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Article

Initial In-Flight Spectral Calibration of the Near-Infrared Spectra Acquired by the MarSCoDe Onboard the Zhurong Rover

1
Key Laboratory of Space Active Opto-Electronics Technology, Shanghai Institute of Technical Physics, Chinese Academy of Sciences, Shanghai 200083, China
2
University of Chinese Academy of Sciences, Beijing 100049, China
3
Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, China
4
Hangzhou Institute for Advanced Study, University of Chinese Academy of Sciences, Hangzhou 310024, China
5
Key Laboratory of Lunar and Deep Space Exploration, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China
6
Anhui Institute of Optics and Fine Mechanics, Chinese Academy of Sciences, Hefei 230000, China
*
Author to whom correspondence should be addressed.
Remote Sens. 2022, 14(9), 2137; https://doi.org/10.3390/rs14092137
Submission received: 30 March 2022 / Revised: 26 April 2022 / Accepted: 27 April 2022 / Published: 29 April 2022
(This article belongs to the Special Issue Planetary Remote Sensing: Chang’E-4/5 and Mars Applications)

Abstract

The Zhurong rover successfully landed in southern Utopia Planitia as part of the Tianwen-1 mission on 15 May 2021. One of the objectives of the Mars Surface Composition Detector (MarSCoDe) onboard the rover is to investigate mineral compositions on the Martian surface by measuring the near-infrared reflectance spectra. Before conducting spectral interpretation, in-flight data calibration is a crucial step due to the significant differences between the laboratory and the Martian environment. The work of the MarSCoDe spectrometer is based on an acousto-optic tunable filter (AOTF). The temperature variation of the AOTF could induce wavelength offset, making mineral identification uncertain. We first analyzed the viewing geometry of the spectral measurements of the calibration targets on the Mars rover according to its attitude to identify the anomalous data. The wavelength offsets were then determined by fitting the absorption positions of CO2 at ~1400 and ~2000 nm, representing the primary composition of the Martian atmosphere. The results showed 2–8 nm wavelength offsets, which correlated well with AOTF temperatures. The artifacts were removed in the wavelength-corrected reflectance spectra, which is critical to identify the material types on Mars, especially water-related minerals.
Keywords: Zhurong rover; near-infrared; AOTF; in-flight calibration; wavelength offset Zhurong rover; near-infrared; AOTF; in-flight calibration; wavelength offset

Share and Cite

MDPI and ACS Style

Wu, B.; Liu, C.; Xu, R.; Lin, H.; Xu, X.; Yan, W.; Tan, Y.; Liu, B.; Ren, X.; Xu, W.; et al. Initial In-Flight Spectral Calibration of the Near-Infrared Spectra Acquired by the MarSCoDe Onboard the Zhurong Rover. Remote Sens. 2022, 14, 2137. https://doi.org/10.3390/rs14092137

AMA Style

Wu B, Liu C, Xu R, Lin H, Xu X, Yan W, Tan Y, Liu B, Ren X, Xu W, et al. Initial In-Flight Spectral Calibration of the Near-Infrared Spectra Acquired by the MarSCoDe Onboard the Zhurong Rover. Remote Sensing. 2022; 14(9):2137. https://doi.org/10.3390/rs14092137

Chicago/Turabian Style

Wu, Bing, Chengyu Liu, Rui Xu, Honglei Lin, Xuesen Xu, Wei Yan, Yongjian Tan, Bin Liu, Xin Ren, Weiming Xu, and et al. 2022. "Initial In-Flight Spectral Calibration of the Near-Infrared Spectra Acquired by the MarSCoDe Onboard the Zhurong Rover" Remote Sensing 14, no. 9: 2137. https://doi.org/10.3390/rs14092137

APA Style

Wu, B., Liu, C., Xu, R., Lin, H., Xu, X., Yan, W., Tan, Y., Liu, B., Ren, X., Xu, W., Liu, X., Zhang, Z., Yang, B., He, Z., & Shu, R. (2022). Initial In-Flight Spectral Calibration of the Near-Infrared Spectra Acquired by the MarSCoDe Onboard the Zhurong Rover. Remote Sensing, 14(9), 2137. https://doi.org/10.3390/rs14092137

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