'Energy flux' diaporamas de présentation

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1.39k views • 127 slides

TODAY: SIT ANYWHERE YOU WANT TODAY !

Tuesday Sep 21st. TODAY: SIT ANYWHERE YOU WANT TODAY !. ANNOUNCEMENTS:. REMINDER: SELF TEST & RQ-3 are DUE THIS WEEK! RQ-3 will be cut off Thursday ( Sep 23rd ) 30 minutes before class!

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KINETIC THEORY AND MICRO/NANOFLUDICS

KINETIC THEORY AND MICRO/NANOFLUDICS. Kinetic Description of Dilute Gases Transport Equations and Properties of Ideal Gases The Boltzmann Transport Equation Micro/Nanofludics and Heat Transfer. Kinetic Description of Dilute Gases.

975 views • 74 slides

Fitness vs. Fatness Debate

China Medical University, Lifu Teaching Building Taichung, Taiwan; April26 th 2011. Fitness vs. Fatness Debate. Eric.Ravussin@pbrc.edu. Obesity Facts. Over 66% of Americans are overweight or obese Number of Obese American adults rose to 33% Over last decade alone an increase of

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Physical-Space Decimation and Constrained Large Eddy Simulation

Physical-Space Decimation and Constrained Large Eddy Simulation. Shiyi Chen College of Engineering, Peking University Johns Hopkins University. Collaborator: Yi-peng Shi (PKU) Zuoli Xiao (PKU&JHU) Suyang Pei (PKU)

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CE 394K.2 Hydrology, Lecture 3 Water and Energy Flow

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Scaling of Ion Beams from Plasma Focus in Various Gases S Lee 1,2,3 & S H Saw 1,2

Scaling of Ion Beams from Plasma Focus in Various Gases S Lee 1,2,3 & S H Saw 1,2 1 INTI International University, 71800 Nilai, Malaysia 2 Institute for Plasma Focus Studies, Chadstone, VIC 3148, Australia 3 University of Malaya, Kuala Lumpur, Malaysia

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Magnetic field and flavor effects on the neutrino fluxes from cosmic accelerators

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Ron Remillard Kavli Institute for Astrophysics and Space Research

XIV Advanced School on Astrophysics Topic III: Observations of the Accretion Disks of Black Holes and Neutron Stars. Ron Remillard Kavli Institute for Astrophysics and Space Research Massachusetts Institute of Technology http://xte.mit.edu/~rr/XIVschool_III.1.ppt.

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Magnetic field and flavor effects on the neutrino fluxes from cosmic accelerators

441 views • 32 slides

Maxim Barkov University of Leeds, UK, Space Research Institute, Russia

Blandford-Znajek mechanism and GRB jets. Serguei Komissarov University of Leeds, UK. Maxim Barkov University of Leeds, UK, Space Research Institute, Russia. TexPoint fonts used in EMF. Read the TexPoint manual before you delete this box.: A A. Plan of this talk.

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Conversations with the Earth Tom Burbine tburbine@framingham

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Record the definitions for these key terms in your science notebooks

Producer : An autotroph , makes up the first trophic level of an ecosystem. Supports all other levels. Usually a phosynthetic organism. Hetertroph : An organism that obtains organic food molecules by eating other organisms or their by products.

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Expected Loads on ICRH Antenna A. Loarte with input from M. Sugihara, M. Shimada, and many others

Expected Loads on ICRH Antenna A. Loarte with input from M. Sugihara, M. Shimada, and many others. Radiation loads to First Wall Plasma Fluxes to First Wall in steady state and ELMs and scaling in ICRH shadow Plasma Fluxes to First Wall associated with ICRH heating and scaling in ICRH shadow

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Coupling between magnetospheric and auroral ionospheric scales during space weather events

Coupling between magnetospheric and auroral ionospheric scales during space weather events. M. ECHIM (1,2), M. ROTH(1) and J. DE KEYSER(1) (1) Belgian Institute for Space Aeronomy, Brussels, Belgium (2) Institute for Space Sciences, Bucharest, Romania. Outline of the talk.

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Joachim Saur, Timo Grambusch , Stefan Duling University of Cologne, Germany

Moon-Planet and Exoplanet -Star Couplings: Common Electrodynamic Interaction Mechanisms Throughout the Universe. Joachim Saur, Timo Grambusch , Stefan Duling University of Cologne, Germany. Magnetic coupling: Satellite-planet. Clarke et al., 2002. Magnetic coupling : Planet-star.

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Internal Tides, Mixing and the Bottom Boundary Layer

Internal Tides, Mixing and the Bottom Boundary Layer. James Girton and Eric Kunze APL/UW and Univ. Victoria. Monterey Canyon Internal Tides. From Kunze, Rosenfeld, Carter, and Gregg (JPO 2002). Beams and Flux Divergence. From Kunze, Rosenfeld, Carter, and Gregg (JPO 2002).

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Bare rock model

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O. Marghitu (1, 3), M. Hamrin (2), B.Klecker (3)

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Latent heat flux

Water flux Evaporation rate, E (mm/day). Energy flux Latent heat flux (W/m 2 ), H l. Latent heat flux. r = 1000 kg/m 3 l v = 2.5 MJ/kg. 28.94 W/m 2 = 1 mm/day. Area = 1 m 2. Energy Balance of Earth. 70. 20. 100. 6. 6. 26. 4. 38. 15. 19. 21. Sensible heat flux 7

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