131 citations · 867 across the 27 of their papers we have counts for
27 papers
The East-West Asymmetry of Particle Intensity in Energetic Storm Particle Events
Zheyi Ding, Gang Li, Adolfo Santa Fe Dueñas +3
We examine the East-West asymmetry of the peak intensity in energetic storm particle (ESP) events using the improved Particle Acceleration and Transport in the Heliosphere (iPATH)…
First report of a solar energetic particle event observed by China's Tianwen-1 mission in transit to Mars
Shuai Fu, Zheyi Ding, Yongjie Zhang +15
Solar energetic particles (SEPs) associated with flares and/or coronal mass ejection (CME)-driven shocks can impose acute radiation hazards to space explorations. To measure energe…
Relating the Solar Wind Turbulence Spectral Break at the Dissipation Range with an Upstream Spectral Bump at Planetary Bow Shocks
Michael Terres, Gang Li
At scales much larger than the ion inertial scale and the gyro-radius of thermal protons, magnetohydrodynamic (MHD) theory is well equipped to describe the nature of solar wind tur…
Current sheets, plasmoids and flux ropes in the heliosphere. Part II: Theoretical aspects
O. Pezzi, F. Pecora, J. le Roux +13
Our understanding of processes occurring in the heliosphere historically began with reduced dimensionality - one-dimensional (1D) and two-dimensional (2D) sketches and models, whic…
Automated identification of current sheets -- a new tool to study turbulence and intermittency in the solar wind
Olga Khabarova, Timothy Sagitov, Roman Kislov +1
We propose a new method of the automated identification of current sheets (CSs) that represents a formalization of the visual inspection approach employed in case studies. CSs are…
Do All Interplanetary Coronal Mass Ejections Have A Magnetic Flux Rope Structure Near 1 AU?
Hongqiang Song, Jie Zhang, Xin Cheng +6
Interplanetary coronal mass ejections (ICMEs) often consist of a shock wave, sheath region, and ejecta region. The ejecta regions are divided into two broad classes: magnetic cloud…
Statistical analysis of interplanetary magnetic field path lengths from solar energetic electron events observed by WIND
Lulu Zhao, Gang Li, Ming Zhang +3
We calculate the interplanetary magnetic field path lengths traveled by electrons in solar electron events detected by the WIND 3DP instrument from to . The velocity d…
Is the enhancement of type II radio bursts during CME interactions related to the associated solar energetic particle event?
Liu-Guan Ding, Zhi-Wei Wang, Li Feng +2
We investigated 64 pairs of interacting-CME events identified by the simultaneous observations of SOHO and STEREO spacecraft from 2010 January to 2014 August, to examine the relati…
Probing the Puzzle of Behind-the-Limb -ray Flares: Data-driven Simulations of Magnetic Connectivity and CME-driven Shock Evolution
Meng Jin, Vahe Petrosian, Wei Liu +8
Recent detections of high-energy -rays from behind-the-limb (BTL) solar flares by the \emph{Fermi -ray Space Telescope} pose a puzzle and challenge on the particle accelerati…
Modeling Transport of Energetic Particles in Corotating Interaction Region -- A case Study
Lulu Zhao, Gang Li, R. W. Ebert +5
We investigate energetic particle transport in Corotating Interaction Regions (CIRs) through a case study. The CIR event we study occurred on February and was observed…
Interchange reconnection associated with a confined filament eruption: Implications for the source of transient cold-dense plasma in solar winds
Ruisheng Zheng, Yao Chen, Bing Wang +1
The cold-dense plasma is occasionally detected in the solar wind with in situ data, but the source of the cold-dense plasma remains illusive. Interchange reconnections (IRs) betwee…
Observation of a Metric Type N Solar Radio Burst
Xiangliang Kong, Yao Chen, Shiwei Feng +7
Type III and type-III-like radio bursts are produced by energetic electron beams guided along coronal magnetic fields. As a variant of type III bursts, Type N bursts appear as the…
The injection of ten electron/He-rich SEP events
Linghua Wang, Säm Krucker, Glenn M. Mason +2
We have derived the particle injections at the Sun for ten good electron/He-rich solar energetic particle (SEP) events, using a 1.2 AU particle path length (suggested by anal…
On the identification of time interval threshold in the twin-CME scenario
Liu-Guan Ding, Gang Li, Li-Hua Dong +3
Recently it has been suggested that the "twin-CME" scenario Li.etal2012 may be a very effective mechanism in causing extreme Solar Energetic Particle (SEP) events and in particular…
Seed population in large Solar Energetic Particle events and the twin-CME scenario
Liu-Guan Ding, Gang Li, Gui-Ming Le +2
It has been recently suggested that large solar energetic particle (SEP) events are often caused by twin CMEs. In the twin-CME scenario, the preceding CME is to provide both an enh…
A Statistical Study of the Average Iron Charge Distributions inside Magnetic Clouds for Solar Cycle 23
Hongqiang Song, Ze Zhong, Yao Chen +5
Magnetic clouds (MCs) are the interplanetary counterpart of coronal magnetic flux ropes. They can provide valuable information to reveal the flux rope characteristics at their erup…
Microwave imaging of a hot flux rope structure during the pre-impulsive stage of an eruptive M7.7 solar flare
Z. Wu, Y. Chen, G. Huang +7
Corona structures and processes during the pre-impulsive stage of solar eruption are crucial to understanding the physics leading to the subsequent explosive energy release. Here w…
Electron Acceleration at a Coronal Shock Propagating Through a Large-scale Streamer-like Magnetic Field
Xiangliang Kong, Yao Chen, Fan Guo +3
With a test-particle simulation, we investigate the effect of large-scale coronal magnetic fields on electron acceleration at an outward-propagating coronal shock with a circular f…
An observational revisit of band-split solar type-II radio bursts
Guohui Du, Xiangliang Kong, Yao Chen +3
Band split of solar type II radio bursts, discovered several decades ago, is a fascinating phenomenon with the type-II lanes exhibiting two almost-parallel sub-bands with similar m…
Nonthermally Dominated Electron Acceleration during Magnetic Reconnection in a Low-beta Plasma
Xiaocan Li, Fan Guo, Hui Li +1
By means of fully kinetic simulations, we investigate electron acceleration during magnetic reconnection in a nonrelativistic proton--electron plasma with conditions similar to sol…
Imaging and spectroscopic observations of magnetic reconnection and chromospheric evaporation in a solar flare
Hui Tian, Gang Li, Katharine K. Reeves +5
Magnetic reconnection is believed to be the dominant energy release mechanism in solar flares. The standard flare model predicts both downward and upward outflow plasmas with speed…
Possible role of coronal streamer as magnetically-closed structure in shock-induced energetic electrons and metric type II radio bursts
Xiangliang Kong, Yao Chen, Fan Guo +4
Two solar type II radio bursts, separated by ~24 hours in time, are examined together. Both events are associated with coronal mass ejections (CMEs) erupting from the same active r…
First- and Second-order Fermi Acceleration at Parallel Shocks
Arto Sandroos, Gang Li, Lulu Zhao
We report on a new Monte Carlo method for simulating diffusive shock acceleration (DSA) of solar energetic particles at upstream and downstream regions of quasi-parallel collisionl…
A solar type II radio burst from CME-coronal ray interaction: simultaneous radio and EUV imaging
Yao Chen, Guohui Du, Li Feng +5
Simultaneous radio and extreme ultraviolet (EUV)/white-light imaging data are examined for a solar type II radio burst occurring on 2010 March 18 to deduce its source location. Usi…