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The mean gravity disturbance generated by the geoid is given as (Tenzer et al. 2005) {overline{delta g}}^{NT}=frac{R}{4pi {H}^O}{displaystyle underset{varOmega^{hboxin {varOmega}_O}{int int}overline{K}left[R+{H}^O,psi, Rright]}times delta {g}^{NT}d{varOmega}^{hbox, (10).
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I don't mean gravity as in seriousness; I mean gravity as in the force that makes things fall downward rather than float upward.
Its great size means gravity has pulled it into a roughly spherical shape.
The asteroid's sheer size means gravity has pulled it into a near-spherical form.
Fig. 5. Gravity disturbance arising from precipitation.
Mean gravity norm formula.
A crossover analysis of the airborne gravity data indicates a mean gravity accuracy of 1.7 mGal.
This can be attributed to the contributions of gravitational attraction due to terrain roughness and geoid generated gravity disturbance.
The gravity generated by masses inside the geoid, can further be divided into the contribution of normal gravity and that of gravity disturbance due to masses inside the geoid (δg NT, e.g. Vaníček et al. 2004).
Finally, the analysis of crossover difference and the terrestrial gravity data are used to evaluate the accuracy of gravity disturbance estimates.
Helmert (1890) defined the approximate value for the mean gravity along the plumbline using Poincaré-Prey's gravity gradient.
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