Some Features of the Two Sunspot Group Populations’ Properties


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Abstract

This paper describes some features of the two sunspot group populations’ properties: Large Long-living Groups, LLG, and Small Short-living, SSG (each distributed lognormally), divided by the lifetime of the group (less and strictly more than 5 days). It is shown that the relative fraction of LLG varies with the latitude from 0.45 at mid-latitudes to 0.25–0.30 at low and high latitudes. The SSG has a wider spread in latitude than the LLG. It is shown that the N-S asymmetry is an overall global process to which both the LLG and the SSG are exposed. At the same time, the asymmetry of LLG shows a slightly higher dispersion of oscillations than the asymmetry of SSG. Other properties of sunspot groups in the context of the two separate populations existence are considered.

About the authors

Yu. A. Nagovitsyn

Central Astronomical observatory of RAS at Pulkovo; State University of Aerospace Instrumentation

Author for correspondence.
Email: nag@gaoran.ru
Russian Federation, St. Petersburg; St. Petersburg

A. A. Pevtsov

Central Astronomical observatory of RAS at Pulkovo; National Solar Observatory

Email: nag@gaoran.ru
Russian Federation, St. Petersburg; Boulder, CO 80303

A. A. Osipova

Central Astronomical observatory of RAS at Pulkovo

Email: nag@gaoran.ru
Russian Federation, St. Petersburg

V. G. Ivanov

Central Astronomical observatory of RAS at Pulkovo

Email: nag@gaoran.ru
Russian Federation, St. Petersburg

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