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Time-lag of cosmic-ray intensity

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Abstract

The best correlation coefficient between the monthly cosmic-ray intensity of the Inuvik Station and various kinds of solar, interplanetary, and geophysical parameters has been found. It is calculated for different time-lags of cosmic-ray intensity with respect to these parameters. The maximum of these coefficients lead us to a useful empirical model for the 11-year cosmic-ray modulation.

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Authors and Affiliations

  1. Cosmic-Ray Group, Nuclear Physics Laboratory, University of Athens, Greece

    H. Mavromichalaki

  2. Research Centre for Astronomy and Applied Mathematics, Academy of Athens, Greece

    B. Petropoulos

Authors
  1. H. Mavromichalaki
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  2. B. Petropoulos
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Mavromichalaki, H., Petropoulos, B. Time-lag of cosmic-ray intensity. Astrophys Space Sci 106, 61–71 (1984). https://doi.org/10.1007/BF00653915

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  • DOI: https://doi.org/10.1007/BF00653915

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