G. RICCOBENE INFN-LNS KM3NET CALIB WG LEADER - CU PDR 02/07/2019 G. RICCOBENE INFN-LNS - CERN INDICO
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KM3NeT: the giant scale neutrino telescope neutrino telescope Network of cabled observatories located in deep waters of the Mediterranean Sea. Array of optical sensors Centrally managed: common hardware, software, data handling and control Cherenkov light Astronomy: ARCA @ Capo Passero muon Phase 1 under construction, Phase 2 defined: Cable to shore 2 building blocks (few km among the blocks) interaction 115 Detection Units(DU) / block 18 DOMs (36 m inter-DOM) neutrino 90 m inter-DU distance 1 km3 volume Oscillations and Mass Hierarchy: ORCA @ Toulon 1 building block 115 detection Units 18 DOMs (9 m inter-DOM) 6 Mton volume G. Riccobene INFN-LNS CU PDR 02/07/2019
KM3NeT: The Detector 750 m Digital Optical Module (DOM) A fly’s eye light detector Inside a 17’’ glass sphere 2 km2 Plus: compass, acoustic sensor, KM3NeT - ARCA front-end and data Detection Unit 230 Detection Units transmission electronics A vertical slender sling KM3NeT - ORCA with 18 DOMs 115 Detection Units 1 hydrophone at each 260 W Detection Unit base 400 Mbps Data sent in real-time to shore for analysis G. Riccobene INFN-LNS CU PDR 02/07/2019
KM3NeT: The Sites ORCA: 2500 m wd, 45 km offshore ARCA: 3500 m wd, 95 km offshore 230 DUs 115 DUs Footprint: 2 x 1000 x 1000 m Footprint: 300 x 300 m height: 700 m height: 300 m inter DU distance (average): 80 m inter DU distance: 25 m Phase 1: Phase 1: 24 DUs 7 DUs G. Riccobene INFN-LNS CU PDR 02/07/2019
KM3NeT: Challenges Transportation (truck, ship) “Standard” Deployment and Recovery (ship, rov) Design: safe monoueving Marking: rigging, lashing, connection, disconnection, grabbing Labelling: WiA, WiW Interaction with third parties: certifications Operation (seawater) “No” vibration Constant “low” temperature (13.5°) High External Pressure Conductive and “live” medium: Corrosion, short circuit propagation No maintenance during detector operation lifetime! G. Riccobene INFN-LNS CU PDR 02/07/2019
This Review: Who are we Miles Lindsay Clark (APC): Technical Coordinator of KM3NeT Ernst Jan Buis (TNO): Chief System Engineer of KM3NeT Giorgos Androulakis (Demokritos): QA/QC Task leader of KM3NeT Giorgio Riccobene: Calibration WG leader IU ORCA: P. Keller (L), Ph. Lagier, A. Cosquer - CPPM CB ARCA: M. Anghinolfi (L), R. Cereseto, S. Ottonello – INFN Genova Laser Beacon: R. Le Breton (L), A. Creusot, A. Ilioni, S. Boutonet - APC CB ORCA: A. Ilioni (L), C. Boutonet, S. Colonges, L. Confucius – APC IU ARCA: Rovelli (L), C. D’Amato, A. Grmek – INFN LNS G. Riccobene INFN-LNS CU PDR 02/07/2019
This Review: what we want Deals with mechanics of the assets (but suggestions on others are welcome!) We ask you to help us to: verify that materials and design are OK to fulfil the request all documentation is in place and clear Tell us clearly: what is good what is “wrong” what is not clear what we must do, yet what would be diligent to do G. Riccobene INFN-LNS CU PDR 02/07/2019
This Review: Documentation We use CERN indico https://indico.cern.ch/event/829590/ and vydio https://vidyoportal.cern.ch/join/3moTzTrv6r Documents will be stored on Google Drive https://drive.google.com/open?id=1OjRW4kaF8G2Ngfut4BPAuBsWFBGerTQf G. Riccobene INFN-LNS CU PDR 02/07/2019
This Review: Documentation On Indico and Gdrive: Calibration_Unit_Preliminary_Design_Review_PDR.zip On Gdrive: KM3NeT_CALIB_2019_103_MechReview_RIDtemplate.xlsx https://drive.google.com/open?id=1rgdelCxhyGiOxgLkhSkhr90 CrqbSRlcczCmUswnRrnQ G. Riccobene INFN-LNS CU PDR 02/07/2019
KM3NeT at Capo Passero: The ARCA Calib Unit Calibration Base Lifetime 20 y 300 m electro-optical interlink cable CB-JB Teldyne ODI NRH CB electronics/optics container (DU base design) Host 2 instruments Hydrophone -> Acoustic Positioning System M.Anghinolfi INFN-Genova Acoustic Beacon -> Acoustic Positioning System Permits connection to IU G. Riccobene INFN-LNS CU PDR 02/07/2019
KM3NeT at Capo Passero: The ARCA Calib Unit Instrumentation Unit Recovered evey 2/3 years for instrument recalibration and battery change A.Rovelli INFN-LNS Base of the IU: design inherited from ITF and SHB Working at CP site since January 2019 G. Riccobene INFN-LNS CU PDR 02/07/2019
KM3NeT at Toulon: The ORCA Calibration Unit Calibration Base Lifetime 15 y Host 3 instruments Laser Beacon -> Time Calibration Hydrophone -> Positioning System Acoustic Beacon -> Positioning System Permits connection to IU A. Ilioni APC G. Riccobene INFN-LNS CU PDR 02/07/2019
KM3NeT at Toulon: The ORCA Calib Unit Instrumentation Unit P. Keller CPPM Recovered evey 2/3 years for instrument recalibration and battery change Base of the IU IU electronics vessel (ANTARES) Base of the IU: design inherided from ITF and SHB G. Riccobene INFN-LNS CU PDR 02/07/2019
The Laser Beacon Lifetime 20 years Emit short pulses of laser light to Flange illuminate all DUs at the “same” time Laser Same Design for Titanium cylinder ORCA (Calibration Base) Quartz rod ARCA (JB) LPMI+ O-rings Flange Laser board control Connector Internal Structure O-rings R. Le Breton APC G. Riccobene INFN-LNS CU PDR 02/07/2019
PBS G. Riccobene INFN-LNS CU PDR 02/07/2019
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