[1] |
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[C]//COSPAR Colloquia series. Pergamon:COSPAR, 2002, 12:127-135
|
[2] |
DMITRIEV A V, CHAO J K, WU D J. Comparative study of bow shock models using WIND and Geotail observations[J]. J. Geophys. Res., 2003, 108(A12):1464
|
[3] |
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
|
[4] |
VERIGIN M I, KOTOVA G A, SLAVIN J, et al. Analysis of the 3-D shape of the terrestrial bow shock by Interball/Magion 4 observations[J]. Adv. Space Res., 2001, 28(6):857-862
|
[5] |
HU Huiping, LU Jianyong, ZHOU Quan, et al. Simulation of three-dimensional Earth's bow shock[J]. Chin. J. Space Sci., 2015, 35(1):1-8(胡慧萍,吕建永,周全,等.地球弓激波的三维模拟[J].空间科学学报, 2015, 35(1):1-8)
|
[6] |
CHAPMAN J F, CAIRNS I H, LYON J G, et al. MHD simulations of Earth's bow shock:interplanetary magnetic field orientation effects on shape and position[J]. J. Geophys. Res.:Space Phys., 2004, 109(A4):A04215. DOI: 10.1029/2003JA010235
|
[7] |
VERIGIN M, SLAVIN J A, KOTOVA G, GOMBOSI T.Planetary bow shocks:asymptotic MHD Mach cones[J]. Earth Planets Space, 2003, 55:33-38
|
[8] |
PETRINEC S M, RUSSELL C T. An examination of the effect of dipole tilt angle and cusp regions on the shape of the dayside magnetopause[J]. J. Geophys. Res.:Space Phys., 1995, 100(A6):9559-9566
|
[9] |
ZHOU X W, RUSSELL C T. The location of the highlatitude polar cusp and the shape of the surrounding magnetopause[J]. J. Geophys, Res., 1997, 89:11048-11052
|
[10] |
TSYGANENKO N A. Modeling of twisted/warped magnetospheric configurations using the general deformation method[J]. J. Geophys. Res.:Space Phys., 1998, 103(A10):23551-23563
|
[11] |
ŠAFRÁNKOVÁ J, DUŠÍK Š, NěME?EK Z. The shape and location of the high-latitude magnetopause[J]. Adv. Space Res., 2005, 36(10):1934-1939
|
[12] |
BOARDSEN S A, EASTMAN T E, SOTIRELIS T, et al. An empirical model of the high-latitude magnetopause[J]. J. Geophys. Res.:Space Phys., 2000, 105(A10):23193-23219
|
[13] |
LIN R L, ZHANG X X, LIU S Q, et al. A threedimensional asymmetric magnetopause model[J]. J. Geophys. Res., 2010, 115:A04207
|
[14] |
LIU Z Q, LU J Y, WANG C, et al. A three-dimensional high Mach number asymmetric magnetopause model from global MHD simulation[J]. J. Geophys Res.:Space Phys., 2015, 120:5645-5666
|
[15] |
MERKA J, SZABO A. Bow shock's geometry at the magnetospheric flanks[J]. J. Geophys. Res., 2004, 109(A12):A12224. DOI: 10.1029/2004JA010567
|
[16] |
JELÍNEK K, NěM?CEK Z, ŠAFRÁNKOVÁ J, et al. Influence of the tilt angle on the bow shock shape and location[J]. J. Geophys. Res., 2008, 113(A5):521-532
|
[17] |
FORMISANO V. Orientation and shape of the Earth's bow shock in three dimensions[J]. Planet. Space Sci., 1979, 27(9):1151-1161
|
[18] |
PEREDO M, SLAVIN J A, MAZUR E, et al. Threedimensional position and shape of the bow shock and their variation with Alfvenic, sonic and magnetosonic Mach numbers and interplanetary magnetic field orientation[J]. J. Geophys. Res.:Space Phys., 1995, 100(A5):7907-7916
|
[19] |
RUSSELL C T, PETRINECS M. Towards an MHD theory for the standoff distance of Earth's bow shock[J]. Geophys. Res. Lett., 1996, 23(3):309-310
|
[20] |
LIU Z Q, LU J Y, KABIN K, et al. Dipole tilt control of the magnetopause for southward IMF from global magnetohydrodynamic simulations[J]. J. Geophys. Res.:Space Phys., 2012, 117(A7):282-292
|