Commit 35a425dc authored by Maciej Lipinski's avatar Maciej Lipinski

included all but one (figure clarity) feedback

parent 95f065f4
@misc{biblio:whiteRabbit, @misc{biblio:whiteRabbit,
title = "{White Rabbit Project}", title = "{White Rabbit Project}",
howpublished = {\url{www.ohwr.org/projects/white-rabbit}}, howpublished = {\url{www.ohwr.org/projects/white-rabbit}},
} }
@ARTICLE{biblio:802.1Q, @ARTICLE{biblio:802.1Q,
journal="{IEEE Std 802.1Q-2014}", journal="{IEEE Std 802.1Q-2014}",
title = {{IEEE Standard for LAN}}, title = {{IEEE Standard for LAN}},
year={2014}, year={2014},
month={Dec}, month={Dec},
keywords={IEEE standards;access protocols;local area networks;metropolitan area networks;IEEE standard;MAC service;VLAN bridges;bridged networks;local area networks;media access control service;metropolitan area networks;Bridged circuits;IEEE standards;Local area networks;Media Access Protocol;Metropolitan area networks;Protofcols;Virtual environments;Bridged Network;IEEE 802.1Q(TM);LAN;MAC Bridge;MSTP;Multiple Spanning Tree Protocol;PBN;Provider Bridged Network;RSTP;Rapid Spanning Tree Protocol;SPB Protocol;Shortest Path Bridging Protocol;VLAN Bridge;Virtual Bridged Network;local area network;metropolitan area networks;virtual LAN}, keywords={IEEE standards;access protocols;local area networks;metropolitan area networks;IEEE standard;MAC service;VLAN bridges;bridged networks;local area networks;media access control service;metropolitan area networks;Bridged circuits;IEEE standards;Local area networks;Media Access Protocol;Metropolitan area networks;Protofcols;Virtual environments;Bridged Network;IEEE 802.1Q(TM);LAN;MAC Bridge;MSTP;Multiple Spanning Tree Protocol;PBN;Provider Bridged Network;RSTP;Rapid Spanning Tree Protocol;SPB Protocol;Shortest Path Bridging Protocol;VLAN Bridge;Virtual Bridged Network;local area network;metropolitan area networks;virtual LAN},
doi={10.1109/IEEESTD.2014.6991462},} doi={10.1109/IEEESTD.2014.6991462},}
@online{biblio:allan90, @online{biblio:allan90,
author = {D.B. Sullivan and D.W. Allan and D.A. Howe and F.L. Walls}, author = {D.B. Sullivan and D.W. Allan and D.A. Howe and F.L. Walls},
title = {{Characterization of Clocks and Oscillators}}, title = {{Characterization of Clocks and Oscillators}},
url = {tf.nist.gov/general/pdf/868.pdf}, url = {tf.nist.gov/general/pdf/868.pdf},
note = "{NIST Technical Note 1337}", note = "{NIST Technical Note 1337}",
urldate = {1990}, urldate = {1990},
} }
@article{biblio:IEEE802.3, @article{biblio:IEEE802.3,
journal="{IEEE 802.3-2012}", journal="{IEEE 802.3-2012}",
title = {{IEEE Standard for Ethernet}}, title = {{IEEE Standard for Ethernet}},
doi = {10.1109/IEEESTD.2012.6419735}, doi = {10.1109/IEEESTD.2012.6419735},
abstract = {Ethernet local area network operation is specified for selected speeds of operation from 1 Mb/s to 100 Gb/s using a common media access control ({MAC}) specification and management information base ({MIB}). The Carrier Sense Multiple Access with Collision Detection ({CSMA}/{CD}) {MAC} protocol specifies shared medium (half duplex) operation, as well as full duplex operation. Speed specific Media Independent Interfaces ({MIIs}) allow use of selected Physical Layer devices ({PHY}) for operation over coaxial, twisted-pair or fiber optic cables. System considerations for multisegment shared access networks describe the use of Repeaters that are defined for operational speeds up to 1000 Mb/s. Local Area Network ({LAN}) operation is supported at all speeds. Other specified capabilities include various {PHY} types for access networks, {PHYs} suitable for metropolitan area network applications, and the provision of power over selected twisted-pair {PHY} types.}, abstract = {Ethernet local area network operation is specified for selected speeds of operation from 1 Mb/s to 100 Gb/s using a common media access control ({MAC}) specification and management information base ({MIB}). The Carrier Sense Multiple Access with Collision Detection ({CSMA}/{CD}) {MAC} protocol specifies shared medium (half duplex) operation, as well as full duplex operation. Speed specific Media Independent Interfaces ({MIIs}) allow use of selected Physical Layer devices ({PHY}) for operation over coaxial, twisted-pair or fiber optic cables. System considerations for multisegment shared access networks describe the use of Repeaters that are defined for operational speeds up to 1000 Mb/s. Local Area Network ({LAN}) operation is supported at all speeds. Other specified capabilities include various {PHY} types for access networks, {PHYs} suitable for metropolitan area network applications, and the provision of power over selected twisted-pair {PHY} types.},
date = {2012-12}, date = {2012-12},
keywords = {1000BASE, 100BASE, 100GBASE, 100 Gigabit Ethernet, 10BASE, 10GBASE, 10 Gigabit Ethernet, 40GBASE, 40 Gigabit Ethernet, attachment unit interface, {AUI}, Auto Negotiation, Backplane Ethernet, bit rate 1 Mbit/s to 100 Gbit/s, carrier sense multiple access, carrier sense multiple access with collision detection, coaxial cable, coaxial cables, computer network management, {CSMA}-{CD}, data processing, {DTE} Power via the {MDI}, {EPON}, Ethernet, Ethernet in the First Mile, Ethernet networks, Ethernet passive optical network, Fast Ethernet, formal specification, full duplex operation, Gigabit Ethernet, {GMII}, {IEEE} standards, {IEEE} Std 802.3-2008 Revision, {IEEE} Std 802.3-2012, information exchange, local area network, {MAC} protocol specification, management, management information base, {MDI}, media access control, media independent interface, medium dependent interface, metropolitan area network, Metropolitan area networks, {MIB}, {MII}, multisegment shared access network, network interfaces, keywords = {1000BASE, 100BASE, 100GBASE, 100 Gigabit Ethernet, 10BASE, 10GBASE, 10 Gigabit Ethernet, 40GBASE, 40 Gigabit Ethernet, attachment unit interface, {AUI}, Auto Negotiation, Backplane Ethernet, bit rate 1 Mbit/s to 100 Gbit/s, carrier sense multiple access, carrier sense multiple access with collision detection, coaxial cable, coaxial cables, computer network management, {CSMA}-{CD}, data processing, {DTE} Power via the {MDI}, {EPON}, Ethernet, Ethernet in the First Mile, Ethernet networks, Ethernet passive optical network, Fast Ethernet, formal specification, full duplex operation, Gigabit Ethernet, {GMII}, {IEEE} standards, {IEEE} Std 802.3-2008 Revision, {IEEE} Std 802.3-2012, information exchange, local area network, {MAC} protocol specification, management, management information base, {MDI}, media access control, media independent interface, medium dependent interface, metropolitan area network, Metropolitan area networks, {MIB}, {MII}, multisegment shared access network, network interfaces,
optical fibre {LAN}, optical repeaters, Passive optical networks, {PHY}, physical coding sublayer, Physical layer, physical layer device, physical medium attachment, {PMA}, Power over Ethernet, repeater, twisted pair cable, twisted pair cables, type field, {VLAN} {TAG}, {XGMII}} optical fibre {LAN}, optical repeaters, Passive optical networks, {PHY}, physical coding sublayer, Physical layer, physical layer device, physical medium attachment, {PMA}, Power over Ethernet, repeater, twisted pair cable, twisted pair cables, type field, {VLAN} {TAG}, {XGMII}}
} }
@article{biblio:IEEE1588, @article{biblio:IEEE1588,
journal = "{IEEE 1588-2008}", journal = "{IEEE 1588-2008}",
title = "{IEEE} {Standard} for {PTP}", title = "{IEEE} {Standard} for {PTP}",
organization = "IEEE", organization = "IEEE",
address = "New York", address = "New York",
} }
@Misc{biblio:WRPTP, @Misc{biblio:WRPTP,
author = "E.G. Cota and M. Lipi\'{n}ski et al.", author = "E.G. Cota and M. Lipi\'{n}ski et al.",
title = "{White Rabbit Specification: Draft for Comments}", title = "{White Rabbit Specification: Draft for Comments}",
month = "July", month = "July",
year = "2011", year = "2011",
howpublished = {\url{www.ohwr.org/attachments/1169/WhiteRabbitSpec.v2.0.pdf}}, howpublished = {\url{www.ohwr.org/attachments/1169/WhiteRabbitSpec.v2.0.pdf}},
} }
@inproceedings{biblio:ISPCS2011, @inproceedings{biblio:ISPCS2011,
author = "M. Lipi\'{n}ski and et al.", author = "M. Lipi\'{n}ski and et al.",
title = "{White Rabbit: a PTP application for robust sub-nanosecond synchronization}", title = "{White Rabbit: a PTP application for robust sub-nanosecond synchronization}",
booktitle = "ISPCS", booktitle = "ISPCS",
year = "2011", year = "2011",
} }
@Inproceedings{biblio:WRproject, @Inproceedings{biblio:WRproject,
author = "J. Serrano and et al.", author = "J. Serrano and et al.",
title = "{The White Rabbit Project}", title = "{The White Rabbit Project}",
booktitle = "ICALEPCS", booktitle = "ICALEPCS",
year = "2015", year = "2015",
} }
@mastersthesis{biblio:TomekMSc, @mastersthesis{biblio:TomekMSc,
author = "T. W\l{}ostowski", author = "T. W\l{}ostowski",
title = "Precise time and frequency transfer in a {White} {Rabbit} network", title = "Precise time and frequency transfer in a {White} {Rabbit} network",
year = "2011", year = "2011",
school = "Warsaw University of Technology", school = "Warsaw University of Technology",
note = {\url{www.ohwr.org/documents/80}}, note = {\url{www.ohwr.org/documents/80}},
} }
@phdthesis{biblio:MaciekPhD, @phdthesis{biblio:MaciekPhD,
author = "Lipinski, Maciej", author = "Lipinski, Maciej",
title = "{Methods to Increase Reliability and Ensure title = "{Methods to Increase Reliability and Ensure
Determinism in a White Rabbit Network}", Determinism in a White Rabbit Network}",
year = "2016", year = "2016",
school = "Warsaw University of Technology", school = "Warsaw University of Technology",
note = {\url{cds.cern.ch/record/2261452}}, note = {\url{cds.cern.ch/record/2261452}},
} }
@phdthesis{biblio:CesarPhD, @phdthesis{biblio:CesarPhD,
author = "Prados, Cesar", author = "Prados, Cesar",
title = "{Rock Solid WR Network for GSI/FAIR Control System}", title = "{Rock Solid WR Network for GSI/FAIR Control System}",
year = "Unpublished", year = "Unpublished",
school = "Technische Universität Darmstadt", school = "Technische Universität Darmstadt",
address = "Darmstadt, Germany" address = "Darmstadt, Germany"
} }
@ARTICLE{biblio:JosePhD, @ARTICLE{biblio:JosePhD,
author={F. Ramos and et al.}, author={F. Ramos and et al.},
journal={IEEE Transactions on Industrial Informatics}, journal={IEEE Transactions on Industrial Informatics},
title={Accurate Timing Networks for Dependable Smart Grid Applications}, title={Accurate Timing Networks for Dependable Smart Grid Applications},
year={2018}, year={2018},
} }
@online{biblio:CERN, @online{biblio:CERN,
title = {{European Organization for Nuclear Research (CERN)}}, title = {{European Organization for Nuclear Research (CERN)}},
url = {www.cern.ch/}, url = {www.cern.ch/},
howpublished = {\url{www.cern.ch/}}, howpublished = {\url{www.cern.ch/}},
abstract = {{CERN}, the European Organization for Nuclear Research, is one of the world’s largest and most respected centres for scientific research. Its business is fundamental physics, finding out what the Universe is made of and how it works.}, abstract = {{CERN}, the European Organization for Nuclear Research, is one of the world’s largest and most respected centres for scientific research. Its business is fundamental physics, finding out what the Universe is made of and how it works.},
urldate = {2014-06-17}, urldate = {2014-06-17},
keywords = {{CERN}, high-energy physics, Large Hadron Collider, {LHC}, particles, physics, science}, keywords = {{CERN}, high-energy physics, Large Hadron Collider, {LHC}, particles, physics, science},
} }
@inproceedings{biblio:GMT, @inproceedings{biblio:GMT,
author = "J. Serrano and et al.", author = "J. Serrano and et al.",
title = "{Nanosecond} {Level} {UTC} {Timing} {Generation} and {Stamping} in {CERN}'s {LHC}", title = "{Nanosecond} {Level} {UTC} {Timing} {Generation} and {Stamping} in {CERN}'s {LHC}",
booktitle = "ICALEPCS", booktitle = "ICALEPCS",
year = "2013", year = "2013",
} }
@misc{biblio:GMTJavierPres, @misc{biblio:GMTJavierPres,
title = {{CERN} {General} {Machine} {Timing} {System}: status and evolution}, title = {{CERN} {General} {Machine} {Timing} {System}: status and evolution},
author = {{J. Serrano}}, author = {{J. Serrano}},
date = {2008-02-15}, date = {2008-02-15},
note= {{CERN Presentation}}, note= {{CERN Presentation}},
year=2008, year=2008,
file = {CERN-GMT.pdf:/home/mlipinsk/.mozilla/firefox/64taeemp.default-1397950810482/zotero/storage/F3RGN3RC/CERN-GMT.pdf:application/pdf}, file = {CERN-GMT.pdf:/home/mlipinsk/.mozilla/firefox/64taeemp.default-1397950810482/zotero/storage/F3RGN3RC/CERN-GMT.pdf:application/pdf},
