Low-Power Radiofrequency Systems for the RNO-G Project
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 compos...
Published in: | Proceedings of 38th International Cosmic Ray Conference — PoS(ICRC2023) |
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Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Other Authors: | , |
Format: | Article in Journal/Newspaper |
Language: | English |
Published: |
Sissa Medialab
2024
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Subjects: | |
Online Access: | https://hdl.handle.net/11370/9905783d-f817-4aea-bee3-364f959ba4fd https://research.rug.nl/en/publications/9905783d-f817-4aea-bee3-364f959ba4fd https://doi.org/10.22323/1.444.1171 https://pure.rug.nl/ws/files/1230462173/ICRC2023_1171.pdf http://www.scopus.com/inward/record.url?scp=85212255878&partnerID=8YFLogxK |
Summary: | 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. |
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