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How the discovery of Cold Noise delayed the production of ATLAS ITk strip tracker modules by a year
The construction of the ATLAS strip tracker barrel will require the assembly of 12,000 barrel detector modules over the course of 3.5 years. In 2022, during the module pre-production phase, modules were found to display clusters of noisy channels outside required specifications when tested at operat...
Autores principales: | , |
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Lenguaje: | eng |
Publicado: |
2023
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Materias: | |
Acceso en línea: | http://cds.cern.ch/record/2875747 |
_version_ | 1780978913736916992 |
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author | Dyckes, Ian Kurth, Matthew Glenn |
author_facet | Dyckes, Ian Kurth, Matthew Glenn |
author_sort | Dyckes, Ian |
collection | CERN |
description | The construction of the ATLAS strip tracker barrel will require the assembly of 12,000 barrel detector modules over the course of 3.5 years. In 2022, during the module pre-production phase, modules were found to display clusters of noisy channels outside required specifications when tested at operating temperatures (-40 ºC), called “Cold Noise”. Extensive investigations into the cause and mechanism of Cold Noise interrupted pre-production and occupied most barrel module assembly sites. This contribution presents an overview of the year-long investigations into Cold Noise, the final identification of the underlying mechanism and necessary changes for the transition to production. |
id | cern-2875747 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2023 |
record_format | invenio |
spelling | cern-28757472023-10-16T18:55:10Zhttp://cds.cern.ch/record/2875747engDyckes, IanKurth, Matthew GlennHow the discovery of Cold Noise delayed the production of ATLAS ITk strip tracker modules by a yearParticle Physics - ExperimentThe construction of the ATLAS strip tracker barrel will require the assembly of 12,000 barrel detector modules over the course of 3.5 years. In 2022, during the module pre-production phase, modules were found to display clusters of noisy channels outside required specifications when tested at operating temperatures (-40 ºC), called “Cold Noise”. Extensive investigations into the cause and mechanism of Cold Noise interrupted pre-production and occupied most barrel module assembly sites. This contribution presents an overview of the year-long investigations into Cold Noise, the final identification of the underlying mechanism and necessary changes for the transition to production.ATL-ITK-SLIDE-2023-559oai:cds.cern.ch:28757472023-10-16 |
spellingShingle | Particle Physics - Experiment Dyckes, Ian Kurth, Matthew Glenn How the discovery of Cold Noise delayed the production of ATLAS ITk strip tracker modules by a year |
title | How the discovery of Cold Noise delayed the production of ATLAS ITk strip tracker modules by a year |
title_full | How the discovery of Cold Noise delayed the production of ATLAS ITk strip tracker modules by a year |
title_fullStr | How the discovery of Cold Noise delayed the production of ATLAS ITk strip tracker modules by a year |
title_full_unstemmed | How the discovery of Cold Noise delayed the production of ATLAS ITk strip tracker modules by a year |
title_short | How the discovery of Cold Noise delayed the production of ATLAS ITk strip tracker modules by a year |
title_sort | how the discovery of cold noise delayed the production of atlas itk strip tracker modules by a year |
topic | Particle Physics - Experiment |
url | http://cds.cern.ch/record/2875747 |
work_keys_str_mv | AT dyckesian howthediscoveryofcoldnoisedelayedtheproductionofatlasitkstriptrackermodulesbyayear AT kurthmatthewglenn howthediscoveryofcoldnoisedelayedtheproductionofatlasitkstriptrackermodulesbyayear |