EXCITATION OF THE EARTH ROTATION |
The Earth
rotation undergoes changes under the influence of the lunisolar gravitational
torque and various geophysical excitations. Whereas the lunisolar forcing
can be well modelled as the sum of periodic terms through the Tides Generating
Potential (TGP) , the geophysical excitation remains unpredictable, and
has to be computed from various sets of geophysical data. In the following
page we present links to time series of :
- Atmospheric Angular Momentum (AAM) excitation functions (routinely derived) and atmospheric torque on the solid Earth
- Oceanic Angular Momentum (OAM)
- Hydrological Angular Momentum (HAM) excitation functions
- Core angular momentum (CAM) associated with core-mantle electromagnetic coupling
These forcings can be compared to the ones observed in polar motion
(PM) and lenght of day (LOD). Here below we provide also the "observed
excitation" for periods > 5-10 d, as computed from EOP combined
series "C04" for PM and LOD.
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Observed excitation
comparison with geophysical excitation
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IERS Global Geophysical Fluid Center
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Atmospheric excitation
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Oceanic excitation
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Hydrological excitation |
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Core-mantle coupling |
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