Haber and Hindman used images from SOHO's Michelson Doppler Imager telescope and examined them with a computational technique called ring-diagram analysis to measure the speed and direction of acoustic waves in small regions of the solar surface. This method allowed them to create three-dimensional maps of the wind directions at each point on the solar photosphere and below, layer by layer. The maps reveal patterns of steady, jet-stream-like flows with typical speeds of around 160 kilometers (100 miles) per hour, as well as swirling storms large enough to swallow Jupiter but lasting just three weeks.
Perhaps the most interesting find is a long-term change in flow patterns that may be analogous to the El Nino phenomenon. Haber and Hindman found that in the six years of measurements collected so far, there was a steady, uniform poleward flow in both hemispheres for the first two years. But in 1998 that flow suddenly halted and reversed direction in the northern hemisphere, starting about 10,000 km below the surface. The reversed flow has continued since then.
The poleward flows are important in generating the solar magnetic field and its 11-year cycle of activity. According to Alexander Kosovichev, a solar researcher at Stanford University, "the reversal of this flow is puzzling, and has important implications for our understanding of the solar activity cycle."
Monitoring these solar patterns could also play an important part in improving our ability to predict weather on the Sun that affects us on Earth — by making it possible to forecast coronal mass ejections and solar flares that can cause geomagnetic storms and disrupt electronics on satellites. "We can't predict them now, but we hope we'll be able to do that," Haber says.