The Sun and other stars are magnetic: magnetism pervades their interiors and affects their
evolution in a variety of ways. In the Sun, both the fields themselves and their influence on …

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Kepler ultra-high precision photometry of long and continuous observations provides a
unique dataset in which surface rotation and variability can be studied for thousands of stars …

Oscillations detected on the solar surface provide a unique opportunity for investigations of
the interior properties of a star. Through major observational efforts, including extensive …

Until the last few decades, investigations of stellar interiors had been restricted to theoretical
studies only constrained by observations of their global properties and external …

Helioseismology has allowed us to study the structure of the Sun in unprecedented detail.
One of the triumphs of the theory of stellar evolution was that helioseismic studies had …

▪ Abstract Three cases for mixing not present in standard stellar models are presented: Light
element depletion in low mass main-sequence stars, deep mixing in massive stars, and …

The Sun's rotation profile and lithium content have been difficult to understand in the context
of conventional models of stellar evolution. Classical hydrodynamic models predict that the …

The internal properties of stars in the red-giant phase undergo significant changes on
relatively short timescales. Long near-uninterrupted high-precision photometric timeseries …

We present estimates of the amplitudes of intrinsically stable stochastically excited radial
oscillations in stars near the main sequence. The amplitudes are determined by the balance …