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1 ENH1 Detector Integration Meeting 18/6/2015 D.Autiero (IPNL) WA105:  Detector installation requirements  Detector racks and power requirements Note:

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Presentation on theme: "1 ENH1 Detector Integration Meeting 18/6/2015 D.Autiero (IPNL) WA105:  Detector installation requirements  Detector racks and power requirements Note:"— Presentation transcript:

1 1 ENH1 Detector Integration Meeting 18/6/2015 D.Autiero (IPNL) WA105:  Detector installation requirements  Detector racks and power requirements Note: Just some first infos, quickly gathered given the very short notice of this meeting

2 2 Detectors installation requirements: Some discussion at the Neutrino Platform meeting on April 9th https://indico.cern.ch/event/385747/ “WA105 large prototype requirements (cryogenics and cryostats)” Detector Installation procedures studied in the LAGUNA-LBNO DS in collaboration with the industrial partners A few basic concepts reminded in the following slides taken from that presentation:  Use of the cryostat as clean room for detector assembly  Temporary Construction Opening (TCO) to insert materials inside the cryostat (opening dimensions redefined as a 3x2 m2 in Dimitar ’s first cryostat steel-frame design)  Clean Room Buffer in the pit, crane to bring materials to CRB from the EHN1 floor  Platform on top of the detector to access signal chimneys  Area for top-caps assembly A few slides from the presentation given on April 9th 

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6 3x1 top cap

7 Baseline WA105 design (TDR fig: 12,13,14)  12 signal chimneys in a central cross (4 « 3x1 like » top caps  HV FT  Slow control FTs not represented (4 FTs), can be integrated in signal top caps ?  Suspension FTs not represented (4 FTs)  Cryogenic and gas FTs and man-hole not represented  (to be put outside the 6x6 active area) responsibility of the cryogenic group

8 Cross of chimneys arranged in four «3x1 like» top caps We started discussing the constraints from the steel structure and interference of the I- beams in the structure with the positions of the feedthroughs

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10 10 Detectors racks and power requirements

11 11 uTCA crates Readout in groups of 640 channels/chimney  64O channels/chimney  1 uTCA crate/chimney  10 AMC digitization boards/crate, 64 ch./AMC  12 uTCA crates for charge readout + 1 uTCA crate for light readout uTCA charge readout architecture

12 12 Global uTCA DAQ architecture integrated with « White Rabbit » (WR) Time and Trigger distribution network + WR MCH slaves in uTCA crates

13 13 Online storage and data processing Defined basic architecture for local network, storage and computing:  Possibility to run with the beams without zero suppression at 100 Hz, event size 150 MB 15 GB/s, Huffman lossless compression under study  Online buffer storage up to ~PB  Online processing farm for event reconstruction, purity and gain analysis from cosmic ray tracks overlapped to beam events in a +-4ms window around the beam triggers

14 14 Preliminary power estimates:  DAQ system (13 uTCA crates) + FE + Slow Control and safety + counting room: ~60 kW (…+ some margin to be added)  Online storage and data processing (OSDP): 15 storage servers, 384 cores, metadata servers, configuration servers, switches: ~50 kW (…+ some margin to be added). OSDP evaluation based on preliminary design of the facility and offers from DELL corresponding to that design with detailed description of the components, space occupancy 4 racks  Air conditioning/cooling for the OSDP facility + DAQ back-end and time servers, (50+5 kW heath dissipation), cooling power ? Total occupancy 5 racks (4 OSDP + 1 DAQ BE+Time), minimal space 3x5 m2. No particular constraints on the place of the OSDP room (optical fiber links to the uTCA crates)  Air conditioning for the counting room (close to OSDP room ?)


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