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Manufacture Details of a SWGO Double-Layer Tank Design - Water Cherenkov Detector Prototype

  • SWGO Collaboration
    ,
  • José Bellido(Author)
    ,
  • Michael Schneider(Author)
    ,
  • P. Abreu(Author)
    ,
  • A. Albert(Author)
    ,
  • R. Alfaro(Author)
  • Adelaide University
    ,
  • University of Maryland, College Park
    ,
  • University of Lisbon
    ,
  • Laboratório de Instrumentação e Física Experimental de Partículas
    ,
  • Los Alamos National Laboratory
    ,
  • Universidad Nacional Autónoma de México
Research Output:
Contribution to journal
Conference article
Peer-review

Publication metrics

Metrics

SciVal
Citations
1
Scopus
Citations
SciVal
FWCI
1.64
SciVal
Author count
259
SciVal
Paper percentile
83

Abstract

Water-Cherenkov detectors (WCD) have been manufactured in Australia by the company AQUAMATE as part of the RD activities for SWGO. They consist of a steel tank frame with a bladder on its interior satisfying the SWGO double-layer tank design. Tanks and bladders have been custom designed to optimally accommodate the bladder inside the tank and with minimal material usage. They are delivered in compact boxes that are easy to transport. These boxes are designed to fit 24 tanks in a 20-foot container. The double-layer tank design has introduced new features to improve the discrimination between gamma-rays and cosmic rays. Some of these features created challenges for the manufacturing. Some units have been delivered to one of Peru’s candidate sites at 4800 m and to Mexico (the HAWC Observatory, 4100 m) for prototype tests in real conditions. In this contribution we will describe manufacturing and construction details of the first SWGO prototype WCD. These details were envisaged to facilitate: the transport of the units, the assembly, the deployment and maintenance activities of the detectors. Furthermore, the units need to be resistant to strong winds, rain, snow and earthquakes.The costs are scalable with the detector volume. This information could be of interest to other Observatories that are in RD phase, such as the Global Cosmic Ray Observatory (GCOS) for the study of the highest-energy particles in the Universe and the Tau Air Shower Mountain-Based Observatory (TAMBO) for the search of PeV neutrinos.

Publication Information

Output type

Research Output:
Contribution to journal
Conference article
Peer-review

Original language

English

Article number

803

Journal (Volume, Issue Number)

Proceedings of Science (Volume 444)

Publication milestones

  • Published - 27/09/2024

Publication status

Published - 27/09/2024

Publication IDs

  • Scopus: 85212269570

Related Event

Title

38th International Cosmic Ray Conference, ICRC 2023

Event type

Conference

Date

26/07/2023 - 03/08/2023

Location

NagoyaJapan