'Radiative cooling' presentation slideshows

Project X Reference Design Overview

Project X Reference Design Overview. Sergei Nagaitsev April 12, 2011. Reference Design. Reference Design Capabilities. 3 GeV CW superconducting H- linac with 1 mA average beam current. Flexible provision for variable beam structures to multiple users

615 views • 48 slides

The Weather that Makes the Dots

The Weather that Makes the Dots. TESSE 22 July 2008 Eric Kelsey Institute for the Study of Earth, Ocean and Space - UNH. Temperature Cycle over 7 Glacial Cycles. 600. Projected Concentration After 50 More Years of Unrestricted Fossil Fuel Burning. 500. 400. 300. 280. 260. 240.

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529 views • 34 slides

Simulations of Ly ? emission: fluorescence, cooling, galaxies

311 views • 30 slides

Diurnal circulations in Southern California

Diurnal circulations in Southern California. Mimi Hughes and Alex Hall. Outline. Motivation Experiment design Description of climatological diurnal winds Explanation for and impact of diurnal winds Model Validation Conclusions and future work. Motivation.

381 views • 27 slides

The general circulation of the atmosphere revisited

The general circulation of the atmosphere revisited. Kevin E. Trenberth NCAR Boulder, CO.

435 views • 26 slides

Stability and Cloud Development

Stability and Cloud Development. Please read Chapter 7 in Ahrens. Why is stability important?. Vertical motions in the atmosphere are a critical part of energy transport and strongly influence the hydrologic cycle

875 views • 25 slides

Cool Roofs Cool Cities Cool Planet

Cool Roofs Cool Cities Cool Planet. Ronnen Levinson, Ph.D . Acting Leader, Heat Island Group Environmental Energy Technologies Division Lawrence Berkeley National Lab RMLevinson@LBL.gov; tel. 510-486-7494; http://CoolColors.LBL.gov.

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Experimental Test of Radiative Cooling

348 views • 22 slides

Inner Planets (Part I)

530 views • 21 slides

The Sensitivity of a Simulated Supercell to Emulated Radiative Cooling beneath the Anvil

The Sensitivity of a Simulated Supercell to Emulated Radiative Cooling beneath the Anvil. Paul Markowski and Jerry Harrington Penn State University. Motivation.

286 views • 20 slides

Pan American Land Feedbacks on Precipitation

Pan American Land Feedbacks on Precipitation. Robert E. Dickinson (Gatech) Acknowledging contributions from Rong Fu (Gatech), and Guiling Wang (U Conn.).

362 views • 20 slides

CHAPTER 4: ATMOSPHERIC TRANSPORT

CHAPTER 4: ATMOSPHERIC TRANSPORT. Forces in the atmosphere: Gravity Pressure-gradient Coriolis Friction. to R of direction of motion (NH) or L (SH). Equilibrium of forces:. In vertical: barometric law In horizontal: geostrophic flow parallel to isobars. g p. P. v. P + D P.

524 views • 19 slides

Large-Eddy Simulation of a stratocumulus to cumulus transition as observed during the First Lagrangian of ASTEX

Large-Eddy Simulation of a stratocumulus to cumulus transition as observed during the First Lagrangian of ASTEX. cumulus penetrating stratocumulus, Bretagne, France. View on Delft, Johannes Vermeer, 1661. Stephan de Roode and Johan van der Dussen Delft University of Technology , Netherlands .

288 views • 17 slides

Simple tropical models and their relationship to GCMs

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New LEIF I3 Transnational access to ELISA Department of Physics and Astronomy

229 views • 11 slides

Frenk, Bauch Cole, Lacey

Wang 2000; Chandra obs of NGC4632. Frenk, Bauch Cole, Lacey. Hydrostatic Equilirium of Gas in DM potential wells. Radiative Cooling: I Collisional Excitation. v. T ~ 10 5 - 10 8 K. j. g. i. v. hv=E ij. Condition: En. of Elettrons E ? KT > D E lu. Collision rate.

233 views • 9 slides

Some considerations on radiative cooling

Some considerations on radiative cooling. V. Fafone , Y. Minenkov , I. Modena, A. Rocchi INFN Roma Tor Vergata. Working principle see LIGO?G080414?00?R. The cold source is imaged onto the centre of the test mass

152 views • 8 slides

AGN-controlled gas cooling in elliptical galaxies and galaxy clusters

AGN-controlled gas cooling in elliptical galaxies and galaxy clusters Christian R. Kaiser, Edward C.D. Pope, Georgi Pavlovski, Hans Fangohr, Southampton Philip N. Best, Edinburgh.

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Ch. 3 Radiation

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