File:Cloud Streets - Mars Express (27956397993).png

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Cumulus cloud streets form during the autumn in the Martian high latitudes. These cloud streets form as convective rolls. The streets form where rising air from the surface diverges, allowing the meager water content of the atmosphere to condense. Normally, these convective patterns would form a jumbled mass of individual cumulus clouds, but here they are shaped by regional winds that preferentially align these convective regions into more or less straight lines.

This image was taken by HRSC during Mars Express' 5554th orbit of Mars, April 29, 2008.

Image Credit: ESA/DLR/FU Berlin/J. Cowart, CC BY-SA 3.0 IGO
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Source Cloud Streets - Mars Express
Author Justin Cowart

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This image was originally posted to Flickr by jccwrt at https://flickr.com/photos/132160802@N06/27956397993. It was reviewed on 3 December 2020 by FlickreviewR 2 and was confirmed to be licensed under the terms of the cc-by-sa-2.0.

3 December 2020

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current12:29, 3 December 2020Thumbnail for version as of 12:29, 3 December 20207,680 × 2,400 (22.11 MB)Eyes Roger (talk | contribs)Transferred from Flickr via #flickr2commons

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