Package {hmmTMB}


Type: Package
Title: Fit Hidden Markov Models using Template Model Builder
Version: 2.0.0
Maintainer: Theo Michelot <theo.michelot@dal.ca>
Description: Fitting hidden Markov models using automatic differentiation and Laplace approximation, allowing for fast inference and flexible covariate effects (including random effects and smoothing splines) on model parameters. The package is described by Michelot (2025) <doi:10.18637/jss.v114.i05>.
URL: https://github.com/TheoMichelot/hmmTMB
License: GPL-3
Depends: R6, mgcv, TMB, ggplot2
Imports: Matrix, stringr, MASS, tmbstan, methods, fmesher
LinkingTo: TMB, RcppEigen
Suggests: rstan, testthat, knitr, rmarkdown, expm, MSwM
Encoding: UTF-8
VignetteBuilder: knitr
Config/roxygen2/version: 8.1.0
NeedsCompilation: yes
Packaged: 2026-11-10 13:15:57 UTC; theo
Author: Theo Michelot [aut, cre], Richard Glennie [aut], Jan-Ole Fischer [ctb] (SPDE smooths), Duncan Cameron-Steinke [ctb] (Forecast class), Pauline Rocu [ctb] (schisq distribution), Litty Mathew [ctb] (hnbinom distribution)
Repository: CRAN
Date/Publication: 2026-11-10 15:10:10 UTC

hmmTMB: Fit Hidden Markov Models using Template Model Builder

Description

Fitting hidden Markov models using automatic differentiation and Laplace approximation, allowing for fast inference and flexible covariate effects (including random effects and smoothing splines) on model parameters. The package is described by Michelot (2025) doi:10.18637/jss.v114.i05.

Details

The package hmmTMB is based on three main classes (i.e., types of objects): MarkovChain, Observation, and HMM. Type ?MarkovChain, ?Observation or ?HMM to find their documentation, or consult the package vignettes for detailed examples of the hmmTMB workflow.

Author(s)

Maintainer: Theo Michelot theo.michelot@dal.ca

Authors:

Other contributors:

See Also

Useful links:


R6 class for probability distribution

Description

Contains the probability density/mass function, and the link and inverse link functions for a probability distribution.

Methods

Public methods


Dist$new()

Create a Dist object

Usage
Dist$new(
  name,
  pdf,
  rng,
  cdf = NULL,
  link,
  invlink,
  npar,
  parnames,
  parapprox = NULL,
  fixed = NULL,
  name_long = name,
  par_alt = NULL
)
Arguments
name

Name of distribution

pdf

Probability density/mass function of the distribution (e.g. dnorm for normal distribution).

rng

Random generator function of the distribution (e.g. rnorm for normal distribution).

cdf

Cumulative distribution function of the distribution (e.g., pnorm for normal distribution). This is used to compute pseudo-residuals.

link

Named list of link functions for distribution parameters

invlink

Named list of inverse link functions for distribution parameters

npar

Number of parameters of the distribution

parnames

Character vector with name of each parameter

parapprox

Function that takes a sample and produces approximate values for the unknown parameters

fixed

Vector with element for each parameter which is TRUE if parameter is fixed

name_long

Long version of the name of the distribution, possibly more user-readable than name.

par_alt

Function that takes a vector of the distribution parameters as input and returns them in a different format. Only relevant for some distributions (e.g., MVN, where the SDs and correlations can be reformatted into a covariance matrix)

Returns

A new Dist object


Dist$name()

Return name of Dist object

Usage
Dist$name()

Dist$pdf()

Return pdf of Dist object

Usage
Dist$pdf()

Dist$cdf()

Return cdf of Dist object

Usage
Dist$cdf()

Dist$rng()

Return random generator function of Dist object

Usage
Dist$rng()

Dist$link()

Return link function of Dist object

Usage
Dist$link()

Dist$invlink()

Return inverse link function of Dist object

Usage
Dist$invlink()

Dist$npar()

Return number of parameters of Dist object

Usage
Dist$npar()

Dist$parnames()

Return names of parameters

Usage
Dist$parnames()

Dist$parapprox()

Return function that approximates parameters

Usage
Dist$parapprox()

Dist$fixed()

Return which parameters are fixed

Usage
Dist$fixed()

Dist$code()

Return code of Dist object

Usage
Dist$code()

Dist$name_long()

Human-readable name of Dist object

Usage
Dist$name_long()

Dist$set_npar()

Set number of parameters this distribution has

Usage
Dist$set_npar(new_npar)
Arguments
new_npar

Number of parameters


Dist$set_parnames()

Set parameter names

Usage
Dist$set_parnames(new_parnames)
Arguments
new_parnames

Parameter names


Dist$set_code()

Set distribution code

Usage
Dist$set_code(new_code)
Arguments
new_code

Distribution code


Dist$pdf_apply()

Evaluate probability density/mass function

This method is used in the Dist$obs_probs() method. It is a wrapper around Dist$pdf(), which prepares the parameters and passes them to the function.

Usage
Dist$pdf_apply(x, par, log = FALSE)
Arguments
x

Value at which the function should be evaluated

par

Vector of parameters. The entries should be named if they are not in the same order as expected by the R function. (E.g. shape/scale rather than shape/rate for gamma distribution.)

log

Logical. If TRUE, the log-density is returned. Default: FALSE.

Returns

Probability density/mass function evaluated at x for parameters par


Dist$rng_apply()

Random number generator

This method is a wrapper around Dist$rng(), which prepares the parameters and passes them to the function.

Usage
Dist$rng_apply(n, par)
Arguments
n

Number of realisations to generate

par

Vector of parameters. The entries should be named if they are not in the same order as expected by the R function. (E.g. shape/scale rather than shape/rate for gamma distribution.)

Returns

Vector of n realisations of this distribution


Dist$par_alt()

Alternative parameter formatting

Usage
Dist$par_alt(par)
Arguments
par

Vector of distribution parameters

Returns

Formatted parameters


Dist$n2w()

Natural to working parameter transformation

This method transforms parameters from the natural scale (i.e., their domain of definition) to the "working" or "linear predictor" scale (i.e., the real line). It is a wrapper for Dist$link().

Usage
Dist$n2w(par)
Arguments
par

List of parameters

Returns

Vector of parameters on the working scale


Dist$w2n()

Working to natural parameter transformation

This method transforms parameters from the "working" or "linear predictor" scale (i.e., the real line) to the natural scale (i.e., their domain of definition). It is a wrapper for Dist$invlink().

Usage
Dist$w2n(wpar, as_matrix = FALSE)
Arguments
wpar

Vector of working parameters

as_matrix

Logical. If TRUE, the natural parameters are returned as a matrix with one row for each state and one column for each parameter. If FALSE, the natural parameters are returned as a list (default).

Returns

List or matrix of parameters on natural scale


Dist$clone()

The objects of this class are cloneable with this method.

Usage
Dist$clone(deep = FALSE)
Arguments
deep

Whether to make a deep clone.


R6 Class for Forecast in Hidden Markov Models

Description

Creates a forecast object from a fitted HMM model, projecting future state probabilities and unconditional observation densities for a user-defined horizon using a covariate data-frame if applicable. Forecasting occurs in the constructor; results are accessible via public methods.

Methods

Public methods


Forecast$new()

Construct a forecast object.

