Butterfly Diagram and Other Properties of Plage Areas from Kodaikanal Ca ii K Photographs Covering 1904 – 2007

Ca ii K observations of the Sun have a great potential for probing the Sun's magnetism and activity, as well as for reconstructing solar irradiance. The Kodaikanal Solar Observatory (KoSO) in India, houses one of the most prominent Ca ii K archives, spanning from 1904 to 2007, obtained under the same experimental conditions over a century, a feat very few other sites have achieved. However, the KoSO Ca ii K archive suffers from several inconsistencies (e.g., missing/incorrect timestamps of observations and orientation of some images) which have limited the use of the archive. This study is a step towards bringing the KoSO archive to its full potential. We did this by developing an automatic method to orient the images more accurately than in previous studies. Furthermore, we included more data than in earlier studies (considering images that could not previously be analyzed by other techniques, as well as 2845 newly digitized images), while also accounting for mistakes in the observational date/time. These images were accurately processed to identify plage regions along with their locations, enabling us to construct the butterfly diagram of plage areas from the entire KoSO Ca ii K archive covering 1904 - 2007. Our butterfly diagram shows significantly fewer data gaps compared to earlier versions due to the larger set of data used in this study. Moreover, our butterfly diagram is consistent with Spörer's law for sunspots, validating our automatic image orientation method. Additionally, we found that the mean latitude of plage areas calculated over the entire period is <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mn>20.5</mml:mn> <mml:mi>%</mml:mi> <mml:mo>±</mml:mo> <mml:mn>2.0</mml:mn></mml:math> higher than that of sunspots, irrespective of the phase or the strength of the solar cycle. We also studied the north-south asymmetry showing that the northern hemisphere dominated plage areas during solar cycles 19 and 20, while the southern hemisphere dominated during Solar Cycles 21 - 23.

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Journal
Solar Physics
Published
2024-12-01
DOI
https://doi.org/10.1007/s11207-024-02408-6
Citations
3
Primary Topic
Solar and Space Plasma Dynamics
Type
article
Field-Weighted Citation Impact
0.99

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article

Butterfly Diagram and Other Properties of Plage Areas from Kodaikanal Ca ii K Photographs Covering 1904 – 2007

I. Ermolli, Dipankar Banerjee, S. K. Solanki, Theodosios Chatzistergos et al.
3 citations
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article

Butterfly Diagram and Other Properties of Plage Areas from Kodaikanal Ca ii K Photographs Covering 1904 – 2007

I. Ermolli, Dipankar Banerjee, S. K. Solanki, Theodosios Chatzistergos, Aditya Priyadarshi, Bibhuti Kumar Jha, N. A. Krivova
article en
3 citations

Abstract

Ca ii K observations of the Sun have a great potential for probing the Sun's magnetism and activity, as well as for reconstructing solar irradiance. The Kodaikanal Solar Observatory (KoSO) in India, houses one of the most prominent Ca ii K archives, spanning from 1904 to 2007, obtained under the same experimental conditions over a century, a feat very few other sites have achieved. However, the KoSO Ca ii K archive suffers from several inconsistencies (e.g., missing/incorrect timestamps of observations and orientation of some images) which have limited the use of the archive. This study is a step towards bringing the KoSO archive to its full potential. We did this by developing an automatic method to orient the images more accurately than in previous studies. Furthermore, we included more data than in earlier studies (considering images that could not previously be analyzed by other techniques, as well as 2845 newly digitized images), while also accounting for mistakes in the observational date/time. These images were accurately processed to identify plage regions along with their locations, enabling us to construct the butterfly diagram of plage areas from the entire KoSO Ca ii K archive covering 1904 - 2007. Our butterfly diagram shows significantly fewer data gaps compared to earlier versions due to the larger set of data used in this study. Moreover, our butterfly diagram is consistent with Spörer's law for sunspots, validating our automatic image orientation method. Additionally, we found that the mean latitude of plage areas calculated over the entire period is <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mn>20.5</mml:mn> <mml:mi>%</mml:mi> <mml:mo>±</mml:mo> <mml:mn>2.0</mml:mn></mml:math> higher than that of sunspots, irrespective of the phase or the strength of the solar cycle. We also studied the north-south asymmetry showing that the northern hemisphere dominated plage areas during solar cycles 19 and 20, while the southern hemisphere dominated during Solar Cycles 21 - 23.

Solar PhysicsVol. 299(12)
Indian Institute of Science Education and Research Kolkata (IN), Southwest Research Institute (US), Indian Institute of Astrophysics (IN), Astronomical Observatory of Rome (IT), Aryabhatta Research Institute of Observational Sciences (IN), Max Planck Institute for Solar System Research (DE), National Institute for Astrophysics (IT)
National Aeronautics and Space Administration, H2020 European Research Council
Openalex Percentile: Top 22%
Solar and Space Plasma Dynamics
0.99
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