Calibration of the Zero Offset of the Fluxgate Magnetometer on Board the Tianwen‐1 Orbiter in the Martian Magnetosheath

Author:

Wang Guoqiang12ORCID,Xiao Sudong12,Wu Mingyu12,Zhao Yangdong3,Jiang Song3,Pan Zonghao45ORCID,Hao Xinjun45ORCID,Li Yiren45ORCID,Liu Kai45,Chi Yutian6ORCID,Zou Zhuxuan45,Chen Manming45,Su Zhenpeng45ORCID,Shen Chenglong45ORCID,Guo Jingnan45,Cheng Long45,Wu Zhiyong45,Xu Mengjiao6,Wang Yuming45ORCID,Zhang Tielong1257ORCID

Affiliation:

1. Institute of Space Science and Applied Technology Harbin Institute of Technology Shenzhen China

2. Shenzhen Key Laboratory of Numerical Prediction for Space Storm Harbin Institute of Technology Shenzhen China

3. Aerospace System Engineering Shanghai China

4. Deep Space Exploration Laboratory/School of Earth and Space Sciences University of Science and Technology of China Hefei China

5. CAS Center for Excellence in Comparative Planetology/CAS Key Laboratory of Geospace Environment/Mengcheng National Geophysical Observatory University of Science and Technology of China Hefei China

6. Institute of Deep Space Sciences Deep Space Exploration Laboratory Hefei China

7. Space Research Institute Austrian Academy of Sciences Graz Austria

Abstract

AbstractHigh‐precision measurements of the magnetic field are critical to explore the near‐Mars environment. The Mars Orbiter MAGnetometer (MOMAG) is one of seven payloads on board the Tianwen‐1 orbiter. Its zero offset needs regular calibration, and the Wang‐Pan method I is applied to the MOMAG when the Tianwen‐1 orbiter is in the solar wind. The orbiter will remain out of the solar wind over tens of days each year, a method is necessary to ensure the accuracy of the zero offset during this period. Recently, a new method was proposed by Wang (2022b), https://doi.org/10.3847/1538-4357/ac822c, which is referred to as the Wang method II for ease of description. Here, we test the performance of this method using the MOMAG data measured in the Martian magnetosheath. We find that the zero offset Ow determined by the Wang method II varies around the zero offset Owp calculated by the Wang‐Pan method I using the potential Alfvénic fluctuations in the solar wind. After smoothing with a temporal window of 27 days, Ow is able to achieve an accuracy close to Owp. If the data segment has no gaps and its duration is < 27 days, the smoothed Ow might have an error >2 nT, but the error tends to be smaller if the segment's duration is longer. Our tests suggest that the Wang method II is suitable for the in‐flight calibration of the MOMAG when the Tianwen‐1 orbiter remains out of the solar wind.

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

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