  Unraveling the geological processes ongoing at Io's numerous sites of active
volcanism requires high spatial resolution to, for example, measure the areal
coverage of lava flows or identify the presence of multiple emitting regions
within a single volcanic center. In de Kleer et al. (2017) we described
observations with the Large Binocular Telescope (LBT) during an occultation of
Io by Europa at ~6:17 UT on 2015 March 08, and presented a map of the
temperature distribution within Loki Patera derived from these data. Here we
present emission maps of three other volcanic centers derived from the same
observation: Pillan Patera, Kurdalagon Patera, and the vicinity of Ulgen
Patera/PV59/N Lerna Regio. The emission is localized by the light curves and
resolved into multiple distinct emitting regions in two of the cases. Both
Pillan and Kurdalagon Paterae had undergone eruptions in the months prior to
our observations, and the location and intensity of the emission is interpreted
in the context of the temporal evolution of these eruptions observed from other
facilities. The emission from Kurdalagon Patera is resolved into two distinct
emitting regions separated by only a few degrees in latitude that were
unresolved by Keck observations from the same month.
