INSTRUMENTATION NEEDS FOR THE CALIBRATION UNIT …AS A WORK DOCUMENT Pascale Keller KM3Net Meeting CPPM, 29-31 january 2013 Inputs from : Miguel Ardid, Tassos.

Slides:



Advertisements
Similar presentations
Tachometers – An Overview
Advertisements

Kay Graf University of Erlangen for the ANTARES Collaboration 13th Lomonosov Conference on Elementary Particle Physics Moscow, August 23 – 29, 2007 Acoustic.
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.
Aloha Proof Module Design Cabled Observatory Presentation School of Ocean and Earth Science and Technology February 2006.
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.
Hanoi, Aug. 6-12, 2006 Pascal Vernin 1 Antares Status report P.Vernin CEA Saclay, Dapnia On behalf of the Antares collaboration P.Vernin
Coincidence analysis in ANTARES: Potassium-40 and muons  Brief overview of ANTARES experiment  Potassium-40 calibration technique  Adjacent floor coincidences.
Francisco Salesa Greus IFIC (CSIC–Universitat de València, Spain) Representing the KM3NeT Consortium 4 th International Workshop on Very Large Volume Neutrino.
1 S. E. Tzamarias Hellenic Open University N eutrino E xtended S ubmarine T elescope with O ceanographic R esearch Readout Electronics DAQ & Calibration.
Amsterdam 29 March 2011 Fernando Urbano IFIC (CSIC – Universidad de Valencia) KM3NeT Optical Calibration Laser Beacon and Nanobeacon Status.
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.
Maintenance of the ANTARES deep-sea neutrino telescope 1 Marco Circella --- INFN Bari on behalf of the ANTARES Collaboration.
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.
Characterization of the electro-optical transceivers in the KM3NeT optical network S.Pulvirenti, F. Ameli, A. D’Amico, G. Kieft, J-W Schmelling for KM3NeT.
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.
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, –
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 calibration system for the KM3NeT deep sea neutrino telescope S. Toscano, IFIC (Instituto de Física Corpuscular)
Calibration of Under Water Neutrino Telescope ANTARES Garabed HALLADJIAN October 15 th, 2008 GDR Neutrino, CPPM, Marseille.
G. Riccobene, INFN-LNS Nikhef, May 24-25, 2012 Giorgio Riccobene INFN-Laboratori Nazionali del Sud Abyssal undular vortices in the Eastern Mediterranean.
Tiltmeter, Compass,Temperature modules for the PPM.
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.
F. Simeone – INFN, Sez. Roma1 RICAP07 Conference, Rome June 2007 Data taking system for NEMO experiment RICAP07.
Development of combined sensors for UHE neutrino detection Alexander Enzenhöfer ARENA 2010 Nantes,
G. Larosa, M. Ardid (for the KM3NeT Consortium) Institut d’Investigació per a la Gestió Integrada de les Zones Costaneres - Universitat Politècnica de.
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.
The sector of the Antares line to be deployed in the NEMO site Davide Piombo – INFN sez. Genova
Acoustic transceivers for the KM3NeT positioning system Miguel Ardid KM3NeT General Meeting Marseille, January 29 – February 1, 2013.
ATM-900 Series Acoustic Telemetry Modems Introduction and Overview Communication Group: Justin Manley – Senior Director of Business Development Debbie.
Isabella Amore VLV T08, Toulon, France April 2008 International Workshop on a Very Large Volume Neutrino Telescope for the Mediterranean Sea Results.
M. Circella – ANTARES connectionINFN Comm. II, 5/6/2008 The ANTARES Connection Marco Circella --- INFN Bari 1.
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.
KM3NeT Optical Calibration Umberto Emanuele IFIC (CSIC – University of Valencia, Spain) WPF/L KM3NeT Meeting Nikhef 5 th - 7 th July
Marseille 29 January 2013 Diego Real IFIC (CSIC – Universidad de Valencia) Instrumentation for Optical Calibration: Laser Beacon and Nanobeacon.
KM3NeT WPF/L NIKHEF- MECABAR 1 A.Cosquer on behalf of the KM3NeT consortium MECABAR PROJECT PLAN 1- Context 2- 3D views and responsibilities 3-
Site for the PPM-DU String Layout Possible Site / Properties Power / Communication Contribution / Planning R.Papaleo, P.Lamare, E.Heine Bologna.
Giorgio Riccobene, LNS-INFN KM3NeT WPF/L Meeting, NIKHEF 5-7/07/2010 Status of the Acoustic Calibration System for KM3NeT.
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.
DOM developments Mini DOM PPM-DOM in Antares PPM future WP F-L.
Status of the NEMO tower validation Integration Tests Improvements Deployment program M.Anghinolfi- km3-day meeting )
Pre-Production Models for KM3NeT
PORFIDO Use neutrino telescopes infrastructure (power, communication)
PORFIDO Use neutrino telescopes infrastructure (power, communication)
Positioning system Hardware
Deep-sea neutrino telescopes
DOM acceptance and calibration
On behalf of Patrick Lamare
Interdisciplinary Activity ANTARES
Robert Lahmann VLVnT – Toulon – 24-April-2008
T. Eberl for Robert Lahmann and the Erlangen acoustic group
White Rabbit in KM3NeT Mieke Bouwhuis NIKHEF 9th White Rabbit Workshop
Acoustic Position Calibration of the KM3NeT Neutrino Telescope
Overview of AMADEUS and Positioning for KM3NeT
Junction Boxes for KM3NeT
ANTARES time calibration
Robert Lahmann for the ANTARES Collaboration
The Instrumentation Unit of The KM3NeT Calibration Unit
Nanobeacon: A low cost calibration instrument for KM3NeT
Acoustic Measurements in ANTARES: Status and Aims
Presentation transcript:

