Page 13 - A Comprehensive Guide to Solar Energy Systems
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Chapter 1 • Why Solar Energy?  5



                 1.2  How Much Solar Energy Falls on the Earth and How
                 Much is Used to Make Electricity?

                 There are many ways of expressing how much solar energy falls on the earth. Chris Goodall
                 writes in The Switch that the sun supplies enough power in 90 min to meet the world’s total
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                 energy needs for a year [6]. In more scientific language, the Earth receives 174 × 10  W
                 [174 PW (petawatts)] of incoming solar radiation (insolation) at the upper atmosphere.
                 Approximately 30% of this is reflected back to space, while the rest is absorbed by the
                 oceans and landmasses and things on the earth. At night this 70% absorbed energy is radi-
                 ated back into space keeping the earth at a constant temperature.
                   The total solar energy absorbed by the Earth’s atmosphere, oceans, and land masses is
                                                      −1
                 approximately 3.85 × 10  J a  [3.85 yJ a  (yottajoules per annum)] [7]. Photosynthesis
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                                           −1
                                                                      −1
                 captures less than 0.1% of this, approximately 3.0 × 10  ZJ a  (zettajoules per annum), in
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                 biomass [8]. The total energy consumption in the world today is less than 0.02% of the total
                 solar energy shining on the earth.
                   Most people in the world live in areas with insolation levels of 150–300 W m  or 3.5–
                                                                                         −2
                 7.0 kW h m  d , where d refers to day [9]. This magnitude of solar energy available makes
                           –2
                              –1
                 it an appealing source of electricity. The United Nations development Programme in its
                 2000 World Energy Assessment found that the annual potential of solar energy was be-
                 tween 16 000 and 50 000 × 10  J (16 000–50 000 EJ). This is many times larger than the total
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                 world energy consumption, which was 559.8 EJ in 2012 [10].
                   Solar energy supplied only 0.45% of the total primary energy consumption in 2015. This
                 is far below traditional forms of energy or other renewable forms of energy (Table 1.1) and
                 reference [11]. Additionally, as mentioned earlier, solar energy produces 1.5% of all the
                 electricity used globally. Therefore, much work has to be done to realize the suggestion of
                 the International Energy Agency (IEA) that the sun could be the largest source of electricity
                 by 2050, ahead of fossil fuels, wind, hydro, and nuclear. According to a recent report by IEA,
                 solar PV systems could generate up to 16% of the world’s electricity by 2050, while solar
                 thermal electricity (STE) from concentrated solar power (CSP) plants could provide an
                 additional 11%; this will require an early and sustained investment in existing and future
                 solar technologies [12].

                        Table 1.1  World Energy Primary Consumption, 2015, Percentages [11]
                        Energy Types                     Percentages (%)
                        Oil                              32.9
                        Coal                             29.2
                        Gas                              23.9
                        Nuclear                          4.4
                        Hydro                            6.8
                        Wind                             1.4
                        Solar                            0.45
                        Note this table is not referring to electricity production. For the breakdown of electricity production see
                        Table 1.3 in Section 1.7.
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