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2012 | OriginalPaper | Buchkapitel

7. Solar Energy

verfasst von : Efstathios E. (Stathis) Michaelides

Erschienen in: Alternative Energy Sources

Verlag: Springer Berlin Heidelberg

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Abstract

At an average rotational radius around the Sun of 1.49*1011 m and with an average radius of 6,378 km, the planet Earth receives solar radiation power of approximately 1.73*1014 kW, a quantity that surpasses by far all the power requirements of the Earth’s inhabitants. This continuously received power, which is called incident solar radiation and shortened to insolation , integrates to a total energy of 5.46*1021 MJ per year, or more than 100 million times the total energy used by earthlings in a year. This tremendous amount of energy is abundant, free of charge, almost uniformly distributed and available to all nations and inhabitants of the planet. However, only a very small fraction of the incident solar radiation is used by the Earth’s population. Passive solar heating systems provide with space heating and hot water a low fraction of the buildings, primarily in OECD countries, while thermal solar power plants and photovoltaic cells provide a small fraction of the electricity consumed. Despite its low utilization at present, and because of the enormous amounts of power reaching the Earth, solar energy is a prime alternative energy source and has the potential to supply a very high fraction, if not all, of the power used by the Earth’s population. This chapter starts with a short exposition on the amount of solar energy available and continues with the exposition of the two main families of systems that are currently used for power production from solar energy: solar thermal systems and photovoltaic systems. Photovoltaic solar cells and solar thermal systems utilize the solar energy in entirely different ways and are examined separately. Emphasis is given on the electric power production by solar energy as well as the current and proposed systems used for electric power production. A brief mention of the passive heating systems and the environmental effects of solar energy utilization are also included in the chapter.

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Fußnoten
1
Solstice may be roughly translated as the day when the sun stands still in the sky and equinox (equal night) implies that daytime and nighttime are equal. During the two solstices the sun is at the northernmost and the southernmost points. At these points the sun appears to stop moving and reverses its direction, thus receding towards the equator. Despite the meaning of the term, during the two equinoxes, day and night are not exactly equal because of the refraction and diffusion of the sunlight, which is caused by the atmosphere of the Earth.
 
2
Solar thermal power plants are rated based on the maximum power they may deliver. The average power produced by a solar power plant is always significantly less than the rated power.
 
3
“Heliostat” literally means “one that keeps the sun still.” Because the heliostats rotate with the sun, from the point of view of the central receiver the sun remains still at the same point in the horizon.
 
4
Wind is generally stronger in areas that have high insolation, because of the strong ground heating and the natural convection that follows.
 
Metadaten
Titel
Solar Energy
verfasst von
Efstathios E. (Stathis) Michaelides
Copyright-Jahr
2012
Verlag
Springer Berlin Heidelberg
DOI
https://doi.org/10.1007/978-3-642-20951-2_7