
Period and Q w of The Chandler Wobble
Author(s) -
Currie Robert G.
Publication year - 1974
Publication title -
geophysical journal of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.302
H-Index - 168
eISSN - 1365-246X
pISSN - 0016-8009
DOI - 10.1111/j.1365-246x.1974.tb04115.x
Subject(s) - speed wobble , homogeneous , geodesy , maximum entropy method , period (music) , physics , geology , mathematics , statistical physics , classical mechanics , acoustics
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.