Temporal evolutions and quasi-periodic variations present in the sunspot number and group sunspot area data measured at Kodaikanal Observatory for solar cycles 14 to 24
Belur Ravindra, Partha Chowdhury, Pratap Chandra Ray, Kumaravel, Pichamani

TL;DR
This study analyzes long-term sunspot data from Kodaikanal Observatory, revealing hemispheric differences, multiple periodicities, and complex temporal behaviors in solar activity over more than a century.
Contribution
It provides a detailed analysis of hemispheric asymmetries and quasi-periodicities in sunspot data across solar cycles 14 to 24 using wavelet techniques.
Findings
Hemispheric differences in sunspot activity peaks.
Detection of multiple periodicities including 11-year and quasi-biennial cycles.
Hemispheric data show some dependency despite differences.
Abstract
The Kodaikanal Observatory has made synoptic observations of the Sun in white light since 1904, and these images are sketched on the Stonyhurst grids called sun charts. These continuous hand-drawn data sets are used for long-term studies of the Sun. This article investigates temporal and periodic variations of the monthly hemispheric sunspot number and sunspot group area for 1905--2016, covering solar cycles 14 to 24. We find that the temporal variations of the sunspot number and group area are different in each hemisphere and peak at different times of the solar cycle in the opposite hemisphere. For both the data sets, Cycle 19 shows maximum amplitude. For the sunspot number time series, Cycle 24 was the weakest, and Cycle 15 for the group area. The existence of double peaks and violation of the ``odd-even rule'' was found in both data sets. We have studied the periodic and…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Solar Radiation and Photovoltaics · Geophysics and Gravity Measurements
