<xml>
  <records>
    <record>
       <contributors>
          <authors>
             <author>Ohnishi, Y.</author>
             <author>Funakoshi, Y.</author>
             <author>Koiso, H.</author>
             <author>Morita, A.</author>
             <author>Oide, K.</author>
             <author>Sugimoto, H.</author>
          </authors>
       </contributors>
       <titles>
          <title>
             Optics Correction and Low Emittance Tuning at the Phase 1 commissioning of SuperKEKB
          </title>
       </titles>
		 <publisher>JACoW</publisher>
       <pub-location>Geneva, Switzerland</pub-location>
		 <isbn>978-3-95450-187-8</isbn>
		 <electronic-resource-num>10.18429/JACoW-eeFACT2016-TUT3BH2</electronic-resource-num>
		 <language>English</language>
		 <pages>143-146</pages>
       <pages>TUT3BH2</pages>
       <keywords>
          <keyword>ion</keyword>
          <keyword>sextupole</keyword>
          <keyword>emittance</keyword>
          <keyword>optics</keyword>
          <keyword>coupling</keyword>
       </keywords>
       <work-type>Contribution to a conference proceedings</work-type>
       <dates>
          <year>2017</year>
          <pub-dates>
             <date>2017-07</date>
          </pub-dates>
       </dates>
       <urls>
          <related-urls>
              <url>https://doi.org/10.18429/JACoW-eeFACT2016-TUT3BH2</url>
              <url>http://jacow.org/eefact2016/papers/tut3bh2.pdf</url>
          </related-urls>
       </urls>
       <abstract>
          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.
       </abstract>
    </record>
  </records>
</xml>
