Atmospheric acceleration and Earth-expansion deceleration of the Earth rotation
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作者:
Wenbin Shen
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Department of Geophysics,School of Geodesy and Geomatics,Key Laboratory of Geospace Environment and Geodesy of Ministry of Education, Wuhan UniversityDepartment of Geophysics,School of Geodesy and Geomatics,Key Laboratory of Geospace Environment and Geodesy of Ministry of Education, Wuhan University
Wenbin Shen
[1
]
Sung-Ho Na
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机构:Department of Geophysics,School of Geodesy and Geomatics,Key Laboratory of Geospace Environment and Geodesy of Ministry of Education, Wuhan University
Sung-Ho Na
[2
]
机构:
[1] Department of Geophysics,School of Geodesy and Geomatics,Key Laboratory of Geospace Environment and Geodesy of Ministry of Education, Wuhan University
Previous studies suggest that tidal friction gives rise to the secular deceleration of the Earth rotation by a quantity of about 2.25 ms/cy. Here we just consider additional contributions to the secular Earth rotation deceleration. Atmospheric solar semi-diurnal tide has a small amplitude and certain amount of phase lead. This periodic global air-mass excess distribution exerts a quasi-constant torque to accelerate the Earth’s spin rotation. Using an updated atmospheric tide model, we re-estimate the amounts of this atmospheric acceleration torque and corresponding energy input, of which the associated change rate in LOD(length of day) is-0.1 ms/cy. In another aspect, evidences from space-geodesy and sea level rise observations suggest that Earth expands at a rate of 0.35 mm/yr in recent decades, which gives rise to the increase of LOD at rate of 1.0 ms/cy. Hence, if the previous estimate due to the tidal friction is correct, the secular Earth rotation deceleration due to tidal friction and Earth expansion should be 3.15 ms/cy.