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Main Authors: Verniero, Jaye, Stephenson, Bryan, Alexander, Robert
Format: Recurso digital
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Published: Zenodo 2025
Online Access:https://doi.org/10.5281/zenodo.14796817
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author Verniero, Jaye
Stephenson, Bryan
Alexander, Robert
author_facet Verniero, Jaye
Stephenson, Bryan
Alexander, Robert
contents <p>An audio-visual rendering of magnetic field measurements captured by Parker Solar Probe's Fluxgate Magnetometer during the "Gorgeous Switchback" of November 21, 2021 (14:06-14:10 UT) during Encounter 10. The original RTN (Radial-Tangential-Normal) coordinates have been transformed into 4D space using the Hopf fibration and rendered in 3D through stereographic projection.</p> <p>The visualization represents the transformed magnetic field data through synchronized visual and auditory elements. The visual component displays data points in XYZ space with time-based color coding. The sonification maps spatial parameters to sound: height (Y-axis) controls the pitch of mandolin samples played back via granular synthesis, lateral position (X-axis) determines stereo panning, and depth (Z-axis) modulates amplitude.</p> <p>The data playback rate is approximately one data point per 30ms, allowing for detailed exploration of the magnetic field structure during the switchback event. This novel representation enables the identification of previously hidden patterns through both visual and auditory analysis.</p>
format Recurso digital
id zenodo_https___doi_org_10_5281_zenodo_14796817
institution Zenodo
language
publishDate 2025
publisher Zenodo
record_format zenodo
spellingShingle Audio-Visual Rendering of Parker Solar Probe Magnetic Field Data Using the Hopf Fibration (E10 Switchback)
Verniero, Jaye
Stephenson, Bryan
Alexander, Robert
<p>An audio-visual rendering of magnetic field measurements captured by Parker Solar Probe's Fluxgate Magnetometer during the "Gorgeous Switchback" of November 21, 2021 (14:06-14:10 UT) during Encounter 10. The original RTN (Radial-Tangential-Normal) coordinates have been transformed into 4D space using the Hopf fibration and rendered in 3D through stereographic projection.</p> <p>The visualization represents the transformed magnetic field data through synchronized visual and auditory elements. The visual component displays data points in XYZ space with time-based color coding. The sonification maps spatial parameters to sound: height (Y-axis) controls the pitch of mandolin samples played back via granular synthesis, lateral position (X-axis) determines stereo panning, and depth (Z-axis) modulates amplitude.</p> <p>The data playback rate is approximately one data point per 30ms, allowing for detailed exploration of the magnetic field structure during the switchback event. This novel representation enables the identification of previously hidden patterns through both visual and auditory analysis.</p>
title Audio-Visual Rendering of Parker Solar Probe Magnetic Field Data Using the Hopf Fibration (E10 Switchback)
url https://doi.org/10.5281/zenodo.14796817