'Radiation field' diaporamas de présentation

MA inzer MI krotron MAMI : A precision accelerator for nucleon structure investigations

MA inzer MI krotron MAMI : A precision accelerator for nucleon structure investigations. Kurt Aulenbacher Reactor Training Course U-South Carolina May, 28, 2008. l : Wavelength. d: object size. d:. required resolution. l < d. l :. Lightwaves and particle waves. l :.

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GRAVITATIONAL RADIATION IN ULTRAPLANCKIAN COLLISIONS

GRAVITATIONAL RADIATION IN ULTRAPLANCKIAN COLLISIONS. Theodore Tomaras University of Crete. 7 th Crete Regional Meeting on String Theory Kolymbari , 16-23 June 2013 . OBSERVATION: About 12% initial-state energy losses in e+e - collisions at Z 0

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Radiation Protection in Laboratory work

Radiation Protection in Laboratory work. Mats Isaksson, prof. Department of radiation physics , GU mats.isaksson@radfys.gu.se. Fundamental principles (ICRP). Justification Optimisation Application of dose limits. Fundamental principles (ICRP). Justification

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Irradiation Facilities at the SPS North Experimental Area Helmut Vincke on behalf of RP

Irradiation Facilities at the SPS North Experimental Area Helmut Vincke on behalf of RP. Content. CERF TCC2 irradiation facility CERF++. Hadron beam. CERN-EU high-energy Reference Field (CERF) facility. Detectors. CERF exists since 1992. Concrete shielding.

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CHANNEL MODEL for INFOSTATIONS

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RDCH 702 Lecture 7: Radiation Reactions: Dosimetry and Hot Atom Chemistry

RDCH 702 Lecture 7: Radiation Reactions: Dosimetry and Hot Atom Chemistry. Readings: Reading: Modern Nuclear Chemistry, Chap. 17; Nuclear and Radiochemistry, Chap. 6, Chap 11.C. Interaction of radiation with matter Neutron, positive ions, electrons, photons Dosimetry

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Hawking radiation as tunneling

Hawking radiation as tunneling. Baocheng Zhang Wuhan institute of Physics and Mathematics Chinese Academy of Sciences. The coauthors : Qing-yu Cai Ming-sheng Zhan. Introduction. Backgroud Hawking radiation as tunneling through quantum horizon. Backgroud. Hawking radiation.

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Luca Belluzzi 1 and Javier Trujillo Bueno 2

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Atomic Processes in Gaseous Nebulae

Andri Prozesky MSc. Atomic Processes in Gaseous Nebulae. Outline. Introduction Atomic Processes Modelling Nebulae Why is this New? Why is this Important? Results Future Work. Introduction. Introduction. Atomic Processes - Radiative. Bound-bound processes. Absorption

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Models for heat and moisture transport in a microwave oven

Models for heat and moisture transport in a microwave oven. Andrew Hill & Prof. C.J. Budd University of Bath, UK Greg Hooper CCFRA, UK. Faraday CASE award. Microwave oven. Thermal image of surface of food after 5 minutes heating. Aims.

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Concept of the LORD experiment

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Paul Scherrer Institut

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MASSIVE STARS IN COLLIDING WIND SYSTEMS: THE GLAST PERSPECTIVE

MASSIVE STARS IN COLLIDING WIND SYSTEMS: THE GLAST PERSPECTIVE. Anita & Olaf Reimer, HEPL & KIPAC, Stanford University 1 st GLAST Symposium, Stanford, Febr. 2007. Courtesy: J. Pittard. -Anita Reimer, HEPL/KIPAC Stanford University -. Massive Stars.

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Equation of state and HEDP

Equation of state and HEDP. Steven Rose Clarendon Laboratory University of Oxford and AWE, Aldermaston UK. Plasma conditions achieved with high-power lasers. long-pulse (nsec) laser short-pulse (psec) laser combined long and short-pulse laser. Energy exchange in a laser-produced plasma.

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Diamonds in CDF

Diamonds in CDF. Peter Dong, UCLA Ricardo Eusebi, FNAL Anna Sfyrla, Geneva Rick Tesarek, FNAL Rainer Wallny, UCLA With much help from Jonathan Lewis (FNAL) and the PPD EE Department Silicon Workshop II Friday, May 12, 2006. Why do we want diamonds?.

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Parity

Let us examine the parity operator (P) and its eigenvalues. The parity operator acting on a wavefunction is defined by: P Y (x, y, z) = Y (-x, -y, -z) P 2 Y (x, y, z) = P Y (-x, -y, -z) = Y (x, y, z) Therefore P 2 = I and the parity operator is unitary.

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Objectives

Objectives. The objectives of the workshop are to stimulate discussions around the use of 3D (and probably 4D = 3D+time) realistic modeling of canopy structure to be used in remote sensing applications .

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GIF++ Technical specifications

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Single Pass SASE Free Electron Lasers A potential 4th generation light source

Linac 0. Linac 1. Linac 2. Linac 3. RF Gun. Undulator. Bunch Compressor 1. Bunch Compressor 2. To Photon Lines. To Existing Linac. To B Factory. 1 km. Single Pass SASE Free Electron Lasers A potential 4th generation light source. EECS 213 Final Report Kevin Bowers

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Computed Verification of light and Radiation field size Superimposition on Cobalt-60

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