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| 001 | 405413 | ||
| 005 | 20211110150957.0 | ||
| 024 | 7 | _ | |a 10.3204/PUBDB-2018-02151 |2 datacite_doi |
| 037 | _ | _ | |a PUBDB-2018-02151 |
| 041 | _ | _ | |a English |
| 100 | 1 | _ | |a Chae, Yong-Chul |0 P:(DE-H253)PIP1080789 |b 0 |e Corresponding author |
| 111 | 2 | _ | |a 9th International Particle Accelerator Conference |g IPAC'18 |c Vancouver |d 2018-04-29 - 2018-05-04 |w Canada |
| 245 | _ | _ | |a Microwave instability and energy spread measurement via vertical dispersion bump in PETRA III |
| 260 | _ | _ | |c 2018 |
| 300 | _ | _ | |a 3 |
| 336 | 7 | _ | |a CONFERENCE_PAPER |2 ORCID |
| 336 | 7 | _ | |a Conference Paper |0 33 |2 EndNote |
| 336 | 7 | _ | |a INPROCEEDINGS |2 BibTeX |
| 336 | 7 | _ | |a conferenceObject |2 DRIVER |
| 336 | 7 | _ | |a Output Types/Conference Paper |2 DataCite |
| 336 | 7 | _ | |a Contribution to a conference proceedings |b contrib |m contrib |0 PUB:(DE-HGF)8 |s 1527752104_25939 |2 PUB:(DE-HGF) |
| 520 | _ | _ | |a The recent measurement of bunch length versus current indicated that the longitudinal impedance (Z/n) is 0.15 Ohm in close agreement with the impedance model [1]. Naïve application of Keil-Schnell criteria predicts that the threshold of microwave instability at 0.25 mA. Since the single bunch intensity is in the range of 0.2 – 2.5 mA depending on the fill pattern of PETRA III, we expect to observe the fill-pattern dependent energy spread according to the theory. However, the 3rd generation light sources comparable to PETRA III often reported the observation which was much greater than the theoretical one. In order to induce the beam size variation we had used skew quadrupoles to generate the dispersion in vertical plane. In particular we made dispersion bump at the undulator sector so that we were able to use the x-ray optics for the precise determination of small vertical beam size. In this paper we report the experimental setup and measurement data with the estimate on the instability threshold. We also report the vertical emittance and energy spread based on the x-ray beam size measurement as well as the rf signal which was excited by the beam at the longitudinal feedback cavity. |
| 536 | _ | _ | |a 631 - Accelerator R & D (POF3-631) |0 G:(DE-HGF)POF3-631 |c POF3-631 |f POF III |x 0 |
| 536 | _ | _ | |a 6G3 - PETRA III (POF3-622) |0 G:(DE-HGF)POF3-6G3 |c POF3-622 |f POF III |x 1 |
| 693 | _ | _ | |a PETRA III |e Facility (machine) PETRA III |1 EXP:(DE-H253)PETRAIII-20150101 |0 EXP:(DE-H253)PETRAIII(machine)-20150101 |5 EXP:(DE-H253)PETRAIII(machine)-20150101 |x 0 |
| 700 | 1 | _ | |a Keil, Joachim |0 P:(DE-H253)PIP1002277 |b 1 |
| 700 | 1 | _ | |a Sahoo, Gajendra Kumar |0 P:(DE-H253)PIP1003493 |b 2 |
| 700 | 1 | _ | |a Wanzenberg, Rainer |0 P:(DE-H253)PIP1001362 |b 3 |
| 700 | 1 | _ | |a Ebert, Michael |0 P:(DE-H253)PIP1003177 |b 4 |
| 700 | 1 | _ | |a Novokshonov, Artem |0 P:(DE-H253)PIP1024225 |b 5 |
| 700 | 1 | _ | |a Kube, Gero |0 P:(DE-H253)PIP1002168 |b 6 |
| 700 | 1 | _ | |a Falkenberg, Gerald |0 P:(DE-H253)PIP1002716 |b 7 |
| 700 | 1 | _ | |a Sprung, Michael |0 P:(DE-H253)PIP1007141 |b 8 |
| 700 | 1 | _ | |a Dzhigaev, Dmitry |0 P:(DE-H253)PIP1014827 |b 9 |
| 700 | 1 | _ | |a Westermeier, Fabian |0 P:(DE-H253)PIP1006002 |b 10 |
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| 913 | 1 | _ | |a DE-HGF |b Forschungsbereich Materie |l Materie und Technologie |1 G:(DE-HGF)POF3-630 |0 G:(DE-HGF)POF3-631 |2 G:(DE-HGF)POF3-600 |v Accelerator R & D |x 0 |4 G:(DE-HGF)POF |3 G:(DE-HGF)POF3 |
| 913 | 1 | _ | |a DE-HGF |b Forschungsbereich Materie |l Von Materie zu Materialien und Leben |1 G:(DE-HGF)POF3-620 |0 G:(DE-HGF)POF3-622 |2 G:(DE-HGF)POF3-600 |v Facility topic: Research on Matter with Brilliant Light Sources |9 G:(DE-HGF)POF3-6G3 |x 1 |4 G:(DE-HGF)POF |3 G:(DE-HGF)POF3 |
| 914 | 1 | _ | |y 2018 |
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| 920 | 1 | _ | |0 I:(DE-H253)MPY-20120731 |k MPY |l Beschleunigerphysik |x 0 |
| 920 | 1 | _ | |0 I:(DE-H253)FS-PE-20120731 |k FS-PE |l Experimentebetreuung PETRA III |x 1 |
| 920 | 1 | _ | |0 I:(DE-H253)MPE-20120731 |k MPE |l PETRA |x 2 |
| 980 | _ | _ | |a contrib |
| 980 | _ | _ | |a VDB |
| 980 | _ | _ | |a UNRESTRICTED |
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