activity
20182026
most citedOn the observations of rapid forced reconnection in the solar corona

45 citations · 140 across the 16 of their papers we have counts for

collaborators

17 papers

astro-ph.SR2026

Dynamical and thermal evolution of localized reconnecting current sheets under varying guide-fields in the solar corona

Saksham Pande, Abhishekh Kumar Srivastava, Fabio Bacchini +9

Although magnetic reconnection in coronal current sheets (CSs) is a fundamental energy release mechanism in the solar corona, the role of guide-fields in governing its formation an…

astro-ph.SR2026

Recurrent Coronal Jets and QPPs: Periodic Reconnection and Localized Heating Across Quiet-Sun to Active Regions

Sudheer K. Mishra, Kartika Sangal, Balveer Singh +3

We analyze quasi-periodic pulsations (QPPs) in recurrent coronal jets driven by periodic magnetic reconnection associated with successive flux emergence in the fan-spine magnetic t…

astro-ph.SR2025

Localized Heating and Dynamics of the Solar Corona due to a Symbiosis of Waves and Reconnection

A. K. Srivastava, Sripan Mondal, Eric R. Priest +6

The Sun's outer atmosphere, the corona, is maintained at mega-Kelvin temperatures and fills the heliosphere with a supersonic outflowing wind. The dissipation of magnetic waves and…

astro-ph.SR2025

Formation of Jet-driven Forced Reconnection Region and Associated Plasma Blobs in a Prominence Segment

Sudheer K. Mishra, A. K. Srivastava, S. P. Rajaguru +1

We use data from the Atmospheric Imaging Assembly (AIA) onboard the Solar Dynamics Observatory (SDO) to study the most likely formation of a forced reconnection region and associat…

astro-ph.SR2024

Deciphering the Evolution of Thermodynamic Properties and their Connection to the Global Kinematics of High-Speed Coronal Mass Ejections Using FRIS Model

Soumyaranjan Khuntia, Wageesh Mishra, Yuming Wang +3

Most earlier studies have been limited to estimating the kinematic evolution of coronal mass ejections (CMEs), and only limited efforts have been made to investigate their thermody…

astro-ph.SR2024

Alfvén Pulse Driven Spicule-like Jets in the Presence of Thermal Conduction and Ion-Neutral Collision in Two-Fluid Regime

A. K. Srivastava, Anshika Singh, Balveer Singh +6

We present the formation of quasi-periodic cool spicule-like jets in the solar atmosphere using 2.5-D numerical simulation in two-fluid regime (ions+neutrals) under the presence of…

astro-ph.SR2023

Unraveling the Thermodynamic Enigma between Fast and Slow Coronal Mass Ejections

Soumyaranjan Khuntia, Wageesh Mishra, Sudheer K Mishra +3

Coronal Mass Ejections (CMEs) are the most energetic expulsions of magnetized plasma from the Sun that play a crucial role in space weather dynamics. This study investigates the di…

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.SR2023★ 15 cited

Origin of Quasi-Periodic Pulsation at the Base of Kink Unstable Jet

Sudheer K. Mishra, Kartika Sangal, Pradeep Kayshap +3

We study a blowout jet that occurs at the west limb of the Sun on August 29, 2014 using high-resolution imaging/spectroscopic observations provided by SDO/AIA and IRIS. An i…

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

The prominence driven forced reconnection in the solar corona and associated plasma dynamics

A. K. Srivastava, Sudheer K. Mishra, P. Jelínek

Using the multi-temperature observations from SDO/AIA on 30th December 2019, we provide a signature of prominence driven forced magnetic reconnection in the corona and associated p…

astro-ph.SR2020★ 10 cited

Large-Scale Vortex Motion and Multiple Plasmoid Ejection Due to Twisting Prominence Threads and Associated Reconnection

Sudheer K. Mishra, Abhishek K. Srivastava, P. F. Chen

We analyze the characteristics of a quiescent polar prominence using the Atmospheric Imaging Assembly (AIA) onboard the Solar Dynamics Observatory (SDO). Initially, small-scale bar…

astro-ph.SR2019★ 15 cited

Linkage of Geoeffective Stealth CMEs Associated with the Eruption of Coronal Plasma channel and Jet-Like Structure

Sudheer K. Mishra, A. K. Srivastava

We analyze the eruption of a coronal plasma channel (CPC) and an overlying flux rope using \textit{Atmospheric Imaging Assembly/Solar Dynamic Observatory} (AIA/SDO) and \textit{Sol…

astro-ph.SR2019★ 15 cited

The Evolution of Magnetic Rayleigh-Taylor Unstable Plumes and Hybrid KH-RT Instability into A Loop-like Eruptive Prominence

Sudheer K. Mishra, A. K. Srivastava

MRT unstable plumes are observed in a loop-like eruptive prominence using SDO/AIA observations. The small-scale cavities are developed within the prominence, where perturbations tr…

astro-ph.SR2019★ 45 cited

On the observations of rapid forced reconnection in the solar corona

A. K. Srivastava, Sudheer K. Mishra, P. Jelínek +7

Using multiwavelength imaging observations from the Atmospheric Imaging Assembly (AIA) onboard the Solar Dynamics Observatory (SDO) on 03 May 2012, we present a novel physical scen…

astro-ph.SR2018★ 1 cited

Propagation of MRT Unstable Plasma Spikes in the Inter-planetary Space

S. K. Mishra, Talwinder Singh, P. Kayshap +1

We have used the Coronagraphic and Heliospheric Imaging data from Solar TErrestrial RElations Observatory (STEREO) to observe a prominence which is erupted on June 7th, 2011. This…

astro-ph.SR2018★ 24 cited

Evolution of Magnetic Rayleigh-Taylor Instability into the Outer Solar Corona and Low Inter Planetary Space

Sudheer K. Mishra, Talwinder Singh, P. Kayshap +1

We analyze the observations from Solar TErrestrial RElations Observatory (STEREO)-A\&B/COR-1 of an eruptive prominence in the intermediate corona on 7 June 2011 at 08:45 UT, which…