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
12 papers · 2 filters
On Sun-to-Earth Propagation of Coronal Mass Ejections: 2. Slow Events and Comparison with Others
Ying D. Liu, Huidong Hu, Chi Wang +4
As a follow-up study on Sun-to-Earth propagation of fast coronal mass ejections (CMEs), we examine the Sun-to-Earth characteristics of slow CMEs combining heliospheric imaging and…
Fine Magnetic Structure and Origin of Counter-Streaming Mass Flows in a Quiescent Solar Prominence
Yuandeng Shen, Yu Liu, Ying D. Liu +4
We present high-resolution observations of a quiescent solar prominence which was consisted of a vertical and a horizontal foot encircled by an overlying spine, and counter-streami…
Properties of the Fast Forward Shock Driven by the July 23 2012 Extreme Coronal Mass Ejection
Pete Riley, Ronald M. Caplan, Joe Giacalone +2
Late on July 23, 2012, the STEREO-A spacecraft encountered a fast forward shock driven by a coronal mass ejection launched from the Sun earlier that same day. The estimated travel…
Proton Heating in Solar Wind Compressible Turbulence with Collisions between Counter-propagating Waves
Jiansen He, Chuanyi Tu, Eckart Marsch +6
Magnetohydronamic turbulence is believed to play a crucial role in heating the laboratorial, space, and astrophysical plasmas. However, the precise connection between the turbulent…
Why does the apparent mass of a coronal mass ejection increase?
Li Feng, Yuming Wang, Fang Shen +4
Mass is one of the most fundamental parameters characterizing the dynamics of a coronal mass ejection (CME). It has been found that CME apparent mass measured from the brightness e…
A Comparison Study of a Solar Active-Region Eruptive Filament and a Neighboring Non-Eruptive Filament
Chaowei Jiang, S. T. Wu, Xueshang Feng +1
Solar active region (AR) 11283 is a very magnetically complex region and it has produced many eruptions. However, there exists a non-eruptive filament in the plage region just next…
A Two-ribbon White-light Flare Associated with a Failed Solar Eruption Observed by ONSET, SDO, and IRIS
X. Cheng, Q. Hao, M. D. Ding +4
Two-ribbon brightenings are one of the most remarkable characteristics of an eruptive solar flare and are often used for predicting the occurrence of coronal mass ejections (CMEs).…
Testing a Solar Coronal Magnetic Field Extrapolation Code with the Titov-Demoulin Magnetic Flux Rope Model
Chaowei Jiang, Xueshang Feng
In the solar corona, magnetic flux rope is believed to be a fundamental structure accounts for magnetic free energy storage and solar eruptions. Up to the present, the extrapolatio…
Numerical simulations of solar energetic particle event timescales associated with ICMES
S. -Y. Qi, G. Qin, Y. Wang
Recently, S.W. Kahler studied the solar energetic particle (SEP) event timescales associated with coronal mass ejections (CMEs) from spacecraft data analysis. They obtained differe…
Simulations of a gradual solar energetic particle event observed by Helios 1, Helios 2, and IMP 8
G. Qin, Y. Wang
In this work, a gradual solar energetic particle (SEP) event observed by multispacecraft has been simulated. The time profiles of SEP fluxes accelerated by an interplanetary shock…
Satistical Study of the Interplanetary Coronal Mass Ejections from 1996 to 2014
Yutian Chi, Chenglong Shen, Yuming Wang +2
In this work, we establish an ICME list from 1996 to 2014 based on the in-situ observations from the WIND and ACE satellites. Based on this ICME list, we extend the statistical ana…
Improvements of the shock arrival times at the Earth model STOA
H. -L. Liu, G. Qin
Prediction of the shocks' arrival times (SATs) at the Earth is very important for space weather forecast. There is a well-known SAT model, STOA, which is widely used in the space w…