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1.Wang C, Wang J, Lopez R, Li H, Zhang J and Tang B (2018) Determination of Polar Cap Boundary for the Substorm Event of 8 March 2008. Front. Phys. 6:50. doi: 10.3389/fphy.2018.00050
2.Li. H., C. Wang, J. D. Richardson, et al. (2017), Evolution of Alfvénic Fluctuations inside an Interplanetary Coronal Mass Ejection and Their Contribution to Local Plasma Heating: Joint Observations from 1.0 to 5.4 au, ApJL, 851, 1.
3.Wang, C., J.Y. Wang, R.E. Lopez, L. Q. Zhang, B. B. Tang, T. R. Sun, and H. Li (2016), Effects of the interplanetary magnetic ?eld on the location of the open-closed ?eld line boundary, J. Geophys. Res. Space Physics,121, doi:10.1002/2016JA022784.
4.Sun, T. R., C. Wang, J. J. Zhang,V. A. Pilipenko, Y. Wang, and J. Y. Wang (2015), The chain response of the magnetospheric and ground magnetic field to interplanetary shocks, J. Geophys. Res. Space Physics, 120, 157–165, doi:10.1002/2014JA020754.
5.Wang, C., J. P. Han, H. Li, Z. Peng, J. D. Richardson (2014), Solar wind-magnetosphere energy coupling function fitting: Results from a global MHD simulation, J. Geophys. Res. Space Physics, DOI: 10.1002/2014JA019834
6.Wang, C., Z. Y. Xia, Z. Peng, and Q. M. Lu (2013), Estimating the open magnetic flux from the interplanetary and ionospheric conditions, J. Geophys. Res. Space Physics, 118, 1899–1903, doi:10.1002/jgra.50255.
7.Wang, C., Q. Zhang, P. J. Chi, and C. Li (2013), Simultaneous observations of plasmaspheric and ionospheric variations during magnetic storms in 2011: First result from Chinese Meridian Project, J. Geophys. Res., 118, doi:10.1029/2012JA017967.
8.Wang, C, Guo X C, Peng Z, et al. (2013), Magnetohydrodynamics (MHD) numerical simulations on the interaction of the solar wind with the magnetosphere: A review. Science China: Earth Sciences, 56: 1141–1157, doi: 10.1007/s11430-013-4608-3
9.Wang C, Li H, Guo X C, et al. (2012) Numerical study on the response of the Earth’s magnetosphere-ionosphere system to a super solar storm. Sci China Earth Sci,, doi: 10.1007/s11430-012-4405-4
10.Wang, C., J. J. Zhang, B. B. Tang, and S. Y. Fu (2011), Comparison of equivalent current systems for the substorm event of 8 March 2008 derived from the global PPMLR-MHD model and the KRM algorithm, J. Geophys. Res., 116, A07207, doi:10.1029/2011JA016497.
11.Wang, C., T. R. Sun, X. C. Guo, and J. D. Richardson (2010), Case study of nightside magnetospheric magnetic field response to interplanetary shocks, J. Geophys. Res., 115, A10247, doi:10.1029/2010JA015451.
12.Wang, C., H. Li, J. D. Richardson, and J. R. Kan (2010), Interplanetary shock characteristics and associated geosynchronous magnetic field variations estimated from sudden impulses observed on the ground, J. Geophys. Res., 115, A09215, doi:10.1029/2009JA014833.
13.Wang, C., J. B. Liu, H. Li, Z. H. Huang, J. D. Richardson, and J. R. Kan (2009), Geospace magnetic field responses to interplanetary shocks, J. Geophys. Res., 114, A05211, doi:10.1029/2008JA013794.
14.Richardson, J.D., J.C. Kasper, C. Wang, J.W. Belcher, and A. J. Lazarus(2008), Cool heliosheath plasma and deceleration of the upstream solar wind at the termination shock, Nature, 454, doi:10.1038/nature07024.
15.Wang, C., J. B. Liu, Z. H. Huang, and J. D. Richardson (2007), Response of the magnetic field in the geosynchronous orbit to solar wind dynamic pressure pulses, J. Geophys. Res., 112, A12210, doi:10.1029/2007JA012664
16.Wang C., C.X. Li, Z.H. Huang, and J.D. Richardson(2006), The effect of interplanetary shock strengths and orientations on storm sudden commencement rise times,Geophys. Res. Lett,33, L14104, doi:10.1029/2006GL025966
17.Wang C., D. Du, J.D. Richardson(2005), Characteristics of the interplanetary coronal mass ejections in the heliosphere between 0.3 and 5.4 AU, J. Geophys. Res., 110, A10107,doi:10.1029/2005JA011198
18.Wang C. and J.D. Richardson (2004), Interplanetary coronal mass ejections observed by Voyager 2 between 1 and 30 AU, J. Geophys. Res., 109, A06104, doi:10.1029/2004JA010379.
19.Wang, C., J. D. Richardson, L.F. Burlaga, and N.F. Ness (2003), On the radial heliospheric magnetic fields: Voyager 2 observation and model, J. Geophys. Res., 108, 1205, doi:10.1029/2002JA009809.
20.Wang, C. and J.D. Richardson (2003), Determination of the solar wind slowdown near solar maximum, J. Geophys. Res., 108(A2), 1058, doi:10.1029/2002JA009322.
21.Wang, C. and J.D. Richardson(2002), Development of a strong shock in the distant heliosphere, Geophys. Res. Lett.., Vol.29, No.8, doi:10.1029/2001GL014472.
22.Wang C. and J.D. Richardson (2001), Energy partition between the solar wind protons and pickup ions in the distant heliosphere: A Three-fluid approach, J. Geophys. Res., 106, 29401.
23.Wang, C. J. D. Richardson, and L. F. Burlaga, Propagation of the Bastille Day 2000 CME Shock in the Outer Heliosphere, Solar Physics, 204, 413, 2001.
24.Wang, C., J. D. Richardson, and K. I. Paularena. Predicted Voyager observations of the Bastille Day 2000 coronal mass ejection, J. Geophys. Res., 106, 13,007, 2001.
25.Wang, C. and J. D. Richardson, Voyager 2 observations of helium abundance enhancements from 1-60 AU, J. Geophys. Res.,106,5683, 2001.
26.Wang, C., J. D. Richardson and J. T. Gosling, Slowdown of the solar wind in the outer heliosphere and the interstellar neutral density, Geophys. Res. Lett., 16, 2429, 2000.
27.Wang, C., J. D. Richardson and J. T. Gosling, A numerical study of solar wind from Ulysses to Voyager 2, J. Geophys. Res., 105, 2337, 2000.
28.Wang, C. and J. W. Belcher, The heliospheric boundary response to large scale solar wind fluctuations: A gasdynamic model with pickup ions, J. Geophys. Res.,104 , 549 , 1999.
29.Wang, C. and J. W. Belcher, Numerical investigation of hydrodynamic instabilities of the heliopause, J. Geophys. Res., 103, 247, 1998.