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

5 citations · 14 across the 8 of their papers we have counts for

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7 papers · 1 filter

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

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.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.SR2025★ 4 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★ 2 cited

Source location and evolution of a multi-lane type II radio burst

P. Zucca, P. Zhang, K. Kozarev +8

Shocks in the solar corona can accelerate electrons that in turn generate radio emission known as type II radio bursts. The characteristics and morphology of these radio bursts in…

astro-ph.SR2024★ 5 cited

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…