Morphometric and topographic data of small and medium size landforms in the Northern Circumpolar Region of Mars

A substantial dataset containing topographic landforms at Olympia Undae and Scandia Cavi in the Northern circumpolar region of Mars was created by Sanchez-Bayton et al. (2022) [1]. This dataset contains the essential morphometric parameters of 200 small and medium-size landforms. In particular, it i...

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Detalles Bibliográficos
Autores: Sánchez Bayton, Marina, Herraiz Sarachaga, Miguel, Martin, Patrick, Sánchez-Cano Moreno de Redrojo, Beatriz, Tréguier, Erwan, Kereszturi, Akos
Tipo de recurso: artículo
Fecha de publicación:2022
País:España
Institución:Universidad Complutense de Madrid (UCM)
Repositorio:Docta Complutense
Idioma:inglés
OAI Identifier:oai:docta.ucm.es:20.500.14352/71774
Acceso en línea:https://hdl.handle.net/20.500.14352/71774
Access Level:acceso abierto
Palabra clave:550.2
Mars Northern polar region
Volcanic landforms
Impact craters
Morphometric and topographic data
Scandia Cavi
Olympia Undae
Mars Express
Mars Reconnaissance Orbiter
Astrofísica
Descripción
Sumario:A substantial dataset containing topographic landforms at Olympia Undae and Scandia Cavi in the Northern circumpolar region of Mars was created by Sanchez-Bayton et al. (2022) [1]. This dataset contains the essential morphometric parameters of 200 small and medium-size landforms. In particular, it includes cratered, non-cratered, and complex irregular structures. Experimental Data Records (EDR) were obtained from the Mars Express, Mars Reconnaissance Orbiter, and Mars Global Surveyor missions, and the analysed dataset was produced thanks to the Java Mission-planning and Analysis for Remote Sensing (JMARS) software. This dataset constitutes a significant improvement in the characterisation of the small and medium-size topographic structures in the Northern circumpolar region of Mars and it contributes towards better understanding of the Northern circumpolar area. This dataset is of great value for modellers and other studies of the Martian surface processes, related to volcanic structures, aeolian processes driving to erosion or deposition, sublimation and subglacial processes, and several impact events.