Continuous observations of the earth tides with Verbaandert-Melchior pendulums at Akagane Observation Station was commenced in 1967. Hourly reading values of the records have been sent every three months to the International Centre of the Earth Tides at the Royal Observatory of Belgium. On the other hand, the data have beenn analyzed successively by means of Lecolazet's method in our observatory.
Tidal factors of four main waves were determined by the analysis, but they were very peculiar values in comparison with that of global values of 0.60.8. As shown in Table II, γ of the diurnal waves were larger than 1.0, on the contrary, that of the semidiurnal waves were too small. After detailed examinations it was considered to be affected mainly by the oceanic tides, because the observation station was located merely 50 kilometers distant from the pacific coast.
Attraction (A) of oceanic waters, the flexure (B) of the earth's crust due to the water and the potential variation (C) due to the earth's flexure were calculated using co-tidal maps under the following assumptions.
For the first approximation, the Boussinesq's formula for solving the deformation of the earth due to surface load was applied. Then, the total oceanic term was expressed as, A+B+C =(1+υ+ε)A. The value of v increases proportional to the depth, and it iss expressed as the hyperbolic function,
υ=C
2/γ+C
1,
where r denotes angle distance in degree between the observation station and the point mass. C
1 and C
2 depend on underground structure and distribution of the rigidity.
In this paper, the values of C
1, C
2 and ε are adopted as 12.6, 3.0 and 0.5 respectively, which were determined by Dr. Nishimura.
Consequently, the total oceanic term was expressed as follows,
A+B+C=(1+12.6/γ+3.0-0.5)·A.
The corrected values of ?A for M
2 wave became larger than that of previous values as shown in Table IV. The first approximation shows good result, and further investigations for local indirect effect of oceanic tides are now continued.
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