# Torsional Oscillations in the Suns rotation contribute to the   Waldmeier-effect in Solar Cycles

**Authors:** Sushant S. Mahajan, Dibyendu Nandy, H.M. Antia, B.N. Dwivedi

arXiv: 1803.07758 · 2018-03-22

## TL;DR

This study shows that torsional oscillations in the Sun influence the Waldmeier effect in solar cycles, providing a physical basis for cycle prediction and linking internal solar dynamics with surface phenomena.

## Contribution

The paper introduces a flux transport dynamo model incorporating observed torsional oscillations, demonstrating their role in reproducing the Waldmeier effect in solar cycles.

## Key findings

- Torsional oscillations do not significantly alter overall solar cycle amplitude.
- Variations in torsional oscillations reproduce Waldmeier effect characteristics.
- The Waldmeier effect may result from cycle-to-cycle modulation of torsional oscillations.

## Abstract

Temporal variations in the Suns internal velocity field with a periodicity of about 11 years have been observed over the last four decades. The period of these torsional oscillations and their latitudinal propagation roughly coincides with the period and equatorward propagation of sunspots which originate from a magnetohydrodynamic dynamo mechanism operating in the Suns interior. While the solar differential rotation plays an important role in this dynamo mechanism by inducting the toroidal component of magnetic field, the impact of torsional oscillations on the dynamo mechanism and hence the solar cycle is not well understood. Here, we include the observed torsional oscillations into a flux transport dynamo model of the solar cycle to investigate their effect. We find that the overall amplitude of the solar cycle does not change significantly on inclusion of torsional oscillations. However, all the characteristics of the Waldmeier effect in the sunspot cycle are qualitatively reproduced by varying only the amplitude of torsional oscillations. The Waldmeier effect, first noted in 1935, includes the important characteristic that the amplitude of sunspot cycles is anti-correlated to their rise time; cycles with high initial rise rate tend to be stronger. This has implications for solar cycle predictions. Our results suggest that the Waldmeier effect could be a plausible outcome of cycle to cycle modulation of torsional oscillations and provides a physical basis for sunspot cycle forecasts based on torsional oscillation observations. We also provide a theoretical explanation based on the magnetic induction equation thereby connecting two apparently disparate phenomena.

## Full text

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## Figures

8 figures with captions in the complete paper: https://tomesphere.com/paper/1803.07758/full.md

## References

36 references — full list in the complete paper: https://tomesphere.com/paper/1803.07758/full.md

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Source: https://tomesphere.com/paper/1803.07758