INSTRUMENTATION NEEDS FOR THE CALIBRATION UNIT …AS A WORK DOCUMENT Pascale Keller KM3Net Meeting CPPM, january 2013 Inputs from : Miguel Ardid, Tassos Belias, Vincent Bertin, Robert Lahmann, Diego Real, Giorgio Riccobene

Plan : Resume on DOM instrumentation Possible instruments for Calibration Units ? Some open questions 2

Status on DOM instrumentation (for info)  Orientation : Tiltmeter and compass (from Tassos) Measurement Technology, NS-25/DQL2-IXA tilts accuracy : ±0.1° resolution 0.02° dimensions : w x d x h 25 x 25 x 16 mm 5 VDC, I = 10 mA I2C serial link 1 in PPM-DOM 1 per DOM ( or perhaps the one of the Ocean Server compas will be accurate enough ) OceanServer Technology, OS4000-T heading accuracy : 0.5 degrees, 0.1 resolution Roll & Pitch full rotation (<1 °) dimensions : 15 x 15 x 3 mm 3.3V-5V, I < 30 mA TTL serial communication 1 in PPM-DOM 1 per DOM tiltmeter heading 3

Status on DOM instrumentation (for info)  Orientation : Compass and tilmeter 1 tiltmeter and 1 compass in the PPM-DOM need to have one tilt and heading measurement in each DOM for PMTs positioning in association with acoustic triangulation Antares experience :  compass has to be calibrated in situ using soft/hard iron internal algorithms  calibration done in situ for the LCM compasses  but not possible for the SCM because the it is attached to the BSS 4

Status on DOM instrumentation (for info)  Optical calibration : nanoBeacon (see Diego’s talk) 1 pulser : 17 x 28 mm + 1 control board : 45 x 75 x 10 mm 3.3 or 5 VDC, power < 160 mW pulse length : 2.5 ns, wavelenght : 470 nm internal or external LVDS trigger I2C control command nanoBeacon 1 in PPM-DOM 8 in NEMO phase II tower 1 or 2 per DOM Intra DU optical calibration  no need in Calibration Units 5

Status on DOM instrumentation (for info)  Relative Humidity and temperature sensors (from Diego) IST DigiPicco Basic I2C accuracy : ± 3%RH ; ± 0.5 °C dimensions : 10x47x2,8 mm 5 VDC, I < 3 mA I2C serial link 1 in PPM-DOM needed in each DOM ?  needed in any container (CU) ? RH and temperature board 6

Status on DOM instrumentation (for info)  Acoustics positioning : receiver (from Giorgio, Miquel, Robert) All data to shore : on shore acoustics detection algorithm, multidisciplinary sea science, neutrino detection ? A – internal hydrophone : piezo sensor (ECAP proposal) (see Salvo’s talk) dimensions : Ø 25,4 mm height 10 mm 3,3 VDC, I = 20 mA need of preamplification board digitalization made by AcouPlug (INFN) Preamplifier board on octopus Piezosensor in DOM no need for external DOM connector uncertainty on noise robustness 1 in PPM-DOM 2 in NEMO phase II in a single PM OM 1 per DOM 7

