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火星弓激波上游离子回旋波的观测研究

李家威 杨磊 吴德金 戴存礼 李建平 向梁 罗庆宇 程征伟

天文学进展2024,Vol.42Issue(2):286-298,13.
天文学进展2024,Vol.42Issue(2):286-298,13.DOI:10.3969/j.issn.1000-8349.2024.02.07

火星弓激波上游离子回旋波的观测研究

Observations of Ion Cyclotron Waves Upstream from the Martian Bow Shock

李家威 1杨磊 1吴德金 2戴存礼 3李建平 4向梁 5罗庆宇 6程征伟7

作者信息

  • 1. 中国科学院紫金山天文台行星科学重点实验室,南京 210023||中国科学技术大学天文与空间科学学院,合肥 230026||中国科学院 国家空间科学中心空间天气学国家重点实验室,北京 100190
  • 2. 中国科学院紫金山天文台行星科学重点实验室,南京 210023||中国科学技术大学天文与空间科学学院,合肥 230026
  • 3. 南京农业大学理学院,南京 210095
  • 4. 中国科学院紫金山天文台暗物质与空间天文重点实验室,南京 210023
  • 5. 洛阳师范学院空间物理研究所,洛阳 471934||洛阳师范学院 电磁变换与探测重点实验室,洛阳 471934
  • 6. 中国科学院紫金山天文台行星科学重点实验室,南京 210023
  • 7. 中国科学院 国家空间科学中心空间天气学国家重点实验室,北京 100190
  • 折叠

摘要

Abstract

Ion cyclotron waves are widely present upstream from the Martian bow shock,with frequencies near the local proton cyclotron frequency in the spacecraft frame.The waves propagate quasi-parallel to the background magnetic field,and are associated with the Solar wind picking up newly-ionized hydrogen from the Martian exosphere.In this work,a typical ion cyclotron wave event was observed by MAVEN upstream from the Martian bow shock.The further MAV analysis results for this event show that the magnetic field perturbations are left-handed polarized and propagate quasi-parallel(the propagation angle θ=12.37°)to the background magnetic field.The relationship between the plasma perturbations and magnetic field perturbations is theoretically derived for slow magnetosonic,Alfvén,and fast magnetosonic waves based on the magnetohydrodynamic theory.If we take the wave propagation angle θ=12.37° estimated from the MVA analysis,the theoretically expected density perturbation and velocity perturbation along the background magnetic field are in serious disagreement with the MAVEN data.Through fitting the plasma density fluctuation,velocity fluctuation and magnetic field fluctuation,it is found that the ion cyclotron wave event can be explained by the superposition of oblique fast magnetosonic waves with a propagation angle of 63° relative to the background magnetic field and parallel propagating Alfvén waves.The results are helpful to further understand the physical nature of the observed ion cyclotron wave-related perturbations upstream from the Martian bow shock and have guiding implications for the re-modeling and numerical simulation of the plasma physical processes therein.

关键词

离子回旋波/火星上游/磁流体力学/快磁声波/阿尔文波/慢磁声波

Key words

ion cyclotron wave/upstream from Mars/magnetohydrodynamics(MHD)/fast magnetosonic wave/Alfvén wave/slow magnetosonic wave

分类

天文与地球科学

引用本文复制引用

李家威,杨磊,吴德金,戴存礼,李建平,向梁,罗庆宇,程征伟..火星弓激波上游离子回旋波的观测研究[J].天文学进展,2024,42(2):286-298,13.

基金项目

国家自然科学基金(41874201,12250014,11790302,42174195,11873018) (41874201,12250014,11790302,42174195,11873018)

国家重点实验室专项基金 ()

天文学进展

OA北大核心CSTPCD

1000-8349

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