3D (anaglyph) image of the mouth of Mamers Valles on Mars
3D (anaglyph) image of the mouth of Mamers Valles on Mars
Using the nadir channel, which is directed perpendicular to the Martian surface, and one of the oblique stereo channels of the HRSC camera, 'anaglyph' images can be generated. When viewed with red-blue or red-green glasses, they provide a three-dimensional view of the landscape. The high image resolution of 20 metres per pixel allows even the smallest topographic features to be visualised – including landslides on the slopes of the mesas (table mountains), accumulations of dust covered ice in some of the Mamers valleys, and mesas protruding from the ancient highlands of Arabia Terra.
