activity
20172026
most citedGeometry, Kinematics and Heliospheric Impact of a Large CME-driven Shock in 2017 September

36 citations · 186 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.SR2026★ 2 cited

A Major Geomagnetic Storm in 2024 October Linked to Sympathetic CME--Prominence Eruptions

Rui Wang, Huidong Hu, Xiaowei Zhao +11

Improving predictions of the geomagnetic impact of coronal mass ejections (CMEs) requires understanding how solar source properties relate to in-situ measurements at Earth. However…

physics.space-ph2025★ 2 cited

Lateral Deformation of Large-scale Coronal Mass Ejections during the Transition from Non-radial to Radial Propagation

Huidong Hu, Chong Chen, Yiming Jiao +4

Many coronal mass ejections (CMEs) initially propagate non-radially, and then transition to radial propagation in the corona. This directional transition is a significant process t…

astro-ph.SR2024★ 4 cited

Limb Observations of Global Solar Coronal Extreme-ultraviolet Wavefronts: The Inclination, Kinematics, Coupling with the Expanding Coronal Mass Ejections, and Connection with the Coronal Mass Ejection Driven Shocks

Huidong Hu, Bei Zhu, Ying D. Liu +3

We select and investigate six global solar extreme-ultraviolet (EUV) wave events using data from the Solar Dynamics Observatory and the Solar and Heliospheric Observatory. These er…

astro-ph.SR2019★ 24 cited

The Structure of Solar Coronal Mass Ejections in the Extreme-Ultraviolet Passbands

H. Q. Song, J. Zhang, L. P. Li +5

So far most studies on the structure of coronal mass ejections (CMEs) are conducted through white-light coronagraphs, which demonstrate about one third of CMEs exhibit the typical…

astro-ph.SR2019★ 32 cited

Characteristics of a Gradual Filament Eruption and Subsequent CME Propagation in Relation to a Strong Geomagnetic Storm

Chong Chen, Ying D. Liu, Rui Wang +3

An unexpected strong geomagnetic storm occurred on 2018 August 26, which was caused by a slow coronal mass ejection (CME) from a gradual eruption of a large quiet-region filament.…

astro-ph.SR2019★ 23 cited

Effects of Coronal Density and Magnetic Field Distributions on a Global Solar EUV Wave

Huidong Hu, Ying D. Liu, Bei Zhu +4

We investigate a global extreme-ultraviolet (EUV) wave associated with a coronal mass ejection (CME)-driven shock on 2017 September 10. The EUV wave is transmitted by north- and so…

astro-ph.SR2019★ 33 cited

A Comparative Study of 2017 July and 2012 July Complex Eruptions: Are Solar Superstorms "Perfect Storms" in Nature?

Ying D. Liu, Xiaowei Zhao, Huidong Hu +2

It is paramount from both scientific and societal perspectives to understand the generation of extreme space weather. We discuss the formation of solar superstorms based on a compa…

astro-ph.SR2018★ 36 cited

Geometry, Kinematics and Heliospheric Impact of a Large CME-driven Shock in 2017 September

Ying D. Liu, Bei Zhu, Xiaowei Zhao

A powerful coronal mass ejection (CME) occurred on 2017 September 10 near the end of the declining phase of the historically weak solar cycle 24. We obtain new insights concerning…

astro-ph.SR2018★ 19 cited

Investigation of energetic particle release using multi-point imaging and in situ observations

Bei Zhu, Ying D. Liu, Ryun-Young Kwon +1

The solar eruption on 2012 January 27 resulted in a wide-spread solar energetic particle (SEP) event observed by STEREO A and the near-Earth spacecraft (separated by 108\degree). T…

physics.space-ph2017★ 11 cited

Propagation and Interaction Properties of Successive Coronal Mass Ejections in Relation to a Complex Type II Radio Burst

Ying D. Liu, Xiaowei Zhao, Bei Zhu

We examine the propagation and interaction properties of three successive coronal mass ejections (CMEs) from 2001 November 21-22, with a focus on their connection with the behavior…