Martian Surface/Atmosphere Web Interface

Welcome to this innovative platform that transforms data from NASA Ames General Circulation Model (GCM) into valuable insights on the interaction between atmospheric flows and surface materials on Mars. This interface enables users to:

• Analyze sand flux directions and dune orientations.
• Examine dune orientation under high sand availability (bed instability mode).
• Study dune alignment under limited sand availability and complex flow patterns (finger mode).
• Adjust key planetary parameters like obliquity, eccentricity, and atmospheric pressure to explore long-term climatic changes.

Designed for the scientific community, this platform offers a powerful tool to test atmospheric models and enhance our understanding of Martian local geology.