This vignette focuses on random sampling from extreme value posterior
distributions using the function `rpost`

. From version 1.2.0
onwards sampling can be achieved more quickly using the function
`rpost_rcpp`

. See the vignette Faster simulation using
revdbayes for details.

Performing posterior predictive extreme value inference using posterior samples is covered in a separate vignette Posterior Predictive Extreme Value Inference using the revdbayes Package

The *revdbayes* package tackles the same problem as the
*evdbayes* package (Stephenson and Ribatet
2014), that is, sampling from posterior distributions that occur
in some relatively simple Bayesian extreme value analyses. The essential
difference between these two packages is that evdbayes performs sampling
using Markov Chain Monte Carlo (MCMC) techniques, whereas revdbayes uses
the generalised ratio-of-uniforms method (Wakefield, Gelfand, and Smith 1991),
implemented using the *rust* package (Northrop 2017). Otherwise, these two packages
have similar functionality and their functions have a similar syntax.
For example, a prior distribution specified using one package may be
used in posterior sampling implemented by the other. For details of
setting prior distributions see the `set_prior`

function.

For details of Bayesian extreme value analyses see the review of Stephenson (2016) and the evdbayes user guide (available in the evdbayes doc directory). Typically, MCMC is used to sample from extreme value posterior distributions. This requires tuning parameters of the MCMC algorithm to be set and results in a dependent sample from the posterior. Diagnostics checks, based on running multiple chains from different starting values, are used to check convergence and to decide which values should be discarded prior to approximate convergence. An advantage of using a direct method of simulation, such as the generalised ratio-of-uniforms method, is that it produces a random sample from the posterior distribution. This method also involves tuning parameters, but the revdbayes package has been designed to set those automatically.

The current version of revdbayes samples from posterior distributions
based on the Generalised Extreme Value (GEV) model, the Generalised
Pareto (GP) model, the point process (PP) model and the
*r*-largest order statistics (OS) model. The evdbayes package
offers in addition some extreme value regression models.

We consider how to use the two main functions in revdbayes, namely
`set_prior`

(used to define the prior distribution) and
`rpost`

(used to sample from the posterior distribution). We
use the examples in the evdbayes user guide for illustration. Please see
the evdbayes user guide for details of the models underlying these
analyses.

The ratio-of-uniforms method is an acceptance-rejection type of
simulation algorithm. A crude measure of the efficiency of the algorithm
is the probability \(p_a\) that a
proposed value is accepted. In the *rust* package (Northrop 2017) variable transformation is used
to increase \(p_a\). In the current
context two transformations are of interest: (i) marginal Box-Cox
transformation of (positive functions of) extreme value parameters
(using argument `trans = "BC"`

to `rpost`

instead
of the default `trans = "none"`

), and/or (ii) rotation of
parameter axes about the estimated mode of the posterior (the default
`rotate = TRUE`

instead of the `rotate = FALSE`

),
based on the estimated Hessian of the log-posterior at this mode.
Transformation (i) seeks to reduce skewness in the marginal posterior
distributions. Transformation (ii) tends to reduce posterior dependence
between the parameters. The ratio-of-uniforms algorithm is then
performed after relocating the mode of the posterior to the origin,
because this tends to increase the probability of acceptance (Wakefield, Gelfand, and Smith 1991).

For details of the ratio-of-uniforms method and the transformations
used see the vignette of the *rust* package (Northrop 2017). In the *rust* vignette
it is argued that the largest attainable value of \(p_a\) for a typical \(d\)-dimensional problem is the value
resulting from the special case of a \(d\)-dimensional normal distribution with
independent components. For \(d=2\)
this value is 0.534, for \(d=3\) the
value is 0.316. In an object `ru_object`

returned from
`rpost`

an estimate of this probability is given by
`ru_object$pa`

. The examples presented in this vignette
suggest that often rotation to reduce dependence is more helpful than
marginal transformation to reduce skewness. This
(`trans = "none"`

and `rotate = TRUE`

) is the
default setting of `rpost`

and seems to work well enough for
most problems.

The computations in the following sections were performed using a notebook containing a 3.0GHz Intel processor and 8GB RAM.

