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[16] Wu, C. S.; Yoon, P. H.; Wang, C. B., 2009, On nonresonant proton heating via intrinsic Alfvenic turbulence, Physics of Plasmas, 16(5), p 054503
[17] Wang, C. B.; Wu, C. S., 2009, Pseudoheating of protons in the presence of Alfvenic turbulence, Physics of Plasmas, 16(2), p 020703
[18] Yoon, Peter H.; Wang, C. B.; Wu, C. S., 2007, Ring-beam driven maser instability for quasiperpendicular shocks, Physics of Plasmas, 14(2), p 022901
[19] Wu, CS; Wang, CB; Lu, QM, 2006, Density depletion in a coronal flux tube associated with solar radio emission, Solar Physics, 235(1-2), pp 317-329
[20] Wang, CB; Wu, CS; Yoon, PH, 2006, Heating of ions by Alfven waves via nonresonant interactions, Physical Review Letters, 96(12), p 125001
[21] Zheng, HN; Zhang, YY; Wang, S; Wang, CB; Li, Y, 2006, Propagation of fast magnetoacoustic waves in stratified solar atmosphere, Chinese Physics Letters, 23(2), pp 399-402
[22] Xue, XH; Wang, CB; Dou, XK, 2005, An ice-cream cone model for coronal mass ejections, Journal of Geophysical Research, 110(A8), p A08103
[23] Chen, YP; Wang, CB; Zhou, GC, 2005, Maser instability driven by an electron beam with losscone-beam distribution, Acta Physica Sinica, 54(7), pp 3221-3227
[24] Wu, CS; Wang, CB; Zhou, GC; Wang, S; Yoon, PH, 2005, Altitude-dependent emission of type III solar radio bursts, Astrophysical Journal, 621(2), pp 1129-1136
[25] Wang, CB; Chao, JK, 2003, Comment on "Effects of fast and slow solar wind on the correlation between interplanetary medium and geomagnetic activity" by P. Ballatore, Journal of Geophysical Research, 108(A10), p 1386
[26] Wang, CB; Chao, JK; Lin, CH, 2003, Influence of the solar wind dynamic pressure on the decay and injection of the ring current, Journal of Geophysical Research, 108(A9), p 1341
[27] Wang, CB; Zhao, JK; Cheng, HH; Li, Y; Wang, S; Sun, W; Akasofu, SI, 2002, Prediction of the IMF B-z using 3-D kinematic code, Chinese Journal of Geophysics, 45(6), pp 749-758
[28] Yoon, PH; Wu, CS; Wang, CB, 2002, Generation of type III solar radio bursts in the low corona by direct amplification. II. Further numerical study, Astrophysical Journal, 576(1), pp 552-560
[29] Wu, CS; Wang, CB; Yoon, PH; Zheng, HN; Wang, S, 2002, Generation of type III solar radio bursts in the low corona by direct amplification, Astrophysical Journal, 575(2), pp 1094-1103
[30] Wang, CB; Wang, S, 2001, Pressure influences on the coupling of double tearing mode in a multiple current sheet, Chinese Journal of Geophysics, 44(2), pp 145-153
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