The time-average palaeomagnetic field during Upper Tertiary times has as its source a dipole which is offset 285 ± 74 km north of the equatorial plane, but which remains axial. Modification of pole positions, taking the offset source dipole into account, suggests that no significant (> 1°) continental drift, polar wandering, or very long-term dipole wobble have been present during the Upper Tertiary. Four different analyses of the data have shown the dipole offset to be a real phenomenon, not due to peculiarities of the method of calculation.
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R. L. Wilson (1971) studied this question.
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