The GP distribution is used to model *threshold excesses*,
that is, the amounts by which *threshold exceedances* exceed some
threshold. It has two parameters: a scale parameter \(\sigma_u\) and shape parameter \(\xi\). We use the following example to
illustrate the use of the transformation strategies implemented by the
arguments `rotate`

and `trans`

to
`rpost`

and how the user can specify their own prior
distribution.

The numeric vector `gom`

contains 315 storm peak
significant wave heights from a location in the Gulf of Mexico, from the
years 1900 to 2005. These data are analysed in Northrop, Attalides, and Jonathan (2017). We set
the threshold at the 65% sample quantile and use `set_prior`

to set a prior.

We sample first on the \((\sigma_u, \xi)\) scale, with mode relocation only.

```
t1 <- system.time(
gp1 <- rpost(n = n, model = "gp", prior = fp, thresh = thresh, data = gom,
rotate = FALSE)
)[3]
```

Then we add a rotation of \((\sigma_u, \xi)\) about the estimated posterior mode.

Now we add marginal Box-Cox transformation. We apply Box-Cox transformation to the parameters \(\phi_1 = \sigma_u\) and \(\phi_2 = \xi + \sigma / x_{(m)}\), where \(x_{(m)}\) is the largest threshold excess. The parameters \(\phi_1\) and \(\phi_2\) are positive for all combinations of \((\sigma_u, \xi)\) for which the GP likelihood is positive.

```
t3 <- system.time(
gp3 <- rpost(n = n, model = "gp", prior = fp, thresh = thresh, data = gom,
rotate = FALSE, trans = "BC")
)[3]
t4 <- system.time(
gp4 <- rpost(n = n, model = "gp", prior = fp, thresh = thresh, data = gom,
trans = "BC")
)[3]
```

We plot the samples obtained with the contours of the corresponding densities superimposed. The plot on the top left is on the original \((\sigma_u, \xi)\) scale. The other plots are on the scale used for the ratio-of-uniforms algorithm, that is, with relocation of the mode to the origin. In the following the \(\rho_i, i = 1, \ldots, d\), \(\rho_1\) and \(\rho_2\) in this example, are the variables to which the ratio-of-uniforms algorithm is applied, i.e. after any transformation (Box-Cox and/or rotation of axes) and relocation of the mode to the origin.

```
plot(gp1, ru_scale = FALSE, cex.main = 0.75, cex.lab = 0.75,
main = paste("no transformation \n pa = ", round(gp1$pa, 3),
", time = ", round(t1, 2), "s"))
plot(gp2, ru_scale = TRUE, cex.main = 0.75, cex.lab = 0.75,
main = paste("rotation \n pa = ", round(gp2$pa, 3),
", time = ", round(t2, 2), "s"))
plot(gp3, ru_scale = TRUE, cex.main = 0.75, cex.lab = 0.75,
main = paste("Box-Cox \n pa = ", round(gp3$pa, 3),
", time = ", round(t3, 2), "s"))
plot(gp4, ru_scale = TRUE, cex.main = 0.75, cex.lab = 0.75,
main = paste("Box-Cox and rotation \n pa = ", round(gp4$pa, 3),
", time = ", round(t4, 2), "s"))
```

Comparison of the plots on the right to the plots on the left shows
that rotation of the parameter axes about the mode of the posterior has
reduced dependence between the components. The estimated probabilities
of acceptance for the plots on the right are close to the 0.534 obtained
for a 2-dimensional normal distribution with independent components.
Box-Cox transformation has increased the estimated value of \(p_a\) but not by much. In fact, the extra
computation time required to calculate the Box-Cox transformation each
time that the posterior density is evaluated means that posterior
sampling is slower than the default setting of
`rotate = TRUE`

and `trans = "none"`

. That is, in
this example at least, the increase is \(p_a\) resulting from the addition of the
Box-Cox transformation is not sufficient to offset the extra time needed
to compute the posterior density.

