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Stars as Laboratories for Fundamental Physics - MPP Theory Group

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Solar Neutrinos 375<br />

Fig. 10.16. 37 Ar production rate at Homestake, integral number of sunspots,<br />

and neutron counts at McMurdo (Antarctica) which are indicative of the<br />

primary cosmic-ray proton flux above 0.4 GeV; annual bins each. In the<br />

center panel, the number of the solar cycle is also indicated. (Adapted from<br />

Bieber et al. 1990.)<br />

man rank-order correlation coefficient and Kendall’s tau (e.g. Press<br />

et al. 1986). They found a moderate statistical significance level of<br />

1.3% (Spearman) and 0.9% (Kendall) <strong>for</strong> the argon-production rate to<br />

be correlated with the sunspot index. 56<br />

Most recently, a correlation between the 1970−1991 argon production<br />

rate and the solar activity cycle w<strong>as</strong> investigated by Oakley et al.<br />

(1994). They used the Mt. Wilson 150-ft. tower magnetograms <strong>as</strong> an<br />

indicator <strong>for</strong> the solar magnetic surface flux, both <strong>for</strong> the full solar disk<br />

56 The significance level gives approximately the probability that a random shuffling<br />

of the data gives an equally good or better (anti)correlation. A significance<br />

level smaller than 1% is considered “highly significant.”

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