activity
20082023
most citedStructure, Stability, and Evolution of Magnetic Flux Ropes from the Perspective of Magnetic Twist

315 citations · 4.2k across the 108 of their papers we have counts for

collaborators
Showing 2019Show all

8 papers · 1 filter

astro-ph.SR2019★ 24 cited

Formation of a Magnetic Flux Rope in the Early Emergence Phase of NOAA Active Region 12673

Lijuan Liu, Xin Cheng, Yuming Wang +1

In this work, we investigate the formation of a magnetic flux rope (MFR) above the central polarity inversion line (PIL) of NOAA Active Region 12673 during its early emergence phas…

astro-ph.SR2019★ 29 cited

Unusual plasma and particle signatures at Mars and STEREO-A related to CME-CME interaction

Mateja Dumbovic, Jingnan Guo, Manuela Temmer +15

On July 25 2017 a multi-step Forbush decrease (FD) with the remarkable total amplitude of more than 15\% was observed by MSL/RAD at Mars. We find that these particle signatures are…

astro-ph.SR2019

How Many Twists Do Solar Coronal Jets Release?

Jiajia Liu, Yuming Wang, Robertus Erdélyi

Highly twisted magnetic flux ropes, with finite length, are subject to kink instabilities, and could lead to a number of eruptive phenomena in the solar atmosphere, including flare…

astro-ph.SR2019★ 7 cited

Forward Modeling of the Type III Radio Burst Exciter

Peijin Zhang, Chuanbing Wang, Lin Ye +1

In this work, we propose a forward-modeling method to study the trajectory and speed of the interplanetary (IP) Type-III radio burst exciter. The model assumes that the source of a…

astro-ph.SR2019★ 15 cited

Extreme-ultraviolet Late Phase Caused by Magnetic Reconnection over Quadrupolar Magnetic Configuration in a Solar Flare

Zhenjun Zhou, Xin Cheng, Lijuan Liu +3

A second emission enhancement in warm coronal extreme-ultraviolet (EUV) lines (about 2-7 MK) during some solar flares is known as the EUV late phase. Imaging observations confirm t…

astro-ph.SR2019★ 51 cited

Why torus-unstable solar filaments experience failed eruption?

Zhenjun Zhou, Xin Cheng, Jie Zhang +5

To investigate the factors that control the success and/or failure of solar eruptions, we study the magnetic field and 3-Dimensional (3D) configuration of 16 filament eruptions dur…