We repeat the rotation only and Box-Cox transformation plus rotation analyses for a much higher threshold, set at the 95% sample quantile.

```
thresh <- quantile(gom, probs = 0.95)
fp <- set_prior(prior = "flat", model = "gp", min_xi = -1)
t2 <- system.time(
gp2 <- rpost(n = n, model = "gp", prior = fp, thresh = thresh, data = gom)
)[3]
t4 <- system.time(
gp4 <- rpost(n = n, model = "gp", prior = fp, thresh = thresh, data = gom,
trans = "BC")
)[3]
```

It is optimistic to use such a high threshold in this example, because it results in only 16 threshold excesses. In the rotation only case, a convergence warning is triggered by one of the optimisations used to created the bounding box of the ratio-of-uniforms method. This appears to be a spurious warning, because the plots of the simulations below seem fine. When a Box-Cox transformation is used there are no warnings, because the optimisations have greater stability and it is now easier for the convergence of the optimisations to be confirmed.

Strong asymmetry in the posterior distribution means that the combination of marginal Box-Cox transformation and rotation produces a larger improvement in \(p_a\) and means that now this strategy is competitive with using rotation alone in terms of computation time.

**A User-defined prior**

Suppose that we wish to use a prior for \((\sigma_u, \xi)\) with a density that is
proportional to \(\sigma_u^{-1}
(1+\xi)^{\alpha-1} (1-\xi)^{\beta-1}\), for \(\sigma_u > 0, -1 < \xi < 1\) and
for some \(\alpha > 0\) and \(\beta > 0\). This is an improper prior
in which \(\sigma_u\) and \(\xi\) are independent *a priori*,
\(\log \sigma_u\) is uniform over the
real line and \(\xi\) has beta(\(\alpha, \beta\))-type distribution on the
interval \((-1, 1)\). We can do this by
creating a function that returns the prior log-density and passing this
function to `set_prior`

. The first argument of the prior
log-density function must be the parameter vector (the GP parameters
\((\sigma_u, \xi)\) in this case),
followed by any hyperparameters.

```
u_prior_fn <- function(x, ab) {
#
# Calculates the the log of the (improper) prior density for GP parameters
# (sigma_u, xi) in which log(sigma_u) is uniform on the real line and xi has
# a beta(alpha, beta)-type prior on the interval (-1, 1).
#
# Args:
# x : A numeric vector. GP parameter vector (sigma, xi).
# ab : A numeric vector. Hyperparameter vector (alpha, beta), where
# alpha and beta must be positive.
#
# Returns : the value of the log-prior at x.
#
if (x[1] <= 0 | x[2] <= -1 | x[2] >= 1) {
return(-Inf)
}
return(-log(x[1]) + (ab[1] - 1) * log(1 + x[2]) +
(ab[2] - 1) * log(1 - x[2]))
}
up <- set_prior(prior = u_prior_fn, ab = c(2, 2), model = "gp")
gp_u <- rpost(n = n, model = "gp", prior = up, thresh = thresh, data = gom)
```

See also the “Posterior predictive extreme value inference” section of the Posterior Predictive Extreme Value Inference using the revdbayes Package for an analysis that adds inferences about the probability of threshold exceedance to the analysis of threshold excesses using a GP distribution.

We consider two examples involving the GEV distribution, which is
used to model block maxima. The GEV distribution has three parameters: a
location parameter \(\mu\), a scale
parameter \(\sigma\) and a shape
parameter \(\xi\). In the first example
we illustrate the use of `set_prior`

to set a prior
distribution for the GEV parameters and show that a prior set using
`set_prior`

(including user-defined prior) can be used as an
argument to the evdbayes function `posterior`

. In the second
example we show that the reverse is also true, that is, a prior set
using an evdbayes function (`prior.prob`

) can be used an an
argument to the revdbayes function `rpost`

.

