|Title||Solar spectral optical properties of pigments—Part II: survey of common colorants|
|Publication Type||Journal Article|
|Year of Publication||2005|
|Authors||Levinson, Ronnen M., Paul Berdahl, and Hashem Akbari|
|Journal||Solar Energy Materials and Solar Cells|
|Keywords||cool roofs, Kubelka-Munk absorption and backscattering coefficients, Pigment characterization, Solar spectral optical properties, Titanium dioxide|
Various pigments are characterized by determination of parameters S (backscattering) and K (absorption) as functions of wavelength in the solar spectral range of 300–2500 nm. Measured values of S for generic titanium dioxide (rutile) white pigment are in rough agreement with values computed from the Mie theory, supplemented by a simple multiple scattering model. Pigments in widespread use are examined, with particular emphasis on those that may be useful for formulating non-white materials that can reflect the near-infrared (NIR) portion of sunlight, such as the complex inorganic color pigments (mixed metal oxides). These materials remain cooler in sunlight than comparable NIR-absorbing colors. NIR-absorptive pigments are to be avoided. High NIR reflectance can be produced by a reflective metal substrate, an NIR-reflective underlayer, and/or by the use of a pigment that scatters strongly in the NIR.