Kodaikanal Digitized White-light Data Archive (1921-2011): Analysis of various solar cycle features
Sudip Mandal, Manjunath Hegde, Tanmoy Samanta, Gopal Hazra, Dipankar, Banerjee, B Ravindra

TL;DR
This study analyzes 90 years of Kodaikanal white-light sunspot data using advanced semi-automated detection to examine solar cycle features, revealing distribution patterns, hemispheric asymmetries, and periodicities related to solar activity.
Contribution
It introduces a semi-automated sunspot detection method applied to long-term data, enabling detailed analysis of solar cycle features and hemispheric asymmetries.
Findings
Sunspot areas follow an exponential decay distribution per cycle.
Latitudinal distribution of sunspots is Gaussian centered at ~15°.
Clear evidence of Waldmeier effect correlating cycle rise time and amplitude.
Abstract
Long-term sunspot observations are key to understand and predict the solar activities and its effects on the space weather.Consistent observations which are crucial for long-term variations studies,are generally not available due to upgradation/modifications of observatories over the course of time. We present the data for a period of 90 years acquired from persistent observation at the Kodaikanal observatory in India. We use an advanced semi-automated algorithm to detect the sunspots form each calibrated white-light image. Area, longitude and latitude of each of the detected sunspots are derived. Implementation of a semi-automated method is very necessary in such studies as it minimizes the human bias in the detection procedure. Daily, monthly and yearly sunspot area variations obtained from the Kodaikanal, compared well with the Greenwich sunspot area data. We find an exponentially…
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