howpublished = {\url{indico.cern.ch/event/28233/contribution/1/material/slides/1.pdf}}, howpublished = {\url{indico.cern.ch/event/28233/contribution/1/material/slides/1.pdf}},
} }
@Inproceedings{P1588-HA-enhancements, @Inproceedings{P1588-HA-enhancements,
author={O. Ronen and M. Lipinski}, author={O. Ronen and M. Lipinski},
booktitle={ISPCS2015}, booktitle={ISPCS2015},
title={Enhanced synchronization accuracy in {IEEE1588}}, title={Enhanced synchronization accuracy in {IEEE1588}},
} }
@electronic{biblio:fmc-dio-5cha, @electronic{biblio:fmc-dio-5cha,
title = "{FMC 5-channel Digital I/O module}", title = "{FMC 5-channel Digital I/O module}",
howpublished = {\url{www.ohwr.org/projects/fmc-dio-5chttla/wiki/wiki}} howpublished = {\url{www.ohwr.org/projects/fmc-dio-5chttla/wiki/wiki}}
} }
@electronic{biblio:fmc-dio-del, @electronic{biblio:fmc-dio-del,
title = "{MC DEL 1ns 4cha delay module }", title = "{MC DEL 1ns 4cha delay module }",
howpublished = {\url{www.ohwr.org/projects/fmc-delay-1ns-8cha/wiki/wiki}} howpublished = {\url{www.ohwr.org/projects/fmc-delay-1ns-8cha/wiki/wiki}}
} }
@electronic{biblio:fmc-tdc-5cha, @electronic{biblio:fmc-tdc-5cha,
title = "{FMC TDC 1ns 5cha}", title = "{FMC TDC 1ns 5cha}",
howpublished = {\url{www.ohwr.org/projects/fmc-tdc/wiki/wiki}} howpublished = {\url{www.ohwr.org/projects/fmc-tdc/wiki/wiki}}
} }
@misc{biblio:WR@LIST, @misc{biblio:WR@LIST,
title = {{LHC} {Instabilities} {Trigger} {Distribution}}, title = {{LHC} {Instabilities} {Trigger} {Distribution}},
url = {https://indico.cern.ch/event/295937/contribution/1/material/slides/0.pdf}, url = {https://indico.cern.ch/event/295937/contribution/1/material/slides/0.pdf},
author = {T. Wlostowski}, author = {T. Wlostowski},
note="{CERN Presentation}", note="{CERN Presentation}",
howpublished = {\url{indico.cern.ch/event/295937/contribution/1/material/slides/0.pdf}}, howpublished = {\url{indico.cern.ch/event/295937/contribution/1/material/slides/0.pdf}},
date ="2014" date ="2014"
} }
@inproceedings{biblio:WR-LIST, @inproceedings{biblio:WR-LIST,
author = "T. Wlostowski and et al.", author = "T. Wlostowski and et al.",
title = "{Trigger and RF distribution using White Rabbit}", title = "{Trigger and RF distribution using White Rabbit}",
booktitle = "{ICALEPCS}", booktitle = "{ICALEPCS}",
year = "2015", year = "2015",
} }
@inproceedings{biblio:WR-LIST-2, @inproceedings{biblio:WR-LIST-2,
author = "T. Levens and et al.", author = "T. Levens and et al.",
title = "INSTABILITY DIAGNOSTICS", title = "INSTABILITY DIAGNOSTICS",
booktitle = "{Evian Workshop}", booktitle = "{Evian Workshop}",
year = "2015", year = "2015",
} }
@electronic{biblio:wr-streamers, @electronic{biblio:wr-streamers,
title = "{White Rabbit Streamers IP Core}", title = "{White Rabbit Streamers IP Core}",
howpublished = {\url{www.ohwr.org/projects/wr-cores/wiki/wr-streamers}} howpublished = {\url{www.ohwr.org/projects/wr-cores/wiki/wr-streamers}}
} }
@INPROCEEDINGS{biblio:wr-cngs, @INPROCEEDINGS{biblio:wr-cngs,
author={M. Lipinski and et al.}, author={M. Lipinski and et al.},
booktitle={Proceedings of ISPCS2012}, booktitle={Proceedings of ISPCS2012},
title={Performance results of the first White Rabbit installation for CNGS time transfer}, title={{Performance results of the first White Rabbit installation for CNGS time transfer}},
year={2012}, year={2012},
} }
@Misc{biblio:PolaRx4e, @Misc{biblio:PolaRx4e,
title = "{PolaRx4/PolaRx4TR: Multi-frequency GNSS Reference Station}", title = "{PolaRx4/PolaRx4TR: Multi-frequency GNSS Reference Station}",
} }
@Misc{biblio:CS4000, @Misc{biblio:CS4000,
title = "{Symmetricom frequency standards, Time and Frequency Systems}", title = "{Symmetricom frequency standards, Time and Frequency Systems}",
} }
@online{biblio:WR-Btrain-MM, @online{biblio:WR-Btrain-MM,
title = "{Real-Time Distribution of Magnetic Field Measurements Over White-Rabbit}", title = "{Real-Time Distribution of Magnetic Field Measurements Over White-Rabbit}",
year = "2016", year = "2016",
author = "M. Roda", author = "M. Roda",
urldate = "2016-03-16", urldate = "2016-03-16",
howpublished = {\url{www.ohwr.org/attachments/4270/2\_PS-BTrain-9th-WR-workshop-Marco\_Roda.pdf}} howpublished = {\url{www.ohwr.org/attachments/4270/2\_PS-BTrain-9th-WR-workshop-Marco\_Roda.pdf}}
} }
@Misc{biblio:WR-Btrain, @Misc{biblio:WR-Btrain,
title = "{{BTrain} over White Rabbit}", title = "{{BTrain} over White Rabbit}",
howpublished = "{\url{gitlab.cern.ch/BTrain-TEAM/Btrain-over-WhiteRabbit/wikis/home}}" howpublished = "{\url{gitlab.cern.ch/BTrain-TEAM/Btrain-over-WhiteRabbit/wikis/home}}"
} }
@Misc{biblio:WR-Btrain-status, @Misc{biblio:WR-Btrain-status,
author = "Maciej Lipinski", author = "Maciej Lipinski",
title = "{Real-Time distribution of magnetic field values using White Rabbit the FIRESTORM project}", title = "{Real-Time distribution of magnetic field values using White Rabbit the FIRESTORM project}",
howpublished = {\url{www.ohwr.org/attachments/5795/BE-CO-TM-WR-BTrain.pdf}} howpublished = {\url{www.ohwr.org/attachments/5795/BE-CO-TM-WR-BTrain.pdf}}
} }
@inproceedings{biblio:WR-BTrain-RF, @inproceedings{biblio:WR-BTrain-RF,
author = "D. Perrelet and et al.", author = "D. Perrelet and et al.",
title = "{White-Rabbit Based Revolution Frequency Program for the Longitudinal Beam Control of the CERN PS}", title = "{White-Rabbit Based Revolution Frequency Program for the Longitudinal Beam Control of the CERN PS}",
booktitle = "{ICALEPCS}", booktitle = "{ICALEPCS}",
year = "2015", year = "2015",
} }
@inproceedings{biblio:NPL,
@Misc{biblio:FAIRtimingSystem, author = "P. Whibberley and et al.",
author = "T. Fleck and et al.", title = "{Evaluation of White Rabbit for Time Service Distribution}",
title = "{FAIR Timing System}", booktitle = "{EFTF2018}",
institution = "GSI", year = "2018",
address = "Darmstadt, Germany",
year = "2009", }
}
@Misc{biblio:FAIRtimingSystem,
author = "T. Fleck and et al.",
@inproceedings{biblio:WR-GSI, title = "{FAIR Timing System}",
author = "C. Prados and et al.", institution = "GSI",
title = "{A Reliable White Rabbit Network for the FAIR General Machine Timing}", address = "Darmstadt, Germany",
booktitle = "{ICALEPCS}", year = "2009",
year = "2017", }
howpublished = "{\url{accelconf.web.cern.ch/AccelConf/icalepcs2017/papers/tupha091.pdf}}"
}
@inproceedings{biblio:WR-GSI,
@thesis{biblio:MathiasPhD, author = "C. Prados and et al.",
author = "Kreider, Mathias", title = "{A Reliable White Rabbit Network for the FAIR General Machine Timing}",
title = "{On Time, in Style: Nanosecond Accuracy in Network Control Systems}", booktitle = "{ICALEPCS}",
year = "2017", year = "2017",
school = "University of Wales", howpublished = "{\url{accelconf.web.cern.ch/AccelConf/icalepcs2017/papers/tupha091.pdf}}"
howpublished = "{\url{www-acc.gsi.de/wiki/pub/Timing/TimingSystemDocuments/kreiderPhdwiki.pdf}}" }
}
@Misc{biblio:GSI-schedule, @thesis{biblio:MathiasPhD,
title = "{GSI - General Plan of Accelerator Operation 2018}", author = "Kreider, Mathias",
} title = "{On Time, in Style: Nanosecond Accuracy in Network Control Systems}",
@Misc{biblio:OHWR, year = "2017",
title = "{Open Hardware Repository}", school = "University of Wales",
howpublished = {\url{www.ohwr.org}}, howpublished = "{\url{www-acc.gsi.de/wiki/pub/Timing/TimingSystemDocuments/kreiderPhdwiki.pdf}}"
} }
@Misc{biblio:wr-switch, @Misc{biblio:GSI-schedule,
title = "{WR Switch}", title = "{GSI - General Plan of Accelerator Operation 2018}",
howpublished = {\url{www.ohwr.org/projects/white-rabbit/wiki/switch}}, }
} @Misc{biblio:OHWR,
@Misc{biblio:wr-node, title = "{Open Hardware Repository}",
title = "{WR Node}", howpublished = {\url{www.ohwr.org}},
howpublished = {\url{www.ohwr.org/projects/white-rabbit/wiki/node}}, }
} @Misc{biblio:wr-switch,
@Misc{biblio:spec, title = "{WR Switch}",
title = "{Simple PCIe FMC carrier}", howpublished = {\url{www.ohwr.org/projects/white-rabbit/wiki/switch}},
howpublished = {\url{www.ohwr.org/projects/spec/wiki}}, }
} @Misc{biblio:wr-node,
@Misc{biblio:svec, title = "{WR Node}",
title = "{Simple VME FMC Carrier}", howpublished = {\url{www.ohwr.org/projects/white-rabbit/wiki/node}},
howpublished = {\url{www.ohwr.org/projects/svec/wiki}}, }
} @Misc{biblio:spec,
@Misc{biblio:crio, title = "{Simple PCIe FMC carrier}",
title = "{CompactRIO White Rabbit}", howpublished = {\url{www.ohwr.org/projects/spec/wiki}},
howpublished = {\url{www.ohwr.org/projects/crio-wr/wiki}}, }
} @Misc{biblio:svec,
@Misc{biblio:AFC, title = "{Simple VME FMC Carrier}",
title = "{AMC FMC Carrier}", howpublished = {\url{www.ohwr.org/projects/svec/wiki}},
howpublished = {\url{www.ohwr.org/projects/afc/wiki}}, }
} @Misc{biblio:crio,
@Misc{biblio:AFCK, title = "{CompactRIO White Rabbit}",
title = "{AMC FMC Kindex Carrier}", howpublished = {\url{www.ohwr.org/projects/crio-wr/wiki}},
howpublished = {\url{www.ohwr.org/projects/afck/wiki}}, }
} @Misc{biblio:AFC,
@Misc{biblio:cute-wr-dp, title = "{AMC FMC Carrier}",
title = "{Compact Universal Timing Endpoint Based on White Rabbit with Dual Ports}", howpublished = {\url{www.ohwr.org/projects/afc/wiki}},
howpublished = {\url{www.ohwr.org/projects/cute-wr-dp/wiki}}, }
} @Misc{biblio:AFCK,
@Misc{biblio:spexi, title = "{AMC FMC Kindex Carrier}",
title = "{Simple PXI express FMC Carrier Board}", howpublished = {\url{www.ohwr.org/projects/afck/wiki}},
howpublished = {\url{www.ohwr.org/projects/spexi/wiki}}, }
} @Misc{biblio:cute-wr-dp,
@Misc{biblio:STRUCK, title = "{Compact Universal Timing Endpoint Based on White Rabbit with Dual Ports}",
title = "{SIS1160 8 LANE GEN3 PCI EXPRESS CARRIER FOR DIGITIZER FMCS}", howpublished = {\url{www.ohwr.org/projects/cute-wr-dp/wiki}},
howpublished = {\url{www.struck.de/sis1160.html}}, }
} @Misc{biblio:spexi,
@Misc{biblio:sundance, title = "{Simple PXI express FMC Carrier Board}",
title = "{Sundance PXIe700}", howpublished = {\url{www.ohwr.org/projects/spexi/wiki}},
howpublished = {\url{www.sundance.technology/som-cariers/pxi-boards/pxie700/}}, }
} @Misc{biblio:STRUCK,
@Misc{biblio:spdevices, title = "{SIS1160 8 LANE GEN3 PCI EXPRESS CARRIER FOR DIGITIZER FMCS}",
title = "{DAQ Unit - Digitizer: 14-bit, 10 GSPS digitizer platform, 1-2 chan}", howpublished = {\url{www.struck.de/sis1160.html}},
howpublished = {\url{www.spdevices.com/products/hardware/14-bit-digitizers/adq7dc}}, }
} @Misc{biblio:sundance,
title = "{Sundance PXIe700}",
@Misc{biblio:WR-LJD, howpublished = {\url{www.sundance.technology/som-cariers/pxi-boards/pxie700/}},
title = "{WRS Low Jitter Daugherboard}", }
howpublished = {\url{www.ohwr.org/projects/wrs-low-jitter/wiki/wiki}}, @Misc{biblio:spdevices,
} title = "{DAQ Unit - Digitizer: 14-bit, 10 GSPS digitizer platform, 1-2 chan}",
@ARTICLE{biblio:MIKES+VSL, howpublished = {\url{www.spdevices.com/products/hardware/14-bit-digitizers/adq7dc}},
author={E. F. Dierikx and et al.}, }
journal={IEEE T-UFFC},
title={White Rabbit Precision Time Protocol on Long-Distance Fiber Links}, @Misc{biblio:WR-LJD,
year={2016}, title = "{WRS Low Jitter Daugherboard}",
} howpublished = {\url{www.ohwr.org/projects/wrs-low-jitter/wiki/wiki}},
}
@inproceedings{biblio:MIKES-50km, @ARTICLE{biblio:MIKES+VSL,
author = "Anders Wallin and et al.", author={E. F. Dierikx and et al.},
title = "{Improved Systematic and Random Errors for Long-Distance Time-Transfer Using PTP White Rabbit }", journal={IEEE T-UFFC},
booktitle = "{EFTF}", title={{White Rabbit Precision Time Protocol on Long-Distance Fiber Links}},
year = "2018", year={2016},
} }
http://www.epapers.org/eftf2018/ESR/paper_details.php?PHPSESSID=t03vf3ur1ksr5rafkq24fe8k64&paper_id=7160
@INPROCEEDINGS{biblio:SYRTE-LNE-25km, @inproceedings{biblio:MIKES-50km,
author={N. Kaur and et al.}, author = "Anders Wallin and et al.",
booktitle={EFTF2016}, title = "{Improved Systematic and Random Errors for Long-Distance Time-Transfer Using PTP White Rabbit }",
title={Time transfer over a White Rabbit network}, booktitle = "{EFTF}",
year={2016}, year = "2018",
volume={}, }
number={}, http://www.epapers.org/eftf2018/ESR/paper_details.php?PHPSESSID=t03vf3ur1ksr5rafkq24fe8k64&paper_id=7160
pages={1-4}, @INPROCEEDINGS{biblio:SYRTE-LNE-25km,
keywords={frequency standards;optical fibre networks;time measurement;transfer standards;Allan deviation;LNE-SYRTE;White Rabbit network;frequency dissemination;long haul telecommunication network;optical fiber spool;time dissemination;time transfer;Chromatic dispersion;Optical fiber dispersion;Optical fiber networks;Rabbits;Time measurement;Time-frequency analysis;Wavelength division multiplexing;Chromatic dispersion;Long haul time and frequency dissemination;White Rabbit}, author={N. Kaur and et al.},
doi={10.1109/EFTF.2016.7477793}, booktitle={EFTF2016},
ISSN={}, title={Time transfer over a White Rabbit network},
