Correlation of PC 3, 4, and 5 activity with solar wind speed

Details Correlation of PC 3, 4, and 5 activity with solar wind speed Correlation of PC 3, 4, and 5 activity with solar wind speed

Nov 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979jgr....84.6694g&link_type=abstract

Journal of Geophysical Research, vol. 84, Nov. 1, 1979, p. 6694-6696. Research sponsored by the National Research Council of Ca

Physics

11

Geomagnetic Micropulsations, Solar Terrestrial Interactions, Solar Wind Velocity, Interplanetary Magnetic Fields, Kelvin-Helmholtz Instability

Scientific paper

Positive correlations of magnetic pulsation amplitude with solar wind speed are found for Pc 3, 4, and 5 at both Calgary and Leduc. The data, obtained in September and October 1970, confirm and extend similar results found in an earlier interval for Pc 3, 4 at Calgary alone, thus adding further evidence for a velocity-controlled contribution, such as the Kelvin-Helmholtz instability, to pulsation activity

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