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Kinetic evidence of magnetic reconnection due to Kelvin-Helmholtz waves
Journal article   Peer reviewed

Kinetic evidence of magnetic reconnection due to Kelvin-Helmholtz waves

W Li, M Andre, YuV Khotyaintsev, A Vaivads, D Graham, S Toledo-Redondo, C Norgren, P Henri, C Wang, B Tang, …
Geophysical research letters, Vol.43(11), pp.5635-5643
06/16/2016
DOI: 10.1002/2016GL069192

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Abstract

The Kelvin-Helmholtz (KH) instability at the Earth's magnetopause is predominantly excited during northward interplanetary magnetic field (IMF). Magnetic reconnection due to KH waves has been suggested as one of the mechanisms to transfer solar wind plasma into the magnetosphere. We investigate KH waves observed at the magnetopause by the Magnetospheric Multiscale (MMS) mission; in particular, we study the trailing edges of KH waves with Alfvenic ion jets. We observe gradual mixing of magnetospheric and magnetosheath ions at the boundary layer. The magnetospheric electrons with energy up to 80 keV are observed on the magnetosheath side of the jets, which indicates that they escape into the magnetosheath through reconnected magnetic field lines. At the same time, the low-energy (below 100 eV) magnetosheath electrons enter the magnetosphere and are heated in the field-aligned direction at the high-density edge of the jets. Our observations provide unambiguous kinetic evidence for ongoing reconnection due to KH waves. Key Points * Magnetosheath electrons enter magnetosphere and magnetospheric electrons escape due to reconnection * Field-aligned heating of magnetosheath electrons at the high-density edges of the jets * Gradual ion mixing across the magnetopause
High density Interplanetary magnetic fields Jets Magnetic fields Magnetopause Magnetosheath Magnetospheres Trailing edges

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