'Cosmic ray' diaporamas de présentation

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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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High Energy Neutrino Astronomy

High Energy Neutrino Astronomy. Gisela Anton LAUNCH 09 Heidelberg, November 10 th , 2009. Content. Introduction to high energy neutrino astronomy Neutrino-Telescopes: IceCube and ANTARES Selected results Future perspectives of IceCube und KM3NeT.

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Cosmic Ray Physics with the IceCube Observatory

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CME-GEOMETRY AND COSMIC-RAY ANISOTROPY OBSERVED BY A PROTOTYPE MUON DETECTOR NETWORK

CME-GEOMETRY AND COSMIC-RAY ANISOTROPY OBSERVED BY A PROTOTYPE MUON DETECTOR NETWORK.

495 views • 36 slides

Neutrino Physics

Neutrino Physics. Member Eriko kusunoki Kenji shu Takeshi saito Mesanori iwamoto Mitsutaka nakao. NISHIMURA Group. CONTENTS. ? - Source. Theory of Neutrino Physics Super Kamiokande (Super K) Measuring Cosmic Rays T2K Experiment Analyzing T2K data. ? - Oscillation.

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425 views • 31 slides

hubblesite/newscenter/archive/releases/2006/30/image/a/format/xlarge_web/

Particle Acceleration by Shocks. Tony Bell with Brian Reville, Klara Schure, Gwenael Giacinti University of Oxford. http://hubblesite.org/newscenter/archive/releases/2006/30/image/a/format/xlarge_web/. Cassiopeia A. Radio (VLA). Infrared (Spitzer). chandra.harvard.edu/photo/

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WHY LHC?

WHY LHC?. D. P. ROY Homi Bhabha Centre for Science Education Tata Institute of Fundamental Research Mumbai, India. Contents. Basic Constituents of Matter and their Interactions : Matter Fermions and Gauge Bosons (Std Model) High Energy Colliders

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Background

Cosmic Ray Physics at Hartnell College : A Case Study in Successful Undergraduate Research at a Two-Year College. Leo Osornio Hartnell College Presented at the 2012 AAPT Summer Meeting, Philadelphia July 30, 2012. Background. Hartnell College Salinas, CA Prospective Physics Teacher

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Pan-STARRS observational requirements specification

Pan-STARRS observational requirements specification. Outline. Benchmark design specs Telescopes Detectors Pipeline Data products Precision goals Specification of observational requirements Format for input to science DWG. Pan-STARRS in a Nutshell. Who?

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Pan-STARRS observational requirements specification

Pan-STARRS observational requirements specification. Outline. Benchmark design specs Telescopes Detectors Pipeline Data products Precision goals Specification of observational requirements Format for input to science DWG. Pan-STARRS in a Nutshell. Who?

277 views • 16 slides

Night Sky Live!

Night Sky Live!. All-Sky Transient Detection Using the Night Sky Live! Network Lior Shamir & Robert J. Nemiroff Abstract

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Eddington - MSSL Areas of interest/expertise

Eddington - MSSL Areas of interest/expertise. General Points Used to working in either paradigm - as industrial contractor e.g. GOES-SXI, Solar-B FPP (Lockheed) Integral-OMC (Prodex) - as nationally-funded Institute (~30 satellite payloads)

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PA/QA STATUS

PA/QA STATUS. MPE /PACS/IGL. PACS PA/QA TEAM. PA/QA Documents. Open Critical Items as available yet. IAC : No formal qualification for soldering (CRISA) Critical delivery schedule for PSC ASIC IMEC: Some minor critical items are listed:

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VOYAGER 2

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WBS 1.3.9 Simulation and Offline Analysis

WBS 1.3.9 Simulation and Offline Analysis . Yury Kolomensky UC Berkeley. Components. Simulation tools in support of the detector design Muon production rates and beamline simulation Background estimates Solenoid modeling, field maps Detector modeling and optimizations Tracker

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Intermediate Silicon Tracker For STAR HFT Upgrade

Intermediate Silicon Tracker For STAR HFT Upgrade. Yaping Wang 1, 3 , Gerrit J. van Nieuwenhuizen 2 , Zhenyu Ye 1, 3 for the STAR Collaboration. 1 University of Illinois at Chicago, 2 Massachusetts Institute of Technology, 3 Central China Normal University. Abstract.

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Hadronic Physics Not Covered by Current Models

Hadronic Physics Not Covered by Current Models. ULTLA High Energy Model Much beyond LHC 14TeV cms Air shower from highest energy cosmic ray 1020 eV (proton, Fe?) Isotope production Activation Anti Particles Neutrino Biassing.

88 views • 1 slides