collaborators

12 papers

astro-ph.SR2026

A high-frequency type II radio burst associated with an X2.3 class flare

Divya Paliwal, Anshu Kumari, Vishwa Vijay Singh +3

Radio observations provide a powerful diagnostic of the solar corona, enabling investigations of dynamic phenomena associated with solar flares, coronal mass ejections (CMEs), and…

astro-ph.SR2026

Multi-lane type II radio bursts: Insights into shock propagation in the corona

Nadiya K., Divya Paliwal, Anshu Kumari

Type II solar radio bursts are considered as the signatures of the coronal shocks. These bursts are generated from plasma waves excited by magnetohydrodynamic (MHD) shocks, and the…

astro-ph.IM2026

RAISE: A Low-Frequency Space-Based Payload for Solar Radio and RFI Measurements on the SMiLE Mission

Sangeetha A, Harsha Avinash Tanti, Abhirup Datta +2

We present the Radio-wave Apparatus for Investigating Solar & Earth interference (RAISE), a compact low-frequency radio payload proposed for hosting on the SMiLE mission. Operating…

astro-ph.SR2026

Role of SKA in Advancing Remote Measurements of Magnetic Fields of Solar Coronal Mass Ejections

Devojyoti Kansabanik, Surajit Mondal, Shaheda Begum Shaik +13

Coronal Mass Ejections (CMEs) are large expulsions of magnetized plasma from the Sun into interplanetary space and are the primary drivers of extreme space weather variations. The…

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

Radio Wave Propagation as a Probe of the Solar Corona and Solar Wind

K. Sasikumar Raja, Prasad Subramanian, Susanta Kumar Bisoi +3

Radio waves propagating through an inhomogeneous, turbulent medium such as the solar corona and solar wind become distorted, causing the initially plane wavefronts becomes corrugat…

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.SR2026

Solar energetic particles and their association with radio emissions

Diana E. Morosan, Anshu Kumari, Immanuel Jebaraj +6

Energetic particle populations are ubiquitous throughout the Universe. In our solar system, the most prominent sources of energetic particles are solar flares or collisionless shoc…

astro-ph.SR2026

Probing the Solar Corona and the Solar Wind Using Angular Broadening Observations with the SKA

Peijin Zhang, John Morgan, Divya Oberoi +9

Angular broadening observations of compact radio sources provide a powerful method for probing the solar corona and solar wind. Such observations enable studies of the phase struct…

astro-ph.SR2026

Solar Radio Bursts in the metric to kilometric range

Anshu Kumari, Mugundhan V., Diana E. Morosan +6

Solar radio bursts (SRBs) are intense emissions observed in radio wavelengths most frequently during solar transients, such as coronal mass ejections (CMEs) and flares. SRBs are di…

astro-ph.IM2021

Solar Radio Spectro-polarimetry (50-500 MHz) : Design and Development of Cross-Polarized Log-Periodic Dipole antenna and configuration of receiver system

Anshu Kumari, G. V. S. Gireesh, C. Kathiravan +2

A radio spectro-polarimeter was developed at the Gauribidanur radio observatory to study the characteristics of the polarized radio waves that are emitted by the impetuous solar co…