Li W H, Raeder J, Thomsen M F, et al. Solar wind plasma entry into the magnetosphere under northward IMF conditions. J. Geophys. Res., 2008, 113: A04204, doi: 10. 1029/2007JA012604.
[2]
Shi Q Q, Zong Q G, Zhang H, et al. Cluster observations of the entry layer equatorward of the cusp under northward interplanetary magnetic field. J. Geophys. Res., 2009, 114: A12219, doi: 10. 1029/2009JA014475.
[3]
Nishida A, Mukai T, Yamamoto T, et al. A unified model of the magnetotail convection in geomagnetically quiet and active times. J. Geophys. Res., 1998, 103(A3): 4409-4418, doi:10.1029/97JA01617.
[4]
Petrukovich A A, Baumjohann W, Nakamura R, et al. Plasma sheet structure during strongly northward IMF. J. Geophys. Res., 2003, 108(A6): 1258, doi: 10. 1029/2002JA009738.
[5]
Safránková J, Měrka J, Němecek Z. Plasma flow across the cusp-magnetosheath boundary under northward IMF. Adv. Space Res., 2002, 30(12): 2787-2792.
[6]
郭九苓, 沈超, 刘振兴. IMF北向时磁层顶重联的模拟研究. 地球物理学进展, 2013, 28(2):540-544. Guo J L, Shen C, Liu Z X. Simulation of magnetic reconnection on the magnetopause under northward IMF condition. Progress in Geophysics (in Chinese), 2013, 28(2): 540-544.
[7]
Tsyganenko N A, Mukai T. Tail plasma sheet models derived from Geotail particle data. J. Geophys. Res., 2003, 108(A3): 1136, doi: 10.1029/2002JA009707.
[8]
Baumjohann W, Paschmann G, Gattell C A. Average plasma properties in the central plasma sheet. J. Geophys. Res., 1989, 94(A6): 6597-6606.
[9]
Terasawa T, Fujimoto M, Mukai T, et al. Solar wind control of density and temperature in the near-Earth plasma sheet: WIND-GEOTAIL collaboration. Geophys. Res. Lett., 1997, 24(8): 935-938.
[10]
Fujimoto M, Terasawa T, Mukai T, et al. Plasma entry from the flanks of the near-Earth magnetotail: Geotail observations. J. Geophys. Res., 1998, 103(A3): 4391-4408.
[11]
Fujimoto M, Mukai T, Matsuoka A, et al. Multi-point observations of cold-dense plasma sheet and its relation with tail-LLBL. Adv. Space Sci., 2000, 25(7-8): 1607-1616.
[12]
Kessel R L, Chen S H, Green J L, et al. Evidence of high-latitude reconnecting during northward IMF: Hawkeye observations. Geophys. Res. Lett., 1996, 23(5): 583-586.
[13]
Hasegawa H, Retinò A, Vaivads A, et al. Retreat and reformation of X-line during quasi-continuous tailward-of-the-cusp reconnection under northward IMF. Geophys. Res. Lett., 2008, 35: L15104, doi: 10.1029/2008GL034767.
[14]
Taylor M G G T, Lavraud B, Escoubet C P, et al. The plasma sheet and boundary layers under northward IMF: A multi-point and multi-instrument perspective. Adv. Space Res., 2008, 41(10): 1619-1629.
[15]
Song P, Russell C T. Model of the formation of the low-latitude boundary layer for strongly northward interplanetary magnetic field. J. Geophys. Res., 1992, 97(A2): 1411-1420.
[16]
Li W H, Raeder J, Dorelli J, et al. Plasma sheet formation during long period of northward IMF. Geophys. Res. Lett., 2005, 32: L12S08, doi: 10. 1029/2004GL021524.
[17]
Parker E N. Dynamics of the interplanetary gas and magnetic fields. Astrophys. J., 1958, 128: 664-676.
[18]
Guo J L, Liu Z X. Simulation of the dawn-dusk magnetosheath asymmetry under quasi-steady states. Chinese Sci. Bull., 2005, 50(4): 341-346.
[19]
郭九苓, 王继业, 刘振兴. 不考虑磁层顶磁重联的全球三维MHD模型. 地球物理学报, 2005, 48(1): 7-12. Guo J L, Wang J Y, Liu Z X. No magnetic reconnection at the magnetopause: A new 3D MHD simulation model. Chinese J. Geophys. (in Chinese), 2005, 48(1): 7-12.
[20]
郭九苓, 沈超, 刘振兴. IMF北向与南向时地球磁尾等离子片粒子注入机制. 科学通报, 2012, 57(34): 3295-3300. Guo J L, Shen C, Liu Z X. Simulation and comparison of particle entering into the plasma sheet under north- and southward IMF conditions. Chinese Sci. Bull. (in Chinese), 2012, 57(34): 3295-3300.
[21]
Raeder J, Vaisberg O, Smirnov V, et al. Reconnection driven lobe convection: Interball tail probe observations and global simulations. J. Atmos. Terr. Phys., 2000, 62(10): 833-849.
[22]
Raeder J, Mcpherron R L, Frank L A, et al. Global simulation of the Geospace Environment Modeling substorm challenge event. J. Geophys. Res., 2001, 106(A1): 381-395.
[23]
Fuselier S A, Petrinec S M, Trattner K J. Antiparallel magnetic reconnection rates at the Earth''s magnetopause. J. Geophys. Res., 2010, 115, A10207, doi: 10. 1029/2010JA015302.
[24]
Taguchi S, Hoffman R A. Ionospheric plasma convection in the midnight sector for northward interplanetary magnetic field. Journal of Geomagnetism and Geoelectricity, 1996, 48(5): 925-933.
[25]
Cowley S W H. Magnetospheric asymmetries associated with the y-component of the IMF. Planet. Space Sci., 1981, 29(1): 79-96.
[26]
Kaymaz Z, Siscoe G L, Luhmann J G, et al. Interplanetary magnetic field control of magnetotail magnetic field geometry: IMP 8 observations. J. Geophys. Res., 1994, 99(A6): 11113-11126, doi: 10.1029/94JA00300.
[27]
Elsen R K, Winglee R M. The average shape of the magnetopause: A comparison of three-dimensional global MHD and empirical models. J. Geophys. Res., 1997,102(A3): 4799-4819.
[28]
Powell K G, Roe P L, Linde T J, et al. A solution-adaptive upwind scheme for ideal magnetohydrodynamics. J. Comput. Phys., 1999, 154(2): 284-309.
