Influence of the magnetic cycle on the excitation of solar-like acoustic modes
The Sun's convective envelope generates, by dynamo effect, a surface magnetic field whose strength evolves on an 11-year cycle, with a change in polarity at the end of each cycle. Similar activity cycles exist in other solar-type stars, influencing the stars' dynamics, including the properties of acoustic oscillations, which are excited by
Panetier, Eva et al.
Fecha de publicación:
8
2024