Research Aims - Study the tectonics features and the stress field in Noctis Labyrinthus. - Scrutinize the Pit Chains morphology and evolution. - Reveal the processes responsible for the complex ramify rift systems and troughs
Noctis Labyrinthus is an intricate system of Late Hesperian and Early Amazonian linear troughs and r...
To determine whether the structural evolution of the Northern Cerberus Fossae (NCF) was dominated by...
Volcanic activity is widespread within the inner Solar system and it can be commonly observed on roc...
Research Aims - Study the tectonics features and the stress field in Noctis Labyrinthus. - Scrutiniz...
ResearchAims: 1. Study the tectonic features and the stress field in NoctisLabyrinthus. 2. Scruti...
Oral Presentation - 2nd Planetary Mapping and Virtual Observatory Workshop 1-3 July 2019, Domaine de...
Pit chains commonly occur along a bounding fault, allowing to infer a genetic relationship between ...
Noctis Labyrinthus (Mars) is characterized by many tectonic features, which represent brittle deform...
Noctis Labyrinthus is made up by inter-connected canyons with complex branched networks of extensio...
Noctis Labyrinthus is made up by inter-connected canyons with complex branched networks of extension...
Noctis Labyrinthus is a region located in the western part of Valles Marineris, bordering Syria Plan...
Abstract. - Noctis Labyrinthus shows a network of depressions on Mars. Its relief associates two mor...
Large extensional tectonic surface structures on Mars are investigated on the basis of image and top...
The Noachis-Sabaea region in the southern highlands preserves some of the oldest Martian crust. It r...
We have investigated the links between regional stress fields, the volcanic centers, rifts, graben a...
Noctis Labyrinthus is an intricate system of Late Hesperian and Early Amazonian linear troughs and r...
To determine whether the structural evolution of the Northern Cerberus Fossae (NCF) was dominated by...
Volcanic activity is widespread within the inner Solar system and it can be commonly observed on roc...
Research Aims - Study the tectonics features and the stress field in Noctis Labyrinthus. - Scrutiniz...
ResearchAims: 1. Study the tectonic features and the stress field in NoctisLabyrinthus. 2. Scruti...
Oral Presentation - 2nd Planetary Mapping and Virtual Observatory Workshop 1-3 July 2019, Domaine de...
Pit chains commonly occur along a bounding fault, allowing to infer a genetic relationship between ...
Noctis Labyrinthus (Mars) is characterized by many tectonic features, which represent brittle deform...
Noctis Labyrinthus is made up by inter-connected canyons with complex branched networks of extensio...
Noctis Labyrinthus is made up by inter-connected canyons with complex branched networks of extension...
Noctis Labyrinthus is a region located in the western part of Valles Marineris, bordering Syria Plan...
Abstract. - Noctis Labyrinthus shows a network of depressions on Mars. Its relief associates two mor...
Large extensional tectonic surface structures on Mars are investigated on the basis of image and top...
The Noachis-Sabaea region in the southern highlands preserves some of the oldest Martian crust. It r...
We have investigated the links between regional stress fields, the volcanic centers, rifts, graben a...
Noctis Labyrinthus is an intricate system of Late Hesperian and Early Amazonian linear troughs and r...
To determine whether the structural evolution of the Northern Cerberus Fossae (NCF) was dominated by...
Volcanic activity is widespread within the inner Solar system and it can be commonly observed on roc...
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