Diurnal physical temperature at Sinus Iridum area retrieved from observations of Chinese Chang’E-1 microwave radiometer

[1]  Ya-Qiu Jin,et al.  Global inventory of Helium-3 in lunar regoliths estimated by a multi-channel microwave radiometer on the Chang-E 1 lunar satellite , 2010 .

[2]  Ya-Qiu Jin,et al.  A primary analysis of microwave brightness temperature of lunar surface from Chang-E 1 multi-channel radiometer observation and inversion of regolith layer thickness , 2010 .

[3]  A. Vasavada,et al.  Apollo Lunar Heat Flow Experiments and the LRO Diviner Radiometer , 2010 .

[4]  Ya-Qiu Jin,et al.  An inversion approach for lunar regolith layer thickness using optical albedo data and microwave emission simulation , 2009 .

[5]  J. Oberst,et al.  Lunar Global Shape and Polar Topography Derived from Kaguya-LALT Laser Altimetry , 2009, Science.

[6]  Judith C. Chow,et al.  Spatial and seasonal distributions of carbonaceous aerosols over China , 2007 .

[7]  Ya-Qiu Jin,et al.  Quantitative estimation of helium-3 spatial distribution in the lunar regolith layer , 2007 .

[8]  Yaqiu Jin,et al.  Simulation of brightness temperature from lunar surface and inversion of regolith‐layer thickness , 2007 .

[9]  A. Vasavada,et al.  Near-Surface Temperatures on Mercury and the Moon and the Stability of Polar Ice Deposits☆ , 1999 .

[10]  C. Dalton,et al.  Conceptual design of a lunar colony , 1972 .

[11]  R. Shorthill,et al.  Nonuniform Cooling of the Eclipsed Moon: A Listing of Thirty Prominent Anomalies , 1965, Science.

[12]  C. Allen,et al.  The Lunar Reconnaissance Orbiter Diviner Lunar Radiometer Experiment , 2010 .

[13]  Kang-Tsung Chang,et al.  Introduction to Geographic Information Systems , 2001 .

[14]  S. Keihm,et al.  Comparison of theoretical and observed 3.55 cm wavelength brightness temperature maps of the full moon , 1979 .

[15]  S. Keihm,et al.  The Revised Lunar Heat Flow Values , 1976 .