month={April},} year={2016},
volume={},
@INPROCEEDINGS{biblio:SYRTE-LNE-500km, number={},
author={Kaur, Namneet and Frank, Florian and Pottie, Paul-Erik and Tuckey Philip}, pages={1-4},
booktitle={EFTF/IFCS}, keywords={frequency standards;optical fibre networks;time measurement;transfer standards;Allan deviation;LNE-SYRTE;White Rabbit network;frequency dissemination;long haul telecommunication network;optical fiber spool;time dissemination;time transfer;Chromatic dispersion;Optical fiber dispersion;Optical fiber networks;Rabbits;Time measurement;Time-frequency analysis;Wavelength division multiplexing;Chromatic dispersion;Long haul time and frequency dissemination;White Rabbit},
title={Time and frequency transfer over a 500 km cascaded {WR} network}, doi={10.1109/EFTF.2016.7477793},
year={2017}, ISSN={},
keywords={atomic clocks;data acquisition;optical fibre communication;synchronisation;White Rabbit link;active telecommunication networks;cascaded White Rabbit network;commercial White Rabbit equipment;distance 500.0 km;frequency dissemination;frequency transfer stability;integration time;long distance optical fiber links;software parameters;time transfer stability;unidirectional link setup;Clocks;Optical switches;Rabbits;Temperature measurement;Thermal stability;Time-frequency analysis}, month={April},}
doi={10.1109/FCS.2017.8088808},
ISSN={}, @INPROCEEDINGS{biblio:SYRTE-LNE-500km,
} author={Kaur, Namneet and Frank, Florian and Pottie, Paul-Erik and Tuckey Philip},
booktitle={EFTF/IFCS},
@ARTICLE{biblio:WR-ultimate-limits, title={Time and frequency transfer over a 500 km cascaded {WR} network},
author={M. Rizzi and M. Lipinski and P. Ferrari and S. Rinaldi and A. Flammini}, year={2017},
journal={IEEE Transactions on Ultrasonics, Ferroelectrics, and Frequency Control}, keywords={atomic clocks;data acquisition;optical fibre communication;synchronisation;White Rabbit link;active telecommunication networks;cascaded White Rabbit network;commercial White Rabbit equipment;distance 500.0 km;frequency dissemination;frequency transfer stability;integration time;long distance optical fiber links;software parameters;time transfer stability;unidirectional link setup;Clocks;Optical switches;Rabbits;Temperature measurement;Thermal stability;Time-frequency analysis},
title={White Rabbit clock synchronization: ultimate limits on close-in phase noise and short-term stability due to FPGA implementation}, doi={10.1109/FCS.2017.8088808},
year={2018}, ISSN={},
volume={}, }
number={},
pages={1-1}, @ARTICLE{biblio:WR-ultimate-limits,
keywords={Allan Deviation;Frequency transfer;IEEE 1588;Optical link;Oscillator;PLL;PTP;Phase noise;Stability;Synchronization;Synchronous Ethernet;Time transfer}, author={M. Rizzi and M. Lipinski and P. Ferrari and S. Rinaldi and A. Flammini},
doi={10.1109/TUFFC.2018.2851842}, journal={IEEE Transactions on Ultrasonics, Ferroelectrics, and Frequency Control},
ISSN={0885-3010}, title={{White Rabbit clock synchronization: ultimate limits on close-in phase noise and short-term stability due to FPGA implementation}},
month={},} year={2018},
volume={},
@Misc{biblio:WR-LJD-switch, number={},
title = "ASTERICS: PRODUCTION OF ULTRA-LOW-NOISE {WR} SWITCHES", pages={1-1},
howpublished = {\url{www.asterics2020.eu/article/production-ultra-low-noise-white-rabbit-switches}}, keywords={Allan Deviation;Frequency transfer;IEEE 1588;Optical link;Oscillator;PLL;PTP;Phase noise;Stability;Synchronization;Synchronous Ethernet;Time transfer},
} doi={10.1109/TUFFC.2018.2851842},
@Misc{biblio:optical-amplifier, ISSN={0885-3010},
title = "{OPNT's quasi bidirectional optical amplifiers}", month={},}
howpublished = {\url{www.opnt.nl/\#timing}},
} @Misc{biblio:WR-LJD-switch,
@inproceedings{biblio:WR-NIST, title = "ASTERICS: PRODUCTION OF ULTRA-LOW-NOISE {WR} SWITCHES",
author = "J. Savory and et al.", howpublished = {\url{www.asterics2020.eu/article/production-ultra-low-noise-white-rabbit-switches}},
title = "{White Rabbit-Based Time Distribution at NIST}", }
booktitle = "{IEEE International Frequency Control Symposium 2018}", @Misc{biblio:optical-amplifier,
year = "2018", title = "{OPNT's quasi bidirectional optical amplifiers}",
} howpublished = {\url{www.opnt.nl/\#timing}},
@Misc{biblio:wr-sfps, }
title = "{SFP transceiver and fibre type to use for White Rabbit}", @inproceedings{biblio:WR-NIST,
howpublished = {\url{www.ohwr.org/projects/white-rabbit/wiki/SFP}}, author = "J. Savory and et al.",
} title = "{White Rabbit-Based Time Distribution at NIST}",
@inproceedings{biblio:WR-INRIM, booktitle = "{IEEE International Frequency Control Symposium 2018}",
author = "G. Fantino and et al.", year = "2018",
title = "{White Rabbit Time Transfer on Medium and Long Fibre Hauls at INRIM}", }
booktitle = "{PTTI}", @Misc{biblio:wr-sfps,
year = "2014", title = "{SFP transceiver and fibre type to use for White Rabbit}",
} howpublished = {\url{www.ohwr.org/projects/white-rabbit/wiki/SFP}},
@Misc{biblio:WR-INRIM-400km, }
title = "{WR}-based time transfer between INRIM and Milano", @inproceedings{biblio:WR-INRIM,
howpublished = {\url{www.top-ix.org/en/2018/03/22/the-time-as-service-service-becomes-operational/}}, author = "G. Fantino and et al.",
} title = "{{White Rabbit Time Transfer on Medium and Long Fibre Hauls at INRIM}}",
booktitle = "{PTTI}",
@inproceedings{biblio:GSI-WR-GMT, year = "2014",
author = "C. Prados and et al.", }
title = "A RELIABLE {W}HITE {R}ABBIT NETWORK FOR THE FAIR GENERAL TIMING MACHINE", @Misc{biblio:WR-INRIM-400km,
booktitle = "{ICALEPCS}", title = "{WR}-based time transfer between INRIM and Milano",
year = "2018", howpublished = {\url{www.top-ix.org/en/2018/03/22/the-time-as-service-service-becomes-operational/}},
} }
@Misc{biblio:GSI-WR-GMT-wiki, @inproceedings{biblio:GSI-WR-GMT,
title = "{WR-based General Machine Timing System at GSI}", author = "C. Prados and et al.",
howpublished = {\url{www-acc.gsi.de/wiki/Timing/TimingSystemDocuments}}, title = "A RELIABLE {W}HITE {R}ABBIT NETWORK FOR THE {FAIR} {G}ENERAL {T}IMING {M}ACHINE",
} booktitle = "{ICALEPCS}",
@inproceedings{biblio:GSI-WR-GMT-CRYRING, year = "2018",
author = "M. Kreider and et al.", }
title = "TWO YEARS OF FAIR {G}ENERAL {M}ACHINE {T}IMING – EXPERIENCES AND IMPROVEMENTS",
booktitle = "{ICALEPCS}", @Misc{biblio:GSI-WR-GMT-wiki,
year = "2018", title = "{WR-based General Machine Timing System at GSI}",
} howpublished = {\url{www-acc.gsi.de/wiki/Timing/TimingSystemDocuments}},
@Inproceedings{biblio:LHAASO, }
author = "G. Gong and et al.", @inproceedings{biblio:GSI-WR-GMT-CRYRING,
title = "{Sub-nanosecond Timing System Designed And Developed For LHAASO Project}", author = "M. Kreider and et al.",
booktitle = "ICALEPCS", title = "TWO YEARS OF FAIR {G}ENERAL {M}ACHINE {T}IMING – EXPERIENCES AND IMPROVEMENTS",
} booktitle = "{ICALEPCS}",
@Inproceedings{biblio:LHAASO-WR-temp, year = "2018",
author = "Hongming Li and et al.", }
title = "{Temperature Effect and Correction Method of White Rabbit Timing Link}", @Inproceedings{biblio:LHAASO,
booktitle = "IEEE Transactions on Nuclear Science", author = "G. Gong and et al.",
year = "2015", title = "{Sub-nanosecond Timing System Designed And Developed For LHAASO Project}",
} booktitle = "ICALEPCS",
@Inproceedings{biblio:LHAASO-WR-calibrator, }
author = "Hongming Li and Guanghua Gong and Jianmin Li", @Inproceedings{biblio:LHAASO-WR-temp,
title = "{Portable Calibration Node for LHAASO-KM2A Detector Array}", author = "Hongming Li and et al.",
booktitle = "IEEE Transactions on Nuclear Science", title = "{Temperature Effect and Correction Method of White Rabbit Timing Link}",
year = "2017", booktitle = "IEEE Transactions on Nuclear Science",
} year = "2015",
@Inproceedings{biblio:LHAASO-WR-prototype, }
author = "Hongming Li and et al.", @Inproceedings{biblio:LHAASO-WR-calibrator,
title = "PROTOTYPE OF {W}HITE {R}ABBIT NETWORK IN {LHAASO}", author = "Hongming Li and Guanghua Gong and Jianmin Li",
booktitle = "ICALEPCS", title = "{Portable Calibration Node for LHAASO-KM2A Detector Array}",
year = "2015", booktitle = "IEEE Transactions on Nuclear Science",
} year = "2017",
@misc{biblio:KM3NeT, }
title = "{The Cubic Kilometre Neutrino Telescope (KM3NeT)}", @Inproceedings{biblio:LHAASO-WR-prototype,
howpublished = {\url{km3net.org}}, author = "Hongming Li and et al.",
} title = "PROTOTYPE OF {W}HITE {R}ABBIT NETWORK IN {LHAASO}",
@Misc{biblio:WR-KM3NeT-Letter, booktitle = "ICALEPCS",
title = "KM3NeT 2.0: Letter of Intent for ARCA and ORCA", year = "2015",
howpublished = {\url{https://arxiv.org/pdf/1601.07459.pdf}}, }
} @misc{biblio:KM3NeT,
@Misc{biblio:WR-KM3NeT-presentation, title = "{The Cubic Kilometre Neutrino Telescope (KM3NeT)}",
title = "{White Rabbit in KM3NeT}", howpublished = {\url{km3net.org}},
howpublished = {\url{www.ohwr.org/attachments/4263/ 6\_wr\_km3net\_15032016.pptx}}, }
} @Misc{biblio:WR-KM3NeT-Letter,
title = "{KM3NeT 2.0: Letter of Intent for ARCA and ORCA}",
@Misc{biblio:SKA, howpublished = {\url{https://arxiv.org/pdf/1601.07459.pdf}},
title = "Square Kilometre Array ", }
howpublished = {\url{www.skatelescope.org}}, @Misc{biblio:WR-KM3NeT-presentation,
} title = "{White Rabbit in KM3NeT}",
howpublished = {\url{www.ohwr.org/attachments/4263/ 6\_wr\_km3net\_15032016.pptx}},
@Misc{biblio:ELI-ALP-WR, }
title = "{ELI-ALPS: Synchronization issues}",
howpublished = {\url{www.ohwr.org/attachments/3565/ WR\_WS\_GENEVA\_6OCT2014\_IK\_ELI\_ALPS.pptx}}, @Misc{biblio:SKA,
} title = "{Square Kilometre Array}",
@Misc{biblio:ELI-BEAMS-WR, howpublished = {\url{www.skatelescope.org}},
title = "{ELI-BEAMS: Electronic Timing System at Facility Level}", }
howpublished = {\url{www.mrf.fi/dmdocuments/TIMING\_WORKSHOP/02-PavelBastl/ELI-BL-4442-PRE-00000116-B.ppt}},
} @Misc{biblio:ELI-ALP-WR,
@Inproceedings{biblio:DLR-WR, title = "{ELI-ALPS: Synchronization issues}",
author = "D. Hamp and et al.", howpublished = {\url{www.ohwr.org/attachments/3565/ WR\_WS\_GENEVA\_6OCT2014\_IK\_ELI\_ALPS.pptx}},
title = "{First successful satellite laser ranging with a fibre-based transmitter}", }
howpublished = {\url{https://arxiv.org/abs/1605.07429}}, @Misc{biblio:ELI-BEAMS-WR,
} title = "{ELI-BEAMS: Electronic Timing System at Facility Level}",
@Inproceedings{biblio:CTA-WR-timestamps, howpublished = {\url{www.mrf.fi/dmdocuments/TIMING\_WORKSHOP/02-PavelBastl/ELI-BL-4442-PRE-00000116-B.ppt}},
author = "M. Bruckner and et al.", }
title = "A TIME STAMPING TDC FOR SPEC AND ZEN PLATFORMS BASED ON {W}HITE {R}ABBIT", @Inproceedings{biblio:DLR-WR,
booktitle = "ICALEPCS", author = "D. Hamp and et al.",
year = "2017", title = "{First successful satellite laser ranging with a fibre-based transmitter}",
} howpublished = {\url{https://arxiv.org/abs/1605.07429}},
@INPROCEEDINGS{biblio:EPFL-WR-PMU, }
author={R. Razzaghi and et al.}, @Inproceedings{biblio:CTA-WR-timestamps,
booktitle={ISGT-Europe}, author = "M. Bruckner and et al.",
title={{A White Rabbit synchronized PMU}}, title = "A TIME STAMPING {TDC} FOR {SPEC} AND {ZEN} PLATFORMS BASED ON {W}HITE {R}ABBIT",
year={2017}, booktitle = "ICALEPCS",
volume={}, year = "2017",
number={}, }
pages={1-6}, @INPROCEEDINGS{biblio:EPFL-WR-PMU,
keywords={calibration;phase estimation;phasor measurement;synchronisation;GPS;PMU calibrator;Phasor Measurement Units networks;WR network;WR-PMU;White Rabbit technology;power systems applications;single WR switch;time dissemination techniques;Clocks;Global Positioning System;Hardware;Phasor measurement units;Protocols;Rabbits;Synchronization;Phasor Measurement Unit (PMU);White Rabbit;calibration;synchrophasor;time synchronization}, author={R. Razzaghi and et al.},
doi={10.1109/ISGTEurope.2017.8260178}, booktitle={ISGT-Europe},
ISSN={}, title={{A White Rabbit synchronized PMU}},
month={Sept},} year={2017},
volume={},
@Inproceedings{biblio:OASIS, number={},
author = "Deghaye, S and et al.", pages={1-6},
title = "{OASIS: A New System to Acquire and Display the Analog keywords={calibration;phase estimation;phasor measurement;synchronisation;GPS;PMU calibrator;Phasor Measurement Units networks;WR network;WR-PMU;White Rabbit technology;power systems applications;single WR switch;time dissemination techniques;Clocks;Global Positioning System;Hardware;Phasor measurement units;Protocols;Rabbits;Synchronization;Phasor Measurement Unit (PMU);White Rabbit;calibration;synchrophasor;time synchronization},
Signals for LHC}", doi={10.1109/ISGTEurope.2017.8260178},
booktitle = "ICALEPCS", ISSN={},
year = "2003", month={Sept},}
}
@Misc{biblio:WRXI, @Inproceedings{biblio:OASIS,
title = "{WRXI}", author = "Deghaye, S and et al.",
howpublished = {\url{www.ohwr.org/projects/wrxi/wiki/wiki}}, title = "{OASIS: A New System to Acquire and Display the Analog
} Signals for LHC}",
