TL;DR
The paper introduces HipFT, a high-performance, open-source Surface Flux Transport model designed for solar magnetic field mapping, featuring modular design, parallel computing, and extensibility for improved solar physics research.
Contribution
It presents HipFT, an open-source, high-performance SFT code with advanced numerical methods, parallelism, and user-extensible features, filling a gap in existing solar magnetic field modeling tools.
Findings
HipFT achieves efficient multi-CPU and GPU parallelism.
Validated numerical methods ensure accurate flux transport simulations.
Enables ensemble modeling for uncertainty quantification.
Abstract
Global solar photospheric magnetic maps play a critical role in solar and heliospheric physics research. Routine magnetograph measurements of the field occur only along the Sun-Earth line, leaving the far-side of the Sun unobserved. Surface Flux Transport (SFT) models attempt to mitigate this by modeling the surface evolution of the field. While such models have long been established in the community (with several releasing public full-Sun maps), none are open source. The Open Source Flux Transport (OFT) model seeks to fill this gap by providing an open and user-extensible SFT model that also builds on the knowledge of previous models with updated numerical and data acquisition/assimilation methods along with additional user-defined features. In this first of a series of papers on OFT, we introduce its computational core: the High-performance Flux Transport (HipFT) code…
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