S. T. Yao, H. Zhang, Q. Q. Shi, J. Liu, R. L. Guo, W. J. Sun, Daniel J. Gershman, M. Hamrin, A. W. Degeling, R. A. Treumann, T. Pitkänen, A. M. Tian
{"title":"Electron Vortex Generation in Earth's Collisionless Bow Shock: MMS Observations","authors":"S. T. Yao, H. Zhang, Q. Q. Shi, J. Liu, R. L. Guo, W. J. Sun, Daniel J. Gershman, M. Hamrin, A. W. Degeling, R. A. Treumann, T. Pitkänen, A. M. Tian","doi":"10.1029/2024JA032980","DOIUrl":null,"url":null,"abstract":"<p>In astrophysics and space, supercritical shock is generated when an object interacts with an incoming supersonic plasma stream. Its downstream plasmas are highly turbulent, containing abundant vortices on all scales from magnetohydrodynamic to electron gyroscales. Understanding the production of these vortices is at the forefront, especially on the electron scale. Using ultrafast measurements of NASA's Magnetospheric Multiscale spacecraft, we report on the fortunate multi-spacecraft observation of the formation of an electron vortex directly generated inside the Earth's quasi-parallel bow shock transition and propagated to the downstream turbulent magnetosheath. The vortex is generated inside the shock transition by anisotropic ∼100–600 eV electrons trapped in an ion-scale magnetic hole which could show a tornado-like magnetic morphology. Our results demonstrate that the electron vortex can develop not only as a product of the forward cascade but also from the shock transition into its downstream turbulence, which adds to the short-scale turbulence and dissipation.</p>","PeriodicalId":15894,"journal":{"name":"Journal of Geophysical Research: Space Physics","volume":null,"pages":null},"PeriodicalIF":2.6000,"publicationDate":"2024-09-20","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Geophysical Research: Space Physics","FirstCategoryId":"89","ListUrlMain":"https://onlinelibrary.wiley.com/doi/10.1029/2024JA032980","RegionNum":2,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
In astrophysics and space, supercritical shock is generated when an object interacts with an incoming supersonic plasma stream. Its downstream plasmas are highly turbulent, containing abundant vortices on all scales from magnetohydrodynamic to electron gyroscales. Understanding the production of these vortices is at the forefront, especially on the electron scale. Using ultrafast measurements of NASA's Magnetospheric Multiscale spacecraft, we report on the fortunate multi-spacecraft observation of the formation of an electron vortex directly generated inside the Earth's quasi-parallel bow shock transition and propagated to the downstream turbulent magnetosheath. The vortex is generated inside the shock transition by anisotropic ∼100–600 eV electrons trapped in an ion-scale magnetic hole which could show a tornado-like magnetic morphology. Our results demonstrate that the electron vortex can develop not only as a product of the forward cascade but also from the shock transition into its downstream turbulence, which adds to the short-scale turbulence and dissipation.
在天体物理学和太空中,当物体与进入的超音速等离子体流相互作用时会产生超临界冲击。其下游等离子体是高度湍流的,包含从磁流体力学到电子陀螺仪等各种尺度的大量涡旋。了解这些旋涡的产生是当务之急,尤其是在电子尺度上。利用美国宇航局磁层多尺度航天器的超快测量,我们报告了多航天器观测到的幸运现象,即在地球准平行弓形冲击转变内部直接产生电子涡旋,并传播到下游湍流磁鞘。漩涡是由各向异性的 ∼100-600 eV 电子在冲击转换内部产生的,这些电子被困在一个离子尺度的磁洞中,该磁洞可能呈现出类似龙卷风的磁形态。我们的研究结果表明,电子漩涡不仅可以作为前向级联的产物,还可以从冲击转变发展到其下游湍流,从而增加短尺度湍流和耗散。