The numeric vector `portpirie`

contains 65 annual maximum
sea levels (in metres) recorded at Port Pirie, South Australia, from
1923 to 1987.

```
data(portpirie)
mat <- diag(c(10000, 10000, 100))
pn <- set_prior(prior = "norm", model = "gev", mean = c(0,0,0), cov = mat)
p1 <- rpost(n = n, model = "gev", prior = pn, data = portpirie)
p1$pa
#> [1] 0.2981159
```

The proportion of accepted values is close to the best we can hope
for in this 3-dimensional example, i.e. 0.316. The following plots
illustrate the effect of `rotate = TRUE`

. The first set of
plots below show the simulated values of the GEV parameters. There is
some association between the parameters *a posteriori*, albeit
weak association. The second set of plots show the values simulated on
the scale used in the ratio-of-uniforms algorithm. The association has
been reduced by rotating the parameter axes. The increase in the
proportion of accepted values is only modest in this example (from
approximately 0.26 to 0.30) but this improvement is more substantial in
other examples.

We produce plots of the estimated marginal posterior densities.

The numeric vector `oxford`

contains 80 annual maximum
temperatures, in degrees Fahrenheit, from 1901 to 1980 at Oxford,
England.

```
data(oxford)
prox <- set_prior(prior = "prob", model = "gev", quant = c(85, 88, 95),
alpha = c(4, 2.5, 2.25, 0.25))
# revdbayes
ox_post <- rpost(n = 1000, model = "gev", prior = prox, data = oxford)
```

We produce plots of the estimated marginal posterior densities.

```
oldpar <- par(mfrow = c(1,3))
plot(density(ox_post$sim_vals[, 1], adj = 2), main = "", xlab = expression(mu))
plot(density(ox_post$sim_vals[, 2], adj = 2), main = "", xlab = expression(sigma))
plot(density(ox_post$sim_vals[, 3], adj = 2), main = "", xlab = expression(xi))
```

We do not illustrate the use of marginal Box-Cox transformation in
the GEV case. If `trans = "BC"`

then we use \(\phi_1 = \mu\), \(\phi_2 = [\sigma + \xi (x_{(1)} - \mu) ] /
(x_{(m)} - x_{(1)})^{1/2}\) and \(\phi_3 = [\sigma + \xi (x_{(m)} - \mu) ] /
(x_{(m)} - x_{(1)})^{1/2}\), where \(x_{(1)}\) and \(x_{(m)}\) are the smallest and largest
sample block maxima respectively. This transformation has been
standardised to have Jacobian 1. We apply Box-Cox transformation only to
the (positive) parameters \(\phi_2\)
and \(\phi_3\), because \(\phi_1 = \mu\) is not constrained to be
positive and tends to have a marginal posterior distribution that is not
strongly skewed.

Like the GP model the PP model involves exceedances of a threshold
`thresh`

. However, the PP model has one more parameter than
the GP model, three parameters \((\mu, \sigma,
\xi)\) say, because it considers the number of threshold
exceedances (that is, in addition to the sizes of the threshold
excesses. The interpretation of the parameters \((\mu, \sigma, \xi)\) is determined by the
number of periods of observation, or blocks, into which the data are
grouped. This is set using the argument `noy`

to
`rpost`

. Under the PP model the distribution of the maximum
over each of these blocks has approximately a GEV distribution with
parameters \((\mu, \sigma, \xi)\),
provided that the numbers of observations within each block are large.
Although the user may require a posterior sample based on a particular
value of `noy`

it may be that the sampling itself is more
efficient when a different value of `noy`

is used.

We illustrate the use of a prior created by the evdbayes package as
an argument to the revdbayes function `rpost`

. We also show
how the choice of parameterisation of the model affects the strength
posterior dependence between those parameters and hence the efficiency
of simulation from the posterior. Wadsworth,
Tawn, and Jonathan (2010) note that posterior dependence between
the location parameter and the other two parameters tends to be reduced
if we use a parameterisation in which the number of blocks is equal to
the number of threshold excesses, rather the typical parameterisation
where the number of blocks is equal to the number of years of data. This
is because, in the context of the likelihood alone, \(\mu\) is orthogonal to (\(\sigma, \xi\)) under this parameterisation.
Suppose that \((\mu, \sigma, \xi)\) is
the parameter vector on the scale of interest, that is, when the number
of blocks is equal to `noy`

and \((\mu_e, \sigma_e, \xi)\) is the parameter
vector when the number of blocks is set equal to the number of threshold
excesses \(n_{exc}\). Then \(\mu_e = \mu + \sigma (c ^ \xi - 1) / \xi\),
and \(\sigma_e = \sigma c ^ \xi\) where
\(c=\)`noy`

\(/n_{exc}\).