Usage
Forecast$new(
  hmm = NULL,
  n = NULL,
  forecast_data = NULL,
  preset_eval_range = NULL,
  starting_state_distribution = "last"
)
Arguments
hmm

A fitted HMM object.

n

Forecast horizon: a whole number greater than zero. Ignored if forecast_data is provided.

forecast_data

data.frame of future covariates / IDs. Must include all covariates in fitted hmm.

preset_eval_range

Named list: elements are numeric vectors (univariate) or matrices (multivariate, rows as dimension ex. mu1, mu2, columns as points). For any observation variable without an entry, a default grid of 100 equally spaced points is used, spanning the range of the training data for that variable with each endpoint expanded outward by 10% of its magnitude. A warning is issued whenever this default is applied, as the resulting grid may not suit the distribution's support.

starting_state_distribution

Distribution over states at the first forecast step. Either a numeric vector of length nstates() that is non-negative and sums to 1, or one of "last" (state probabilities at the final training row, propagated one step) or "stationary" (the model's stationary distribution).

Details

Algorithm overview

  1. Validate the arguments.

  2. Build or accept the future design matrix (forecast_data).

  3. Obtain time-varying transition matrices (tpm_forecast) and observation parameters (obs_par_forecast) via HMM$predict().

  4. Forward-propagate the hidden-state distribution (hidden_state_forecast).

  5. Marginalise over states to obtain unconditional pdfs on the evaluation grid (forecast_dists).

Returns

A Forecast object. Results are read back with the accessor methods below, each invoked with ():

hidden_state_forecast

Matrix of nstates rows by n forecast steps.

obs_par_forecast

Array of time-varying observation parameters.

tpm_forecast

Array of time-varying transition matrices.

forecast_dists

List of unconditional pdf matrices, one per observation variable.

eval_range

List of grids on which each pdf was evaluated.

forecast_data

The data.frame of future covariates used for prediction.

The evaluation grid can be changed after construction with update_eval_range(), which recomputes forecast_dists.

Examples
data(faithful)

# Create training and forecast data frames
training_fraction <- 0.8
n_training <- floor(nrow(faithful) * training_fraction)
training_df <- data.frame(
  ID = rep(1, n_training),
  waiting = faithful$waiting[1:n_training],
  eruptions = faithful$eruptions[1:n_training]
)
forecast_df <- data.frame(
  ID = rep(1, nrow(faithful) - n_training),
  waiting = faithful$waiting[(n_training + 1):nrow(faithful)],
  eruptions = faithful$eruptions[(n_training + 1):nrow(faithful)]
)
# Create 2-state model with non-linear effect of waiting on all transitions
hid_model <- MarkovChain$new(
  data = training_df,
  n_states = 2,
  formula = ~ s(waiting, k = 10, bs = "cs")
)

# Create observation model with normal distribution for duration
obs_model <- Observation$new(
  data = training_df,
  n_states = 2,
  dists = list(eruptions = "norm"),
  par = list(eruptions = list(
    mean = c(0, 0),
    sd = c(1, 1)
  ))
)
# Update model parameters to suggested
obs_model$update_par(par = obs_model$suggest_initial())
# Create HMM model
hmm <- HMM$new(
  hid = hid_model,
  obs = obs_model
)
hmm$fit(silent = TRUE)
# Create forecast object. Setting the evaluation grid explicitly is
# recommended; omitting it falls back to a default grid and warns.
forecast <- Forecast$new(
  hmm = hmm,
  forecast_data = forecast_df,
  preset_eval_range = list(eruptions = seq(1, 6, length.out = 100)),
  starting_state_distribution = "last"
)

# Unconditional predictive densities: grid points x forecast steps
dim(forecast$forecast_dists()$eruptions)

Forecast$obs_par_forecast()

Get predicted observation parameters.

Usage
Forecast$obs_par_forecast()

Forecast$tpm_forecast()

Get predicted transition matrices.

Usage
Forecast$tpm_forecast()

Forecast$eval_range()

Get the evaluation grid for each response variable.

Usage
Forecast$eval_range()

Forecast$forecast_data()

Get the forecast data used for predictions.

Usage
Forecast$forecast_data()

Forecast$update_eval_range()

Update the evaluation grid for forecast pdfs. This method reconfigures the evaluation range used to compute unconditional predictive pdfs. It validates the new eval_range, updates internal state, reinitializes forecast densities, and returns the object invisibly for chaining.

Usage
Forecast$update_eval_range(eval_range)
Arguments
eval_range

A named list specifying the new evaluation grid for each observation variable.

Returns

The Forecast object (invisibly), allowing method chaining.


Forecast$hidden_state_forecast()

Get the forward state probabilities.

Usage
Forecast$hidden_state_forecast()

Forecast$forecast_dists()

Get the unconditional predictive pdfs.

Usage
Forecast$forecast_dists()

Forecast$quantile()

Quantiles of forecast distribution

Usage
Forecast$quantile(var, probs)
Arguments
var

Name of observation variable, as character string

probs

Numeric vector of probabilities

Returns

Data frame with one column for each quantile probability and one row for each time step in the forecast


Forecast$mean()

Mean of forecast distribution

Usage
Forecast$mean(var)
Arguments
var

Name of observation variable, as character string

Returns

Numeric vector of means, with one element for each time step in the forecast


Forecast$plot()

Plot forecast

Usage
Forecast$plot(var, show_data = FALSE)
Arguments
var

Name of observation variable, as character string

show_data

Logical: should data be included in the plot?

Details

The plot shows the mean of the forecast distribution over time (red line), as well as bands of decreasing opacity for the 50 90

Returns

A ggplot object


Forecast$clone()

The objects of this class are cloneable with this method.

Usage
Forecast$clone(deep = FALSE)
Arguments
deep

Whether to make a deep clone.

See Also

HMM for the fitted model that is forecast from, and MarkovChain and Observation for the hidden state and observation components it is built from.

Examples


## ------------------------------------------------
## Method `Forecast$new()`
## ------------------------------------------------


data(faithful)

# Create training and forecast data frames
training_fraction <- 0.8
n_training <- floor(nrow(faithful) * training_fraction)
training_df <- data.frame(
  ID = rep(1, n_training),
  waiting = faithful$waiting[1:n_training],
  eruptions = faithful$eruptions[1:n_training]
)
forecast_df <- data.frame(
  ID = rep(1, nrow(faithful) - n_training),
  waiting = faithful$waiting[(n_training + 1):nrow(faithful)],
  eruptions = faithful$eruptions[(n_training + 1):nrow(faithful)]
)
# Create 2-state model with non-linear effect of waiting on all transitions
hid_model <- MarkovChain$new(
  data = training_df,
  n_states = 2,
  formula = ~ s(waiting, k = 10, bs = "cs")
)

# Create observation model with normal distribution for duration
obs_model <- Observation$new(
  data = training_df,
  n_states = 2,
  dists = list(eruptions = "norm"),
  par = list(eruptions = list(
    mean = c(0, 0),
    sd = c(1, 1)
  ))
)
# Update model parameters to suggested
obs_model$update_par(par = obs_model$suggest_initial())
# Create HMM model
hmm <- HMM$new(
  hid = hid_model,
  obs = obs_model
)
hmm$fit(silent = TRUE)
# Create forecast object. Setting the evaluation grid explicitly is
# recommended; omitting it falls back to a default grid and warns.
forecast <- Forecast$new(
  hmm = hmm,
  forecast_data = forecast_df,
  preset_eval_range = list(eruptions = seq(1, 6, length.out = 100)),
  starting_state_distribution = "last"
)

# Unconditional predictive densities: grid points x forecast steps
dim(forecast$forecast_dists()$eruptions)


R6 class for hidden Markov model

Description

Encapsulates the observation and hidden state models for a hidden Markov model.

