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Data acquisition system for the Baikal-GVD neutrino telescope Denis Kuleshov Denis Kuleshov Valday, February 3, 2015

Data acquisition system for the Baikal-GVD neutrino telescope Denis Kuleshov Valday, February 3, 2015

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Page 1: Data acquisition system for the Baikal-GVD neutrino telescope Denis Kuleshov Valday, February 3, 2015

Data acquisition system for the Baikal-GVD neutrino telescope

Denis KuleshovDenis Kuleshov Valday, February 3, 2015

Page 2: Data acquisition system for the Baikal-GVD neutrino telescope Denis Kuleshov Valday, February 3, 2015

1. GVD DAQ architecture

2. Basic elements of the telescope: - Optical module and measuring channel - OM Section and String - GVD Cluster - Underwater Cluster network

3. Reliability

Summary

OUTLINE

Page 3: Data acquisition system for the Baikal-GVD neutrino telescope Denis Kuleshov Valday, February 3, 2015

GVD DAQ architecture

Cluster DAQ center

Section electronic module

Optical module

String electronic module

SE

CT

ION

SE

CT

ION

ST

RIN

G

Basic principles of GVD design:- Simplicity of all elements;- Deployment convenience from the ice cover;- Detector extensibility and configuration

flexibility.

Basic GVD elements-Optical module (OM);

-Section: 12 OM (spaced by 15 m) Section electronic module (12-ch FADC)

-String: 2 or 3 Sections & String electronic module

-Cluster: 8 strings & DAQ center.

R ~ 60 mH

~ 35

0 m

Cluster with 8 two-section strings

Page 4: Data acquisition system for the Baikal-GVD neutrino telescope Denis Kuleshov Valday, February 3, 2015

Optical module and measuring channel

HV converter: SHV 12-2.0 K 1000 P 0 …+ 2000 VDC, stability 0.05% ripple and noise 8 mVpk-pk

Passive divider: 18 M2-channel amplifier: Output channel and PMT noise monitoring channel.

2 LEDs L7113: 470 nm, 5-7 ns- regulation of intensities in the range 1…~108 photons (100m Baikal water)- LED pulse delay regulation: 0 … 1000 ns

Slow control board: SiLabs C8051F121Control of electronics operation and monitoring of PMT parameters via RS485 interface.

OM electronics

Mu-metal cage

PMT

Optical gel

Glass sphere VETROVEX (17”)

Optical module design: as simple as possible.

OMSEM

PMT: 107 Ampl. ADC Board

90 m coax. cable

Page 5: Data acquisition system for the Baikal-GVD neutrino telescope Denis Kuleshov Valday, February 3, 2015

GVD Section

12-channel ADC unit: PMTs analog pulse conversion, time synchronization, data processing, local trigger.Data transmission: Two outputs of ADC board: optical output (for future detector extension) and 100 BASE-TX (present stage).shDSL modem: Extending the Ethernet line up to 1 km.Slow control board: OM power on/off and control of OM operation (RS-485).

Flash ADC (AD9430) 12bit, 200 MSPS

FPGA (Xilinx Spartan 6) Enable to on-line data filtration. Cut the pulses from data frame and paste to output data stream. Rejection factor : 50-100

Section electronic module

Optical output

Section (basic DAQ cell) – 12 OM and Section electronics module (SeM).

Page 6: Data acquisition system for the Baikal-GVD neutrino telescope Denis Kuleshov Valday, February 3, 2015

Functional scheme of one FADC channel

ADC 200 MSPS

Duble-buffered memory,

30 mks WF data

Datatransmitter

Data control

Peak detectorAmplitude analyser

Smoothing2-level

comparator

Inte

rface

Trigger/Stop

Waveform, 5 mks

Histogram

Request builder

Channel request

L

H

Smoothing level 1...8

Accumulation time

Waveform interval

Thresholds

PMTpulse

FPGAFADC (AD9430) 12bit, 200 MSPS FPGA (Xilinx Spartan 6) - Trigger logic: 2-level adjustable digital comparator forms low threshold L and high threshold H channel requests (section trigger is L&H coincidence of neighboring channels). - Data channel (triggered) consists of double-buffered memory and data transmitter.- Monitor channel (non-triggered) includes peak detector and amplitude analyzer.

LED pulse

Noise

Waveform stamp example (5 mks)

Single PE pulses

Monitor histogram examples

Monitor channelData channel

ADC channel

Page 7: Data acquisition system for the Baikal-GVD neutrino telescope Denis Kuleshov Valday, February 3, 2015

Trigger Commutator: splits for the section acknowledges & combines requests.

Data transmission: DSL line.

Power Commutator: Controls power to the SEM, OMs and peripherals.

String communication module combines 2 or 3 sections.

Functions:

GVD String

Functional scheme of Power Commutator

Page 8: Data acquisition system for the Baikal-GVD neutrino telescope Denis Kuleshov Valday, February 3, 2015

8

GVD ClusterCluster - a full functional detection system, working both independently and as a part

of the full detector.Cluster – 8 strings and DAQ center. DAQ center: trigger logic, string power supply, communication to shore.Cluster center electronics is located in 3 glass spheres and metallic box for optical cable attachment “optical box”.

