Nonlinear dynamics in a SPEAR wiggler

BL11, the most recently installed wiggler in the SPEAR storage ring at the Stanford Synchrotron Radiation Laboratory, produces a large nonlinear perturbation of the electron beam dynamics, which was not directly evident in the integrated magnetic field measurements. Measurements of tune shifts with...

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Main Authors: J. Safranek, C. Limborg, A. Terebilo, K. I. Blomqvist, P. Elleaume, Y. Nosochkov
Format: Article
Language:English
Published: American Physical Society 2002-01-01
Series:Physical Review Special Topics. Accelerators and Beams
Online Access:http://doi.org/10.1103/PhysRevSTAB.5.010701
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spelling doaj-c0207b664b1e4915be6b0deb88ae18642020-11-25T01:13:59ZengAmerican Physical SocietyPhysical Review Special Topics. Accelerators and Beams1098-44022002-01-015101070110.1103/PhysRevSTAB.5.010701Nonlinear dynamics in a SPEAR wigglerJ. SafranekC. LimborgA. TerebiloK. I. BlomqvistP. ElleaumeY. NosochkovBL11, the most recently installed wiggler in the SPEAR storage ring at the Stanford Synchrotron Radiation Laboratory, produces a large nonlinear perturbation of the electron beam dynamics, which was not directly evident in the integrated magnetic field measurements. Measurements of tune shifts with betatron oscillation amplitude and closed orbit shifts were used to characterize the nonlinear fields. Because of the narrow pole width in BL11, the nonlinear fields seen along the wiggling electron trajectory are dramatically different from the magnetic measurements made along a straight line with a stretched wire. This difference explains the tune shift measurements and the observed degradation in dynamic aperture. Because of the relatively large dispersion (1.2 m) at BL11, the nonlinearities particularly reduced the off-energy dynamic aperture. Because of the nature of these nonlinear fields, it is impossible, even theoretically, to cancel them completely with short multipole correctors. Magic finger corrector magnets were built, however, that partially correct the nonlinear perturbation, greatly improving the storage ring performance.http://doi.org/10.1103/PhysRevSTAB.5.010701
collection DOAJ
language English
format Article
sources DOAJ
author J. Safranek
C. Limborg
A. Terebilo
K. I. Blomqvist
P. Elleaume
Y. Nosochkov
spellingShingle J. Safranek
C. Limborg
A. Terebilo
K. I. Blomqvist
P. Elleaume
Y. Nosochkov
Nonlinear dynamics in a SPEAR wiggler
Physical Review Special Topics. Accelerators and Beams
author_facet J. Safranek
C. Limborg
A. Terebilo
K. I. Blomqvist
P. Elleaume
Y. Nosochkov
author_sort J. Safranek
title Nonlinear dynamics in a SPEAR wiggler
title_short Nonlinear dynamics in a SPEAR wiggler
title_full Nonlinear dynamics in a SPEAR wiggler
title_fullStr Nonlinear dynamics in a SPEAR wiggler
title_full_unstemmed Nonlinear dynamics in a SPEAR wiggler
title_sort nonlinear dynamics in a spear wiggler
publisher American Physical Society
series Physical Review Special Topics. Accelerators and Beams
issn 1098-4402
publishDate 2002-01-01
description BL11, the most recently installed wiggler in the SPEAR storage ring at the Stanford Synchrotron Radiation Laboratory, produces a large nonlinear perturbation of the electron beam dynamics, which was not directly evident in the integrated magnetic field measurements. Measurements of tune shifts with betatron oscillation amplitude and closed orbit shifts were used to characterize the nonlinear fields. Because of the narrow pole width in BL11, the nonlinear fields seen along the wiggling electron trajectory are dramatically different from the magnetic measurements made along a straight line with a stretched wire. This difference explains the tune shift measurements and the observed degradation in dynamic aperture. Because of the relatively large dispersion (1.2 m) at BL11, the nonlinearities particularly reduced the off-energy dynamic aperture. Because of the nature of these nonlinear fields, it is impossible, even theoretically, to cancel them completely with short multipole correctors. Magic finger corrector magnets were built, however, that partially correct the nonlinear perturbation, greatly improving the storage ring performance.
url http://doi.org/10.1103/PhysRevSTAB.5.010701
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