Physics – Condensed Matter – Disordered Systems and Neural Networks
Scientist
Physics
Condensed Matter
Disordered Systems and Neural Networks
Scientist
Département de Physique, Université de Montréal, Montréal, PQ, H3C 3J7, Canada Universite de Montreal, Montreal, QC, Canada;
Physics, University of Montreal, Montreal, QC, Canada;
Département de Physique, Universitéde Montréal, Montréal, Quebec, Canada
U. Montreal
Département de Physique, Université of Montréal
Departement de Physique Universite de Montreal, C.P. 6128, succ. centre-ville, Montreal, QC H3C 3J7, Canada
HAO / NCAR
Montreal, Universite; Mont-Megantic, Observatoire, Montreal, Canada
Universite de Montreal
High Altitude Observatory, Boulder, CO
National Center for Atmospheric Research, Boulder, CO, US
HAO / NCAR, POBox 3000, Boulder, CO 80307-3000, USA Altitude Observatory, National Center for Atmospheric Research PO Box 3000, Boulder, CO 80307, USA de Physique, Université de Montréal, Montreal, Quebec, Canada
Universite de Montreal, Canada
HAO
HAO, NCAR
High Altitude Observatory, National Center for Atmospheric Research, P.O. Box 3000, Boulder, CO 80307 de Physique, Université de Montréal, Montréal, QC, H3C 3J7, Canada.
High Altitude Observatory, National Center for Atmospheric Research, P.O. Box 3000, Boulder, CO 80307-3000
Universite de Montreal, Department of Physics, Montreal, QC H3C3J7, Canada de Physique, Université de Montréal, QC, H3C 3J7, Canada
Département de Physique, Université de Montréal, C.P. 6128, Succursale Centre-ville, Montréal, QC H3C3J7 Canada Altitude Observatory, National Center for Atmospheric Research, P.O. Box 3000, Boulder, CO. 80307-3000, USA
Universite de Montreal, Montreal, QC, Canada
Department of Physics, University of Montreal, Montreal, QC, Canada
A Model for the Total Solar Irradiance Based on Active Region Decay
A Monte Carlo Approach for Studying Microphases Applied to the Axial Next-Nearest-Neighbor Ising and the Ising-Coulomb Models
A New Avalanche Model for Solar Flares
Abnormal cycles from normal dynamos (Invited)
Absorption of p-Modes by Slender Magnetic Flux Tubes and p-Mode Lifetimes
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