Fast orbit feedback for Diamond-II
The electron beam stability is critical for 4th generation light sources. As opposed to 10 % of beam size up to 140 Hz at Diamond, advances in detector speed and resolution at Diamond-II increase the stability requirements to 3 % up to 1 kHz. This paper presents a novel control methodology for the f...
Main Authors: | , , , , , |
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Format: | Conference item |
Language: | English |
Published: |
Publisher JACoW Publishing
2023
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_version_ | 1811140320778256384 |
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author | Kempf, I Abbott, M Bobb, L Christian, GB Rehm, G Duncan, S |
author_facet | Kempf, I Abbott, M Bobb, L Christian, GB Rehm, G Duncan, S |
author_sort | Kempf, I |
collection | OXFORD |
description | The electron beam stability is critical for 4th generation light sources. As opposed to 10 % of beam size up to 140 Hz at Diamond, advances in detector speed and resolution at Diamond-II increase the stability requirements to 3 % up to 1 kHz. This paper presents a novel control methodology for the fast orbit feedback at Diamond-II, which will stabilise the beam using two arrays of 252 slow and 144 fast correctors and 252 beam position monitors at 100 kHz. In contrast to existing approaches that separate slow and fast feedback loops, our approach is based on a two-matrix factorisation called the generalised singular value decomposition (GSVD), which decouples the system into 144 two-input modes controlled by slow and fast magnets and 108 modes controlled by slow magnets only. The GSVD-based controller is implemented in the existing Diamond storage ring using a centralised communication architecture, such as planned for Diamond-II. We present results from the Diamond storage ring and simulation, which confirm that the proposed approach meets the target specification for Diamond-II. |
first_indexed | 2024-09-25T04:20:07Z |
format | Conference item |
id | oxford-uuid:2bf1b3e5-1552-4e1b-9684-ba4ffb0a5370 |
institution | University of Oxford |
language | English |
last_indexed | 2024-09-25T04:20:07Z |
publishDate | 2023 |
publisher | Publisher JACoW Publishing |
record_format | dspace |
spelling | oxford-uuid:2bf1b3e5-1552-4e1b-9684-ba4ffb0a53702024-08-07T13:41:48ZFast orbit feedback for Diamond-IIConference itemhttp://purl.org/coar/resource_type/c_5794uuid:2bf1b3e5-1552-4e1b-9684-ba4ffb0a5370EnglishSymplectic ElementsPublisher JACoW Publishing2023Kempf, IAbbott, MBobb, LChristian, GBRehm, GDuncan, SThe electron beam stability is critical for 4th generation light sources. As opposed to 10 % of beam size up to 140 Hz at Diamond, advances in detector speed and resolution at Diamond-II increase the stability requirements to 3 % up to 1 kHz. This paper presents a novel control methodology for the fast orbit feedback at Diamond-II, which will stabilise the beam using two arrays of 252 slow and 144 fast correctors and 252 beam position monitors at 100 kHz. In contrast to existing approaches that separate slow and fast feedback loops, our approach is based on a two-matrix factorisation called the generalised singular value decomposition (GSVD), which decouples the system into 144 two-input modes controlled by slow and fast magnets and 108 modes controlled by slow magnets only. The GSVD-based controller is implemented in the existing Diamond storage ring using a centralised communication architecture, such as planned for Diamond-II. We present results from the Diamond storage ring and simulation, which confirm that the proposed approach meets the target specification for Diamond-II. |
spellingShingle | Kempf, I Abbott, M Bobb, L Christian, GB Rehm, G Duncan, S Fast orbit feedback for Diamond-II |
title | Fast orbit feedback for Diamond-II |
title_full | Fast orbit feedback for Diamond-II |
title_fullStr | Fast orbit feedback for Diamond-II |
title_full_unstemmed | Fast orbit feedback for Diamond-II |
title_short | Fast orbit feedback for Diamond-II |
title_sort | fast orbit feedback for diamond ii |
work_keys_str_mv | AT kempfi fastorbitfeedbackfordiamondii AT abbottm fastorbitfeedbackfordiamondii AT bobbl fastorbitfeedbackfordiamondii AT christiangb fastorbitfeedbackfordiamondii AT rehmg fastorbitfeedbackfordiamondii AT duncans fastorbitfeedbackfordiamondii |