The Multi-PMT Optical Module P.Kooijman, University of Amsterdam University of Utrecht Nikhef.

Slides:



Advertisements
Similar presentations
CDR Feb 2006Mar 2008Dec 2009 Mar Design Study Preparatory Phase TDR tendering construction data taking governance legal entity pre-production.
Advertisements

Peter Križan, Ljubljana Peter Križan University of Ljubljana and J. Stefan Institute The HERA-B RICH counter.
Basic Measurement of the Hamamatsu 10 inch PMT at –40 degree –40 degree Hiroko Miyamoto Dept. of Physics CHIBA University Angular Response of 10inch PMT.
Angular Response of 10inch PMT for IceCube Hiroko Miyamoto Dept. of Physics Chiba University.
Calibration of the 10inch PMT for IceCube Experiment 03UM1106 Kazuhiro Fujimoto A thesis submitted in partial fulfillment of the requirements of the degree.
Development of a thermal cooling system for a PMT (Photo Multiplier Tube) Summer Researcher Yasmine Salas Colorado State University Advisor: Dr. Julia.
Could CKOV1 become RICH? 1. Simulations 2. Sensitive area of the detection plane 3. Example of a workable solution 4. Geometrical efficiency of the photon.
The AMS-02 detector is based on a large acceptance (~0.5 m²sr) and high sensitivity spectrometer composed by a super-conducting magnet (0.8 T), cooled.
Veto Wall Test Hyupwoo Lee MINERvA/Jupiter Group Meeting Apr, 16, 2008.
Prototype string for a km3 Baikal neutrino telescope Roma International Conference on Astroparticle Physics V.Aynutdinov, INR RAS for the Baikal Collaboration.
A feasibility study for the detection of SuperNova explosions with an Undersea Neutrino Telescope A. Leisos, A. G. Tsirigotis, S. E. Tzamarias Physics.
Special Issues on Neutrino Telescopy Apostolos G. Tsirigotis Hellenic Open University School of Science & Technology Particle and Astroparticle Physics.
Antares/KM3NeT M. de Jong. neutrinos  p Scientific motivation: – origin cosmic rays – birth & composition relativistic jets – mechanism of cosmic particle.
Hamamatsu R7525 HA: outer conductive coating with insulating sleeve CC: convex-concave window mm thick (standard plano-concave: 1mm center, 6.1.
PD Kobe Univ. 06/29/2007 General performance of the IceCube detector and the calibration results I am Mina Inaba from Chiba university. I will.
Photon detection Visible or near-visible wavelengths
The Transverse detector is made of an array of 256 scintillating fibers coupled to Avalanche PhotoDiodes (APD). The small size of the fibers (5X5mm) results.
Proposal of new electronics integrated on the flanges for LAr TPC S. Cento, G. Meng CERN June 2014.
Report on SiPM Tests SiPM as a alternative photo detector to replace PMT. Qauntify basic characteristics Measure Energy, Timing resolution Develop simulation.
1 Performance of multi-anode PMT employing an ultra bi-alkali photo-cathode and rugged dynodes Takahiro Toizumi Tokyo Institute of Technology S. Inagwa.
In-Beam PET Status Report -- TPS. 2 TPS project PET monitoring prototype 2D view of the FOV coverage of the 4+4 modules Use of 4 modules vs. 4 modules.
1 S. E. Tzamarias Hellenic Open University N eutrino E xtended S ubmarine T elescope with O ceanographic R esearch Readout Electronics DAQ & Calibration.
Fast Detectors for Medical and Particle Physics Applications Wilfried Vogel Hamamatsu Photonics France March 8, 2007.
Experimental set-up Abstract Modeling of processes in the MCP PMT Timing and Cross-Talk Properties of BURLE Multi-Channel MCP PMTs S.Korpar a,b, R.Dolenec.
SINP MSU, July 7, 2012 I.Belolaptikov behalf BAIKAL collaboration.
Data acquisition system for the Baikal-GVD neutrino telescope Denis Kuleshov Valday, February 3, 2015.
Status of the NO ν A Near Detector Prototype Timothy Kutnink Iowa State University For the NOvA Collaboration.
Status of the PSD upgrade - Status of production of new temperature, HV control systems MAPD gain monitoring system. -Status of the PSD temperature stabilization.
Status of the Genova activity on a direction-sensitive optical module toward the KM3 detector M.Taiuti WP3 PYLOS 16/4/2007.
