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Invariant latitude : ウィキペディア英語版
Dipole model of the Earth's magnetic field

The dipole model of the Earth's magnetic field is a first order approximation of the rather complex true Earth's magnetic field. Due to effects of the interplanetary magnetic field, and the solar wind, the dipole model is particularly inaccurate at high L-shells (e.g., above L=3), but may be a good approximation for lower L-shells. For more precise work, or for any work at higher L-shells, a more accurate model that incorporates solar effects, such as the Tsyganenko magnetic field model, is recommended.
==Equations==
The following equations describe the dipole magnetic field.
First, define B_0 as the mean value of the magnetic field at the magnetic equator on the Earth's surface. Typically B_0=3.12\times10^\ \textrm.
Then, the radial and azimuthal fields can be described as
B_r = -2B_0\left(\frac\right)^3\cos\theta
B_\theta = -B_0\left(\frac\right)^3\sin\theta
|B| = B_0\left(\frac\right)^3 \sqrt
where R_E is the mean radius of the Earth (approximately 6370 km), r is the radial distance from the center of the Earth (using the same units as used for R_E), and \theta is the azimuth measured from the north magnetic pole.
It is sometimes more convenient to express the magnetic field in terms of magnetic latitude and distance in earth radii. The magnetic latitude \lambda is measured northwards from the equator (analogous to geographic latitude) and is related to \theta by \lambda = \pi/2 - \theta. In this case, the radial and azimuthal components of the magnetic field (the latter still in the \theta direction, measured from the axis of the north pole) are given by
B_r = -\frac\sin\lambda
B_\theta = \frac\cos\lambda
|B| = \frac \sqrt
where R in this case has units of Earth radii (R = r/R_E).

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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