Fig. 2.

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Interplanetary CME measured in situ on 10 January 1997 (left panels) and 3 November 2000 (right panels). From top to bottom, the following parameters are shown: Magnetic field magnitude in black and magnetic field fluctuations in gray (right scale); GSE magnetic field components (red, Bx; blue, By; green, Bz); proton density in black, temperature in red, and expected temperature in blue; solar wind speed in black and plasma beta parameter in gray; GSE velocity components (blue, By; green, Bz). From left to right, the vertical magenta lines mark the shock arrival, the end of the clear sheath, and the MO end time. In the right panels, the end of the clear sheath part does not coincide with the MO onset time, and there is an additional vertical magenta line present.
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