A contribution to ULF activity in the Pc 3-4 range correlated with IMF radial orientation

Details A contribution to ULF activity in the Pc 3-4 range correlated with IMF radial orientation A contribution to ULF activity in the Pc 3-4 range correlated with IMF radial orientation

Nov 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977jgr....82.4991g&link_type=abstract

Journal of Geophysical Research, vol. 82, Nov. 1, 1977, p. 4991-4996. Research supported by the National Research Council of Ca

Mathematics

Probability

5

Geomagnetic Micropulsations, Interplanetary Magnetic Fields, Solar Activity Effects, Solar Wind, Amplitudes, Bow Waves, Explorer 35 Satellite, Kp Index, Shock Wave Propagation

Scientific paper

The paper describes an experiment to determine whether the radial orientation of the interplanetary magnetic field (IMF) is associated with ULF activity in the Pc 3-4 range. Data are obtained from base levels, undisturbed intervals, IMF and disturbance selection, and trigonometric correlation. The results obtained are discussed, noting particularly that for low Kp, the probability of enhanced amplitude noise rises as IMF orientation with respect to the nominal solar wind flow decreases in both Pc 3 and Pc 4 channels.

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