Fig. 1.

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(a) Schematic of a cylindrical MC (solid red curve), the ecliptic plane (grey), and the position of the Sun S and the spacecraft E at L1. The AW, η, Sun-centre Oc and the CME source location Os on the solar disk are labelled in the figure. The FR axis is shown as the dash-dotted red line. The Sun-Earth line OcE is shown by the dashed black line and is on the ecliptic plane. The lines OsX and PQ indicate the heliocentric distance r and LMC, respectively. The perpendicular distance p is denoted by the violet line BX. The line BX is perpendicular to OcE. (b) The expanding circular cross-section of a cylindrical MC. X is the centre of the cross-section. At t = 0, the MC cross-sectional circumference is denoted by the red circle. The radial expansion of the MC with speed Vρ is in the direction of the yellow arrows, and in the FR frame of reference, the spacecraft propagates with a speed Vpro towards the path indicated by black arrows.
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