Reconnection Inside a Dipolarization Front of a Diverging Earthward Fast Flow

被引：5

作者：

Hosner, M. ^{[1
,2
]}

Nakamura, R. ^{[1
]}

Schmid, D. ^{[1
]}

Nakamura, T. K. M. ^{[1
,3
]}

Panov, E. V. ^{[1
]}

Volwerk, M. ^{[1
]}

Voros, Z. ^{[1
,4
]}

Roberts, O. W. ^{[1
]}

Blasl, K. A. ^{[1
,2
]}

Settino, A. ^{[1
]}

Korovinskiy, D. ^{[1
]}

Marshall, A. T. ^{[5
]}

Denton, R. E. ^{[6
]}

Burch, J. L. ^{[7
]}

Giles, B. L. ^{[8
]}

Torbert, R. B. ^{[7
,9
]}

Le Contel, O. ^{[10
]}

Escoubet, C. P. ^{[11
]}

Dandouras, I. S. ^{[12
]}

Carr, C. ^{[13
]}

Fazakerley, A. N. ^{[14
]}

机构：

[1] Austrian Acad Sci, Space Res Inst, Graz, Austria

[2] Karl Franzens Univ Graz, Inst Phys, Graz, Austria

[3] Krimgen Llc, Hiroshima, Japan

[4] Inst Earth Phys & Space Sci, Sopron, Hungary

[5] Rice Univ, Dept Phys & Astron, Houston, TX USA

[6] Dartmouth Coll, Dept Phys & Astron, Hanover, NH USA

[7] Southwest Res Inst, San Antonio, TX USA

[8] NASA, Goddard Space Flight Ctr, Greenbelt, MD USA

[9] Univ New Hampshire, Space Sci Ctr, Durham, NH USA

[10] Univ Paris Saclay, Sorbonne Univ, Ecole Polytech, Inst Polytech Paris,CNRS,Observ Paris,LPP, Paris, France

[11] Estec, ESA, Noordwijk, Netherlands

[12] Univ Toulouse, CNRS, UPS, CNES,IRAP, Toulouse, France

[13] Imperial Coll London, London, England

[14] Mullard Space Sci Lab, Dorking, England

来源：

JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS | 2024年 / 129卷 / 01期

基金：

奥地利科学基金会;

关键词：

polynomial reconstruction; MMS; cluster; dipolarization front; magnetic reconnection; NONORTHOGONAL X-LINE; MAGNETIC RECONNECTION; ELECTRIC-FIELD; MAGNETOPAUSE; FLUX;

D O I：

10.1029/2023JA031976

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We examine a Dipolarization Front (DF) event with an embedded electron diffusion region (EDR), observed by the Magnetospheric Multiscale (MMS) spacecraft on 08 September 2018 at 14:51:30 UT in the Earth's magnetotail by applying multi-scale multipoint analysis methods. In order to study the large-scale context of this DF, we use conjunction observations of the Cluster spacecraft together with MMS. A polynomial magnetic field reconstruction technique is applied to MMS data to characterize the embedded electron current sheet including its velocity and the X-line exhaust opening angle. Our results show that the MMS and Cluster spacecraft were located in two counter-rotating vortex flows, and such flows may distort a flux tube in a way that the local magnetic shear angle is increased and localized magnetic reconnection may be triggered. Using multi-point data from MMS we further show that the local normalized reconnection rate is in the range of R similar to 0.16 to 0.18. We find a highly asymmetric electron in- and outflow structure, consistent with previous simulations on strong guide-field reconnection events. This study shows that magnetic reconnection may not only take place at large-scale stable magnetopause or magnetotail current sheets but also in transient localized current sheets, produced as a consequence of the interaction between the fast Earthward flows and the Earth's dipole field. Magnetic Reconnection is a key energy conversion process, where magnetic energy is converted into kinetic energy of plasma particles. During this process the magnetic field topology changes and the plasma particles decouple from the magnetic field in the so-called diffusion region and get accelerated, forming a fast outflow jet. Over the last decades, hints arise that reconnection can take place at many different places in the magnetosphere and also very locally and intermittently. Fast plasma flows in the Magnetotail, moving toward the Earth, are assumed to be a consequence of magnetic reconnection, and are often accompanied by dipolar-shaped magnetic flux bundles, embedded into them. The leading edges of such flux bundles are called dipolarization fronts (DF). In this work, we investigate a DF event, which hosts a diffusion region. First, we study the large-scale characteristics of the DF, by utilizing data from both the Magnetospheric Multiscale (MMS) and the Cluster mission, that observe different regions of the event almost simultaneously. Second, we performed a 3D magnetic field reconstruction technique and compared the results to MMS data, to investigate the event on small scales. A thin current sheet inside a dipolarization front, embedded in a diverging flow is analyzed using a polynomial reconstruction techniqueTransient reconnection event is detected in a high magnetic shear region, where the magnetic field is deflected due to duskward fast plasma flowThe reconstructed current sheet has a guide field of similar to 1.8 the reconnecting component with normalized reconnection rate between 0.16 and 0.18

引用

页数：20