'Energy flux' presentation slideshows

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Internal Tides, Mixing and the Bottom Boundary Layer

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).

By wilona
(84 views)

Record the definitions for these key terms in your science notebooks

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.

By istas
(81 views)

Latent heat flux

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

By dragon
(558 views)

Coupling between magnetospheric and auroral ionospheric scales during space weather events

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.

By taber
(86 views)

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

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.

By alaula
(264 views)

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

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

CE 394K.2 Hydrology, Lecture 3 Water and Energy Flow. Literary quote for today:. “If I should die, think only this of me;    That there's some corner of a foreign field  That is for ever England. ” Rupert Brooke, English poet, “The Soldier”

By hina
(133 views)

Bare rock model

Bare rock model

Bare rock model. Assumptions Amount of energy coming into the planet from sunlight is equal the amount of energy leaving the earth as IR. F in = F out No atmosphere. Energy Balance of a Bare Rock. T earth = 259 K = -14° C = 6°F. How much solar energy reaches the Earth?.

By aric
(562 views)

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

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.

By phuc
(107 views)

KINETIC THEORY AND MICRO/NANOFLUDICS

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.

By mitch
(129 views)

Ron Remillard Kavli Institute for Astrophysics and Space Research

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.

By gilda
(153 views)

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

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

By phila
(98 views)

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

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

Investigation of the energy conversion in the auroral magnetosphere with conjugated CLUSTER and FAST data. O. Marghitu (1, 3), M. Hamrin (2), B.Klecker (3) (1) Institute for Space Sciences, Bucharest, Romania (2) Physics Department, Umeå University, Umeå, Sweden

By oded
(101 views)

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

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

By orrick
(94 views)

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

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

Magnetic field and flavor effects on the neutrino fluxes from cosmic accelerators. WIN 2011 January 31-February 5, 2011 Cape Town , South Africa Walter Winter Universität Würzburg. TexPoint fonts used in EMF: A A A A A A A A. Contents. Introduction

By rod
(102 views)

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

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

Magnetic field and flavor effects on the neutrino fluxes from cosmic accelerators. NUSKY 2011 June 20-24, 2011 ICTP Trieste, Italy Walter Winter Universität Würzburg. TexPoint fonts used in EMF: A A A A A A A A. Contents. Introduction Simulation of sources

By elia
(142 views)

TODAY: SIT ANYWHERE YOU WANT TODAY !

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!

By niabi
(206 views)

Conversations with the Earth Tom Burbine tburbine@framingham

Conversations with the Earth Tom Burbine tburbine@framingham

Conversations with the Earth Tom Burbine tburbine@framingham.edu. Albedo. Albedo is the reflectivity of the surface. Albedo goes from 0 to 1 High albedo – reflective Low albedo - absorbing. Planetary Energy Balance Equation. Exercise 5 1) What does energy balance mean?.

By krikor
(80 views)

brightnightgallery/

brightnightgallery/

From a location with little light pollution (+ some camera tricks). http://www.brightnightgallery.com/. Lecture 8. ASTR 111 – Section 002. Mid-term evaluations/grades. Required for Freshman and Sophomores Due by October 17 th I entered mid-term grades for everyone

By elkan
(70 views)

Fitness vs. Fatness Debate

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

By kimberly
(157 views)

Physical-Space Decimation and Constrained Large Eddy Simulation

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)

By elam
(161 views)

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