Research on the Detection Method of Martian Atmospheric Temperature and Pressure Profile Based on Laser Occultation Technology

As an important target of space exploration, Mars has attracted a lot of attention due to its unique geographical and atmospheric conditions. The detection of the vertical profiles of Mars atmospheric parameters provides deeper insights into the structure and composition of the Martian atmosphere. M...

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Main Authors: Ye Liu, Wei Kong, Xue Shen, Tao Chen, Genghua Huang
Format: Article
Language:English
Published: MDPI AG 2024-12-01
Series:Remote Sensing
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Online Access:https://www.mdpi.com/2072-4292/17/1/87
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author Ye Liu
Wei Kong
Xue Shen
Tao Chen
Genghua Huang
author_facet Ye Liu
Wei Kong
Xue Shen
Tao Chen
Genghua Huang
author_sort Ye Liu
collection DOAJ
description As an important target of space exploration, Mars has attracted a lot of attention due to its unique geographical and atmospheric conditions. The detection of the vertical profiles of Mars atmospheric parameters provides deeper insights into the structure and composition of the Martian atmosphere. Meanwhile, it holds significant importance for the design and execution of Mars exploration missions. This paper presents a detection method for the Martian atmosphere utilizing laser occultation technology based on a network of high-orbit and low-orbit satellites around Mars. The measurement principle of Mars laser occultation is first introduced, which is that the atmospheric temperature and pressure are measured by analyzing the absorption spectrum characteristics of infrared carbon dioxide. Then, a detailed simulation process is described, including the establishment and validation of both the radiation intensity calculation model for laser occultation signals and the method for retrieving atmospheric parameters. A set of satellite payload parameters is also designed. The simulation results reveal that this method can accurately measure temperature and pressure at a vertical resolution of 100 m from 5 km to 50 km altitude of the Martian atmosphere with deviations of 0.43 K and 1.06%, respectively. It is indicated that the proposed laser occultation method can achieve effective detection of temperature and pressure and provide a promising approach for high vertical resolution profile detection of the Martian atmosphere in the future.
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spelling doaj-art-d07b318b78784722ac75382a8574720a2025-01-10T13:20:11ZengMDPI AGRemote Sensing2072-42922024-12-011718710.3390/rs17010087Research on the Detection Method of Martian Atmospheric Temperature and Pressure Profile Based on Laser Occultation TechnologyYe Liu0Wei Kong1Xue Shen2Tao Chen3Genghua Huang4Key Laboratory of Space Active Opto-Electronics Technology, Shanghai Institute of Technical Physics, Chinese Academy of Sciences, Shanghai 200083, ChinaKey Laboratory of Space Active Opto-Electronics Technology, Shanghai Institute of Technical Physics, Chinese Academy of Sciences, Shanghai 200083, ChinaKey Laboratory of Space Active Opto-Electronics Technology, Shanghai Institute of Technical Physics, Chinese Academy of Sciences, Shanghai 200083, ChinaKey Laboratory of Space Active Opto-Electronics Technology, Shanghai Institute of Technical Physics, Chinese Academy of Sciences, Shanghai 200083, ChinaKey Laboratory of Space Active Opto-Electronics Technology, Shanghai Institute of Technical Physics, Chinese Academy of Sciences, Shanghai 200083, ChinaAs an important target of space exploration, Mars has attracted a lot of attention due to its unique geographical and atmospheric conditions. The detection of the vertical profiles of Mars atmospheric parameters provides deeper insights into the structure and composition of the Martian atmosphere. Meanwhile, it holds significant importance for the design and execution of Mars exploration missions. This paper presents a detection method for the Martian atmosphere utilizing laser occultation technology based on a network of high-orbit and low-orbit satellites around Mars. The measurement principle of Mars laser occultation is first introduced, which is that the atmospheric temperature and pressure are measured by analyzing the absorption spectrum characteristics of infrared carbon dioxide. Then, a detailed simulation process is described, including the establishment and validation of both the radiation intensity calculation model for laser occultation signals and the method for retrieving atmospheric parameters. A set of satellite payload parameters is also designed. The simulation results reveal that this method can accurately measure temperature and pressure at a vertical resolution of 100 m from 5 km to 50 km altitude of the Martian atmosphere with deviations of 0.43 K and 1.06%, respectively. It is indicated that the proposed laser occultation method can achieve effective detection of temperature and pressure and provide a promising approach for high vertical resolution profile detection of the Martian atmosphere in the future.https://www.mdpi.com/2072-4292/17/1/87laser occultationMartian atmospheretemperature and pressure profilescarbon dioxide
spellingShingle Ye Liu
Wei Kong
Xue Shen
Tao Chen
Genghua Huang
Research on the Detection Method of Martian Atmospheric Temperature and Pressure Profile Based on Laser Occultation Technology
Remote Sensing
laser occultation
Martian atmosphere
temperature and pressure profiles
carbon dioxide
title Research on the Detection Method of Martian Atmospheric Temperature and Pressure Profile Based on Laser Occultation Technology
title_full Research on the Detection Method of Martian Atmospheric Temperature and Pressure Profile Based on Laser Occultation Technology
title_fullStr Research on the Detection Method of Martian Atmospheric Temperature and Pressure Profile Based on Laser Occultation Technology
title_full_unstemmed Research on the Detection Method of Martian Atmospheric Temperature and Pressure Profile Based on Laser Occultation Technology
title_short Research on the Detection Method of Martian Atmospheric Temperature and Pressure Profile Based on Laser Occultation Technology
title_sort research on the detection method of martian atmospheric temperature and pressure profile based on laser occultation technology
topic laser occultation
Martian atmosphere
temperature and pressure profiles
carbon dioxide
url https://www.mdpi.com/2072-4292/17/1/87
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