P.F.Timmer Nikhef Amsterdam Electronics- Technology Very low power, High Voltage base for a Photo Multiplier Tube for the KM3NeT deep sea neutrino telescope.
TOP counter overview and issues K. Inami (Nagoya university) 2008/7/3-4 2 nd open meeting for proto-collaboration - Overview - Design - Performance - Prototype.
Bbbbb 1.Introduction to ET Enterprises Ltd 2.Brief History 3.Product Range 4.Main Applications 5.Recent Developments 6.Current and Past projects 7.Summary.
CLAS12-RICH Mechanical Design Status-Report CLAS12 RICH Review September 5-6 th 2013 S. Tomassini, D. Orecchini1 D. Orecchini, S. Tomassini.
STATUS OF MUV3 CONSTRUCTION A joint IHEP Protvino – Mainz – Pisa project MUV3  Proposed by Italo Mannelli: Thick scintillator tiles with direct light.
AMS-RICH Detector. J. Berdugo – CIEMAT (Madrid, Spain) 1 AMS-02 Phase II Flight Safety Review AMS Ring Imaging CHerenkov PURPOSE: 1.Precise measurement.
HBD Gas and QE Monitoring Craig Woody BNL HBD Working Group Meeting October 19, 2005.
Barrel PID summary K.Inami (Nagoya) Summary of R&D at Hawaii, Cincinnati, Ljubljana and Nagoya.
FSC Status and Plans Pavel Semenov IHEP, Protvino on behalf of the IHEP PANDA group PANDA Russia workshop, ITEP 27 April 2010.
MPPC Test Setup Alam Toro S. 1. Objective Characterize main variables in ideal conditions To provide a setup to characterize multiple devices To provide.
HBD Report Craig Woody BNL DC Meeting January 7, 2009.
FT Prototype Test Purpose: test the prototype of the FT Calorimeter and Scintillator Hodoscope Technique: prototype is installed under the Hall B photon.
PSD upgrade: concept and plans - Why the PSD upgrade is necessary? - Concept of the PSD temperature stabilization and control - Upgrade of HV control system.
PMT and WLS activities at IHEP Vladimir Rykalin IHEP, Protvino CBM meeting JINR Dubna, October 2008.
CDMS II Shielding To Installation To Construction From Design.
The VSiPMT: A new Generation of Photons Detectors G. Barbarino 1,2, F. C. T. Barbato 1,2, R. de Asmundis 2, G. De Rosa 1,2, F. Di Capua 1, P. Migliozzi.
Status of NEWCHOD E.Guschin (INR), S.Kholodenko (IHEP), Yu.Kudenko (INR), I.Mannelli (Pisa), O.Mineev (INR), V.Obraztsov (IHEP), V.Semenov(IHEP), V.Sugonyaev.
G. Kieft Nikhef Amsterdam Electronics- Technology PMT tubes PMT bases PMT asic’s Automatic tester for PMT bases Camac test set-up for PMT tubes LeCroy.
STATUS AND PHYSICS GOALS OF KM3NET Paolo Piattelli P. Piattelli, ICHEP14 Valencia INFN – LNS, Catania (Italy)
Internal Structure of Multi PMT DOM
Silicon Photomultiplier Development at GRAPES-3 K.C.Ravindran T.I.F.R, OOTY WAPP 2010 Worshop On behalf of GRAPES-3 Collaboration.
DOM Electronics (Digital Optical Module) 1 WPFLElectronics PPMDOM ElectronicsF. Louis.
The photomultiplier tubes selection for KM2A electromagnetic particle detectors (EDs) hou chao IHEP The 2nd workshop of air shower detection at high altitudes.
WP F/L Dom production. KM3Net meeting 2012 Erlangen - Edward Berbee - Nikhef22/06/20121.
DOM assembly KM3NeT collaboration meeting Assembly Edward Berbee The cooling mushroom is put in place with tooling, a minimum amount of.
Status report Els de Wolf Annual Meeting 2011, Nikhef.
Shashlyk DAQ and FEE Status and Plans Pavel Semenov IHEP, Protvino on behalf of the IHEP PANDA group PANDA DAQ and FEE Workshop, Rauischholzhausen Castle.
Organizing future KM3NeT production 06-July-2010.
Wild ideas on photon detection P.Kooijman, NIKHEF.
Multi-PMT DOM P.Kooijman University of Amsterdam-GRAPPA Presentation for SSC.
Status procurement of PMTs Oleg Kalekin KM3NeT WPF/L General Meeting Amsterdam
Write-up and Definitions for Cost Model
Status multiPMT OM design
ASTRI camera status Giovanni LA ROSA
P.Kooijman, UVA-GRAPPA, UU, Nikhef
SUMMARY OF THE ORSAY LD-TPC ELECTRONICS MEETING
Multi PMT P.Kooijman Just 1.
Phototube response for a multi-element Optical Module
CLAS12 Forward Detector Element PCAL
Directional Optical Module Integration
Development of hybrid photomultiplier for Hyper-Kamiokande
Presentation transcript:

