'Optical modules' diaporamas de présentation

Huawei SX7 Campus Switches Configuration Quotation Guide ( Overseas)

Huawei SX7 Campus Switches Configuration Quotation Guide ( Overseas). Tools. UniSTAR eCFG Customized Description: Offline quotation tool Training material (channel) UniSTAR SCT Web-based Description: Simplified online quotation tool (only this tool will be provided in future) SCT

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Neutrino Telescopy in the Deep Sea

Neutrino Telescopy in the Deep Sea. Elementary Particle Physics Seminar, University of Oxford. Uli Katz Univ. Erlangen 05.06.2007. Introduction Physics with Neutrino Telescopes ANTARES and Other Current Projects Aiming at a km 3 Detector in the Mediterranean Sea: KM3NeT

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High-Energy Neutrino Searches

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The ANTARES project

The ANTARES project. L. Moscoso DSM/DAPNIA, CEA/Saclay Venice, Italy, Feb. 22-26, 99. The ANTARES project. Construction of a prototype (few lines connected to the shore) of a neutrino telescope extrapolable to a km 3 detector. Programme of measurement of environmental parameters.

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Status of the ANTARES Neutrino-Telescope

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Gigaton Volume Detector in Lake Baikal: status of the project

Gigaton Volume Detector in Lake Baikal: status of the project. QUARKS-2010, Kolomna, 6-12 June, 2010. Zh.-A. Dzhilkibaev (INR, Moscow) for the Baikal Collaboration. Collaboration. Institute for Nuclear Research, Moscow, Russia. Irkutsk State University, Russia.

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Baikal Neutrino Experiment

Baikal Neutrino Experiment. Vladimir Aynutdinov for the Baikal Collaboration Athens, October 13, 2009. Collaboration. Institute for Nuclear Research, Moscow, Russia. Irkutsk State University, Russia. Skobeltsyn Institute of Nuclear Physics MSU, Moscow, Russia.

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Assembly and Design of the Optical Modules for the NEMO Phase-2 E. Leonora , S. Aiello

Assembly and Design of the Optical Modules for the NEMO Phase-2 E. Leonora , S. Aiello INFN, sez. Catania. NEMO Phase-2. It consists of new infrastructure at the deep-sea site of Capo Passero, Sicily, at 3500 m depth : - 100 km cable, linking the site to the shore

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Imaging the High-Energy Neutrino Universe from the South Pole

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Searches for the Highest Energy Neutrino with IceCube

Searches for the Highest Energy Neutrino with IceCube. Aya Ishihara ( JSPS Research Fellow) Chiba University. COSMO/CosPA 2010 September 27, 2010. IceCube at South Pole. 1km 3 volume 80 +6 Holes 60 Optical Modules 17 m between m odules 125 m between holes. construction

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Imaging the Neutrino Universe with AMANDA and IceCube

Imaging the Neutrino Universe with AMANDA and IceCube. Motivations for neutrino astronomy Selected AMANDA results IceCube: Status and Plans. David Hardtke University of California, Berkeley. Lake Louise Winter Institute February 2005. Neutrino Astronomy. Neutrino Production and Detection.

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Imaging the Neutrino Universe with AMANDA and IceCube

Imaging the Neutrino Universe with AMANDA and IceCube. Motivations for neutrino astronomy Selected AMANDA results IceCube: Status and Plans. David Hardtke University of California, Berkeley. Lake Louise Winter Institute February 2005. Neutrino Astronomy. Neutrino Production and Detection.

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PMT measurements in Antares

PMT measurements in Antares. Oleg Kalekin on behalf of Antares collaboration VLVnT 2011 Erlangen 14.10.2011. Motivation Reduction of differences between Monte Carlo and real Antares data charge distribution of the background hits 40 K coincidence rate in two adjacent optical modules

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The NEMO DAQ electronics: Actual characteristics and new features

The NEMO DAQ electronics: Actual characteristics and new features. NEMO tower layout. Electrical link. FCM (Floor Control Module). OM-PMT & FE electronics. Floor 16. 10Mbps. 40m. Floor 15. 40m. Optical link. 10m. Floor 2. 40m. PMT4. PMT3. Floor 1. PMT1. PMT2. Optical link.

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