Solar wind in-situ observation from the OMNI dataset that contain both an ICME and a SIR. From top to bottom are represented the Interplanetary Magnetic Field amplitude and components in Geospheric Solar Magnetospheric (GSM) coordinates, the proton number density, the solar wind velocity, the proton temperature and the plasma parameter β. The vertical solid gray lines indicate the cells on which the identification is made. The ICME (resp. SIR) from the reference catalog is indicated between the red (resp. blue) dashed lines. The grey shaded intervals represent the cells that are responsible for the detection of the ICME (resp. the SIR) represented by the red (resp. blue) interval, the associated vertical solid line that represents their associated characteristic time and the confidence score with which those events are identified, as detailed in Section 2.