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- W4320912061 abstract "提出使用高分辨率的Diviner辐射计红外温度作为月壤热传导的边界输入条件，使得月壤物理温度廓线的模拟更接近月表真实情况. 利用Diviner物理温度廓线模拟的微波亮温与嫦娥二号卫星微波探测仪（CELMS2）的实测亮温匹配，来分析CELMS2数据的有效性和稳定性，为月壤微波特性的反演奠定基础. 以哥白尼坑区域为例，对比分析了Diviner辐射计红外通道温度与CELMS1实测微波亮温的变化趋势. 选择月球虹湾地区内一位置点（45.1°-45.5°N，33.1°-33.5°W），分析了CELMS2在该位置点内5个月球时刻的亮温数据. 通过对实测亮温与模拟亮温在经纬度和太阳高度角的匹配分析得到，在高频微波通道内两者的相关性达到96%以上，表明嫦娥二号微波探测仪亮温数据具有较高的稳定性，可以为月壤特性反演研究提供可靠数据来源." @default.
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- W4320912061 date "2014-01-01" @default.
- W4320912061 modified "2023-09-26" @default.
- W4320912061 title "Comparison between Diviner Data and CELMS Data" @default.
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- W4320912061 doi "https://doi.org/10.11728/cjss2014.03.249" @default.
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