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Figure S1.pdfPDF document2927Kpdf Map showing the location of the regions discussed in this study. Valley networks mapped by Hynek et al. [2010]. WV denotes Warrego Valles, MS denotes the area of Margaritifer Sinus containing Paraná Valles and the valleys of Newcomb Crater, TS denotes the area of Terra Sabea containing Tisia Valles and other valley networks, and TC denotes the area of Terra Cimmeria studied.
Figure S2.pdfPDF document2969Kpdf Valley networks in Margaritifer Sinus. MOLA-shaded THEMIS daytime IR imagery. The image is centered near 22.7°S, 6.5°W. Valleys mapped by Hynek et al. [2010] using 230m/pixel resolution THEMIS-IR imagery are shown in white. Valleys newly visible in ~6 m/pixel resolution CTX and 100 m/pixel resolution THEMIS-IR imagery are shown in black. The rate (in mm/h) of modeled orographic precipitation forced by westerly winds in a 1 bar atmosphere is shown in blue. The white box indicates a region where a west-facing slope and a comparably steep east-facing slope are unequally dissected.
Figure S3.pdfPDF document162Kpdf Wind rose diagrams for the grid box nearest the center of Figure S2, compiled from one Mars year of our GCM simulation with 500 mb (left), 1 bar (center), and 2 bar (right) surface pressure. The length of each column corresponds to the frequency of winds blowing from within a 45° bin centered on each compass direction. The length of colored bands within each column indicates the frequency of the corresponding wind speed range.
Figure S4.pdfPDF document2332Kpdf Valley networks in Terra Sabea. MOLA-shaded THEMIS daytime IR imagery. The image is centered near 4.5°S, 42.7°E. Valleys mapped by Hynek et al. [2010] using 230 m/pixel resolution THEMIS-IR imagery are shown in white. Valleys newly visible in ~6 m/pixel resolution CTX and 100 m/pixel resolution THEMIS-IR imagery are shown in black. The rate (in mm/h) of modeled orographic precipitation forced by northeasterly winds in a 1 bar atmosphere is shown in blue.
Figure S5.pdfPDF document166Kpdf Wind rose diagrams for the grid box nearest the center of Figure S2 compiled from one Mars year of our GCM simulation with 500 mb (left), 1 bar (center), and 2 bar (right) surface pressure. The length of each column corresponds to the frequency of winds blowing from within a 45° bin centered on each compass direction. The length of colored bands within each column indicates the frequency of the corresponding wind speed range.
readme.pdfPDF document59KSupporting information

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