A primary analysis of microwave brightness temperature of lunar surface from Chang-E 1 multi-channel radiometer observation and inversion of regolith layer thickness-Reference-Cited by-同舟云学术

A primary analysis of microwave brightness temperature of lunar surface from Chang-E 1 multi-channel radiometer observation and inversion of regolith layer thickness

Published:2010-06 Issue:2 Volume:207 Page:605-615
ISSN:0019-1035
Container-title:Icarus
language:en
Short-container-title:Icarus

Author:

Fa Wenzhe,Jin Ya-Qiu

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference21 articles.

1. Physical properties of the lunar surface;Carrier,1991

2. Simulation of brightness temperature from lunar surface and inversion of regolith layer thickness;Fa;J. Geophys. Res.,2007

3. Quantitative estimation of helium-3 spatial distribution in the lunar regolith layer;Fa;Icarus,2007

4. Backscattering from an undulating surface with application to radar returns from the Moon;Hagfor;J. Geophys. Res.,1964

5. Lunar Source-Book: A User’s Guide to the Moon;Heiken,1991

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