Intracrater Terminal Dune Fields in Arabia Terra, Mars

Taylor Dorn & Mackenzie Day
Craters are the most prevalent basins and potential depo-centers of sediment on Mars. Within these craters and extending from them, terminal dune fields and wind streaks are abundant, indicating active sediment transport and providing a way to study how wind and sediment interact with crater topography. Here, we explore the role of craters as both sources and sinks in the modern martian sedimentary cycle. Our results show that craters with low albedo wind streaks (indicative...
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3 downloads reported since publication in 2020.

These counts follow the COUNTER Code of Practice, meaning that Internet robots and repeats within a certain time frame are excluded.
What does this mean?