Seasonal variation and magnitude of the solar sector structure-atmospheric vorticity effect

Details Seasonal variation and magnitude of the solar sector structure-atmospheric vorticity effect Seasonal variation and magnitude of the solar sector structure-atmospheric vorticity effect

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975natur.255..539w&link_type=abstract

Nature, vol. 255, June 12, 1975, p. 539, 540. Navy-NASA-NSF-supported research.

Physics

13

Annual Variations, Atmospheric Circulation, Interplanetary Magnetic Fields, Magnetic Field Configurations, Solar Wind, Vorticity, Error Analysis, Solar Magnetic Field, Solar Rotation, Standard Deviation

Scientific paper

Evidence is reported for a seasonal variation in the effect of solar sector structure on terrestrial atmospheric vorticity. Graphs showing average response of the 50,000-Pa vorticity area index to solar magnetic sector structure during the time interval extending from 6 days before to 6 days after the time at which a sector boundary is swept past the earth indicate that a 10% drop in the average value occurs at the time of passage, but this effect is observed only during the winter months.

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