Mapping the Lunar Heat Flow: Methodology and New Constraints From Recalibrated Chang'E-2 Microwave Radiometer Data

被引:5
|
作者
Keihm, Stephen J. [1 ]
Hu, Guoping [2 ,3 ]
Wang, Zhenzhan [4 ]
机构
[1] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[2] Sun Yat sen Univ, Sch Geospatial Engn & Sci, Zhuhai 519082, Peoples R China
[3] Minist Nat Resources, Key Lab Nat Resources Monitoring Trop & Subtrop Ar, Zhuhai 519082, Peoples R China
[4] Chinese Acad Sci, Natl Space Sci Ctr, Key Lab Microwave Remote Sensing, Beijing 100190, Peoples R China
基金
中国国家自然科学基金;
关键词
Chang'E-2 (CE2) microwave radiometer (MRM); lunar heat flow (HF); MOON;
D O I
10.1109/TGRS.2023.3335855
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Basic radiative transfer theory reveals that the physical temperature gradients related to heat flow (HF) within the lunar regolith below the diurnal-varying layer can be constrained by measurements of brightness temperature (TB) variations over a selected wavelength range, coupled with knowledge of the regolith electrical loss properties. We present a methodology illustrating the processing using recalibrated data from the Chang'E-2 (CE2) 10- and 3.85-cm wavelength microwave radiometer (MRM) data (channels 1 and 2). The utilized data are contained in latitude bins of 1 degrees width centered at latitudes of 0,5, . . . , 60, north and south. Results, presented as retrieved HF gradients (dT/dz in K/m) versus longitude for each of the 25 latitude bins, provide useful constraints on the overall variability of the HF gradient within the 60S-60N latitude range. In particular, no evidence is found that HF variations exceeding twice the Apollo value occur widely in the extensive highland regions of low electrical loss. Limitations related primarily to signal-to-noise ratio (SNR) issues in regions of elevated electrical loss severely reduce thermal gradient retrieval accuracy needed for correlation with enhanced thorium concentrations observed in the frontside mare. Analyses of the CE2 data reveal a noise uncertainty of similar to 0.5 K in the TB10-TB3.85 measurements, equivalent to similar to 0.7-1.4 (loss tangent dependent) times the Apollo-measured mean HF value of 1.8e(-6) W/cm(2). The limitations preclude meaningful identification of regional variations within a precision of less than one Apollo HF unit. An analysis is presented demonstrating that a threefold increase in SNR would be attained by addition of a 30-cm wavelength channel to the CE2 MRMs design, providing sufficient resolution to map regional HF variations to similar to 0.5e(-6) W/cm(2) precision, similar to 30% of the averaged Apollo sites' measured HF value.
引用
收藏
页码:1 / 14
页数:14
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