A Machine Learning Enhanced Approach for Automated Sunquake Detection in Acoustic Emission Maps

TL;DR

This paper introduces a machine learning framework utilizing AutoEncoders, Contrastive Learning, and object detection to automate and improve the detection of sunquakes in solar acoustic data, addressing noise and class imbalance challenges.

Contribution

It presents a novel application of machine learning techniques with custom domain-specific data augmentation for sunquake detection, a new approach in astrophysical data analysis.

Findings

Models can identify locations of acoustic emissions

Qualitative association with solar eruptions

Prototype stage with room for metric improvements

Abstract

Sunquakes are seismic emissions visible on the solar surface, associated with some solar flares. Although discovered in 1998, they have only recently become a more commonly detected phenomenon. Despite the availability of several manual detection guidelines, to our knowledge, the astrophysical data produced for sunquakes is new to the field of Machine Learning. Detecting sunquakes is a daunting task for human operators and this work aims to ease and, if possible, to improve their detection. Thus, we introduce a dataset constructed from acoustic egression-power maps of solar active regions obtained for Solar Cycles 23 and 24 using the holography method. We then present a pedagogical approach to the application of machine learning representation methods for sunquake detection using AutoEncoders, Contrastive Learning, Object Detection and recurrent techniques, which we enhance by introducing several custom domain-specific data augmentation transformations. We address the main challenges of the automated sunquake detection task, namely the very high noise patterns in and outside the active region shadow and the extreme class imbalance given by the limited number of frames that present sunquake signatures. With our trained models, we find temporal and spatial locations of peculiar acoustic emission and qualitatively associate them to eruptive and high energy emission. While noting that these models are still in a prototype stage and there is much room for improvement in metrics and bias levels, we hypothesize that their agreement on example use cases has the potential to enable detection of weak solar acoustic manifestations.