'Energy transport' presentation slideshows

Chapter 10 Structure and Formation of Stars

1.68k views • 131 slides

Insights in stars, neutrino physics and in the Earth

564 views • 45 slides

Energy transport in Granular systems

Energy transport in Granular systems. Kiwing To Institute of Physics, Academia Sinica, Taipei. OUTLINE General properties of granular systems Diffusion in granular gas Temperature profile in granular shocks Mixing dynamics in rotating drum Summary & Discussions.

613 views • 43 slides

The Formation of Stars

The Formation of Stars. Chapter 11. Guidepost.

558 views • 41 slides

The Formation and Structure of Stars

Chapter 9. The Formation and Structure of Stars. The Big Picture. Stars exist because of gravity . Gravity causes interstellar material to collapse to form stars. Gravity determines how much energy stars generate. Gravity dictates how stars evolve and die.

983 views • 40 slides

482 views • 38 slides

Presented By: Iin Kurniasih (Jica, 14 November 2011)

CARBOHYDRATE. Presented By: Iin Kurniasih (Jica, 14 November 2011). Do you still remember, what is Macromolecul (Polymer)??. Monomer. Polymer. Polymerication. Natural Polymerization. Carbohydrate. To give us energy. Why do we need carbohydrates...???. Source of Energy. Second. First.

585 views • 36 slides

SOUND

SOUND. The basis for an understanding of sound, music and hearing is the physics of waves. Sound is a wave which is created by vibrating objects and propagated through a medium from one location to another. .

434 views • 28 slides

Adapting to Climate Change Programme

Adapting to Climate Change Programme. Mark Filley 2 March 2011. Overview. Adaptation. Mitigation : Protecting climate from society Adaptation : Protecting society from climate. IPCC Emission Scenarios High Medium Low

422 views • 27 slides

Sound Waves

Sound Waves. Vibration of a tuning fork. http://www.ndt-ed.org/EducationResources/HighSchool/Sound/hs_sound_index.htm. Compression (pressure higher). Rarefaction (pressure lower). Pressure Waves. Sound waves is usually analyzed from the point of view

1.02k views • 26 slides

KEEPING THE LIGHTS ON: STRATEGIES FOR COMPATIBILITY AND INTEROPERABILITY IN ELECTRIC POWER NETWORKS

KEEPING THE LIGHTS ON: STRATEGIES FOR COMPATIBILITY AND INTEROPERABILITY IN ELECTRIC POWER NETWORKS. SURVIVABILITY OF COMPLEX NETWORKS. Ira Kohlberg Kohlberg Associates, Inc. South Shore Road Reston, VA 20190. October 27, 2011.

425 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

Modeling Multiphase Flow in Variably Saturated Media

Modeling Multiphase Flow in Variably Saturated Media. For: BAE 558 By: Kate Burlingame 5/7/07. Introduction.

667 views • 24 slides

369 views • 22 slides

Turbulent Combustion, Conservation Equations Closure

Turbulent Combustion, Conservation Equations Closure. Turbulence and its effects on mass, momentum, species and energy transport Practical devices involve turbulent flows specifically promoted by the design engineer to obtain efficient mixing, preheating and volumetric reaction rates.

510 views • 21 slides

Solar interior

Solar interior. Solar interior Standard solar model Solar evolution, past, present and future. The solar interior. Solar interior cannot be directly observed, information is from: Theoretical models Helioseismology Solar neutrinos.

760 views • 21 slides

Integrated Modeling and Simulations of ITER Burning Plasma Scenarios

Integrated Modeling and Simulations of ITER Burning Plasma Scenarios. C. E. Kessel, R. V. Budny, K. Indireshkumar, D. Meade Princeton Plasma Physics Laboratory IEA Large Tokamak Workshop (W60) Burning Plasma Physics and Simulation Tarragona, Spain July 4-5, 2005.

634 views • 14 slides

Benjamin Schenkel (bschenkel@fsu.edu) and Robert Hart 2012 AMS Annual Meeting

Quantifying the Environmental Memory of Tropical Cyclones: Lingering Footprint or Climate Amnesia?. Benjamin Schenkel (bschenkel@fsu.edu) and Robert Hart 2012 AMS Annual Meeting Department of Earth, Ocean, and Atmospheric Science The Florida State University.

280 views • 13 slides

Recent Progress on QPS D. A. Spong, D.J. Strickler, J. F. Lyon, M. J. Cole, B. E. Nelson, A. S. Ware, D. E. Williamson

Recent Progress on QPS D. A. Spong, D.J. Strickler, J. F. Lyon, M. J. Cole, B. E. Nelson, A. S. Ware, D. E. Williamson. Improved coil design (see recent Stellarator News article) New flux surface optimization target Reduced island size Invariance of surface shape with b

346 views • 12 slides

The Arrival of the Age of LNG

The Arrival of the Age of LNG. Andrei V. Belyi University of Eastern Finland andrey.belyy@uef.fi. Towards diversified gas trading options. Gas chain: virtual trade and physical flows Volumes: l arge pipelines/ L NG, and small pipeline s/ LNG

191 views • 10 slides