Calibration of Aerogel Tiles for the RICH of the HELIX Experiment

Video Player is loading.
Loaded: 0%
Remaining Time 0:00
1x
  • Quality
    • 85 views

    • 0 favorites

    • uploaded July 7, 2021

    Discussion timeslot (ZOOM-Meeting): 16. July 2021 - 18:00
    ZOOM-Meeting URL: https://icrc2021.desy.de/pf_access_abstracts
    Corresponding Session: https://icrc2021-venue.desy.de/channel/Presenter-Forum-1-Evening-All-Categories/48
    Abstract:
    'HELIX (High Energy Light Isotope eXperiment) is a balloon-borne instrument designed to measure the chemical and isotopic abundances of light cosmic-ray nuclei. In particular, HELIX is optimized to measure 10Be and 9Be in the range 0.2 GeV/n to beyond 3 GeV/n. To achieve this, HELIX utilizes a 1 Tesla superconducting magnet with a high-resolution gas drift tracking system, time-of-flight detector, and a ring-imaging Cherenkov (RICH) detector. The RICH detector consists of aerogel tile radiators (refractive index ~1.15) with a silicon photomultiplier detector plane. To adequately discriminate between 10Be and 9Be isotopes, the refractive index of the aerogel tiles must be known to a precision of 0.1%. In this contribution, detailed mapping of the refractive index across the aerogel tiles is presented and the methodology used to obtain these measurements is discussed.'

    Authors: stephan o'brien
    Collaboration: HELIX

    Indico-ID: 1372
    Proceeding URL: https://pos.sissa.it/395/090

    Tags:
    Presenter:

    stephan o'brien


    Additional files

    More Media in "Cosmic Ray Direct"