Low-Power Radiofrequency Systems for the RNO-G Project

RNO-G Collaboration

Low-Power Radiofrequency Systems for the RNO-G Project

RNO-G Collaboration

Physics

Research output: Contribution to journal › Conference article › peer-review

Abstract

The Radio Neutrino Observatory in Greenland (RNO-G) seeks to detect the Askaryan radio emission from energetic neutrinos (> 10 PeV) interacting in the Greenland ice sheet. The RNO-G detector comprises an array of independent and autonomous radio-detector stations, each with a hybrid design composed of deep borehole (∼100m) and surface antennas, which require low-power, robust, and scalable low-noise radiofrequency (RF) amplifier and signal-transport systems over a ∼80-650MHz bandwidth. In this contribution, we will present the design and performance of the custom RNO-G RF signal chains, including a field-proven and low-cost RF-over-fiber (RFoF) unit.

Original language	English (US)
Article number	1171
Journal	Proceedings of Science
Volume	444
State	Published - Sep 27 2024
Event	38th International Cosmic Ray Conference, ICRC 2023 - Nagoya, Japan Duration: Jul 26 2023 → Aug 3 2023

All Science Journal Classification (ASJC) codes

General

Cite this

@article{6b0a24c66d7e4316a504153245c7e916,

title = "Low-Power Radiofrequency Systems for the RNO-G Project",

abstract = "The Radio Neutrino Observatory in Greenland (RNO-G) seeks to detect the Askaryan radio emission from energetic neutrinos (> 10 PeV) interacting in the Greenland ice sheet. The RNO-G detector comprises an array of independent and autonomous radio-detector stations, each with a hybrid design composed of deep borehole (∼100m) and surface antennas, which require low-power, robust, and scalable low-noise radiofrequency (RF) amplifier and signal-transport systems over a ∼80-650MHz bandwidth. In this contribution, we will present the design and performance of the custom RNO-G RF signal chains, including a field-proven and low-cost RF-over-fiber (RFoF) unit.",

author = "\{RNO-G Collaboration\} and E. Oberla and Aguilar, \{J. A.\} and P. Allison and D. Besson and A. Bishop and O. Botner and S. Bouma and S. Buitink and W. Castiglioni and M. Cataldo and Clark, \{B. A.\} and A. Coleman and K. Couberly and P. Dasgupta and \{de Kockere\}, S. and \{de Vries\}, \{K. D.\} and C. Deaconu and DuVernois, \{M. A.\} and A. Eimer and C. Glaser and T. Gl{\"u}senkamp and A. Hallgren and S. Hallmann and Hanson, \{J. C.\} and B. Hendricks and J. Henrichs and N. Heyer and C. Hornhuber and K. Hughes and T. Karg and A. Karle and Kelley, \{J. L.\} and M. Korntheuer and M. Kowalski and I. Kravchenko and R. Krebs and R. Lahmann and P. Lehmann and U. Latif and P. Laub and Liu, \{C. H.\} and J. Mammo and Marsee, \{M. J.\} and Meyers, \{Z. S.\} and M. Mikhailova and K. Michaels and K. Mulrey and M. Muzio and A. Nelles and S. Wissel",

note = "Publisher Copyright: {\textcopyright} Copyright owned by the author(s) under the terms of the Creative Commons.; 38th International Cosmic Ray Conference, ICRC 2023 ; Conference date: 26-07-2023 Through 03-08-2023",

year = "2024",

month = sep,

day = "27",

language = "English (US)",

volume = "444",

journal = "Proceedings of Science",

issn = "1824-8039",

publisher = "Sissa Medialab Srl",

}

TY - JOUR

T1 - Low-Power Radiofrequency Systems for the RNO-G Project

AU - RNO-G Collaboration

AU - Oberla, E.

AU - Aguilar, J. A.

AU - Allison, P.

AU - Besson, D.

AU - Bishop, A.

AU - Botner, O.

AU - Bouma, S.

AU - Buitink, S.

AU - Castiglioni, W.

AU - Cataldo, M.

AU - Clark, B. A.

AU - Coleman, A.

AU - Couberly, K.

AU - Dasgupta, P.

AU - de Kockere, S.

AU - de Vries, K. D.

AU - Deaconu, C.

AU - DuVernois, M. A.

AU - Eimer, A.

AU - Glaser, C.

AU - Glüsenkamp, T.

AU - Hallgren, A.

AU - Hallmann, S.

AU - Hanson, J. C.

AU - Hendricks, B.

AU - Henrichs, J.

AU - Heyer, N.

AU - Hornhuber, C.

AU - Hughes, K.

AU - Karg, T.

AU - Karle, A.

AU - Kelley, J. L.

AU - Korntheuer, M.

AU - Kowalski, M.

AU - Kravchenko, I.

AU - Krebs, R.

AU - Lahmann, R.

AU - Lehmann, P.

AU - Latif, U.

AU - Laub, P.

AU - Liu, C. H.

AU - Mammo, J.

AU - Marsee, M. J.

AU - Meyers, Z. S.

AU - Mikhailova, M.

AU - Michaels, K.

AU - Mulrey, K.

AU - Muzio, M.

AU - Nelles, A.

AU - Wissel, S.

PY - 2024/9/27

Y1 - 2024/9/27

N2 - The Radio Neutrino Observatory in Greenland (RNO-G) seeks to detect the Askaryan radio emission from energetic neutrinos (> 10 PeV) interacting in the Greenland ice sheet. The RNO-G detector comprises an array of independent and autonomous radio-detector stations, each with a hybrid design composed of deep borehole (∼100m) and surface antennas, which require low-power, robust, and scalable low-noise radiofrequency (RF) amplifier and signal-transport systems over a ∼80-650MHz bandwidth. In this contribution, we will present the design and performance of the custom RNO-G RF signal chains, including a field-proven and low-cost RF-over-fiber (RFoF) unit.

AB - The Radio Neutrino Observatory in Greenland (RNO-G) seeks to detect the Askaryan radio emission from energetic neutrinos (> 10 PeV) interacting in the Greenland ice sheet. The RNO-G detector comprises an array of independent and autonomous radio-detector stations, each with a hybrid design composed of deep borehole (∼100m) and surface antennas, which require low-power, robust, and scalable low-noise radiofrequency (RF) amplifier and signal-transport systems over a ∼80-650MHz bandwidth. In this contribution, we will present the design and performance of the custom RNO-G RF signal chains, including a field-proven and low-cost RF-over-fiber (RFoF) unit.

UR - https://www.scopus.com/pages/publications/85212255878

UR - https://www.scopus.com/pages/publications/85212255878#tab=citedBy

M3 - Conference article

AN - SCOPUS:85212255878

SN - 1824-8039

VL - 444

JO - Proceedings of Science

JF - Proceedings of Science

M1 - 1171

T2 - 38th International Cosmic Ray Conference, ICRC 2023

Y2 - 26 July 2023 through 3 August 2023

ER -

Low-Power Radiofrequency Systems for the RNO-G Project

Abstract

All Science Journal Classification (ASJC) codes

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