activity
20142026
most citedEstimating solar flux density at low radio frequencies using a sky brightness model

36 citations · 186 across the 24 of their papers we have counts for

collaborators

25 papers

astro-ph.SR2026

Simulating Ionospheric Distortions in Mock SKA-Low Solar Radio Observations

Rohit Sharma, Mitin

The Square Kilometre Array Observatory (SKAO) will provide unprecedented angular resolution for low-frequency solar radio imaging, enabling access to fine-scale coronal structures.…

astro-ph.IM2026

Radio Galaxies detection and characterization using deep learning techniques

Sanjay Khatik, Rohit Sharma, Pankaj Jain

Future radio telescopes will generate data volumes that are increasingly difficult to analyse using traditional statistical methods, motivating the adoption of machine-learning tec…

astro-ph.SR2026

Probing the Physics of the Solar Corona with High-Resolution Observations using SKA-Mid

Mark C. M. Cheung, John S. Morgan, Rohit Sharma +3

We examine the capability of the SKA-Mid telescope for probing solar coronal structure and evolution. Using radiative magnetohydrodynamics simulations of a solar flare, we synthesi…

astro-ph.SR2026

Solar, Heliospheric and Ionospheric Physics: Pathfinders, Precursors and SKAO Perspective

Pietro Zucca, Rohit Sharma, Divya Oberoi +5

The Solar, Heliospheric and Ionospheric (SHI) Physics Science Working Group of the Square Kilometre Array Observatory (SKAO) addresses the full chain of plasma processes linking th…

astro-ph.IM2026

Advancing Astrophysics with the SKA II

Anna Bonaldi, Tyler L. Bourke, Philippa Hartley +45

Advancing Astrophysics with the SKA II (AASKAII), written by our science community, outlines the transformative scientific advances that will be enabled by the SKA telescopes. In t…

astro-ph.SR2026

Unravelling the nonthermal emissions from the quiet solar corona with the SKA

Surajit Mondal, Divya Oberoi, Rohit Sharma +4

Investigation of the nonthermal emissions from the quiet solar corona has been rather limited. This primarily stems from the fact that the emission is expected to be quite weak and…

astro-ph.SR2026

Radio Diagnostics of Particle Acceleration in Solar Flares with SKAO Observations

Rohit Sharma, Marina Battaglia, Sijie Yu +3

Particle acceleration is a fundamental astrophysical process occurring across diverse systems and scales, producing electromagnetic emission across all wavelengths. Radio bursts fr…

astro-ph.IM2025

Karabo: A versatile SKA Observation Simulation Framework

Rohit Sharma, Simon Felix, Luis Fernando Machado Poletti Valle +12

Karabo is a versatile Python-based software framework simplifying research with radio astronomy data. It bundles existing software packages into a coherent whole to improve the eas…

astro-ph.CO2024★ 5 cited

Deep learning approach for identification of HII regions during reionization in 21-cm observations -- III. image recovery

Michele Bianco, Sambit. K. Giri, Rohit Sharma +7

The low-frequency component of the upcoming Square Kilometre Array Observatory (SKA-Low) will be sensitive enough to construct 3D tomographic images of the 21-cm signal distributio…

astro-ph.SR2024

Study of Particle Acceleration using Fine Structures and Oscillations in Microwaves from Electron Cyclotron Maser

Rohit Sharma, Marina Battaglia, Sijie Yu +3

The accelerated electrons during solar flares produce radio bursts and nonthermal X-ray signatures. The quasi-periodic pulsations (QPPs) and fine structures in spatial-spectral-tem…

astro-ph.SR2023

Detection of long-lasting aurora-like radio emission above a sunspot

Sijie Yu, Bin Chen, Rohit Sharma +5

Auroral radio emissions in planetary magnetospheres typically feature highly polarized, intense radio bursts, usually attributed to electron cyclotron maser (ECM) emission from ene…

astro-ph.IM2023★ 3 cited

Magnetic Energy Powers the Corona: How We Can Understand its 3D Storage & Release

Amir Caspi, Daniel B. Seaton, Roberto Casini +12

The coronal magnetic field is the prime driver behind many as-yet unsolved mysteries: solar eruptions, coronal heating, and the solar wind, to name a few. It is, however, still poo…

astro-ph.SR2022★ 9 cited

Multiple Regions of Nonthermal Quasi-Periodic Pulsations during the Impulsive Phase of a Solar Flare

