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

4 citations · 6 across the 3 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2025

STORMY : A Real-time Triggering Framework using Yamagawa Solar Spectrograph for Active Solar Emission Observations with the MWA

Deepan Patra, Devojyoti Kansabanik, Divya Oberoi +5

Some of the most interesting insights into solar physics and space weather come from studying radio emissions associated with solar activity, which remain inherently unpredictable.…

astro-ph.SR20252 cited

Solar Observation with MeerKAT: Demonstration of Technical Readiness and Initial Science Highlight

Devojyoti Kansabanik, Marcel Gouws, Deepan Patra +6

Solar radio emissions offer unique diagnostic insights into the solar corona. However, their dynamic and multiscale nature, along with several orders of magnitude variations in int…

astro-ph.SR2025

An automated, self-calibration based pipeline for high-fidelity solar imaging with LOFAR: SIMPL

Soham Dey, Divya Oberoi, Pietro Zucca +3

The LOw Frequency ARray (LOFAR) is capable of imaging spectroscopy of the Sun in the 10-240 MHz frequency range, with high spectral, temporal, and spatial resolution. However, the…

astro-ph.SR20254 cited

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.SR2025

On Using Gradient Dynamic Spectra (GraDS) to Study Type-II Solar Radio Bursts

Puja Majee, Devojyoti Kansabanik, Divya Oberoi

Solar type-II radio bursts are coherent plasma emissions arising from magnetohydrodynamic shocks produced by either coronal mass ejections (CMEs) or flares. Type-II bursts sometime…