7–11 Oct 2024
SLAC
America/Los_Angeles timezone

Session

Tools & Monitoring I

10 Oct 2024, 08:35
51/1-102 - Kavli Auditorium (SLAC)

51/1-102 - Kavli Auditorium

SLAC

150

Conveners

Tools & Monitoring I

  • Mika Masuzawa (KEK)

Presentation materials

There are no materials yet.

  1. Witold Niewiem (CERN)
    10/10/2024, 08:35

    The Structured Laser Beam (SLB) is a pseudo-non-diffractive optical beam characterized by the low divergence of the Inner Core (IC), down to 10 μrad, and the presence of concentric rings, with the most prominent being the Outer Ring (OR). The size of the IC and OR can vary depending on the SLB generator setup. SLBs have the potential to serve as straight reference lines for long-distance...

    Go to contribution page
  2. Jean-Christophe Gayde (CERN)
    10/10/2024, 09:00

    As part of the study on using structured laser light for alignment, an innovative technique is proposed for generating symmetrical pseudo-non-diffracting layers of caustic optical beams, known as Layer Beams (LB). The state of the art for producing similar beams consists of using spatial light modulators. Our approach is based on the design of a generator with a specific arrangement of...

    Go to contribution page
  3. Zhenqiang He (Institute of High Energy Physics, Chinese Academy of Sciences (IHEP CAS))
    10/10/2024, 09:25

    Alignment of superconducting cavities is a critical concern for the China Spallation Neutron Source Phase II (CSNS II) linac. To measure cavity displacement during the cooling process to liquid helium temperature, a new laser-based Poisson Spot Monitor (PSM) system was introduced. This system utilizes the diffraction spot captured on a CMOS camera when a parallel laser beam passes through a...

    Go to contribution page
  4. Hélène Mainaud Durand (CERN)
    10/10/2024, 09:50

    The High-Luminosity Large Hadron Collider (HL-LHC) project at CERN aims to enhance the LHC's performance and expand its potential for discoveries beyond 2029. New components will be installed within the 220 meters before the collision points of the ATLAS and CMS experiments, including 16 NB3Sn quadrupoles to focus the beam before collision and 8 radio frequency crab cavities to allow beam...

    Go to contribution page
Building timetable...