activity
20112023
most citedImaging and spectroscopic observations of magnetic reconnection and chromospheric evaporation in a solar flare

131 citations · 867 across the 27 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

22 papers · 1 filter

astro-ph.SR2023★ 6 cited

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)…

astro-ph.SR2022★ 14 cited

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…

astro-ph.SR2021

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…

astro-ph.SR2020★ 18 cited

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…

astro-ph.SR2019★ 34 cited

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…

astro-ph.SR2018★ 10 cited

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…

astro-ph.SR2018★ 49 cited

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…

astro-ph.SR2017★ 19 cited

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…

astro-ph.SR2016★ 14 cited

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…

astro-ph.SR2016★ 49 cited

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…

astro-ph.SR2016★ 17 cited

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…

astro-ph.SR2016★ 18 cited

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…

astro-ph.SR2016★ 40 cited

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…

astro-ph.SR2016★ 28 cited

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…

astro-ph.SR2016★ 20 cited

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…

astro-ph.SR2015★ 26 cited

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…

astro-ph.SR2015★ 94 cited

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…

astro-ph.SR2014★ 131 cited

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…

astro-ph.SR2014★ 35 cited

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…

astro-ph.SR2014★ 48 cited

A solar eruption driven by rapid sunspot rotation

Guiping Ruan, Yao Chen, Shuo Wang +8

We present the observation of a major solar eruption that is associated with fast sunspot rotation. The event includes a sigmoidal filament eruption, a coronal mass ejection, and a…

astro-ph.SR2012★ 54 cited

A broken solar type II radio burst induced by a coronal shock propagating across the streamer boundary

Xiang-Liang Kong, Yao Chen, Gang Li +4

We discuss an intriguing type II radio burst that occurred on 2011 March 27. The dynamic spectrum was featured by a sudden break at about 43 MHz on the well-observed harmonic branc…

astro-ph.SR2011★ 35 cited

A Statistical Study on the Morphology of Rays and Dynamics of Blobs in the Wake of Coronal Mass Ejections

Hong-Qiang Song, Xiang-Liang Kong, Yao Chen +4

In this paper, with a survey through the Large Angle and Spectrometric Coronagraph (LASCO) data from 1996 to 2009, we present 11 events with plasma blobs flowing outwards sequentia…