NCAR & UCAR News

Clock paints picture of a more orderly, predictable Sun

Jun 10, 2020 – by Laura Snider

Solar scientists have taken a mathematical technique used by Earth scientists to analyze cyclic phenomena, such as the ebb and flow of ocean tides, and applied it to the confounding irregularity of cycles on the Sun. The result is an elegant “Sun clock” that shows that solar activity starts and stops on a much more precise schedule than could be discerned when looking at observations of the Sun in the traditional way – plotted linearly over time.

The new research, published in the journal Geophysical Research Letters, was led by the University of Warwick in England and involved researchers from the National Center for Atmospheric Research (NCAR) and NASA.

Solar cycles – marked by the rhythmic waxing and waning of activity on the Sun – occur every 11 years on average, but they can last years longer or shorter. They also vary in their strength. While they all build from a quiet start toward the cycle’s solar maximum before quieting again, the magnitude of that maximum can change significantly from cycle to cycle. During and after solar maximum, the Sun is more likely to produce space weather that can impact Earth, damaging satellites, scrambling radio communications, and disrupting power grids, among other impacts. The new sun clock could be used as a planning tool to help keep space- and ground-based infrastructure safe.

The clock was created using a technique known as the Hilbert transform to convert the linear observations of past solar cycles onto a circle, stretching and shrinking the cycles as necessary to a standard 11 years. As the cycles were overlaid on top of each other on the clock’s face, distinct “times” on the clock face when solar activity is flipped on and off came into focus.