Interplanetary Coronal Mass Ejections are the interplanetary counterpart of Coronal Mass Ejections, the expulsion of large quantities of plasma and magnetic field at the solar surface detected by in situ instrumentation, with specific imprints in the observations. Here we propose a visual suggestion of the last 6 months of in-situ data provided by WIND. We used the method provided by Nguyen et al. (ApJ, 2019) to give a visual suggestion of regions in data that could contain one or several ICMEs.