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

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

Apr 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973sci...180..185w&link_type=abstract

Science, Volume 180, Issue 4082, pp. 185-186

Physics

28

Scientific paper

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.

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