Early Mars climate near the Noachian-Hesperian boundary: Independent evidence for cold conditions from basal melting of the south polar ice sheet (Dorsa Argentea Formation) and implications for valley network formation

Fastook, J.L. / Head, J.W. / Marchant, D.R. / Forget, François / Madeleine, J.-B. - 2015

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Lien externe vers le document:

https://hal.archives-ouvertes.fr/hal-01111698

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Auteur(s):

Fastook, J.L. / Head, J.W. / Marchant, D.R. / Forget, François / Madeleine, J.-B. - 2015

Editeur:

HAL CCSD

Contributeur:

Computer Science, University of Maine, 223 Neville Hall, Orono, ME 04469, United States

Department of Geological Sciences, Brown University, Providence, RI 02912, United States

Department of Earth Sciences, Boston University, Boston, MA 02215, United States

Laboratoire de Météorologie Dynamique (LMD) ; CNRS - INSU - Polytechnique - X - École normale supérieure - Paris (ENS Paris) - Université Pierre et Marie Curie - Paris 6 (UPMC)

Langue:

ANGLAIS

Candidats descripteurs:

[SDU.STU.GL] Sciences of the Universe/Earth Sciences/Glaciology

[SDU.STU.PL] Sciences of the Universe/Earth Sciences/Planetology

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Early Mars climate near the Noachian-Hesperian boundary: Independent evidence for cold conditions from basal melting of the south polar ice sheet (Dorsa Argentea Formation) and implications for valley network formation

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