| Issue |
A&A
Volume 708, April 2026
|
|
|---|---|---|
| Article Number | L21 | |
| Number of page(s) | 5 | |
| Section | Letters to the Editor | |
| DOI | https://doi.org/10.1051/0004-6361/202659586 | |
| Published online | 24 April 2026 | |
Letter to the Editor
Ultra-fast simulations of the solar dipole and open flux
Space Physics and Astronomy Research Unit, University of Oulu, POB 8000, FI-90014 Oulu, Finland
★ Corresponding author: This email address is being protected from spambots. You need JavaScript enabled to view it.
Received:
24
February
2026
Accepted:
12
April
2026
Abstract
Context. The solar dipole captures important information characterizing the large-scale solar magnetic field. The evolution of the solar magnetic field including the solar dipole can be simulated with a surface flux transport (SFT) model, but these simulations are more extensive than is otherwise necessary to produce the evolution of the dipole alone.
Aims. We present a dipole flux transport (DFT) matrix method that combines the classic SFT model with dipole vector representation of the solar magnetic field, which enables significantly faster simulations of the solar dipole.
Methods. By simulating the evolution of basis vectors of a synoptic map, we were able to construct propagator matrices that produce the time evolution of the solar magnetic field by means of matrix multiplication. The computational speedup was achieved by compressing the propagator matrices to very small fraction (< 10−4) of their original size with a recent vector sum method.
Results. Depending on the time resolution, the DFT performs 100−1000 times faster than a 4-year SFT simulation of a single active region, while producing equivalent results. For multiple source regions, daily propagation matrices are sufficient to produce results that agree within 1% with the SFT simulation of solar cycle 24, while performing 80 times faster. If the evolution of individual active regions is needed, the DFT is equipped to perform 50000 times faster than the SFT model.
Conclusions. Overall, DFT makes solar dipole simulations extremely fast, making it possible to run thousands of simulations in a few minutes with a basic laptop setup. As the magnitude of the dipole vector closely matches the open solar flux (OSF) from the potential field source surface model, the DFT can be used to study the development of OSF in various scenarios in an extremely efficient way.
Key words: Sun: activity / Sun: corona / Sun: magnetic fields / Sun: photosphere
© The Authors 2026
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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