Lunar surface dielectric constant, regolith thickness, and 3He abundance distributions retrieved from the microwave brightness temperatures of CE-1 Lunar Microwave Sounder

Author:

Wang ZhenZhan,Li Yun,Jiang JingShan,Li DiHui

Publisher

Springer Science and Business Media LLC

Subject

General Earth and Planetary Sciences

Reference12 articles.

1. Zhang X H, Jiang J S, Wang Z Z, et al. Design for Chang’E I lunar microwave sounder. Sci Technol Front China, 2008, 11: 103–129

2. Wang Z Z, Li Y, Jiang J S, et al. A Microwave Radiative Transfer Model Applied To Lunar Soil Remote Sensing. Electromagnetic field problems and applications, In: The International Conference on Electromagnetic Field Problems and Applications, April 26–28, 2008. Chongqing: China Chongqing University

3. Wang Z Z, Li Y, Jiang J S, et al. Methods of remote sensing lunar surface by Microwave sounder on CE-1. In: 2008 International Conference on Microwave and Millimeter Wave Technology, Nanjing, China. 2008. 4: 21–24

4. Olhoeft G R, Strangway D W. Dielectical properties of the first 100 meters of the Moon. Earth Planet Sci Lett, 1975, 24: 394–404

5. Li Y, Wang Z Z, Jiang J S. Simulation on the influence of lunar surface temperature profiles on CE-1 lunar microwave sounder brightness temperature. Sci China Earth Sci, 2010, doi: 10.1007/s11430-010-4021-0

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