First measurements of the longitudinal bunch profile of a 28.5 GeV beam using coherent Smith-Purcell radiation

Coherent Smith-Purcell (SP) radiation originating from three different gratings has been measured at End Station A, SLAC, and has been used to reconstruct the time profile of the electron bunches. The beam energy during these experiments was 28.5 GeV (γ≅55 773) and the number of electrons in the bun...

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Main Authors: V. Blackmore, G. Doucas, C. Perry, B. Ottewell, M. F. Kimmitt, M. Woods, S. Molloy, R. Arnold
Format: Article
Language:English
Published: American Physical Society 2009-03-01
Series:Physical Review Special Topics. Accelerators and Beams
Online Access:http://doi.org/10.1103/PhysRevSTAB.12.032803
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spelling doaj-91265dc2243c43d6baa5697360e659382020-11-25T01:33:16ZengAmerican Physical SocietyPhysical Review Special Topics. Accelerators and Beams1098-44022009-03-0112303280310.1103/PhysRevSTAB.12.032803First measurements of the longitudinal bunch profile of a 28.5 GeV beam using coherent Smith-Purcell radiationV. BlackmoreG. DoucasC. PerryB. OttewellM. F. KimmittM. WoodsS. MolloyR. ArnoldCoherent Smith-Purcell (SP) radiation originating from three different gratings has been measured at End Station A, SLAC, and has been used to reconstruct the time profile of the electron bunches. The beam energy during these experiments was 28.5 GeV (γ≅55 773) and the number of electrons in the bunch was 0.9–1.4×10^{10}. The spectral distribution of the radiated energy was measured by means of an array of 11 pyroelectric detectors. Typical values of the FWHM of the bunch length are about 2.5 ps, but sharper peaks with FWHM less than 2.0 ps have also been observed. The longitudinal profile also varies with accelerator conditions and can best be approximated by a superposition of 3–4 Gaussian curves. Some typical profiles are presented, together with a discussion of the limitations and strengths of coherent SP radiation as a diagnostic tool. It is concluded that SP radiation offers excellent prospects in this respect, not only in the picosecond range, but potentially in the femtosecond range as well.http://doi.org/10.1103/PhysRevSTAB.12.032803
collection DOAJ
language English
format Article
sources DOAJ
author V. Blackmore
G. Doucas
C. Perry
B. Ottewell
M. F. Kimmitt
M. Woods
S. Molloy
R. Arnold
spellingShingle V. Blackmore
G. Doucas
C. Perry
B. Ottewell
M. F. Kimmitt
M. Woods
S. Molloy
R. Arnold
First measurements of the longitudinal bunch profile of a 28.5 GeV beam using coherent Smith-Purcell radiation
Physical Review Special Topics. Accelerators and Beams
author_facet V. Blackmore
G. Doucas
C. Perry
B. Ottewell
M. F. Kimmitt
M. Woods
S. Molloy
R. Arnold
author_sort V. Blackmore
title First measurements of the longitudinal bunch profile of a 28.5 GeV beam using coherent Smith-Purcell radiation
title_short First measurements of the longitudinal bunch profile of a 28.5 GeV beam using coherent Smith-Purcell radiation
title_full First measurements of the longitudinal bunch profile of a 28.5 GeV beam using coherent Smith-Purcell radiation
title_fullStr First measurements of the longitudinal bunch profile of a 28.5 GeV beam using coherent Smith-Purcell radiation
title_full_unstemmed First measurements of the longitudinal bunch profile of a 28.5 GeV beam using coherent Smith-Purcell radiation
title_sort first measurements of the longitudinal bunch profile of a 28.5 gev beam using coherent smith-purcell radiation
publisher American Physical Society
series Physical Review Special Topics. Accelerators and Beams
issn 1098-4402
publishDate 2009-03-01
description Coherent Smith-Purcell (SP) radiation originating from three different gratings has been measured at End Station A, SLAC, and has been used to reconstruct the time profile of the electron bunches. The beam energy during these experiments was 28.5 GeV (γ≅55 773) and the number of electrons in the bunch was 0.9–1.4×10^{10}. The spectral distribution of the radiated energy was measured by means of an array of 11 pyroelectric detectors. Typical values of the FWHM of the bunch length are about 2.5 ps, but sharper peaks with FWHM less than 2.0 ps have also been observed. The longitudinal profile also varies with accelerator conditions and can best be approximated by a superposition of 3–4 Gaussian curves. Some typical profiles are presented, together with a discussion of the limitations and strengths of coherent SP radiation as a diagnostic tool. It is concluded that SP radiation offers excellent prospects in this respect, not only in the picosecond range, but potentially in the femtosecond range as well.
url http://doi.org/10.1103/PhysRevSTAB.12.032803
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