Estimating the crustal power spectrum from vector Magsat data

The Earth's magnetic field can be subdivided into core and crustal componen ts and we seek to characterize the crustal part through its spatial power s pectrum, R-1. We process vector Magsat data to isolate the crustal field an d then invert power spectral densities of flight-local components along-tra ck for R-1 following O'Brien et al. [1999]. Our model, designated LPPC, is accurate up to approximately spherical harmonic degree 45 (lambda = 900 km) : this is the resolution limit of our data and suggests that global crustal anomaly maps constructed from vector Magsat data should not contain featur es with wavelengths less than 900 km. We find continental power spectra to be greater than oceanic ones and attribute this to the relative thicknesses of continental and oceanic crust.