169 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Chinese Academy of SciencesCN124 papers
- National Space Science CenterCN91 papers
- University of Chinese Academy of SciencesCN32 papers
- University of Science and Technology of ChinaCN15 papers
- National Astronomical ObservatoriesCN14 papers
- Harbin Institute of TechnologyCN11 papers
- Institute of Theoretical PhysicsCN11 papers
- Purple Mountain ObservatoryCN11 papers
- Yunnan ObservatoriesCN11 papers
- Key Laboratory of Solar Activities, Chinese Academy of SciencesCN10 papers
- Shandong UniversityCN10 papers
- Space Sciences LaboratoryUS10 papers
28 papers · 2 filters
Imaging observations of chromospheric evaporation in a circular-ribbon flare
Q. M. Zhang, D. Li, Y. Huang
In this paper, we report our multiwavelength imaging observations of chromospheric evaporation in a C5.5 circular-ribbon flare (CRF) on 2014 August 24. The flare was observed by th…
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…
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…
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…
Roles of photospheric motions and flux emergence in the major solar eruption on 2017 September 6
Rui Wang, Ying D. Liu, J. Todd Hoeksema +2
We study the magnetic field evolution in the active region (AR) 12673 that produced the largest solar flare in the past decade on 2017 September 6. Fast flux emergence is one of th…
Radio, Hard X-Ray, and Gamma-Ray Emissions Associated with a Far-Side Solar Event
V. V. Grechnev, V. I. Kiselev, L. K. Kashapova +9
The SOL2014-09-01 far-side solar eruptive event produced hard electromagnetic and radio emissions observed with detectors at near-Earth vantage points. Especially challenging was a…
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…
A Survey of Changes in Magnetic Helicity Flux on the Photosphere During Relatively Low Class Flares
Yi Bi, Ying D Liu, Yanxiao Liu +3
Using the 135-second cadence of the photospheric vector data provided by the Helioseismic and Magnetic Imager telescope on board the Solar Dynamic Observatory, we examined the time…
Global Non-Potential Magnetic Models of the Solar Corona During the March 2015 Eclipse
A. R. Yeates, T. Amari, I. Contopoulos +17
Seven different models are applied to the same problem of simulating the Sun's coronal magnetic field during the solar eclipse on 2015 March 20. All of the models are non-potential…
Coronal EUV, QFP, and kink waves simultaneously launched during the course of jet-loop interaction
Yuandeng Shen, Zehao Tang, Hongbo Li +1
We present the observations of an extreme ultraviolet (EUV) wave, a quasi-periodic fast-propagating (QFP) magnetosonic wave, and a kink wave that were simultaneously associated wit…
Two Kinds of Dynamic Behavior in a Quiescent Prominence Observed by the NVST
Dong Li, Yuandeng Shen, Zongjun Ning +2
We present high-resolution observations of two kinds of dynamic behavior in a quiescent prominence using the New Vacuum Solar Telescope, i.e., Kelvin-Helmholtz instabilities (KHIs)…
A Solar Eruption with Relatively Strong Geo-effectiveness Originating from Active Region Peripheral Diffusive Polarities
Rui Wang, Ying D. Liu, Huidong Hu +1
We report the observations of a moderate but relatively intense geo-effective solar eruption on 2015 November 4 from the peripheral diffusive polarities of active region 12443. We…
Spectroscopic and imaging observations of small-scale reconnection events
Dong Li, Leping Li, Zongjun Ning
We present spectroscopic and imaging observations of small-scale reconnection events on the Sun. Using the Interface Region Imaging Spectrograph (IRIS) observations, one reconnecti…
EUV Waves Driven by the Sudden Expansion of Transequatorial Loops Caused by Coronal Jets
Yuandeng Shen, Zehao Tang, Yuhu Miao +2
We present two events to study the driving mechanism of extreme-ultraviolet (EUV) waves that are not associated with coronal mass ejections (CMEs), by using high resolution observa…
Formation and Eruption of a Double-decker Filament Triggered by Micro-bursts and Recurrent Jets in the Filament Channel
Zhanjun Tian, Yuandeng Shen, Yu Liu
We present the observations of a double-decker filament to study its formation, triggering, and eruption physics. It is observed that the double-decker filament was formed by split…
Homologous large-amplitude Nonlinear fast-mode Magnetosonic Waves Driven by Recurrent Coronal Jets
Yuandeng Shen, Yu Liu, Ying D. Liu +3
The detailed observational analysis of a homologous Extreme-ultraviolet (EUV) wave event is presented to study the driving mechanism and the physical property of the EUV waves, com…
Kinetic Properties of an Interplanetary Shock Propagating inside a Coronal Mass Ejection
Mingzhe Liu, Ying D. Liu, Zhongwei Yang +2
We investigate the kinetic properties of a typical fast-mode shock inside an interplanetary coronal mass ejection (ICME) observed on 1998 August 6 at 1 AU, including particle distr…
The 2015 Summer Solstice Storm: one of the major geomagnetic storms of solar cycle 24 observed at ground level
C. R. A. Augusto, C. E. Navia, M. N. de Oliveira +8
We report on the 22-23 June 2015 geomagnetic storm. There has been a shortage of intense geomagnetic storms during the current solar cycle 24 in relation to the previous cycle. Thi…
Modulations of the Surface Magnetic Field on the Intra-cycle Variability of Total Solar Irradiance
J. C. Xu, D. F. Kong, F. Y. Li
Solar photospheric magnetic field plays a dominant role in the variability of total solar irradiance (TSI). The modulation of magnetic flux at six specific ranges on TSI is charact…
A Model of Sunspot Number with Modified Logistic Function
G. Qin, S. -S. Wu
Solar cycles are studied with the Version 2 monthly smoothed international sunspot number, the variations of which are found to be well represented by the modified logistic differe…
New estimation of non-thermal electron energetics in the giant solar flare on 28 October 2003 based on Mars Odyssey observations
B. A. Nizamov, I. V. Zimovets, D. V. Golovin +5
A new estimation of the total number and energy of the non-thermal electrons produced in the giant () solar flare on 2003 October 28 is presented based on the analysis…
Dispersively Formed Quasi-Periodic Fast Magnetosonic Wavefronts Due to the Eruption of a Nearby Mini-filament
Yuandeng Shen, Tengfei Song, Yu Liu
The observational analysis is performed to study the excitation mechanism and the propagation properties of a quasi-periodic fast-propagating (QFP) magnetosonic wave. The QFP wave…
Properties of a Small-scale Short-duration Solar Eruption with a Driven Shock
Beili Ying, Li Feng, Lei Lu +5
Large-scale solar eruptions have been extensively explored over many years. However, the properties of small-scale events with associated shocks have been rarely investigated. We p…
Successive X-class flares and coronal mass ejections driven by shearing motion and sunspot rotation in active region NOAA 12673
X. L. Yan, J. C. Wang, G. M. Pan +5
We present a clear case study on the occurrence of two successive X-class flares including a decade-class flare (X9.3) and two coronal mass ejections (CMEs) triggered by shearing m…