Interplanetary coronal mass ejections (ICMEs) are the interplanetary counterpart of coronal mass ejections (CMEs). Continually interacting with planetary environments, these impactful manifestations of solar activity drive the most extreme forms of space weather in our solar system and are not yet fully understood. Nevertheless, their geoeffectiveness and capability to trigger magnetic storms have societal impacts, which cannot be disregarded. Automatically detecting ICMEs in solar wind in situ data is a crucial part for accurately forecasting these events and their consequences, and significantly contributes to the way statistical studies of ICME parameters can be carried out.Initial studies (Burlaga et al., 1981;Gosling et al., 1973;Klein & Burlaga, 1982) and consecutive investigations of in situ measurements (Kilpua et al., 2017) led to a more thorough understanding of the typical appearance of ICMEs. Figure 1 depicts an example event exhibiting the typical signatures of an ICME featuring a magnetic cloud (MC), notwithstanding the existence of events without the presence of aforementioned structure (Rouillard, 2011). The top panel shows a smooth rotation of the magnetic field components and an enhanced