solar radiation on the given day, and σradmon\sigma rad_{mon} is the standard deviation for daily solar radiation during the month (MJ m2^{-2}).

The user is required to input standard deviation for maximum and minimum temperature. For solar radiation the standard deviation is estimated as ¼ of the difference between the extreme and mean value for each month.

σradmon=Hmxμradmon4\sigma rad_{mon}=\frac{H_{mx}-\mu rad_{mon}}{4} 1:3.4.13

where σradmon\sigma rad_{mon} is the standard deviation for daily solar radiation during the month (MJ m2^{-2}), HmxH_{mx} is the maximum solar radiation that can reach the earth’s surface on a given day (MJ m2^{-2}), and μradmon\mu rad_{mon} is the average daily solar radiation for the month (MJ m2^{-2}).

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