![state property 2002 torrent state property 2002 torrent](https://www.researchgate.net/profile/Claire-Pernollet/publication/274637694/figure/fig4/AS:294669067014148@1447265988518/Torrent-Duck-monthly-densities-upstream-and-downstream-from-the-two-hydropower-schemes-in_Q320.jpg)
Mars Orbiter Laser Altimeter: experiment summary after the first year of global mapping of Mars. New Martian valley network volume estimate consistent with ancient ocean and warm and wet climate. A progressive black top hat transformation algorithm for estimated valley volumes on Mars. Geologic Map of Mars US Geological Survey Scientific Investigations Map SIM 3292 (2014). Rapid formation of a modern bedrock canyon by a single flood event. Catastrophic flooding origin of shelf valley systems in the English Channel. Magnitudes and implications of peak discharges from glacial Lake Missoula. Precipitation and aridity constraints from paleolakes on early Mars. Insights into surface runoff on early Mars from paleolake basin morphology and stratigraphy.
![state property 2002 torrent state property 2002 torrent](https://ars.els-cdn.com/content/image/1-s2.0-B9780123919380000057-f05-03-9780123919380.jpg)
Constraints on the Noachian paleoclimate of the martian highlands from landscape evolution modeling. The timing of martian valley network activity: Constraints from buffered crater counting. Valley formation on early Mars by subglacial and fluvial erosion. Did martian valley networks substantially modify the landscape? Earth Planet. Scaling relations for large Martian valleys. Drainage basins and channel incision on Mars. Incision of Licus Vallis, Mars from multiple lake overflow floods. Fill and spill of giant lakes in the eastern Valles Marineris region of Mars. in Megaflooding on Earth and Mars (eds Burr, D. Incision of paleolake outlet canyons on Mars from overflow flooding. Geomorphology of Ma’adim Vallis, Mars, and associated paleolake basins. A large paleolake basin at the head of Ma’adim Vallis, Mars.
![state property 2002 torrent state property 2002 torrent](https://m.media-amazon.com/images/M/MV5BMTIwNDU3NTA5M15BMl5BanBnXkFtZTcwNDA4MjYxMQ@@._V1_.jpg)
Valley network-fed, open-basin lakes on Mars: distribution and implications for Noachian surface and subsurface hydrology. Increased runoff and paleolake development. An intense terminal epoch of widespread fluvial activity on early Mars: 2. Distribution, classification, and ages of Martian impact crater lakes.
![state property 2002 torrent state property 2002 torrent](https://64.media.tumblr.com/86d6676d67f5c8e5363b11ca28012575/56065405be1eed08-4a/s400x600/8f7c2e5f53bc65440af93c6e39123700c0cecd83.jpg)
Updated global map of Martian valley networks and implications for climate and hydrologic processes. Valley network incision and associated deposits. An intense terminal epoch of widespread fluvial activity on early Mars: 1. Martian valleys: morphology, distribution, age, and origin. Our results indicate that the importance of lake breach floods should be considered when reconstructing the formative conditions for Martian valley systems. We conclude that lake breach floods were a major geomorphic process responsible for valley incision on early Mars, which in turn influenced the topographic form of many Martian valley systems and the broader landscape evolution of the cratered highlands. Here, we demonstrate the global importance of lake breach flooding, and find that it was responsible for eroding at least 24% of the volume of incised valleys on early Mars, despite representing only approximately 3% of total valley length. Much past work has recognized the local importance of lake breach floods on Mars for rapidly incising large valleys 7, 8, 9, 10, 11, 12 however, on a global scale, valley systems have often been interpreted as recording more persistent fluvial erosion linked to a distributed Martian hydrologic cycle 1, 2, 3, 13, 14, 15, 16. Over 200 of these lake basins filled with sufficient water to breach the confining topography 4, 6, causing catastrophic flooding and incision of outlet canyons 7, 8, 9, 10. The surface environment of early Mars had an active hydrologic cycle, including flowing liquid water that carved river valleys 1, 2, 3 and filled lake basins 4, 5, 6.