  We present a catalogue of 35 interplanetary coronal mass ejections (ICMEs)
observed by the Juno spacecraft and at least one other spacecraft during its
cruise phase to Jupiter. We identify events observed by MESSENGER, Venus
Express, Wind, and STEREO with magnetic features that can be matched
unambiguously with those observed by Juno. A multi-spacecraft study of ICME
properties between 0.3 and 2.2 AU is conducted: we firstly investigate the
global expansion by tracking the variation in magnetic field strength with
increasing heliocentric distance of individual ICME events, finding significant
variability in magnetic field relationships for individual events in comparison
with statistical trends. With the availability of plasma data at 1 AU, the
local expansion at 1 AU can be compared with global expansion rates between 1
AU and Juno. Despite following expected trends, the local and global expansion
rates are only weakly correlated. Finally, for those events with clearly
identifiable magnetic flux ropes, we investigate the orientation of the flux
rope axis as they propagate; we find that 64% of events displayed a decrease in
inclination with increasing heliocentric distance, and 40% of events undergo a
significant change in orientation as they propagate towards Juno. The
multi-spacecraft catalogue produced in this study provides a valuable link
between ICME observations in the inner heliosphere and beyond 1 AU, thereby
improving our understanding of ICME evolution.