The `rotate = TRUE`

argument of `rpost`

produces a similar effect, but it can reduce posterior dependence
between all parameters. Also, rotating the posterior accounts for the
influence of the prior in the posterior, whereas the argument for
setting `noy`

equal to the number of threshold excesses is
based on the likelihood alone.

We illustrate the use of `rpost`

to sample from a
posterior distribution under the PP using the `rainfall`

dataset, which contains 20820 daily rainfall totals, in mm, recorded at
a rain gauge in England over a 57 year period. Three of these years
contain only missing values so if we wish to parameterise the model in
terms of the GEV parameters of annual maxima we should set
`noy = 54`

when calling `rpost`

. We use the prior
from the evdbayes user’s guide and a threshold of 40mm.

```
data(rainfall)
rthresh <- 40
prrain <- set_prior(prior = "quant", model = "gev", prob = 10^-(1:3),
shape = c(38.9, 7.1, 47), scale = c(1.5, 6.3, 2.6))
```

The first set of plots below relate to the standard parameterisation.
There is posterior dependence between all parameters. The second set of
plots show that rotating the posterior using `rotate = TRUE`

reduces the dependence.

```
# Annual maximum parameterisation (number of blocks = number of years of data)
rn0 <- rpost(n = n, model = "pp", prior = prrain, data = rainfall,
thresh = rthresh, noy = 54, rotate = FALSE)
plot(rn0)
```

```
rn0$pa
#> [1] 0.1693652
# Rotation about maximum a posteriori estimate (MAP)
system.time(
rn1 <- rpost(n = n, model = "pp", prior = prrain, data = rainfall,
thresh = rthresh, noy = 54)
)
#> user system elapsed
#> 3.28 0.05 3.40
plot(rn1, ru_scale = TRUE)
```

Using the Wadsworth, Tawn, and Jonathan
(2010) parameterisation reduces the posterior dependence between
\(\mu\) and the other two parameters,
but not between \(\sigma\) and \(\xi\) (see plot on the right labelled with
\(\rho_1\) and \(\rho_2\)). Using the Wadsworth, Tawn, and Jonathan (2010)
parameterisation and `rotate = TRUE`

also reduces posterior
dependence between all parameters but the earlier plot suggests that
using `rotate = TRUE`

alone is sufficient in this
example.

```
# Number of blocks = number of threshold excesses
n_exc <- sum(rainfall > rthresh, na.rm = TRUE)
rn2 <- rpost(n = n, model = "pp", prior = prrain, data = rainfall,
thresh = rthresh, noy = 54, use_noy = FALSE, rotate = FALSE)
rn2$pa
#> [1] 0.193039
plot(rn2, ru_scale = TRUE)
```

```
# Number of blocks = number of threshold excesses, rotation about MAP
system.time(
rn3 <- rpost(n = n, model = "pp", prior = prrain, data = rainfall,
thresh = rthresh, noy = 54, use_noy = FALSE)
)
#> user system elapsed
#> 3.64 0.08 3.78
plot(rn3, ru_scale = TRUE)
```

In this example, rotation of the posterior about its mode using
`rotate = TRUE`

produces the greatest increases in \(p_a\) and, if this is performed, there is
little to choose between the two choices of the number of blocks.
Setting the number of blocks equal to the number of threshold excesses
does reduce posterior dependence between \(\mu\) and the other parameters but enough
dependence between \(\sigma\) and \(\xi\) remains that the value of \(p_a\) doesn’t increase substantially. The
reparameterisation resulting from the rotation is linear in the
parameters \((\mu, \sigma, \xi)\),
which is simpler than the non-linear transformation from one value of
the number of blocks to another. Using this non-linear transformation in
addition to the rotation has increased the computation time in this
example, that is, `rn1`

takes a little longer to produce than
`rn3`

and this is also the case for other choices of
prior.

