Multipoint interplanetary coronal mass ejections observed with Solar Orbiter, BepiColombo, Parker Solar Probe, Wind and STEREO-A

We report the result of the first search for multipoint in situ and imaging observations of interplanetary coronal mass ejections (ICMEs) starting with the first Solar Orbiter data in April 2020 to April 2021. A data exploration analysis is performed including visualizations of the magnetic field and plasma observations made by the five spacecraft Solar Orbiter, BepiColombo, Parker Solar Probe, Wind and STEREO-A, in connection with coronagraph and heliospheric imaging observations from STEREO-Ahead/SECCHI and SOHO/LASCO. We identify ICME events that could be unambiguously followed with the STEREO-A heliospheric imagers during their interplanetary propagation to their impact at the aforementioned spacecraft, and look for events where the same ICME is seen in situ by widely separated spacecraft. We highlight two events: (1) a small streamer blowout CME on 2020 June 23 observed with a triple lineup by Parker Solar Probe, BepiColombo and Wind, guided by imaging with STEREO-A, and (2) the first fast CME of solar cycle 25 ($ \approx 1600$ km s$^{-1}$) on 2020 Nov 29 observed in situ by Parker Solar Probe and STEREO-A. These results are useful for modeling the magnetic structure of ICMEs, the interplanetary evolution and global shape of their flux ropes and shocks, and for studying the propagation of solar energetic particles. The combined data from these missions is already turning out to be a treasure trove for space weather research and is expected to become even more valuable with an increasing number of ICME events expected during the rise and maximum of solar cycle 25.