'High energy cosmic rays' diaporamas de présentation

Air Cherenkov Methods in Cosmic Rays: A Review and Some History

Air Cherenkov Methods in Cosmic Rays: A Review and Some History. A.S. Lidvansky, Institute for Nuclear Research, Moscow. The Vavilov-Cherenkov radiation of high energy cosmic rays in air:.

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Cosmic Rays and Gamma Ray Bursts Origin of Cosmic Rays: A Complete Model

Gamma Ray Bursts and the Origin of Cosmic Rays Chuck Dermer (NRL) Colloquium, NRAO Charlottesville 20 January 2005 dermer@gamma.nrl.navy.mil Armen Atoyan (UdeM) Jeremy Holmes (TJHSST, NRL, FIT) Stuart Wick (NRL, SMU). Cosmic Rays and Gamma Ray Bursts Origin of Cosmic Rays: A Complete Model

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THE ORIGIN OF COSMIC RAYS

THE ORIGIN OF COSMIC RAYS. Pasquale Blasi Fermilab/Center for Particle Astrophysics INAF/Arcetri Astrophysical Observatory, Italy. Early History of Cosmic Rays. Ionized by what?. 1895: X-rays (Roengten) 1896: Radioactivity (Becquerel)

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Pratik Majumdar SINP, Kolkata

Astroparticle Physics : High Energy Particles and Non Thermal Radiation. Outline: Cosmic rays History and Discovery Composition and propagation Non thermal Radiation How do we see cosmic rays ? . Pratik Majumdar SINP, Kolkata. Reading Materials. Longair : High Energy Astrophysics

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Giant resonances, exotic modes & astrophysics

Giant resonances, exotic modes & astrophysics. 1) The dipole strength : r-process Ultra-High Energy Cosmic Rays 2) Exotic modes : SuperGiant Resonances Giant Pairing Vibrations 3) Surprise ?. E. Khan.

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The Status of IceCube

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G. Battistoni, A. Margiotta, S. Muraro, M. Sioli

The FLUKA high energy cosmic ray generator: predictions for the charge ratio of muons detected underground. G. Battistoni, A. Margiotta, S. Muraro, M. Sioli. FLUKA Meeting 28 th April 2009.

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Uppsala University June 9, 2009

Uppsala University June 9, 2009. Solar Physics with the IceTop Air Shower Array Paul Evenson University of Delaware (aka New Sweden) Department of Physics and Astronomy. The First Extraterrestrial Event Detected by IceCube. IceTop and Spaceship Earth Observations of the Solar Flare.

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THE UNIVERSITY IN TIMES OF CULTURAL SHOCK (The Federal University of ABC)

THE UNIVERSITY IN TIMES OF CULTURAL SHOCK (The Federal University of ABC). SPIDER WEB. Luiz Bevilacqua February 2013. THE CORNERSTONE OF THE KNOWLEDGE BOOM. Ability to make scientific observations and experiments

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Moon shadow analysis -- Using ARGO experiment

Wang Bo, Zhang Yi, Zhang Jianli, Guo Yiqing, Hu Hongbo. Apri. 27 2008 for NanJing Meeting. wangb@ihep.ac.cn. Moon shadow analysis -- Using ARGO experiment. OUTLINE. 1. Why to study Moon shadow? 2. Experiment introduction . 3. Data and Reconstruction. 4. Moon shadow Analysis

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Ultra-High Energy Neutrino Fluxes

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High Energy Cosmic Rays The Primary Particle Types Paul Sommers for Alan Watson

High Energy Cosmic Rays The Primary Particle Types Paul Sommers for Alan Watson Epiphany Conference, Cracow January 10, 2004. High Energy Cosmic Rays The Primary Particle Types Paul Sommers for Alan Watson Epiphany Conference, Cracow January 10, 2004. See astro-ph/0312475. Overview

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Air Showers in a Self-Triggered Neutron Monitor

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Bruce Gendre LAM/OAMP

What GRBs can bring to Particle Astrophysics (and vice-versa) ?. Bruce Gendre LAM/OAMP. The Gamma-Ray Burst phenomenon. Sudden and unpredictable bursts of hard X and soft ? rays Typical durations of tens of seconds Cosmological origin Typical isotropic energy: 10 51 to 10 54 erg.

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Appendix E: Intro to the Banff Feb06 Annual Meeting

Appendix E: Intro to the Banff Feb06 Annual Meeting. See the body of the text, Section 3.2, for an introduction to this introduction. The slides were taken from the Planning Meeting summary (with small updates) associated with the C&G Annual Meeting in Mont Tremblant in March 2005

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ASPERA Status

per aspera ad astra. AStroparticle ERAnet. ASPERA Status. Astronet GB 20 September 2006 S.Katsanevas CNRS/IN2P3. What is the AstroParticle ERA net (ASPERA)?. An EU ERANET program with

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Physics on the Extreme: Theoretical (high energy) A strophysics

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High-energy particle acceleration in the shell of a supernova remnant

High-energy particle acceleration in the shell of a supernova remnant. F.A. Aharonian et al (the HESS Collaboration) Nature 432 , 75 (2004) Nuclear Physics Group Journal Club Jan. 31, 2005 as interpreted by J.W. Martin University of Winnipeg. Cosmic Rays.

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Introduction by Y. suzuki

Introduction by Y. suzuki. for the External Review Committee October 19 th and 20 th , 2006 Institute for Cosmic Ray Research The University of Tokyo. Purpose of this review committee.

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C losing

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