Application of Machine Learning to Identify Radio Pulses of Air Showers at the South Pole (ARENA 2024)
Frank G. Schroeder, Abdul Rehman (for the IceCube Collaboration)

TL;DR
This study demonstrates that convolutional neural networks can effectively identify cosmic-ray air-shower radio pulses, increasing detection rates and purity while maintaining angular resolution, thus enhancing radio detection capabilities at the South Pole.
Contribution
The paper introduces a CNN-based method for radio pulse identification in air-shower measurements, improving detection sensitivity and background cleaning over traditional techniques.
Findings
Detected five times more events than traditional methods.
Improved event purity despite lower detection threshold.
Maintained angular resolution of shower direction reconstruction.
Abstract
Machine learning is a useful tool for identifying radio pulses from cosmic-ray air showers and for cleaning such pulses from radio background. This can lower the detection threshold and increase the accuracy for the pulse time and amplitude. We have trained Convolutional Neural Networks (CNNs) using CoREAS simulations and background recorded by a prototype station at the IceTop surface array at the South Pole and have applied them to air-shower measurements by this station. The station consists of 3 SKALA antennas and 8 scintillators, which are used to trigger the readout of the antennas upon a sixfold coincidence. Afterwards, the radio signal is filtered to the band of 70-350 MHz. By applying neural networks to search for radio signals in about four months of data, we find about five times more events than by a traditional method based on a signal-to-noise ratio cut after filtering for…
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