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VIRTIS
Atmospheric stripe-like structures are observed on Venus at a wavelength of 380 nm. -
VIRTIS
A sequence of eight images at 2.3 μm from eight orbits in February 2007 shows the difference in atmospheric flow characteristics on Venus as a function of latitude. -
VIRTIS
The VIRTIS instrument has made the first detection of hydroxyl (OH) in the atmosphere of Venus. -
VIRTIS
Global and detailed images of cloud features on Venus obtained at ultraviolet wavelengths (365 nm) are presented. They clearly show the variation of cloud structures with latitude. -
VIRTIS
A faint and variable nightglow of nitric oxide (NO) has been unambiguously detected in the upper atmosphere of Venus. -
VIRTIS
The derived differences in surface rock composition are consistent with suspicions that Venus once had a plate tectonics system and an ocean of water.