activity
20062020
most citedMagnetohydrodynamic Simulation of Magnetic Null-point Reconnections and Coronal dimmings during the X2.1 flare in NOAA AR 11283

44 citations · 130 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2020★ 15 cited

Magnetic reconnections in the presence of three-dimensional magnetic nulls and quasi-separatrix layers

Sanjay Kumar, Sushree S. Nayak, Avijeet Prasad +1

Three-dimensional (3D) magnetohydrodynamic simulations are carried out to explore magnetic reconnections in the presence of 3D magnetic nulls and quasi-separatrix layers (QSLs). Th…

astro-ph.SR2020★ 44 cited

Magnetohydrodynamic Simulation of Magnetic Null-point Reconnections and Coronal dimmings during the X2.1 flare in NOAA AR 11283

Avijeet Prasad, Karin Dissauer, Qiang Hu +4

The magnetohydrodynamics of active region NOAA 11283 is simulated using an initial non-force-free magnetic field extrapolated from its photospheric vector magnetogram. We focus on…

astro-ph.SR2018★ 44 cited

Magnetohydrodynamic simulation of magnetic null-point reconnections in NOAA AR12192 initiated with an extrapolated non-force-free-field

A. Prasad, R. Bhattacharyya, Qiang Hu +2

Magnetohydrodynamics of the solar corona is simulated numerically. The simulation is initialized with an extrapolated non-force-free magnetic field using the vector magnetogram of…

astro-ph.SR2018

Magnetic field topology from non-force free extrapolation and magnetohydrodynamic simulation of its eventual dynamics

Sushree S. Nayak, R. Bhattacharyya, A. Prasad +1

Magnetic reconnections (MRs) for various magnetic field line (MFL) topologies are believed to be the initiators of various solar eruptive events like flares and coronal mass ejecti…

astro-ph.SR2017★ 22 cited

Magnetohydrodynamic modeling of solar coronal dynamics with an initial non-force-free magnetic field

A. Prasad, R. Bhattacharyya, Sanjay Kumar

The magnetic fields in the solar corona are generally neither force-free nor axisymmetric and have complex dynamics that are difficult to characterize. Here we simulate the topolog…

astro-ph.SR2016★ 5 cited

A viable non-axisymmetric non-force-free field to represent solar active regions

A. Prasad, R. Bhattacharyya

A combination of analytical calculations and vectormagnetogram data are utilized to develop a non-axisymmetric non-force-free magnetic field and asses its viability in describing s…