Fig. 5
From: Detection of Martian dust storms using mask regional convolutional neural networks
2nd strategy: the training, validation and testing images are selected randomly from MY 25 to MY 28. a and c are ground-truth images from spring season (\(r18\_040\)) at \(L_{\mathrm{{S}}}=53.47^{\circ }\) and summer seasons (\(r22\_008\)) at \(L_{\mathrm{{S}}}=105.36^{\circ }\), respectively. b and d are their predicted dust maps