What are the colors seen by MISR?
In each of the nine MISR cameras, images will be obtained in four spectral bands, i.e. in four different colors, one each for blue, green, red, and near-infrared. The center wavelength of each of these bands is 446, 558, 672, and 867 nanometers respectively.
Why are these particular color bands chosen?
The bands in the red and near-infrared (672 and 867 nm) provide vegetated surface identification owing to their positioning on either side of the "red edge" marking the transition between chlorophyll absorption and cellulose reflectance. These two bands are also useful for marine aerosol studies since water is nearly black at these wavelengths.
The green band at 558 nm is near the peak of the solar spectrum, and thus will be given high weight in studies to estimate broadband reflecting properties (albedos).
A wide range of spectral coverage is essential to using the wavelength dependence of aerosol opacity to estimate the size distribution of the aerosol particulates. Thus the blue channel at 446 nm provides nearly a twofold change in particle size-to-wavelength ratio relative to the near-infrared channel at 867 nm.
The four bands also comprise an effective set for ocean color studies at low ocean pigment concentrations.
Overall, the MISR wavelengths have been selected to avoid known ranges of strong atmospheric gas absorption and solar Fraunhofer lines. These absorption effects would complicate the retrieval of aerosol information, and make the instrument more sensitive to changes in spectral response that might occur over time during the life of the mission.