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Updated: Jul 27, 2025

Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
David Santalices1,2, Mateo Martínez-García1, Jesús Belmar1
1LIR-Infrared Laboratory, Department of Physics, Universidad Carlos III de Madrid, 28911 Leganés, Spain.
A new method characterizes Martian dust by mapping its interaction volume using experimental data and tomography. This improves understanding of Martian climate and reduces simulation time for dust sensor instruments.
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