Application of parabolic equation methods to in-ice radiowave propagation for ultra high energy neutrino detection experiments
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Issue Date
2022-03-18Author
Prohira, S.
Sbrocco, C.
Allison, P.
Beatty, J.
Besson, D.
Connolly, A.
Dasgupta, P.
Deaconu, C.
De Kockere, S.
de Vries, K.
Frikken, D.
Hast, C.
Huesca Santiago, E.
Kuo, C.Y.
Latif, U.A.
Lukic, V.
Meures, T.
Mulrey, K.
Nam, J.
Nozdrina, A.
Oberla, E.
Ralston, John P.
Stanley, R.S.
Torres, J.
Toscano, S.
Van den Broeck, D.
van Eijndhoven, N.
Wissel, S.
Type
Article
Article Version
Scholarly/refereed, publisher version
Published Version
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© Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0).
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Many ultra-high-energy neutrino-detection experiments seek radio wave signals from neutrino interactions deep within the polar ice, and an understanding of in-ice radio wave propagation is therefore of critical importance. The parabolic equation (PE) method for modeling the propagation of radio waves is a suitable intermediate between ray tracing and finite-difference time domain (FDTD) methods in terms of accuracy and computation time. The RET collaboration has developed the first modification of the PE method for use in modeling in-ice radio wave propagation for ultra high energy cosmic ray and neutrino detection experiments. In this proceeding we will detail the motivation for the development of this technique, the process by which it was modified for in-ice use, and showcase the accuracy of its results by comparing to FDTD and ray tracing.
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Citation
S. Prohira et al. Application of parabolic equation methods to in-ice radiowave propagation for ultra high energy neutrino detection experiments. 37th International Cosmic Ray Conference (ICRC 2021). July 12th – 23rd, 2021. Online – Berlin, Germany.
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