G. Larosa, M. Ardid (for the KM3NeT Consortium) Institut d’Investigació per a la Gestió Integrada de les Zones Costaneres - Universitat Politècnica de.

Slides:



Advertisements
Similar presentations
Miguel Ardid Ramírez IGIC- Universitat Politècnica de València.
Advertisements

Kay Graf Physics Institute 1 University of Erlangen ARENA 2006 University of Northumbria June 28 – 30, 2006 Integration of Acoustic Neutrino Detection.
Status of the ANTARES Neutrino-Telescope Alexander Kappes Physics Institute University Erlangen-Nuremberg for the ANTARES Collaboration WIN´05, 6.–11.
Kay Graf Physics Institute University of Erlangen TeV Particle Astrophysics II Madison, WI, USA August 28 – 31, 2006 Towards Acoustic Detection of UHE.
By E. Anassontzis, A. Belias, E. Kappos, K. Manolopoulos, P. Rapidis on behalf of the KM3NeT Collaboration.
Paolo Musico on behalf of KM3NeT collaboration The Central Logic Board for the KM3NeT detector: design and production Abstract The KM3NeT deep sea neutrino.
Deep-sea neutrino telescopes Prof. dr. Maarten de Jong Nikhef / Leiden University.
ANTARES: Towards Acoustic Detection of Highest Energy Neutrinos Kay Graf for the ANTARES Collaboration Erlangen Centre for Astroparticle Physics VLV T.
Amsterdam 29 March 2011 Fernando Urbano IFIC (CSIC – Universidad de Valencia) KM3NeT Optical Calibration Laser Beacon and Nanobeacon Status.
Concepts of Multiplexing Many input signals to one transmission media Reduces the number of channels or conductors running from point A to point B Added.
ARENA Workshop, May, 2005 First Activities in Acoustic Detection of Particles in UPV M. Ardid, J. Ramis, V. Espinosa, J.A. Martínez-Mora, F. Camarena,
Data acquisition system for the Baikal-GVD neutrino telescope Denis Kuleshov Valday, February 3, 2015.
INSTRUMENTATION NEEDS FOR THE CALIBRATION UNIT …AS A WORK DOCUMENT Pascale Keller KM3Net Meeting CPPM, january 2013 Inputs from : Miguel Ardid, Tassos.
S. Viola VLVνT 2015, Rome – 14/09/2015 Characterization and testing of the KM3NeT acoustic positioning system F. Simeone VLVνT 2015 – Rome, 14/09/2015.
INFN Bari, Bologna, Catania, Genova, LNF, LNS, Napoli, Pisa, Roma Università Bari, Bologna, Catania, Genova, Napoli, Pisa, Roma “La Sapienza” CNR Istituto.
ACoRNE*, UK The calibration and experiment of transmitter array for the acoustic neutrino detection W. Ooppakaew*, S. Danaher*, R. Lahmann**, K. Graf**
Review of Positioning in ANTARES Dr. Lee F. Thompson Department of Physics and Astronomy University of Sheffield Special thanks to Vincent Bertin, CPPM.
Calibration Methods and Tools for KM3NeT V. Kulikovskiy on behalf of the KM3NeT collaboration.
Salvatore Viola, INFN-LNS VLVνT 2011, Erlangen - October 12-14, 2011 Salvatore Viola 5th International Workshop on Very Large Volume Neutrino Telescopes.
Digital & Analog electronics for an autonomous, deep-sea Gamma Ray Burst Neutrino prototype detector K. Manolopoulos, A. Belias, E. Kappos, C. Markou DEMOKRITOS.
KM3NeT Pylos meeting, April, 2007 Some preliminary studies for the positioning calibration of KM3NeT Miguel Ardid Universitat Politècnica de València.
Acoustic Calibration for the KM3NeT Pre-Production Module Alexander Enzenhöfer on behalf of the KM3NeT consortium VLV T 2011 Erlangen, –
Antares Slow Control Status 2007 International Conference on Accelerator and Large Experimental Physics Control Systems - Knoxville, Tennessee - October.
The ANTARES Project Sino-French workshop on the Dark Universe Stephanie Escoffier Centre de Physique des Particules de Marseille On behalf of the ANTARES.
Time over Threshold electronics for an underwater neutrino telescope G. Bourlis, A.G.Tsirigotis, S.E.Tzamarias Physics Laboratory, School of Science and.
Time calibration system for the KM3NeT deep sea neutrino telescope S. Toscano, IFIC (Instituto de Física Corpuscular)
VLVnT11 - Erlangen 12-14/10/ Giorgio Cacopardo NEMO Phase2 mechanical design G. Cacopardo on behalf of NEMO collaboration.
Time and amplitude calibration of the Baikal-GVD neutrino telescope Vladimir Aynutdinov, Bair Shaybonov for Baikal collaboration S Vladimir Aynutdinov,
A Device for Detection of Acoustic Signals from Super High Energy Neutrinos Presenter: Presenter: G.L.Pan'kov Applied Physics Institute of Irkutsk State.
