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地球磁鞘中的喷流与镜像模式波

Jets and Mirror Mode Waves in Earth's Magnetosheath.

作者信息

Blanco-Cano X, Rojas-Castillo D, Kajdič P, Preisser L

机构信息

Instituto de Geofísica Universidad Nacional Autónoma de México Circuito de la Investigación Científica s/n Ciudad Universitaria Mexico City Mexico.

Space Research Institute Austrian Academy of Sciences Graz Austria.

出版信息

J Geophys Res Space Phys. 2023 Jul;128(7):e2022JA031221. doi: 10.1029/2022JA031221. Epub 2023 Jul 22.

DOI:10.1029/2022JA031221
PMID:38439786
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC10909539/
Abstract

Magnetosheath jets are localized plasma structures with high dynamic pressure which are frequently observed downstream of the Earth's bow shock. In this work we analyze Magnetospheric MultiScale magnetic field and plasma data and show that jets can be found in the quasi-perpendicular magnetosheath in regions permeated by Mirror mode waves (MMWs). We show that structures identified as jets by their enhanced dynamic pressure can have very different internal structure, with variable signatures in magnetic field magnitude and components, velocity, and density and can be associated to ion distribution functions of various types. This suggests that jets observed in the quasi-perpendicular magnetosheath are generated by different mechanisms. We find that jets can be related to traveling foreshocks, flux transfer events, and some have MMWs inside them. Our results suggest that some jets have a local source and their formation does not depend on upstream structures. We find that different types of ion distributions can exist inside the jets, while in some cases anisotropic distributions are present, in others counterstreaming distributions exist. We also show that for jets with MMWs inside them, ion distributions can be modulated. This highlights the importance of using ion distributions to identify and classify different types of jets.

摘要

磁鞘喷流是具有高动压的局部等离子体结构,经常在地球弓形激波下游观测到。在这项工作中,我们分析了磁层多尺度磁场和等离子体数据,结果表明,在准垂直磁鞘中由镜像模波(MMWs)渗透的区域可以发现喷流。我们表明,通过其增强的动压识别为喷流的结构可能具有非常不同的内部结构,在磁场大小和分量、速度和密度方面具有可变特征,并且可以与各种类型的离子分布函数相关联。这表明在准垂直磁鞘中观测到的喷流是由不同机制产生的。我们发现喷流可能与行进的前震、通量传输事件有关,并且有些喷流内部存在MMWs。我们的结果表明,一些喷流有局部源,其形成不依赖于上游结构。我们发现喷流内部可以存在不同类型的离子分布,在某些情况下存在各向异性分布,在其他情况下存在反向流动分布。我们还表明,对于内部有MMWs的喷流,离子分布可以被调制。这突出了利用离子分布来识别和分类不同类型喷流的重要性。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b717/10909539/07ec1662c9dd/JGRA-128-e2022JA031221-g010.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b717/10909539/4db16ac14b5b/JGRA-128-e2022JA031221-g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b717/10909539/00f62250f60b/JGRA-128-e2022JA031221-g001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b717/10909539/e1bcdea53f5f/JGRA-128-e2022JA031221-g005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b717/10909539/e5faa214837b/JGRA-128-e2022JA031221-g011.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b717/10909539/5f4198b5e7bb/JGRA-128-e2022JA031221-g009.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b717/10909539/3f2e251705ba/JGRA-128-e2022JA031221-g006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b717/10909539/baf838b05d29/JGRA-128-e2022JA031221-g007.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b717/10909539/bb572d01792c/JGRA-128-e2022JA031221-g004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b717/10909539/63bcef4d27c4/JGRA-128-e2022JA031221-g003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b717/10909539/d5926a6b89a4/JGRA-128-e2022JA031221-g008.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b717/10909539/07ec1662c9dd/JGRA-128-e2022JA031221-g010.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b717/10909539/4db16ac14b5b/JGRA-128-e2022JA031221-g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b717/10909539/00f62250f60b/JGRA-128-e2022JA031221-g001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b717/10909539/e1bcdea53f5f/JGRA-128-e2022JA031221-g005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b717/10909539/e5faa214837b/JGRA-128-e2022JA031221-g011.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b717/10909539/5f4198b5e7bb/JGRA-128-e2022JA031221-g009.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b717/10909539/3f2e251705ba/JGRA-128-e2022JA031221-g006.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b717/10909539/baf838b05d29/JGRA-128-e2022JA031221-g007.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b717/10909539/bb572d01792c/JGRA-128-e2022JA031221-g004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b717/10909539/63bcef4d27c4/JGRA-128-e2022JA031221-g003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b717/10909539/d5926a6b89a4/JGRA-128-e2022JA031221-g008.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b717/10909539/07ec1662c9dd/JGRA-128-e2022JA031221-g010.jpg

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本文引用的文献

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Downstream high-speed plasma jet generation as a direct consequence of shock reformation.作为激波重整的直接结果而产生的下游高速等离子体射流。
Nat Commun. 2022 Feb 1;13(1):598. doi: 10.1038/s41467-022-28110-4.
2
The Location of Magnetic Reconnection at Earth's Magnetopause.地球磁层顶处磁重联的位置
Space Sci Rev. 2021;217(3):41. doi: 10.1007/s11214-021-00817-8. Epub 2021 Mar 29.
3
Characteristics of Minor Ions and Electrons in Flux Transfer Events Observed by the Magnetospheric Multiscale Mission.磁层多尺度任务观测到的通量传输事件中的小离子和电子特征
J Geophys Res Space Phys. 2020 Jul;125(7):e2020JA027778. doi: 10.1029/2020JA027778. Epub 2020 Jul 20.
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The Space Physics Environment Data Analysis System (SPEDAS).空间物理环境数据分析系统(SPEDAS)。
Space Sci Rev. 2019;215(1):9. doi: 10.1007/s11214-018-0576-4. Epub 2019 Jan 22.
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Direct observations of a surface eigenmode of the dayside magnetopause.对向阳面磁层顶表面本征模的直接观测。
Nat Commun. 2019 Feb 12;10(1):615. doi: 10.1038/s41467-018-08134-5.
6
Geoeffective jets impacting the magnetopause are very common.影响磁层顶的地球有效喷流非常常见。
J Geophys Res Space Phys. 2016 Apr;121(4):3240-3253. doi: 10.1002/2016JA022534. Epub 2016 Apr 23.
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On the generation of magnetosheath high-speed jets by bow shock ripples.关于由弓形激波涟漪产生磁鞘高速射流的研究
J Geophys Res Space Phys. 2013 Nov;118(11):7237-7245. doi: 10.1002/2013JA019172. Epub 2013 Nov 27.
8
Supermagnetosonic jets behind a collisionless quasiparallel shock.碰撞非平行准直激波后的超音磁激波喷流。
Phys Rev Lett. 2009 Dec 11;103(24):245001. doi: 10.1103/PhysRevLett.103.245001. Epub 2009 Dec 9.