activity
20062023
most citedCoronal heating by MHD waves

243 citations · 2k across the 75 of their papers we have counts for

collaborators

75 papers

astro-ph.SR2023

Numerical Simulations of the Decaying Transverse Oscillations in the Cool Jet

Abhishek K. Srivastava, Balveer Singh

We describe a 2.5D MHD simulation describing the evolution of cool jets triggered by initial vertical velocity perturbations in the solar chromosphere. We implement random velocity…

astro-ph.SR2023★ 9 cited

Reconnection generated plasma flows in the quasi-separatrix layer in localised solar corona

Sripan Mondal, A. K. Srivastava, Sudheer K. Mishra +8

Multiwavelength observations of the propagating disturbances (PDs), discovered by Atmospheric Imaging Assembly (AIA) onboard Solar Dynamics Observatory (SDO), are analyzed to deter…

astro-ph.SR2022★ 15 cited

Two-fluid numerical model of chromospheric heating and plasma outflows in a quiet-Sun

K. Murawski, Z. E. Musielak, S. Poedts +2

\textbf{Purpose:} This paper addresses long-standing solar physics problems, namely, the heating of the solar chromosphere and the origin of the solar wind. Our aim is to reveal th…

astro-ph.SR2022

Quasi-periodic spicule-like cool jets driven by Alfvén pulses

B. Singh, A. K. Srivastava, K. Sharma +2

We perform a 2.5 dimensional magnetohydrodynamic (MHD) simulation to understand a comprehensive view of the formation of spicule-like cool jets due to initial transverse velocity p…

astro-ph.SR2021★ 6 cited

Evolution of Kelvin-Helmholtz Instability in the Fan-Spine Topology

Sudheer K. Mishra, Balveer Singh, A. K. Srivastava +2

We use multiwavelength imaging observations from the Atmospheric Imaging Assembly (AIA) onboard the Solar Dynamics Observatory (SDO) to study the evolution of Kelvin-Helmholtz (K-H…

astro-ph.SR2021★ 145 cited

Kink oscillations of coronal loops

V. M. Nakariakov, S. A. Anfinogentov, P. Antolin +13

Kink oscillations of coronal loops, i.e., standing kink waves, is one of the most studied dynamic phenomena in the solar corona. The oscillations are excited by impulsive energy re…