Fig. 6
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. Left panel shows ground-truth maps, and right panel shows predicted maps. a and c are ground-truth images from fall season (\(r08\_005\)) at \(L_{\mathrm{{S}}}=238.51^{\circ }\) and winter season (\(r12\_017\)) at \(L_{\mathrm{{S}}}=313.57^{\circ }\) and b and d are their predicted dust maps