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The top documents tagged [h simulations]
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Why observe M dwarfs? M9V M6V M3V M1V Due to current technical limits (~ 1m/s ---), the reflex velocities of earth-mass planets in the HZ are only observable
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Magnetic thin films: from basic research to spintronics Christian Binek 11/18/2005 Physics 201H Why thin films Length (and time) scales determine the physics
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Colloque GRETSI, Paris, 8-11 septembre 2003 Sur la Décomposition Modale Empirique P. Flandrin (Cnrs - Éns Lyon) et P. Gonçalvès (Inrialpes)
103 views
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Three Species Collisionless Reconnection: Effect of O + on Magnetotail Reconnection Michael Shay – Univ. of Maryland Preprints at: shay/papers
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The Influence of the Downstream State on ET: Danielle and Earl (1998) Ron McTaggart-Cowan John Gyakum, Peter Yau
293 views
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Project AIST-CAMVis Meeting Agenda Start at 2:00 PM EST on March 27, 2009 Items: introductions/warm-up activities (~5 minutes) project overview (3~5 minutes)
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Thermal flows along the south-eastern Adriatic Maja Telišman Prtenjak & Sanda Đivanović Department of Geophysics, Faculty of Science, University of Zagreb,
213 views
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Folding @ Home - Distributed Parallel Protein folding Chris Garlock
232 views