## Abstract A new non‐polar spherical co‐ordinate system for the three‐dimensional space is introduced. The co‐ordinate system is composed of six local co‐ordinate systems mapped from six faces of a cube on to the 2‐sphere. Weakly orthogonal and orthogonal spherical harmonics are constructed in thi
Fast spin ±2 spherical harmonics transforms and application in cosmology
✍ Scribed by Y. Wiaux; L. Jacques; P. Vandergheynst
- Book ID
- 104021680
- Publisher
- Elsevier Science
- Year
- 2007
- Tongue
- English
- Weight
- 474 KB
- Volume
- 226
- Category
- Article
- ISSN
- 0021-9991
No coin nor oath required. For personal study only.
✦ Synopsis
A fast and exact algorithm is developed for the spin ±2 spherical harmonics transforms on equi-angular pixelizations on the sphere. It is based on the Driscoll and Healy fast scalar spherical harmonics transform. The theoretical exactness of the transform relies on a sampling theorem. The associated asymptotic complexity is of order OðL 2 log 2 2 LÞ, where 2L stands for the square-root of the number of sampling points on the sphere, also setting a band limit L for the spin ±2 functions considered. The algorithm is presented as an alternative to existing fast algorithms with an asymptotic complexity of order OðL 3 Þ on other pixelizations. We also illustrate these generic developments through their application in cosmology, for the analysis of the cosmic microwave background (CMB) polarization data.
📜 SIMILAR VOLUMES