1. The Big from the Small How particle theory advances in the last century allow us to understand the origin and structure of the universe on the largest scales.Byron Philhour,…

1. Dark Energy & Dark Matter Shamit Kachru (Stanford and SLAC)LASER, Stanford, August 2012Tuesday, August 7, 2012 2. Introduction It was the burden of Newton to teach…

Slide 1Cosmology GREAT WEB RESOURCE: http://www.astro.ucla.edu/~wright/cosmolog.htm http://www.astro.ucla.edu/~wright/cosmolog.htm Contains a cosmological calculator A tutorial…

Slide 1The Disk Dynamo: How to drive a dynamo in an accretion disk through shear and a local instability Collaborators: Jungyeon Cho --- Chungnam U. Dmitry Shapovalov ---…

Slide 1GEOG 361 Sedimentary & Ecological Flows: Process, Form and Management Lecture 3: A lovely Flan Lecture 3: Alluvial Fans http://www.geog.ucsb.edu/~jeff/wallpaper2/page2.html…

1.Many-Task Computing Tools forMultiscale ModelingDaniel S. Katz ([email protected])Senior Fellow, Computation Institute (Universityof Chicago & Argonne National Laboratory)…

1.1.1ASTRONOMICAL MEASUREMENTS2. Where Are You?To find our place among the stars, we will zoom out from a familiar scene, to the largest scales of the universe.Each picture…

Establishing homogeneity of the universe in the shadow of dark energy Chris Clarkson Astrophysics, Cosmology & Gravity Centre, and, Department of Mathematics and Applied…

Atmospheric Sciences tools are more fully described in the section on Paleoclimate. A full understanding of Precipitation Processes requires detailed knowledge of cloud microphysical…

Slide 1Ensemble Forecasting of High-Impact Weather Richard Swinbank with thanks to various, mainly Met Office, colleagues High-Impact Weather THORPEX follow-on project meeting,…