Volume 44 Issue 2
Apr.  2024
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Article Navigation >  Chinese Journal of Space Science  > 2024  >  44(2): 270-286 Open Access
YANG Yazhou, MILLIKEN Ralph E, BRAMBLE Michael S, PATTERSON William R, ZOU Yongliao, LIU Yang. Laboratory Thermal Emission Spectral Measurement and Calibration Methods for Planetary Science Research (in Chinese). Chinese Journal of Space Science, 2024, 44(2): 270-286 doi: 10.11728/cjss2024.01.2023-0116
Citation: YANG Yazhou, MILLIKEN Ralph E, BRAMBLE Michael S, PATTERSON William R, ZOU Yongliao, LIU Yang. Laboratory Thermal Emission Spectral Measurement and Calibration Methods for Planetary Science Research (in Chinese). Chinese Journal of Space Science, 2024, 44(2): 270-286 doi: 10.11728/cjss2024.01.2023-0116
shu

Laboratory Thermal Emission Spectral Measurement and Calibration Methods for Planetary Science Research

doi: 10.11728/cjss2024.01.2023-0116 cstr: 32142.14.cjss2024.01.2023-0116
  • 1.

    State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing 100190

  • 2.

    Department of Earth, Environmental, and Planetary Sciences, Brown University, Providence 02912

  • Received Date: 2023-10-22
  • Accepted Date: 2024-01-15
  • Rev Recd Date: 2023-11-19
    • Available Online: 2023-12-04
    Abstract
  • Accurate information regarding the surface composition is crucial for understanding the formation and evolution history of planetary bodies. Visible and near-infrared remote sensing spectroscopic techniques have long been used for the detection of surface composition. However, in the thermal infrared spectral range, various types of planetary surface materials exhibit richer spectral features. With the development of thermal emission spectroscopic techniques, it has been increasingly used in planetary exploration. Particularly, in the ongoing and planned asteroid exploration missions, thermal emission spectrometers are employed as key payloads. In order to better interpret the thermal emission spectral data to be obtained in the future, it is essential to establish scientifically reasonable data processing and calibration schemes. This paper provides a comprehensive overview on the design of thermal emission spectral measurement devices for planetary science research, the measurement process, and data reduction methods. To obtain accurate emissivity spectra data, the challenge of distinguishing sample radiation signals from instrument radiation during thermal emission measurements must be properly addressed first. Especially, for measurements conducted under low-temperature and vacuum conditions that are similar to the surface conditions of the Moon and asteroids. This paper proposes and demonstrates a data reduction method based on interferograms, which are the original signals measured by FTIR spectrometer. This method can effectively separate the actual radiation signal from the samples, thus yielding more accurate emissivity spectra data. The insights derived from this study can serve as valuable references for the development and construction of thermal emission measurement devices and can facilitate the processing and scientific interpretation of data from future missions such as Tianwen-2.

     

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