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太阳磁场扇形结构:与地球大气环流的关系。

Solar Magnetic Sector Structure: Relation to Circulation of the Earth's Atmosphere.

出版信息

Science. 1973 Apr 13;180(4082):185-6. doi: 10.1126/science.180.4082.185.

Abstract

The solar magnetic sector structure appears to be related to the average area of high positive vorticity centers (low-pressure troughs) observed during winter in the Northern Hemisphere at the 300-millibar level. The average area of high vorticity decreases (low-pressure troughs become less intense) during a few days near the times at which sector boundaries are carried past the earth by the solar wind. The amplitude of the effect is about 10 percent.

摘要

太阳磁扇区结构似乎与北半球在 300 毫巴高度冬季观测到的高正涡度中心(低压槽)的平均面积有关。在太阳风将扇区边界带至地球附近的几天内,高涡度的平均面积减小(低压槽变得不那么强烈)。该效应的幅度约为 10%。

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