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On 3 July 2001, the four Cluster satellites traversed along the dawnsidemagnetospheric flank and observed large variations in all plasma parameters.The estimated magnetopause boundary normals were oscillating in thez-direction and the normal component of the magnetic field showedsystematic  2–3 min bipolar variations for 1 h when the IMF had asmall positive bz-component and a Parker-spiral orientation in thex,y-plane. Brief  33 s intervals with excellent deHoffman Tellerframes were observed satisfying the Walén relation. Detailed comparisonswith 2-D MHD simulations indicate that Cluster encountered rotationaldiscontinuities generated by Kelvin-Helmholtz instability. We estimate a wavelength of  6 RE and a wave vector with a significantz-component

Cluster observations of reconnection due to the Kelvin-Helmholtz instability at the dawnside magnetospheric flank