本文研究了卡林顿自转周1591- 1592中冕流偏振亮度的变化。
The variation of the polarization brightness of coronal streamer in Carrington Rotations 1591-1592 is investigated.
在子午面内，研究具有嵌套闭磁场结构冕流背景对触发日冕物质抛射(CME)特征的影响。
The influence of a streamer background with nested close magnetic structures on the properties of CME initiated from its bottom is investigated in a solar meridian plane.
本文采用了2 5维MHD方程，用数值模拟方法研究了CME和冕流结构之间复杂的相互作用过程。
In this paper, by using the 2 5-dimension MHD equations, the complicated process of the interaction between the CME and helmet streamer is studied through numerical simulation.
然而，这一次，向两极移动的冕流却慢腾腾的，它意味着我们可能将在2013年经历一个非常弱的太阳活动峰值——这也许会延迟甚至阻止下个太阳活动周期的开始。
This time, however, the rush to the poles is more of acrawl, which means we could be headed toward a very weak solar maximum in2013—and it may delay or even prevent the start of the next solar cycle.
然而，这一次，向两极移动的冕流却慢腾腾的，它意味着我们可能将在2013年经历一个非常弱的太阳活动峰值——这也许会延迟甚至阻止下个太阳活动周期的开始。
This time, however, the rush to the poles is more of acrawl, which means we could be headed toward a very weak solar maximum in2013—and it may delay or even prevent the start of the next solar cycle.
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