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Wall-Current-Monitor based Ghost and Satellite Bunch Detection in the CERN PS and the LHC Accelerators
While most LHC detectors and instrumentation systems are optimised for a nominal bunch spacing of 25 ns, the LHC RF cavities themselves operate at the 10th harmonic of the maximum bunch frequency. Due to the beam production scheme and transfers in the injector chain, part of the nominally ‘empty’ RF...
Autores principales: | , , , , |
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Lenguaje: | eng |
Publicado: |
2012
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Materias: | |
Acceso en línea: | http://cds.cern.ch/record/1476075 |
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author | Steinhagen, R J Bart-Pedersen, S Belleman, J Bohl, T Damerau, H |
author_facet | Steinhagen, R J Bart-Pedersen, S Belleman, J Bohl, T Damerau, H |
author_sort | Steinhagen, R J |
collection | CERN |
description | While most LHC detectors and instrumentation systems are optimised for a nominal bunch spacing of 25 ns, the LHC RF cavities themselves operate at the 10th harmonic of the maximum bunch frequency. Due to the beam production scheme and transfers in the injector chain, part of the nominally ‘empty’ RF buckets may contain particles, referred to as ghost or satellite bunches. These populations must be accurately quantified for high-precision experiments, luminosity calibration and control of parasitic particle encounters at the four LHC interaction points. This contribution summarises the wall-current-monitor based ghost and satellite bunch measurements in CERN’s PS and LHC accelerators. Instrumentation set-up, post-processing and achieved performance are discussed. |
id | cern-1476075 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2012 |
record_format | invenio |
spelling | cern-14760752022-08-17T13:25:51Zhttp://cds.cern.ch/record/1476075engSteinhagen, R JBart-Pedersen, SBelleman, JBohl, TDamerau, HWall-Current-Monitor based Ghost and Satellite Bunch Detection in the CERN PS and the LHC AcceleratorsAccelerators and Storage RingsWhile most LHC detectors and instrumentation systems are optimised for a nominal bunch spacing of 25 ns, the LHC RF cavities themselves operate at the 10th harmonic of the maximum bunch frequency. Due to the beam production scheme and transfers in the injector chain, part of the nominally ‘empty’ RF buckets may contain particles, referred to as ghost or satellite bunches. These populations must be accurately quantified for high-precision experiments, luminosity calibration and control of parasitic particle encounters at the four LHC interaction points. This contribution summarises the wall-current-monitor based ghost and satellite bunch measurements in CERN’s PS and LHC accelerators. Instrumentation set-up, post-processing and achieved performance are discussed.CERN-ATS-2012-249oai:cds.cern.ch:14760752012-04-15 |
spellingShingle | Accelerators and Storage Rings Steinhagen, R J Bart-Pedersen, S Belleman, J Bohl, T Damerau, H Wall-Current-Monitor based Ghost and Satellite Bunch Detection in the CERN PS and the LHC Accelerators |
title | Wall-Current-Monitor based Ghost and Satellite Bunch Detection in the CERN PS and the LHC Accelerators |
title_full | Wall-Current-Monitor based Ghost and Satellite Bunch Detection in the CERN PS and the LHC Accelerators |
title_fullStr | Wall-Current-Monitor based Ghost and Satellite Bunch Detection in the CERN PS and the LHC Accelerators |
title_full_unstemmed | Wall-Current-Monitor based Ghost and Satellite Bunch Detection in the CERN PS and the LHC Accelerators |
title_short | Wall-Current-Monitor based Ghost and Satellite Bunch Detection in the CERN PS and the LHC Accelerators |
title_sort | wall-current-monitor based ghost and satellite bunch detection in the cern ps and the lhc accelerators |
topic | Accelerators and Storage Rings |
url | http://cds.cern.ch/record/1476075 |
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