The ASKAP update for June reports on the status of ongoing survey operations, VAST scheduling, development priorities, the first RACS-mid data release, and solar interference. The Sun is a particularly bright source that, even though it sits outside the field of view during any day-time observation, can be detected in the sidelobes of the PAF beams. The active Sun appears as a collection of relatively compact sources within the solar disk, but these can be quite dynamic and hard to characterise. The image above shows data from a recent POSSUM observation, split into 1- hour integrations and re-imaged in the direction of the Sun to show its impact before (panels 1-5), during (panel 6) and after (panels 7-10) sunrise. Note the complicated structure in these images prior to deconvolution, most likely resulting from small active regions on the surface of the Sun. (Image credit: Stefan Duchesne)