The local weather conditions on the evening of November 19 were far from optimal, with a strong breeze and almost overcast conditions throughout the evening.
Nevertheless, some decent imagery was captured showing a fair amount of Martian detail. Based on the observations made by other planetary imagers such as Damien Peach and Christopher Go, their reported dust cloud can also be traced on my images specifically on the upper left side of the RGB-IR(L) image situated over Solis Lacus and extending over part of Aonius Sinus and further northwards.
The outline of Solis Lacus is quite faint, but not completely obscured by the dust. My results show that the dust event is quite extensive but not very dense. The origin of this dust cloud started all the way from Mare Erythraeum on the other side of Mars on November 12.