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On observing the compositional variability of the surface of Venus using nightside near-infrared thermal radiation

✍ Scribed by Hashimoto, George L.

Book ID
119661786
Publisher
American Geophysical Union
Year
2003
Tongue
English
Weight
208 KB
Volume
108
Category
Article
ISSN
0148-0227

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Lava eruptions can be observed remotely on Venus' nightside using a near-infrared window at a 1.0-micrometer wavelength, i.e., radiation at this wavelength emitted from the planetary surface traverses through the thick Venus atmosphere and clouds. Due to the strong dependence of the intensity of the