A primary analysis of microwave brightness temperature of lunar surface from Chang-E 1 multi-channel radiometer observation and inversion of regolith layer thicknessWenzhe Fa(Fudan University), Ya‐Qiu Jin(Fudan University)IcarusDecember 6, 200910.1016/j.icarus.2009.11.034Cited by 129SaveCiteExport RISWatch citationsAbstractRelated PapersLunar iron and titanium abundance algorithms based on final processing of Clementine ultraviolet‐visible imagesP. G. Lucey, D. T. Blewett, Bradley L. Jolliff|Journal of Geophysical Research Atmospheres|2000|613Near-Surface Temperatures on Mercury and the Moon and the Stability of Polar Ice DepositsA. R. Vasavada|Icarus|1999|606A Model of Spectral Albedo of Particulate Surfaces: Implications for Optical Properties of the MoonYurij G. Shkuratov, L. V. Starukhina, H. Hoffmann et al.|Icarus|1999|455The Lunar RegolithD. S. McKay, G. Heiken, A. Basu et al.|Unknown|1991|338Thickness determinations of the lunar surface layer from lunar impact cratersW. L. Quaide, V. R. Oberbeck|Journal of Geophysical Research Atmospheres|1968|327