Timing diagram of simulated radial velocity, V_r, in km s⁻¹ (a, d), proton number density in units of 10³ cm⁻³ (b, e), and magnetic field strength in unit of Gauss (c, f) observed by two virtual satellites located at the HDLS (a, b, c) and LDHS (d, e, f) regions. The solid black lines denote variables observed at (r,θ,ϕ) = (20 R_s,0,201°) and (r,θ,ϕ) = (20 R_s,−70°,201°) during the 82nd and 735th hours of the time-evolving coronal simulation. For the quasi-steady-state coronal simulations constrained by magnetograms at 82 (denoted by dashed black lines) and 735 (denoted by dash-dot black lines) of this time interval, the heliolongitude is mapped to a CR period corresponding to the time series on the horizontal axis of the timing diagram. The solid grey line (a) denotes the velocity observed by the WIND satellite and mapped from 1 AU to 20 R_s following the ballistic propagation.