collaborators

6 papers

astro-ph.SR2026

Microwave Polar Brightening and Its Connection to Polar Coronal Holes

Rohan Bose, Anshu Kumari, Vaibhav Pant +3

Polar brightening (PB) observed at microwave frequencies serves as an important probe to study the thermal and magnetic properties in the Sun's polar regions. Building on earlier s…

astro-ph.SR2026

Radio Signature of Higher Atmospheric Meridional Flow and Implications for Magnetic Trees in the Sun

Srinjana Routh, Anshu Kumari, Rohan Bose +4

The coupling between plasma flows and magnetic fields in the solar atmosphere governs the transport of angular momentum and the redistribution of magnetic flux, yet its manifestati…

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

Polar Filaments Capture High Latitude Solar Poloidal Field Interactions and can Foretell the Future Sunspot Cycle Amplitude before Polar Field Precursors

Srinjana Routh, Shaonwita Pal, Dibyendu Nandy +3

Polar fields at the minimum of a sunspot cycle -- which are a manifestation of the radial component of the Sun's poloidal field -- are deemed to be the best indicator of the streng…

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

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…