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April 4, 2026JACOW0 citationsOpen Access

Design of a damping wiggler at SPring-8-II as a high-energy X-ray source

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KTKoji TsubotaHOHaruhiko OhashiSSSatsuki Shimizu

Key Points

  • The research aims to design a damping wiggler for SPring-8-II to reduce emittance and increase photon flux above 100 keV.
  • Designed a damping wiggler for installation in a 30 m straight section of synchrotron
  • Optimized parameters such as unit number, period length, gap, and total length
  • Evaluated the power density at the mask to manage heat load
  • Achieved low emittance with the optimized damping wiggler design
  • Enhanced photon flux suitable for high-energy X-ray applications
  • Managed radiation loads of up to 75 kW with effective mask aperture design

Abstract

SPring-8 will be upgraded to SPring-8-II, a fourth-generation synchrotron with a multi-bend achromat lattice, by 2028. The beam energy will be reduced from 8 to 6 GeV, substantially lowering emittance. To further reduce the emittance, a damping wiggler is planned for installation in a 30 m straight section. High-energy X-ray above 100 keV are in demand for industrial use, but lowering the beam energy reduces photon flux in this range. A damping wiggler can enhance this flux. We therefore designed the wiggler not only for emittance reduction but also as a high-energy X-ray source. The wiggler will be installed in a straight section with five drift spaces, each about 4 m long, to accommodate the wiggler, masks and related components. Its parameters—unit number, period length, gap and total length—were optimized to achieve low emittance, high photon flux and reduced heat load on absorbers. To handle radiation up to 75 kW and 800 W/mm² over a wide solid angle, the mask aperture was designed to limit angular spread and reduce the heat load on the absorber at the downstream bending magnet chamber. This study presents the optimized wiggler design and power density evaluation at the mask.

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Cite This Study

Tsubota et al. (2026) studied this question.

synapsesocial.com/papers/69d0af9a659487ece0fa59aehttps://doi.org/10.18429/jacow-medsi2025-wep17
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