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Outline

3D gravity inversion by planting anomalous densities

2011

Abstract

This paper presents a novel gravity inversion method for estimating a 3D density-contrast distribution defined on a grid of prisms. Our method consists of an iterative algorithm that does not require the solution of a large equation system. Instead, the solution grows systematically around user-specified prismatic elements called "seeds". Each seed can have a different density contrast, allowing the interpretation of multiple bodies with different density contrasts and interfering gravitational effects. The compactness of the solution around the seeds is imposed by means of a regularizing function. The solution grows by the accretion of neighboring prisms of the current solution. The prisms for the accretion are chosen by systematically searching the set of current neighboring prisms. Therefore, this approach allows that the columns of the Jacobian matrix be calculated on demand. This is a known technique from computer science called "lazy evaluation", which greatly reduces the demand of computer memory and processing time. Test on synthetic data and on real data collected over the ultramafic Cana Brava complex, central Brazil, confirmed the ability of our method in detecting sharp and compact bodies.

References (7)

  1. Camacho, A. G., Montesinos, F. G. and Vieira, R., 2000, Gravity inversion by means of growing bodies: Geophysics, Vol. 65, No. 1, p95-101.
  2. Carminatti, M. G., Marangoni, Y. R., Correia, C. T., 2003, Modelagem gravim étrica do complexo de Cana Brava e Figure 5: Gravity data of the Cana Brava complex. a) Residual Bouguer anomaly map, contour of the outcropping portion (black lines), and seeds used in the inversion (blue, green, and red circles). Seeds shown in blue and green have a density contrast of 0.27 g.cm -3 and the ones shown in red have 0.39 g.cm -3 . Seeds in blue and red where placed at z = 0 km and seeds in green at z = 2 km. b) Fit of the data predicted by the inversion (red lines) against the residual Bouguer anomaly map (blue lines). Data points are shown as + symbols. sequ ência de Palmeir ópolis, GO: Revista Brasileira de Geoci ências, Vol. 33, p245-254.
  3. Li, Y., Oldenburg, D. W., 1998, 3-D inversion of gravity data: Geophysics, Vol. 63, No .1, p109-119.
  4. Nagy, D., Papp, G., Benedek, J., 2000, The gravitational potential and its derivatives for the prism: Journal of Geodesy, Vol. 74, p552-560.
  5. Portniaguine, O., Zhdanov, M. S., 2002, 3-D magnetic inversion with data compression and image focusing: Geophysics, Vol. 67, No. 5, p1532-1541.
  6. Ren é, R. M., 1986, Gravity inversion using open, reject, and "shape-of-anomaly" fill criteria: Geophysics, Vol. 51, No. 4, p988-994.
  7. Silva Dias, F. J. S., Barbosa, V.C.F., Silva, J.B.C, 2009, 3D gravity inversion through an adaptive-learning procedure: Geophysics, Vol. 74, No. 3, pI9-I21.