Fluid Dynamics Research Evan Lemley Engineering and Physics Department Research Roundtable Dec. 5, 2008.
Parametrization of the planetary boundary layer (PBL) Martin Köhler & Anton Beljaars (rooms 108/114) Introduction.Martin Surface layer and surface fluxes.Anton.
November 18 AP Physics. In: Objective: To begin our study of fluid dynamics Equation of continuity Bernoullis equation Success criteria: Be able to use.
Solar Energy/ Energy Saving Getting the best out of FITs / RHI Save Money? and the Planet? Is it as simple as that? - what are the catches? 1 Reach Within.
Pg 1 of xx AGI STK for Live Forecasted Weather Tony Faulds, President, Trinnovations.
From protostellar cores to disk galaxies - Zurich - 09/2007 S.Walch, A.Burkert, T.Naab Munich University Observatory S.Walch, A.Burkert, T.Naab Munich.
Accretion Disks Prof. Hannah Jang-Condell. Accretion Disks Galaxy: M81 Protoplanetary Disk: AB Aurigae Neutron Star (artists conception) (Giovanni Benintende)(M.
Atmospheric Effects on Flight Review 1 ATC Chapter 7.
JOINT SERVICE PARACHUTE CENTRE NETHERAVON. CANOPY CONTROL.
1 LifePaths Evaluating Earnings Replacement After Retirement: The Evolution of Retirement Income Adequacy in Canada Kevin D. Moore Statistic Canadas Modelling.
TURBULENCE Is uncomfortable But not dangerous. Why the wings move To make it smoother for you To make it easier for the wings.
Implications of Tidal Phasing for Power Generation at a Tidal Energy Site Brian Polagye and Jim Thomson Northwest National Marine Renewable Energy Center.