Anaglyph image of a dust storm front high in the northern latitudes of Mars
Anaglyph image of a dust storm front high in the northern latitudes of Mars
Anaglyph images are produced using the data acquired by the nadir channel of the Mars Express High Resolution Stereo Camera (HRSC), the field of view of which is aligned perpendicular to the surface of Mars, and one of the four obliquely angled stereo channels. Anaglyphs create a realistic, three-dimensional impression of the landscape when viewed through red/blue or red/green glasses. This 3D view shows the dust storm front forming above the subpolar plains.