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Cited article:

How well does surface magnetism represent deep Sun-like star dynamo action?

A. J. Finley, A. S. Brun, A. Strugarek and R. Cameron
Astronomy & Astrophysics 684 A92 (2024)
https://doi.org/10.1051/0004-6361/202347862

The influence of small bipolar magnetic regions on basic solar quantities

B. Hofer, N. A. Krivova, R. Cameron, S. K. Solanki and J. Jiang
Astronomy & Astrophysics 683 A48 (2024)
https://doi.org/10.1051/0004-6361/202245635

A Babcock-Leighton dynamo model of the Sun incorporating toroidal flux loss and the helioseismically inferred meridional flow

S. Cloutier, R. H. Cameron and L. Gizon
Astronomy & Astrophysics 680 A42 (2023)
https://doi.org/10.1051/0004-6361/202347022

The crucial role of surface magnetic fields for stellar dynamos: ϵ Eridani, 61 Cygni A, and the Sun

S. V. Jeffers, R. H. Cameron, S. C. Marsden, et al.
Astronomy & Astrophysics 661 A152 (2022)
https://doi.org/10.1051/0004-6361/202142202

Toroidal Flux Loss due to Flux Emergence Explains why Solar Cycles Rise Differently but Decay in a Similar Way

Akash Biswas, Bidya Binay Karak and Robert Cameron
Physical Review Letters 129 (24) (2022)
https://doi.org/10.1103/PhysRevLett.129.241102

Towards an algebraic method of solar cycle prediction

Melinda Nagy, Kristóf Petrovay, Alexandre Lemerle and Paul Charbonneau
Journal of Space Weather and Space Climate 10 46 (2020)
https://doi.org/10.1051/swsc/2020051