太阳活动周期与表面环流有关

A new analysis of the unusually long solar cycle that ended in 2008 suggests that one reason for the long cycle could be a stretching of the Sun's conveyor belt, a current of plasma¹（等离子体，血浆） that circulates（传播，循环） between the Sun's equator（赤道） and its poles. The results should help scientists better understand the factors controlling the timing² of solar cycles and could lead to better predictions. The study was conducted by Mausumi Dikpati, Peter Gilman, and Giuliana de Toma, all scientists in the High Altitude Observatory³ at the National Center for Atmospheric⁴ Research (NCAR), and by Roger Ulrich at the University of California, Los Angeles. It appeared on July 30 in Geophysical Research Letters. The study was funded by the National Science Foundation, NCAR's sponsor, and by NASA.

The Sun goes through cycles lasting⁵ approximately 11 years that include phases with increased magnetic activity, more sunspots（太阳黑子，雀斑） , and more solar flares⁶, than phases with less activity. The level of activity on the Sun can affect navigation and communications systems on Earth. Puzzlingly, solar cycle 23, the one that ended in 2008, lasted longer than previous cycles, with a prolonged（延长的，拖延的） phase of low activity that scientists had difficulty explaining.

The new NCAR analysis suggests that one reason for the long cycle could be changes in the Sun's conveyor belt. Just as Earth's global ocean circulation transports water and heat around the planet, the Sun has a conveyor belt in which plasma flows along the surface toward the poles, sinks, and returns toward the equator, transporting magnetic flux⁷（磁通量） along the way.

"The key for explaining the long duration of cycle 23 with our dynamo（发电机） model is the observation of an unusually long conveyor belt during this cycle," Dikpati says. "Conveyor belt theory indicates that shorter belts, such as observed in cycle 22, should be more common in the Sun."

Recent measurements gathered and analyzed⁸ by Ulrich and colleagues show that in solar cycle 23, the poleward（向极的） flow extended all the way to the poles, while in previous solar cycles the flow turned back toward the equator at about 60 degrees latitude⁹. Furthermore, as a result of mass conservation, the return flow was slower in cycle 23 than in previous cycles.

In their paper, Dikpati, Gilman, and de Toma used simulations to model how the solar plasma conveyor belt affected¹⁰ the solar cycle. The authors found that the longer conveyor belt and slower return flow could have caused the longer duration of cycle 23.

The NCAR team's computer model, known as the Predictive Flux-transport Dynamo Model, simulates the evolution of magnetic fields in the outer third of the Sun's interior (the solar convection zone). It provides a physical basis for projecting the nature of upcoming solar cycles from the properties of previous cycles, as opposed to statistical¹¹ models that emphasize correlations¹² between cycles. In 2004, the model successfully predicted that cycle 23 would last longer than usual.

According to Dikpati, the duration of a solar cycle is probably determined¹³ by the strength of the Sun's meridional flow（经向气流） . The combination of this flow and the lifting and twisting of magnetic fields near the bottom of the convection zone generates the observed symmetry（对称，整齐） of the Sun's global field with respect to（关于，至于） the solar equator.

"This study highlights the importance of monitoring and improving measurement of the Sun's meridional circulation," Ulrich says. "In order to improve predictions of the solar cycle, we need a strong effort to understand large-scale patterns of solar plasma motion."