On the current solar magnetic activity in the light of its behaviour during the Holocene
F. Inceoglu, R. Simoniello, M. F. Knudsen, C. Karoff, J. Olsen, and S., Turck-Chi\`eze

TL;DR
This study investigates the Sun's magnetic activity over the Holocene using cosmogenic nuclide data, revealing patterns of grand minima and maxima that suggest a non-linear, oscillatory dynamo behavior influenced by the Lorentz force.
Contribution
It provides a novel analysis of Holocene solar magnetic activity patterns and links them to non-linear dynamo models with memory effects, based on cosmogenic radionuclide data.
Findings
71% of grand maxima were followed by grand minima
Patterns suggest the Sun acts as a relaxation oscillator
Magnetic activity exhibits non-uniform temporal distribution
Abstract
Solar modulation potential (SMP) reconstructions based on cosmogenic nuclide records reflect changes in the open solar magnetic field and can therefore help us obtain information on the behaviour of the open solar magnetic field over the Holocene period. We aim at comparing the Sun's large-scale magnetic field behaviour over the last three solar cycles with variations in the SMP reconstruction through the Holocene epoch. To achieve these objectives, we use the IntCal13 C data to investigate distinct patterns in the occurrences of grand minima and maxima during the Holocene period. We then check whether these patterns might mimic the recent solar magnetic activity by investigating the evolution of the energy in the Sun's large-scale dipolar magnetic field using the Wilcox Solar Observatory data. The cosmogenic radionuclide data analysis shows that 71\% of grand maxima during…
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.
