Open AccessLunar and solar torques on the oceanic tides
Author(s) -
Ray Richard D.,
Bills Bruce G.,
Chao Benjamin Fong
Publication year - 1999
Publication title -
journal of geophysical research: solid earth
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/1999jb900165
Subject(s) - angular momentum , rotation (mathematics) , torque , ocean tide , earth's rotation , geodesy , atmospheric tide , altimeter , geology , satellite , tidal locking , physics , acceleration , geophysics , astronomy , thermosphere , ionosphere , classical mechanics , geometry , mathematics , thermodynamics
A general framework for calculating lunar and solar torques on the oceanic tides is developed in terms of harmonic constituents. Axial torques and their associated angular momentum and Earth rotation variations are deduced from recent satellite‐altimeter and satellite‐tracking tide solutions. Torques on the prograde components of the tide produce the familiar secular braking of the rotation rate. The estimated secular acceleration is approximately −1300 arcseconds/century 2 (less 4% after including atmospheric tides); the implied rate of change in the length of day is 2.28 milliseconds/century. Torques on the retrograde components of the tide produce periodic rotation variations at twice the tidal frequency. Interaction torques (for example, solar torques on lunar tides) generate a large suite of rotation‐rate variations at sums and differences of the original tidal frequencies. These are estimated for periods from 18.6 years to 6 hours. At subdaily periods the angular momentum variations are 5 to 6 orders of magnitude smaller than the variations caused by ocean tidal currents.