The power spectrum of cosmic ray fluctuations and its role in discriminating the statistically significant fluctuations in detection data
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Abstract
The results of the ground-based observations of the cosmic ray intensity with scintillator telescopes, neutron supermonitors, and muon telescopes are used to calculate the spectra of cosmic ray fluctuation power on the Earth's surface in various periods of solar and geomagnetic activity. It has been shown that the reliability of calculations of the relative sampled spectral estimates is much higher when made on the basis of the calculated spectra.
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References
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