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Estimated Impact of Ground Motion on HL-LHC Beam Orbit
The High Luminosity LHC (HL-LHC) will require unprecedented orbit stability at the low beta collision points (IP1 and IP5), and the effect of seismic noise might become a relevant source of luminosity loss. Many studies have been conducted in the past to characterise the actual ground motion in the...
Autores principales: | , , , , |
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Lenguaje: | eng |
Publicado: |
2018
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.18429/JACoW-IPAC2018-THPAF040 http://cds.cern.ch/record/2648557 |
_version_ | 1780960768713293824 |
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author | Gamba, Davide Corsini, Roberto Guinchard, Michael Schaumann, Michaela Wenninger, Jorg |
author_facet | Gamba, Davide Corsini, Roberto Guinchard, Michael Schaumann, Michaela Wenninger, Jorg |
author_sort | Gamba, Davide |
collection | CERN |
description | The High Luminosity LHC (HL-LHC) will require unprecedented orbit stability at the low beta collision points (IP1 and IP5), and the effect of seismic noise might become a relevant source of luminosity loss. Many studies have been conducted in the past to characterise the actual ground motion in the LHC tunnel, and recently a few geo-phones have been installed to permanently monitor the ground stability at IP1 and IP5. An estimate of the impact of the main machine element vibration on orbit at the IPs and collimators is presented, together with a first look at the data collected by the installed geo-phones. |
id | oai-inspirehep.net-1690362 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2018 |
record_format | invenio |
spelling | oai-inspirehep.net-16903622022-08-17T12:59:52Zdoi:10.18429/JACoW-IPAC2018-THPAF040http://cds.cern.ch/record/2648557engGamba, DavideCorsini, RobertoGuinchard, MichaelSchaumann, MichaelaWenninger, JorgEstimated Impact of Ground Motion on HL-LHC Beam OrbitAccelerators and Storage RingsThe High Luminosity LHC (HL-LHC) will require unprecedented orbit stability at the low beta collision points (IP1 and IP5), and the effect of seismic noise might become a relevant source of luminosity loss. Many studies have been conducted in the past to characterise the actual ground motion in the LHC tunnel, and recently a few geo-phones have been installed to permanently monitor the ground stability at IP1 and IP5. An estimate of the impact of the main machine element vibration on orbit at the IPs and collimators is presented, together with a first look at the data collected by the installed geo-phones.CERN-ACC-2018-132oai:inspirehep.net:16903622018 |
spellingShingle | Accelerators and Storage Rings Gamba, Davide Corsini, Roberto Guinchard, Michael Schaumann, Michaela Wenninger, Jorg Estimated Impact of Ground Motion on HL-LHC Beam Orbit |
title | Estimated Impact of Ground Motion on HL-LHC Beam Orbit |
title_full | Estimated Impact of Ground Motion on HL-LHC Beam Orbit |
title_fullStr | Estimated Impact of Ground Motion on HL-LHC Beam Orbit |
title_full_unstemmed | Estimated Impact of Ground Motion on HL-LHC Beam Orbit |
title_short | Estimated Impact of Ground Motion on HL-LHC Beam Orbit |
title_sort | estimated impact of ground motion on hl-lhc beam orbit |
topic | Accelerators and Storage Rings |
url | https://dx.doi.org/10.18429/JACoW-IPAC2018-THPAF040 http://cds.cern.ch/record/2648557 |
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