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

169 citations

Showing 2013 · astro-ph.SRShow all

11 papers · 2 filters

astro-ph.SR2013★ 28 cited

Estimation of the release time of solar energetic particles near the Sun

Y. Wang, G. Qin

This paper investigates the onset time of Solar Energetic Particle (SEP) events with numerical simulations, and analyses the accuracy of the Velocity Dispersion Analysis (VDA) meth…

astro-ph.SR2013★ 100 cited

Formation and Eruption of an Active Region Sigmoid: I. Study by Nonlinear Force-Free Field Modeling

Chaowei Jiang, S. T. Wu, Xueshang Feng +1

We present a magnetic analysis of the formation and eruption of an active region (AR) sigmoid in AR 11283 from 2011 September 4 to 6. To follow the quasi-static evolution of the co…

astro-ph.SR2013★ 84 cited

Tracking the Evolution of A Coherent Magnetic Flux Rope Continuously from the Inner to the Outer Corona

X. Cheng, M. D. Ding, Y. Guo +6

The magnetic flux rope (MFR) is believed to be the underlying magnetic structure of coronal mass ejections (CMEs). However, it remains unclear how an MFR evolves into and forms the…

astro-ph.SR2013★ 64 cited

Modulation of galactic cosmic rays during the unusual solar minimum between cycles 23 and 24

L. -L. Zhao, G. Qin, M. Zhang +1

During the recent solar minimum between cycles 23 and 24 (solar minimum ) the intensity of Galactic Cosmic Rays (GCRs) measured at the Earth was the highest ever recorde…

astro-ph.SR2013★ 11 cited

Using Coordinated Observations in Polarised White Light and Faraday Rotation to Probe the Spatial Position and Magnetic Field of an Interplanetary Sheath

Ming Xiong, Jackie A. Davies, Xueshang Feng +4

Coronal mass ejections (CMEs) can be continuously tracked through a large portion of the inner heliosphere by direct imaging in visible and radio wavebands. White-light (WL) signat…

astro-ph.SR2013★ 37 cited

Preprocess the Photospheric Vector Magnetograms for NLFFF Extrapolation using a Potential Field Model and an Optimization Method

Chaowei Jiang, Xueshang Feng

Numerical reconstruction/extrapolation of coronal nonlinear force-free magnetic field (NLFFF) usually takes the photospheric vector magnetogram as input at the bottom boundary. Mag…

astro-ph.SR2013★ 157 cited

MHD Simulation of a Sigmoid Eruption of Active Region 11283

Chaowei Jiang, Xueshang Feng, S. T. Wu +1

Current magnetohydrodynamic (MHD) simulations of the initiation of solar eruptions are still commonly carried out with idealized magnetic field models, whereas the realistic corona…

astro-ph.SR2013★ 96 cited

Investigating Two Successive Flux Rope Eruptions In A Solar Active Region

X. Cheng, J. Zhang, M. D. Ding +4

We investigate two successive flux rope (FR1 and FR2) eruptions resulting in two coronal mass ejections (CMEs) on 2012 January 23. Both FRs appeared as an EUV channel structure in…

astro-ph.SR2013★ 145 cited

On Sun-to-Earth Propagation of Coronal Mass Ejections

Ying D. Liu, Janet G. Luhmann, Noé Lugaz +4

We investigate how coronal mass ejections (CMEs) propagate through, and interact with, the inner heliosphere between the Sun and Earth, a key question in CME research and space wea…

astro-ph.SR2013★ 92 cited

Extrapolation of the Solar Coronal Magnetic Field from SDO/HMI Magnetogram by a CESE--MHD--NLFFF Code

Chaowei Jiang, Xueshang Feng

Due to the absence of direct measurement, the magnetic field in the solar corona is usually extrapolated from the photosphere in numerical way. At the moment, the nonlinear force-f…

astro-ph.SR2013★ 54 cited

Diagnostics on the source properties of type II radio burst with spectral bumps

S. W. Feng, Y. Chen, X. L. Kong +4

In recent studies (Feng et al., 2012; Kong et al., 2012), we proposed that source properties of type II radio bursts can be inferred through a causal relationship between the speci…