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Period and Qw of The Chandler Wobble
Authors:Robert G Currie
Institution:Magnetic Observatory of the CSIR Hermanus, Cape Province, South Africa
Abstract:A splined ILS/IPMS data set (1900–1973) from the most homogeneous values available has been analysed by the maximum entropy method of Burg. Principal conclusions are: (1) the spectral character of the Chandler wobble is a single broad peak, (2) the period is 432·95 ± 1·02 mean solar days and, (3) the Q w is 36±10. Measurements indicate that Q w is non- stationary in time.
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