Status on DOM instrumentation (for info)  Acoustics positioning : receiver part B – external hydrophone : SMID (INFN) or FFR-SX30 (UPV) dimensions : Ø 29 mm height 188 mm 5 VDC, I = 80 mA integrates a preamplifier : + 38 dB digitalization made by AcouPlug (INFN) need for external DOM connector 1 in PPM-DOM 1 in PPM-DU ? tested in NEMO phase II tower acouPlug dimensions : Ø 29 mm height 188 mm 5 VDC, I = 200 mA 200 kHz, 24 bits I2S low noise preamplifier connected to CLB for clock and data transfer integration of acouPlug in CLB V2 under study SMID hydrophone 8

Instrumentation for Calibration Units (CU) 1 (or 2) external transducers (E/R) + one electronic board dimension : Ø 44 mm; height 25 mm frequency range : kHz [30 kHz] dB ref 1 m will be tested in IL12 mandatory on the fixed anchor of the CU could also be used as receiver hydrophone (/SMID)  will be tested in IL12 + NEMO phase II  Acoustic positioning : emitter part (from Miquel) FFR-SX30 Sensor Technology FFR-SX30 dimension : 105 x 73 mm 12 VDC I=1 mA + 5VDC I=100 mA max signal 400 pp ? RS232 serial link (or other possibility) external LVDS trigger signal on demand sinusoïdal, arbitrary, MLS signals Sound Emission Board SEB (UPV) SEB 9

10 Oceanographic Instruments for CU  Sound velocity (SV) evaluation (from Vincent) A- direct measurement : sound velocimeter Antares experience : unexpected behavior, data not used market study on SV performed in 2010 (P.Keller) B- Indirect measurement : CTD probes (conductivity, temperature, depth) computed from Chen and Millero formula Antares experience : all CTD probes data are in agreement Sound velocity used for alignement : one initial SV L1 measurement corrected by column of water height Hand made measurement between 2 short distances transducer ?  SV evaluation is needed How many ? SV reliability ? CTD ?

11 Instrumentation for Calibration Units (CU)  need to know the precise position of the acoustic emitter : need for heading and tilt of the fixed part of the CU Antares experience :  problem due to the metallic mass of the BSS, the heading given by the Compass board inside SCM is false  orientation has been measured by an external gyrocompass of the ROV for Calibration Unit :  local Compas/tilt measurement possible ? or external measurement (ROV) ?  Compass/tilt (from Vincent)  needed to have a precise measurement of each acoustic emitter depth (<10 cm) in alignment reconstruction Antares experience : BSS pressure sensors have a drift behavior. possibility to make measurement with an external accurate scientific sensor on ROV (Paroscientific type)  Pressure sensor (from Vincent)

Instrumentation for Calibration Units (CU)  Inter DU optical calibration : laser Beacon (see Diego’s talk)  Needed for the optical calibration dimension : Ø 142 mm; height 542 mm proposal : 48 V, power < 100 W wavelength : 532 nm serial link proposal : I2C pulses < 1 ns no synchronization needed will be tested in Antares IL12 and NEMO phase II up to 25 µJ expected for next version 1 every 6 DU ? Laser beacon 12

 RH/temperature Instrumentation for Calibration Units (CU)  do we need to monitor Relative Humidity and temperature in each CU container ? 13  Measurement off light transmissivity (from Vincent)  needed to evaluate the attenuation of Cherenkov light Antares experience : unexpected behavior of dedicated instrument (CSTAR) evaluation comes from LedBeacon studies  needed for KM3Net detector dedicated device ? Or could it be evaluated from optical calibration devices study ? How many ? Another possibility : used data from turbidimeter used in seascience lines  Seacurrent meter ( ADCP ) (from Vincent)  needed in KM3Net, to be defined  how many ?

Resume of instrument needs in CU DeviceFonction needed Device available for CU Need continuous data Backup solution Acoustic E/Ryes Currentmeteryes LaserBeaconyesYesyes Velocimeteryes??Use CTD sensors or compute SV from a constant ? Travel times on a short known distance ? Pressure sensor yes noExtra measurement from independant device Light transmissivity yes??Analyses from light Beacons or turbidimeter (oceanographic line ?) Compass/tiltyes?noExtra measurement from independant device RH/Temp.?yes 14

Some open questions ? Could the CLBV2 be used to interface the CU instruments ? Or Shall we need a new board to manage some interfaces from CU intruments ? Could we use the DOM power board or do we need a specific CU power board ? Definition of the container, connectics and mechanical interfaces Thank you for your kind attention 15