Optical constants of ice from the ultraviolet to the microwave: A revised compilation

By S. Warren, R. Brandt. 2008

989 citations recorded by the source corpus.

Subfields: Atmospheric Science, Global and Planetary Change

View Paper: https://www.semanticscholar.org/paper/c50626fadadc2a4c7cf18d3f718a63b320f5b479

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Citations in the corpus

Physically based snow albedo model for calculating broadband albedos and the solar heating profile in snowpack for general circulation models (2011, methodology): “In the present study, we employed the refractive index of ice revised by Warren and Brandt [2008] , in which the imaginary part at the wavelengths 0.2 < l < 0.5 mm is much lower than that in the previous data set compiled by Warren [1984].”
The 2009 edition of the GEISA spectroscopic database (2011, background): “Table 13 gives the list of refractive indices [349-376], representing a contribution from”
A review of snow and ice albedo and the development of a new physically based broadband albedo parameterization (2010, background): “…1980; Wiscombe and Warren, 1980; Warren, 1982; Mullen and Warren, 1988; Askebjer et al., 1997; Warren et al., 2002; Ackermann et al., 2006; Warren and Brandt, 2008], but there have been few attempts to derive theoretically based, computationally simple broadband (spectrally integrated)…”
NOMAD, an Integrated Suite of Three Spectrometers for the ExoMars Trace Gas Mission: Technical Description, Science Objectives and Expected Performance (2018, methodology): “The refractive indexes that are adopted for the Mie computation are from Warren and Brandt (2008) for H 2 O ice, from Wolff et al. (2009, 2010) for Martian dust and from Hansen (1997, 2005) for CO 2 ice.”
Improvements in Shortwave Bulk Scattering and Absorption Models for the Remote Sensing of Ice Clouds (2011, background): “The complex refractive index of ice from the ultraviolet to the microwave regions has been updated in Warren and Brandt (2008).”
The 2015 edition of the GEISA spectroscopic database (2016, background): “Table 13 gives the list of refractive indices [347-374], representing a contribution from”
OPTICAL CONSTANTS OF AMORPHOUS AND CRYSTALLINE H2O-ICE: 2.5–22 μm (4000–455 cm−1) OPTICAL CONSTANTS OF H2O-ICE (2009, background): “The region near 3 μm of the H2O-ice spectrum has been well studied (Bertie & Whalley 1964; Hale & Querry 1973; Whalley 1977; Bergren et al. 1978; Warren 1984; Warren & Brandt 2008) but usually at temperatures too high or too low for direct comparison to solar system objects.”
Evidence for exposed water ice in the Moon’s south polar regions from Lunar Reconnaissance Orbiter ultraviolet albedo and temperature measurements (2015, methodology): “We used water ice optical constants from Warren and Brandt (2008), and a modified version of the lunar regolith simulated optical constants as in Hendrix et al. (2012).”
Observations of the Icy Universe (2015, background): “Some ices also have strong electronic transitions in the UV, e.g. in the case of H2O near 0.14 µm (Warren & Brandt, 2008).”
Spectrally Consistent Scattering, Absorption, and Polarization Properties of Atmospheric Ice Crystals at Wavelengths from 0.2 to 100 um (2013, methodology): “In our calculations, we used the most recent compilation of the refractive index of ice (Warren and Brandt 2008) from 0.”
A general database of hydrometeor single scattering properties at microwave and sub-millimetre wavelengths (2018, positive): “The long column, short column, block column, thick plate and thin plate, taken from Liu (2008), are all hexagonal and have axial ratios of 4, 2, 1, 0.2 and 0.05, respectively.”