(a): STIX source positions as seen from Solar Orbiter. All positions have been rescaled to 1 au. The size of the circles corresponds to the GOES peak estimate, while the colours indicate the composition. (b): STIX X-ray source longitude as seen from Solar Orbiter. (c): Heliographic latitude difference between the STIX source and the footpoint of magnetic connectivity. Impulsive event distributions are shown in blue, gradual ones in red, and the black histogram represents all events. Dotted lines show the medians of the distributions for impulsive and gradual events. (d): As in (c), but showing the heliographic longitude difference between the STIX source and the footpoint of magnetic connectivity.