Seasonal Slumps in Juventae Chasma, Mars
Dark topographic slumps several meters wide, tens of meters in length, and up to a meter in depth are observed on the slopes of Juventae Chasma (JC), Valles Marineris (VM), Mars. These slumps usually originate near the terminal points of recurring slope lineae (RSL). Near their initiation points, th...
Main Authors: | , , , , , , , , , , |
---|---|
Other Authors: | |
Language: | en |
Published: |
AMER GEOPHYSICAL UNION
2017
|
Online Access: | http://hdl.handle.net/10150/626275 http://arizona.openrepository.com/arizona/handle/10150/626275 |