activity
20072023
most citedA fundamental mechanism of solar eruption initiation

156 citations · 1.8k across the 60 of their papers we have counts for

collaborators
Showing 2020Show all

9 papers · 1 filter

astro-ph.SR2020★ 56 cited

Detection of small magnetic flux ropes from the third and fourth Parker Solar Probe encounters

L. -L. Zhao, G. P. Zank, Q. Hu +22

We systematically search for magnetic flux rope structures in the solar wind to within the closest distance to the Sun of 0.13 AU, using data from the third and fourth orbits of th…

astro-ph.SR2020★ 9 cited

On the quasi-three dimensional configuration of magnetic clouds

Qiang Hu, Wen He, Jiong Qiu +2

We develop an optimization approach to model the magnetic field configuration of magnetic clouds, based on a linear-force free formulation in three dimensions. Such a solution, dub…

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.SR2020★ 18 cited

Do All Interplanetary Coronal Mass Ejections Have A Magnetic Flux Rope Structure Near 1 AU?

Hongqiang Song, Jie Zhang, Xin Cheng +6

Interplanetary coronal mass ejections (ICMEs) often consist of a shock wave, sheath region, and ejecta region. The ejecta regions are divided into two broad classes: magnetic cloud…

astro-ph.SR2020★ 1 cited

A data-driven MHD model of the weakly-ionized chromosphere

Mehmet Sarp Yalim, Avijeet Prasad, Nikolai Pogorelov +2

The physics of the solar chromosphere is complex from both theoretical and modeling perspectives. The plasma temperature from the photosphere to corona increases from ~5,000 K to ~…

astro-ph.SR2020★ 16 cited

Effects of Cowling Resistivity in the Weakly-Ionized Chromosphere

Mehmet Sarp Yalim, Avijeet Prasad, Nikolai Pogorelov +2

The physics of the solar chromosphere is complex from both theoretical and modeling perspectives. The plasma temperature from the photosphere to corona increases from ~5,000 K to ~…