NEMO-O DE NEMO First results from the NEMO Test Site G. Riccobene, for the NEMO Collaboration The NEMO Collaboration is performing the Phase 1 of the project,
Calibration of Under Water Neutrino Telescope ANTARES Garabed HALLADJIAN October 15 th, 2008 GDR Neutrino, CPPM, Marseille.
The Trigger and Data Acquisition System for the KM3NeT neutrino telescope Carmelo Pellegrino Tommaso Chiarusi INFN - Sezione di Bologna VLVnT 2015 | Rome,
HOT CAR BABY DETECTOR Group #20 Luis Pabon, Jian Gao ECE 445 Dec. 8, 2014.
C.Sollima INFN - University of Pisa for the KM3NeT Consortium “Quality Control Considerations for the KM3NeT Very Large Volume neutrino Telescope” The.
Acoustics in Phase IIG. Riccobene Oct. 17, 2012 NEMO Phase II Acoustic positioning system (or the “zombie”) FACTS: - Standard ACSA-LBL calibration procedure:
Simona Toscano In the frame of KM3NeT consortium VLV T workshop - Toulon, April 2008.
Status and First Results of the Acoustic Detection System AMADEUS in ANTARES Robert Lahmann for the ANTARES Collaboration ARENA 08, Rome, 26-June-2008.
Development of combined sensors for UHE neutrino detection Alexander Enzenhöfer ARENA 2010 Nantes,
Status and Advances on the Acoustic Positioning System for KM3NeT Giuseppina Larosa, IGIC-UPV KM3NeT General Meeting, Nikhef 28-31/03/2011.
VLVNT’08 - ToulonM. Ardid – Positioning System of the ANTARES Neutrino Telescope Positioning system of the ANTARES Neutrino Telescope Miguel Ardid (IGIC.
Acoustic transceivers for the KM3NeT positioning system Miguel Ardid KM3NeT General Meeting Marseille, January 29 – February 1, 2013.
Isabella Amore VLV T08, Toulon, France April 2008 International Workshop on a Very Large Volume Neutrino Telescope for the Mediterranean Sea Results.
Status and Perspectives of the BAIKAL-GVD Project Zh.-A. Dzhilkibaev, INR (Moscow), for the Baikal Collaboration for the Baikal Collaboration September.
G. Riccobene, INFN-LNS Pylos - Km3Net General Meeting April 2007 G. Riccobene Acoustic positioning system for NEMO phase II.
DOM Electronics (Digital Optical Module) 1 WPFLElectronics PPMDOM ElectronicsF. Louis.
Umberto Emanuele IFIC (CSIC-UV), Valencia (Spain) Status of Time Calibration System forKM3NeT.
High energy neutrino acoustic detection activities in Lake Baikal: status and plans N.Budnev for the Baikal Collaboration Irkutsk State University, Russia.
Giorgio Riccobene, LNS-INFN KM3NeT WPF/L Meeting, NIKHEF 5-7/07/2010 Status of the Acoustic Calibration System for KM3NeT.
WP F/L Detection Unit Mechanical Structure and Deployment R. Papaleo 130/03/2011.
Calibration and Instrumentation: Overview and General Issues Robert Lahmann WPFL meeting Amsterdam 6-July-2010.
Summary of Calibration and Instrumentation Session Robert Lahmann KM3NeT Collaboration Meeting, CPPM, 31-Jan-2013.
23 April, 2008Gabriele Giovanetti – INFN - LNS1 New electronics architecture in NEMO – phase 2. Gabriele Giovanetti – INFN – LNS NEMO Phase 1: 4 floor.
Status of the NEMO tower validation Integration Tests Improvements Deployment program M.Anghinolfi- km3-day meeting )
Bou-Cabo Manuel Ardid-Ramírez Miguel Camarena-Femenía Francisco Espinosa-ResolloVíctor Larosa Giuseppina Martínez-Mora Juan A (IGIC- Universitat Politècnica.
Bou-Cabo Manuel Ardid-Ramírez Miguel Camarena-Femenía Francisco Espinosa-ResolloVíctor Larosa Giuseppina Martínez-Mora Juan A (IGIC- Universitat Politècnica.
Pre-Production Models for KM3NeT
A DWDM link for Real-Time data acquisition systems
Positioning system Hardware
Deep-sea neutrino telescopes
P.Kooijman, UVA-GRAPPA, UU, Nikhef
Robert Lahmann VLVnT – Toulon – 24-April-2008
T. Eberl for Robert Lahmann and the Erlangen acoustic group
Els de Wolf 20 February 2012, Catania
Acoustic Position Calibration of the KM3NeT Neutrino Telescope
Overview of AMADEUS and Positioning for KM3NeT
Junction Boxes for KM3NeT
M.Bou-Cabo, J.A. Martínez.-Mora on behalf of the ANTARES Collaboration
Front-end electronic system for large area photomultipliers readout
Calibration of Sensors for Acoustic Detection of Neutrinos
Nanobeacon: A low cost calibration instrument for KM3NeT
Presentation transcript:

