Figure 1. Mars slope streaks. MOC M00/02117. Figure 2. Slope Streaks in the ADV; Left: digitate streaks, image
width 220 m; Right: parallel streaks and effect of local topography at lower left; image width 260 m. Slope is 20-300, top to bottom. Slope streaks in the Antarctic Dry Valleys: Characteristics, candidate formation mechanisms, and implications for slope streak formation in the Martian environment
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| Format: | Text |
| Language: | English |
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| Online Access: | http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.456.753 http://people.bu.edu/marchant/Dave_Conference Abstracts/Other/Head_ISAES_2007_177.pdf |
| Summary: | width 220 m; Right: parallel streaks and effect of local topography at lower left; image width 260 m. Slope is 20-300, top to bottom. Slope streaks in the Antarctic Dry Valleys: Characteristics, candidate formation mechanisms, and implications for slope streak formation in the Martian environment |
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