Methods

Public methods


HMM$new()

Create new HMM object

Usage
HMM$new(
  obs = NULL,
  hid = NULL,
  file = NULL,
  init = NULL,
  fixpar = NULL,
  bw = NULL
)
Arguments
obs

Observation object, created with Observation$new(). This contains the formulation for the observation model.

hid

MarkovChain object, created with MarkovChain$new(). This contains the formulation for the state process model.

file

Path to specification file for HMM. If this argument is used, then obs and hid are unnecessary.

init

HMM object, used to initialise the parameters for this model. If init is passed, then all parameters that are included in init and in the present model are copied. This may be useful when fitting increasingly complex models: start from a simple model, then pass it as init to create a more complex model, and so on.

fixpar

Named list, with optional elements: 'hid', 'obs', 'delta0', 'lambda_obs', and 'lambda_hid'. Each element is a named vector of parameters in coeff_fe that should either be fixed (if the corresponding element is set to NA) or estimated to a common value (using integers or factor levels).don See examples in the vignettes, and check the TMB documentation to understand the inner workings (argument map of TMB::MakeADFun()).

bw

Bandwidth of the banded forward algorithm; see HMM$update_bw(). Defaults to NULL, i.e. 15 if the model contains a Gaussian field and 0 (the exact algorithm) otherwise.

Returns

A new HMM object

Examples
# Load data set (included with R)
data(nottem)
data <- data.frame(temp = as.vector(t(nottem)))

# Create hidden state and observation models
hid <- MarkovChain$new(data = data, n_states = 2)
par0 <- list(temp = list(mean = c(40, 60), sd = c(5, 5)))
obs <- Observation$new(data = data, n_states = 2,
                       dists = list(temp = "norm"),
                       par = par0)

# Create HMM
hmm <- HMM$new(hid = hid, obs = obs)

HMM$obs()

Observation object for this model

Usage
HMM$obs()

HMM$hid()

MarkovChain object for this model

Usage
HMM$hid()

HMM$out()

Output of optimiser after model fitting

Usage
HMM$out()

HMM$tmb_obj()

Model object created by TMB. This is the output of the TMB function MakeADFun, and it is a list including elements

fn

Objective function

gr

Gradient function of fn

par

Vector of initial parameters on working scale

Usage
HMM$tmb_obj()

HMM$tmb_obj_joint()

Model object created by TMB for the joint likelihood of the fixed and random effects. This is the output of the TMB function MakeADFun, and it is a list including elements

fn

Objective function

gr

Gradient function of fn

par

Vector of initial parameters on working scale

Usage
HMM$tmb_obj_joint()

HMM$tmb_rep()

Output of the TMB function sdreport, which includes estimates and standard errors for all model parameters.

Usage
HMM$tmb_rep()

HMM$states()

Vector of estimated states, after viterbi has been run

Usage
HMM$states()

HMM$coeff_fe()

Coefficients for fixed effect parameters

Usage
HMM$coeff_fe()

HMM$coeff_re()

Coefficients for random effect parameters

Usage
HMM$coeff_re()

HMM$coeff_list()

List of all model coefficients

These are the parameters estimated by the model, including fixed and random effect parameters for the observation parameters and the transition probabilities, (transformed) initial probabilities, and smoothness parameters.

Usage
HMM$coeff_list()

HMM$fixpar()

Fixed parameters

Usage
HMM$fixpar(all = FALSE)
Arguments
all

Logical. If FALSE, only user-specified fixed parameters are returned, but not parameters that are fixed by definition (e.g., size of binomial distribution).


HMM$coeff_array()

Array of working parameters

Usage
HMM$coeff_array()

HMM$lambda()

Smoothness parameters

Usage
HMM$lambda()

HMM$bw()

Bandwidth of the forward algorithm (0 = exact)

Usage
HMM$bw()

HMM$update_bw()

Update bandwidth of the forward algorithm

The exact forward algorithm accumulates log-likelihood contributions that are each conditional on the entire process history, so the Hessian with respect to latent variables spread over time is dense. The banded algorithm of Fischer (2026) splits the time series into blocks of length bw and truncates that conditioning at the previous block, which makes the Hessian banded. It costs about twice as much per evaluation, and its error decays geometrically in bw, because an ergodic Markov chain forgets its initial condition exponentially fast.

A model containing a Gaussian field is banded by default, with bw = 15, because the dense Hessian of the exact algorithm defeats the sparsity such a field exists to provide. That default is a starting point, not an answer: the bandwidth needed depends on how fast the chain forgets its initial condition, so a persistent chain needs more. Every other model is exact by default. Use HMM$check_bw() to choose a bandwidth before fitting, and afterwards check that raising it leaves the estimates unchanged.

Usage
HMM$update_bw(bw = NULL)
Arguments
bw

Non-negative integer (0 = exact algorithm), or NULL to choose automatically. This is TMB data, so changing it discards any existing setup, which is rebuilt on the next setup() or fit().


HMM$check_bw()

Profile the log-likelihood against the bandwidth

Evaluates the joint log-likelihood at the model's current parameter values for a range of bandwidths. A sensible bandwidth is the smallest one beyond which the value no longer changes appreciably. This is evaluated at fixed parameters, so it is cheap and does not require the model to be re-fitted.

Usage
HMM$check_bw(bws = seq(5, 40, by = 5), silent = TRUE)
Arguments
bws

Vector of bandwidths (each at least 2)

silent

Logical. If TRUE (default), TMB tracing output is hidden.

Returns

Data frame with columns bw and llk, including a row with bw = Inf for the exact forward algorithm.


HMM$update_par()

Update parameters stored inside model object

Usage
HMM$update_par(par_list = NULL, iter = NULL)
Arguments
par_list

List with elements for coeff_fe_obs, coeff_fe_hid, coeff_re_obs, coeff_re_hid, log_delta0, log_lambda_hid, and log_lambda_obs

iter

Optional argument to update model parameters based on MCMC iterations (if using rstan). Either the index of the iteration to use, or "mean" if the posterior mean should be used.


HMM$sd_re()

Standard deviation of smooth terms (or random effects)

This function transforms the smoothness parameter of each smooth term into a standard deviation, given by SD = 1/sqrt(lambda). It is particularly helpful to get the standard deviations of independent normal random effects.

Usage
HMM$sd_re()
Returns

List of standard deviations for observation model and hidden state model.


HMM$par()

Model parameters

Usage
HMM$par(t = 1)
Arguments
t

returns parameters at time t, default is t = 1

Returns

A list with elements:

obspar

Parameters of observation model

tpm

Transition probability matrix of hidden state model


HMM$set_priors()

Set priors for coefficients

Usage
HMM$set_priors(new_priors = NULL)
Arguments
new_priors

is a named list of matrices with optional elements coeff_fe_obs, coeff_fe_hid, log_lambda_obs, andlog_lambda_hid. Each matrix has two columns (first col = mean, second col = sd) specifying parameters for normal priors.


