activity
20242026
collaborators

7 papers

astro-ph.SR2026

Coronal Magnetography using Spectropolarimetry with SKA Telescopes

Deepan Patra, Puja Majee, Soham Dey +6

The solar coronal magnetic field drives nearly every aspect of solar phenomena and activity -- from flares, coronal mass ejections, and solar wind that governs space weather to the…

astro-ph.SR2026

State-of-the-art Observation, Calibration, and Imaging Framework for Solar and Heliospheric Sciences with SKA

Divya Oberoi, Devojyoti Kansabanik, Soham Dey +6

The Sun is a surprisingly difficult radio source to observe and image, even with the SKA. It is multiple orders brighter than the typical radio sources, which sensitive radio teles…

astro-ph.SR2025

First Robust Detection of Linear Polarization from Metric Solar Emissions: Challenging Established Paradigms

Soham Dey, Devojyoti Kansabanik, Divya Oberoi +1

Polarimetric radio observations of the Sun can provide rich information about emission mechanisms and the propagation medium. For the past five decades, solar polarimetric studies…

astro-ph.SR2025

Observation and Modeling of Small Spatial Structures of Solar Radio Noise Storms using the uGMRT

Surajit Mondal, Peijin Zhang, Devojyoti Kansabanik +2

One of the most commonly observed solar radio sources in the metric and decametric wavelengths is the solar noise storm. These are generally associated with active regions and are…

astro-ph.IM2025

A Formalism for Calibrating the Instrumental Polarization of Radio Interferometric Arrays at Meter Wavelengths using Unpolarized Sky: A Demonstration using the MWA Observations

Devojyoti Kansabanik, Angelos Vourlidas, Soham Dey +2

Calibration of instrumental polarization is critical for measuring polarized radio emissions from astrophysical sources to extract the magnetic field information in astrophysical,…

astro-ph.SR2024

New Insights into Type-I Solar Noise Storms from High Angular Resolution Spectroscopic Imaging with the Upgraded Giant Metrewave Radio Telescope

Surajit Mondal, Devojyoti Kansabanik, Divya Oberoi +1

Type-I solar noise storms are perhaps the most commonly observed active radio emissions from the Sun at meter-wavelengths. Noise storms have a long-lived and wideband continuum bac…