@Inproceedings{biblio:CSNS-WR, booktitle = "ICALEPCS",
author = "Jian Zhuang and et al.", year = "2003",
title = "THE DESIGN OF {CSNS} INSTRUMENT CONTROL", }
booktitle = "ICALEPCS", @Misc{biblio:WRXI,
year = "2017", title = "{WRXI}",
} howpublished = {\url{www.ohwr.org/projects/wrxi/wiki/wiki}},
@Misc{biblio:JINR, }
title = "The Joint Institute for Nuclear Research ", @Inproceedings{biblio:CSNS-WR,
howpublished = {\url{www.jinr.ru/main-en/}}, author = "Jian Zhuang and et al.",
} title = "THE DESIGN OF {CSNS} INSTRUMENT CONTROL",
@Misc{biblio:JINR-WR, booktitle = "ICALEPCS",
title = "{JINR AFI} Electronics", year = "2017",
howpublished = {\url{afi.jinr.ru/CategoryWhiteRabbit}}, }
} @Misc{biblio:JINR,
@Misc{biblio:ESRF, title = "{The Joint Institute for Nuclear Research}",
title = "{European Synchrotron Radiation Facility}", howpublished = {\url{www.jinr.ru/main-en/}},
howpublished = {\url{www.esrf.eu/about}}, }
} @Misc{biblio:JINR-WR,
@Inproceedings{biblio:ESRF-WR, title = "{JINR AFI} Electronics",
author = "G. Goujon and et al.", howpublished = {\url{afi.jinr.ru/CategoryWhiteRabbit}},
title = "REFURBISHMENT OF THE {ESRF} ACCELERATOR SYNCHRONISATION SYSTEM USING {W}HITE {R}ABBIT", }
booktitle = "ICALEPCS", @Misc{biblio:ESRF,
year = "2017", title = "{European Synchrotron Radiation Facility}",
} howpublished = {\url{www.esrf.eu/about}},
@online{biblio:wrCalibration, }
title = "{WR calibration procedure}", @Inproceedings{biblio:ESRF-WR,
howpublished = {\url{www.ohwr.org/documents/213}}, author = "G. Goujon and et al.",
author = {G. Daniluk}, title = "REFURBISHMENT OF THE {ESRF} ACCELERATOR SYNCHRONISATION SYSTEM USING {W}HITE {R}ABBIT",
urldate = {August 13, 2014}, booktitle = "ICALEPCS",
} year = "2017",
}
@INPROCEEDINGS{biblio:WR-characteristics, @online{biblio:wrCalibration,
author={M. Rizzi and M. Lipiński and T. Wlostowski and J. Serrano and G. Daniluk and P. Ferrari and S. Rinaldi}, title = "{WR calibration procedure}",
booktitle={2016 IEEE International Symposium on Precision Clock Synchronization for Measurement, Control, and Communication (ISPCS)}, howpublished = {\url{www.ohwr.org/documents/213}},
title={White rabbit clock characteristics}, author = {G. Daniluk},
year={2016}, urldate = {August 13, 2014},
volume={}, }
number={},
pages={1-6}, @INPROCEEDINGS{biblio:WR-characteristics,
keywords={clocks;frequency measurement;phase locked loops;synchronisation;transfer standards;ITU-T G.8262;Precision Time Protocol;frequency transfer characteristics;phase locked loop;phase noise analysis;phase noise reduction;subnanosecond accuracy synchronisation;subpicoseconds precision synchronisation;white rabbit clock characteristics;Clocks;Frequency measurement;Phase locked loops;Phase measurement;Phase noise;Switches;Synchronization}, author={M. Rizzi and M. Lipiński and T. Wlostowski and J. Serrano and G. Daniluk and P. Ferrari and S. Rinaldi},
doi={10.1109/ISPCS.2016.7579514}, booktitle={ISPCS2016},
ISSN={}, title={{White Rabbit Clock Characteristics}},
month={Sept},} year={2016},
volume={},
@Misc{biblio:SPS-WR-LLRF, number={},
title = "{MicroTCA Low-level RF WR Node}", pages={1-6},
howpublished = {\url{www.ohwr.org/projects/ertm15-llrf-wr/wiki}}, keywords={clocks;frequency measurement;phase locked loops;synchronisation;transfer standards;ITU-T G.8262;Precision Time Protocol;frequency transfer characteristics;phase locked loop;phase noise analysis;phase noise reduction;subnanosecond accuracy synchronisation;subpicoseconds precision synchronisation;white rabbit clock characteristics;Clocks;Frequency measurement;Phase locked loops;Phase measurement;Phase noise;Switches;Synchronization},
} doi={10.1109/ISPCS.2016.7579514},
@Inproceedings{biblio:SKA-80km, ISSN={},
author = "Paul Boven", month={Sept},}
title = "{DWDM Stabilized Optics for White Rabbit}",
booktitle = "32nd European Frequency and Time Forum", @Misc{biblio:SPS-WR-LLRF,
year = "2018", title = "{MicroTCA Low-level RF WR Node}",
} howpublished = {\url{www.ohwr.org/projects/ertm15-llrf-wr/wiki}},
}
@Misc{biblio:WR-calibration, @Inproceedings{biblio:SKA-80km,
title = "{WR} Calibration", author = "Paul Boven",
howpublished = {\url{www.ohwr.org/projects/wr-calibration/wiki/wiki}}, title = "{DWDM Stabilized Optics for White Rabbit}",
} booktitle = "32nd European Frequency and Time Forum",
@Misc{biblio:P1588, year = "2018",
title = "{P1588 Working Group}", }
howpublished = {\url{ieee-sa.imeetcentral.com/1588public/}},
} @Misc{biblio:WR-calibration,
@Misc{biblio:WRin1588, title = "{WR} Calibration",
title = "{White Rabbit integration into IEEE15880-20XX as High Accuracy}", howpublished = {\url{www.ohwr.org/projects/wr-calibration/wiki/wiki}},
howpublished = {\url{www.ohwr.org/projects/wr-std/wiki/wrin1588}}, }
} @Misc{biblio:P1588,
@Misc{biblio:WRusers, title = "{P1588 Working Group}",
title = "{WR Users}", howpublished = {\url{ieee-sa.imeetcentral.com/1588public/}},
howpublished = {\url{www.ohwr.org/projects/white-rabbit/wiki/WRUsers}}, }
} @Misc{biblio:WRin1588,
@Misc{biblio:WRcompanies, title = "{White Rabbit integration into IEEE15880-20XX as High Accuracy}",
title = "{Companies producing White Rabbit Devices}", howpublished = {\url{www.ohwr.org/projects/wr-std/wiki/wrin1588}},
howpublished = {\url{www.ohwr.org/projects/white-rabbit/wiki/wrcompanies}}, }
} @Misc{biblio:WRusers,
@Misc{biblio:TAIGA-WR-harsh-env, title = "{WR Users}",
title = "TESTING {W}HITE {R}ABBIT HARDWARE IN FIELD CONDITIONS IN SIBERIA", howpublished = {\url{www.ohwr.org/projects/white-rabbit/wiki/WRUsers}},
howpublished = {\url{www.asterics2020.eu/article/testing-white-rabbit-hardware-field-conditions-siberia}}, }
} @Misc{biblio:WRcompanies,
@Misc{biblio:GVD, title = "{Companies producing White Rabbit Devices}",
title = "{Baikal Neutrino Observatory}", howpublished = {\url{www.ohwr.org/projects/white-rabbit/wiki/wrcompanies}},
howpublished = {\url{www.inr.ru/eng/ebgnt.html}}, }
} @Misc{biblio:TAIGA-WR-harsh-env,
@Inproceedings{biblio:TAIGA-WR-1, title = "TESTING {W}HITE {R}ABBIT HARDWARE IN FIELD CONDITIONS IN {S}IBERIA",
author = "M. Bruckner and et al.", howpublished = {\url{www.asterics2020.eu/article/testing-white-rabbit-hardware-field-conditions-siberia}},
title = "{A White Rabbit setup for sub-nsec synchronization, timestamping and time calibration in large scale astroparticle physics experiments}", }
booktitle = "ICRS", @Misc{biblio:GVD,
year = "2013", title = "{Baikal Neutrino Observatory}",
} howpublished = {\url{www.inr.ru/eng/ebgnt.html}},
@Inproceedings{biblio:TAIGA-WR-2, }
author = "Ralf Wischnewski and et al.", @Inproceedings{biblio:TAIGA-WR-1,
title = "{Time Synchronization with White Rabbit -- Experience from Tunka-HiSCORE}", author = "M. Bruckner and et al.",
booktitle = "ICRS", title = "{A White Rabbit setup for sub-nsec synchronization, timestamping and time calibration in large scale astroparticle physics experiments}",
year = "2015", booktitle = "ICRS",
} year = "2013",
@Misc{biblio:HAWK, }
title = "{{High Altitude Water Cherenkov (HAWC) observatory}”}", @Inproceedings{biblio:TAIGA-WR-2,
howpublished = {\url{www.hawc-observatory.org}}, author = "Ralf Wischnewski and et al.",
} title = "{Time Synchronization with White Rabbit -- Experience from Tunka-HiSCORE}",
@Misc{biblio:GM-Meinberg, booktitle = "ICRS",
title = "{Meinberg LANTIME M1000-IMS /10003285}", year = "2015",
} }
@Inproceedings{biblio:VLS-WR-insite-calib, @Misc{biblio:HAWK,
author = "J.C.J. Koelemeij", title = "{{High Altitude Water Cherenkov (HAWC) observatory}”}",
title = "{Sub-nanosecond time distribution through long-haul fiber-optic links using White Rabbit Ethernet}", howpublished = {\url{www.hawc-observatory.org}},
booktitle = "PTTI", }
year = "2017", @Misc{biblio:GM-Meinberg,
} title = "{Meinberg LANTIME M1000-IMS /10003285}",
@Misc{biblio:WRITE, }
title = "{{WRITE}: White Rabbit Industrial Timing Enhancement (SRT-i26: Selected Research Topic, was JRP-i26)}", @Inproceedings{biblio:VLS-WR-insite-calib,
} author = "J.C.J. Koelemeij",
@Misc{biblio:WRITE-2, title = "{Sub-nanosecond time distribution through long-haul fiber-optic links using White Rabbit Ethernet}",
title = "{{Publishable Summary for 17IND14 WRITE Precision Time for Industry}}", booktitle = "PTTI",
booktitle = "EUROMET", year = "2017",
howpublished = {\url{www.euramet.org}}, }
} @Misc{biblio:WRITE,
@Misc{biblio:SPEV7, title = "{{WRITE}: White Rabbit Industrial Timing Enhancement (SRT-i26: Selected Research Topic, was JRP-i26)}",
title = "{Simple PCIe FMC carrier 7}", }
howpublished = {\url{www.ohwr.org/projects/spec7/wiki/}}, @Misc{biblio:WRITE-2,
} title = "{{Publishable Summary for 17IND14 WRITE Precision Time for Industry}}",
booktitle = "EUROMET",
@Misc{biblio:WR-EUREXCHANGE, howpublished = {\url{www.euramet.org}},
title = "{High Precision Time (White Rabbit) Pilot}", }
howpublished = {\url{www.eurexchange.com/exchange-en/technology/t7/implementation-news/High-Precision-Time--White-Rabbit--Pilot/3450694}}, @Misc{biblio:SPEV7,
} title = "{Simple PCIe FMC carrier 7}",
howpublished = {\url{www.ohwr.org/projects/spec7/wiki/}},
@Misc{biblio:WR-CALIB-ABSOLUTE, }
title = "{White Rabbit Absolute Calibration Procedure}",
author = "{P.P.M Jansweijer and et al.}", @Misc{biblio:WR-EUREXCHANGE,
howpublished = {\url{ohwr.org/attachments/4542/WhiteRabbitAbsoluteCalibrationProcedure.pdf}}, title = "{High Precision Time (White Rabbit) Pilot}",
} howpublished = {\url{www.eurexchange.com/exchange-en/technology/t7/implementation-news/High-Precision-Time--White-Rabbit--Pilot/3450694}},
}
@Misc{biblio:WR-CALIB-ABSOLUTE,
title = "{White Rabbit Absolute Calibration Procedure}",
author = "{P.P.M Jansweijer and et al.}",
howpublished = {\url{ohwr.org/attachments/4542/WhiteRabbitAbsoluteCalibrationProcedure.pdf}},
}
@article{biblio:WR-CALIB-ABSOLUTE-2, @article{biblio:WR-CALIB-ABSOLUTE-2,
author = {H. Z. Peek and et al.}, author = {H. Z. Peek and et al.},
journal = {Opt. Express}, journal = {Opt. Express},
...@@ -597,4 +604,9 @@ month = {May}, ...@@ -597,4 +604,9 @@ month = {May},
year = {2018}, year = {2018},
doi = {10.1364/OE.26.014650}, doi = {10.1364/OE.26.014650},
abstract = {We present a new measurement principle to determine the absolute time delay of a waveform from an optical reference plane to an electrical reference plane and vice versa. We demonstrate a method based on this principle with 2 ps uncertainty. This method can be used to perform accurate time delay determinations of optical transceivers used in fiber-optic time-dissemination equipment. As a result the time scales in optical and electrical domain can be related to each other with the same uncertainty. We expect this method will be a new breakthrough in high-accuracy time transfer and absolute calibration of time-transfer equipment.}, abstract = {We present a new measurement principle to determine the absolute time delay of a waveform from an optical reference plane to an electrical reference plane and vice versa. We demonstrate a method based on this principle with 2 ps uncertainty. This method can be used to perform accurate time delay determinations of optical transceivers used in fiber-optic time-dissemination equipment. As a result the time scales in optical and electrical domain can be related to each other with the same uncertainty. We expect this method will be a new breakthrough in high-accuracy time transfer and absolute calibration of time-transfer equipment.},
}
@Misc{biblio:WR-APPLICATIONS-SNAPSHOT,
title = "{WR Applications Snapshot June 2018}",
howpublished = {\url{www.ohwr.org/projects/white-rabbit/wiki/wr-applications-snapshot-june-2018}},
} }
\ No newline at end of file
...@@ -55,7 +55,7 @@ enhancements to the White Rabbit (WR) extension of the IEEE 1588 Precision Time ...@@ -55,7 +55,7 @@ enhancements to the White Rabbit (WR) extension of the IEEE 1588 Precision Time
Initially developed to serve accelerators at the European Organization for Initially developed to serve accelerators at the European Organization for
Nuclear Research (CERN), WR has become a widely-used synchronization solution Nuclear Research (CERN), WR has become a widely-used synchronization solution
in scientific installations. This article classifies WR applications in scientific installations. This article classifies WR applications
into five types, briefly explains each and describes its example into five types, briefly explains each and describes example
installations. The article then summarizes WR enhancements that have been triggered by installations. The article then summarizes WR enhancements that have been triggered by
different applications and outlines WR's integration into the PTP standard. different applications and outlines WR's integration into the PTP standard.