HMM$priors()

Extract stored priors

Usage
HMM$priors()

HMM$iters()

Iterations from stan MCMC fit

Usage
HMM$iters(type = "response")
Arguments
type

Either "response" for parameters on the response (natural) scale, or "raw" for parameters on the linear predictor scale.

Returns

see output of as.matrix in stan


HMM$out_stan()

fitted stan object from MCMC fit

Usage
HMM$out_stan()
Returns

the stanfit object


HMM$llk()

Log-likelihood at current parameters

Usage
HMM$llk()
Returns

Log-likelihood


HMM$edf()

Effective degrees of freedom

Usage
HMM$edf()
Returns

Number of effective degrees of freedom (accounting for flexibility in non-parametric terms implied by smoothing)


HMM$suggest_initial()

Suggest initial parameter values

Uses K-means clustering to split the data into naive "states", and estimates observation parameters within each of these states. This is meant to help with selecting initial parameter values before model fitting, but users should still think about the values carefully, and try multiple set of initial parameter values to ensure convergence to the global maximum of the likelihood function.

Usage
HMM$suggest_initial()
Returns

List of initial parameters


HMM$setup()

TMB setup

This creates an attribute tmb_obj, which can be used to evaluate the negative log-likelihood function.

Usage
HMM$setup(silent = TRUE)
Arguments
silent

Logical. If TRUE, all tracing outputs are hidden (default).


HMM$fit_stan()

Fit model using tmbstan

Consult documentation of the tmbstan package for more information. After this method has been called, the Stan output can be accessed using the method out_stan(). This Stan output can for example be visualised using functions from the rstan package. The parameters stored in this HMM object are automatically updated to the mean posterior estimate, although this can be changed using update_par().

Usage
HMM$fit_stan(..., silent = FALSE)
Arguments
...

Arguments passed to tmbstan

silent

Logical. If FALSE, all tracing outputs are shown (default).


HMM$fit()

Model fitting

The negative log-likelihood of the model is minimised using the function nlminb(). TMB uses the Laplace approximation to integrate the random effects out of the likelihood.

After the model has been fitted, the output of nlminb() can be accessed using the method out(). The estimated parameters can be accessed using the methods par() (for the HMM parameters, possibly dependent on covariates), predict() (for uncertainty quantification and prediction of the HMM parameters for new covariate values), coeff_fe() (for estimated fixed effect coefficients on the linear predictor scale), and coeff_re() (for estimated random effect coefficients on the linear predictor scale).

Usage
HMM$fit(silent = FALSE, ...)
Arguments
silent

Logical. If FALSE, all tracing outputs are shown (default).

...

Other arguments to nlminb which is used to optimise the likelihood. This currently only supports the additional argument control, which is a list of control parameters such as eval.max and iter.max (see ?nlminb)

Examples
# Load data set (included with R)
data(nottem)
data <- data.frame(temp = as.vector(t(nottem)))

# Create hidden state and observation models
hid <- MarkovChain$new(data = data, n_states = 2)
par0 <- list(temp = list(mean = c(40, 60), sd = c(5, 5)))
obs <- Observation$new(data = data, n_states = 2,
                       dists = list(temp = "norm"),
                       par = par0)

# Create HMM
hmm <- HMM$new(hid = hid, obs = obs)

# Fit HMM
hmm$fit(silent = TRUE)

HMM$mle()

Get maximum likelihood estimates once model fitted

Usage
HMM$mle()
Returns

list of maximum likelihood estimates as described as input for the function update_par()


HMM$forward_backward()

Forward-backward algorithm

The forward probability for time step t and state j is the joint pdf/pmf of observations up to time t and of being in state j at time t, p(Z[1], Z[2], ..., Z[t], S[t] = j). The backward probability for time t and state j is the conditional pdf/pmf of observations between time t + 1 and n, given state j at time t, p(Z[t+1], Z[t+2], ..., Z[n] | S[t] = j). This function returns their logarithm, for use in other methods state_probs, and sample_states.

Usage
HMM$forward_backward()
Returns

Log-forward and log-backward probabilities


HMM$pseudores()

Pseudo-residuals

Compute pseudo-residuals for the fitted model. If the fitted model is the "true" model, the pseudo-residuals follow a standard normal distribution. Deviations from normality suggest lack of fit.

Usage
HMM$pseudores()
Returns

List (of length the number of variables), where each element is a vector of pseudo-residuals (of length the number of data points)


HMM$viterbi()

Viterbi algorithm

Usage
HMM$viterbi()
Returns

Most likely state sequence


HMM$sample_states()

Sample posterior state sequences using forward-filtering backward-sampling

The forward-filtering backward-sampling algorithm returns a sequence of states, similarly to the Viterbi algorithm, but it generates it from the posterior distribution of state sequences, i.e., accounting for uncertainty in the state classification. Multiple generated sequences will therefore generally not be the same.

Usage
HMM$sample_states(nsamp = 1, full = FALSE)
Arguments
nsamp

Number of samples to produce

full

If TRUE and model fit by fit_stan then parameter estimates are sampled from the posterior samples before simulating each sequence

Returns

Matrix where each column is a different sample of state sequences, and each row is a time of observation


HMM$state_probs()

Compute posterior probability of being in each state

Usage
HMM$state_probs()
Returns

matrix with a row for each observation and a column for each state


HMM$post_coeff()

Posterior sampling for model coefficients

Usage
HMM$post_coeff(n_post)
Arguments
n_post

Number of posterior samples

Returns

Matrix with one column for each coefficient and one row for each posterior draw


HMM$post_linpred()

Posterior sampling for linear predictor

Usage
HMM$post_linpred(n_post)
Arguments
n_post

Number of posterior samples

Returns

List with elements obs and hid, where each is a matrix with one column for each predictor and one row for each posterior draw


HMM$post_fn()

Create posterior simulations of a function of a model component

Usage
HMM$post_fn(fn, n_post, comp = NULL, ..., level = 0, return_post = FALSE)
Arguments
fn

Function which takes a vector of linear predictors as input and produces either a scalar or vector output

n_post

Number of posterior simulations

comp

Either "obs" for observation model linear predictor, or "hid" for hidden model linear predictor

...

Arguments passed to fn

level

Confidence interval level if required (e.g., 0.95 for 95 confidence intervals). Default is 0, i.e., confidence intervals are not returned.

return_post

Logical indicating whether to return the posterior samples. If FALSE (default), only mean estimates and confidence intervals are returned

Returns

A list with elements:

post

If return_post = TRUE, this is a vector (for scalar outputs of fn) or matrix (for vector outputs) with a column for each simulation

mean

Mean over posterior samples

lcl

Lower confidence interval bound (if level !=0)

ucl

Upper confidence interval bound (if level !=0)


HMM$predict()

Predict estimates from a fitted model

By default, this returns point estimates of the HMM parameters for a new data frame of covariates. See the argument 'n_post' to also get confidence intervals.

Usage
HMM$predict(
  what,
  t = 1,
  newdata = NULL,
  n_post = 0,
  level = 0.95,
  return_post = FALSE,
  as_list = TRUE
)
Arguments
what

Which estimates to predict? Options include transition probability matrices "tpm", stationary distributions "delta", or observation distribution parameters "obspar"

t

Time points to predict at

newdata

New dataframe to use for prediction

n_post

If greater than zero then n_post posterior samples are produced, and used to create confidence intervals.

level

Level of the confidence intervals, e.g. CI = 0.95 will produce 95% confidence intervals (default)

return_post

Logical. If TRUE, a list of posterior samples is returned.

as_list

Logical. If confidence intervals are required for the transition probabilities or observation parameters, this argument determines whether the MLE, lower confidence limit and upper confidence limit are returned as separate elements in a list (if TRUE; default), or whether they are combined into a single array (if FALSE). Ignored if what = "delta" or if n_post = 0.

