作者: D. P. Stern , N. A. Tsyganenko
DOI: 10.1029/91EO00359
关键词: Ionospheric dynamo region 、 Geophysics 、 Earth's magnetic field 、 L-shell 、 Plasma sheet 、 Physics 、 Mercury's magnetic field 、 Dipole model of the Earth's magnetic field 、 Magnetosphere 、 Ring current 、 Computational physics 、 General Earth and Planetary Sciences
摘要: When exploring a new country, one needs good map. The Earth's magnetosphere is such and its “maps” are models of the geomagnetic field. In essence they mathematical prescriptions implemented by computer which, given (x,y,z) point other supporting information, return point's expected magnetic components (Bx, By, Bz) [Tsyganenko, 1990]. At present, empirical field Tsyganenko [1987, 1989a, c; denoted henceforth as T87 T89] often used in various studies magnetosphere. Stern [1990] has devised modifications with current-free tail lobes plasma sheet that warps response to dipole tilt [Peredo Stern, 1991].