Based on the presented variety of WR applications and enhancements, it concludes Based on the presented variety of WR applications and enhancements, it concludes
...@@ -95,10 +95,11 @@ implement WR enhancements: ...@@ -95,10 +95,11 @@ implement WR enhancements:
% \textcolor{red}{(802.1Q end stations)} that implement WR enhancements: % \textcolor{red}{(802.1Q end stations)} that implement WR enhancements:
\begin{enumerate} \begin{enumerate}
\item \textbf{Synchronization with sub-nanosecond accuracy and tens of picoseconds precision} among all \item \textbf{Synchronization with sub-nanosecond accuracy and tens of picoseconds precision} among all
WR switches/nodes. Such synchronization is provided by the WR extension to PTP (WR-PTP, WR switches/nodes. %\footnote{The accuracy is the mean offset between the times of two synchronized WR switches/nodes while precision is the standard deviation of this offset.}.
Such synchronization is provided by the WR extension to PTP (WR-PTP
\cite{biblio:WRPTP}) and its supporting hardware \cite{biblio:ISPCS2011}\cite{biblio:TomekMSc}\cite{biblio:WRproject}. \cite{biblio:WRPTP}) and its supporting hardware \cite{biblio:ISPCS2011}\cite{biblio:TomekMSc}\cite{biblio:WRproject}.
\item \textbf{Deterministic and low-latency communication} between WR nodes provided by \item \textbf{Deterministic and low-latency communication} between WR nodes provided by
a purposely customized and open design of the WR switch, described in a purposely-made and open design of the WR switch, described in
\cite{biblio:MaciekPhD}. \cite{biblio:MaciekPhD}.
\end{enumerate} \end{enumerate}
Studies \cite{biblio:MaciekPhD}\cite{biblio:CesarPhD}\cite{biblio:JosePhD} have shown Studies \cite{biblio:MaciekPhD}\cite{biblio:CesarPhD}\cite{biblio:JosePhD} have shown
...@@ -113,57 +114,55 @@ manner ensuring at most a single failure per year for a network of 2000 WR nodes ...@@ -113,57 +114,55 @@ manner ensuring at most a single failure per year for a network of 2000 WR nodes
% \end{figure} % \end{figure}
Since its conception in 2008, the number of WR applications has grown beyond Since its conception in 2008, the number of WR applications has grown beyond
any expectations. The WR Users website \cite{biblio:WRusers} attempts to keep any expectation. The WR Users website \cite{biblio:WRusers} attempts to keep
track of WR applications. Apart from the suitable synchronization performance, the reasons for such a proliferation of WR applications track of WR applications and the newsletter in \cite{biblio:WR-APPLICATIONS-SNAPSHOT}
provides a status of a number of WR application in June 2018. Apart from the suitable synchronization performance, the reasons for such a proliferation of WR applications
are the open nature of the WR project and the fact that the WR technology is based are the open nature of the WR project and the fact that the WR technology is based
on standards. The former encourages collaboration, on standards. The former encourages collaboration,
reuse of work and adaptations that also prevent vendor lock-in. The latter allows using reuse of work and adaptations that also prevent vendor lock-in. The latter allows using
off-the-shelf solutions with WR networks and catalyzes off-the-shelf solutions with WR networks and catalyzes
collaboration with companies. collaboration with companies.
What started as a project to renovate one of the most critical systems at CERN, What started as a project to renovate one of the most critical systems at CERN,
GMT \cite{biblio:GMT}\cite{biblio:GMTJavierPres}, is now a multilaboratory, the General Machine Timing (GMT \cite{biblio:GMT}\cite{biblio:GMTJavierPres}), is now a multilaboratory,
multicompany and multinational collaboration developing a technology that is multicompany and multinational collaboration developing a technology that is
commercially available, used all over the world, and being incorporated into commercially available, used worldwide, and incorporated into
the original PTP standard \cite{biblio:P1588}\cite{P1588-HA-enhancements}. the original PTP \cite{biblio:P1588}\cite{P1588-HA-enhancements}.
% This article attempts at providing a snapshot of the various WR applications, % This article attempts at providing a snapshot of the various WR applications,
% the ongoing work on enhancing WR and evolution of WR into IEEE 1588. % the ongoing work on enhancing WR and evolution of WR into IEEE 1588.
The article briefly describes in Section~\ref{sec:wrElements} the portfolio of This article briefly describes in Section~\ref{sec:wrElements} the portfolio of
readily available WR network elements. It then explains in readily available WR network elements. It then explains in
Sections~\ref{sec:time-and-freq}-\ref{sec:RFoverWR} different types of Sections~\ref{sec:time-and-freq}-\ref{sec:RFoverWR} different types of
WR applications, their concept and use examples, WR applications, their concept and use examples,
summarized in Table~\ref{tab:applications}. Application-triggered enhancements are described in summarized in Table~\ref{tab:applications}.
Section~\ref{sec:WRenhancements}. Finally, in Section~\ref{sec:WRin1588} we
briefly describe the integration of WR into the
IEEE 1588 standard and we conclude in Section~\ref{sec:conclusions}.
\begin{table}[!t] \begin{table}[!t]
\caption{Non-exhaustive list of White Rabbit applications} \caption{Non-exhaustive list of White Rabbit applications}
\centering \centering
\scriptsize \scriptsize
\begin{tabular} \begin{tabular}
{| p{0.9cm} | p{1cm} | p{0.6cm} | p{0.7cm} | p{0.7cm} | p{0.99cm} | p{1.1cm} |} \hline {| p{0.8cm} | p{1.1cm} | p{0.6cm} | p{0.7cm} | p{0.7cm} | p{0.99cm} | p{1.1cm} |} \hline
& & & & \multicolumn{2}{c |}{\textbf{ Network Size}} & \\ & & & & \multicolumn{2}{c |}{\textbf{ Network Size}} & \\
\textbf{Facility}&\textbf{Location}&\textbf{Type}&\textbf{Link} & \textbf{in 2018}& \textbf{$>$2020} &\textbf{Reference} \\ \textbf{Facility}&\textbf{Location}&\textbf{Type}&\textbf{Link} & \textbf{2018}& \textbf{$>$2020} &\textbf{Reference} \\
& & &\textbf{len.} & N / S / L & N / S / L & \\ \hline & & &\textbf{len.} & N/S/L & N/S/L & \\ \hline
% & & & (max) & & & \\ \hline % & & & (max) & & & \\ \hline
\multicolumn{7}{|c|}{\textbf{Accelerators, synchrotrons and spallation sources}} \\ \hline \multicolumn{7}{|c|}{\textbf{Accelerators, synchrotrons and spallation sources}} \\ \hline
CERN & Switz. & TF & 10~km & 0/2/1 & 0/2/1 & \\ \hline CERN & Switzerland & TF & 10~km & 0/2/1 & 0/2/1 & \\ \hline
CERN & Switz. & FL & 1~km & 6/2/1 & 20/8/1 & \cite{biblio:wr-streamers}\cite{biblio:WR-Btrain}\cite{biblio:WR-Btrain-MM} \cite{biblio:WR-BTrain-RF}\cite{biblio:WR-Btrain-status}\\ \hline CERN & Switzerland & FL & 1~km & 6/2/1 & 20/8/1 & \cite{biblio:wr-streamers}\cite{biblio:WR-Btrain}\cite{biblio:WR-Btrain-MM} \cite{biblio:WR-BTrain-RF}\cite{biblio:WR-Btrain-status}\\ \hline
CERN & Switz. & TD & 10~km & 8/2/1 & 65/31/2 & \cite{biblio:WR-LIST}\cite{biblio:WR-LIST-2}\cite{biblio:WRXI} \\ \hline CERN & Switzerland & TD & 10~km & 8/2/1 & 65/31/2 & \cite{biblio:WR-LIST}\cite{biblio:WR-LIST-2}\cite{biblio:WRXI} \\ \hline
CERN & Switz. & RF & 10~km & -/-/- & 13/1/1 & \cite{biblio:WR-LIST} \\ \hline CERN & Switzerland & RF & 10~km & -/-/- & 13/1/1 & \cite{biblio:WR-LIST} \\ \hline
CERN & Switz. & TC & 10~km & -/-/ & 500/40/4 & \\ \hline CERN & Switzerland & TC & 10~km & -/-/ & 500/40/4 & \\ \hline
GSI & Germany & TC & 1~km & 35/4/4 & 2000/300/4& \cite{biblio:WR-GSI} \\ \hline GSI & Germany & TC & 1~km & 35/4/4 & 2000/300/4& \cite{biblio:WR-GSI} \\ \hline
JINR & Russia & TS,TD & 1~km & 50/15/3 & 250/30/3 & \cite{biblio:JINR-WR} \\ \hline JINR & Russia & TS,TD & 1~km & 50/15/3 & 250/30/3 & \cite{biblio:JINR-WR} \\ \hline
ESRF & France & RF,TS & 1~km & 7/1/1 & 40/5/2 & \cite{biblio:ESRF-WR} \\\hline ESRF & France & RF,TS & 1~km & 7/1/1 & 40/5/2 & \cite{biblio:ESRF-WR} \\\hline
CSNS & Chine & TF,TS, TD & 1~km & 50/4/2 & 50/4/2 &\cite{biblio:CSNS-WR} \\ \hline CSNS & China & TF,TS, TD & 1~km & 50/4/2 & 50/4/2 &\cite{biblio:CSNS-WR} \\ \hline
\multicolumn{7}{|c|}{\textbf{Neutrino Detectors}} \\ \hline \multicolumn{7}{|c|}{\textbf{Neutrino Detectors}} \\ \hline
CERN & Switz. & TS & 10~km & 10/4/2 & & \cite{biblio:wr-cngs} \\ \hline CERN & Switzerland & TS & 10~km & 10/4/2 & & \cite{biblio:wr-cngs} \\ \hline
KM3Net & France & TF,TS & 40~km & 18/1/1 & 4140/270/3 & \cite{biblio:KM3NeT}\cite{biblio:WR-KM3NeT-Letter}\cite{biblio:WR-KM3NeT-presentation} \\ \hline KM3Net & France & TF,TS & 40~km & 18/1/1 & 4140/270/3 & \cite{biblio:KM3NeT}\cite{biblio:WR-KM3NeT-Letter}\cite{biblio:WR-KM3NeT-presentation} \\ \hline
KM3Net & Spain & TF,TS & 100~km & 18/1/1 & 2070/130/2 & \cite{biblio:KM3NeT}\cite{biblio:WR-KM3NeT-Letter}\cite{biblio:WR-KM3NeT-presentation} \\ \hline KM3Net & Spain & TF,TS & 100~km & 18/1/1 & 2070/130/2 & \cite{biblio:KM3NeT}\cite{biblio:WR-KM3NeT-Letter}\cite{biblio:WR-KM3NeT-presentation} \\ \hline
% CHIPS & USA & & 1km & & 200/16/? & \\ \hline % CHIPS & USA & & 1km & & 200/16/? & \\ \hline
...@@ -187,10 +186,10 @@ HAWC & Mexico & TF,TS, TD & 1~km & 6/1/1 & 6/ ...@@ -187,10 +186,10 @@ HAWC & Mexico & TF,TS, TD & 1~km & 6/1/1 & 6/
\multicolumn{7}{|c|}{\textbf{National Time Laboratories}} \\ \hline \multicolumn{7}{|c|}{\textbf{National Time Laboratories}} \\ \hline
MIKES & Finland & TF & 950~km & 10/few/2 & 10/few/2 & \cite{biblio:MIKES-50km}\cite{biblio:MIKES+VSL} \\ \hline MIKES & Finland & TF & 950~km & 10/few/2 & 10/few/2 & \cite{biblio:MIKES-50km}\cite{biblio:MIKES+VSL} \\ \hline
LNE-SYRTE & France & TF & 125~km & 4/2/4 & 4/2/4 & \cite{biblio:SYRTE-LNE-25km}\cite{biblio:SYRTE-LNE-500km} \\ \hline LNE-SYRTE & France & TF & 125~km & 4/2/4 & 4/2/4 & \cite{biblio:SYRTE-LNE-25km}\cite{biblio:SYRTE-LNE-500km} \\ \hline
VLS & Nederland & TF & 137~km & 4/2/1 & 4/2/1 & \cite{biblio:MIKES+VSL} \\ \hline VLS & Netherlands & TF & 137~km & 4/2/1 & 4/2/1 & \cite{biblio:MIKES+VSL} \\ \hline
NIST & USA & TF & 10~km & 2/-/1 & expanding & \cite{biblio:WR-NIST} \\ \hline NIST & USA & TF & 10~km & 2/-/1 & expanding & \cite{biblio:WR-NIST} \\ \hline
NLP & UK & TF & & & & \\ \hline NLP & UK & TF & 80~km & 2/3/2 & expanding & \cite{biblio:NPL} \\ \hline
INRIM & Italy & TF,TS & 400~km & 8/1/1 & expanding & \cite{biblio:WR-INRIM}\cite{biblio:WR-INRIM-400km} \\ \hline INRIM & Italy & TF,TS & 400~km & 8/1/1 & expanding & \cite{biblio:WR-INRIM}\cite{biblio:WR-INRIM-400km} \\ \hline
...@@ -198,23 +197,27 @@ INRIM & Italy & TF,TS & 400~km & 8/1/1 ...@@ -198,23 +197,27 @@ INRIM & Italy & TF,TS & 400~km & 8/1/1
SKA & Australia/ Africa& TF & 80~km & 2/1/1 & 233/15/3 & \cite{biblio:SKA-80km} \\ \hline SKA & Australia/ Africa& TF & 80~km & 2/1/1 & 233/15/3 & \cite{biblio:SKA-80km} \\ \hline
DLR & Germany & TD & 1~km & 1/1/1 & 1/1/1 & \cite{biblio:ELI-BEAMS-WR} \\ \hline DLR & Germany & TD & 1~km & 1/1/1 & 1/1/1 & \cite{biblio:ELI-BEAMS-WR} \\ \hline
ELI-ALPS & Hungry & TS & 1~km & & & \cite{biblio:ELI-ALP-WR} \\ \hline ELI-ALPS & Hungry & TS & 1~km & & & \cite{biblio:ELI-ALP-WR} \\ \hline
ELI-BEAMS & Czech & TF,TS, TD,TC& 1~km & 70/16/2 & 70/16/2 & \cite{biblio:ELI-BEAMS-WR} \\ \hline ELI-BEAMS & Czech Republic & TF,TS, TD,TC& 1~km & 70/16/2 & 70/16/2 & \cite{biblio:ELI-BEAMS-WR} \\ \hline
EPFL & Switzerland & TS & 1~km & 2/1/1 & 2/1/1 & \cite{biblio:EPFL-WR-PMU} \\ \hline EPFL & Switzerland & TS & 1~km & 2/1/1 & 2/1/1 & \cite{biblio:EPFL-WR-PMU} \\ \hline
Deutsche Boerse & Germany & TS & 1~km & & & \cite{biblio:WR-EUREXCHANGE} \\ \hline Deutsche B{\"o}rse & Germany & TS & 1~km & & & \cite{biblio:WR-EUREXCHANGE} \\ \hline
\multicolumn{4}{|r|}{\textbf{Total number of WR nodes: }} & \textbf{462} & \textbf{17592} & \\ \multicolumn{7}{|c|}{\textbf{Total number of WR network elements in the applications listed above }} \\ \hline
\multicolumn{4}{|r|}{\textbf{Total number of WR switches: }} & \textbf{79} & \textbf{1532} & \\ \hline % \multicolumn{7}{|c|}{\textbf{(out of few hundred WR Switches and few thousands WR Nodes sold as of 2018) }} \\ \hline
\multicolumn{4}{|r|}{\textbf{WR nodes} (few thousands sold till 2018): } & \textbf{464} & \textbf{17592} & \\
\multicolumn{4}{|r|}{\textbf{WR switches} (few hundreds sold till 2018): } & \textbf{82} & \textbf{1532} & \\ \hline
% \multicolumn{7}{|l|}{\textbf{Abbreviations used}} \\ % \multicolumn{7}{|l|}{\textbf{Abbreviations used}} \\
\multicolumn{7}{|l|}{TF= time and frequency transfer, TC= time-triggered control, TS= timestamping,} \\ \multicolumn{7}{|l|}{TF= time and frequency transfer, TC= time-triggered control, TS= timestamping,} \\
\multicolumn{7}{|l|}{TD= trigger distribution, FL= Fixed-latency data transfer, RF= Radio-Freq. transfer} \\ \multicolumn{7}{|l|}{TD= trigger distribution, FL= Fixed-latency data transfer, RF= Radio-Freq. transfer} \\
\multicolumn{7}{|l|}{N= number of WR nodes, S= number of WR switches, L= number of layers} \\ \hline \multicolumn{7}{|l|}{N= number of WR nodes, S= number of WR switches, L= number of layers} \\ \hline
% \multicolumn{7}{|l|}{A: accuracy, P: precision, Link len. - it is the lenght of link between devices in the network, Tot. distance = the total distance that the networks spans } \\ % \multicolumn{7}{|l|}{A: accuracy, P: precision, Link len. - it is the lenght of link between devices in the network, Tot. distance = the total distance that the networks spans } \\
% \multicolumn{7}{|l|}{} \\ \hline % \multicolumn{7}{|l|}{} \\ \hline
\end{tabular} \end{tabular}
\label{tab:applications} \label{tab:applications}
\end{table} \end{table}
Application-triggered enhancements are described in
Section~\ref{sec:WRenhancements}. Finally, in Section~\ref{sec:WRin1588} we
briefly describe the integration of WR into the
IEEE 1588 standard and we conclude in Section~\ref{sec:conclusions}.
