A spatiospectral localization approach to estimating potential fields on the surface of a sphere from noisy, incomplete data taken at satellite altitudes
Frederik J. Simons, F. A. Dahlen

TL;DR
This paper introduces a localized spherical basis derived from Slepian functions to improve potential field estimation on the Earth's surface from incomplete satellite data, especially in polar gap regions.
Contribution
We develop a spherical Slepian basis for localized analysis, connecting it to wavelets, and address computational challenges for irregular domains.
Findings
The basis effectively concentrates energy in specific regions of the sphere.
The method improves potential field estimates in data-sparse polar gaps.
Connections to wavelets reveal asymptotic self-similarity.
Abstract
Satellites mapping the spatial variations of the gravitational or magnetic fields of the Earth or other planets ideally fly on polar orbits, uniformly covering the entire globe. Thus, potential fields on the sphere are usually expressed in spherical harmonics, basis functions with global support. For various reasons, however, inclined orbits are favorable. These leave a "polar gap": an antipodal pair of axisymmetric polar caps without any data coverage, typically smaller than 10 degrees in diameter for terrestrial gravitational problems, but 20 degrees or more in some planetary magnetic configurations. The estimation of spherical harmonic field coefficients from an incompletely sampled sphere is prone to error, since the spherical harmonics are not orthogonal over the partial domain of the cut sphere. Although approaches based on wavelets have gained in popularity in the last decade, we…
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