Lunar Brightness Temperature Model Based on the Microwave Radiometer Data of Chang'e-2

The brightness temperature (TB) data of the Moon acquired by the microwave radiometer (MRM) on-board the Chinese Chang'e-2 (CE-2) lunar probe are valuable and comprehensive data, which can be helpful in studying the physical properties of the lunar regolith, such as thickness, physical temperat...

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Published inIEEE transactions on geoscience and remote sensing Vol. 55; no. 10; pp. 5944 - 5955
Main Authors Cai, Zhanchuan, Lan, Ting
Format Journal Article
LanguageEnglish
Published New York IEEE 01.10.2017
The Institute of Electrical and Electronics Engineers, Inc. (IEEE)
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Abstract The brightness temperature (TB) data of the Moon acquired by the microwave radiometer (MRM) on-board the Chinese Chang'e-2 (CE-2) lunar probe are valuable and comprehensive data, which can be helpful in studying the physical properties of the lunar regolith, such as thickness, physical temperature, and dielectric constant. To construct the accurate and high-resolution lunar TB model with the TB data obtained by the MRM on-board CE-2, 2401 tracks of the original TB data are quantized by using the hour angle processing, and the hierarchical MK splines function (HMKSF) method is presented, which uses a hierarchy of coarse-to-fine control lattices to generate a sequence of TB model functions. The TB model constructor is the sum of the TB model functions derived at each level of the hierarchy. In addition, the lunar TB models with a resolution of 0.5°×0.5° in all four frequency channels are constructed for both the daytime and the nighttime. The obtained models show rich information, e.g., the global distribution of TB over the lunar surface, the effect of frequency on the TB model.
AbstractList The brightness temperature (TB) data of the Moon acquired by the microwave radiometer (MRM) on-board the Chinese Chang'e-2 (CE-2) lunar probe are valuable and comprehensive data, which can be helpful in studying the physical properties of the lunar regolith, such as thickness, physical temperature, and dielectric constant. To construct the accurate and high-resolution lunar TB model with the TB data obtained by the MRM on-board CE-2, 2401 tracks of the original TB data are quantized by using the hour angle processing, and the hierarchical MK splines function (HMKSF) method is presented, which uses a hierarchy of coarse-to-fine control lattices to generate a sequence of TB model functions. The TB model constructor is the sum of the TB model functions derived at each level of the hierarchy. In addition, the lunar TB models with a resolution of 0.5°×0.5° in all four frequency channels are constructed for both the daytime and the nighttime. The obtained models show rich information, e.g., the global distribution of TB over the lunar surface, the effect of frequency on the TB model.
Author Zhanchuan Cai
Ting Lan
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Snippet The brightness temperature (TB) data of the Moon acquired by the microwave radiometer (MRM) on-board the Chinese Chang'e-2 (CE-2) lunar probe are valuable and...
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SubjectTerms Brightness
Brightness temperature
Brightness temperature (TB)
Chang’e-2 (CE-2)
Chinese spacecraft
Data
Data acquisition
Data models
Dielectric constant
Lattices
Lunar exploration
Lunar probes
Lunar surface
Mathematical models
microwave radiometer (MRM)
Microwave radiometers
Microwave radiometry
Microwave theory and techniques
Moon
Physical properties
Radiometers
Regolith
Resolution
Splines
Splines (mathematics)
Surface radiation temperature
TB model
Temperature
Temperature effects
Title Lunar Brightness Temperature Model Based on the Microwave Radiometer Data of Chang'e-2
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