...

Other arguments to the respective functions for hid$tpm, hid$delta, obs$par

Returns

Maximum likelihood estimates (mle) of predictions, and confidence limits (lcl and ucl) if requested. The format of the output depends on whether confidence intervals are required (specified through n_post), and on the argument as_list.

Examples
# Load data set (included with R)
data(nottem)
data <- data.frame(temp = as.vector(t(nottem)))

# Create hidden state and observation models
hid <- MarkovChain$new(data = data, n_states = 2)
par0 <- list(temp = list(mean = c(40, 60), sd = c(5, 5)))
obs <- Observation$new(data = data, n_states = 2,
                       dists = list(temp = "norm"),
                       par = par0)

# Create HMM
hmm <- HMM$new(hid = hid, obs = obs)

# Fit HMM
hmm$fit(silent = TRUE)

# Get transition probability matrix with confidence intervals
hmm$predict(what = "tpm", n_post = 1000)

HMM$confint()

Confidence intervals for working parameters

This function computes standard errors for all fixed effect model parameters based on the diagonal of the inverse of the Hessian matrix, and then derives Wald-type confidence intervals.

Usage
HMM$confint(level = 0.95)
Arguments
level

Level of confidence intervals. Defaults to 0.95, i.e., 95% confidence intervals.

Returns

List of matrices with three columns: mle (maximum likelihood estimate), lcl (lower confidence limit), ucl (upper confidence limit), and se (standard error). One such matrix is produced for the working parameters of the observation model, the working parameters of the hidden state model, the smoothness parameters of the observation model, and the smoothness parameters of the hidden state model.


HMM$simulate()

Simulate from hidden Markov model

Usage
HMM$simulate(n, data = NULL, silent = FALSE)
Arguments
n

Number of time steps to simulate

data

Optional data frame including covariates

silent

if TRUE then no messages are printed

Returns

Data frame including columns of data (if provided), and simulated data variables


HMM$check()

Compute goodness-of-fit statistics using simulation

Many time series are simulated from the fitted model, and the statistic(s) of interest are calculated for each. A histogram of those values can for example be used to compare to the observed value of the statistic. An observation far in the tails of the distribution of simulated statistics suggests lack of fit.

Usage
HMM$check(check_fn, nsims = 100, full = FALSE, silent = FALSE)
Arguments
check_fn

Goodness-of-fit function which accepts "data" as input and returns a statistic (either a vector or a single number) to be compared between observed data and simulations.

nsims

Number of simulations to perform

full

If model fitted with 'fit_stan', then full = TRUE will sample from posterior for each simulation

silent

Logical. If FALSE, simulation progress is shown. (Default: TRUE)

Returns

List with elements:

obs_stat:

Vector of values of goodness-of-fit statistics for the observed data

stats:

Matrix of values of goodness-of-fit statistics for the simulated data sets (one row for each statistic, and one column for each simulation)

plot:

ggplot object


HMM$plot_ts()

Time series plot coloured by states

Creates a plot of the data coloured by the most likely state sequence, as estimated by the Viterbi algorithm. If one variable name is passed as input, it is plotted against time. If two variables are passed, they are plotted against each other.

Usage
HMM$plot_ts(var, var2 = NULL, line = TRUE)
Arguments
var

Name of the variable to plot.

var2

Optional name of a second variable, for 2-d plot.

line

Logical. If TRUE (default), lines are drawn between successive data points. Can be set to FALSE if another geom is needed (e.g., geom_point).

Returns

A ggplot object


HMM$plot_dist()

Plot observation distributions weighted by frequency in Viterbi

This is a wrapper around Observation$plot_dist, where the distribution for each state is weighted by the proportion of time spent in that state (according to the Viterbi state sequence).

Usage
HMM$plot_dist(var = NULL)
Arguments
var

Name of data variable. If NULL, a list of plots are returned (one for each observation variable)

Returns

Plot of distributions with data histogram


HMM$plot()

Plot a model component

Usage
HMM$plot(
  what,
  var = NULL,
  covs = NULL,
  i = NULL,
  j = NULL,
  n_grid = 50,
  n_post = 1000
)
Arguments
what

Name of model component to plot: should be one of "tpm" (transition probabilities), "delta" (stationary state probabilities), or "obspar" (state-dependent observation parameters)

var

Name of covariate to plot on x-axis

covs

Optional named list for values of covariates (other than 'var') that should be used in the plot (or dataframe with single row). If this is not specified, the mean value is used for numeric variables, and the first level for factor variables.

i

If plotting tpm then rows of tpm; if plotting delta then indices of states to plot; if plotting obspar then full names of parameters to plot (e.g., obsvar.mean)

j

If plotting tpm then columnss of tpm to plot; if plotting delta then this is ignored,; if plotting obspar then indices of states to plot

n_grid

Number of points in grid over x-axis (default: 50)

n_post

Number of posterior simulations to use when computing confidence intervals; default: 1000. See predict function for more detail.

Returns

A ggplot object


HMM$plot_2d()

Plot a model component over two covariates

The two-dimensional counterpart of HMM$plot(), for a model containing a bivariate smooth such as s(x, y) or a Gaussian field. HMM$plot() varies one covariate and holds the rest fixed, which for a bivariate term shows a single slice through the surface; this varies both and draws the surface itself.

Nothing here is specific to any basis. The surface is built from HMM$predict() on a lattice of covariate values, so it works for any smoother hmmTMB accepts on two covariates – a thin plate spline, bs = "gp", an SPDE field – and for two covariates that enter the model separately, where it shows their combined effect.

Usage
HMM$plot_2d(
  what,
  var,
  var2,
  covs = NULL,
  i = NULL,
  j = NULL,
  n_grid = 50,
  n_post = 0,
  level = 0.95,
  show = "mle",
  too_far = 0.1,
  contour = TRUE,
  padding = 0
)
Arguments
what

Name of model component to plot: one of "tpm" (transition probabilities), "delta" (stationary state probabilities), or "obspar" (state-dependent observation parameters)

var

Name of covariate on the x-axis

var2

Name of covariate on the y-axis

covs

Optional named list for values of covariates other than var and var2. If not specified, the mean is used for numeric covariates and the first level for factors.

i

If plotting tpm then rows of tpm; if plotting delta then indices of states; if plotting obspar then full names of parameters

j

If plotting tpm then columns of tpm; if plotting delta then ignored; if plotting obspar then indices of states

n_grid

Number of points along each axis, so the surface is evaluated at n_grid^2 points (default: 50). At the default n_post = 0 this costs one prediction and is cheap even for a fine grid; with posterior simulation the cost grows with n_grid^2, so it is worth lowering there.

n_post

Number of posterior simulations used for the confidence interval. Defaults to 0, i.e. the maximum likelihood surface only, because a surface needs many more evaluation points than a curve does. Required to be positive for show = "ci".

level

Confidence level, when n_post > 0 (default: 0.95)

show

What the fill shows: "mle" for the estimate itself, or "ci" for the width of the confidence interval, which says where the surface is well determined and where it is not.

too_far

Cells whose distance from the nearest observation exceeds this, as a proportion of the plot's diagonal, are left blank. This is mgcv::exclude.too.far(), and it matters for a bivariate smooth: the corners of the lattice are usually extrapolation. Set to 0 to show the whole rectangle (default: 0.1).

contour

Add contour lines over the surface (default: TRUE)

padding

Numeric vector of length 1 or 2 giving the amount to pad the 'var' and 'var2' ranges beyond the data. A single value is recycled to both axes, and a length-2 vector is interpreted as (padding in var, padding in var2). Defaults to 0.

