Fitting linear mixed effects model with latent Whittle-Matern models.
rspde_lme(
formula,
loc,
loc_time = NULL,
data,
model = NULL,
repl = NULL,
which_repl = NULL,
optim_method = "L-BFGS-B",
possible_methods = c("L-BFGS-B", "Nelder-Mead"),
use_data_from_graph = TRUE,
rspde_order = NULL,
mean_correction = FALSE,
previous_fit = NULL,
fix_coeff = FALSE,
model_options = list(),
smoothness_upper_bound = 4,
parallel = FALSE,
n_cores = parallel::detectCores() - 1,
optim_controls = list(),
improve_hessian = FALSE,
hessian_args = list(),
alpha = lifecycle::deprecated(),
nu = lifecycle::deprecated(),
beta = lifecycle::deprecated(),
starting_values_latent = lifecycle::deprecated(),
start_sigma_e = lifecycle::deprecated(),
start_alpha = lifecycle::deprecated(),
start_nu = lifecycle::deprecated(),
start_beta = lifecycle::deprecated(),
nu_upper_bound = lifecycle::deprecated()
)
A list containing the fitted model.
Formula object describing the relation between the response variables and the fixed effects. If the response variable is a matrix, each column of the matrix will be treated as a replicate.
A vector with the names of the columns in data
that contain the
observation locations, or a matrix
or a data.frame
containing the
observation locations. If the model is of class metric_graph
, the locations
must be either a matrix
or a data.frame
with two columns, or a character
vector with the names of the two columns. The first column being the number of
the edge, and the second column being the normalized position on the edge.
If the model is a 2d model, loc
must be either a matrix
or data.frame
with two columns or a character vector with the name of the two columns that
contain the location, the first entry corresponding to the x
entry and the
second corresponding to the y
entry.
For spatio-temporal models, the name of the column in data
that
is the time variable, or a matrix
or vector
containing the observation time
points.
A data.frame
containing the data to be used.
Object generated by matern.operators()
, spde.matern.operators()
or spacetime.operators()
. If NULL
, simple linear regression will be performed.
Vector indicating the replicate of each observation.
If NULL
it will assume there is only one replicate. If the model is generated from graphs from
metric_graph
class and use_data_from_graph
is TRUE
, repl
needs to be the name of the
column inside the metric graph data that contains the replicate. If NULL
it will assume there is only
one replicate.
Which replicates to use? If NULL
all replicates will be used.
The method to be used with optim
function.
The optimization methods to try if the model fitting fails.
Logical. Only for models generated from graphs from
metric_graph
class. In this case, should the data, the locations and the
replicates be obtained from the graph object?
The order of the rational approximation to be used while fitting the model. If not given, the order from the model object will be used. Not used for spatio-temporal models.
If TRUE, use mean correction for intrinsic models. Default FALSE.
An object of class rspde_lme
. Use the fitted coefficients as starting values.
If using a previous fit, should all coefficients be fixed at the starting values?
A list containing additional options to be used in the model. This will take preference over the values extracted from previous_fit. Currently, it is possible to fix parameters during the estimation or change the starting values of the parameters. The general structure of the elements of the list is fix_parname
and start_parname
, where parname
stands for the name of the parameter. If fix_parname
is not NULL
, then the model will be fitted with the parname
being fixed at the value that was passed. If start_parname
is not NULL
, the model will be fitted using the value passed as starting value for parname
. For 'rSPDE' and 'rSPDE1d' models, the possible elements of the list are fix_sigma_e
, start_sigma_e
, fix_nu
, start_nu
, fix_sigma
, start_sigma
, fix_range
, start_range
. Alternatively, one can also use the elements fix_sigma_e
, start_sigma_e
, fix_nu
, start_nu
, fix_tau
, start_tau
, fix_kappa
, start_kappa
. For 'spacetime' models, the possible elements of the list are fix_sigma_e
, start_sigma_e
, fix_kappa
, start_kappa
, fix_sigma
, start_sigma
, fix_gamma
, start_gamma
, fix_rho
, start_rho
. For dimension 2, the second coordinate of rho
has name rho2
and must be passed as start_rho2
and fix_rho2
. For 'rSPDE2d' models, the possible elements of the list are fix_sigma_e
, start_sigma_e
, fix_nu
, start_nu
, fix_sigma
, start_sigma
, fix_hx
, start_hx
, fix_hy
, start_hy
, fix_hxy
, start_hxy
. For nonstationary models, we have two options: the first is to pass the starting values as a vector with name start_theta
and a vector with the names of the parameters to be fixed with name fix_theta
; the second option is to handle the individual parameters, by passing the names thetan
where n
is the number of the parameter to pass the starting value or to be fixed. For example, to pass the starting value for theta3
one simply pass start_theta3
, and to fix theta2
, one simply pass fix_theta2
.
Upper bound for nu
, when nu
is the smoothness parameter, or for alpha - d/2
when alpha
is the smoothness parameter, or for max\{alpha - d/2, beta - d/2)
for intrinsic models.
logical. Indicating whether to use optimParallel or not.
Number of cores to be used if parallel is true.
Additional controls to be passed to optim
or optimParallel
.
Should a more precise estimate of the hessian be obtained? Turning on might increase the overall time.
List of controls to be used if improve_hessian
is TRUE
.
The list can contain the arguments to be passed to the method.args
argument
in the numDeriv::hessian
function. See the help of the hessian
function in
numDeriv
package for details. Observe that it only accepts the "Richardson"
method for now, the method "complex" is not supported.