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Figure 1.11. Polar chart showing the apparent motion of the sun for an observer
                            at 35°S. ("Copyright © CSIRO 1992, Reproduced by permission of CSIRO
                            PUBLISHING, Melbourne Australia from Sunshine and Shade in Australasia 6th
                            edition (R.O. Phillips) http://www.publish.csiro.au/pid/147.htm)


                     1.8    SOLAR INSOLATION DATA AND ESTIMATION
                     Good reviews of this field have been done by, for example, Duffie and Beckman
                     (1991), Iqbal (1983), Reddy (1987), Perez et al. (2001) and Lorenzo (1989, 2003).
                     Extraterrestrial irradiation is known from geometry and the solar constant (see
                     Eqn. 1.5) but terrestrial intensities are less well defined.
                     Photovoltaic system designers often need estimates of the insolation expected to fall
                     on arbitrarily-tilted surfaces. For most purposes, monthly average daily insolation
                     values are sufficient (Lorenzo, 2003) and ‘characteristic’ days near the middle of each
                     month are often used to define average monthly values (Appendix C). Asterisks are
                     used in this book to denote variables based on characteristic days and overbars
                     indicate monthly averages. Separated direct and diffuse components are usually
                     required for estimation of the effects of module tilt, but these need to be estimated
                     from global values if not separately measured. Hence, there are three basic problems:
                         1. Evaluating the global radiation on a horizontal surface for a given site from
                            available measured quantities.






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