Large-scale fluctuations in underground muon time series

Details Large-scale fluctuations in underground muon time series Large-scale fluctuations in underground muon time series

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989jgr....94.2667b&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 94, March 1, 1989, p. 2667-2671.

Physics

3

Cosmic Rays, Interplanetary Magnetic Fields, Muons, Solar Activity, Time Series Analysis, Least Squares Method, Perturbation Theory, Power Spectra, Random Noise, Solar Wind

Scientific paper

The self-affine properties of intensity fluctuations of underground muons generated by primary cosmic rays of rigidity greater than 1600 GV are examined. Muon time series were recorded between 1981 and 1983 at a vertical depth of 570 Hg/sq cm. The period of study includes the intense solar activity during the summer of 1982. The analysis of muon behavior is used to investigate the large-scale behavior of IMF fluctuations. The results show the fractal behavior of large-scale muon fluctuations in the range from a few hours to more than 10 days. The evolution of large time scale muon fluctuations during the 1981-1983 period is described.

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