Electron-beam calibration of aerogel tiles for the HELIX RICH detector

P. Allison, M. Baiocchi, J. J. Beatty, L. Beaufore, D. H. Calderone, Y. Chen, S. Coutu, E. Ellingwood, N. Green, D. Hanna, H. B. Jeon, R. Mbarek, K. McBride, I. Mognet, J. Musser, S. Nutter, S. O'Brien, N. Park, T. Rosin, M. TabataG. Tarlé, G. Visser, S. P. Wakely, M. Yu

Research output: Contribution to journalArticlepeer-review

3 Scopus citations

Abstract

The HELIX cosmic-ray detector is a balloon-borne instrument designed to measure the flux of light isotopes in the energy range from 0.2 GeV/n to beyond 3 GeV/n. It will rely on a ring-imaging Cherenkov (RICH) detector for particle identification at energies greater than 1 GeV/n and will use aerogel tiles with refractive index near 1.15 as the radiator. To achieve the performance goals of the experiment it is necessary to know the refractive index and its position dependence over the lateral extent of the tiles to a precision of O(10−4). In this paper we describe the apparatus and methods developed to calibrate the HELIX tiles in an electron beam, in order to meet this requirement.

All Science Journal Classification (ASJC) codes

  • Nuclear and High Energy Physics
  • Instrumentation

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