activity
20202026
most citedA case-study of multi-temperature coronal jets for emerging flux MHD models

43 citations · 144 across the 19 of their papers we have counts for

collaborators

22 papers

astro-ph.SR2026

Supersonic flows observed by THEMIS related to a coronal bright point and filament

Garima Karki, Brigitte Schmieder, Ramesh Chandra +3

In this paper, we report on the dynamics of the fine structure of a solar quiescent filament observed on September 28, 2023, with the Télescope Héliographique pour l'Etude du Magné…

astro-ph.SR2026

Kinematic Relationship Between Solar Extreme Ultraviolet Waves and Type II Metric Radio Bursts

Ramesh Chandra, Apoorv Dashora, P. F. Chen +1

Solar extreme-ultraviolet (EUV) waves are large-scale disturbances that manifest as bright wavefronts, often during coronal mass ejections (CMEs). According to the magnetic field l…

astro-ph.SR2025

Partial Null Point Reconnection of an Eruptive Filament

Pooja Devi, Cristina H. Mandrini, Ramesh Chandra +4

Solar filaments are cool and dense plasma structures suspended in the solar corona against gravity. We present observations of a quiescent filament eruption that occurs on 13 July…

astro-ph.SR2025

Band Splitting in m-Type II radio Bursts and their Role in Coronal Parameter Diagnostics

Pooja Devi, Ramesh Chandra, Rositsa Miteva +2

Type II radio bursts are signatures of shock waves generated by solar eruptions, observed at radio wavelengths. While metric (m) type II bursts originate in the lower corona, their…

astro-ph.SR2025

Two Cases of Non-Radial Filament Eruption and Associated CME Deflection

Kostadinka Koleva, Ramesh Chandra, Pooja Devi +2

The purpose of this paper is to analyze the multi-wavelength and multi-instrument observations of two quiescent filament eruptions as well as the deflection of associated CMEs from…

astro-ph.SR2025

EUV Wave and Coronal Seismology

Pooja Devi, Ramesh Chandra, Arun Kumar Awasthi +2

We present an investigation of the Extreme-Ultraviolet (EUV) wave linked to the flare that occurred on 28 October 2021, along with the associated coronal loop oscillation and type…