simulate.rda.Rd
Function simulates a response data frame so that it adds
Gaussian error to the fitted responses of Redundancy Analysis
(rda
), Constrained Correspondence Analysis
(cca
) or distance-based RDA (capscale
).
The function is a special case of generic simulate
, and
works similarly as simulate.lm
.
# S3 method for rda simulate(object, nsim = 1, seed = NULL, indx = NULL, rank = "full", correlated = FALSE, ...)
object | |
---|---|
nsim | number of response matrices to be simulated. Only one
dissimilarity matrix is returned for |
seed | an object specifying if and how the random number
generator should be initialized (‘seeded’). See
|
indx | Index of residuals added to the fitted values, such as
produced by |
rank | The rank of the constrained component: passed to
|
correlated | Are species regarded as correlated in parametric
simulation or when |
... | additional optional arguments (ignored). |
The implementation follows "lm"
method of
simulate
, and adds Gaussian (Normal) error to the fitted
values (fitted.rda
) using function rnorm
if correlated = FALSE
or mvrnorm
if
correlated = TRUE
. The standard deviations (rnorm
)
or covariance matrices for species (mvrnorm
) are
estimated from the residuals after fitting the constraints.
Alternatively, the function can take a permutation index that is used
to add permuted residuals (unconstrained component) to the fitted
values. Raw data are used in rda
. Internal Chi-square
transformed data are used in cca
within the function,
but the returned matrix is similar to the original input data. The
simulation is performed on internal metric scaling data in
capscale
, but the function returns the Euclidean
distances calculated from the simulated data. The simulation uses
only the real components, and the imaginary dimensions are ignored.
If nsim = 1
, returns a matrix or dissimilarities (in
capscale
) with similar additional arguments on random
number seed as simulate
. If nsim > 1
, returns a
similar array as returned by simulate.nullmodel
with
similar attributes.
simulate
for the generic case and for
lm
objects, and simulate.nullmodel
for
community null model simulation. Functions fitted.rda
and fitted.cca
return fitted values without the error
component. See rnorm
and mvrnorm
(MASS package) for simulating Gaussian random error.
data(dune) data(dune.env) mod <- rda(dune ~ Moisture + Management, dune.env) ## One simulation update(mod, simulate(mod) ~ .)#> Call: rda(formula = simulate(mod) ~ Moisture + Management, data = #> dune.env) #> #> Inertia Proportion Rank #> Total 90.1198 1.0000 #> Constrained 62.6416 0.6951 6 #> Unconstrained 27.4781 0.3049 13 #> Inertia is variance #> #> Eigenvalues for constrained axes: #> RDA1 RDA2 RDA3 RDA4 RDA5 RDA6 #> 27.116 20.223 6.368 3.919 2.941 2.074 #> #> Eigenvalues for unconstrained axes: #> PC1 PC2 PC3 PC4 PC5 PC6 PC7 PC8 PC9 PC10 PC11 PC12 PC13 #> 6.284 4.493 3.701 2.663 2.272 1.899 1.778 1.266 1.070 0.787 0.558 0.432 0.276 #>## Simulate a set of null communities with permutation of residuals simulate(mod, indx = shuffleSet(nrow(dune), 99))#> An object of class “simulate.rda” #> ‘simulate index’ method (abundance, non-sequential) #> 20 x 30 matrix #> Number of permuted matrices = 99 #>