Formation of Ares Vallis (Mars) by effusions of low-viscosity lava within multiple regions of chaotic terrain-Reference-Cited by-同舟云学术

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Formation of Ares Vallis (Mars) by effusions of low-viscosity lava within multiple regions of chaotic terrain

Published:2019-11 Issue: Volume:345 Page:106828
ISSN:0169-555X
Container-title:Geomorphology
language:en
Short-container-title:Geomorphology

Author:

Leverington David W.

Publisher

Elsevier BV

Subject

Earth-Surface Processes

Reference300 articles.

1. A search for minerals associated with serpentinization across Mars using CRISM spectral data;Amador;Icarus,2018

2. Hydrological modeling of outflow channels and chaos regions on Mars;Andrews-Hanna;J. Geophys. Res.,2007

3. Evaporite karst in three interior layered deposits in Iani Chaos, Mars;Baioni;Geomorphology,2015

4. The Channels of Mars;Baker,1982

5. Water and the Martian landscape;Baker;Nature,2001

Cited by 8 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Valley Relief of the Northeastern Part of Terra Cimmeria on Mars;Solar System Research;2024-05-20

2. Megaflood Erosion on Mars—How Lava‐Filled Craters Became Mesas (With Insights From Lava Physics, Stream Power, and Rock Mechanics);Journal of Geophysical Research: Planets;2024-02

3. Constraints on the effusive volcanic eruptions that formed Kallistos Vallis, Venus;Geomorphology;2023-08

4. Development of Shalbatana Vallis (Mars) by dry volcanic processes;Planetary and Space Science;2022-06

5. Explosive Volcanism on Mars;Mars: A Volcanic World;2021

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