Periodicities of solar activity and solar radiation derived from observations and their links with the terrestrial environment
Valentina V. Zharkova, Irina Vasilieva, Simon Shepherd, Elena, Popova

TL;DR
This study analyzes various solar activity cycles, from 11-year sunspot cycles to millennial periods, using spectral analysis methods to understand their links with Earth's environment and climate variations.
Contribution
It identifies multiple solar periodicities, including a newly derived grand solar cycle of 330-380 years, using PCA and spectral analysis of observational data.
Findings
Detected 10.7-year sunspot cycle and 22-year Hale cycle.
Confirmed grand solar cycle of approximately 342-350 years.
Identified millennial cycles of 2200-2300 years in solar irradiance data.
Abstract
Solar magnetic activity is expressed via variations of sunspots and active regions varying on different timescales. The most accepted is an 11-year period supposedly induced by the electromagnetic solar dynamo mechanism. There are also some shorter or longer timescales detected: the biennial cycle (2-2.7 years), Gleisberg cycle (80-100 years), and Hallstatt's cycle (2100-2300 years). Recently, using Principal Component Analysis (PCA) of the observed solar background magnetic field (SBMF), another period of 330-380 years, or Grand Solar Cycle (GSC), was derived from the summary curve of two eigenvectors of SBMF. In this paper, a spectral analysis of the averaged sunspot numbers, solar irradiance, and the summary curve of eigenvectors of SBMF was carried out using Morlet wavelet and Fourier transforms. We detect a 10.7-year cycle from the sunspots and modulus summary curve of eigenvectors…
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Taxonomy
TopicsSolar and Space Plasma Dynamics
