Mystery of solar cycle illuminated

In the convection zone of the star, the plasma currents make a huge turnover that lasts about 22 years. (mps) Solar activity fluctuates in a rhythm of about eleven years, which is reflected among other things in the frequency of sunspots. A complete magnetic period lasts 22 years. Scientists have long been puzzling over what causes this cycle. It must be related to the conditions beneath the "skin" of our star: A layer of hot plasma - electrically-conductive gas - extends from the surface to 200,000 kilometers below. The plasma within this convection zone is constantly in motion. A team of scientists from the Max Planck Institute for Solar System Research, the University of Göttingen and New York University Abu Dhabi has now succeeded in drawing the most comprehensive picture of the plasma flows in nort-south-direction to date.