output
20072022
most citedForecasting the Arrival Time of Coronal Mass Ejections: Analysis of the CCMC CME Scoreboard

169 citations

125 papers

astro-ph.EP2022★ 8 cited

Measurement of the vertical atmospheric density profile from the X-ray Earth occultation of the Crab Nebula with Insight-HXMT

Daochun Yu, Haitao Li, Baoquan Li +8

In this paper, the X-ray Earth occultation (XEO) of the Crab Nebula is investigated by using the Hard X-ray Modulation Telescope (Insight-HXMT). The pointing observation data on th…

astro-ph.SR2020★ 11 cited

Reconstructing solar wind inhomogeneous structures from stereoscopic observations in white-light: Solar wind transients in 3D

Xiaolei Li, Yuming Wang, Rui Liu +7

White-light images from Heliospheric Imager-1 (HI1) onboard the Solar Terrestrial Relations Observatory (STEREO) provide 2-dimensional (2D) global views of solar wind transients tr…

astro-ph.SR2020★ 27 cited

Observations of a quasi-periodic pulsation in the coronal loop and microwave flux during a solar preflare phase

Dong Li, Ying Li, Lei Lu +3

We report a quasi-periodic pulsation (QPP) event simultaneously detected from the spatial displacements of coronal loop at both EUV images and microwave emission during the preflar…

astro-ph.IM2020★ 10 cited

Study of the Modified Gaussian Model on olivine diagnostic spectral features and its applications in space weathering experiments

Hui-Jie Han, Xiao-Ping Lu, Ya-Zhou Yang +2

The absorption features of olivine in visible and near-infrared (VNIR) reflectance spectra are the key spectral parameters in its mineralogical studies. Generally, these spectral p…

astro-ph.SR2020★ 29 cited

Quasi-periodic pulsation detected in Lyman-alpha emission during solar flares

Dong Li, Lei Lu, Zongjun Ning +3

We investigated the quasi-periodic pulsation (QPP) in Lyman-alpha, X-ray and extreme-ultraviolet (EUV) emissions during two solar flares, i.e., an X-class (SOL2012-01-27T) and a C-…

physics.space-ph2020★ 40 cited

Evolution of the Earth's Magnetosheath Turbulence: A statistical study based on MMS observations

Hui Li, Wence Jiang, Chi Wang +5

Composed of shocked solar wind, the Earth's magnetosheath serves as a natural laboratory to study the transition of turbulence from low Alfv{é}n Mach number, , to hig…

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★ 72 cited

A Study of Pre-Flare Solar Coronal Magnetic Fields: Magnetic Flux Ropes

Aiying Duan, Chaowei Jiang, Wen He +3

Magnetic flux ropes (MFRs) are thought to be the central structure of solar eruptions, and their ideal MHD instabilities can trigger the eruption. Here we performed a study of all…

physics.space-ph2019★ 16 cited

Effects of alpha-proton differential flow on proton temperature anisotropy instabilities in the solar wind: Wind observations

G. Q. Zhao, H. Li, H. Q. Feng +3

Plasma kinetic waves and alpha-proton differential flow are two important subjects on the topic of evolution of the solar wind. Based on the Wind data during 2005-2015, this paper…

astro-ph.SR2019★ 14 cited

Quantifying the Propagation of Fast Coronal Mass Ejections from the Sun to Interplanetary Space Combining Remote Sensing and Multi-Point in-situ Observations

Xiaowei Zhao, Ying D. Liu, Huidong Hu +1

In order to have a comprehensive view of the propagation and evolution of coronal mass ejections (CMEs) from the Sun to deep interplanetary space beyond 1 au, we carry out a kinema…

astro-ph.SR2019★ 17 cited

Energy partition in two M-class circular-ribbon flares

Q. M. Zhang, J. X. Cheng, L. Feng +6

In this paper, we investigate the energy partition of two homologous M1.1 circular-ribbon flares (CRFs) in active region (AR) 12434. They were observed by \textit{SDO}, \textit{GOE…

physics.space-ph2019★ 56 cited

Electron Heating by Debye-Scale Turbulence in Guide-Field Reconnection

Yu. V. Khotyaintsev, D. B. Graham, K. Steinvall +14

We report electrostatic Debye-scale turbulence developing within the diffusion region of asymmetric magnetopause reconnection with moderate guide field using observations by the Ma…

physics.space-ph2019★ 5 cited

Spectral fluctuation analysis of ionospheric inhomogeneities over Brazilian territory Part II: E-F valley region plasma instabilities

Neelakshi J., Reinaldo R. Rosa, Siomel Savio +4

The turbulent-like process associated with ionospheric instabilities, has been identified as the main nonlinear process that drives the irregularities observed in the different ion…

astro-ph.SR2018★ 13 cited

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…

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★ 36 cited

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…

astro-ph.SR2018★ 69 cited

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…

astro-ph.SR2018★ 27 cited

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…

physics.space-ph2018★ 169 cited

Forecasting the Arrival Time of Coronal Mass Ejections: Analysis of the CCMC CME Scoreboard

Pete Riley, Leila Mays, Jesse Andries +15

Accurate forecasting of the properties of coronal mass ejections as they approach Earth is now recognized as an important strategic objective for both NOAA and NASA. The time of ar…

astro-ph.SR2018★ 27 cited

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…

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…

astro-ph.SR2018★ 12 cited

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…

astro-ph.SR2018★ 67 cited

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…

astro-ph.SR2018★ 40 cited

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…