Time-Variant Vector Field Visualization for Magnetic Fields of Neutron Star Simulations
Simon J. Lieb, William Cook, Jan Hombeck, Sebastiano Bernuzzi, Kai, Lawonn

TL;DR
This paper introduces a new interactive visualization tool for exploring the complex, time-dependent magnetic fields in neutron star simulations, aiding astrophysicists in understanding their evolution and stability.
Contribution
The paper presents a novel visualization application combining sparse and dense vector field techniques for interactive, real-time exploration of large, time-resolved neutron star simulation data.
Findings
Experts rated the tool very positively.
The tool enables intuitive investigation of magnetic field evolution.
It supports real-time domain-specific data analysis.
Abstract
We present a novel visualization application designed to explore the time-dependent development of magnetic fields of neutron stars. The strongest magnetic fields in the universe can be found within neutron stars, potentially playing a role in initiating astrophysical jets and facilitating the outflow of neutron-rich matter, ultimately resulting in the production of heavy elements during binary neutron star mergers. Since such effects may be dependent on the strength and configuration of the magnetic field, the formation and parameters of such fields are part of current research in astrophysics. Magnetic fields are investigated using simulations in which various initial configurations are tested. However, the long-term configuration is an open question, and current simulations do not achieve a stable magnetic field. Neutron star simulations produce data quantities in the range of…
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Taxonomy
TopicsGeophysics and Sensor Technology · Geophysics and Gravity Measurements · Geomagnetism and Paleomagnetism Studies
