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- W1810633843 abstract "We have generated fully three-dimensional, high-resolution magnetohydrodynamic (MHD) simulations of the Kelvin–Helmholtz (KH) Instability during Parker-Spiral Interplanetary Magnetic Field (IMF) conditions at the dawnside magnetospheric flank magnetopause. Results of these simulations show that, although the draping of a strong tangential magnetic field component around the magnetopause, tailward of the terminator (due to the Parker-Spiral orientation), tends to stabilize the growth of such instabilities within the shear-flow plane, Kelvin–Helmholtz waves with a k-vector tilted out of this plane may, nonetheless, develop into the nonlinear phase. This result suggests that obliquely propagating KH waves may contribute to the dawn-dusk asymmetries observed in plasma sheet parameters." @default.
- W1810633843 created "2016-06-24" @default.
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- W1810633843 date "2016-07-01" @default.
- W1810633843 modified "2023-10-15" @default.
- W1810633843 title "The Kelvin–Helmholtz instability under Parker-Spiral Interplanetary Magnetic Field conditions at the magnetospheric flanks" @default.
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- W1810633843 doi "https://doi.org/10.1016/j.asr.2015.09.013" @default.
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