Fluctuations of the Earth's rotational speed and local residuals in astronomical obser vations might be related with motions of the solid Earth. In order to study these relations a comparison is made between variations of strain, which are observed at the Esashi Earth Tides Station (9h25m20.5s E, 39s08'53" N) and UT2-TAI, published by BIH, residuals of time, UTO-UTC, and latitude of the PZT and Danjon Astrolabe at Mizusawa (9
h24
m31.5
sE, 39°08'03"N) published by the IPMS, since Tune 1979. By using one year running mean and adjusting a constant rate, we obtain a good correlation between variations of the Earth's rotational speed and UTO-UTC of the Mizusawa PZT with the East-West component of strain. The residuals of latitude shows a phase lag of about 3 month to variations of the North-South component of strain. These relations suggest that variations of the Earth's rotational motions may be related with those of the density distributions near the Earth's surface.
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