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@inproceedings{sajaev:ipac2021-thpab067,
author = {V. Sajaev},
title = {{Simulation of the APS-U Orbit Motion Due to RF Noise}},
booktitle = {Proc. IPAC'21},
pages = {3911--3914},
eid = {THPAB067},
language = {english},
keywords = {simulation, synchrotron, resonance, cavity, photon},
venue = {Campinas, SP, Brazil},
series = {International Particle Accelerator Conference},
number = {12},
publisher = {JACoW Publishing, Geneva, Switzerland},
month = {08},
year = {2021},
issn = {2673-5490},
isbn = {978-3-95450-214-1},
doi = {10.18429/JACoW-IPAC2021-THPAB067},
url = {https://jacow.org/ipac2021/papers/thpab067.pdf},
note = {https://doi.org/10.18429/JACoW-IPAC2021-THPAB067},
abstract = {{APS Upgrade storage ring will keep the same rf system that is presently used at APS. This rf system has amplitude and phase noise dominated by the lines at 60, 180, and 360 Hz. APS presently operates with synchrotron frequency close to 2 kHz, which is far away from the rf noise frequencies, and still the rf system noise contributes over 2 micrometers rms into the horizontal orbit noise due to beam energy variation. APS-U will operate with a bunch-lengthening cavity, which will lower the synchrotron frequency down to about 200 Hz. This could potentially lead to large orbit noise and other negative consequences due to energy variation caused by the rf system noise. In this paper, we will present simulations of the rf noise-induced orbit motion at APS and APS-U and define the rf amplitude and phase noise requirements that need to be achieved for APS-U operation.}},
}