Optical boxCluster DAQ center

Cluster DAQ center

Page 9: Data acquisition system for the Baikal-GVD neutrino telescope Denis Kuleshov Valday, February 3, 2015

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GVD Cluster

Power Module:300VDC 12-ch manageable commutator.

Optical Box: conversion 1000 BASE-FX to 100 BASE-TX.

Data module:8 DSL-modems for transmission the string data.8-channel COM-server for DSL speed control.

Trigger Module:12-channel ADC unit: 8 string trigger requests, global trigger for 8 strings.

Page 10: Data acquisition system for the Baikal-GVD neutrino telescope Denis Kuleshov Valday, February 3, 2015

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Cluster underwater network

Segments of underwater network:1. Section electronics module – String module2. String module – Cluster DAQ center3. Cluster DAQ center – Optical box4. Optical box – Shore DAQ center

100…200 Hz data event rate are expectedfor the basic trigger L×H.

Section Line speed, Кbit/s SNR, dB

String 1 7040 11

String 2 7552 12

String 3 10048 11

String 4 10048 10

String 5 10048 12

Segment Length Data rate

Line speed Technique

1 100…300 m

1 Mbit ~10 Mbit shDSL

2 ~1000 m 3 Mbit ~10 Mbit shDSL

3 3 m 25 Mbit 100 Mbit 100 BaseTX

4 ~6000 m 25 Mbit 1000 Mbit 1000 BaseFX

(1) Slow data transmission (triggered mode):OM coincidences produce a trigger that rejects the

PMT noise.

(2) Fast data transmission*: optical line from ADC module to Shore Center (all data to shore).

Possibility to use two modes of operation:

Data line speed in 2014

Page 11: Data acquisition system for the Baikal-GVD neutrino telescope Denis Kuleshov Valday, February 3, 2015

1. Optical modules:The OM electronics failure rate: 3 OM / 140 / Year - 1 OM: HV control system. Failure of the OM controller. - 2 OM: not connection via RS485 bus (out of operation at April 2014). Probable reason is transient error of the slow control board (it was modernized in late 2014). 2. Cable communications: 2 cables are out of operation. Reason - old technology of the sealing (cables of 2011). New sealing technology is applied after 2012.3. Network devices a) Industrial devices (Switches, Eternet-RS485 converters, IEX-402 DSL) – no failure b) Non-industrial DSL-modems: - Unreliable connection to 1 string at 2013 and 1 Section at 2014. We plan to use industrial IEX-402 shDSL, that were presented by MOXA firm at 2013.4. ADC boards - no failure.5. Glass sphere and Connectors - no failure.6. Power supply units (300 VDC commutators, DC/DC converters) - no failure

Reliability

(without long-term laboratory tests and stress tests)

Results from 2011 up to end of 2014

Page 12: Data acquisition system for the Baikal-GVD neutrino telescope Denis Kuleshov Valday, February 3, 2015

Summary

1. DAQ system was tested with 5-strings engineering array and will be applied

for GVD-Baikal full functional Cluster in this year.

2. Baikal-GVD technical design is basically finalized.

3. Next step of the DAQ development is investigation the possibility to use optical

connections with sections. - Optical hybrid cable is designed (connection between Cluster Center and

Shore)- Optical output of ADC board (SEM) is foreseen.- Optical connectors ???

Page 13: Data acquisition system for the Baikal-GVD neutrino telescope Denis Kuleshov Valday, February 3, 2015
Page 14: Data acquisition system for the Baikal-GVD neutrino telescope Denis Kuleshov Valday, February 3, 2015
Page 15: Data acquisition system for the Baikal-GVD neutrino telescope Denis Kuleshov Valday, February 3, 2015

Backup slides

Page 16: Data acquisition system for the Baikal-GVD neutrino telescope Denis Kuleshov Valday, February 3, 2015

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FADC (AD9430) 12bit, 200 MSPS FPGA (Xilinx Spartan 6) - Trigger logic: 2-level adjustable digital comparator forms low threshold L and high threshold H channel requests- Data channel (triggered) consists of double-buffered memory and data transmitter.- Monitor channel (non-triggered) includes peak detector and amplitude analyzer.

ADC board12-ch 200 MSPS

ADC

- Trigger logic(L&H coincidence of neighboring channels- Data readout from ADC buffer - Control of OM mode of operation - Connection via local Ethernet to the cluster DAQ center

Page 17: Data acquisition system for the Baikal-GVD neutrino telescope Denis Kuleshov Valday, February 3, 2015

Triggering and Data Transmission

SECTION CLUSTER

Page 18: Data acquisition system for the Baikal-GVD neutrino telescope Denis Kuleshov Valday, February 3, 2015

Prototype arrays: 2012: 36 OM, 2013: 72 OM, 2014: 120 OM

A summarized time of the OMs operation is ~170 years

3 OM failures during this period:

- 1 OM: HV control system out of operation (2013).

- 2 OM: not reliable connection via RS485 bus (2014).

The OM electronics failure rate ~2% / year

Repairing possibility: 8% / year for 100 strings installation (GVD Phase 1).

OM reliability

(without stress tests of electronics during prototyping phase )

Results from 2012 to 2014