Page 315 - Applied Photovoltaics
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                     where the units are kW/m , Į is the noon-time altitude of the sun for month i, given
                     by Eqn. (1.22), ȕ is the angle of inclination of the array on which I si is incident, AM is
                     the air mass (1/sinĮ) and the factor 1.10 allows for the inclusion of the diffuse
                     component for a cloudless day.































                            Figure H.1:  Procedure for determining light intensity incident on solar panels at
                            angle ȕ at noon.


                     Similarly, for typical cloudy days, the maximum light intensity I ci  for month i is
                     estimated from

                                              I ci     . 1  353u  7 . 0  AM  . 0  678  u  . 0  20  (H.2)

                     where the factor 0.20 represents the assumed diffuse light intensity, which is assumed
                     to be independent of b.
                         1. From the values for I si and I ci for each month i, use Fig. H.2 to estimate the
                            light intensity incident on the array at inclination angle ȕ throughout each day
                            for sunny and cloudy days, respectively. This facilitates the calculation of the
                                  2
                            kWh/m /day for both sunny and cloudy days by using appropriate values for
                            the ‘time’ axis, as given by N in Fig. H.2.

                         2. Determine the percentage of sunny days given by Fig. H.2 with I equated to
                            I si for each month. This can be found from Eqn. (H.3), which gives the
                            average daily global radiation (G i ) falling on the array at inclination ȕ for
                            each month (i) in the design period as the sum of the sunny-day and cloudy-
                            day components of insolation

                                       G    X u 76  u  N u  I    Y u 76 u  N u  I  (H.3)
                                                .
                                                                6
                                                                 .
                                               6
                                         i   i        i   si  i        i  ci
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