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@inproceedings{yu:ipac2021-mopab039,
author = {L.H. Yu and G. Bassi and Y. Hidaka and B. Podobedov and V.V. Smaluk and G.M. Wang and X. Yang},
% author = {L.H. Yu and G. Bassi and Y. Hidaka and B. Podobedov and V.V. Smaluk and G.M. Wang and others},
% author = {L.H. Yu and others},
title = {{Amplitude-Dependent Shift of Betatron Tunes and Its Relation to Long-Term Circumference Variations at NSLS-II}},
booktitle = {Proc. IPAC'21},
pages = {175--177},
eid = {MOPAB039},
language = {english},
keywords = {lattice, sextupole, simulation, closed-orbit, wiggler},
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-MOPAB039},
url = {https://jacow.org/ipac2021/papers/mopab039.pdf},
note = {https://doi.org/10.18429/JACoW-IPAC2021-MOPAB039},
abstract = {{The comparison of amplitude tune dependence measured for NSLSII lattices with models indicated the large change of amplitude tune dependence over time apparently can not be solely explained by magnets variation or beta function changes, but it seems can be explained by energy changes. On the other hand, the energy change required by fitting with the amplitude tune dependence change is too large to be explained by the RF frequency change and the change of the sum of correctors in the period of the measurements. To explain this apparent contradiction, our analysis shows the long term storage ring circumference change can explain the apparent energy change. Our data indeed shows a seasonal change of the amplitude tune dependence over long term observation. This clearly also indicated a relation to long term closed orbit drift. Hence the current work indicates a new strategy to study how to use amplitude tune dependence as a guideline to analyze long term lattice parameter shifts and closed orbit drift, and improve the orbit and machine performance stability.}},
}