Machine Learning Based Identification of Solar Disk and Plages in Kodaikanal Solar Observatory Historical Suncharts

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Main Authors: Mishra, Dibya Kirti, Chatterjee, Subhamoy, Jha, Bibhuti Kumar, Raju, Hemapriya, Priyadarshi, Aditya, Hegde, Manjunath, Routh, Srinjana, Banerjee, Dipankar, Khan, M. Saleem
Format: Preprint
Published: 2025
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author Mishra, Dibya Kirti
Chatterjee, Subhamoy
Jha, Bibhuti Kumar
Raju, Hemapriya
Priyadarshi, Aditya
Hegde, Manjunath
Routh, Srinjana
Banerjee, Dipankar
Khan, M. Saleem
author_facet Mishra, Dibya Kirti
Chatterjee, Subhamoy
Jha, Bibhuti Kumar
Raju, Hemapriya
Priyadarshi, Aditya
Hegde, Manjunath
Routh, Srinjana
Banerjee, Dipankar
Khan, M. Saleem
contents Kodaikanal Solar Observatory (KoSO) is one of the oldest solar observatories, possessing an archive of multi-wavelength solar observations, including white light, Ca II K, and H-alpha images spanning over a century. In addition to these observations, KoSO has preserved hand-drawn suncharts (1904-2022), on which various solar features such as sunspots, plages, filaments, and prominences are marked on the Stonyhurst grid with distinct colour coding. In this study, we present the first comprehensive result that includes the entire data set from these suncharts using a supervised Machine Learning model called "Convolutional Neural Networks (CNNs)", firstly to identify the solar disks from the charts (1909-2007), secondly to identify the plages, spanning 9 solar cycles (1916-2007). We train the CNN with the manually identified solar disk and plage. We first detect the solar limb and the North-South line in the suncharts, which enables the extraction of disk centre coordinates, radius, and P-angle. Following that, we use a CNN similar architecture to achieve accurate image segmentation for the identification of plages. We compare plage areas derived from the suncharts with those obtained from Ca II K full-disk observations, and find good agreement that demonstrates the potential application of such an ML technique for historical data. The results of this study further demonstrate the potential application of sunchart data to fill the existing data gaps in the KoSO multi-wavelength observations and contribute toward constructing a composite series over the last century.
format Preprint
id arxiv_https___arxiv_org_abs_2511_19040
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Machine Learning Based Identification of Solar Disk and Plages in Kodaikanal Solar Observatory Historical Suncharts
Mishra, Dibya Kirti
Chatterjee, Subhamoy
Jha, Bibhuti Kumar
Raju, Hemapriya
Priyadarshi, Aditya
Hegde, Manjunath
Routh, Srinjana
Banerjee, Dipankar
Khan, M. Saleem
Solar and Stellar Astrophysics
Kodaikanal Solar Observatory (KoSO) is one of the oldest solar observatories, possessing an archive of multi-wavelength solar observations, including white light, Ca II K, and H-alpha images spanning over a century. In addition to these observations, KoSO has preserved hand-drawn suncharts (1904-2022), on which various solar features such as sunspots, plages, filaments, and prominences are marked on the Stonyhurst grid with distinct colour coding. In this study, we present the first comprehensive result that includes the entire data set from these suncharts using a supervised Machine Learning model called "Convolutional Neural Networks (CNNs)", firstly to identify the solar disks from the charts (1909-2007), secondly to identify the plages, spanning 9 solar cycles (1916-2007). We train the CNN with the manually identified solar disk and plage. We first detect the solar limb and the North-South line in the suncharts, which enables the extraction of disk centre coordinates, radius, and P-angle. Following that, we use a CNN similar architecture to achieve accurate image segmentation for the identification of plages. We compare plage areas derived from the suncharts with those obtained from Ca II K full-disk observations, and find good agreement that demonstrates the potential application of such an ML technique for historical data. The results of this study further demonstrate the potential application of sunchart data to fill the existing data gaps in the KoSO multi-wavelength observations and contribute toward constructing a composite series over the last century.
title Machine Learning Based Identification of Solar Disk and Plages in Kodaikanal Solar Observatory Historical Suncharts
topic Solar and Stellar Astrophysics
url https://arxiv.org/abs/2511.19040