Weibull Bulk and GPD Tail Interval Transition Mixture Model
Weibull Bulk and GPD Tail Interval Transition Mixture Model
Density, cumulative distribution function, quantile function and random number generation for the Weibull bulk and GPD tail interval transition mixture model. The parameters are the Weibull shape wshape and scale wscale, threshold u, interval half-width epsilon, GPD scale sigmau and shape xi.
lower.tail: logical, if FALSE then upper tail probabilities
p: cumulative probabilities
n: sample size (positive integer)
Returns
ditmweibullgpd gives the density, pitmweibullgpd gives the cumulative distribution function, qitmweibullgpd gives the quantile function and ritmweibullgpd gives a random sample.
Details
The interval transition mixture model combines a Weibull for the bulk model with GPD for the tail model, with a smooth transition over the interval (u−epsilon,u+epsilon). The mixing function warps the Weibull to map from (u−epsilon,u) to (u−epsilon,u+epsilon) and warps the GPD from (u,u+epsilon) to (u−epsilon,u+epsilon).
The cumulative distribution function is defined by
F(x)=κ(Ht(q(x))+G(p(x)))
where Ht(x) and G(X) are the truncated Weibull and conditional GPD cumulative distribution functions (i.e. pweibull(x, wshape, wscale) and pgpd(x, u, sigmau, xi)) respectively. The truncated Weibull is not renormalised to be proper, so Ht(x) contrubutes pweibull(u, wshape, wscale) to the cdf for all x≥(u+ϵ). The normalisation constant κ ensures a proper density, given by 1/(1+pweibull(u, wshape, wscale)) where 1 is from GPD component and latter is contribution from Weibull component.
The mixing functions q(x) and p(x) suggested by Holden and Haug (2013) have been implemented. These are symmetric about the threshold u. So for computational convenience only q(x;u) has been implemented as qmix
for a given u, with the complementary mixing function is then defined as p(x;u)=−q(−x;−u).
A minor adaptation of the mixing function has been applied. For the mixture model to function correctly q(x)>=u for all x≥u+ϵ, as then the bulk model will contribute the constant Ht(u)=H(u) for all x above the interval. Holden and Haug (2013) define q(x)=x−ϵ for all x≥u. For more straightforward and interpretable computational implementation the mixing function has been set to the threshold q(x)=u for all x≥u, so the cdf/pdf of the Weibull model can be used directly. We do not have to define cdf/pdf for the non-proper truncated Weibull seperately. As such q′(x)=0 for all x≥u in qmixxprime, which also it makes clearer that Weibull does not contribute to the tail above the interval and vice-versa.
The quantile function within the transition interval is not available in closed form, so has to be solved numerically. Outside of the interval, the quantile are obtained from the Weibull and GPD components directly.
Note
All inputs are vectorised except log and lower.tail. The main inputs (x, p or q) and parameters must be either a scalar or a vector. If vectors are provided they must all be of the same length, and the function will be evaluated for each element of vector. In the case of ritmweibullgpd any input vector must be of length n.
Default values are provided for all inputs, except for the fundamentals x, q and p. The default sample size for ritmweibullgpd is 1.
Missing (NA) and Not-a-Number (NaN) values in x, p and q are passed through as is and infinite values are set to NA. None of these are not permitted for the parameters.
Error checking of the inputs (e.g. invalid probabilities) is carried out and will either stop or give warning message as appropriate.
Examples
## Not run:set.seed(1)par(mfrow = c(2,2))xx = seq(0.001,5,0.01)u =1.5epsilon =0.4kappa =1/(1+ pweibull(u,2,1))f = ditmweibullgpd(xx, wshape =2, wscale =1, epsilon, u, sigmau =1, xi =0.5)plot(xx, f, ylim = c(0,1), xlim = c(0,5), type ='l', lwd =2, xlab ="x", ylab ="density")lines(xx, kappa * dgpd(xx, u, sigmau =1, xi =0.5), col ="red", lty =2, lwd =2)lines(xx, kappa * dweibull(xx,2,1), col ="blue", lty =2, lwd =2)abline(v = u + epsilon * seq(-1,1), lty = c(2,1,2))legend('topright', c('Weibull-GPD ITM','kappa*Weibull','kappa*GPD'), col = c("black","blue","red"), lty = c(1,2,2), lwd =2)# cdf contributionsF = pitmweibullgpd(xx, wshape =2, wscale =1, epsilon, u, sigmau =1, xi =0.5)plot(xx, F, ylim = c(0,1), xlim = c(0,5), type ='l', lwd =2, xlab ="x", ylab ="cdf")lines(xx[xx > u], kappa *(pweibull(u,2,1)+ pgpd(xx[xx > u], u, sigmau =1, xi =0.5)), col ="red", lty =2, lwd =2)lines(xx[xx <= u], kappa * pweibull(xx[xx <= u],2,1), col ="blue", lty =2, lwd =2)abline(v = u + epsilon * seq(-1,1), lty = c(2,1,2))legend('topright', c('Weibull-GPD ITM','kappa*Weibull','kappa*GPD'), col = c("black","blue","red"), lty = c(1,2,2), lwd =2)# simulated data density histogram and overlay true density x = ritmweibullgpd(10000, wshape =2, wscale =1, epsilon, u, sigmau =1, xi =0.5)hist(x, freq =FALSE, breaks = seq(0,1000,0.1), xlim = c(0,5))lines(xx, ditmweibullgpd(xx, wshape =2, wscale =1, epsilon, u, sigmau =1, xi =0.5), lwd =2, col ='black')## End(Not run)
Scarrott, C.J. and MacDonald, A. (2012). A review of extreme value threshold estimation and uncertainty quantification. REVSTAT - Statistical Journal 10(1), 33-59. Available from http://www.ine.pt/revstat/pdf/rs120102.pdf
Holden, L. and Haug, O. (2013). A mixture model for unsupervised tail estimation. arxiv:0902.4137
See Also
weibullgpd, gpd
and dweibull
Other itmweibullgpd: fitmweibullgpd, fweibullgpdcon, fweibullgpd, weibullgpdcon, weibullgpd
Other weibullgpd: fitmweibullgpd, fweibullgpdcon, fweibullgpd, weibullgpdcon, weibullgpd
Other weibullgpdcon: fweibullgpdcon, fweibullgpd, weibullgpdcon, weibullgpd