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- W3023610179 abstract "This chapter presents an overview of selective surfaces. Selective surfaces are surfaces for solar thermal absorbers that reduce reradiation losses and, hence, increase thermal efficiency of collectors. They were first demonstrated in practical collectors in 1955, and the first commercial plant for coating full-size collector plates was set up some twenty years ago. The following are the basic requirements of a practical selective surface for a solar collector: (1) high solar absorbtivity, (2) low thermal emittance, (3) long-term stability at the desired operating temperature, (4) stability to (or recovery from) short-term overheating because of a failure to extract energy from the collector, (4) stability against atmospheric corrosion, (5) applicability to given substrate materials, (6) reproducibility, and (7) reasonable cost. The physics of selective surfaces are governed by the following four physical laws: (1) Stephan–Boltzmann equation, (2) Kirchhoff's law, (3) Planck's law, and (4) Wein's law. The classical selective material is clear glass that is substantially transparent over the whole of the solar spectrum but opaque above about 2.5 μm. A glass cover over a black receiver is, therefore, often called a sunshine trap as it allows the solar radiation in but does not allow the radiation (thermal) out." @default.
- W3023610179 created "2020-05-13" @default.
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- W3023610179 date "1979-01-01" @default.
- W3023610179 modified "2023-09-24" @default.
- W3023610179 title "SELECTIVE SURFACES" @default.
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- W3023610179 doi "https://doi.org/10.1016/b978-0-08-024744-1.50014-0" @default.
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