Returns

A ggplot object


HMM$AIC_marginal()

Marginal Akaike Information Criterion

The marginal AIC is for example defined by Wood (2017), as AIC = - 2L + 2k where L is the maximum marginal log-likelihood (of fixed effects), and k is the number of degrees of freedom of the fixed effect component of the model

Usage
HMM$AIC_marginal()
Returns

Marginal AIC


HMM$AIC_conditional()

Conditional Akaike Information Criterion

The conditional AIC is for example defined by Wood (2017), as AIC = - 2L + 2k where L is the maximum joint log-likelihood (of fixed and random effects), and k is the number of effective degrees of freedom of the model (accounting for flexibility in non-parametric terms implied by smoothing)

Usage
HMM$AIC_conditional()
Returns

Conditional AIC


HMM$print_obspar()

Print observation parameters at t = 1

Usage
HMM$print_obspar()

HMM$print_tpm()

Print observation parameters at t = 1

Usage
HMM$print_tpm()

HMM$formulation()

Print model formulation

Usage
HMM$formulation()

HMM$print()

Print HMM object

Usage
HMM$print()

HMM$clone()

The objects of this class are cloneable with this method.

Usage
HMM$clone(deep = FALSE)
Arguments
deep

Whether to make a deep clone.

Examples


## ------------------------------------------------
## Method `HMM$new()`
## ------------------------------------------------

# Load data set (included with R)
data(nottem)
data <- data.frame(temp = as.vector(t(nottem)))

# Create hidden state and observation models
hid <- MarkovChain$new(data = data, n_states = 2)
par0 <- list(temp = list(mean = c(40, 60), sd = c(5, 5)))
obs <- Observation$new(data = data, n_states = 2,
                       dists = list(temp = "norm"),
                       par = par0)

# Create HMM
hmm <- HMM$new(hid = hid, obs = obs)

## ------------------------------------------------
## Method `HMM$fit()`
## ------------------------------------------------

# Load data set (included with R)
data(nottem)
data <- data.frame(temp = as.vector(t(nottem)))

# Create hidden state and observation models
hid <- MarkovChain$new(data = data, n_states = 2)
par0 <- list(temp = list(mean = c(40, 60), sd = c(5, 5)))
obs <- Observation$new(data = data, n_states = 2,
                       dists = list(temp = "norm"),
                       par = par0)

# Create HMM
hmm <- HMM$new(hid = hid, obs = obs)

# Fit HMM
hmm$fit(silent = TRUE)

## ------------------------------------------------
## Method `HMM$predict()`
## ------------------------------------------------

# Load data set (included with R)
data(nottem)
data <- data.frame(temp = as.vector(t(nottem)))

# Create hidden state and observation models
hid <- MarkovChain$new(data = data, n_states = 2)
par0 <- list(temp = list(mean = c(40, 60), sd = c(5, 5)))
obs <- Observation$new(data = data, n_states = 2,
                       dists = list(temp = "norm"),
                       par = par0)

# Create HMM
hmm <- HMM$new(hid = hid, obs = obs)

# Fit HMM
hmm$fit(silent = TRUE)

# Get transition probability matrix with confidence intervals
hmm$predict(what = "tpm", n_post = 1000)

R6 class for HMM hidden process model

Description

Contains the parameters and model formulas for the hidden process model.

Methods

Public methods


MarkovChain$new()

Create new MarkovChain object

Usage
MarkovChain$new(
  data = NULL,
  formula = NULL,
  n_states,
  tpm = NULL,
  initial_state = "estimated",
  fixpar = NULL,
  ref = 1:n_states,
  gam_args = NULL
)
Arguments
data

Data frame, needed to create model matrices, and to identify the number of time series (which each have a separate initial distribution)

formula

Either (1) R formula, used for all transition probabilities, or (2) matrix of character strings giving the formula for each transition probability, with "." along the diagonal (or for reference elements; see ref argument). (Default: no covariate dependence.)

n_states

Number of states. If not specified, then formula needs to be provided as a matrix, and n_states is deduced from its dimensions.

tpm

Optional transition probability matrix, to initialise the model parameters (intercepts in model with covariates). If not provided, the default is a matrix with 0.9 on the diagonal.

initial_state

Specify model for initial state distribution. There are five different options:

  • "estimated": a separate initial distribution is estimated for each ID (default)

  • "stationary": the initial distribution is fixed to the stationary distribution of the transition probability matrix for the first time point of each ID

  • "shared": a common initial distribution is estimated for all IDs

  • integer value between 1 and n_states: used as the known initial state for all IDs

  • vector of integers between 1 and n_states (of length the number of IDs): each element is used as the known initial state for the corresponding ID

fixpar

List with optional elements "hid" (fixed parameters for transition probabilities), "lambda_hid" (fixed smoothness parameters), and "delta0" (fixed parameters for initial distribution). Each element is a named vector of coefficients that should either be fixed (if the corresponding element is set to NA) or estimated to a common value (using integers or factor levels).

ref

Vector of indices for reference transition probabilities, of length n_states. The i-th element is the index for the reference in the i-th row of the transition probability matrix. For example, ref = c(1, 1) means that the first element of the first row Pr(1>1) and the first element of the second row Pr(2>1) are used as reference elements and are not estimated. If this is not provided, the diagonal transition probabilities are used as references.

gam_args

Named list of arguments passed to mgcv::gam() in MarkovChain$make_mat(), e.g., "knots". Use at your own risk.

Returns

A new MarkovChain object

Examples
# Load data set from MSwM package
data(energy, package = "MSwM")

# Create 2-state covariate-free model and initialise transition 
# probability matrix
hid <- MarkovChain$new(data = energy, n_states = 2,
                       tpm = matrix(c(0.8, 0.3, 0.2, 0.7), 2, 2))

# Create 2-state model with non-linear effect of Oil on all transition 
# probabilities
hid <- MarkovChain$new(data = energy, n_states = 2,
                       formula = ~ s(Oil, k = 5, bs = "cs"))

# Create 2-state model with quadratic effect of Oil on Pr(1 > 2)
structure <- matrix(c(".", "~poly(Oil, 2)",
                      "~1", "."),
                    ncol = 2, byrow = TRUE)
hid <- MarkovChain$new(data = energy, n_states = 2,
                       formula = structure)

MarkovChain$formula()

Formula of MarkovChain model

Usage
MarkovChain$formula()

MarkovChain$formulas()

List of formulas for MarkovChain model

Usage
MarkovChain$formulas()

MarkovChain$tpm()

Get transition probability matrices

Usage
MarkovChain$tpm(t = 1, linpred = NULL)
Arguments
t

Time index or vector of time indices; default = 1. If t = "all" then all transition probability matrices are returned.

linpred

Optional custom linear predictor

Returns

Array with one slice for each transition probability matrix


MarkovChain$ref()

Indices of reference elements in transition probability matrix

Usage
MarkovChain$ref()

MarkovChain$ref_mat()

Matrix of reference elements in transition probability matrix

Usage
MarkovChain$ref_mat()

MarkovChain$ref_delta0()

Indices of reference elements in initial distribution

Usage
MarkovChain$ref_delta0()

MarkovChain$coeff_fe()

Current parameter estimates (fixed effects)

Usage
MarkovChain$coeff_fe()

MarkovChain$delta()

Stationary distribution

Usage
MarkovChain$delta(t = NULL, linpred = NULL)
Arguments
t

Time point(s) for which stationary distribution should be returned. If t = "all", all deltas are returned; else this should be a vector of time indices. If NULL (default), the stationary distribution for the first time step is returned.

linpred

Optional custom linear predictor

Returns

Matrix of stationary distributions. Each row corresponds to a row of the design matrices, and each column corresponds to a state.


