PoS - Proceedings of Science
Volume 395 - 37th International Cosmic Ray Conference (ICRC2021) - NU - Neutrinos & Muons
Optical analysis of the Pacific Ocean Neutrino Experiment (P-ONE) site using data from the first pathfinder mooring
Presented by C. Fruck*, A. Gartner, I.C. Rea and J. Stacho  on behalf of N. Bailly, J. Bedard, M. Bohmer, J. Bosma, D. Brussow, J. Cheng, K. Clark, B. Croteau, M. Danninger, F.D. Leo, N. Deis, M. Ens, R. Fox, R. Gernhäuser, D. Grant, H. He, F. Henningsen, K. Holzapfel, R. Hotte, R. Jenkyns, H. Johnson, A. Katil, C. Kopper, C. Krauss, I. Kulin, K. Leismüller, S. Leys, T.T.Y. Lin, P. Macoun, T. McElroy, S.A. Meighen-Berger, J. Michel, R. Moore, M. Morley, L. Papp, B. Pirenne, T. Qiu, M. Rankin, E. Resconi, A. Round, A. Ruskey, R. Rutley, C. Spannfellner, R. Timmerman, M. Tomlin, M. Tradewell, M. Traxler, M. Uganecz, S. Wagner, J.P. Yanez and Y. Zhenget al. (click to show)
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Pre-published on: July 31, 2021
Published on: March 18, 2022
Abstract
The Pacific Ocean Neutrino Experiment (P-ONE) is an initiative by a collaboration of Canadian and German universities as well as Ocean Networks Canada (ONC) to develop a new large-scale neutrino telescope 2600 m below the ocean off the coast of western Canada. While the instrumented volume needs to be at least on the order of km³ for the physics goals of P-ONE to be met, the density of photo sensors needs to be kept as low as possible in order to minimize construction costs. Naturally, this puts very high demands on the optical properties of water at the deployment site. Ideally, the water should exhibit minimal photon extinction and scattering to optimize the light yield and timing needed for reconstructing neutrino-induced Cherenkov light flashes. In addition, a low light background from natural undersea sources such as bioluminescence and K40 radioactive decay is necessary for achieving high sensitivity to neutrino events. In order to evaluate the proposed site for P-ONE, two pathfinder missions have been deployed successfully, one in 2018 and the other in 2020. We present the results from the first mission that was primarily aimed at evaluating the optical properties of the site in terms of attenuation length, and backgrounds.
DOI: https://doi.org/10.22323/1.395.1160
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