Constraining Martian mineralogical compositions using hyperspectral images

Constraining the martian surface composition using hyperspectral images is a difficult task due to the high diversity of the potential minerals. Here we present hypothesis, rationale, and results in the Syrtis Major region.

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Traitement du signal et de l'image [eess.SP]

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https://hal.science/hal-04240681

Soumis le : vendredi 13 octobre 2023-11:48:23

Dernière modification le : lundi 30 septembre 2024-13:58:25

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hal-04240681 , version 1 (13-10-2023)

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HAL Id : hal-04240681 , version 1

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Frédéric Schmidt, Sébastien Bourguignon, Stéphane Le Mouélic, Nicolas Dobigeon, Erwan Tréguier. Constraining Martian mineralogical compositions using hyperspectral images. 43rd Lunar and Planetary Science Conference, Lunar and Planetary Institute (LPI), Mar 2012, Texas, United States. pp.(electronic medium). ⟨hal-04240681⟩

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