Global Dataset of Martian Aeolian Landform : Transverse Aeolian Ridges and Crater-associated Wind Streaks

This dataset includes two key types of aeolian landforms: Transverse Aeolian Ridges (TARs) and crater-associated wind streaks.We applied the SegFormer (Xie et al., 2021) model to perform high-precision binary segmentation of TARs across the entire globe, resulting in the identification of over 90 million individual TARs features. Additionally, we utilized a YOLO (Jocher & Qiu, 2024) model to recognize approximately 24,000 crater-associated wind streaks.

The morphology of these landforms records the dominant surface wind directions at the time of their formation, serving as crucial proxies for reconstructing Martian paleoclimate.Data Storage Formats:TARs (Binary Segmentation Results): These segmentation results are stored in a binary raster image format. Each raster file adheres to the naming convention established for the MurrayLab CTX imagery.Crater-associated Wind Streaks (Vector Data): This data is stored in a Shapefile format.