Stochastic Properties of Solar Activity Proxies

机译：太阳能活动的随机性能

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The sunspot number (SSN), the total solar irradiance (TSI), a TSI reconstruction, and the solar flare index (SFI) are analyzed for long-range persistence. The SSN, TSI, and TSI reconstruction are almost certainly long-range persistent with most probable Hurst exponent H ≈0.7. The SFI process, however, is either very weakly persistent (H < 0.6) or completely uncorrelated.

机译：对远程持久性分析了Sunspot Number（SSN），总太阳辐照度（TSI），TSI重建和太阳闪光指数（SFI）。 SSN，TSI和TSI重建几乎肯定是远程持久性，最有可能的赫斯特指数H≈0.7。然而，SFI过程是非常弱持久（H <0.6）或完全不相关。

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《International astrophysics forum》|2012年||共6页
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Kristoffer Rypdal; Martin Rypdal;
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中图分类空间天体物理学;
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Stochastic Properties of Solar Activity Proxies

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