A New Method for Simulation of Lunar Microwave Brightness Temperatures and Evaluation of Chang'E‐2 MRM Data Using Thermal Constraints From Diviner

Author:

Wei Guangfei123ORCID,Li Xiongyao134,Gan Hong25,Blewett David T.6ORCID,Neish Catherine D.7,Greenhagen Benjamin T.6

Affiliation:

1. Center for Lunar and Planetary Sciences, Institute of GeochemistryChinese Academy of Sciences Guiyang China

2. State Key Laboratory of Lunar and Planetary SciencesMacau University of Science and Technology Macau China

3. CAS Center for Excellence in Comparative Planetology Hefei China

4. Key Laboratory of Space Manufacturing TechnologyChinese Academy of Sciences Beijing China

5. Analyzing and Testing CenterGuizhou Institute of Technology Guiyang China

6. Planetary Exploration GroupJohns Hopkins University Applied Physics Laboratory Laurel MD USA

7. Department of Earth SciencesWestern University London Ontario Canada

Funder

China Scholarship Council

National Natural Science Foundation of China

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics

Reference55 articles.

1. Lunar surface rock abundance and regolith fines temperatures derived from LRO Diviner Radiometer data;Bandfield J. L.;Journal of Geophysical Research,2011

2. Lunar surface roughness derived from LRO Diviner Radiometer observations;Bandfield J. L.;Icarus,2015

3. Blewett D. Zheng Y. C. Chan K. Hu G. Neish C. Tsang K. &Zhu Y.(2018).Chang'E‐2 microwave brightness temperature maps of the Moon. InLunar and Planetary Science Conference(Vol.49).

4. Lobate impact melt flows within the extended ejecta blanket of Pierazzo crater;Braya V. J.;Icarus,2018

5. Carrier W. Mitchell J. &Mahmood A.(1973).The relative density of lunar soil. InProceedings of the Lunar Science Conference(Vol.4 pp.2403–2411).Houston.

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