First identification of mirror mode waves in Venus' magnetosheath?
First identification of mirror mode waves in Venus' magnetosheath?
First identification of mirror mode waves in Venus' magnetosheath?
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X - 14VOLWERK ET AL.: VENUS’ MIRROR MODE WAVESFigure 1.The magnetic field data for 5 May 2006. The spacecraft moves from thesolar w<strong>in</strong>d (SW), through the bowshock (BS) <strong>in</strong>to the <strong>magnetosheath</strong> (MS). The twobottom panels show the fluctuation <strong>of</strong> the magnetic field ∆B/B and the angle betweenthe maximum variance direction and the mean magnetic field θ Bmv (black dots), and theangle between the m<strong>in</strong>imum variance direction and the mean magnetic field β Bmv (redplusses).Figure 2.Power spectra for <strong>in</strong>tervals I (top panel 5 May, bottom panel 2 October)<strong>of</strong> <strong>mirror</strong> <strong>mode</strong> <strong>waves</strong> for the compressional (solid) , and right- (dotted) and left-handed(dashed) polarized components <strong>of</strong> the magnetic field. The obsevered compressional <strong>waves</strong>are marked with a vertical l<strong>in</strong>e.Figure 3.The magnetic field data for 2 October 2006. The spacecraft moves fromperiapsis <strong>in</strong> Venus’ magnetosphere (MSp), through the magnetopause (MP) <strong>in</strong>to the<strong>magnetosheath</strong> (MS). The two bottom panels show the fluctuation <strong>of</strong> the magnetic field∆B/Band the angle between the maximum variance direction and the mean magneticfield θ Bmv (black dots), and the angle between the m<strong>in</strong>imum variance direction and themean magnetic field β Bmv (red plusses).D R A F T February 13, 2008, 4:35am D R A F T