Determination of Current Density in Magnetospheric Plasma: Multispacecraft and Particle Approaches

IF 0.4 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS
B. A. Petrenko, L. V. Kozak, N. O. Khalimonenko
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引用次数: 0

Abstract

A comparative analysis of two methods for determining electric current density in the near-Earth magnetospheric plasma is presented: the multispacecraft curlometer technique and the particle-based (kinetic) approach relying on plasma moments. The study is based on data from the Magnetospheric Multiscale Mission (MMS) for six magnetic reconnection events in Earth’s magnetotail observed between 2019 and 2024. It is shown that the results of both methods agree well under conditions of stable spacecraft configuration and the absence of radiation contamination in the measurements. The particle-based approach systematically yields overestimated current densities, likely due to locally enhanced ion density near the spacecraft. Spectral analysis reveals that particle-derived data exhibit increased noise levels at frequencies above 1 Hz. The obtained results are important for refining our understanding of energy-dissipation mechanisms and the dynamics of magnetic reconnection processes.

Abstract Image

磁层等离子体中电流密度的测定:多航天器和粒子方法
对近地磁层等离子体电流密度测定的两种方法进行了比较分析:多航天器曲率计技术和基于等离子体矩的粒子(动力学)方法。该研究基于磁层多尺度任务(MMS)对2019年至2024年间地球磁尾中6次磁重联事件的观测数据。结果表明,在航天器结构稳定和测量中没有辐射污染的条件下,两种方法的结果吻合良好。基于粒子的方法系统地产生了高估的电流密度,可能是由于航天器附近局部离子密度的增强。频谱分析显示,粒子衍生的数据在频率高于1hz时显示出增加的噪声水平。所得结果对于完善我们对能量耗散机制和磁重联过程动力学的理解具有重要意义。
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来源期刊
Kinematics and Physics of Celestial Bodies
Kinematics and Physics of Celestial Bodies ASTRONOMY & ASTROPHYSICS-
CiteScore
0.90
自引率
40.00%
发文量
24
审稿时长
>12 weeks
期刊介绍: Kinematics and Physics of Celestial Bodies is an international peer reviewed journal that publishes original regular and review papers on positional and theoretical astronomy, Earth’s rotation and geodynamics, dynamics and physics of bodies of the Solar System, solar physics, physics of stars and interstellar medium, structure and dynamics of the Galaxy, extragalactic astronomy, atmospheric optics and astronomical climate, instruments and devices, and mathematical processing of astronomical information. The journal welcomes manuscripts from all countries in the English or Russian language.
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