Mutual impedance experiments in a magnetized plasma

IF 5.8 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Astronomy & Astrophysics Pub Date : 2025-04-01 DOI:10.1051/0004-6361/202450312
P. Dazzi, P. Henri, L. Bucciantini, F. Lavorenti, F. Califano, G. Wattieaux, O. Randriamboarison, K. Issautier
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Abstract

Context. A mutual impedance experiment is an active in situ space plasma diagnostic that is used to determine the electron density and temperature. Such parameters are inferred from the mutual impedance spectrum measured between a pair of electric antennas embedded in the plasma. This state-of-the-art plasma diagnostic technique is limited to unmagnetized plasmas; that is, ones with a plasma frequency much larger than the electron cyclotron frequency. This limit is not expected to be valid in the plasma environment surrounding magnetized planets such as Mercury and Jupiter that will be explored by the ESA JUICE and joint ESA/JAXA Bepi-Colombo missions.Aims. The goal of this work is to extend the mutual impedance diagnostic technique to magnetized plasmas, focusing on measurements of the electron density and temperature, and to extend it to the electron temperature anisotropy.Methods. To achieve this, we developed the first quantitative three-dimensional instrumental model for mutual impedance experiments in a magnetized plasma. This model is valid for arbitrary values of the electron temperature and magnetic field. Our model is based on the linearized Vlasov-Maxwell coupled system of equations. We numerically computed the electric potential generated and simultaneously measured by the mutual impedance experiment, in order to compute the mutual impedance spectrum in a magnetized plasma.Results. First, we identify in the numerical mutual impedance spectra a number of local spectral signatures, associated with characteristic frequencies that can be used for plasma diagnostics. We show how the magnetic field strength and direction modify such spectral signatures. Second, we show that electron-neutral collision smooth out the spectrum, as long as the scattering-to-plasma frequency ratio is greater than 10−3 . Below such a value, mutual impedance experiments are insensitive to electron-neutral scattering and the plasma can be considered collisionless. Third, we show that the electron temperature directly controls the amplitude of the mutual impedance spectra, so that such behavior can be used as an electron temperature diagnostic. Fourth, we explore for the first time the possibility of diagnosing electron temperature anisotropies with mutual impedance experiments. We show how an electron temperature anisotropy significantly modifies the mutual impedance spectral signatures, as a result of the modified propagation of the electron Bernstein waves generated by the experiment.Conclusions. The results of our model, in terms of plasma diagnostics, are discussed in terms of the propagation properties in a magnetized plasma of the electrostatic waves generated by the active mutual impedance experiment. The results of our model will significantly extend the plasma diagnostic capabilities of the current and future mutual impedance experiment such as the PWI/AM2P experiment on board BepiColombo and the RPWI/MIME experiment on board JUICE.
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磁化等离子体的相互阻抗实验
上下文。互阻抗实验是一种主动的原位空间等离子体诊断方法,用于确定电子密度和温度。这些参数是从嵌入在等离子体中的一对电天线之间测量的相互阻抗谱推断出来的。这种最先进的等离子体诊断技术仅限于未磁化的等离子体;也就是说,等离子体频率比电子回旋频率大得多的等离子体。这一限制预计在磁化行星(如水星和木星)周围的等离子体环境中无效,这些行星将由ESA JUICE和ESA/JAXA Bepi-Colombo联合任务探索。本工作的目的是将互阻抗诊断技术扩展到磁化等离子体,重点是电子密度和温度的测量,并将其扩展到电子温度的各向异性。为了实现这一目标,我们开发了第一个用于磁化等离子体相互阻抗实验的定量三维仪器模型。该模型适用于电子温度和磁场的任意值。我们的模型是基于线性化的Vlasov-Maxwell耦合方程组。为了计算磁化等离子体的互阻抗谱,对互阻抗实验产生的电势和同时测量的电势进行了数值计算。首先,我们在数值互阻抗谱中识别出一些与可用于等离子体诊断的特征频率相关的局部谱特征。我们展示了磁场强度和方向如何改变这种光谱特征。其次,我们发现,只要散射与等离子体的频率比大于10−3,电子中性碰撞就会使光谱平滑。在此值以下,相互阻抗实验对电子中性散射不敏感,等离子体可以认为是无碰撞的。第三,我们证明了电子温度直接控制互阻抗谱的振幅,因此这种行为可以用作电子温度诊断。第四,我们首次探索了用互阻抗实验诊断电子温度各向异性的可能性。我们展示了电子温度各向异性如何显著地改变相互阻抗谱特征,这是实验产生的电子伯恩斯坦波的修正传播的结果。从等离子体诊断的角度,讨论了由有源互阻抗实验产生的静电波在磁化等离子体中的传播特性。该模型的结果将大大扩展当前和未来互阻抗实验的等离子体诊断能力,如BepiColombo上的PWI/AM2P实验和JUICE上的RPWI/MIME实验。
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来源期刊
Astronomy & Astrophysics
Astronomy & Astrophysics 地学天文-天文与天体物理
CiteScore
10.20
自引率
27.70%
发文量
2105
审稿时长
1-2 weeks
期刊介绍: Astronomy & Astrophysics is an international Journal that publishes papers on all aspects of astronomy and astrophysics (theoretical, observational, and instrumental) independently of the techniques used to obtain the results.
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