A mechanical design for a detection unit for a deep-sea neutrino telescope

Authors
  • E.M. Berbee
  • H. Boer Rookhuizen
  • E. Heine
  • E. de Wolf
Publication date 2013
Journal Nuclear Instruments & Methods in Physics Research Section A - Accelerators Spectrometers Detectors and Associated Equipment
Volume | Issue number 725
Pages (from-to) 237-240
Organisations
  • Faculty of Science (FNWI) - Institute of Physics (IoP) - Institute for High Energy Physics (IHEF)
Abstract
The future KM3NeT neutrino telescope will be built on the seabed of the Mediterranean Sea at a depth between three and five kilometers. The high ambient pressure, but also the fact that the detector is hardly accessible, put severe constraints on the mechanical design of the detection units of the telescope. A detection unit is a vertical structure that supports the optical sensors of the telescope. It has a height of almost 900 m; two data cables run along the full length of the structure. The detection unit will be installed at the seabed as a compact package. Once acoustically released, it unfurls to its full length. The stability of the detection unit during unfurling and during operation is an important requirement for the mechanical design of the structure. We present the evolution of the design of the detection unit for the KM3NeT detector.
Document type Article
Note On behalf of theKM3NeT Consortium
Language English
Published at https://doi.org/10.1016/j.nima.2012.12.098
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