1996
DOI: 10.1016/0040-6090(95)08023-6
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Optimum thickness determination to maximise the spectral selectivity of black pigmented coatings for solar collectors

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Cited by 26 publications
(7 citation statements)
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“…The terrestrial solar spectral irradiance distribution curve commences at wavelength λ≥0.3 μm, while for λ≥2 μm it is almost insignificant. For temperatures lower than 773 K, most thermal radiation (98%) occurs at λ≥2 μm due to black body radiation [52]. This leads to the following formal definitions.…”
Section: Solar Absorptance and Thermal Emittancementioning
confidence: 99%
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“…The terrestrial solar spectral irradiance distribution curve commences at wavelength λ≥0.3 μm, while for λ≥2 μm it is almost insignificant. For temperatures lower than 773 K, most thermal radiation (98%) occurs at λ≥2 μm due to black body radiation [52]. This leads to the following formal definitions.…”
Section: Solar Absorptance and Thermal Emittancementioning
confidence: 99%
“…One of the most common strategies in preparing a spectrally selective surface is to apply a highly solar absorptive thin film onto a non-selective highly reflective metal substrate (absorber-reflector tandem). The absorptive layers need to be transparent in the infrared region to maintain the low thermal emittance of the substrate [45,52,54]. To further supplement the understanding of these concepts, the absorption, transmission and emission in the solar selective absorber-reflector tandem system are illustrated in Fig.…”
Section: Solar Absorptance and Thermal Emittancementioning
confidence: 99%
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“…The increase in the absorptivity with thickness points to well-established light-absorption and scattering phenomena as the reason for the selectivity. 25 The PC data in Fig. 4, on the other hand, show a more distinct nonlinearity compared to the reference coating and point to another mechanism behind the relation between the selectivity and the thickness of the coating.…”
Section: Spectral Selectivitymentioning
confidence: 98%