'Energy release' diaporamas de présentation

U. Washington Tsunami Certificate Program Course 2: Tsunami Warning Systems Session 7 Tsunami Warning Data Processing Ju

U. Washington Tsunami Certificate Program Course 2: Tsunami Warning Systems Session 7 Tsunami Warning Data Processing July 28, 2007 1:15-2:45pm. Outline. Seismic Data Processing Seismic Basics Seismic Processing Architecture Sea Level Processing GIS Data bases Forecasting Techniques

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Finite Elements and Fracture Mechanics

Finite Elements and Fracture Mechanics. Leslie Banks-Sills The Dreszer Fracture Mechanics Laboratory Department of Solid Mechanics, Materials and Systems Tel Aviv University. ISCM-1 5 , October, 2003. Outline. Introduction to fracture mechanics (homogeneous material).

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Earthquakes

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Bias Fields and Pattern Complexity

Bias Fields and Pattern Complexity. M.E. Glicksman Allen S. Henry Professor of Engineering Mechanical & Aerospace Engineering Dept. Florida Institute of Technology, Melbourne, FL. Presentation at the UCLA Institute for Pure & Applied M athematics Los Angeles, CA November 13, 2012.

534 views • 42 slides

Hydrogen burning under extreme conditions

Hydrogen burning under extreme conditions. Scenarios:. Hot bottom burning in massive AGB stars (> 4 solar masses) . (T 9 ~ 0.08). Nova explosions on accreting white dwarfs. (T 9 ~ 0.4). X-ray bursts on accreting neutron stars. (T 9 ~ 2). accretion disks around low mass black holes ?

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Using (LiFepo4) Lithium Iron Phosphate Batteries in Aviation

Using (LiFepo4) Lithium Iron Phosphate Batteries in Aviation . Engine Starting Batteries. Destructive Testing. Why is LiFePo4 safe ?. Impedance Values .. 19 mohms. 10.5mohms. Low Impedance .. 10.8 mohms. SLA discharge curve low C-rate. Lithium discharge curves, hi C rate.

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The Science of Nuclear Reactors and the Regulatory Framework

The Science of Nuclear Reactors and the Regulatory Framework. A Presentation to Wake Forest University School of Physics September 12, 2002 M.T. Cash. Historical Perspective . Science and Law are often best understood in a historical perspective

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Magnetohydrodynamics of pulsar winds and plerions

Magnetohydrodynamics of pulsar winds and plerions. Yuri Lyubarsky. Ben-Gurion University, Israel. Pulsar magnetosphere. Pulsar wind. Pulsar wind nebula. electro-magnetic fields. j. j. B. v. v. v. j. j. v. v. B. v. v. j. j. v. The hoop stress. j. F. B.

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SuperWIMP Dark Matter

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Chemical Reactions & Enzymes

Chemical Reactions & Enzymes. Chemical Reactions. A change of one set of chemicals into another Can be slow or fast Require collisions between molecules Involves changes in chemical bonds. Chemical Reactions. Reactants: elements or compounds that enter into a chemical reaction

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Flare Particle Acceleration in Large-scale Magnetic Fields

Flare Particle Acceleration in Large-scale Magnetic Fields. Peter Cargill Imperial College With thanks to Rim Turkmani, Loukas Vlahos, Heinz Isliker and Klaus Galsgaard, ISSI October 5, 2006. The context: solar flares. Release of 10 32 ergs in 1000 sec.

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Photosynthesis vs. Cellular Respiration

Photosynthesis vs. Cellular Respiration. Cellular Energy & Biochemistry Chapter 5. Photosynthesis (autotrophs) CO 2 + H 2 O C 6 H 12 O 6 + O 2 Carbon dioxide Glucose & & water oxygen Respiration (heterotrophs). Energy Cycle. Photosynthesis. Respiration.

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Physics 222 UCSD/225b UCSB

Physics 222 UCSD/225b UCSB. Lecture 2 Weak Interactions Intro and Overview V-A nature of weak current Nuclear beta decay. Weak Interactions. Some of the most surprising & mysterious phenomena in particle physics: Violates fundamental symmetries C, T, P, CP

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The Cleaner World Through Pyro Thermic Reaction

The Cleaner World Through Pyro Thermic Reaction. Introduction Time Lapse Technology Comparisons New Era Treatment Zones Power Process Maintenance. Process Flow Diagram Desalination Operator Controls Construction Plant List Mobile Plant Contact Details. 1. 8. 9. 2. 3. 10.

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Evolution of H a Flare Kernels and Energy Release

Evolution of H a Flare Kernels and Energy Release. Ayumi ASAI Nobeyama Solar Radio Observatory, NAOJ 6 th Solar-B Science Meeting November 11, 2005 @Kyoto. What can we learn from Flare Kernels/Ribbons?. 2001-Apr-10 flare (Hida Obs.). Evolution of flare ribbons

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ISSI team : The Role of Spectroscopy and Imaging Data in Understanding Coronal Heating

ISSI team : The Role of Spectroscopy and Imaging Data in Understanding Coronal Heating. A.O. Benz, E. Buchlin, P.J. Cargill, S. Galtier, J. A. Klimchuk, E. Landi, H.E. Mason, S. Parenti, S. Patsourakos, H. Peter, F. Reale, D. Spadaro, J. Sylwester. www.issibern.ch/teams/Spectdata/. Topics:.

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RESPIRATION & OXIDATION

RESPIRATION & OXIDATION. GLYCOLYSIS. Step 1: Phosphorylation: Glucose + 2ATP ? Fructose 1,6-diphosphate + 2ADP Step 2: Splitting 6C sugar to 2 x 3C sugars: Fructose 1,6-diphosphate ? 2 Glyceraldehyde Phosphate Step 3: Energy release:

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RESIK_weekly

RESIK_weekly. The launch of CORONAS_F. The CORONAS-F launch took place early morning on 31 July 2001 from Plesetsk Cosmodrome. Below is a schematic map of the Plesetsk range (more info availabla on http://www.russianspaceweb.com/plesetsk.html). Some launch photos.

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XRBs in 2d: Hydrodynamic Modeling of a 4 He Burst Prior to Peak Light

XRBs in 2d: Hydrodynamic Modeling of a 4 He Burst Prior to Peak Light Chris Malone 1 , A. S. Almgren 2 , J. B. Bell 2 , A. J. Nonaka 2 , M. Zingale 1 1 Dept. of Physics and Astronomy, SUNY Stony Brook, 2 CCSE / LBNL.

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