activity
20182021
most citedEffects of Coronal Density and Magnetic Field Distributions on a Global Solar EUV Wave

23 citations · 35 across the 4 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2021

Configuration of a Magnetic Cloud from Solar Orbiter and Wind Spacecraft In-situ Measurements

Qiang Hu, Wen He, Lingling Zhao +1

Coronal mass ejections (CMEs) represent one type of the major eruption from the Sun. Their interplanetary counterparts, the interplanetary CMEs (ICMEs), are the direct manifestatio…

astro-ph.SR2020

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…

physics.plasm-ph20204 cited

Intrinsic current drive by electromagnetic electron drift wave turbulence in tokamak pedestal region

Wen He, Lu Wang, Ge Zhuang

The local intrinsic parallel current density driven by electron drift wave (DW) turbulence including electromagnetic (EM) effects is analytically studied. The scalings of the ratio…

physics.plasm-ph20208 cited

Intrinsic current drive by electromagnetic electron temperature gradient turbulence in tokamak plasmas

Wen He, Lu Wang, Shuitao Peng +2

The mean parallel current density evolution equation is presented using electromagnetic (EM) gyrokinetic equation. There exist two types of intrinsic current driving mechanisms res…

astro-ph.SR2020

Data-driven MHD Simulation of the Formation and Initiation of a Large-scale Pre-flare Magnetic Flux Rope in Solar Active Region 12371

Wen He, Chaowei Jiang, Peng Zou +4

Solar eruptions are the most powerful drivers of space weather. To understand their cause and nature, it is crucial to know how the coronal magnetic field evolves before eruption.…

astro-ph.SR2019

A Study of Pre-Flare Solar Coronal Magnetic Fields: Magnetic Flux Ropes

Aiying Duan, Chaowei Jiang, Wen He +3

Magnetic flux ropes (MFRs) are thought to be the central structure of solar eruptions, and their ideal MHD instabilities can trigger the eruption. Here we performed a study of all…