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X-Band LLRF Developments for High Power CLIC Test Stands and Waveguide Interferometry for Phase Stabilisation
This thesis describes the upgrade of the first high power X-band RF test for high gradient accelerating structures at CERN, as required for the e+ e- collider research program; Compact Linear Collider, CLIC. Significant improvements to the control system and operation of the first test stand, Xbox-1, a...
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Lenguaje: | eng |
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2022
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Acceso en línea: | http://cds.cern.ch/record/2843363 |
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author | Edwards, Amelia Veronica |
author_facet | Edwards, Amelia Veronica |
author_sort | Edwards, Amelia Veronica |
collection | CERN |
description | This thesis describes the upgrade of the first high power X-band RF test for high gradient accelerating structures at CERN, as required for the e+ e- collider research program; Compact Linear Collider, CLIC. Significant improvements to the control system and operation of the first test stand, Xbox-1, are implemented. The design and commissioning of the new Low Level Radio Frequency, LLRF, system is described in detail. The upgrade also en- compasses software, interlock systems, timing, safety and control. The new LLRF requires an up-convertor to convert an input signal at 187.4 MHz to 11.806 GHz. The most common method is a phase locked loop, PLL, an alternative method was envi- sioned which uses single side-band up-convertor. This necessitated the design and manufacture of a custom cavity filter. The up-convertor and PLL are compared and both are implemented in the new LLRF. The new LLRF system is implemented at Xbox1 and used to RF condition a 50 MW CPI klystron, the final output power was 45 MW for a 50 ns RF pulse length. The phase and amplitude of the LLRF, TWT and klystron are characterised with both the PLL and up-convertor. The klystron phase stability was studied using a sensitivity analysis. The waveguide network between the klystron and the accelerating structures is approximately 30 m. This network is subject to environmental phase changes which affect the phase stability of the RF arriving at the structures. A single path inteferom- eter was designed which will allow a phase measurement pulse at a secondary fre- quency to be injected into the waveguide network interleaved with klystron pulses. The interferometer is commissioned in the lab and low power measurements val- idate its operation. The system is then integrated into the high power network at Xbox1 and used to measure phase shifts in the waveguide network which are corre- lated with temperature. |
id | cern-2843363 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2022 |
record_format | invenio |
spelling | cern-28433632022-12-13T19:39:14Zhttp://cds.cern.ch/record/2843363engEdwards, Amelia VeronicaX-Band LLRF Developments for High Power CLIC Test Stands and Waveguide Interferometry for Phase StabilisationEngineeringAccelerators and Storage RingsThis thesis describes the upgrade of the first high power X-band RF test for high gradient accelerating structures at CERN, as required for the e+ e- collider research program; Compact Linear Collider, CLIC. Significant improvements to the control system and operation of the first test stand, Xbox-1, are implemented. The design and commissioning of the new Low Level Radio Frequency, LLRF, system is described in detail. The upgrade also en- compasses software, interlock systems, timing, safety and control. The new LLRF requires an up-convertor to convert an input signal at 187.4 MHz to 11.806 GHz. The most common method is a phase locked loop, PLL, an alternative method was envi- sioned which uses single side-band up-convertor. This necessitated the design and manufacture of a custom cavity filter. The up-convertor and PLL are compared and both are implemented in the new LLRF. The new LLRF system is implemented at Xbox1 and used to RF condition a 50 MW CPI klystron, the final output power was 45 MW for a 50 ns RF pulse length. The phase and amplitude of the LLRF, TWT and klystron are characterised with both the PLL and up-convertor. The klystron phase stability was studied using a sensitivity analysis. The waveguide network between the klystron and the accelerating structures is approximately 30 m. This network is subject to environmental phase changes which affect the phase stability of the RF arriving at the structures. A single path inteferom- eter was designed which will allow a phase measurement pulse at a secondary fre- quency to be injected into the waveguide network interleaved with klystron pulses. The interferometer is commissioned in the lab and low power measurements val- idate its operation. The system is then integrated into the high power network at Xbox1 and used to measure phase shifts in the waveguide network which are corre- lated with temperature.CERN-THESIS-2022-245oai:cds.cern.ch:28433632022-12-08T09:40:16Z |
spellingShingle | Engineering Accelerators and Storage Rings Edwards, Amelia Veronica X-Band LLRF Developments for High Power CLIC Test Stands and Waveguide Interferometry for Phase Stabilisation |
title | X-Band LLRF Developments for High Power CLIC Test Stands and Waveguide Interferometry for Phase Stabilisation |
title_full | X-Band LLRF Developments for High Power CLIC Test Stands and Waveguide Interferometry for Phase Stabilisation |
title_fullStr | X-Band LLRF Developments for High Power CLIC Test Stands and Waveguide Interferometry for Phase Stabilisation |
title_full_unstemmed | X-Band LLRF Developments for High Power CLIC Test Stands and Waveguide Interferometry for Phase Stabilisation |
title_short | X-Band LLRF Developments for High Power CLIC Test Stands and Waveguide Interferometry for Phase Stabilisation |
title_sort | x-band llrf developments for high power clic test stands and waveguide interferometry for phase stabilisation |
topic | Engineering Accelerators and Storage Rings |
url | http://cds.cern.ch/record/2843363 |
work_keys_str_mv | AT edwardsameliaveronica xbandllrfdevelopmentsforhighpowerclicteststandsandwaveguideinterferometryforphasestabilisation |