In situ measurements given in day-of-year (DOY) time series around 2021 November 4 (DOY 308) from Solar Orbiter (left panels) and OMNI (right panels). Top row: magnetic field strength. Second row: x-, y-, and z-component (red, blue and green, respectively) of the magnetic field in the Geocentric solar ecliptic (GSE). Third row: plasma density (black), plasma temperature (red), and expected temperature (blue). Bottom row: plasma flow speed (black) and plasma-β (gray). Observed features corresponding to the sheath region, frontal region of the interplanetary flux rope, and magnetic cloud are indicated by green-, olive-, and red-shaded areas, respectively.