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All available surface and airborne observations of magnetic declination from 1955.0 and of vector force components from 1945.0 up to mid-June 1964 have been brought up to the epoch 1965.0. The reduced data have been subjected to a series of four spherical harmonic analyses in such a way that the apparent external part has been reduced whilst retaining a reasonable fit to the observations. Three similar analyses have been performed on the extrapolated time derivatives of X, Y and Z at 113 magnetic observatories. Results are given in terms of Schmidt quasi-normal coefficients up to the 8th order and degree for the main field and up to the 6th order and degree for its rate of change.
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Leaton et al. (1965) studied this question.
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