Physical models and predictions for recurring slope lineae formed by wet and dry processes.

C Huber, L Ojha, L Lark, JW Head - Icarus, 2020 - Elsevier
The observation of low albedo, elongated and transient features lengthening downhill on
Mars has attracted wide interest because of the possible role of aqueous fluids in their …

Can we constrain the origin of Mars' recurring slope lineae using atmospheric observations?

H Kurokawa, T Kuroda, S Aoki, H Nakagawa - Icarus, 2022 - Elsevier
Flowing water and brine have been proposed to cause seasonally reappearing dark streaks
called recurring slope lineae (RSL) on steep warm slopes on Mars, along with other …

Planetary landscapes and the role of volatiles in their making

SJ Conway - 2023 - hal.science
This thesis concerns the study of planetary landscapes with the objective of understanding
the role of volatiles in sculpting these landscapes which falls under the broad theme of …

Pāhoehoe Breakouts and Lava-Substrate Interactions: Insights From Large-Scale Experimental Lava Flows

CJ Sant - 2023 - search.proquest.com
Basaltic lava flows are one of the most visible geologic processes on Earth. Gaining a
thorough knowledge of basaltic lava flow behavior is imperative to understanding Earth's …

Influence of ice degradation on planetary landscapes

M Philippe - 2023 - theses.hal.science
The present thesis aims at getting new understandings on how ground water ice and
periglacial processes influence surface geomorphology on Earth and on Mars. I am hence …

Experimental study of sediment transport processes by liquid water and brine under Martian pressure

M Philippe, SJ Conway, J Raack, S Carpy, M Massé… - Icarus, 2023 - Elsevier
We present here an experimental study to compare the behaviour of water and brine
releases over loose sediments under present-day Martian pressure. Water has been …

[PDF][PDF] Experimental study of sediment transport processes by liquid water and brine under Martian pressure

M Philippe, SJ Conway, J Raack, S Carpy… - Europlanet Science …, 2019 - hal.science
Martian slopes host several downslope movement morphologies, including Recurring Slope
Lineae (dark linear flows–[1]) and gullies (mass-wasting sediment movements composed of …