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

169 citations

Showing 2017Show all

8 papers · 1 filter

physics.space-ph2017★ 48 cited

Modulation of Galactic Cosmic Rays in the Inner Heliosphere over Solar Cycles

Z. -N. Shen, G. Qin

The 11-year and 22-year modulation of galactic cosmic rays (GCRs) in the inner heliosphere are studied using a numerical model developed by Qin and Shen in 2017. Based on the numer…

astro-ph.SR2017★ 16 cited

Magnetic structure of solar flare regions producing hard X-ray pulsations

I. V. Zimovets, R. Wang, Y. D. Liu +5

We present analysis of the magnetic field in seven solar flare regions accompanied by the pulsations of hard X-ray (HXR) emission. These flares were studied by Kuznetsov et al. (20…

physics.space-ph2017★ 13 cited

Model of energy spectrum parameters of ground level enhancement events in solar cycle 23

S. -S. Wu, G. Qin

Mewaldt et al. 2012 fitted the observations of the ground level enhancement (GLE) events during solar cycle 23 to the double power-law equation to obtain the four energy spectra pa…

physics.space-ph2017★ 45 cited

Modulation of Galactic Cosmic Rays in the Inner Heliosphere, Comparing with PAMELA Measurements

Gang Qin, Zhenning Shen

We develop a numerical model to study the time-dependent modulation of galactic cosmic rays (GCRs) in the inner heliosphere. In the model a time-delayed modified Parker heliospheri…

astro-ph.SR2017★ 16 cited

Multi-spacecraft Observations of the Coronal and Interplanetary Evolution of a Solar Eruption Associated with Two Active Regions

Huidong Hu, Ying D. Liu, Rui Wang +3

We investigate the coronal and interplanetary evolution of a coronal mass ejection (CME) launched on 2010 September 4 from a source region linking two active regions (ARs) 11101 an…

physics.space-ph2017★ 16 cited

Numerical simulations of particle acceleration at interplanetary quasi-perpendicular shocks

F. -J. Kong, G. Qin, L. -H. Zhang

Using test particle simulations we study particle acceleration at highly perpendicular () shocks under conditions of modeling magnetic turbulence. We adopt a b…

astro-ph.HE2017★ 1 cited

Study of time evolution of the bend-over energy in the energetic particle spectrum at a parallel shock

F. -J. Kong, G. Qin, S. -S. Wu +4

Shock acceleration is considered one of the most important mechanisms for the acceleration of astrophysical energetic particles. In this work, we calculate the trajectories of a la…

math.NA2017★ 2 cited

3D B_2 Model for Radiative Transfer Equation Part I: Modelling

Ruo Li, Weiming Li

We extend to three-dimensional space the approximate M_2 model for the slab geometry studied in our previous paper. The B_2 model therein, as a special case of the second order ext…