First-authored, refereed papers of Gang Li, ordered by citations


A list of first-authored, refereed publications of Gang Li, derived from the SAO/NASA Astrophysics Data System (ADS) and ordered by the numbers of citations. Publications above the horizontal line count towards the h-index.

Orcid ID: 0000-0003-4695-8866

Number of papers: 20
No. of citations: 856

165 Energetic particle acceleration and transport at coronal mass ejection-driven shocks
Li, Gang, Zank, G. P. & Rice, W. K. M., 2003, Journal of Geophysical Research (Space Physics), 108, 1082
101 A Twin-CME Scenario for Ground Level Enhancement Events
Li, G., Moore, R., Mewaldt, R. A., Zhao, L. & Labrador, A. W., 2012, Space Science Reviews, 171, 141
87 Acceleration and transport of heavy ions at coronal mass ejection-driven shocks
Li, Gang, Zank, G. P. & Rice, W. K. M., 2005, Journal of Geophysical Research (Space Physics), 110, A06104
84 Mixed particle acceleration at CME-driven shocks and flares
Li, G. & Zank, G. P., 2005, Geophysical Research Letters, 32, L02101
72 Particle acceleration and transport at an oblique CME-driven shock
Li, G., Shalchi, A., Ao, X., Zank, G. & Verkhoglyadova, O. P., 2012, Advances in Space Research, 49, 1067
72 Identifying Current-Sheet-like Structures in the Solar Wind
Li, G., 2008, ApJ, 672, L65
70 Shock Geometry and Spectral Breaks in Large SEP Events
Li, G., Zank, G. P., Verkhoglyadova, Olga, Mewaldt, R. A., Cohen, C. M. S., Mason, G. M. & Desai, M. I., 2009, ApJ, 702, 998
60 Effect of Current Sheets on the Solar Wind Magnetic Field Power Spectrum from the Ulysses Observation: From Kraichnan to Kolmogorov Scaling
Li, G., Miao, B., Hu, Q. & Qin, G., 2011, Physical Review Letters, 106, 125001
39 On the Spectral Hardening at gsim300 keV in Solar Flares
Li, G., Kong, X., Zank, G. & Chen, Y., 2013, ApJ, 769, 22
28 Modeling the 2012 May 17 Solar Energetic Particle Event Using the AWSoM and iPATH Models
Li, Gang, Jin, Meng, Ding, Zheyi, Bruno, A., de Nolfo, G. A., Randol, B. M., Mays, L., Ryan, J. & Lario, D., 2021, ApJ, 919, 146
22 Diffusive shock acceleration and large SEP events
Li, G., Zank, G., Verkhoglyadova, O. & Ding, L., 2013, Solar Wind 13 (Editors: Zank, Gary P., Borovsky, Joe, Bruno, Roberto, Cirtain, Jonathan, Cranmer, Steve, Elliott, Heather, Giacalone, Joe, Gonzalez, Walter, Li, Gang, Marsch, Eckart, Moebius, Ebehard, Pogorelov, Nick, Spann, Jim & Verkhoglyadova, Olga), American Institute of Physics Conference Series, 1539, p. 105
13 Acceleration and transport of energetic particles at CME-driven shocks
Li, G., Zank, G. P. & Rice, W. K. M., 2003, Advances in Space Research, 32, 2597
10 Effect of current sheets on the power spectrum of the solar wind magnetic field using a cell model
Li, G., Qin, G., Hu, Q. & Miao, B., 2012, Advances in Space Research, 49, 1327
6 Identification of Two Distinct Electron Populations in an Impulsive Solar Energetic Electron Event
Li, G., Zhao, L., Wang, L., Liu, W. & Wu, X., 2020, ApJ, 900, L16
6 Li et al. Reply:
Li, G., Miao, B., Hu, Q. & Qin, G., 2012, Physical Review Letters, 108, 199502
5 Lagrangian Stochastic Model for the Motions of Magnetic Footpoints on the Solar Wind Source Surface and the Path Lengths of Boundary-driven Interplanetary Magnetic Field Lines
Li, Gang & Bian, N. H., 2023, ApJ, 945, 150
5 Observations of Outward-propagating and Mirroring of the Same Energetic Electrons by Wind
Li, G., Wu, X., Zhao, L. & Yao, S., 2020, ApJ, 905, L1
4 Particle acceleration and transport at CME-Driven shocks: A case study
Li, Gang, Zank, G. P., Desai, M. I., Mason, G. M. & Rice, W. K. M., 2005, Geophysical Monograph Series, 156, 51
4 Constraints on the Electron Acceleration Process in Solar Flare: A Case Study
Li, G., Wu, X., Effenberger, F., Zhao, L., Lesage, S., Bian, N. & Wang, L., 2021, Geophysical Research Letters, 48, e95138
3 Modeling Solar Energetic Neutral Atoms from Solar Flares and CME-driven Shocks
Li, Gang, Shih, Albert Y., Allen, Robert C., Ho, George C., Cohen, Christina M. S., Desai, Mihir, Dayeh, Maher A. & Mason, Glenn M., 2023, ApJ, 944, 196


Created on Wed Jan 22 04:27:50 2025.