Two-stage oscillatory response of the magnetopause to a tangential discontinuity/vortex sheet followed by northward IMF: Cluster observations

[1] We discuss the motion and structure of the magnetopause/boundary layer observed by Cluster in response to a joint tangential discontinuity/vortex sheet (TD/VS) observed by the Advanced Composition Explorer spacecraft on 7 December 2000. The observations are then supplemented by theory. Sharp polarity reversals in the east-west components of the field and flow By and Vy occurred at the discontinuity. These rotations were followed by a period of strongly northward interplanetary magnetic field (IMF). These two factors elicited a two-stage response at the magnetopause, as observed by Cluster situated in the boundary layer at the duskside terminator. First, the magnetopause suffered a large deformation from its equilibrium position, with large-amplitude oscillations of ∼3-min period being set up. These are argued to be mainly the result of tangential stresses associated with ΔVy the contribution of dynamic pressure changes being small in comparison. This strengthens recent evidence of the importance to magnetospheric dynamics of changes in azimuthal solar wind flow. The TD/VS impact caused a global response seen by ground magnetometers in a magnetic local time range spanning at least 12 h. The response monitored on ground magnetometers is similar to that brought about by magnetopause motions driven by dynamic pressure changes. Second, Cluster recorded higher-frequency waves (∼79 s). Two clear phases could be distinguished from the spectral power density, which decreased by a factor of ∼3 in the second phase. Applying compressible linearized MHD theory, we show that these waves are generated by the Kelvin-Helmholtz (KH) instability. Varying the local magnetic shear at the Cluster locale, as suggested by the temporal profile of the IMF clock angle, we find that locally stability was reinstated, so that the reduced power in the second phase is argued to be due residual KH activity arriving from locations farther to the dayside.

[1]  M. Freeman,et al.  Pressure-driven magnetopause motions and attendant response on the ground , 1989 .

[2]  J. Dungey Electrodynamics of the Outer Atmosphere , 1955 .

[3]  J. Steinberg,et al.  Geotail observations of the Kelvin‐Helmholtz instability at the equatorial magnetotail boundary for parallel northward fields , 2000 .

[4]  Wolfgang Baumjohann,et al.  Upstream pressure variations associated with the bow shock and their effects on the magnetosphere , 1990 .

[5]  A. Miura,et al.  Nonlocal stability analysis of the MHD Kelvin-Helmholtz instability in a compressible plasma. [solar wind-magnetosphere interaction] , 1982 .

[6]  J. K. Chao,et al.  Magnetospheric response to solar wind dynamic pressure variations: Interaction of interplanetary tangential discontinuities with the bow shock , 1993 .

[7]  A. Miura Anomalous transport by magnetohydrodynamic Kelvin‐Helmholtz instabilities in the solar wind‐magnetosphere interaction , 1984 .

[8]  M. Kivelson,et al.  The Magnetohydrodynamic Response of the Magnetospheric Cavity to Changes in Solar Wind Pressure , 1990 .

[9]  C. Farrugia,et al.  Concerning a problem on the Kelvin‐Helmholtz stability of the thin magnetopause , 2004 .

[10]  Michael E. Brown,et al.  Introduction to Space Physics , 1995 .

[11]  M. Dunlop,et al.  Triple cusps observed by Cluster—Temporal or spatial effect? , 2004 .

[12]  A. Lazarus,et al.  Surface waves on the tailward flanks of the Earth's magnetopause , 1995 .

[13]  D. Southwood Magnetopause Kelvin-Helmholtz instability , 1979 .

[14]  S. Wing,et al.  Global cooling and densification of the plasma sheet during an extended period of purely northward IMF on October 22–24, 2003 , 2005 .

[15]  J. Borovsky,et al.  Delivery of cold, dense plasma sheet material into the near‐Earth region , 2003 .

[16]  H. Keller Numerical Methods for Two-Point Boundary-Value Problems , 1993 .

[17]  H. Carlson,et al.  Continuous observation of cusp auroral dynamics in response to an IMF BY polarity change , 1999 .

[18]  M. Fujimoto,et al.  Plasma entry from the flanks of the near‐Earth magnetotail: Geotail observations , 1998 .

[19]  C. Farrugia,et al.  Viscous-type processes in the solar wind-magnetosphere interaction , 2001 .

[20]  C. Meng,et al.  Some low‐altitude cusp dependencies on the interplanetary magnetic field , 1989 .

[21]  M. Acuna,et al.  The ACE Magnetic Fields Experiment , 1998 .

[22]  J. W. Griffee,et al.  Solar Wind Electron Proton Alpha Monitor (SWEPAM) for the Advanced Composition Explorer , 1998 .

[23]  Mario H. Acuna,et al.  THE CLUSTER MAGNETIC FIELD INVESTIGATION , 1997 .

[24]  J. Sauvaud,et al.  Coordinated Wind, Interball/tail, and ground observations of Kelvin‐Helmholtz waves at the near‐tail, equatorial magnetopause at dusk: January 11, 1997 , 2000 .

[25]  J. Gratton,et al.  Convective instability of internal modes in accelerated compressible plasmas , 1988 .

[26]  M. Dunlop,et al.  Ground-based and satellite observations of high-latitude auroral activity in the dusk sector of the auroral oval , 2001 .

[27]  M. Fujimoto,et al.  Solar wind control of density and temperature in the near‐Earth plasma sheet: WIND/GEOTAIL collaboration , 1997 .

[28]  L. J. Cahill,et al.  Magnetopause structure and attitude from Explorer 12 observations. , 1967 .

[29]  M. Fujimoto,et al.  Plasma Entry from the Flanks of the Near-Earth Magnetotail : GEOTAIL Observations in the Dawnside LLBL and the Plasma Sheet , 1996 .

[30]  M. Yamauchi,et al.  On the solar wind flow control of the polar cusp , 2001 .

[31]  M. Kivelson,et al.  Anomalous aspects of magnetosheath flow and of the shape and oscillations of the magnetopause during an interval of strongly northward interplanetary magnetic field , 1993 .

[32]  M. Kivelson,et al.  Coupling of global magnetospheric MHD eigenmodes to field line resonances , 1986 .

[33]  J. Rouzaud,et al.  THE CLUSTER ION SPECTROMETRY (CIS) EXPERIMENT , 1997 .

[34]  David G. Sibeck,et al.  Oscillations of magnetospheric boundaries driven by IMF rotations , 1998 .

[35]  C. R. Clauer,et al.  Ionospheric traveling convection vortices observed near the polar cleft: A triggered response to sudden changes in the solar wind , 1988 .

[36]  Michelle F. Thomsen,et al.  Slow mode transition in the frontside magnetosheath , 1992 .

[37]  Hideaki Kawano,et al.  Magnetopause location under extreme solar wind conditions , 1998 .