\section{WR Network Elements} \section{WR Network Elements}
\label{sec:wrElements} \label{sec:wrElements}
...@@ -224,9 +227,9 @@ WR network elements, WR nodes and WR switches, are openly available on the Open ...@@ -224,9 +227,9 @@ WR network elements, WR nodes and WR switches, are openly available on the Open
While all of the WR networks use the same design of While all of the WR networks use the same design of
the WR switch \cite{biblio:wr-switch}, the WR switch \cite{biblio:wr-switch},
the design of WR nodes depends on the application. Therefore the WR node design is made available the design of WR nodes depends on the application. Therefore the WR node design is made available
as an open-source intellectual property (IP) Core \cite{biblio:wr-node} that can be easily used in one of as an open-source intellectual property (IP) core \cite{biblio:wr-node} that can be easily used in one of
the supported boards or integrated into a custom design. WR-compatible boards the supported boards or integrated into a custom design. WR-compatible boards
are available on OHWR in various form factors, including: are available on OHWR in various form factors, including
% Peripheral Component Interconnect Express (PCIe) \cite{biblio:spec}, % Peripheral Component Interconnect Express (PCIe) \cite{biblio:spec},
% Versa Module Europa bus (VME) \cite{biblio:svec}, % Versa Module Europa bus (VME) \cite{biblio:svec},
% Advanced Mezzanine Card (AMC)\cite{biblio:AFC}\cite{biblio:AFCK}, % Advanced Mezzanine Card (AMC)\cite{biblio:AFC}\cite{biblio:AFCK},
...@@ -279,14 +282,16 @@ The most basic application of WR is the transfer of time and frequency from the ...@@ -279,14 +282,16 @@ The most basic application of WR is the transfer of time and frequency from the
Grandmaster WR switch/node (Grandmaster) to all other WR switches/nodes in Grandmaster WR switch/node (Grandmaster) to all other WR switches/nodes in
the WR network. WR ensures that the Pulse Per Second (PPS) outputs of all the the WR network. WR ensures that the Pulse Per Second (PPS) outputs of all the
WR switches/nodes in the WR network are aligned to the PPS output of the WR switches/nodes in the WR network are aligned to the PPS output of the
Grandmaster with a sub-nanosecond accuracy and tens of picoseconds precision. WR switches and Grandmaster with a sub-nanosecond accuracy and tens of picoseconds precision, mean offset and standard deviation respectively.
% The accuracy is the mean offset between the PPS outputs while precision is the standard deviation of this offset.
WR switches and
nodes use and can output a clock signal (e.g. 10MHz, 125MHz) that is traceable to that nodes use and can output a clock signal (e.g. 10MHz, 125MHz) that is traceable to that
of the Grandmaster. of the Grandmaster.
In most applications, the Grandmaster is connected to a clock reference. Typically, In most applications the Grandmaster is connected to a clock reference.
this is a Cesium or Rubidium oscillator disciplined by a global This typically is a Cesium or a Rubidium oscillator disciplined by a global
navigation satellite system (GNSS) \cite{biblio:PolaRx4e}\cite{biblio:CS4000}\cite{biblio:GM-Meinberg}. navigation satellite system (GNSS) \cite{biblio:PolaRx4e}\cite{biblio:CS4000}\cite{biblio:GM-Meinberg}.
In such case, the time and frequency transferred by WR are traceable to In such cases, the time and frequency transferred by WR are traceable to
the International Atomic Time (TAI). the International Atomic Time (TAI).
% Although all of WR applications are based on precise transfer of time and % Although all of WR applications are based on precise transfer of time and
...@@ -311,25 +316,26 @@ USA (NIST) and Italy (INRIM) have WR installations, see Table~\ref{tab:timelabs} ...@@ -311,25 +316,26 @@ USA (NIST) and Italy (INRIM) have WR installations, see Table~\ref{tab:timelabs}
% The improved WR Switches are now commercially available \cite{biblio:WR-LJD-switch}. % The improved WR Switches are now commercially available \cite{biblio:WR-LJD-switch}.
% The results from time laboratories studies are summarized in Table~\ref{tab:timelabs}. % The results from time laboratories studies are summarized in Table~\ref{tab:timelabs}.
\begin{table}[!ht] \begin{table}[!ht]
\caption{} \caption{White Rabbit installations in national time laboratories}
\centering \centering
\scriptsize \scriptsize
\begin{tabular}{ \begin{tabular}{
| p{0.7cm} | p{0.75cm} | p{2.3cm} | p{0.5cm} | p{1.5cm} | c | } \hline | p{0.7cm} | p{0.75cm} | p{2.3cm} | p{0.5cm} | p{1.5cm} | c | } \hline
\textbf{Time} & \textbf{Link} & \textbf{Link } & \textbf{Time } & \textbf{Time} & \textbf{Ref} \\ \textbf{Time} & \textbf{Link} & \textbf{Link } & \textbf{Time } & \textbf{Time} & \textbf{Ref} \\
\textbf{Lab} & \textbf{Length } & \textbf{Type } & \textbf{Error} & \textbf{Stability} & \textbf{} \\ \hline \textbf{Lab} & \textbf{Length } & \textbf{Type } & \textbf{Error} & \textbf{Stability} & \textbf{} \\ \hline
VTT & 950km & unidir. in DWDM & $\pm$2ns & 20ps@1000s & \cite{biblio:MIKES+VSL} \\ \cline{2-6} VTT & 950~km & unidir. in DWDM & $\pm$2ns & 20ps@1000s & \cite{biblio:MIKES+VSL} \\ \cline{2-6}
MIKES & 50km & bidir. on adjacent ITU DWDM channels & $<$1ns & ~2e-12@1s (*) & \cite{biblio:MIKES-50km} \\ \hline MIKES & 50~km & bidir. on adjacent ITU DWDM channels & $<$1ns & ~2e-12@1s (*) & \cite{biblio:MIKES-50km} \\ \hline
VSL & 2x137km & bidir. on CWDM (1470\&1490nm)(\#) & $<$8ns & 10ps@1000s & \cite{biblio:MIKES+VSL} \\ \hline VSL & 2x137~km & bidir. on CWDM (1470\&1490nm)(\#) & $<$8ns & 10ps@1000s & \cite{biblio:MIKES+VSL} \\ \hline
& 25km & unidir. at 1541nm & 150ps & 1-2ps@1000s & \cite{biblio:SYRTE-LNE-25km} \\ \cline{2-6} & 25~km & unidir. at 1541nm & 150ps & 1-2ps@1000s & \cite{biblio:SYRTE-LNE-25km} \\ \cline{2-6}
LNE- & 25km & bidir. at 1310\&1490nm & 150ps & 1-2ps@1000s & \cite{biblio:SYRTE-LNE-25km} \\ \cline{2-6} LNE- & 25~km & bidir. at 1310\&1490nm & 150ps & 1-2ps@1000s & \cite{biblio:SYRTE-LNE-25km} \\ \cline{2-6}
SYRTE & 125km & unidir. in the C-band or close OSC channel & 2.5ns & 1ps@1s (**) & \cite{biblio:SYRTE-LNE-500km} \\ \cline{2-6} SYRTE & 125~km & unidir. in the C-band or close OSC channel & 2.5ns & 1ps@1s (**) & \cite{biblio:SYRTE-LNE-500km} \\ \cline{2-6}
& 4x125km & unidir. in the C-band or close OSC channel & 2.5ns & 5.5ps@1s (**) & \cite{biblio:SYRTE-LNE-500km} \\ \hline & 4x125~km & unidir. in the C-band or close OSC channel & 2.5ns & 5.5ps@1s (**) & \cite{biblio:SYRTE-LNE-500km} \\ \hline
NIST & $<$10km & bidir. standard WR (1310\&1490nm \cite{biblio:wr-sfps}) & below 200ps & 20ps@1s & \cite{biblio:WR-NIST} \\ \hline NIST & $<$10~km & bidir. standard WR (1310\&1490nm \cite{biblio:wr-sfps})& below 200ps & 20ps@1s & \cite{biblio:WR-NIST} \\ \hline
NPL & & & & & \\ \hline NPL & 2x80~km & unidir. in DWDM & $<$1ns & & \cite{biblio:NPL}\\ \cline{2-5}
& 50km & bidir. in WDM & 800ps $\pm$56ps& & \cite{biblio:WR-INRIM} \\ \cline{2-6} & $<$10~km & bidir. standard WR & $<$1ns & & \\ \hline
INRIM & 70k m & bidir. in WDM & 610ps $\pm$47ps& & \cite{biblio:WR-INRIM} \\ \cline{2-6} & 50~km & bidir. in WDM & 800ps $\pm$56ps& & \cite{biblio:WR-INRIM} \\ \cline{2-6}
& 400km & unidir. in DWDM & & & \cite{biblio:WR-INRIM-400km} \\ \hline INRIM & 70~km & bidir. in WDM & 610ps $\pm$47ps& & \cite{biblio:WR-INRIM} \\ \cline{2-6}
& 400~km & unidir. in DWDM & & & \cite{biblio:WR-INRIM-400km} \\ \hline
\multicolumn{6}{|l|}{(D/C)WDM = (Dense/Coarse) Wavelength Division Multiplexing} \\ \multicolumn{6}{|l|}{(D/C)WDM = (Dense/Coarse) Wavelength Division Multiplexing} \\
% \multicolumn{6}{|l|}{DWDM = Dense Wavelength Division Multiplexing} \\ % \multicolumn{6}{|l|}{DWDM = Dense Wavelength Division Multiplexing} \\
...@@ -344,11 +350,11 @@ INRIM & 70k m & bidir. in WDM ...@@ -344,11 +350,11 @@ INRIM & 70k m & bidir. in WDM
\end{table} \end{table}
MIKES and INRIM MIKES and INRIM
use WR to provide their realization of UTC to clients, e.g. UTC(MIKE) over a 50~km use WR to provide their realization of UTC to clients, e.g. UTC(MIKE) over a 50~km
link to the Metsähovi Observatory \cite{biblio:MIKES-50km} for applications in geodesy, link to the Metsähovi Observatory \cite{biblio:MIKES-50km} for applications in geodesy and
% (International GNSS Service, % (International GNSS Service,
% Very-long-baseline interferometry and satellite laser ranging) % Very-long-baseline interferometry and satellite laser ranging)
UTC(INRIM) over UTC(INRIM) over
400~km to the financial district of Millano. NIST and LNE-SYRTE use WR to distribute 400~km to the financial district of Milano. NIST and LNE-SYRTE use WR to distribute
within their campus UTC(NIST) and UTC(OP), respectively. The National Time Laboratories within their campus UTC(NIST) and UTC(OP), respectively. The National Time Laboratories
are studying WR with different types and lengths of fiber links and attempt to are studying WR with different types and lengths of fiber links and attempt to
increase its performance, see Table~\ref{tab:timelabs}. increase its performance, see Table~\ref{tab:timelabs}.
...@@ -361,9 +367,9 @@ Many of the National Time Laboratories are now working together with other WR us ...@@ -361,9 +367,9 @@ Many of the National Time Laboratories are now working together with other WR us
and companies within the EU-funded project WRITE \cite{biblio:WRITE-2} to prepare WR for industrial applications. and companies within the EU-funded project WRITE \cite{biblio:WRITE-2} to prepare WR for industrial applications.
At CERN, the WR-based time and frequency transfer is used to synchronize At CERN, the WR-based time and frequency transfer is used to synchronize the
operation of different accelerators. The controller of operation of different accelerators. The controller of
the Antiproton Decelerator is synchronized over a few kilometers WR link to a similar controller the Antiproton Decelerator is synchronized over a few kilometer long WR link to a similar controller
of the LHC Injection Chain that provides proton beam to both, LHC and AD. of the LHC Injection Chain that provides proton beam to both, LHC and AD.
% Such a WR link ensures traceability to UTC and it is used instead of a GPS receiver. % Such a WR link ensures traceability to UTC and it is used instead of a GPS receiver.
...@@ -431,10 +437,10 @@ time-triggered control system of accelerators, called General Machine Timing (GM ...@@ -431,10 +437,10 @@ time-triggered control system of accelerators, called General Machine Timing (GM
\cite{biblio:GSI-WR-GMT-wiki}. \cite{biblio:GSI-WR-GMT-wiki}.
WR-based GMT has replaced the previously used system for the existing GSI WR-based GMT has replaced the previously used system for the existing GSI
accelerators and will control GSI's new Facility for Antiproton and Ion Research accelerators and will control GSI's new Facility for Antiproton and Ion Research
(FAIR) \cite{biblio:GSI-WR-GMT}. Control of GSI and FAIR requires that the (FAIR) \cite{biblio:GSI-WR-GMT}. Control of the GSI and FAIR accelerators requires that the
control-information is delivered from a common controller to any of the controlled control-information is delivered from a common controller to any of the controlled
subsystems in any of the accelerators within 500~$\mu$s. The most demanding of subsystems in any of the accelerators within 500~$\mu$s. The most demanding of
these subsystems require an accuracy of 1-5~ns. The controller, called Data Master, these subsystems requires an accuracy of 1-5~ns. The controller, called Data Master,
is a WR node. The subsystems are either WR nodes or have a direct interface with WR Nodes. is a WR node. The subsystems are either WR nodes or have a direct interface with WR Nodes.
