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[1] 2015.
[2] Lu, S., Y. Lin, Quanming Lu(*), X. Y. Wang, R. S. Wang, C. Huang, M. Y. Wu, and S. Wang, Evolution of flux ropes in the magnetotail: A three-dimensional global hybrid simulation, Phys. Plasmas, 22, 052901, doi: 10.1063/1.4919615, 2015..
[3] Huang, C., M. Y. Wu, Quanming Lu(*), R. S. Wang, and S. Wang , Electron acceleration in the dipolarization front driven by magnetic reconnection, J. Geophys. Res., 120, 1759–1765, doi:10.1002/2014JA020918, 2015..
[4] Shan, L. C., Quanming Lu(*), C. Mazelle, C. Huang, T. L. Zhang, M. Y. Wu, X. L. Gao, S. Wang, The shape of the Venusian bow shock at solar minimum and maximum: Revisit based on VEX observations, Planetary and Space Science, 109-110, 32-37, 2015..
[5] Guo, Z. F., M. H. Hong, Y. Lin, A. M. Du, X. Y. Wang, M. Y. Wu, and Quanming Lu(*), Generation of kinetic Alfven waves in the high-latitude near-Earth magnetotail: A global hybrid simulation, Phys. Plasmas, 22, 022117, doi: 10.1063/1.4907666, 2015..
[6] 2014.
[7] Wang, R. S., Quanming Lu, A. M. Du, R. Nakamura, S. Lu, C. Huang, C. X. Liu, and M. Y. Wu, In situ observation of magnetic reconnection in the front of bursty bulk flow, J. Geophys. Res, 119, 9952–9961, doi:10.1002/2014JA020335, 2014..
[8] Gao, X. L., W. Li, R. M. Thorne, J. Bortnik, V. Angelopoulos, Quanming Lu, X. Tao, and S. Wang, Statistical results describing the bandwidth and coherence coefficient of whistler mode waves using THEMIS waveform data, J. Geophys. Res., 119, 8992-9003, 2014..
[9] Tao, X., Quanming Lu, S. Wang, and L. Dai, Effects of magnetic field configuration on the day-night asymmetry of chorus occurrence rate: A numerical study, Geophys. Res. Lett., 41, 6577-6582, doi:10.1002/2014GL061493, 2014..
[10] Gao, X. L., W. Li, R. M. Thorne, J. Bortnik, V. Angelopoulos, Quanming Lu, X. Tao, and S. Wang, New evidence for generation mechanisms of discrete and hiss-like whistler mode waves, Geophys. Res. Lett., 41, 4805–4811, doi:10.1002/ 2014GL060707, 2014..