activity
20242026
collaborators

6 papers

astro-ph.SR2026

Visualizing the Magnetic Structure in Interplanetary Coronal Mass Ejections with ATHARV

Vivek Menon, Jyoti Sheoran, Vaibhav Pant +1

Interplanetary coronal mass ejections (ICMEs) are major drivers of space weather, and their geoeffectiveness is strongly governed by the structure and orientation of their internal…

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.SR2025

The effect of poloidal magnetic field and helicity injection on a breakout CME

Nitin Vashishtha, Vaibhav Pant, Dana-Camelia Talpeanu +2

Coronal mass ejections (CMEs), as crucial drivers of space weather, necessitate a comprehensive understanding of their initiation and evolution in the solar corona, in order to bet…

astro-ph.SR2025

Insights into Chromospheric Large-Scale Flows using Nobeyama 17 GHz Radio Observations I. The Differential Rotation Profile

Srinjana Routh, Anshu Kumari, Vaibhav Pant +4

Although the differential rotation rate on the solar surface has long been studied using optical and extreme ultraviolet (EUV) observations, associating these measurements to speci…

astro-ph.SR2025

Exploring the variation in the dynamic rotation profile of the hotter solar atmosphere using mutliwavelength data

Srinjana Routh, Bibhuti Kumar Jha, Dibya Kirti Mishra +4

The global rotational profile of the solar atmosphere and its variation at different layers, although crucial for a comprehensive understanding of the dynamics of the solar magneti…

astro-ph.SR2024

Transition Region Brightenings in a Moss Region and their Relation with Lower Atmospheric Dynamics

Bhinva Ram, Tanmoy Samanta, Yajie Chen +5

Small-scale Brightenings (SBs) are commonly observed in the transition region that separates the solar chromosphere from the corona. These brightenings, omnipresent in active regio…