Relationship of solar wind parameters to continuous, dayside, high latitude traveling ionospheric convection vortices

Details Relationship of solar wind parameters to continuous, dayside, high latitude traveling ionospheric convection vortices Relationship of solar wind parameters to continuous, dayside, high latitude traveling ionospheric convection vortices

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990jgr....9515007m&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 95, Sept. 1, 1990, p. 15007-15022.

Physics

46

Convection, Earth Ionosphere, Solar Wind, Traveling Ionospheric Disturbances, Vortices, Geomagnetic Pulsations, Interplanetary Magnetic Fields, Least Squares Method, Magnetometers, Solar Wind Velocity

Scientific paper

The results of a statistical study of the occurrence of steady traveling ionospheric convection vortices are presented. The upstream solar wind parameters observed by the IMP 8 spacecraft are studied as well. It is suggested that this class of pulsations is most likely to be detected post local noon and when the solar wind speed is low. A correlation between the frequency of dayside pulsations and the solar wind speed is found.

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