Wang Jingsong, Lü Jianyong. Space Weather[M]. Beijing: China Meteorological Press, 2010. In Chinese (王劲松, 吕建永. 空间天气学[M]. 北京: 气象出版社, 2010)
[2]
Fairfield D H. Average and unusual locations of the Earth''s magnetopause and bow shock[J]. J. Geophys. Res., 1971, 76:6700
[3]
Slavin J A, Holzer R E. Solar wind flow about the terrestrial planets[J]. J. Geophys. Res., 1981, 86:11401-11418
[4]
Farris M H, Petrinec S M, Russell C T. The thickness of the magnetosheath-Constraints on the polytropic index[J]. Geophys. Res. Lett., 1991, 18:1821-1824
[5]
Russell C T, Zhang T L. Unusually distant bow shock encounters at Venus[J]. Geophys. Res. Lett., 1992, 19:833
[6]
Verigin M, Kotova G A, Shutte N, et al. Quantitative model of the Martian magnetopause shape and its variation with the solar wind ram pressure based on Phobos-2 observations[J]. J. Geophys. Res., 1997, 102(A2):2147-2156
[7]
Cairns I H, Lyon J G. MHD simulations of Earth''s bow shock at low Mach numbers: Standoff distances[J]. J. Geophys. Res., 1995, 10:17173-17180
[8]
Peredo M, Slavin J A, Mazur E, et al. Three-dimensional position and shape of the bow shock and their variation with Alfvénic, sonic, and magnetosonic Mach numbers and the interplanetary magnetic field orientation[J]. J. Geophys. Res., 1995, 100:7907-7916
[9]
Chapman J F, Cairns I H. Three-dimensional modeling of Earth''s bow shock: Shock shape as a function of Alfvén Mach number[J]. J. Geophys. Res., 2003, 108:1174
[10]
Chapman J F, Cairns I H. MHD simulations of Earth''s bow shock: Interplanetary magnetic field orientation effects on shape and position[J]. J. Geophys. Res., 2004, 109:A04215
[11]
Julian H, Seiff A, Canning T N, et al. Gas Dynamics in Space Exploration[M]. Washington: The United States Government Printing Office, 1962
[12]
Spreiter J R, Briggs B R. Theoretical determination of the form of the boundary of the solar corpuscular stream produced by interaction with the magnetic dipole field of the Earth[J]. J. Geophys. Res., 1962, 67:37
[13]
Farris M H, Russell C T. Determining the standoff distance of the bow shock: Mach number dependence and use of models[J]. J. Geophys. Res., 1994, 99:17681-17689
[14]
Lavraud B, Borovsky J E. Altered solar wind-magnetosphere interaction at low Mach numbers: Coronal mass ejections[J]. J. Geophys. Res., 2008, 113:A00B08
[15]
Bennett L, Kivelson M G, Khurana, K K, et al. A model of the Earth''s distant bow shock[J]. J. Geophys. Res., 1997, 102:26927, doi: 10.1029/97JA01906
[16]
Chao J K, Wu D J, Lin C H, et al. Models for the size and shape of the Earth''s magnetopause and bow shock[J]. Proc. COSPAR Colloq., 2002, 12:127-135
[17]
Hu Youqiu, Peng Zhong, Wang Chi. Rotational asymmetry of Earth''s bow shock[J]. Chin. J. Geophys., 2010, 53(4):773-781. In Chinese (胡友秋, 彭忠, 王赤. 地球弓激波的旋转飞对称性[J]. 地球物理学报, 2010, 53(4):773-781)
[18]
Tóth G, Sokolov I V, Gombosi T I, et al. Space Weather Modeling Framework: A new tool for the space science community[J]. J. Geophys. Res., 2005, A12226
[19]
Powell K G, Roe P L, Linde T J, et al. A solution-adaptive upwind scheme for ideal magnetohydrodynamics[J]. J. Comput. Phys., 1999, 154:284-309
[20]
De Zeeuw D L, Sazykin S, Wolf R A, et al. Coupling of a global MHD code and an inner magnetospheric model: Initial results[J]. J. Geophys. Res., 2004, A12219
[21]
Lü J Y, Liu Z Q, Kabin K, Jing H, Zhao M X, Wang Y. The IMF dependence of the magnetopause from global MHD/simulations[J]. J. Geophys. Res., 2013, 118:3113-3125
[22]
Verigin M, Kotova G A, Szabo A, et al. Wind observations of the terrestrial bow shock: 3-D shape and motion[J]. Earth Planet. Space, 2001, 53(10):1001-1009