activity
20122022
most citedA fundamental mechanism of solar eruption initiation

156 citations · 470 across the 14 of their papers we have counts for

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Showing astro-ph.SRShow all

11 papers · 1 filter

astro-ph.SR2022

Analyses of Flight Time During Solar Proton Events and Solar Flares

X. H. Xu, Y. Wang, F. S. Wei +17

Analyzing the effects of space weather on aviation is a new and developing topic. It has been commonly accepted that the flight time of the polar flights may increase during solar…

astro-ph.SR2022★ 1 cited

Characteristics of Flight Delays during Solar Flares

X. H. Xu, Y. Wang, F. S. Wei +15

Solar flare is one of the severest solar activities on the sun, and it has many important impacts on the near-earth space. It has been found that flight arrival delays will increas…

astro-ph.SR2022★ 2 cited

The Effects of Space Weather on Flight Delays

Y. Wang, X. H. Xu, F. S. Wei +15

Although the sun is really far away from us, some solar activities could still influence the performance and reliability of space-borne and ground-based technological systems on Ea…

astro-ph.SR2021★ 156 cited

A fundamental mechanism of solar eruption initiation

Chaowei Jiang, Xueshang Feng, Rui Liu +8

Solar eruptions are spectacular magnetic explosions in the Sun's corona, and how they are initiated remains unclear. Prevailing theories often rely on special magnetic topologies t…

astro-ph.SR2021★ 9 cited

Is Solar Minimum 24/25 Another Unusual One?

Huichao Li, Xueshang Feng, Fengsi Wei

The solar minimum 23/24 is considered to be unusual because it exhibits features that differ notably from those commonly seen in pervious minima. In this letter, we analyze the sol…

astro-ph.SR2020★ 29 cited

Continuous Null-Point Magnetic Reconnection Builds Up a Torus Unstable Magnetic Flux Rope Triggering the X9.3 Flare in Solar Active Region~12673

Peng Zou, Chaowei Jiang, Fengsi Wei +3

Two X-class solar flares occurred on 2017 September 6 from active region NOAA 12673: the first one is a confined X2.2 flare, and it is followed only hours later by the sec…

astro-ph.SR2019★ 34 cited

A Statistical Study of Solar Filament Eruptions That Forms High-Speed Coronal Mass Ejections

Peng Zou, Chaowei Jiang, Fengsi Wei +2

Coronal mass ejections (CMEs) play a decisive role in driving space weather, especially, the fast ones (e.g., with speeds above ~km~s). Understanding the trigger mechan…

astro-ph.SR2019★ 4 cited

Can Injection Model Replenish the Filaments in Weak Magnetic Environment?

Peng Zou, Chaowei Jiang, Fengsi Wei +1

We observed an H surge occurred in the active region NOAA 12401 on 2015 August 17, and discuss its trigger mechanism, kinematic and thermal properties. It is suggested that this…

astro-ph.SR2018★ 36 cited

A Two-Step Magnetic Reconnection in a Confined X-class Flare in Solar Active Region 12673

Peng Zou, Chaowei Jiang, Xueshang Feng +3

Solar flares are often associated with coronal eruptions, but there are confined ones without eruption, even for some X-class flares. How such large flares occurred and why they ar…

astro-ph.SR2018★ 69 cited

Magnetohydrodynamic Simulation of the X9.3 Flare on 2017 September 6: Evolving Magnetic Topology

Chaowei Jiang, Peng Zou, Xueshang Feng +7

Three-dimensional magnetic topology is crucial to understanding the explosive release of magnetic energy in the corona during solar flares. Much attention has been given to the pre…

astro-ph.SR2018★ 2 cited

Decipher the Three-Dimensional Magnetic Topology of a Great Solar Flare

Chaowei Jiang, Peng Zou, Xueshang Feng +5

Three-dimensional magnetic topology of solar flare plays a crucial role in understanding its explosive release of magnetic energy in the corona. However, such three-dimensional cor…