(13.12.2016)

The team used several years of data from the Helioseismic and Magnetic Imager on NASA‘s Solar Dynamics Observatory satellite to measure a sharp down-turn in the sun‘s rotation rate in its very outer 150km. Kuhn said, „This is a gentle torque that is slowing it down, but over the sun‘s 5 billion year lifetime it has had a very noticeable influence on its outer 35,000km.“ Their paper describes how this photon-braking effect should be at work in most stars.

This change in rotation at the sun‘s surface affects the large-scale solar magnetic field and researchers are now trying to understand how the solar magnetism that extends out into the corona and finally into the Earth‘s environment will be affected by this braking.