Solar Energy Perspectives - IEA
Solar Energy Perspectives - IEA
Solar Energy Perspectives - IEA
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<strong>Solar</strong> <strong>Energy</strong> <strong>Perspectives</strong>: The solar resource and its possible uses<br />
may influence cloud cover and reduce clarity, and the potential of the solar energy resource<br />
in different regions of the globe. Current models suggest, however, that monthly average<br />
changes in solar fluxes will remain very low – though this is not necessarily true with respect<br />
to direct normal irradiance.<br />
Two basic ways to capture the sun’s energy<br />
<strong>Solar</strong> rays can be distinguished according to their wavelengths, which determine visible light,<br />
infrared and ultraviolet radiation. Visible light constitutes about 40% of the radiated energy,<br />
infrared 50% and ultraviolet the remaining 10%. Most of the infrareds are “near infrared” or<br />
“short-wave infrared” rays, with wavelengths shorter than 3 000 nanometres, so they are not<br />
considered “thermal radiation”.<br />
The sun’s primary benefit for most people is light, the use of which can be improved in<br />
buildings to reduce energy consumption. This area of development, called day lighting, is<br />
one of the avenues to reducing energy consumption in buildings.<br />
<strong>Solar</strong> irradiative energy is easily transformed into heat through absorption by gaseous, liquid<br />
or solid materials. Heat can then be used for comfort, in sanitary water heating or pool water<br />
heating, for evaporating water and drying things (notably crops and food), and in space<br />
heating, which is a major driver of energy consumption. Heat can also be transformed into<br />
mechanical work or electricity, and it can run or facilitate chemical or physical transformations<br />
and thus industrial processes or the manufacture of various energy vectors or fuels, notably<br />
hydrogen.<br />
However, solar radiation can also be viewed as a flux of electromagnetic particles or photons.<br />
Photons from the sun are highly energetic, and can promote photoreactions such as in<br />
photosynthesis and generate conduction of electrons in semiconductors, enabling the<br />
photovoltaic conversion of sunlight into electricity. Other photoreactions are also being used,<br />
for example photocatalytic water detoxification.<br />
Note that the two fundamental methods to capture energy from the sun – heat and<br />
photoreaction – can also be combined in several ways to deliver combined energy vectors –<br />
e.g. heat and electricity.<br />
Thus, from the two basic ways of capturing the sun’s energy, apart from day lighting, i.e. heat<br />
and photoreaction, we distinguish four main domains of applications: photovoltaic electricity,<br />
heating (and cooling), solar thermal electricity, and solar fuel manufacture. The relevant<br />
technologies are detailed in Chapters 6 to 9 of this publication.<br />
How this resource varies<br />
Although considerable, the solar resource is not constant. It varies throughout the day and<br />
year, and by location. For a large part, these variations result directly from the earth’s<br />
geography and its astronomical movements (its rotation towards the East, and its orbiting the<br />
sun). But these variations are accentuated and made somewhat less foreseeable from day to<br />
day by the interplay between geography, ocean and land masses, and the ever-changing<br />
composition of the atmosphere, starting with cloud formation.<br />
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© OECD/<strong>IEA</strong>, 2011