Paper |
Title |
Page |
MOOTH2 |
Commissioning of SuperKEKB |
4 |
|
- Y. Funakoshi
KEK, Ibaraki, Japan
|
|
|
After 5 years of upgrade work from KEKB, the Phase 1 beam commissioning of SuperKEKB started on Feb. 1st this year and finished at the end of June. In Phase 1, Belle-II detector and the final focus doublet (QCS) were not installed and no beam collision was performed. Missions of the commissioning in Phase 1 were startup of each hardware component, establishment of beam operation software tools, preparation of Belle-II detector, an optics study and tuning without QCS and the detector solenoid magnet and other machine studies. In this talk, achievements in the Phase 1 commissioning are summarized. Also a plan for the Phase 2 commissioning will be given.
|
|
DOI • |
reference for this paper
※ https://doi.org/10.18429/JACoW-eeFACT2016-MOOTH2
|
|
Export • |
reference for this paper using
※ BibTeX,
※ LaTeX,
※ Text/Word,
※ RIS,
※ EndNote (xml)
|
|
|
TUT3BH2 |
Optics Correction and Low Emittance Tuning at the Phase 1 commissioning of SuperKEKB |
143 |
|
- Y. Ohnishi, Y. Funakoshi, H. Koiso, A. Morita, K. Oide, H. Sugimoto
KEK, Ibaraki, Japan
|
|
|
The SuperKEKB collider has finally come to the first commissioning, Phase 1 without the final focus system and before Belle II detector roll-in. In order to accomplish a extremely high luminosity of 8x1035 cm-2s-1, the nano-beam scheme is adopted. Since the vertical emittance is one of keys in this scheme, optics corrections for low emittance tuning are applied. The non-interleaved sextupole scheme is utilized in the arc section. Skew quadrupole-like corrector is equipped for each sextupole. These skew quadrupole-like correctors can correct both X-Y coupling and physical vertical dispersions which induce the vertical emittance. Beta function and physical horizontal dispersion are corrected by fudge factors of quadrupoles and/or horizontal orbit bumps at the sextupoles. Overall optics performance as well as the strategy of low emittance tuning is also presented.
|
|
DOI • |
reference for this paper
※ https://doi.org/10.18429/JACoW-eeFACT2016-TUT3BH2
|
|
Export • |
reference for this paper using
※ BibTeX,
※ LaTeX,
※ Text/Word,
※ RIS,
※ EndNote (xml)
|
|
|
TUT3BH3 |
Luminosity Tuning at KEKB |
147 |
|
- Y. Funakoshi
KEK, Ibaraki, Japan
|
|
|
KEKB achieved the world's highest luminosity. One of the key issues for the high luminosity at KEKB was a luminosity tuning which was done almost every time even during the physics run to suppress the beam-beam blowup. In this talk, those experiences are summarized. Some experiences of the luminosity tuning at TRISTAN will also mentioned.
|
|
DOI • |
reference for this paper
※ https://doi.org/10.18429/JACoW-eeFACT2016-TUT3BH3
|
|
Export • |
reference for this paper using
※ BibTeX,
※ LaTeX,
※ Text/Word,
※ RIS,
※ EndNote (xml)
|
|
|
THS1H4 |
Summary of IR and MDI Session |
200 |
|
- Y. Funakoshi
KEK, Ibaraki, Japan
|
|
|
A brief summary of talks in IR and MDI session is given. Also features and issues on the IR design in the future colliders are summarized.
|
|
DOI • |
reference for this paper
※ https://doi.org/10.18429/JACoW-eeFACT2016-THS1H4
|
|
Export • |
reference for this paper using
※ BibTeX,
※ LaTeX,
※ Text/Word,
※ RIS,
※ EndNote (xml)
|
|
|