Autocorrelation of Solar Activity

Details Autocorrelation of Solar Activity Autocorrelation of Solar Activity

Jun 1965

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1965natur.206.1035a&link_type=abstract

Nature, Volume 206, Issue 4988, pp. 1035-1036 (1965).

Computer Science

1

Scientific paper

IN this communication we examine the autocorrelation function R of various indexes of solar activity over time-lags,τ, of 1-200 days. Four indexes of solar activity were used: the daily relative sunspot number (Zurich), and the mean daily fluxes from Nagoya at the frequencies 1,000 Mc/s, 3,750 Mc/s and 9,400 Mc/s. The data were analysed for the years 1957-58 (more than 700 days) and for the years 1960-63 (900 days), thus comparing the highly active years of the solar cycle with the less-active years. In addition, the relative sunspot numbers for the years 1947-48 and 1937-38 were analysed for comparison.

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