Empirical Evaluation of S-band Radar Polarimetric Response to Surface Rock Abundance across the Lunar Highlands and Maria

Polarimetric radar measurements are sensitive to viewing geometry, wavelength-scale roughness, and composition. As a result, radar imaging enables characterization of planetary surfaces, but the multiple contributors to backscatter complicate the interpretation of metrics commonly treated as proxies...

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Detalhes bibliográficos

Principais autores:	Edgard G. Rivera-Valentín, Caleb I. Fassett, Anne K. Virkki, Santa L. Pérez-Cortés, Tyler Powell, Dylan C. Hickson, Michael C. Nolan, G. Wesley Patterson
Formato:	Artigo
Idioma:	Inglês
Publicado em:	IOP Publishing 2026-01-01
coleção:	The Planetary Science Journal
Assuntos:	Radar observations Lunar surface Lunar regolith
Acesso em linha:	https://doi.org/10.3847/PSJ/ae6fa4
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