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Quasi-geoid

Fig. 2.10. Telluroid, quasi-geoid, and reference ellipsoid (after Grushinsky). Fig. 2.10. Telluroid, quasi-geoid, and reference ellipsoid (after Grushinsky).
Later we will assume that the difference Wq— Uq is equal to zero. In this equation N is the height of the quasi-geoid, BiB. It also defines an excess of the level surface of the potential W, passing through the point A of the physical surface of the earth over corresponding level surface of the normal potential passing through the point Ai. Let us represent Equation (2.293) in the form... [Pg.132]

The importance of Equation (2.294) is that it establishes a relationship between the height anomaly, N, and the disturbing potential T at the same point of the earth. By definition, we have for the normal height h of the point A over a quasi-geoid... [Pg.132]

Thus, the determination of heights of the quasi-geoid N requires knowledge of the disturbing potential T on the physical surface of the earth. As in the case of the Stokes problem, in order to calculate N we have to determine the disturbing potential, which obeys some boundary condition on the physical surface of the earth instead of the surface of a geoid. This is the main advantage of a new approach. [Pg.132]


See other pages where Quasi-geoid is mentioned: [Pg.116]    [Pg.116]    [Pg.117]    [Pg.118]    [Pg.118]    [Pg.119]    [Pg.128]    [Pg.131]    [Pg.110]    [Pg.122]    [Pg.116]    [Pg.116]    [Pg.117]    [Pg.118]    [Pg.118]    [Pg.119]    [Pg.128]    [Pg.131]    [Pg.110]    [Pg.122]   
See also in sourсe #XX -- [ Pg.116 , Pg.117 , Pg.118 , Pg.128 , Pg.130 , Pg.131 ]




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