MarkovChain$delta0()

Initial distribution

Usage
MarkovChain$delta0(log = FALSE, as_matrix = TRUE)
Arguments
log

Logical indicating whether to return the log of the initial probabilities (default: FALSE). If TRUE, then the last element is excluded, as it is not estimated.

as_matrix

Logical indicating whether the output should be formatted as a matrix (default). If as_matrix is FALSE and log is TRUE, the result is formatted as a column vector.

Returns

Matrix with one row for each time series ID, and one column for each state. For each ID, the i-th element of the corresponding row is the probability Pr(S[1] = i)


MarkovChain$stationary()

Use stationary distribution as initial distribution?

Usage
MarkovChain$stationary()

MarkovChain$fixpar()

Fixed parameters

Usage
MarkovChain$fixpar(all = FALSE)
Arguments
all

Logical. If FALSE, only user-specified fixed parameters are returned, but not parameters that are fixed for some other reason (e.g., from '.' in formula)


MarkovChain$coeff_re()

Current parameter estimates (random effects)

Usage
MarkovChain$coeff_re()

MarkovChain$X_fe()

Fixed effect design matrix

Usage
MarkovChain$X_fe()

MarkovChain$X_re()

Random effect design matrix

Usage
MarkovChain$X_re()

MarkovChain$lambda()

Smoothness parameters

Usage
MarkovChain$lambda()

MarkovChain$sd_re()

Standard deviation of smooth terms

This function transforms the smoothness parameter of each smooth term into a standard deviation, given by SD = 1/sqrt(lambda). It is particularly helpful to get the standard deviations of independent normal random effects. A smooth with its own parameterisation rather than a single smoothness parameter – a Gaussian field, whose parameters are already a marginal standard deviation and a range – has no such transformation and returns NA; read those off lambda() directly.

Usage
MarkovChain$sd_re()

MarkovChain$nstates()

Number of states

Usage
MarkovChain$nstates()

MarkovChain$terms()

Terms of model formulas

Usage
MarkovChain$terms()

MarkovChain$unique_ID()

Number of time series

Usage
MarkovChain$unique_ID()

MarkovChain$initial_state()

Initial state (see constructor argument)

Usage
MarkovChain$initial_state()

MarkovChain$empty()

Empty model? (for simulation only)

Usage
MarkovChain$empty()

MarkovChain$gam_args()

Extra arguments for mgcv::gam (passed to make_matrices)

Usage
MarkovChain$gam_args()

MarkovChain$update_tpm()

Update transition probability matrix

Usage
MarkovChain$update_tpm(tpm)
Arguments
tpm

New transition probability matrix


MarkovChain$update_coeff_fe()

Update coefficients for fixed effect parameters

Usage
MarkovChain$update_coeff_fe(coeff_fe)
Arguments
coeff_fe

Vector of coefficients for fixed effect parameters


MarkovChain$update_coeff_re()

Update coefficients for random effect parameters

Usage
MarkovChain$update_coeff_re(coeff_re)
Arguments
coeff_re

Vector of coefficients for random effect parameters


MarkovChain$update_X_fe()

Update design matrix for fixed effects

Usage
MarkovChain$update_X_fe(X_fe)
Arguments
X_fe

new design matrix for fixed effects


MarkovChain$update_X_re()

Update design matrix for random effects

Usage
MarkovChain$update_X_re(X_re)
Arguments
X_re

new design matrix for random effects


MarkovChain$update_delta0()

Update initial distribution

Usage
MarkovChain$update_delta0(delta0)
Arguments
delta0

Either a matrix where the i-th row is the initial distribution for the i-th time series in the data, or a vector which is then used for all time series. Entries of each row of delta0 should sum to one.


MarkovChain$update_lambda()

Update smoothness parameters

Usage
MarkovChain$update_lambda(lambda)
Arguments
lambda

New smoothness parameter vector


MarkovChain$update_fixpar()

Update information about fixed parameters

Usage
MarkovChain$update_fixpar(fixpar)
Arguments
fixpar

New list of fixed parameters, in the same format expected by MarkovChain$new()


MarkovChain$make_mat()

Make model matrices

Usage
MarkovChain$make_mat(data, new_data = NULL)
Arguments
data

Data frame containing all needed covariates

new_data

Optional new data set, including covariates for which the design matrices should be created. This needs to be passed in addition to the argument 'data', for cases where smooth terms or factor covariates are included, and the original data set is needed to determine the full range of covariate values.

Returns

A list with elements:

X_fe

Design matrix for fixed effects

X_re

Design matrix for random effects

S

Smoothness matrix for random effects

ncol_fe

Number of columns of X_fe for each parameter

ncol_re

Number of columns of X_re and S for each random effect


MarkovChain$make_mat_grid()

Design matrices for grid of covariates

Used in plotting functions such as HMM$plot_tpm and HMM$plot_stat_dist

Usage
MarkovChain$make_mat_grid(var, data, covs = NULL, n_grid = 1000)
Arguments
var

Name of variable

data

Data frame containing the covariates

covs

Optional named list for values of covariates (other than 'var') that should be used in the plot (or dataframe with single row). If this is not specified, the mean value is used for numeric variables, and the first level for factor variables.

n_grid

Grid size (number of points). Default: 1000.

Returns

A list with the same elements as the output of make_mat, plus a data frame of covariates values.


MarkovChain$tpm2par()

Transform transition probabilities to working scale

Apply the multinomial logit link function to get the corresponding parameters on the working scale (i.e., linear predictor scale).

Usage
MarkovChain$tpm2par(tpm)
Arguments
tpm

Transition probability matrix

Returns

Vector of parameters on linear predictor scale


MarkovChain$par2tpm()

Transform working parameters to transition probabilities

Apply the inverse multinomial logit link function to transform the parameters on the working scale (i.e., linear predictor scale) into the transition probabilities.

Usage
MarkovChain$par2tpm(par)
Arguments
par

Vector of parameters on working scale

Returns

Transition probability matrix


MarkovChain$linpred()

Linear predictor for transition probabilities

Usage
MarkovChain$linpred()

MarkovChain$simulate()

Simulate from Markov chain

Usage
MarkovChain$simulate(n, data = NULL, new_data = NULL, silent = FALSE)
Arguments
n

Number of time steps to simulate

data

Optional data frame containing all needed covariates

new_data

Optional new data set, including covariates for which the design matrices should be created. This needs to be passed in addition to the argument 'data', for cases where smooth terms or factor covariates are included, and the original data set is needed to determine the full range of covariate values.

silent

if TRUE then no messages are printed

Returns

Sequence of states of simulated chain


MarkovChain$formulation()

Print model formulation

Usage
MarkovChain$formulation()

MarkovChain$print()

Print MarkovChain object

Usage
MarkovChain$print()

MarkovChain$clone()

The objects of this class are cloneable with this method.