G. Larosa, M. Ardid (for the KM3NeT Consortium) Institut d’Investigació per a la Gestió Integrada de les Zones Costaneres - Universitat Politècnica de València Frontier Detectors for Frontier Physics 12 th Pisa meeting on advanced detectors La Biodola, Isola d’Elba (Italy) May 20 – 26, 2012

KM3NeT  a future underwater neutrino telescope Compact package of the DU Flexible tower The compact package of the DU allows a fast and efficient way for deploying the detector. The DU unfurls once it is placed on the seafloor.

Acoustic Positioning System (APS) Key elements for the Acoustic Positioning System:  Auto-calibrating Long Baseline of acoustic transceivers anchored in known and fixed positions. They define the reference frame.  Array of acoustic sensors (hydrophones) in the Detection Unit mechanical structure.  Auxiliary devices: tiltmeters and compasses, CTDs, sound celerimeters, sea current metres (ADCPs).  Data acquisition and transmission system.  Data analysis system on-shore. Hydrophones will be sampled continuously at a rate of about 200 kHz and a continuous stream of data will be sent to shore for positioning and acoustic monitoring studies. Measurement and Analysis Technique: 1.T Rec (Hydro) – T Em (Beacon)  Distance 2. Geometrical Triangulation  Position Measurement and Analysis Technique: 1.T Rec (Hydro) – T Em (Beacon)  Distance 2. Geometrical Triangulation  Position All elements have been tested in lab, and will be tested in situ In NEMO-Phase II (2012) and in the KM3NeT Pre-Production Model. Scheme of the Acoustic Positioning System

Acoustic Positioning System (APS) for KM3NeT Acoustic receivers and electronics Piezo and preamp Acoustic transceiver Sound Emission Board (SEB) FFRSX30 transducerSEB Diagram SMID hydrophone KM3NeT Acouboard Electronics inside the DOM Piezo in the DOM (external view)  Emission frequency :25 kHz÷45 kHz.  LBL transcievers and hydrophones phased and synchronous.  Acoustic signal amplitude can be set from shore.  All data to shore. Power consumption: 100 VDC 1 VDC Piezo dimensions: 18 mm x 12 mm Sensor dimensions: 21 mm x 30 mm