New observational work provides more information about the evolution of the Sun's interior and origins of its enigmatic 11(-ish) solar cycle. The research potentially opens the door to improved forecasting of decadal-scale solar variability.
On the main-sequence age of the Sun
Asteroseismology of Red-Giant Stars: Mixed Modes, Differential Rotation, and Eccentric Binaries
The Role of the Center-to-Limb Variation in Deduced Photometric Trends
Measuring the solar meridional flow from perturbations of mode eigenfunctions
Magnetic Phenomena on the Solar Surface using 3D radiative MHD simulations
Developments in Large Eddy Simulations for Compressible MHD Turbulence in Space Plasma
Insights into the Small-Scale Solar Dynamo from Ensemble Analysis of Magnetic Features
Comparison of inversion codes for polarized line formation in MHD simulations. Milne-Eddington codes
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