TL;DR
This paper reviews the properties, excitation, damping, and diagnostic analysis of solar-like oscillations in solar-type stars, highlighting recent progress and effects of stellar-cycle variations on low-mass main-sequence stars.
Contribution
It provides a comprehensive summary of the current understanding and recent advances in asteroseismic analysis of solar-type variables, emphasizing diagnostic techniques and stellar-cycle effects.
Findings
Detailed properties of solar-like oscillations
Advances in asteroseismic diagnostic techniques
Effects of stellar-cycle variations on oscillations
Abstract
The rich acoustic oscillation spectrum in solar-type variables make these stars particularly interesting for studying fluid-dynamical aspects of the stellar interior. I present a summary of the properties of solar-like oscillations, how they are excited and damped and discuss some of the recent progress in using asteroseismic diagnostic techniques for analysing low-degree acoustic modes. Also the effects of stellar-cycle variations in low-mass main-sequence stars are addressed.
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