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Directional (version 4.0)

MLE of some circular distributions: MLE of some circular distributions

Description

MLE of some circular distributions.

Usage

spml.mle(x, rads = FALSE, tol = 1e-07)
wrapcauchy(x, rads = FALSE, tol = 1e-07)

Arguments

x

A numerical vector with the circular data. They must be expressed in radians.

rads

If the data are in radians set this to TRUE.

tol

The tolerance level to stop the iterative process of finding the MLEs.

Value

A list including:

iters

The iterations required until convergence.

loglik

The value of the maximised log-likelihood.

param

A vector consisting of the estimates of the two parameters, the mean direction for both distributions and the concentration parameter kappa and the rho for the von Mises and wrapped Cauchy respectively.

gamma

The norm of the mean vector of the angualr Gaussian distribution.

mu

The mean vector of the angular Gaussian distribution.

mumu

In the case of "spml.mle" this is the mean angle in radians.

Details

The parameters of the bivariate angular Gaussian and wrapped Cauchy distributions are estimated. For the Wrapped Cauchy, the iterative procedure described by Kent and Tyler (1988) is used. The Newton-Raphson algortihm for the angular Gaussian is described in the regression setting in Presnell et al. (1998).

References

Mardia K. V. and Jupp P. E. (2000). Directional statistics. Chicester: John Wiley \& Sons.

Sra S. (2012). A short note on parameter approximation for von Mises-Fisher distributions: and a fast implementation of Is(x). Computational Statistics, 27(1): 177-190.

Presnell Brett, Morrison Scott P. and Littell Ramon C. (1998). Projected multivariate linear models for directional data. Journal of the American Statistical Association, 93(443): 1068-1077.

Kent J. and Tyler D. (1988). Maximum likelihood estimation for the wrapped Cauchy distribution. Journal of Applied Statistics, 15(2): 247--254.

See Also

vmf, rvonmises, rvmf

Examples

Run this code
# NOT RUN {
x <- rvonmises(1000, 3, 9)
spml.mle(x)
wrapcauchy(x)
# }

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