specpool
is based on incidences in sample sites, and gives a single estimate
for a collection of sample sites (matrix). Function estimateR
is based on abundances (counts) on single sample site.
specpool(x, pool, smallsample = TRUE)
estimateR(x, ...)
specpool2vect(X, index = c("jack1","jack2", "chao", "boot","Species"))
poolaccum(x, permutations = 100, minsize = 3)
estaccumR(x, permutations = 100, parallel = getOption("mc.cores"))
"summary"(object, display, alpha = 0.05, ...)
"plot"(x, alpha = 0.05, type = c("l","g"), ...)
plot
function.pool
.specpool
result object.how
,
or a permutation matrix where each row gives the permuted indices.parallel = 1
uses ordinary, non-parallel
processing. The parallel processing is done with parallel
package.xyplot
.specpool
returns a data frame with entries for
observed richness and each of the indices for each class in
pool
vector. The utility function specpool2vect
maps
the pooled values into a vector giving the value of selected
index
for each original site. Function estimateR
returns the estimates and their standard errors for each
site. Functions poolaccum
and estimateR
return
matrices of permutation results for each richness estimator, the
vector of sample sizes and a table of means
of permutations
for each estimator.
The incidence-based estimates in specpool
use the frequencies
of species in a collection of sites.
In the following, $S_P$ is the extrapolated richness in a pool,
$S_0$ is the observed number of species in the
collection, $a1$ and $a2$ are the number of species
occurring only in one or only in two sites in the collection, $p_i$
is the frequency of species $i$, and $N$ is the number of
sites in the collection. The variants of extrapolated richness in
specpool
are:
Chao |
$S_P = S_0 + a1^2/(2*a2) * (N-1)/N$ |
Chao bias-corrected |
$S_P = S_0 + a1*(a1-1)/(2*(a2+1)) * (N-1)/N$ |
First order jackknife |
$S_P = S_0 + a1*(N-1)/N$ |
Second order jackknife |
$S_P = S_0 + a1*(2*N-3)/N - a2*(N-2)^2/N/(N-1)$ |
specpool
normally uses basic Chao equation, but when there
are no doubletons ($a2=0$) it switches to bias-corrected
version. In that case the Chao equation simplifies to
$S_0 + (N-1)/N * a1*(a1-1)/2$. The abundance-based estimates in estimateR
use counts
(numbers of individuals) of species in a single site. If called for
a matrix or data frame, the function will give separate estimates
for each site. The two variants of extrapolated richness in
estimateR
are bias-corrected Chao and ACE (O'Hara 2005, Chiu
et al. 2014). The Chao estimate is similar as the bias corrected
one above, but $a_i$ refers to the number of species with
abundance $i$ instead of number of sites, and the small-sample
correction is not used. The ACE estimate is defined as:
ACE |
$S_P = S_abund + S_rare/C_ace + a1/C_ace * gamma^2$ |
where |
$C_{ace} = 1- a1/N_{rare}$ |
Functions estimate the standard errors of the estimates. These only
concern the number of added species, and assume that there is no
variance in the observed richness. The equations of standard errors
are too complicated to be reproduced in this help page, but they can
be studied in the R source code of the function and are discussed
in the vignette
that can be read with the
browseVignettes("vegan")
. The standard error are based on the
following sources: Chiu et al. (2014) for the Chao estimates and
Smith and van Belle (1984) for the first-order Jackknife and the
bootstrap (second-order jackknife is still missing). For the
variance estimator of $S_ace$ see O'Hara (2005).
Functions poolaccum
and estaccumR
are similar to
specaccum
, but estimate extrapolated richness indices
of specpool
or estimateR
in addition to number of
species for random ordering of sampling units. Function
specpool
uses presence data and estaccumR
count
data. The functions share summary
and plot
methods. The summary
returns quantile envelopes of
permutations corresponding the given level of alpha
and
standard deviation of permutations for each sample size. NB., these
are not based on standard deviations estimated within specpool
or estimateR
, but they are based on permutations. The
plot
function shows the mean and envelope of permutations
with given alpha
for models. The selection of models can be
restricted and order changes using the display
argument in
summary
or plot
. For configuration of plot
command, see xyplot
.
Chiu, C.H., Wang, Y.T., Walther, B.A. & Chao, A. (2014). Improved nonparametric lower bound of species richness via a modified Good-Turing frequency formula. Biometrics 70, 671--682. Colwell, R.K. & Coddington, J.A. (1994). Estimating terrestrial biodiversity through extrapolation. Phil. Trans. Roy. Soc. London B 345, 101--118.
O'Hara, R.B. (2005). Species richness estimators: how many species can dance on the head of a pin? J. Anim. Ecol. 74, 375--386.
Palmer, M.W. (1990). The estimation of species richness by extrapolation. Ecology 71, 1195--1198.
Smith, E.P & van Belle, G. (1984). Nonparametric estimation of species richness. Biometrics 40, 119--129.
veiledspec
, diversity
, beals
,
specaccum
. data(dune)
data(dune.env)
attach(dune.env)
pool <- specpool(dune, Management)
pool
op <- par(mfrow=c(1,2))
boxplot(specnumber(dune) ~ Management, col="hotpink", border="cyan3",
notch=TRUE)
boxplot(specnumber(dune)/specpool2vect(pool) ~ Management, col="hotpink",
border="cyan3", notch=TRUE)
par(op)
data(BCI)
## Accumulation model
pool <- poolaccum(BCI)
summary(pool, display = "chao")
plot(pool)
## Quantitative model
estimateR(BCI[1:5,])
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