Solar Dynamics, Rotation, Convection and Overshoot

TL;DR

This paper reviews recent advances in understanding the Sun's internal dynamics, including rotation, convection, and overshoot, through observations, helioseismic methods, and computational modeling.

Contribution

It provides a comprehensive overview of recent observational, theoretical, and modeling progress in solar internal dynamics, highlighting new insights and methodologies.

Findings

Improved understanding of solar rotation profiles

Advances in helioseismic inference techniques

Enhanced computational models of solar convection

Abstract

We discuss recent observational, theoretical and modeling progress made in understanding the Sun's internal dynamics, including its rotation, meridional flow, convection and overshoot. Over the past few decades, substantial theoretical and observational effort has gone into appreciating these aspects of solar dynamics. A review of these observations, related helioseismic methodology and inference and computational results in relation to these problems is undertaken here.