Aditya Priyadarshi
Current Organizations / Institutes
The organizations/institutes from the scholar's latest article
Previous Organizations / Institutes
The organizations / institutes from the scholar's other articles in the past ten years
Research Subjects
Research Interests
Aditya Priyadarshi has a total of 20 co-authors. Here are the top co-authors by number of shared publications:
- Dipankar Banerjee
Indian Institute of Space Science and Technology
5 shared publications - Bibhuti Kumar Jha
Southwest Research Institute, Boulder, CO 80302, USA
4 shared publications - Manjunath Hegde
Indian Institute of Astrophysics
3 shared publications - Subhamoy Chatterjee
Southwest Research Institute, Boulder, CO 80302, USA
3 shared publications - Dibya Kirti Mishra
Aryabhatta Research Institute of Observational Sciences
2 shared publications M. Saleem Khan
Department of Applied Physics, Mahatma Jyotiba Phule Rohilkhand University, Bareilly-243006, Uttar Pradesh, India
2 shared publications
Latest Publications
- Open Access
- 20 February 2026
- Published by American Astronomical Society in The Astrophysical Journal Supplement Series
- Vol. 283 (1) , 19
Machine Learning–based Identification of the Solar Disk and Plages in Kodaikanal Solar Observatory Historical Suncharts
Kodaikanal Solar Observatory (KoSO) is one of the oldest solar observatories, possessing an archive of multiwavelength solar observations, including white light, Ca ii K, and H α 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 color coding. In this study, we present the first comprehensive result that includes the entire dataset from these suncharts using a supervised machine learning (ML) model called “convolutional neural networks” (CNNs), first to identify the solar disks from the charts (1909–2007) and second to identify the plages, spanning nine solar cycles (1916–2007). We train the CNN with the manually identified solar disk and plages. We first detect the solar limb and the north–south line in the suncharts, which enables the extraction of disk center 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 multiwavelength observations and contribute toward constructing a composite series over the last century.
- 20 February 2026
- Published by American Astronomical Society in The Astrophysical Journal Supplement Series
- Vol. 283 (1) , 19
Open AccessMachine Learning–based Identification of the Solar Disk and Plages in Kodaikanal Solar Observatory Historical Suncharts
Kodaikanal Solar Observatory (KoSO) is one of the oldest solar observatories, possessing an archive of multiwavelength solar observations, including white light, Ca ii K, and H α 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 color coding. In this study, we present the first comprehensive result that includes the entire dataset from these suncharts using a supervised machine learning (ML) model called “convolutional neural networks” (CNNs), first to identify the solar disks from the charts (1909–2007) and second to identify the plages, spanning nine solar cycles (1916–2007). We train the CNN with the manually identified solar disk and plages. We first detect the solar limb and the north–south line in the suncharts, which enables the extraction of disk center 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 multiwavelength observations and contribute toward constructing a composite series over the last century.
- Open Access
Machine Learning Based Identification of Solar Disk and Plages in Kodaikanal Solar Observatory Historical Suncharts
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.
Open AccessMachine Learning Based Identification of Solar Disk and Plages in Kodaikanal Solar Observatory Historical Suncharts
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.
- Open Access
- 13 December 2024
- Published by Springer Nature in Solar Physics
- Vol. 299 (12) , 1-22
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 $20.5\%\pm 2.0$ 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.- 13 December 2024
- Published by Springer Nature in Solar Physics
- Vol. 299 (12) , 1-22
Open AccessButterfly 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 $20.5\%\pm 2.0$ 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. - Open Access
- 1 February 2023
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 943 (2) , 140
Detection of Solar Filaments Using Suncharts from Kodaikanal Solar Observatory Archive Employing a Clustering Approach
With over 100 yr of solar observations, the Kodaikanal Solar Observatory (KoSO) is a one-of-a-kind solar data repository in the world. Among its many data catalogs, the “suncharts” at KoSO are of particular interest. These suncharts (1904–2020) are colored drawings of different solar features, such as sunspots, plages, filaments, and prominences, made on papers with a Stonyhurst latitude–longitude grid etched on them. In this paper, we analyze this unique data by first digitizing each sunchart using an industry-standard scanner and saving those digital images in a high-resolution “.tif” format. We then examine cycle 19 and cycle 20 data (two of the strongest cycles of the last century) with the aim of detecting filaments. To this end, we employed the “K-means clustering” method, and obtained different filament parameters such as position, tilt angle, length, and area. Our results show that filament length (and area) increases with latitude and the poleward migration is clearly dominated by a particular tilt sign. Lastly, we cross verified our findings with results from KoSO digitized photographic plate database for the overlapping time period and obtained a good agreement between them. This work, acting as a proof-of-the-concept, will kickstart new efforts to effectively use the entire hand-drawn series of multifeature, full-disk solar data and enable researchers to extract new sciences, such as the generation of pseudomagnetograms for the last 100 yr.
