It is demonstrated by a simple example and an elementary calculation that under certain conditions the moment of a dipole fitted to a distribution of magnetic potential is not necessarily the same as the dipole moment in the original magnetic potential. The dipole moment of the original magnetic potential which is a vector quantity specified by the first three coefficients in the spherical harmonic expansion is invariant, that is, independent of the choice of the origin of the coordinate system. Despite this, the moment of the fitted dipole can be different from the dipole moment in the original magnetic potential, depending on the choice of the optimum condition for the fitting. The optimum condition used here differs from that adopted in Schmidt's definition in that in the present definition coefficients of all degree and order are considered. The present definition becomes identical with Schmidt's definition when the harmonics of degrees higher than the quadrupole are truncated. When all the higher harmonics are included in the definition, we obtain a moment and location of the dipole different from those obtained from the classical method of Schmidt. Moreover, the obtained dipole moment and location are different from those deduced from a generalization of Schmidt's definition by inclusion of all harmonics to the infinite degree. For the present geomagnetic field, this method of analysis gives a dipole position shifted from the conventional eccentric dipole position roughly by 80km, and a moment reduced roughly by 20nT.
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