Cosmic Rays and Solar Coronal Emissions: Cross-Correlations of the Time Series

Details Cosmic Rays and Solar Coronal Emissions: Cross-Correlations of the Time Series Cosmic Rays and Solar Coronal Emissions: Cross-Correlations of the Time Series

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004soph..224..285m&link_type=abstract

Solar Physics, Volume 224, Issue 1-2, pp. 285-290

Physics

1

Scientific paper

The cosmic-ray (CR) time series were compared with the green 530.3 nm coronal emission line intensity over the period 1951 2003. There is a clear asymmetry in the cross-correlation between the cosmic rays and green emission corona for the even- and odd-numbered solar cycles, where a time lag is ranging between 0 and 380 days. While over the period 1954 1964 and 1978 1985 the time lag is above 200 days, over the period 1965 1976 and 1986 1995 the time lag is below 130 days. A possible reason for the lag asymmetry is discussed. The cross-correlations between the cosmic rays and Wolf sunspot number over the period 1951 2003 is also presented.

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