All these WR nodes are connected to a common WR network that provides synchronization, All these WR nodes are connected to a common WR network that provides synchronization,
delivers control-information from the Data Master to all subsystems as well as delivers control-information from the Data Master to all subsystems as well as
...@@ -444,13 +450,16 @@ The WR-based ...@@ -444,13 +450,16 @@ The WR-based
GMT has been operational at GSI since 2015. First, it was used to control GMT has been operational at GSI since 2015. First, it was used to control
a small CRYRING accelerator built purposely to test the WR-based GMT a small CRYRING accelerator built purposely to test the WR-based GMT
\cite{biblio:GSI-WR-GMT-CRYRING} and consisting of 30 WR nodes in three layers of \cite{biblio:GSI-WR-GMT-CRYRING} and consisting of 30 WR nodes in three layers of
WR switches. Then, the GMT system that had been used so far was replaced with WR-based GMT WR switches. Then, the GMT system that had been used so far was replaced with a WR-based GMT
that consists of 35 WR switches and it is commissioned for operation, with a first beam in that consists of 35 WR switches and it is commissioned for operation, with a first beam in
June 2018. When FAIR is completed in 2025, the WR network at GSI and FAIR will include June 2018. When FAIR is completed in 2025, the WR network at GSI and FAIR will include
2000-3000 WR nodes connected to 300 WR switches in five layers. 2000-3000 WR nodes connected to 300 WR switches in five layers.
Despite being the main reason behind WR’s conception, a WR-based GMT to control CERN % \textcolor{gray}{
accelerators is yet to be implemented. % Despite it being the main reason behind WR’s conception, a WR-based GMT to control CERN
% accelerators is yet to be implemented.
% }
% Both, at CERN and GSI, the same WR network that is used for time-triggered control % Both, at CERN and GSI, the same WR network that is used for time-triggered control
% can provide to subsystems precise time and frequency which can be used, % can provide to subsystems precise time and frequency which can be used,
% for example, to timestamp input signals, an application described in the following % for example, to timestamp input signals, an application described in the following
...@@ -472,7 +481,7 @@ to timestamp accurately and/or precisely incoming signals. Such incoming signals ...@@ -472,7 +481,7 @@ to timestamp accurately and/or precisely incoming signals. Such incoming signals
can be either discrete pulses that are timestamped with time-to-digital converters can be either discrete pulses that are timestamped with time-to-digital converters
or analogue signals that are sampled (digitized) with the distributed frequency or analogue signals that are sampled (digitized) with the distributed frequency
and associated with the distributed time. Timestamps are usually produced to and associated with the distributed time. Timestamps are usually produced to
measure the time of flight (ToF) or correlate events between distributed systems. measure the time of flight (ToF) or to correlate events between distributed systems.
% In % In
% such cases, accurate and precise synchronization between these systems is required. % such cases, accurate and precise synchronization between these systems is required.
% If timestamps are used to measure the duration of events detected by distributed subsystems, % If timestamps are used to measure the duration of events detected by distributed subsystems,
...@@ -500,12 +509,12 @@ The most demanding WR applications in terms of timestamping are cosmic ray and ...@@ -500,12 +509,12 @@ The most demanding WR applications in terms of timestamping are cosmic ray and
neutrino detectors that record the time of arrival of particles in individual neutrino detectors that record the time of arrival of particles in individual
detector units distributed over distances up to several kilometers. detector units distributed over distances up to several kilometers.
Based on the difference Based on the difference
in the times of arrival of the same particles detected by different unit, the trajectories of these particles are calculated. For these in the times of arrival of the same particles detected by different units, the trajectories of these particles are calculated. For these
applications, a high precision and accuracy is required in harsh applications, a high precision and accuracy is required in harsh
environmental conditions due to their locations \cite{biblio:TAIGA-WR-harsh-env}. environmental conditions due to their locations \cite{biblio:TAIGA-WR-harsh-env}.
The Large High Altitude Air Shower Observatory (LHAASO), located at 4410~m above The Large High Altitude Air Shower Observatory (LHAASO), located at 4410~m above
sea level in China (Tibert), requires a 500~ps RMS \cite{biblio:LHAASO} alignment sea level in China (Tibetan Plateau), requires a 500~ps RMS \cite{biblio:LHAASO} alignment
of timestamps produced by 7000 WR nodes distributed over 1~km$^2$ and exposed to of timestamps produced by 7000 WR nodes distributed over 1~km$^2$ and exposed to
day-night variation of -10 to +55 degrees Celsius. To meet such requirements, active day-night variation of -10 to +55 degrees Celsius. To meet such requirements, active
compensation of temperature-related hardware delays has been implemented compensation of temperature-related hardware delays has been implemented
...@@ -514,15 +523,15 @@ calibrated using a portable calibrator \cite{biblio:LHAASO-WR-calibrator}. ...@@ -514,15 +523,15 @@ calibrated using a portable calibrator \cite{biblio:LHAASO-WR-calibrator}.
These methods have proved to work in a prototype installation that has been running These methods have proved to work in a prototype installation that has been running
since 2014 (50 WR nodes, 4 WR switches in 4 layers, \cite{biblio:LHAASO-WR-prototype}). since 2014 (50 WR nodes, 4 WR switches in 4 layers, \cite{biblio:LHAASO-WR-prototype}).
The Cubic Kilometre Neutrino Telescope (KM3NeT)\cite{biblio:KM3NeT} is a research The Cubic Kilometre Neutrino Telescope (KM3NeT \cite{biblio:KM3NeT}) is a research
infrastructure housing the next generation neutrino telescopes located at the infrastructure housing the next generation neutrino telescopes located at the
bottom of the Mediterranean Sea, off-shore France and Italy. The needed angular bottom of the Mediterranean Sea. The needed angular
resolution of 0.1 degree means that the submerged \textit{digital optical modules} (DOMs), resolution of 0.1 degree means that the submerged Digital Optical Modules (DOMs),
which constitute KM3NeT, must be synchronized with 1~ns accuracy and a which constitute KM3NeT, must be synchronized with 1~ns accuracy and a
few 100~ps precision. 4140 DOMs at 3500~m depth 100~km off-shore of Italy and few 100~ps precision. 4140 DOMs at 3500~m depth 100~km off-shore of Italy and
2070 DOMs at 2475~m depth 40~km off-shore France will be synchronized with an on-shore 2070 DOMs at 2475~m depth 40~km off-shore of France will be synchronized with an on-shore
reference using WR network \cite{biblio:WR-KM3NeT-Letter}\cite{biblio:WR-KM3NeT-presentation}. reference using a WR network \cite{biblio:WR-KM3NeT-Letter}\cite{biblio:WR-KM3NeT-presentation}.
Initial tests have been successfully performed with 18 DOMs off-shore France and Italy to validate the system. Initial tests have been successfully performed with 18 DOMs to validate the system.
Other applications of WR that use timestamping include Other applications of WR that use timestamping include
% the Cubic Kilometre Neutrino Telescope (KM3NeT) % the Cubic Kilometre Neutrino Telescope (KM3NeT)
...@@ -530,11 +539,11 @@ Other applications of WR that use timestamping include ...@@ -530,11 +539,11 @@ Other applications of WR that use timestamping include
% located at the bottom of the Mediterranean Sea, % located at the bottom of the Mediterranean Sea,
the Tunka Advanced Instrument for cosmic ray physics and Gamma Astronomy (TAIGA) in Siberia the Tunka Advanced Instrument for cosmic ray physics and Gamma Astronomy (TAIGA) in Siberia
\cite{biblio:TAIGA-WR-1}\cite{biblio:TAIGA-WR-2}\cite{biblio:TAIGA-WR-harsh-env}, \cite{biblio:TAIGA-WR-1}\cite{biblio:TAIGA-WR-2}\cite{biblio:TAIGA-WR-harsh-env},
Cherenkov Telescope Array to be built in Chile and Spain \cite{biblio:CTA-WR-timestamps}, Cherenkov Telescope Array (CTA) to be built in Chile and Spain \cite{biblio:CTA-WR-timestamps},
the Extreme Light Infrastructures in Hungary \cite{biblio:ELI-ALP-WR} and Czech Republic the Extreme Light Infrastructures (ELI) in Hungary \cite{biblio:ELI-ALP-WR} and Czech Republic
\cite{biblio:ELI-BEAMS-WR}, Satellite Laser Ranging at German Aerospace Center, \cite{biblio:ELI-BEAMS-WR}, Satellite Laser Ranging at German Aerospace Center (DLR),
High Precision Timestamps Daily File Service at German Stock Exchange (Deutsche Boerse) \cite{biblio:WR-EUREXCHANGE} High Precision Timestamps Daily File Service at German Stock Exchange (Deutsche B{\"o}rse) \cite{biblio:WR-EUREXCHANGE}
or Power Industry and Smart Grid studied at Swiss Federal or Phasor Measurement Units synchronization for Power Industry and Smart Grid studied at Swiss Federal
Institute of Technology Lausanne (EPFL) \cite{biblio:EPFL-WR-PMU}. Institute of Technology Lausanne (EPFL) \cite{biblio:EPFL-WR-PMU}.
...@@ -564,7 +573,7 @@ Institute of Technology Lausanne (EPFL) \cite{biblio:EPFL-WR-PMU}. ...@@ -564,7 +573,7 @@ Institute of Technology Lausanne (EPFL) \cite{biblio:EPFL-WR-PMU}.
\subsection{Basic Concept} \subsection{Basic Concept}
Trigger distribution combines, to some extend, the time-triggered control and precise timestamping Trigger distribution combines, to some extent, the time-triggered control and precise timestamping
described before. In this application, an input trigger signal is timestamped by a WR node and sent over the described before. In this application, an input trigger signal is timestamped by a WR node and sent over the
WR network to many WR nodes that act upon the received message simultaneously, at WR network to many WR nodes that act upon the received message simultaneously, at
a precise delay with respect to the input signal. a precise delay with respect to the input signal.
...@@ -610,8 +619,8 @@ their actions. ...@@ -610,8 +619,8 @@ their actions.
The concept that has been proven to work in WRTD is now being generalized to The concept that has been proven to work in WRTD is now being generalized to
provide trigger distribution for CERN's Open Analog Signals Information System provide trigger distribution for CERN's Open Analog Signals Information System
(OASIS) \cite{biblio:OASIS}. OASIS is a gigantic distributed oscilloscope that (OASIS) \cite{biblio:OASIS}. OASIS is a gigantic distributed oscilloscope that
provides $\approx$6000 input channels and spans all CERN's accelerators except LHC. provides over 6000 input channels and spans all CERN's accelerators except LHC.
Triggers in this system are currently distributed via coax cables that may be 1~km long without Triggers in this system are currently distributed via coax cables that may be one kilometer long without
delay compensation and multiplexed using analogue multiplexers. In order to use delay compensation and multiplexed using analogue multiplexers. In order to use
OASIS to diagnose LHC and to improve its performance, the distribution of triggers OASIS to diagnose LHC and to improve its performance, the distribution of triggers
is being upgraded to use WR. The WR-based trigger distribution in OASIS is meant is being upgraded to use WR. The WR-based trigger distribution in OASIS is meant
...@@ -640,7 +649,7 @@ The time of data transmission is timestamped and this timestamp ...@@ -640,7 +649,7 @@ The time of data transmission is timestamped and this timestamp
is sent in the Ethernet frame with the data. When the data is received, a programmable is sent in the Ethernet frame with the data. When the data is received, a programmable
delay is added to the transmission timestamp and the associated data is provided delay is added to the transmission timestamp and the associated data is provided
to an application precisely at the delayed time. Such a functionality is implemented to an application precisely at the delayed time. Such a functionality is implemented
by the so-called "WR Streamers" IP Core \cite{biblio:wr-streamers} which adds a by the so-called "WR Streamers" IP core \cite{biblio:wr-streamers} which adds a
data transmission layer on top of WR and acts as a fixed-latency FIFO over Ethernet. data transmission layer on top of WR and acts as a fixed-latency FIFO over Ethernet.
By providing such functionality to the application, the application does not need By providing such functionality to the application, the application does not need
to be aware of time but rather processes data as it comes, knowing that all the to be aware of time but rather processes data as it comes, knowing that all the
...@@ -662,7 +671,7 @@ While the RF cavities ...@@ -662,7 +671,7 @@ While the RF cavities
simply follow the ramp of the magnetic field, the power converters adjust the current simply follow the ramp of the magnetic field, the power converters adjust the current
of the magnets such that the intended B-value is obtained, closing a control of the magnets such that the intended B-value is obtained, closing a control
loop. BTrain is essential to the operation of most of CERN accelerators, i.e. loop. BTrain is essential to the operation of most of CERN accelerators, i.e.
Booster, PS, SPS, LEIR, AD, and ELENA. Booster, PS, SPS, LEIR, AD and ELENA.
% \begin{figure}[!ht] % \begin{figure}[!ht]
% \centering % \centering
% \vspace{0.5cm} % \vspace{0.5cm}
...@@ -678,7 +687,7 @@ WR-based distribution of the absolute B-value and additional information ...@@ -678,7 +687,7 @@ WR-based distribution of the absolute B-value and additional information
at 250~kHz (every $4\mu$s) from the measurement WR node to all the other WR nodes at 250~kHz (every $4\mu$s) from the measurement WR node to all the other WR nodes
that are integrated with RF cavities, power converters and beam instrumentation. In the most that are integrated with RF cavities, power converters and beam instrumentation. In the most
demanding accelerator, SPS, the data must be delivered over 2 hops (WR switches) demanding accelerator, SPS, the data must be delivered over 2 hops (WR switches)
with latency of $10\mu s\pm 8ns$. with a latency of $10\mu s\pm 8ns$.
The WR-BTtrain has been successfully evaluated in the PS accelerator where it has The WR-BTtrain has been successfully evaluated in the PS accelerator where it has
been running operationally since 2017 \cite{biblio:WR-BTrain-RF}. By 2021, all been running operationally since 2017 \cite{biblio:WR-BTrain-RF}. By 2021, all
...@@ -688,7 +697,7 @@ the CERN accelerators, except LHC, should be running WR-BTrain operationally \ci ...@@ -688,7 +697,7 @@ the CERN accelerators, except LHC, should be running WR-BTrain operationally \ci
% WR switches and 2-5 WR nodes. % WR switches and 2-5 WR nodes.
% } % }
Fixed-latency data transfer is considered for the operation of the Fixed-latency data transfer is also considered for the operation of the
Nuclotron-based Ion Collider Facility (NICE) at the Joint Institute for Nuclear Nuclotron-based Ion Collider Facility (NICE) at the Joint Institute for Nuclear
Research (JINR) \cite{biblio:JINR} that already uses WR as the main clock Research (JINR) \cite{biblio:JINR} that already uses WR as the main clock
and time distribution system \cite{biblio:JINR-WR}. and time distribution system \cite{biblio:JINR-WR}.
