2009
DOI: 10.1007/978-3-540-85112-7
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Spherical Functions of Mathematical Geosciences

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Cited by 182 publications
(63 citation statements)
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“…the spherical harmonics are dense in the function space L 2 (S) [37,38]. Therefore, the scalar field ψ can be represented as the series expansion…”
Section: A (Vector) Spherical Harmonics Expansionmentioning
confidence: 99%
“…the spherical harmonics are dense in the function space L 2 (S) [37,38]. Therefore, the scalar field ψ can be represented as the series expansion…”
Section: A (Vector) Spherical Harmonics Expansionmentioning
confidence: 99%
“…This is the reason why they do not show any space localization, but ideal frequency (momentum) localization (for a more detailed description see Freeden and Schreiner 2009). This property makes outer harmonics difficult to use for high resolution modeling at local scale.…”
Section: Tensorial Runge-walsh Approximation Propertymentioning
confidence: 95%
“…(for explicit representations see Freeden and Schreiner (2009)). Note that, for sufficiently smooth tensor fields f : → R 3 ⊗ R 3 of the form…”
Section: Tensor Spherical Harmonicsmentioning
confidence: 99%
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