研究人员公布太阳磁场模型

Researchers at the Universities of Leeds and Chicago have uncovered an important mechanism¹ behind the generation of astrophysical（天体物理学的） magnetic fields such as that of the Sun. Scientists have known since the 18th Century that the Sun regularly oscillates（振荡，摆动） between periods of high and low solar activity in an 11-year cycle, but have been unable to fully² explain how this cycle is generated.

 

In the 'Information Age', it has become increasingly important to be able to understand the Sun's magnetic activity, as it is the changes in its magnetic field that are responsible for 'space weather' phenomena³, including solar flares⁴ and coronal mass ejections. When this weather heads in the direction of Earth it can damage satellites, endanger astronauts on the International Space Station and cause power grid⁵ outages on the ground.

 

The research, published in the journal Nature, explains how the cyclical nature of these large-scale magnetic fields emerges, providing a solution to the mathematical equations governing fluids and electromagnetism for a large astrophysical body.

 

The mechanism, known as a dynamo（发电机）, builds on a solution to a reduced set of equations first proposed in the 1950s which could explain the regular oscillation but which appeared to break down when applied⁶ to objects with high electrical conductivity. The mechanism takes into account the 'shear⁷' effect of mass movement of the ionised gas, known as plasma⁸, which makes up the Sun. More importantly it does so in the extreme parameter⁹ regime that is relevant to astrophysical bodies.

 

"Previously¹⁰, dynamos for large, highly conducting bodies such as the Sun would be overwhelmed by small-scale fluctuations¹¹ in the magnetic field. Here, we have demonstrated a new mechanism involving a shear flow, which served to damp these small-scale variations, revealing the dominant¹² large-scale pattern," said Professor Steve Tobias, from the University of Leeds' School of Mathematics, a co-author of the research.

 

What is more, this mechanism could be used to describe other large, spinning astronomical¹³ bodies with large-scale magnetic fields such as galaxies¹⁴.

 

The dynamo was developed through simulations using the high-performance computing¹⁵ facilities located at the University of Leeds.

 

"The fact that it took 50 years and huge supercomputers shows how complicated the dynamo process really is." said Prof Fausto Cattaneo, from the University of Chicago's Department of Astronomy and Astrophysics.

 

The presence of spots on the Sun has been known since antiquity¹⁶（高龄，古物）, and further analysed after the invention of the telescope by Galileo in the 16th Century. However, their cyclic nature, with periods of high activity (lots of sunspots) and low activity (few sunspots) following each other, was not identified until the 18th Century. At the start of the 20th Century it was then recognised that these sunspots were the result of the Sun's magnetic field. Since then much effort has been devoted¹⁷ to understanding what processes lead to the formation of sunspots and the origin of their cyclic behaviour.

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