We produce plots of the estimated marginal posterior densities.

```
oldpar <- par(mfrow = c(1,3))
plot(density(rn1$sim_vals[, 1], adj = 2), main = "", xlab = expression(mu))
plot(density(rn1$sim_vals[, 2], adj = 2), main = "", xlab = expression(sigma))
plot(density(rn1$sim_vals[, 3], adj = 2), main = "", xlab = expression(xi))
```

We do not illustrate the use of marginal Box-Cox transformation in
the PP case. If `trans = "BC"`

then we use \(\phi_1 = \mu\), \(\phi_2 = [\sigma + \xi (u - \mu) ] / (x_{(m)} -
u)^{1/2}\) and \(\phi_3 = [\sigma + \xi
(x_{(m)} - \mu) ] / (x_{(m)} - u)^{1/2}\), where \(u\) is the threshold `thresh`

and \(x_{(m)}\) is the largest sample
value. As in the GEV case we apply Box-Cox transformation only to the
(positive) parameters \(\phi_2\) and
\(\phi_3\).

The OS model is an extension of the GEV model in which the \(r\) largest sample values (the \(r\) largest order statistics) in each block
are modelled, rather than just the block maximum. More generally, if
there are \(m\) blocks then we can use
the \(r_i\) largest order statistics in
block \(i\). For the purposes of
illustrating how `rpost`

can be used to sample from a
posterior distribution under the OS model we use `venice`

dataset, which (apart from one year) contains the 10 largest sea levels
in Venice for the years 1931-1981. Our analysis is flawed because, as
demonstrated in the evdbayes user guide, it is clear that a time trend
in the location parameter \(\mu\)
should be considered.

```
data(venice)
mat <- diag(c(10000, 10000, 100))
pv <- set_prior(prior = "norm", model = "gev", mean = c(0,0,0), cov = mat)
osv <- rpost(n = n, model = "os", prior = pv, data = venice)
plot(osv)
```

We do not illustrate the use of marginal Box-Cox transformation in
the OS case. If `trans = "BC"`

then we use \(\phi_1 = \mu\), \(\phi_2 = [\sigma + \xi (x_{(1)} - \mu) ] /
(x_{(m)} - x_{(1)})^{1/2}\) and \(\phi_3 = [\sigma + \xi (x_{(m)} - \mu) ] /
(x_{(m)} - x_{(1)})^{1/2}\), where \(x_{(1)}\) and \(x_{(m)}\) are the smallest and largest
sample order statistics respectively. Again we apply Box-Cox
transformation only to the (positive) parameters \(\phi_2\) and \(\phi_3\).

Northrop, P. J. 2017. *rust:
Ratio-of-Uniforms Simulation with Transformation*. https://CRAN.R-project.org/package=rust.

Northrop, P. J., N. Attalides, and P. Jonathan. 2017.
“Cross-Validatory Extreme Value Threshold Selection and
Uncertainty with Application to Ocean Storm Severity.”
*Journal of the Royal Statistical Society: Series C (Applied
Statistics)* 66 (1): 93–120. doi:10.1111/rssc.12159.

Stephenson, A. 2016. “Bayesian Inference for Extreme Value
Modelling.” In *Extreme Value Modeling and Risk Analysis:
Methods and Applications*, edited by D. K. Dey and J. Yan, 257–280.
London: Chapman; Hall. doi:10.1201/b19721.

Stephenson, A., and M. Ribatet. 2014. *evdbayes: Bayesian Analysis in Extreme Value
Theory*. https://CRAN.R-project.org/package=evdbayes.

Wadsworth, J. L., J. A. Tawn, and P. Jonathan. 2010. “Accounting
for Choice of Measurement Scale in Extreme Value Modeling.”
*The Annals of Applied Statistics* 4 (3): 1558–1578. doi:10.1214/10-AOAS333.

Wakefield, J. C., A. E. Gelfand, and A. F. M. Smith. 1991.
“Efficient Generation of Random Variates via the Ratio-of-Uniforms
Method.” *Statistics and Computing* 1 (2): 129–133. doi:10.1007/BF01889987.