Yingjie Luo, Bin Chen, Sijie Yu +2

Flare-associated quasiperiodic pulsations (QPPs) in radio and X-ray wavelengths, particularly those related to nonthermal electrons, contain important information about the energy…

astro-ph.IM2022★ 6 cited

Preparing for Solar and Heliospheric Science with the SKAO: An Indian Perspective

Divya Oberoi, Susanta Kumar Bisoi, K. Sasikumar Raja +4

The Square Kilometre Array Observatory (SKAO) is perhaps the most ambitious radio telescope envisaged yet. It will enable unprecedented studies of the Sun, the corona and the helio…

astro-ph.SR2022★ 13 cited

Detection of weak ubiquitous impulsive nonthermal emissions from the solar corona

Rohit Sharma, Divya Oberoi, Marina Battaglia +1

A ubiquitous presence of weak energy releases is one of the most promising hypotheses to explain coronal heating, referred to as the nanoflare hypothesis. The accelerated electrons…

astro-ph.SR2021★ 10 cited

Multiple electron acceleration instances during a series of solar microflares observed simultaneously at X-rays and microwaves

Marina Battaglia, Rohit Sharma, Yingjie Luo +3

Even small solar flares can display a surprising level of complexity regarding their morphology and temporal evolution. Many of their properties, such as energy release and electro…

astro-ph.SR2020

Study of the spatial association between an active region jet and a nonthermal type~ radio burst

Sargam M. Mulay, Rohit Sharma, Gherardo Valori +4

We aim to investigate the spatial location of the source of an active region (AR) jet and its relation with associated nonthermal type~III radio emission. An emission measure (EM)…

astro-ph.SR2020★ 12 cited

Radio and X-ray Observations of Short-lived Episodes of Electron Acceleration in a Solar Microflare

Rohit Sharma, Marina Battaglia, Yingjie Luo +2

Solar flares are sudden energy release events in the solar corona, resulting from magnetic reconnection, that accelerates particles and heats the ambient plasma. During a flare, th…

astro-ph.SR2020★ 23 cited

Propagation Effects in Quiet Sun Observations at Meter Wavelengths

Rohit Sharma, Divya Oberoi

Quiet sun meterwave emission arises from thermal bremsstrahlung in the MK corona, and can potentially be a rich source of coronal diagnostics. On its way to the observer, it gets m…

astro-ph.SR2017★ 25 cited

Quantifying weak non-thermal solar radio emission at low radio frequencies

Rohit Sharma, Divya Oberoi, Mihir Arjunwadkar

The recent availability of fine grained high sensitivity data from the new generation low radio frequency instruments such as the Murchison Widefield Array (MWA) have opened up opp…

astro-ph.IM2017★ 36 cited

Estimating solar flux density at low radio frequencies using a sky brightness model

Divya Oberoi, Rohit Sharma, Alan E. E. Rogers

Sky models have been used in the past to calibrate individual low radio frequency telescopes. Here we generalize this approach from a single antenna to a two element interferometer…

astro-ph.SR2016★ 29 cited

Wavelet-Based Characterization of Small-Scale Solar Emission Features at Low Radio Frequencies

Akshay Suresh, Rohit Sharma, Divya Oberoi +36

Low radio frequency solar observations using the Murchison Widefield Array have recently revealed the presence of numerous weak, short-lived and narrow-band emission features, even…

physics.plasm-ph2016★ 6 cited

On the energisation of charged particles by fast magnetic reconnection

Rohit Sharma, Dhrubaditya Mitra, Divya Oberoi

We study the role of turbulence in magnetic reconnection, within the framework of magneto-hydrodynamics, using three-dimensional direct numerical simulations. For small turbulent i…

astro-ph.SR2016★ 7 cited

On the Bright Loop Top Emission in Post Eruption Arcades

Rohit Sharma, Durgesh Tripathi, Hiroaki Isobe +1

The observations of post eruption arcades (PEAs) in X-rays and EUV reveal strong localised brightenings at the loop top regions. The origin of these brightenings and their dynamics…