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- W2520287797 abstract "Abstract The dusk flank magnetopause was surveyed with instruments on board the Magnetospheric Multiscale (MMS) spacecraft on 28 August 2015 between 13:55 UT and 14:15 UT during a period of persistent southward interplanetary magnetic field (IMF) with varying dawn‐dusk component. Plasma measurements (500 eV electrons, > 2 keV ions) revealed the existence of at least one active reconnection region that persisted throughout the interval. The reconnection region convected equatorward despite the poleward and tailward magnetosheath flow, which ranged from slightly sub‐Alfvénic to slightly super‐Alfvénic throughout the interval. These results suggest that magnetic reconnection moved in response to changes in the IMF clock angle rather than the magnetosheath flow, which is corroborated using predictions of the maximum magnetic shear model." @default.
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- W2520287797 date "2016-09-17" @default.
- W2520287797 modified "2023-09-26" @default.
- W2520287797 title "Stable reconnection at the dusk flank magnetopause" @default.
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- W2520287797 doi "https://doi.org/10.1002/2016gl069692" @default.
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