Abstract
A set of peculiarities of the 24-th solar activity cycle is considered on the base of the data of Kislovodsk Mountain Astronomical Station (www.solarstation.ru) as well as NASA/Marshall data. The peculiarities of the 24-th cycle are: the asymmetry between sunspot areas of northern and southern solar hemispheres; the difference between sunspot latitudes in northern and southern solar hemispheres; low activity of the first years of the cycle; large relative amount of single sunspots.
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