3D (anaglyph) image of the region north of Eumenides Dorsum
3D (anaglyph) image of the region north of Eumenides Dorsum
Anaglyph images can be generated from the nadir channel (which looks directly down at the Martian surface) and one of the oblique-viewing stereo channels of the HRSC. These images, when viewed with red–blue or red–green glasses, provide a three-dimensional view of the landscape. At approximately 20 metres per pixel, the high image resolution allows us to visualise even minor topographical features, such as the prominent impact crater in the centre of the image and the yardangs – ridges sculpted from rock by the wind – in the upper middle of the image.
