Maxwell's multipoles are a natural geometric characterization of real functions on the sphere (with fixed ⌊). The correlations between multipoles for Gaussian random functions are calculated by mapping the spherical functions to random polynomials. In the limit of high ⌊, the 2-point function tends to a form previously derived by Hannay in the analogous problem for the Majorana sphere. The application to the cosmic microwave background (CMB) is discussed
Random dispersions of spheres are useful and appropriate models for a wide class of particulate rand...
We present efficient algorithms for computing the N-point correlation functions (NPCFs) of random fi...
In this paper we study the asymptotic behavior of the angular bispectrum of spherical random field...
A Gaussian isotropic stochastic field on a 2D-sphere is characterized by either its covariance funct...
We establish weak convergence of the empirical process on the spherical harmonics of a Gaussian rand...
The well-known assumption of horizontal plane wave propagation is investigated and evidence suggests...
Context: Two-point correlation functions are used throughout cosmology as a measure for the statisti...
International audienceWhen dealing with modal representations of the Green's function of a complex m...
We consider the correlation structure of the random coefficients for a class of wavelet systems on t...
Any eigenfunction of the Laplacian on a sphere is given in terms of a unique set of directions: thes...
A Gaussian distribution of cosmic microwave background temperature fluctuations is a generic predict...
In this paper we study the solutions of different forms of fractional equations on the unit sphere S...
This paper investigates spatial data on the unit sphere. Traditionally, isotropic Gaussian random fi...
Correlation functions are an omnipresent tool in astrophysics, and they are routinely used to study ...
Measurements of correlation functions and their comparison with theoretical models are often employe...
Random dispersions of spheres are useful and appropriate models for a wide class of particulate rand...
We present efficient algorithms for computing the N-point correlation functions (NPCFs) of random fi...
In this paper we study the asymptotic behavior of the angular bispectrum of spherical random field...
A Gaussian isotropic stochastic field on a 2D-sphere is characterized by either its covariance funct...
We establish weak convergence of the empirical process on the spherical harmonics of a Gaussian rand...
The well-known assumption of horizontal plane wave propagation is investigated and evidence suggests...
Context: Two-point correlation functions are used throughout cosmology as a measure for the statisti...
International audienceWhen dealing with modal representations of the Green's function of a complex m...
We consider the correlation structure of the random coefficients for a class of wavelet systems on t...
Any eigenfunction of the Laplacian on a sphere is given in terms of a unique set of directions: thes...
A Gaussian distribution of cosmic microwave background temperature fluctuations is a generic predict...
In this paper we study the solutions of different forms of fractional equations on the unit sphere S...
This paper investigates spatial data on the unit sphere. Traditionally, isotropic Gaussian random fi...
Correlation functions are an omnipresent tool in astrophysics, and they are routinely used to study ...
Measurements of correlation functions and their comparison with theoretical models are often employe...
Random dispersions of spheres are useful and appropriate models for a wide class of particulate rand...
We present efficient algorithms for computing the N-point correlation functions (NPCFs) of random fi...
In this paper we study the asymptotic behavior of the angular bispectrum of spherical random field...