Detailed distributions of solar wind plasma types in non-ICME cases that have two or more major plasma types (N_{major plasma type} ≥ 2, based on S_strong). Plasma types are based on Xu & Borovsky (2015), calculated on a 12-min cadence. The timeline has been normalized for each case; zero and one are min(ST_Fe, ST_O) and max(ET_Fe, ET_O). The serial numbers of cases (No.) are marked on the y-axis, and they correspond to the case list available at Zenodo (see Data availability).