Comparison between the Shkuratov and Hapke scattering theories for solid planetary surfaces: Application to the surface composition of two Centaurs

By François Poulet, J. Cuzzi, Dale P. Cruikshank, Ted L. Roush, Cristina Dalle Ore. 2002

138 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/76789ecbfc7329edc10208f49a9da0725aa21af4

How researchers see this paper

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In Astronomy and Astrophysics

1. J. Bibring
2. Yves Langevin
3. B. Gondet
4. François Poulet
5. Nicolas Mangold
6. J. Carter
7. J. Michalski
8. D. Loizeau

Citations in the corpus

• VLT/SINFONI OBSERVATIONS OF EUROPA: NEW INSIGHTS INTO THE SURFACE COMPOSITION (2016, methodology): “…spectra of amorphous and crystalline water ices at 120 K were derived from the Shkuratov radiative transfer model (Shkuratov et al. 1999; Poulet et al. 2002) using the optical constants of both types of water ices provided by Mastrapa et al. (2008) and by the GhoSST online database…”
• A Review of Nonlinear Hyperspectral Unmixing Methods (2014, methodology): “This model was compared with the Hapke model in [60], and validated on laboratory mixtures in [61].”
• Abundance of minerals in the phyllosilicate-rich units on Mars (2008, methodology): “Moreover, the model has been successfully applied to spectra of a variety of planetary surfaces including the Martian surface (e.g. Poulet et al. 2002, 2003; Arvidson et al. 2007).”