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当前资源共 4条
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  • 1. ChinaXiv:202303.04467
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    In-flight Calibration of the Magnetometer on the Mars Orbiter of Tianwen-1

    分类: 天文学 >> 天文学 提交时间: 2023-02-19

    Zhuxuan Zou Yuming Wang Tielong Zhang Guoqiang Wang Sudong Xiao Zonghao Pan Zhoubin Zhang Wei Yan Yang Du Yutian Chi Long Cheng Zhiyong Wu Xinjun Hao Yiren Li Kai Liu Manming Chen Zhenpeng Su Chenglong Shen Mengjiao Xu Jingnan Guo

    摘要: Mars Orbiter Magnetometer (MOMAG) is one of seven science payloads onboard Tianwen-1's orbiter. Unlike most of the satellites, Tianwen-1's orbiter is not magnetically cleaned, and the boom where placed the magnetometer's sensors is not long enough. These pose many challenges to the magnetic field data processing. In this paper, we introduce the in-flight calibration process of the Tianwen-1/MOMAG. The magnetic interference from the spacecraft, including spacecraft generated dynamic field and slowly-changing offsets are cleaned in sequence. Then the calibrated magnetic field data are compared with the data from the Mars Atmosphere and Volatile EvolutioN (MAVEN). We find that some physical structures in the solar wind are consistent between the two data sets, and the distributions of the magnetic field strength in the solar wind are very similar. These results suggest that the in-flight calibration of the MOMAG is successful and the MOMAG provides reliable data for scientific research.

    同行评议状态:待评议

     点击量 29  下载量 15  评论 0
  • 2. ChinaXiv:202303.03922
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    In-flight Calibration of the Magnetometer on the Mars Orbiter of Tianwen-1

    分类: 天文学 >> 天文学 提交时间: 2023-02-19

    Zhuxuan Zou Yuming Wang Tielong Zhang Guoqiang Wang Sudong Xiao Zonghao Pan Zhoubin Zhang Wei Yan Yang Du Yutian Chi Long Cheng Zhiyong Wu Xinjun Hao Yiren Li Kai Liu Manming Chen Zhenpeng Su Chenglong Shen Mengjiao Xu Jingnan Guo

    摘要: Mars Orbiter Magnetometer (MOMAG) is one of seven science payloads onboard Tianwen-1's orbiter. Unlike most of the satellites, Tianwen-1's orbiter is not magnetically cleaned, and the boom where placed the magnetometer's sensors is not long enough. These pose many challenges to the magnetic field data processing. In this paper, we introduce the in-flight calibration process of the Tianwen-1/MOMAG. The magnetic interference from the spacecraft, including spacecraft generated dynamic field and slowly-changing offsets are cleaned in sequence. Then the calibrated magnetic field data are compared with the data from the Mars Atmosphere and Volatile EvolutioN (MAVEN). We find that some physical structures in the solar wind are consistent between the two data sets, and the distributions of the magnetic field strength in the solar wind are very similar. These results suggest that the in-flight calibration of the MOMAG is successful and the MOMAG provides reliable data for scientific research.

    同行评议状态:待评议

     点击量 26  下载量 13  评论 0
  • 3. ChinaXiv:202303.08155
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    The Mars Orbiter Magnetometer of Tianwen-1: In-flight Performance and First Science Results

    分类: 天文学 >> 天文学 提交时间: 2023-02-19

    Yuming Wang Tielong Zhang Guoqiang Wang Sudong Xiao Zhuxuan Zou Long Cheng Zonghao Pan Kai Liu Xinjun Hao Yiren Li Manming Chen Zhoubin Zhang Wei Yan Zhenpeng Su Zhiyong Wu Chenglong Shen Yutian Chi Mengjiao Xu Jingnan Guo Yang Du

    摘要: Mars Orbiter MAGnetometer (MOMAG) is a scientifc instrument onboard the orbiter of China's first mission for Mars -- Tianwen-1. It started to routinely measure the magnetic field from the solar wind to magnetic pile-up region surrounding Mars since November 13, 2021. Here we present its in-flight performance and first science results based on the first one and a half months' data. By comparing with the magnetic field data in the solar wind from the Mars Atmosphere and Volatile EvolutioN (MAVEN), the magnetic field by MOMAG is at the same level in magnitude, and the same magnetic structures with the similar variations in three components could be found in MOMAG data. In the first one and a half months, we recognize 158 clear bow shock (BS) crossings from MOMAG data, whose locations statistically match well with the modeled average BS. We also identify 5 pairs of simultaneous BS crossings of the Tianwen-1's orbiter and MAVEN. These BS crossings confirm the global shape of modeled BS as well as the south-north asymmetry of the Martian BS. Two presented cases in this paper suggest that the BS is probably more dynamic at flank than near the nose. So far, MOMAG performs well, and provides accurate magnetic field vectors. MOMAG is continuously scanning the magnetic field surrounding Mars. These measurements complemented by observations from MAVEN will undoubtedly advance our understanding of the plasma environment of Mars.

    同行评议状态:待评议

     点击量 23  下载量 14  评论 0
  • 4. ChinaXiv:202303.03212
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    The Mars Orbiter Magnetometer of Tianwen-1: In-flight Performance and First Science Results

    分类: 天文学 >> 天文学 提交时间: 2023-02-19

    Yuming Wang Tielong Zhang Guoqiang Wang Sudong Xiao Zhuxuan Zou Long Cheng Zonghao Pan Kai Liu Xinjun Hao Yiren Li Manming Chen Zhoubin Zhang Wei Yan Zhenpeng Su Zhiyong Wu Chenglong Shen Yutian Chi Mengjiao Xu Jingnan Guo Yang Du

    摘要: Mars Orbiter MAGnetometer (MOMAG) is a scientifc instrument onboard the orbiter of China's first mission for Mars -- Tianwen-1. It started to routinely measure the magnetic field from the solar wind to magnetic pile-up region surrounding Mars since November 13, 2021. Here we present its in-flight performance and first science results based on the first one and a half months' data. By comparing with the magnetic field data in the solar wind from the Mars Atmosphere and Volatile EvolutioN (MAVEN), the magnetic field by MOMAG is at the same level in magnitude, and the same magnetic structures with the similar variations in three components could be found in MOMAG data. In the first one and a half months, we recognize 158 clear bow shock (BS) crossings from MOMAG data, whose locations statistically match well with the modeled average BS. We also identify 5 pairs of simultaneous BS crossings of the Tianwen-1's orbiter and MAVEN. These BS crossings confirm the global shape of modeled BS as well as the south-north asymmetry of the Martian BS. Two presented cases in this paper suggest that the BS is probably more dynamic at flank than near the nose. So far, MOMAG performs well, and provides accurate magnetic field vectors. MOMAG is continuously scanning the magnetic field surrounding Mars. These measurements complemented by observations from MAVEN will undoubtedly advance our understanding of the plasma environment of Mars.

    同行评议状态:待评议

     点击量 27  下载量 12  评论 0
友情链接 : ChinaXiv PubScholar 哲学社会科学预印本
  • 运营单位: 中国科学院文献情报中心
  • 制作维护:中国科学院文献情报中心知识系统部
  • 邮箱: eprint@mail.las.ac.cn
  • 地址:北京中关村北四环西路33号
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