Intensity of tropospheric circulation associated with solar magnetic sector boundary transits

Details Intensity of tropospheric circulation associated with solar magnetic sector boundary transits Intensity of tropospheric circulation associated with solar magnetic sector boundary transits

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979jatp...41..657w&link_type=abstract

Journal of Atmospheric and Terrestrial Physics, vol. 41, June 1979, p. 657-659. Research supported by Max C. Fleischmann Founda

Physics

2

Atmospheric Circulation, Interplanetary Magnetic Fields, Solar Magnetic Field, Solar Terrestrial Interactions, Troposphere, Northern Hemisphere, Vorticity, Winter

Scientific paper

The fractional decrease in the vorticity area index associated with transits past the earth of interplanetary magnetic sector boundaries increase as the value of vorticity used to compute the index increases. This suggests that after the boundary transit there is an approximately uniform reduction in all the values of vorticity that are not less than 0.00020/sec. In low altitudes and large absolute vorticities not less than 0.00020/sec the average change in the vorticity area index approaches 50%.

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