IMAGE_pic1\100_199\180.GIF,Mariner 10's cameras took this picture of clouds in Venus' atmosphere in ultraviolet light in February 1974.
IMAGE_pic1\200_299\269.GIF,A remarkable view of the surface of Venus obtained by Magellan's radar, showing rugged terrain on a plateau (Lakshmi Planum) in Ishtar Terra, one of the two big continents on the planet.
IMAGE_pic1\200_299\270.GIF,A Magellan radar image of the surface of Venus, showing what appear to be a volcanic crater and lava flows.
IMAGE_pic1\200_299\271.GIF,False-colour imagery has been used to enhance features in a Magellan radar scan of Venus. At bottom right is an impact crater, and surrounding flows of ejected material.
IMAGE_pic1\1000_99\65.GIF,Mosaic image of Venus produced from scans by Magellan's radar in 1991. The view is centred at 0 degrees east longitude.
IMAGE_pic1\1000_99\66.GIF,A computer-simulated view of the surface of Venus, based on radar scans by Magellan in 1991. It shows a volcanic crater with a diameter of about 25 km, surrounded by numerous lava flows.