Tropospheric circulation and interplanetary magnetic sector boundaries followed by MeV proton streams

Details Tropospheric circulation and interplanetary magnetic sector boundaries followed by MeV proton streams Tropospheric circulation and interplanetary magnetic sector boundaries followed by MeV proton streams

Apr 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979natur.278..840w&link_type=abstract

Nature, vol. 278, Apr. 26, 1979, p. 840, 841.

Other

7

Atmospheric Circulation, Interplanetary Magnetic Fields, Proton Flux Density, Solar Wind Velocity, Tropospheric Radiation, Boundary Layer Transition, Cosmic Rays, Geomagnetism, Solar Magnetic Field, Vorticity

Scientific paper

The MeV proton streams which Svestka et al. (1976) connected with certain sector boundary transits appear to select boundary transits associated with unusually active solar wind conditions. Changes in tropospheric circulation linked to the proton boundary transits were larger than those linked to other boundary transits observed during the same interval. This investigation of sector boundary transits also sheds light on the relationship between changes in solar wind velocity, density and magnetic field and terrestrial changes in the vorticity area index, geomagnetic activity, and cosmic ray flux at earth.

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