Role of observable nonlinearities in solar cycle modulation
M. Talafha, M. Nagy, A. Lemerle, and K. Petrovay

TL;DR
This paper investigates the roles of tilt quenching and latitude quenching in solar cycle modulation, revealing how their relative importance depends on model parameters and contributing to understanding solar magnetic activity variability.
Contribution
It systematically compares the effects of tilt and latitude quenching in surface flux transport and dynamo models, highlighting the conditions under which each mechanism dominates.
Findings
Latitude quenching's importance depends on the u0/η ratio.
Analytical interpretation links the effect to the dynamo effectivity range.
Both TQ and LQ significantly influence solar cycle modulation.
Abstract
Context. Two candidate mechanisms have recently been considered for the nonlinear modulation of solar cycle amplitudes. Tilt quenching (TQ) is a negative feedback between cycle amplitude and the mean tilt angle of bipolar active regions relative to the azimuthal direction; latitude quenching (LQ) consists in a positive correlation between cycle amplitude and average emergence latitude of active regions. Aims. Here we explore the relative importance of and the determining factors behind the LQ and TQ effects. Methods. The degree of nonlinearity induced by TQ, LQ and their combination is systematically probed in a grid of surface flux transport (SFT) models. The role of TQ and LQ is also explored in the successful 2x2D dynamo model optimized to reproduce the statistical behaviour of real solar cycles. Results. The relative importance of LQ vs TQ is found to correlate with the ratio u 0…
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