'Auger' diaporamas de présentation

PIERRE AUGER OBSERVATORY

PIERRE AUGER OBSERVATORY. Education and Outreach. Gregory Snow University of Nebraska DPF 2011, Providence, Rhode Island 9-13 August 2011. Outline. Introduction to the Auger Observatory and Goals of the Education and Outreach Task Efforts in Mendoza Province, Argentina

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The Auger Project

The Auger Project. Seeking the Source of Ultra High Energy Cosmic Rays. A New Window on Astronomy. Generic Colloquium Slides Prepared December 11, 1997. David F. Nitz University of Michigan. Outline. Introduction Historical Perspective CR Spectrum Extensive Air Showers Array layout

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The quest for UHECR and ? from space

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The improvement in efficiency of the cell arises from its potential ( i) to absorb below bandgap energy photons and th

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Scientific need, design and construction of a muon telescope for the Pierre Auger Observatory

Scientific need, design and construction of a muon telescope for the Pierre Auger Observatory

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Electron Beam MicroAnalysis- Theory and Application Electron Probe MicroAnalysis - (EPMA)

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Cosmic Ray in the Northern Hemisphere: Results from the Telescope Array Experiment

Cosmic Ray in the Northern Hemisphere: Results from the Telescope Array Experiment. Charlie Jui University of Utah DPF, Brown University Aug. 11, 2011 . Telescope Array Collaboration.

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DOE Annual Program Review Pierre Auger Project (E881) Peter O. Mazur

DOE Annual Program Review Pierre Auger Project (E881) Peter O. Mazur. Czech Republic France Germany Italy Netherlands Poland Portugal Slovenia Spain United Kingdom. Argentina Australia Brasil Bolivia* Mexico USA Vietnam*

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Fermilab Program Advisory Committee

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NNN05 Next Generation of Nucleon Decay and Neutrino Detectors 7-9 April 2005, Aussois, Savoie, France

NNN05 Next Generation of Nucleon Decay and Neutrino Detectors 7-9 April 2005, Aussois, Savoie, France. detector considerations for neutrino physics Tony Wright, Electron Tubes Limited. light detection: large solid angle large cathode area long operating life high gain well-resolved SER

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An Ultra-High-Energy Cosmic Ray Experiment

An Ultra-High-Energy Cosmic Ray Experiment. Glenn Sembroski QuarkNet Summer Workshop July 24,2012. The Big Question Which has become the Big Mystery. Where do Cosmic Rays come from? A multi-part question. i.e. Lots of small mysteries Different answers for different energy regimes

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Electron Spectroscopy for chemical analysis, ESCA and Auger Electron Spectroscopy, AES,

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The Tianshan Radio Experiment for Neutrino Detectio n

The Tianshan Radio Experiment for Neutrino Detectio n. Olivier Martineau-Huynh NAOC G&C lunch talk May 28, 2014. Milky Way over 21CM array ( Gu Junhua ). Physics with UHE cosmic neutrinos. UHE neutrinos as a tool to study violent phenomena in the Universe

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The Pierre Auger Observatory Auger North

The Pierre Auger Observatory Auger North. Features of Auger North R&D Auger Collaboration Cost and Schedule The Role of Fermilab. Denver. Colorado Springs. Features of Auger North. State of Colorado. Auger North: 4400 detectors 1.41mi spacing 8000 mi 2 (21,000 km 2 ).

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Assegnazioni Pd 2009 66 Ricercatori 11 Tecnologi 44.6 FTE

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Absolute Measurement of Air Fluorescence Yield for Ultra-High Energy Cosmic Rays

Fermilab, June 27 2008. Absolute Measurement of Air Fluorescence Yield for Ultra-High Energy Cosmic Rays. Paolo Privitera. Carlos Hojvat. FD. SD. Auger results. Flux suppression. Anisotropy < 75 Mpc. Astrophysical interpretation GZK horizon.

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Advanced Construction Technology

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MEGAPIE Structural Materials Is there a risk of failure?

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Production of nano-thin graphite films by CVD

Production of nano-thin graphite films by CVD A.N. Obraztsov 1,2 * , A.V. Tyurnina 2 , E.A. Obraztsova 2 , A.A. Zolotukhin 2 , K.N. Eltsov 3 , B.V. Andryushechkin 3 1 University of Joensuu, Joensuu 801101, Finland 2 Moscow State University, Moscow 119992, Russia

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DNA photoprotection

Femtosecond Dynamics in the Photoprotection in Thymine Brian McFarland and the LCLS Nucleobase Photoprotection collaboration. UV Excitation . Photoprotection. X-Ray Probe. Motivation:. Experiment:. p*. Auger. p ? p *. n ? p. DNA photoprotection. IP.

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