collaborators

6 papers

astro-ph.SR2025

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

Dibya Kirti Mishra, Subhamoy Chatterjee, Bibhuti Kumar Jha +6

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-al…

astro-ph.SR2025

Insights into Chromospheric Large-Scale Flows using Nobeyama 17 GHz Radio Observations I. The Differential Rotation Profile

Srinjana Routh, Anshu Kumari, Vaibhav Pant +4

Although the differential rotation rate on the solar surface has long been studied using optical and extreme ultraviolet (EUV) observations, associating these measurements to speci…

astro-ph.SR2025

Estimation of Polar Magnetic Fields using Ca II K Polar Network as a Proxy

Dibya Kirti Mishra, Bibhuti Kumar Jha, Theodosios Chatzistergos +3

The polar magnetic field plays a crucial role in the solar dynamo model and contributes to predicting future solar cycles. However, continuous and direct measurements of this polar…

astro-ph.SR2025

Ca II K Polar Network Index of the Sun: A Proxy for Historical Polar Magnetic Field

Dibya Kirti Mishra, Bibhuti Kumar Jha, Theodosios Chatzistergos +4

The Sun's polar magnetic field is pivotal in understanding solar dynamo processes and forecasting future solar cycles. However, direct measurements of the polar field is only avail…

astro-ph.SR2025

Exploring the variation in the dynamic rotation profile of the hotter solar atmosphere using mutliwavelength data

Srinjana Routh, Bibhuti Kumar Jha, Dibya Kirti Mishra +4

The global rotational profile of the solar atmosphere and its variation at different layers, although crucial for a comprehensive understanding of the dynamics of the solar magneti…

astro-ph.SR2024

Exploring the dynamic rotational profile of the hotter solar atmosphere: A multi-wavelength approach using SDO/AIA data

Srinjana Routh, Bibhuti Kumar Jha, Dibya Kirti Mishra +4

Understanding the global rotational profile of the solar atmosphere and its variation is fundamental to uncovering a comprehensive understanding of the dynamics of the solar magnet…