Sand transport and geomorphology on the surface of Mars

Reproducing sediment transport conditions on Mars, P. Claudin and co-workers show that at very low pressure, a new grain movement regime appears, compatible with the observations made on the Red Planet.

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PRE Editors’ Suggestion - Prediction of frequencies in thermosolutal convection from mean flows

S. E. Turton, L. S. Tuckerman and D. Barkley Phys. Rev. E 91, 043009 – Published 14 April 2015. Motivated by studies of the cylinder wake, in (...) 

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PRL editors’ suggestion about wave resonant absorption

Perfect Resonant Absorption of Guided Water Waves by Autler-Townes Splitting L.-P. Euvé, K. Pham, R. Porter, P. Petitjeans, V. Pagneux, and A. (...) 

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Practical information

Laboratoire : 01 40 79 45 22
Directeur : Damien Vandembroucq
Codirecteur : Philippe Petitjeans
Administratrice : Frédérique Auger (01 40 79 45 22)
Gestionnaire : Claudette Barez (01 40 79 58 53)
Courriel : dir (arobase) pmmh.espci.fr