The Potential Impact of Neuromorphic Computing on Radio Telescope Observatories
Nicholas J. Pritchard, Richard Dodson, Andreas Wicenec

TL;DR
Neuromorphic computing, especially Spiking Neural Networks, has the potential to drastically reduce power consumption in radio telescope data processing, enabling more efficient and scalable radio astronomy observations.
Contribution
This paper provides a comprehensive analysis of deploying neuromorphic approaches in radio astronomy, highlighting near-term FPGA and future ASIC implementations for RFI detection.
Findings
Neuromorphic solutions could reduce power use by up to 1000 times.
SNNs are promising for real-time, data-driven RFI detection.
Potential for neuromorphic hardware to transform observatory operational costs.
Abstract
Radio astronomy relies on bespoke, experimental and innovative computing solutions. This will continue as next-generation telescopes such as the Square Kilometre Array (SKA) and next-generation Very Large Array (ngVLA) take shape. Under increasingly demanding power consumption, and increasingly challenging radio environments, science goals may become intractable with conventional von Neumann computing due to related power requirements. Neuromorphic computing offers a compelling alternative, and combined with a desire for data-driven methods, Spiking Neural Networks (SNNs) are a promising real-time power-efficient alternative. Radio Frequency Interference (RFI) detection is an attractive use-case for SNNs where recent exploration holds promise. This work presents a comprehensive analysis of the potential impact of deploying varying neuromorphic approaches across key stages in radio…
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Taxonomy
TopicsNeural Networks and Reservoir Computing · Advanced Memory and Neural Computing · Ferroelectric and Negative Capacitance Devices
