Double Fourier sphere method

In mathematics, the double Fourier sphere (DFS) method is a simple technique that transforms a function defined on the surface of the sphere to a function defined on a rectangular domain while preserving periodicity in both the longitude and latitude directions.

Introduction

First, a function f ( x , y , z ) {\displaystyle f(x,y,z)} on the sphere is written as f ( λ , θ ) {\displaystyle f(\lambda ,\theta )} using spherical coordinates, i.e.,

f ( λ , θ ) = f ( cos λ sin θ , sin λ sin θ , cos θ ) , ( λ , θ ) [ π , π ] × [ 0 , π ] . {\displaystyle f(\lambda ,\theta )=f(\cos \lambda \sin \theta ,\sin \lambda \sin \theta ,\cos \theta ),(\lambda ,\theta )\in [-\pi ,\pi ]\times [0,\pi ].}

The function f ( λ , θ ) {\displaystyle f(\lambda ,\theta )} is 2 π {\displaystyle 2\pi } -periodic in λ {\displaystyle \lambda } , but not periodic in θ {\displaystyle \theta } . The periodicity in the latitude direction has been lost. To recover it, the function is "doubled up” and a related function on [ π , π ] × [ π , π ] {\displaystyle [-\pi ,\pi ]\times [-\pi ,\pi ]} is defined as

f ~ ( λ , θ ) = { g ( λ + π , θ ) , ( λ , θ ) [ π , 0 ] × [ 0 , π ] , h ( λ , θ ) , ( λ , θ ) [ 0 , π ] × [ 0 , π ] , g ( λ , θ ) , ( λ , θ ) [ 0 , π ] × [ π , 0 ] , h ( λ + π , θ ) , ( λ , θ ) [ π , 0 ] × [ π , 0 ] , {\displaystyle {\tilde {f}}(\lambda ,\theta )={\begin{cases}g(\lambda +\pi ,\theta ),&(\lambda ,\theta )\in [-\pi ,0]\times [0,\pi ],\\h(\lambda ,\theta ),&(\lambda ,\theta )\in [0,\pi ]\times [0,\pi ],\\g(\lambda ,-\theta ),&(\lambda ,\theta )\in [0,\pi ]\times [-\pi ,0],\\h(\lambda +\pi ,-\theta ),&(\lambda ,\theta )\in [-\pi ,0]\times [-\pi ,0],\\\end{cases}}}

where g ( λ , θ ) = f ( λ π , θ ) {\displaystyle g(\lambda ,\theta )=f(\lambda -\pi ,\theta )} and h ( λ , θ ) = f ( λ , θ ) {\displaystyle h(\lambda ,\theta )=f(\lambda ,\theta )} for ( λ , θ ) [ 0 , π ] × [ 0 , π ] {\displaystyle (\lambda ,\theta )\in [0,\pi ]\times [0,\pi ]} . The new function f ~ {\displaystyle {\tilde {f}}} is 2 π {\displaystyle 2\pi } -periodic in λ {\displaystyle \lambda } and θ {\displaystyle \theta } , and is constant along the lines θ = 0 {\displaystyle \theta =0} and θ = ± π {\displaystyle \theta =\pm \pi } , corresponding to the poles.

The function f ~ {\displaystyle {\tilde {f}}} can be expanded into a double Fourier series

f ~ j = n n k = n n a j k e i j θ e i k λ {\displaystyle {\tilde {f}}\approx \sum _{j=-n}^{n}\sum _{k=-n}^{n}a_{jk}e^{ij\theta }e^{ik\lambda }}

History

The DFS method was proposed by Merilees[1] and developed further by Steven Orszag.[2] The DFS method has been the subject of relatively few investigations since (a notable exception is Fornberg's work),[3] perhaps due to the dominance of spherical harmonics expansions. Over the last fifteen years it has begun to be used for the computation of gravitational fields near black holes[4] and to novel space-time spectral analysis.[5]

References

  1. ^ P. E. Merilees, The pseudospectral approximation applied to the shallow water equations on a sphere, Atmosphere, 11 (1973), pp. 13–20
  2. ^ S. A. Orszag, Fourier series on spheres, Mon. Wea. Rev., 102 (1974), pp. 56–75.
  3. ^ B. Fornberg, A pseudospectral approach for polar and spherical geometries, SIAM J. Sci. Comp, 16 (1995), pp. 1071–1081
  4. ^ R. Bartnik and A. Norton, Numerical methods for the Einstein equations in null quasispherical coordinates, SIAM J. Sci. Comp, 22 (2000), pp. 917–950
  5. ^ C. Sun, J. Li, F.-F. Jin, and F. Xie, Contrasting meridional structures of stratospheric and tropospheric planetary wave variability in the northern hemisphere, Tellus A, 66 (2014)


  • v
  • t
  • e