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Convective Heat Transfer in Solar Energy Systems

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Solar Energy Thermal Technology

Abstract

In determining the heat loss by buoyancy-driven convection between the collector plate and the glass cover, when mounted at an angle between 0° and 75° from the horizontal, the following correlation (Hollands et al. 1976) is suggested:

$$Nu = 1.144{\left[ {1 - \frac{{1708}}{{Gr\,\Pr \,\cos \,\beta }}} \right]^ + }\left[ {1 - \frac{{{{\left( {1708\,\sin \,1.8\beta } \right)}^{1.6}}}}{{Gr\,\Pr \,\cos \,\beta }}} \right] + \left[ {\frac{{Gr\,\Pr \cos \,{\beta ^{0.33}}}}{{5830}} - 1} \right]$$
((5.1.1.))

The superscript + denotes a positive value for the quantity in brackets if this quantity is greater than zero and a value of zero otherwise. The characteristic length in determining Gr is taken as the thickness of the air cavity.

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© 1992 Springer-Verlag London Limited

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Norton, B. (1992). Convective Heat Transfer in Solar Energy Systems. In: Solar Energy Thermal Technology. Springer, London. https://doi.org/10.1007/978-1-4471-1742-1_5

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  • DOI: https://doi.org/10.1007/978-1-4471-1742-1_5

  • Publisher Name: Springer, London

  • Print ISBN: 978-1-4471-1744-5

  • Online ISBN: 978-1-4471-1742-1

  • eBook Packages: Springer Book Archive

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