Physics
Scientific paper
Aug 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....9.3870m&link_type=abstract
Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int
Physics
Scientific paper
Long-term variations of galactic cosmic ray intensity and sunspot number are analyzed in the present report. It has been well known that there is a strong correlation between both data with about one year time-lag of cosmic ray intensities behind sunspot numbers. In the analysis reported at last ICRC 26-th (SH3.2.01), we have presented the relation between them is not a simple correlation with a single lag-time, but a complicated structural correlation with multiple lag-times. In the present analysis, we try to find a structure of multi-time-lag structure of cosmic ray intensities behind sunspot numbers, by using a cross correlation and cross power spectral analysis. From derived multi-lag-times in the variations, we will be able to speculate the structure of electro-magnetic state affecting galactic cosmic ray propagation in heliomagnetosphere.
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