1.Feng Xueshang, Wu S.T., Wei Fengsi (2003), A class of TVD type combined numerical scheme for MHD equations with a survey about numerical methods in solar wind simulations, Space Sci. Rev., 107, P.43-53.

2.Feng Xueshang, Y. Zhang, W. Sun, M. Dryer, C.D. Fry, and C.S. Deehr (2009), A practical database method for predicting arrivals of ‘‘average’’ interplanetary shocks at Earth, J. Geophys. Res., 114, A01101, doi:10.1029/2008JA013499.

3.Xueshang Feng and Yanqi Hu (2006), MODELING THE RESISTIVE MHD BY THE CESE METHOD, Solar Physics, 235, P.235–257.

4.Xueshang Feng and Xinhua Zhao (2006), A NEW PREDICTION METHOD FOR THE ARRIVAL TIME OF INTERPLANETARY SHOCKS, Solar Physics, 238, P.167–186, DOI: 10.1007/s11207-006-0185-3.

5.Xueshang Feng, Yufen Zhou, and S.T. Wu (2007), A NOVEL NUMERICAL IMPLEMENTATION FOR SOLAR WIND MODELING BY THE MODIFIED CONSERVATION ELEMENT/SOLUTION ELEMENT METHOD, The Astrophysical Journal, 655, P.1110-1126.