File:PIA00096 Three-dimensional perspective views of Venusian Terrains composed of reduced resolution left-looking synthetic-aperture radar images merged with altimetry data from the Magellan spacecraft.jpg

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Description	The view shows most of Galindo (V-40) quadrangle looking east; Atete Corona, in the foreground, is a 600-km-long and about 450-km-wide, circular volcano-tectonic feature. Coronae are believed to form over hot upwellings of magma within the Venusian mantle.
Date	3 June 1998
Source	http://photojournal.jpl.nasa.gov/catalog/PIA00096
Author	NASA/JPL/USGS

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	Date/Time	Thumbnail	Dimensions	User	Comment
current	10:47, 7 August 2016		723 × 425 (62 KB)	PlanetUser (talk \| contribs)	higher res from the same file
	12:01, 15 April 2008		723 × 425 (62 KB)	Wang Ivan (talk \| contribs)	{{Information \|Description=The view shows most of Galindo (V-40) quadrangle looking east; Atete Corona, in the foreground, is a 600-km-long and about 450-km-wide, circular volcano-tectonic feature. Coronae are believed to form over hot upwellings of magma

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