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We present a catalogue of 35 interplanetary coronal mass ejections (ICMEs)observed by the Juno spacecraft and at least one other spacecraft during itscruise phase to Jupiter. We identify events observed by MESSENGER, VenusExpress, Wind, and STEREO with magnetic features that can be matchedunambiguously with those observed by Juno. A multi-spacecraft study of ICMEproperties between 0.3 and 2.2 AU is conducted: we firstly investigate theglobal expansion by tracking the variation in magnetic field strength withincreasing heliocentric distance of individual ICME events, finding significantvariability in magnetic field relationships for individual events in comparisonwith statistical trends. With the availability of plasma data at 1 AU, thelocal expansion at 1 AU can be compared with global expansion rates between 1AU and Juno. Despite following expected trends, the local and global expansionrates are only weakly correlated. Finally, for those events with clearlyidentifiable magnetic flux ropes, we investigate the orientation of the fluxrope axis as they propagate; we find that 64% of events displayed a decrease ininclination with increasing heliocentric distance, and 40% of events undergo asignificant change in orientation as they propagate towards Juno. Themulti-spacecraft catalogue produced in this study provides a valuable linkbetween ICME observations in the inner heliosphere and beyond 1 AU, therebyimproving our understanding of ICME evolution.

Multi-Spacecraft Observations of the Evolution of Interplanetary Coronal Mass Ejections Between 0.3 and 2.2 AU: Conjunctions with the Juno Spacecraft