Projected normal distribution

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In directional statistics, the projected normal distribution (also known as offset normal distribution, angular normal distribution or angular Gaussian distribution)Template:SfnTemplate:Sfn is a probability distribution over directions that describes the radial projection of a random variable with n-variate normal distribution over the unit (n-1)-sphere.

Definition and properties

Given a random variable ๐‘ฟโˆˆโ„n that follows a multivariate normal distribution ๐’ฉn(๐,๐œฎ), the projected normal distribution ๐’ซ๐’ฉn(๐,๐œฎ) represents the distribution of the random variable ๐’€=๐‘ฟโ€–๐‘ฟโ€– obtained projecting ๐‘ฟ over the unit sphere. In the general case, the projected normal distribution can be asymmetric and multimodal. In case ๐ is orthogonal to an eigenvector of ๐œฎ, the distribution is symmetric.Template:Sfn The first version of such distribution was introduced in Pukkila and Rao (1988).Template:Sfn

Density function

The density of the projected normal distribution ๐’ซ๐’ฉn(๐,๐œฎ) can be constructed from the density of its generator n-variate normal distribution ๐’ฉn(๐,๐œฎ) by re-parametrising to n-dimensional spherical coordinates and then integrating over the radial coordinate.

In spherical coordinates with radial component rโˆˆ[0,โˆž) and angles ๐œฝ=(ฮธ1,,ฮธnโˆ’1)โˆˆ[0,ฯ€]nโˆ’2ร—[0,2ฯ€), a point ๐’™=(x1,,xn)โˆˆโ„n can be written as ๐’™=r๐’—, with โ€–๐’—โ€–=1. The joint density becomes

p(r,๐œฝ|๐,๐œฎ)=rnโˆ’1|๐œฎ|(2ฯ€)n2eโˆ’12(r๐’—โˆ’๐)โŠคฮฃโˆ’1(r๐’—โˆ’๐)

and the density of ๐’ซ๐’ฉn(๐,๐œฎ) can then be obtained asTemplate:Sfn

p(๐œฝ|๐,๐œฎ)=โˆซ0โˆžp(r,๐œฝ|๐,๐œฎ)dr.

The same density had been previously obtained in Pukkila and Rao (1988, Eq. (2.4))Template:Sfn using a different notation.

Circular distribution

Parametrising the position on the unit circle in polar coordinates as ๐’—=(cosฮธ,sinฮธ), the density function can be written with respect to the parameters ๐ and ๐œฎ of the initial normal distribution as

p(ฮธ|๐,๐œฎ)=eโˆ’12๐โŠค๐œฎโˆ’1๐2ฯ€|๐œฎ|๐’—โŠค๐œฎโˆ’1๐’—(1+T(ฮธ)ฮฆ(T(ฮธ))ฯ•(T(ฮธ)))I[0,2ฯ€)(ฮธ)

where ฯ• and ฮฆ are the density and cumulative distribution of a standard normal distribution, T(ฮธ)=๐’—โŠค๐œฎโˆ’1๐๐’—โŠค๐œฎโˆ’1๐’—, and I is the indicator function.Template:Sfn

In the circular case, if the mean vector ๐ is parallel to the eigenvector associated to the largest eigenvalue of the covariance, the distribution is symmetric and has a mode at ฮธ=ฮฑ and either a mode or an antimode at ฮธ=ฮฑ+ฯ€, where ฮฑ is the polar angle of ๐=(rcosฮฑ,rsinฮฑ). If the mean is parallel to the eigenvector associated to the smallest eigenvalue instead, the distribution is also symmetric but has either a mode or an antimode at ฮธ=ฮฑ and an antimode at ฮธ=ฮฑ+ฯ€.Template:Sfn

Spherical distribution

Parametrising the position on the unit sphere in spherical coordinates as ๐’—=(cosฮธ1sinฮธ2,sinฮธ1sinฮธ2,cosฮธ2) where ๐œฝ=(ฮธ1,ฮธ2) are the azimuth ฮธ1โˆˆ[0,2ฯ€) and inclination ฮธ2โˆˆ[0,ฯ€] angles respectively, the density function becomes

p(๐œฝ|๐,๐œฎ)=eโˆ’12๐โŠค๐œฎโˆ’1๐|๐œฎ|(2ฯ€๐’—โŠค๐œฎโˆ’1๐’—)32(ฮฆ(T(๐œฝ))ฯ•(T(๐œฝ))+T(๐œฝ)(1+T(๐œฝ)ฮฆ(T(๐œฝ))ฯ•(T(๐œฝ))))I[0,2ฯ€)(ฮธ1)I[0,ฯ€](ฮธ2)

where ฯ•, ฮฆ, T, and I have the same meaning as the circular case.Template:Sfn

See also

References

Template:Reflist

Sources