...@@ -704,9 +713,10 @@ Radio-frequency (RF) transfer over WR network allows the digitization of periodi ...@@ -704,9 +713,10 @@ Radio-frequency (RF) transfer over WR network allows the digitization of periodi
the sending of the sending of
their digital form over a WR network, and the subsequent regeneration of the signal coherently with a fixed delay in many their digital form over a WR network, and the subsequent regeneration of the signal coherently with a fixed delay in many
WR slave nodes. Such a digital RF transfer provides a number of advantages over an analogue transmission of RF signals. For example, it is WR slave nodes. Such a digital RF transfer provides a number of advantages over an analogue transmission of RF signals. For example, it is
scalable and allows transmission of multiple RF signals from multiple sources over a single WR network scalable and allows the transmission of multiple RF signals from multiple sources over a single WR network,
whereas analogue transmission typically requires dedicated network per source and signal. It also allows easy and automatic phase-alignment of the output whereas analogue transmission typically requires a dedicated network per source and signal. It also allows easy and automatic phase-alignment of the output
RF signals with compensation for temperature changes of transmission cables whereas such alignment and compensation in analogue transmission is very challenging. RF signals with compensation for temperature changes of transmission cables, whereas such alignment and compensation in analogue transmission is very challenging.
% Lastly, the digital RF transfer over WR network minimizes bandwidth of transmitted data allowing to use WR network also for other purposes. % Lastly, the digital RF transfer over WR network minimizes bandwidth of transmitted data allowing to use WR network also for other purposes.
In the RF transfer over WR Network schema, depicted in Figure~\ref{fig:RFoverWR} and detailed in \cite{biblio:WR-LIST}, In the RF transfer over WR Network schema, depicted in Figure~\ref{fig:RFoverWR} and detailed in \cite{biblio:WR-LIST},
...@@ -723,7 +733,7 @@ input RF signal. The error measured by the phase detector is an input to a ...@@ -723,7 +733,7 @@ input RF signal. The error measured by the phase detector is an input to a
loop filter (e.g. Integral-Proportional controller) that steers the DDS to produce a signal identical to the RF input - loop filter (e.g. Integral-Proportional controller) that steers the DDS to produce a signal identical to the RF input -
effectively locking the DDS to the input signal. effectively locking the DDS to the input signal.
The tuning words of the DDS are the digital form of the RF input The tuning words of the DDS are the digital form of the RF input
that is sent over WR network. Each of the receiving WR slave nodes recreates the RF input signal that is sent over the WR network. Each of the receiving WR slave nodes recreates the RF input signal
by using the received tuning words to control the local DDS with a fixed delay. by using the received tuning words to control the local DDS with a fixed delay.
In such way, the WR slave nodes produce RF outputs that are syntonized with In such way, the WR slave nodes produce RF outputs that are syntonized with
the RF input, phase-aligned among each other, and delayed with respect to the RF input -- the RF input, phase-aligned among each other, and delayed with respect to the RF input --
...@@ -738,16 +748,16 @@ of the digital RF signal transmission, thus negligible. ...@@ -738,16 +748,16 @@ of the digital RF signal transmission, thus negligible.
The WR-based radio-frequency transfer is being implemented in the European Synchrotron Radiation The WR-based radio-frequency transfer is being implemented in the European Synchrotron Radiation
Facility (ESRF) \cite{biblio:ESRF}\cite{biblio:ESRF-WR}. The operation of the ESRF accelerator facility Facility (ESRF) \cite{biblio:ESRF}\cite{biblio:ESRF-WR}. The operation of the ESRF accelerator facility
is controlled by a "Bunch Clock" system\footnote{ is controlled by a "Bunch Clock" system\footnote{
Bunch Clock is a clock signal that is synchronous with particle bunches A "Bunch Clock" system generates a clock signal that is synchronous with particle bunches
circulating in a synchrotron or an accelerator. The "Bunch Clock" system generates such a clock signal.} circulating in a synchrotron or an accelerator.}
that delivers to accelerator subsystems a that delivers to accelerator subsystems a
$\approx$352 MHz RF signal and triggers initiating sequential actions synchronous $\approx$352 MHz RF signal and triggers initiating sequential actions synchronous
to the RF signal, such as to the RF signal, such as
"gun trigger", "injection trigger" or "extraction trigger"\footnote{ "gun trigger", "injection trigger" or "extraction trigger"\footnote{
"Gun trigger" initiates generation of an electron bunch at the LINAC input, "Gun trigger" initiates generation of an electron bunch at the LINAC input,
"injection trigger" initiates transfer of the bunch from the LINAC into the Booster, "injection trigger" initiates the transfer of the bunch from the LINAC into the Booster,
"extraction trigger" initiates extraction of the bunch from the Booster into the "extraction trigger" initiates the extraction of the bunch from the Booster into the
Storage Ring at the end of acceleration, see \cite{biblio:ESRF-WR} for details. Storage Ring at the end of acceleration \cite{biblio:ESRF-WR}.
}. }.
The jitter of the output RF signal is required to be below 50~ps. The RF signal is continuously The jitter of the output RF signal is required to be below 50~ps. The RF signal is continuously
trimmed around the 352~MHz value as the tuning parameter in the "fast orbit feedback" trimmed around the 352~MHz value as the tuning parameter in the "fast orbit feedback"
...@@ -755,7 +765,7 @@ process. Apart from the 352~MHz signal, other frequencies are distributed, such ...@@ -755,7 +765,7 @@ process. Apart from the 352~MHz signal, other frequencies are distributed, such
355~kHz Storage Ring revolution frequency or the 10~Hz Injection sequence. 355~kHz Storage Ring revolution frequency or the 10~Hz Injection sequence.
The current ESRF "Bunch Clock" system is being refurbished to use WR \cite{biblio:ESRF-WR}. The current ESRF "Bunch Clock" system is being refurbished to use WR \cite{biblio:ESRF-WR}.
The solution has passed a 6-months validation tests in 2015. In 2016, a prototype system The solution has passed a 6-months validation test in 2015. In 2016, a prototype system
successfully injected successfully injected
bunches in the storage ring providing $<$10ps jitter. A system consisting bunches in the storage ring providing $<$10ps jitter. A system consisting
of a WR switch and eight WR nodes is expected to be operational in July 2018. It of a WR switch and eight WR nodes is expected to be operational in July 2018. It
...@@ -1175,15 +1185,15 @@ of WR performance that are summarized in this section. ...@@ -1175,15 +1185,15 @@ of WR performance that are summarized in this section.
The applications of WR for time and frequency transfer in National Time Laboratories The applications of WR for time and frequency transfer in National Time Laboratories
as well as for RF transfer in CERN's SPS require improvement of jitter and clock as well as for RF transfer in CERN's SPS require improvement of jitter and clock
stability. stability.
The frequency transfer over WR network was characterized in The frequency transfer over a WR network was characterized in
\cite{biblio:WR-characteristics} and its ultimate performance limits \cite{biblio:WR-characteristics} and its ultimate performance limits were
studied in \cite{biblio:WR-ultimate-limits}. The studies studied in \cite{biblio:WR-ultimate-limits}. The studies
\cite{biblio:WR-ultimate-limits}\cite{biblio:MIKES-50km}\cite{biblio:SYRTE-LNE-500km} \cite{biblio:WR-ultimate-limits}\cite{biblio:MIKES-50km}\cite{biblio:SYRTE-LNE-500km}
have shown that the performance of a WR switch currently commercially available can be have shown that the performance of a WR switch currently commercially available can be
improved as follows: improved as follows:
\begin{itemize} \begin{itemize}
\item ADEV clock stability (tau=1s) \textbf{from 1e-11 to 1e-12}, \item Allan deviation (ADEV) \textbf{from 1e-11 to 1e-12} ($\tau=1s$),
\item Random jitter \textbf{from 11 to 1.1~ps RMS} (integration bandwidth from 1Hz to 100kHz). \item Random jitter \textbf{from 11 to 1.1~ps RMS} (1~Hz to 100~kHz). %(integration bandwidth from 1~Hz to 100~kHz).
\end{itemize} \end{itemize}
This prompted the development of the Low-Jitter Daughterboard This prompted the development of the Low-Jitter Daughterboard
\cite{biblio:WR-LJD}, which improves the performance of the WR switch to 1e-12 without any \cite{biblio:WR-LJD}, which improves the performance of the WR switch to 1e-12 without any
...@@ -1198,7 +1208,7 @@ within the WRITE project \cite{biblio:WRITE-2}. ...@@ -1198,7 +1208,7 @@ within the WRITE project \cite{biblio:WRITE-2}.
\subsection{Temperature Compensation} \subsection{Temperature Compensation}
\label{sec:} \label{sec:}
The studies \cite{biblio:wr-cngs} have shown that the temperature variation Studies \cite{biblio:wr-cngs} have shown that the temperature variation
of WR nodes and switches degrades synchronization performance, still of WR nodes and switches degrades synchronization performance, still
maintaining sub-nanosecond accuracy. maintaining sub-nanosecond accuracy.
This degradation and its sources have been carefully characterized This degradation and its sources have been carefully characterized
...@@ -1208,9 +1218,9 @@ These delays are usually calibrated for WR devices ...@@ -1208,9 +1218,9 @@ These delays are usually calibrated for WR devices
\cite{biblio:wrCalibration} at a room temperature and assumed constant throughout \cite{biblio:wrCalibration} at a room temperature and assumed constant throughout
operation. Their variation however is linear with temperature and so an online operation. Their variation however is linear with temperature and so an online
correction can be applied. Such correction was developed for the LHAASO correction can be applied. Such correction was developed for the LHAASO
experiment \cite{biblio:wr-cngs}, which requires 500ps RMS experiment \cite{biblio:wr-cngs}, which requires 500~ps RMS
synchronization of 7000 WR nodes in a harsh environmental. For temperatures between synchronization of 7000 WR nodes in a harsh environment. For temperatures between
-10 and 50 degrees Celsius, the developed correction reduces the -10 and +50 degrees Celsius, the developed correction reduces the
peak-to-peak variation from 700~ps to $<$150~ps with a standard deviation $<$50~ps \cite{biblio:LHAASO-WR-temp}. peak-to-peak variation from 700~ps to $<$150~ps with a standard deviation $<$50~ps \cite{biblio:LHAASO-WR-temp}.
% This online compensation % This online compensation
...@@ -1221,7 +1231,7 @@ peak-to-peak variation from 700~ps to $<$150~ps with a standard deviation $<$50~ ...@@ -1221,7 +1231,7 @@ peak-to-peak variation from 700~ps to $<$150~ps with a standard deviation $<$50~
\label{sec:LongLinks} \label{sec:LongLinks}
Experiments have shown that WR can successfully provide sub-nanosecond accuracy on bidirectional links up to 80~km Experiments have shown that WR can successfully provide sub-nanosecond accuracy on bidirectional links up to 80~km
\cite{biblio:WR-INRIM}\cite{biblio:WR-INRIM}\cite{biblio:SYRTE-LNE-25km}\cite{biblio:MIKES-50km}\cite{biblio:SKA-80km}, \cite{biblio:MIKES-50km}\cite{biblio:SYRTE-LNE-25km}\cite{biblio:WR-INRIM}\cite{biblio:SKA-80km},
taking care for the effects described in the next section. taking care for the effects described in the next section.
Links longer than 80~km require active amplifiers and/or unidirectional fibers. Links longer than 80~km require active amplifiers and/or unidirectional fibers.
This deteriorates accuracy due to an unknown asymmetry. This deteriorates accuracy due to an unknown asymmetry.
...@@ -1229,7 +1239,7 @@ On the 137~km bidirectional link in the Netherlands \cite{biblio:MIKES+VSL}, ...@@ -1229,7 +1239,7 @@ On the 137~km bidirectional link in the Netherlands \cite{biblio:MIKES+VSL},
dedicated optical amplifiers that work with bidirectional fibers are used in dedicated optical amplifiers that work with bidirectional fibers are used in
an attempt to overcome these limitation. The tests so far have shown $<$8~ns accuracy an attempt to overcome these limitation. The tests so far have shown $<$8~ns accuracy
while a new "in-site" calibration under development at VLS is expected to calibrate while a new "in-site" calibration under development at VLS is expected to calibrate
out this asymmetry (over a 2x 137km link) to a few 0.1~ns or less \cite{biblio:VLS-WR-insite-calib}. out this asymmetry (over a 2x 137~km link) to a few hundred picoseconds or less \cite{biblio:VLS-WR-insite-calib}.
On the 950~km unidirectional link in Finland \cite{biblio:MIKES+VSL}, GPS precise point positioning On the 950~km unidirectional link in Finland \cite{biblio:MIKES+VSL}, GPS precise point positioning
(PPP) was used to calibrate asymmetry and achieve $\pm$2~ns accuracy. This (PPP) was used to calibrate asymmetry and achieve $\pm$2~ns accuracy. This
method requires re-calibration after any disruption of the network. Laboratory method requires re-calibration after any disruption of the network. Laboratory
...@@ -1247,10 +1257,10 @@ However, the variation of fiber temperature results in changes of the actual ...@@ -1247,10 +1257,10 @@ However, the variation of fiber temperature results in changes of the actual
while the variation of WR nodes/switches temperature result in laser wavelength while the variation of WR nodes/switches temperature result in laser wavelength
variation (e.g. 17~ps/nm km for 1550 nm). These and other variation (e.g. 17~ps/nm km for 1550 nm). These and other
effects analyzed in \cite{biblio:SKA-80km} are significant on long links and effects analyzed in \cite{biblio:SKA-80km} are significant on long links and
can amount to over 3~ns inaccuracy for 80 km bidirectional link using 1490/1550~nm can amount to over 3~ns inaccuracy for 80 km bidirectional links using 1490/1550~nm
and exposed to 50 degrees Celsius temperature variation. The Square Kilometre Array (SKA) \cite{biblio:SKA} and exposed to a 50 degrees Celsius temperature variation. The Square Kilometre Array (SKA) \cite{biblio:SKA}
radio telescope mitigates these effects to achieve $<$1~ns accuracy on 80~km links radio telescope mitigates these effects to achieve $<$1~ns accuracy on 80~km links
by using DWDM SFP on ITU channels C21/C22 (1560.61/1558.98~nm) and combining them by using a DWDM SFP on ITU channels C21/C22 (1560.61/1558.98~nm) and combining them
on a single fiber via a simple DWDM channel filter, as described in \cite{biblio:SKA-80km}. on a single fiber via a simple DWDM channel filter, as described in \cite{biblio:SKA-80km}.
% To meet its $<$2ns accuracy requirement on 173~km WR % To meet its $<$2ns accuracy requirement on 173~km WR
...@@ -1300,8 +1310,8 @@ that mandates a number of IEEE 1588's new optional features. All together, these ...@@ -1300,8 +1310,8 @@ that mandates a number of IEEE 1588's new optional features. All together, these
additions are functionally equivalent to WR and allow the support of WR hardware. additions are functionally equivalent to WR and allow the support of WR hardware.
Along with the new features, informative annexes are added with a "standardized" Along with the new features, informative annexes are added with a "standardized"
description of the WR calibration procedures \cite{biblio:wrCalibration} and description of the WR calibration procedures \cite{biblio:wrCalibration} and
an example implementation of the High Accuracy profile that achieves an example implementation of the High Accuracy profile, a.k.a White Rabbit, that achieves
sub-nanosecond synchronization, a.k.a White Rabbit. The mapping between WR and High Accuracy sub-nanosecond synchronization. The mapping between WR and High Accuracy
is described in \cite{biblio:WRin1588}. is described in \cite{biblio:WRin1588}.
% \newpage % \newpage
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