Listening to the magnetosphere: How best to make ULF waves audible
Martin O. Archer, Marek Cottingham, Michael D. Hartinger, Xueling Shi,, Shane Coyle, Ethan "Duke" Hill, Michael F. J. Fox, Emmanuel V. Masongsong

TL;DR
This paper explores how to convert magnetospheric ULF wave data into audible sound using audification and time scale modification techniques, enhancing scientific analysis and educational outreach.
Contribution
It applies music audio processing methods to space physics data, providing new ways to make ULF waves audible without losing information.
Findings
Audification preserves data integrity in sound conversion.
Time scale modification improves listenability of ULF waves.
Recommendations for researchers on effective audio rendering methods.
Abstract
Observations across the heliosphere typically rely on in situ spacecraft observations producing time-series data. While often this data is analysed visually, it lends itself more naturally to our sense of sound. The simplest method of converting oscillatory data into audible sound is audification -- a one-to-one mapping of data samples to audio samples -- which has the benefit that no information is lost, thus is a true representation of the original data. However, audification can make some magnetospheric ULF waves observations pass by too quickly for someone to realistically be able to listen to effectively. For this reason, we detail various existing audio time scale modification techniques developed for music, applying these to ULF wave observations by spacecraft and exploring how they affect the properties of the resulting audio. Through a public dialogue we arrive at…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
