Dynamic Solar Magnetic and Velocity Fields

威尔科克斯太阳天文台(位于斯坦福大学)继续对不断演变的太阳条件进行足智多谋的调查。研究人员分析了收集到的数据，以进一步了解太阳周期和太阳活动原因、太阳内部条件、运动和磁场之间的相互作用、日冕磁结构和光球层中磁场和速度场的时间演变、预测太阳风CME特征的大小/重要性，以及日球层的大尺度结构。天文台正在升级和更换一些仪器。

The Wilcox Solar Observatory (at Stanford University) continues its resourceful investigations of evolving solar conditions. Investigators analyze the gathered data for further understanding of the solar cycle and solar activity causes, solar interior conditions, interactions between motions and magnetic field, temporal evolution of coronal magnetic structure and both magnetic and velocity fields in the photosphere, prediction of solar wind CME features' size/importance, and the large scale structure of the heliosphere. The Observatory is upgrading and replacing some of its instrumentation.