Temporal Distribution of Solar Cycle 24 Sunspot Groups: Comparison to Cycles 12-23
Jouni J. Takalo

TL;DR
This study compares the temporal distribution of sunspot groups in Solar Cycle 24 with previous cycles, revealing unique features such as hemispheric asymmetry, double-peak structures, and a significant decline in sunspot group areas in even cycles.
Contribution
It provides a detailed analysis of sunspot group distributions across cycles 12-24, highlighting differences between even and odd cycles and their impact on solar activity patterns.
Findings
Cycle 24 is an even cycle with low amplitude.
Double-peak structure is more pronounced in even cycles.
Significant decline in sunspot group areas occurs about four years after cycle start in even cycles.
Abstract
We analyze the temporal distribution of sunspot groups for even and odd cycles in the range SC12-SC24. It seems that cycle 24 is a characteristic even cycle, although with low amplitude. The number of large sunspot groups for cycle 24 is relatively smaller than for the average of both even and odd cycles SC12-SC23, and there is a deep decline of the large groups in the middle of the cycle. Temporal evolution of the sunspot groups of the even cycles is non-synchronous such that the northern hemisphere distribution of groups maximizes earlier that the southern hemisphere groups. This leads to a double-peak structure for the average even cycle. On the other hand, the distributions of the sunspot groups of odd cycles maximize simultaneously. We show that this double-peak structure intensifies the Gnevyshev gap (GG) for the even cycles, but is not its primary cause. On the contrary, we show…
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