2007
DOI: 10.1007/s00041-006-6013-0
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Wavelets on the Two-Sphere and Other Conic Sections

Abstract: ABSTRACT. We survey the construction of the continuous wavelet transform (CWT) on the two-sphere. Then we discuss the discretization of the spherical CWT, obtaining various types of discrete frames. Finally we give some indications on the construction of a CWT on other conic sections.

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Cited by 28 publications
(43 citation statements)
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“…(This is analogous to the usual situation in which all the wavelets at each scale are translates of each other.) Again, w t,x is given by (2). On the sphere S 2 , we have…”
Section: Lemmas On Zonal Harmonicsmentioning
confidence: 99%
See 1 more Smart Citation
“…(This is analogous to the usual situation in which all the wavelets at each scale are translates of each other.) Again, w t,x is given by (2). On the sphere S 2 , we have…”
Section: Lemmas On Zonal Harmonicsmentioning
confidence: 99%
“…In recent years a rapidly growing literature has focussed on the construction of wavelet systems on the sphere, see for instance [1][2][3]48] and the references therein. These attempts have been motivated by strong interest from the applied sciences, for instance in the areas of Geophysics, Medical Imaging and especially Cosmology/Astrophysics.…”
Section: Introductionmentioning
confidence: 99%
“…40 In the sequel of this section, we shall give a rapid overview of the series of works mentioned above, following mostly Ref. 7. As a general reference on 2-D wavelets, we use our recent monograph.…”
Section: The Cwt On the Two-spherementioning
confidence: 99%
“…7 (1) Unlike the usual 2-D CWT, which is fully covariant with respect to translations, rotations and dilations, the spherical CWT is only partially covariant. It is covariant under motions on S 2 : for any o ∈ SO(3), the transform of the rotated signal f (…”
Section: Additional Propertiesmentioning
confidence: 99%
“…In particular, wavelets on the sphere (Antoine & Vandergheynst 1998, 1999Baldi et al 2009;Marinucci et al 2008;McEwen et al 2006a;Narcowich et al 2006;Starck et al 2006a;Wiaux et al 2006aWiaux et al , 2005Wiaux et al , 2007Wiaux et al , 2008aYeo et al 2008) have been applied very successfully to problems in astrophysics and cosmology, where data-sets are increasingly large and need to be analysed at high resolution in order to confront accurate theoretical predictions (e.g. Barreiro et al 2000;Basak & Delabrouille 2012;Cayón et al 2001;Deriaz et al 2012;Labatie et al 2012;Lan & Marinucci 2008;McEwen et al 2006bMcEwen et al , 2007aMcEwen et al ,b, 2008Pietrobon et al 2008;Starck et al 2006b;Schmitt et al 2010;Vielva et al 2004Vielva et al , 2006aVielva et al ,b, 2007Wiaux et al 2006bWiaux et al , 2008b.…”
Section: Introductionmentioning
confidence: 99%