Some features of Pc5 pulsations during a solar cycle

Details Some features of Pc5 pulsations during a solar cycle Some features of Pc5 pulsations during a solar cycle

Jan 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978p%26ss...26....1r&link_type=abstract

Planetary and Space Science, vol. 26, Jan. 1978, p. 1-20.

Physics

1

Geomagnetic Pulsations, Solar Activity Effects, Solar Cycles, Annual Variations, Auroral Zones, Diurnal Variations, Geomagnetism, Magnetic Measurement, Magnetic Variations, Sunspots, Twenty-Seven Day Variation

Scientific paper

Based on Fort Churchill data for the years 1962-72, a 27-day recurrence tendency is suspected for the major characteristics of Pc 5 pulsations. Among the characteristics measured were occurrence, amplitude, and period. Sunspot number was found to strongly affect period (except for diurnal variations), while the correlation of sunspots with occurrence was less pronounced. Occurrence was found to peak in the morning hours during all phases of solar activity. Amplitude varied the most with magnetic activity, as did occurrence to a somewhat lesser degree.

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