Gravity IV: Dipole moment of density anomaly: the ambiguity

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Presentation transcript:

Gravity IV: Dipole moment of density anomaly: the ambiguity We want to know: But actually, gravity anomaly alone cannot provide this information. The ambiguity of a buried sphere: Note the trade off between a and .

Dipole moment of density anomaly: the ambiguity The same gravity anomaly may be explained by different anomalous bodies, having different shapes and located at different depths: measured gravity anomaly Near surface very elongated body Shallow elongated body Deep sphere

Dipole moment of density anomaly: the ambiguity bathymetry free-air The observed Bouguer anomaly above the Mid-Atlantic Ridge may be explained equally well with deep models with small density contrast or shallow models with greater density contrast. deep model Bouguer anomaly 3 shallow modles Figure from Fowler

Dipole moment of density anomaly: isostatic equilibrium We have seen that gravity anomaly shows whether a given region is in a state of isostatic equilibrium. A rule of thumb: A region is in isostatic equilibrium if the Bouguer anomaly is a mirror image of the topography. Figure from Fowler But the Bouguer anomaly does not provide further information regarding the mass distribution, i.e. whether the region in question is in isostatic equilibrium according to Airy or Pratt hypotheses?

Dipole moment of density anomaly: dipole moment of density distribution We have seen that the gravity anomaly due to a horizontal layer of thickness y is: thus the gravity potential of this layer is: The dipole moment of density distribution is just: We shall see that it is the dipole moment of density distribution, which contains information regarding the mass distribution, and may help to discriminate between the two isostatic models.

Dipole moment of density anomaly: gravity potential U=Uobs U=Uref Combining this with the expression on the previous slide leads to:

Dipole moment of density anomaly: Airy versus Pratt In areas of isostatic equilibrium, we would wish to know whether mass is distributed according to Airy or Pratt models. Airy (positive topography): Pratt (positive topography):

Dipole moment of density anomaly: Airy versus Pratt Pratt (positive topography): +y Replacing with leads to: Note the linear relation between N and h.

Dipole moment of density anomaly: Airy versus Pratt Airy (positive topography): +y Replacing with leads to: Note the NON-LINEAR relation between N and h.

Dipole moment of density anomaly: Airy versus Pratt N versus h for Airy and Pratt models. Airy model implies a nearly factor of 3 difference between N/h on-land and off-shore. Pratt Airy Figure from Turcotte and Schubert

Dipole moment of density anomaly: Airy versus Pratt A comparison between Airy-predicted and measured geoid anomaly across the Atlantic continental margin of N. America. It follows from this comparison that the continental margin is in a state of isostatic equilibrium according to Airy model. Figure from Turcotte and Schubert

Dipole moment of density anomaly: Airy versus Pratt At what direction does the Pacific plate moves?

Dipole moment of density anomaly: Airy versus Pratt Dependence of the observed geoid anomaly on bathymetry across the Hawaiian swell and across the Bermuda swell compared with the predicted anomaly according to Airy and Pratt models. Good agreement is obtained for Pratt model with a compensation depth of 100 km. Figure from Turcotte and Schubert If we accept the Pratt model to be applicable, the conclusion is that the mantle rocks beneath these swells have anomalously low density down to a depth of 100 km.