Boundary layer plasma flows from high‐latitude reconnection in the summer hemisphere for northward IMF: THEMIS multi‐point observations
Identifieur interne : 007F17 ( Main/Exploration ); précédent : 007F16; suivant : 007F18Boundary layer plasma flows from high‐latitude reconnection in the summer hemisphere for northward IMF: THEMIS multi‐point observations
Auteurs : H. Hasegawa [Japon] ; J. P. Mcfadden [États-Unis] ; O. D. Constantinescu [Allemagne] ; Y. V. Bogdanova [Australie] ; J. Wang [République populaire de Chine] ; M. W. Dunlop [Royaume-Uni] ; V. Angelopoulos [États-Unis] ; H. U. Frey [États-Unis] ; T. Takada [Japon] ; B. Lavraud [France] ; Q. Zhang [Royaume-Uni] ; Z. Y. Pu [République populaire de Chine] ; A. N. Fazakerley [Royaume-Uni] ; E. V. Panov [Autriche] ; M. Volwerk [Autriche] ; C. Shen [République populaire de Chine] ; J. K. Shi [République populaire de Chine]Source :
- Geophysical Research Letters [ 0094-8276 ] ; 2009-08-16.
Descripteurs français
- Wicri :
- topic : Simulation.
English descriptors
- KwdEn :
- Cdpl, Clock angle, Dayside, Dayside llbl, Dayside magnetopause, Dipole tilt, Field lines, Geophys, Global simulation, Hasegawa, Ieroset, Inner llbl, Lavraud, Llbl, Magnetopause, Magnetosheath, Magnetosheath electrons, Magnetosheath ions, Northern cusp, Northern reconnection, Outer llbl, Phan, Plasma transport, Reconnection, Simulation, Solar wind, Space sciences, Summer hemisphere, Themis, Themis observations, Themis spacecraft.
- Teeft :
- Cdpl, Clock angle, Dayside, Dayside llbl, Dayside magnetopause, Dipole tilt, Field lines, Geophys, Global simulation, Hasegawa, Ieroset, Inner llbl, Lavraud, Llbl, Magnetopause, Magnetosheath, Magnetosheath electrons, Magnetosheath ions, Northern cusp, Northern reconnection, Outer llbl, Phan, Plasma transport, Reconnection, Simulation, Solar wind, Space sciences, Summer hemisphere, Themis, Themis observations, Themis spacecraft.
Abstract
On 2008‐07‐11, the THEMIS spacecraft, separated both longitudinally and radially, traversed the dayside low‐latitude boundary layer (LLBL) under extended northward IMF. They detected southward flows of magnetosheath plasma from magnetopause reconnection poleward of the northern cusp, which were cold‐dense, and had southward velocity ∼100 km/s and longitudinal extent >3 RE. These features all agree with a global MHD simulation of the magnetosphere for similar conditions, in which under large geomagnetic dipole tilt, an LLBL forms via poleward‐of‐the‐cusp reconnection first in the summer hemisphere and later in the other. Contrary to the simulation, however, the observed LLBL was mostly magnetically closed, characterized by balanced field‐aligned and anti‐field‐aligned electron fluxes, and was less thick (≤0.5 RE). The former suggests comparable reconnection rate in both hemispheres, while the latter suggests the actual reconnection rate being lower, and/or the plasma transport toward the magnetotail being faster, than in the simulation.
Url:
DOI: 10.1029/2009GL039410
Affiliations:
- Allemagne, Australie, Autriche, France, Japon, Royaume-Uni, République populaire de Chine, États-Unis
- Angleterre, Californie, Grand Londres, Midi-Pyrénées, Occitanie (région administrative)
- Berkeley (Californie), Londres, Los Angeles, Pékin, Toulouse
- University College de Londres, Université de Pékin
Links toward previous steps (curation, corpus...)
- to stream Istex, to step Corpus: 000A14
- to stream Istex, to step Curation: 000A14
- to stream Istex, to step Checkpoint: 000F54
- to stream Main, to step Merge: 008612
- to stream Main, to step Curation: 007F17
Le document en format XML
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<term>Dayside magnetopause</term>
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<term>Global simulation</term>
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<term>Magnetosheath</term>
<term>Magnetosheath electrons</term>
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<term>Northern cusp</term>
<term>Northern reconnection</term>
<term>Outer llbl</term>
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<front><div type="abstract">On 2008‐07‐11, the THEMIS spacecraft, separated both longitudinally and radially, traversed the dayside low‐latitude boundary layer (LLBL) under extended northward IMF. They detected southward flows of magnetosheath plasma from magnetopause reconnection poleward of the northern cusp, which were cold‐dense, and had southward velocity ∼100 km/s and longitudinal extent >3 RE. These features all agree with a global MHD simulation of the magnetosphere for similar conditions, in which under large geomagnetic dipole tilt, an LLBL forms via poleward‐of‐the‐cusp reconnection first in the summer hemisphere and later in the other. Contrary to the simulation, however, the observed LLBL was mostly magnetically closed, characterized by balanced field‐aligned and anti‐field‐aligned electron fluxes, and was less thick (≤0.5 RE). The former suggests comparable reconnection rate in both hemispheres, while the latter suggests the actual reconnection rate being lower, and/or the plasma transport toward the magnetotail being faster, than in the simulation.</div>
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<name sortKey="Volwerk, M" sort="Volwerk, M" uniqKey="Volwerk M" first="M." last="Volwerk">M. Volwerk</name>
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