Rayleigh distribution

Rayleigh distribution

Probability distribution
name =Rayleigh
type =density
pdf_


cdf_


parameters =sigma>0,
support =xin [0;infty)
pdf =frac{x expleft(frac{-x^2}{2sigma^2} ight)}{sigma^2}
cdf =1-expleft(frac{-x^2}{2sigma^2} ight)
mean =sigma sqrt{frac{pi}{2

median =sigmasqrt{ln(4)},
mode =sigma,
variance =frac{4 - pi}{2} sigma^2
skewness =frac{2sqrt{pi}(pi - 3)}{(4-pi)^{3/2
kurtosis =-frac{6pi^2 - 24pi +16}{(4-pi)^2}
entropy =1+lnleft(frac{sigma}{sqrt{2 ight)+frac{gamma}{2}
mgf =1+sigma t,e^{sigma^2t^2/2}sqrt{frac{pi}{2left( extrm{erf}left(frac{sigma t}{sqrt{2 ight)!+!1 ight)
char =1!-!sigma te^{-sigma^2t^2/2}sqrt{frac{pi}{2!left( extrm{erfi}!left(frac{sigma t}{sqrt{2 ight)!-!i ight)

In probability theory and statistics, the Rayleigh distribution is a continuous probability distribution. It can arise when a two-dimensional vector (e.g. wind velocity) has elements that are normally distributed, are uncorrelated, and have equal variance. The vector’s magnitude (e.g. wind speed) will then have a Rayleigh distribution. The distribution can also arise in the case of random complex numbers whose real and imaginary components are i.i.d. Gaussian. In that case, the modulus of the complex number is Rayleigh-distributed. The distribution was so named after Lord Rayleigh.

The Rayleigh probability density function is

:f(x|sigma) = frac{x expleft(frac{-x^2}{2sigma^2} ight)}{sigma^2}

for x in [0,infty).

Properties

The raw moments are given by:

:mu_k=sigma^k2^{k/2},Gamma(1+k/2),

where Gamma(z) is the Gamma function.

The mean and variance of a Rayleigh random variable may be expressed as:

:mu(X) = sigma sqrt{frac{pi}{2,

and

: extrm{var}(X) = frac{4 - pi}{2} sigma^2,.

The skewness is given by:

:gamma_1=frac{2sqrt{pi}(pi - 3)}{(4-pi)^{3/2.

The excess kurtosis is given by:

:gamma_2=-frac{6pi^2 - 24pi +16}{(4-pi)^2}.

The characteristic function is given by:

:varphi(t)=:1!-!sigma te^{-sigma^2t^2/2}sqrt{frac{pi}{2!left( extrm{erfi}!left(frac{sigma t}{sqrt{2 ight)!-!i ight)

where operatorname{erfi}(z) is the complex error function. The moment generating function is given by

:M(t)=,:1+sigma t,e^{sigma^2t^2/2}sqrt{frac{pi}{2left( extrm{erf}left(frac{sigma t}{sqrt{2 ight)!+!1 ight),

where operatorname{erf}(z) is the error function.

Information entropy

The information entropy is given by

:H=1+lnleft(frac{sigma}{sqrt{2 ight)+frac{gamma}{2}

where gamma is the Euler–Mascheroni constant.

Parameter estimation

Given "N" independent and identically distributed Rayleigh random variables with parameter sigma, the maximum likelihood estimate of sigma is

:hat{sigma}=sqrt{frac{1}{2N}sum_{i=1}^N x_i^2}.

Generating Rayleigh-distributed random variates

Given a random variate "U" drawn from the uniform distribution in the interval (0, 1), then the variate

:X=sigmasqrt{-2ln(1-U)},

has a Rayleigh distribution with parameter sigma. This follows from the form of the cumulative distribution function. Given that U is uniform, (1–U) has the same uniformity and the above may be simplified to

:X=sigmasqrt{-2ln(U)}.

Note that if you are generating random numbers belonging to [0,1), exclude zero values to avoid the natural log of zero.

Related distributions

*R sim mathrm{Rayleigh}(sigma) is a Rayleigh distribution if R = sqrt{X^2 + Y^2} where X sim N(0, sigma^2) and Y sim N(0, sigma^2) are two independent normal distributions. (This gives motivation to the use of the symbol "sigma" in the above parameterization of the Rayleigh density.)
*If R sim mathrm{Rayleigh}(1) then R^2 has a chi-square distribution with two degrees of freedom: R^2 sim chi^2_2
*If X has an exponential distribution X sim mathrm{Exponential}(x|lambda) then Y=sqrt{2Xsigma^2lambda} sim mathrm{Rayleigh}(y|sigma).

*If R sim mathrm{Rayleigh}(sigma) then sum_{i=1}^N R_i^2 has a gamma distribution with parameters N and 2sigma^2: [Y=sum_{i=1}^N R_i^2] sim Gamma(N,2sigma^2).

*The Chi distribution is a generalization of the Rayleigh distribution.
*The Rice distribution is a generalization of the Rayleigh distribution.
*The Weibull distribution is a generalization of the Rayleigh distribution.
*The Maxwell–Boltzmann distribution describes the magnitude of a normal vector in three dimensions.

ee also

*Rayleigh fading
*Rice distribution
* The SOCR Resource provides [http://socr.ucla.edu/htmls/SOCR_Distributions.html interactive interface to Rayleigh distribution] .


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