The Multi-PMT Optical Module P.Kooijman, University of Amsterdam University of Utrecht Nikhef

What is a Multi PMT optical module? Why build a Multi PMT optical module? Requirements Status How to build one CONTENT

WHAT IS A MULTI PMT OPTICAL MODULE? An optical module containing many small PMTs rather than one big one Contains all electronics necessary to read out and control the module Is a self contained unit

Why build a Multi PMT optical module? Can put much more photo- cathode area in a single pressure sphere ‐1260 cm 2 or more with ring ( Oksana ) More compact design ‐Only one sphere to handle ‐3” PMT easy to manipulate ‐1 sphere vs 3 spheres Quite uniform angular acceptance. ‐Reconstruction of downward going muons Counting photons = counting PMTs ‐90% of all 2spe hits are 2PMT hits ‐ 40 K background Less sensitive to failure

REQUIREMENTS Can fit sufficient photomultipliers in a reasonably sized sphere –31 3” Photomultipliers in a 17” sphere –Supported by foam –Optical contact through gel Can house the HV generation inside sphere. –Special HV low power including amplifier Readout electronics must not be 31times –Time over threshold readout House readout electronics in sphere Power dissipation must not lead to excessive temperature inside the sphere Reliability at the level of a few percent failures for ten years

PHOTOMULTIPLIERS Was a Photonis tube XP53B20 – 76 mm cathode diameter – Bialkali cathode, Q.E. 35% – Convex front matching sphere – 10 stage – Gain 5 (1) x 10 6 Photonis is no more for PMTs Hamamatsu has provided prototype (plano-convex) Discussions with ETL towards a prototype concave convex

ELECTRONICS BOARDS HV on the back of PMT together with amplifier and comparator. Signals collected on stem of mushroom Storey logic board for signal processing and communications electronics Converter board for DC/DC converters. Shielded by Aluminium Space for other instrumentation also on auxiliary boards

Estimate 10 W 31 * 30 mW (HV 4.5 mW) (D) DC/DC converters (A) FPGA etc. (B) Data transmission electronics (B) POWER DISSIPATION Aluminium Cooling Mushroom

TEMPERATURE TESTS Temperatures remain low in tests 4W on each electronics board 60 mW on PMT base T 1 ( o C) T 7 ( o C) T 9 ( o C) T 11 ( o C) T 12 ( o C) T 13 ( o C) 20.4/ / / / / /19.2

CONSTRUCTION add optical gel lower hemisphere

CONSTRUCTION upper hemisphere glue add optical gel storage closing the sphere Light-tight box

TESTING Acceptance testing PMTs ( or 1000 /week ) Bases ( or 1000 /week ) PC boards (2x6000 or 60/week ) Assembly testing: Go/nogo test top half of module Go/nogo test of installed PC boards and connectivity Go/nogo test lower half Test of full optical module Standalone using complete readout Burn in and functionality (30/week) Final test before mounting on DU only connectivity

CONCLUSIONS The Multi PMT optical module : Is Compact (lots of photocathode area) Standalone (tests and failures only affect one module) Reliable (necessary FIT rates are achievable) Buildable almost anywhere (no large assembly hall needed) Has Acceptance uniformity (muon background) High granularity (two photon sensitivity)