Geophysical Investigation of Noctis Volcano on (equatorial) Mars using MOLA, MARSIS, and Numerical Plume Modelling.

Most Martian volcanoes have been fed by stationary mantle plumes, leading to the buildup of large shield edifices. A recent investigation on a poorly mapped region, located between equatorial Noctis Labyrinthus and Valles Marineris, revealed a heavily

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Published
2025-11-03
DOI
https://doi.org/10.22541/essoar.176218868.89744519/v1
Primary Topic
Planetary Science and Exploration
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article
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article

Geophysical Investigation of Noctis Volcano on (equatorial) Mars using MOLA, MARSIS, and Numerical Plume Modelling.

Adrien Broquet, Faris Beg
Planetary Science and Exploration
article

Geophysical Investigation of Noctis Volcano on (equatorial) Mars using MOLA, MARSIS, and Numerical Plume Modelling.

Adrien Broquet, Faris Beg
article en

Abstract

Most Martian volcanoes have been fed by stationary mantle plumes, leading to the buildup of large shield edifices. A recent investigation on a poorly mapped region, located between equatorial Noctis Labyrinthus and Valles Marineris, revealed a heavily

Deutsches Zentrum für Luft- und Raumfahrt e. V. (DLR) (DE)
Openalex Percentile: Top 78%
Planetary Science and Exploration
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Geophysical Investigation of Noctis Volcano on (equatorial) Mars using MOLA, MARSIS, and Numerical Plume Modelling. — Adrien Broquet, Faris Beg · (2025) | TGRS Research Map | TGRS