In situ measurements of an event in the solar wind on 12 to 13 May 2022. (a) MAG magnetic field RTN components and magnitude, (b) PAS n_p, (c)–(d) PAS v_p and v_p, th and HIS , and , (e)–(g) elemental charge state distributions of C, O, Fe, (h)–(j) ion charge state ratios, and (k) Fe element abundance ratio. The first solid vertical red line marks the shock arrival time as observed by HIS. The ICME region is bounded vertical dashed black lines. A reverse shock is marked by the second solid vertical red line.