The use of power spectral density as a possible new index of magnetic activity

Physics

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Geomagnetism, Magnetic Variations, Power Spectra, Kp Index, Solar Terrestrial Interactions

Scientific paper

It is argued that power spectral density is a more efficient statistic for measurement of magnetic activity than the K index. A preliminary investigation of the relationship of the power in magnetic activity fluctuations to the K index has been carried out using 1-min values of the horizontal intensity and declination at Hartland for 1989, for night-time 3-h intervals. This has shown that using values for individual intervals, the correlation between total power and K index is poor; some reasons are given for this. Over all intervals, the variation of average power with K is nearly linear and well correlated, however. It is found that the K index correlated better with low-frequency power than high-frequency power. A study of the power spectrum has shown that the spectral slope is steeper for larger values of K, and that the increase of power with K index is greater at low frequencies than high.

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