- 1 February 2023
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 943 (2) , 140
Open AccessDetection of Solar Filaments Using Suncharts from Kodaikanal Solar Observatory Archive Employing a Clustering Approach
With over 100 yr of solar observations, the Kodaikanal Solar Observatory (KoSO) is a one-of-a-kind solar data repository in the world. Among its many data catalogs, the “suncharts” at KoSO are of particular interest. These suncharts (1904–2020) are colored drawings of different solar features, such as sunspots, plages, filaments, and prominences, made on papers with a Stonyhurst latitude–longitude grid etched on them. In this paper, we analyze this unique data by first digitizing each sunchart using an industry-standard scanner and saving those digital images in a high-resolution “.tif” format. We then examine cycle 19 and cycle 20 data (two of the strongest cycles of the last century) with the aim of detecting filaments. To this end, we employed the “K-means clustering” method, and obtained different filament parameters such as position, tilt angle, length, and area. Our results show that filament length (and area) increases with latitude and the poleward migration is clearly dominated by a particular tilt sign. Lastly, we cross verified our findings with results from KoSO digitized photographic plate database for the overlapping time period and obtained a good agreement between them. This work, acting as a proof-of-the-concept, will kickstart new efforts to effectively use the entire hand-drawn series of multifeature, full-disk solar data and enable researchers to extract new sciences, such as the generation of pseudomagnetograms for the last 100 yr.
- 10 January 2022
- Published by Institute of Electrical and Electronics Engineers (IEEE)
- p. 1-6
An ML-based Citizen-Driven Traffic Violation Reporting Android App
As violations in the city are on the rise, we bring out a citizen-driven application to allow them to take responsibility for being a lawful Samaritan was the need of the hour. The Bangalore city Traffic Police has released an application ‘Public Eye’ which only partially serves this purpose. In this project, we attempt to contribute to this good initiative by enhancing the User Experience and adding the power of Machine Learning and Artificial Intelligence to simplify violation detection, while addressing privacy concerns. In our work, we have explored state-of-the-art models available for the task of detection and recognition in images. After studying the needs of users meticulously, we built an effective and meaningful User Experience in the App. The strengths of this App are its ease of use, flexibility, and privacy amongst others for an effective traffic violation reporting. Our approach to gamifying the experience will attract more users to take responsibility of being law abiding citizen. The efficacy of its usage is validated through volunteers.
- 10 January 2022
- Published by Institute of Electrical and Electronics Engineers (IEEE)
- p. 1-6
An ML-based Citizen-Driven Traffic Violation Reporting Android App
As violations in the city are on the rise, we bring out a citizen-driven application to allow them to take responsibility for being a lawful Samaritan was the need of the hour. The Bangalore city Traffic Police has released an application ‘Public Eye’ which only partially serves this purpose. In this project, we attempt to contribute to this good initiative by enhancing the User Experience and adding the power of Machine Learning and Artificial Intelligence to simplify violation detection, while addressing privacy concerns. In our work, we have explored state-of-the-art models available for the task of detection and recognition in images. After studying the needs of users meticulously, we built an effective and meaningful User Experience in the App. The strengths of this App are its ease of use, flexibility, and privacy amongst others for an effective traffic violation reporting. Our approach to gamifying the experience will attract more users to take responsibility of being law abiding citizen. The efficacy of its usage is validated through volunteers.
- 28 January 2021
- Published by Springer Nature in Solar Physics
- Vol. 296 (1) , 1-14
Measurements of Solar Differential Rotation Using the Century Long Kodaikanal Sunspot Data
- 28 January 2021
- Published by Springer Nature in Solar Physics
- Vol. 296 (1) , 1-14
Measurements of Solar Differential Rotation Using the Century Long Kodaikanal Sunspot Data