Usage
MarkovChain$clone(deep = FALSE)
Arguments
deep

Whether to make a deep clone.

Examples


## ------------------------------------------------
## Method `MarkovChain$new()`
## ------------------------------------------------

# Load data set from MSwM package
data(energy, package = "MSwM")

# Create 2-state covariate-free model and initialise transition 
# probability matrix
hid <- MarkovChain$new(data = energy, n_states = 2,
                       tpm = matrix(c(0.8, 0.3, 0.2, 0.7), 2, 2))

# Create 2-state model with non-linear effect of Oil on all transition 
# probabilities
hid <- MarkovChain$new(data = energy, n_states = 2,
                       formula = ~ s(Oil, k = 5, bs = "cs"))

# Create 2-state model with quadratic effect of Oil on Pr(1 > 2)
structure <- matrix(c(".", "~poly(Oil, 2)",
                      "~1", "."),
                    ncol = 2, byrow = TRUE)
hid <- MarkovChain$new(data = energy, n_states = 2,
                       formula = structure)

R6 class for HMM observation model

Description

Contains the data, distributions, parameters, and formulas for the observation model from a hidden Markov model.

Methods

Public methods


Observation$new()

Create new Observation object

Usage
Observation$new(
  data = NULL,
  dists,
  formulas = NULL,
  n_states = NULL,
  par,
  fixpar = NULL,
  gam_args = NULL
)
Arguments
data

Data frame containing response variables (named in dists and par) and covariates (named in formulas). Note that "state" is a reserved column name, used to pass known states to the model (semi- supervised learning).

dists

Named list of distribution names for each data stream, with the following options: beta, binom, cat, dir, exp, foldednorm, gamma, gamma2, lnorm, mvnorm, nbinom, norm, pois, t, truncnorm, tweedie, vm, weibull, wrpcauchy, zibinom, zigamma, zigamma2, zinbinom, zipois, zoibeta, ztnbinom, ztpois. See vignette about list of distributions for more details, e.g., list of parameters for each distribution.

formulas

List of formulas for observation parameters. This should be a nested list, where the outer list has one element for each observed variable, and the inner lists have one element for each parameter. Any parameter that is not included is assumed to have the formula ~1. By default, all parameters have the formula ~1 (i.e., no covariate effects).

n_states

Number of states (optional). If not provided, the number of states is derived from the length of entries of par.

par

List of initial observation parameters. This should be a nested list, where the outer list has one element for each observed variable, and the inner lists have one element for each parameter. The choice of good initial values can be important, especially for complex models; the package vignettes discuss approaches to selecting them (e.g., see Observation$suggest_initial()).

fixpar

List with optional elements "obs" (fixed coefficients for observation parameters), and "lambda_obs" (fixed smoothness parameters), Each element is a named vector of coefficients that should either be fixed (if the corresponding element is set to NA) or estimated to a common value (using integers or factor levels).

gam_args

Named list of arguments passed to mgcv::gam() in Observation$make_mat(), e.g., "knots". Use at your own risk.

Returns

A new Observation object

Examples
# Load data set from MSwM package
data(energy, package = "MSwM")

# Initial observation parameters
par0 <- list(Price = list(mean = c(3, 6), sd = c(2, 2)))

# Model "energy" with normal distributions
obs <- Observation$new(data = energy, 
                       dists = list(Price = "norm"),
                       par = par0)
                       
# Model "energy" with gamma distributions
obs <- Observation$new(data = energy, 
                       dists = list(Price = "gamma2"),
                       par = par0)
                       
# Model with non-linear effect of EurDol on mean price
f <- list(Price = list(mean = ~ s(EurDol, k = 5, bs = "cs")))
obs <- Observation$new(data = energy, 
                       dists = list(Price = "norm"),
                       par = par0, 
                       formula = f)

Observation$data()

Data frame

Usage
Observation$data()

Observation$dists()

List of distributions

Usage
Observation$dists()

Observation$nstates()

Number of states

Usage
Observation$nstates()

Observation$par()

Parameters on natural scale

Usage
Observation$par(t = 1, full_names = TRUE, linpred = NULL, as_list = FALSE)
Arguments
t

Time index or vector of time indices; default t = 1. If t = "all", then return observation parameters for all time points.

full_names

Logical. If TRUE, the rows of the output are named in the format "variable.parameter" (default). If FALSE, the rows are names in the format "parameter". The latter is used in various internal functions, when the parameters need to be passed on to an R function.

linpred

Optional custom linear predictor.

as_list

Logical. If TRUE, the output is a nested list with three levels: (1) time step, (2) observed variable, (3) observation parameter. If FALSE (default), the output is an array with one row for each observation parameter, one column for each state, and one slice for each time step.

Returns

Array of parameters with one row for each observation parameter, one column for each state, and one slice for each time step. (See as_list argument for alternative output format.)

Examples
# Load data set from MSwM package
data(energy, package = "MSwM")

# Initial observation parameters
par0 <- list(Price = list(mean = c(3, 6), sd = c(2, 2)))

# Model with linear effect of EurDol on mean price
f <- list(Price = list(mean = ~ EurDol))
obs <- Observation$new(data = energy, 
                       dists = list(Price = "norm"),
                       par = par0,
                       n_states = 2, 
                       formula = f)

# Set slope coefficients
obs$update_coeff_fe(coeff_fe = c(3, 2, 6, -2, log(2), log(2)))

# Observation parameter values for given data rows
obs$par(t = c(1, 10, 20))

Observation$par_alt()

Alternative parameter output

This function is only useful for the categorical and multivariate normal distributions, and it formats the parameters in a slightly nicer way.

Usage
Observation$par_alt(var = NULL, t = 1)
Arguments
var

Name of observation variable for which parameters are required. By default, the first variable in 'dists' is used.

t

Time index for covariate values. Only one value should be provided.

Returns

List of distribution parameters, with one element for each state


Observation$inipar()

Return initial parameter values supplied

Usage
Observation$inipar()

Observation$coeff_fe()

Fixed effect parameters on working scale

Usage
Observation$coeff_fe()

Observation$coeff_re()

Random effect parameters

Usage
Observation$coeff_re()

Observation$X_fe()

Fixed effect design matrix

Usage
Observation$X_fe()

Observation$X_re()

Random effect design matrix

Usage
Observation$X_re()

Observation$lambda()

Smoothness parameters

Usage
Observation$lambda()

Observation$sd_re()

Standard deviation of smooth terms

This function transforms the smoothness parameter of each smooth term into a standard deviation, given by SD = 1/sqrt(lambda). It is particularly helpful to get the standard deviations of independent normal random effects. A smooth with its own parameterisation rather than a single smoothness parameter – a Gaussian field, whose parameters are already a marginal standard deviation and a range – has no such transformation and returns NA; read those off lambda() directly.

Usage
Observation$sd_re()

Observation$formulas()

List of model formulas for observation model

Usage
Observation$formulas(raw = FALSE)
Arguments
raw

Logical. If FALSE, returns the nested list created by make_formulas (default). If TRUE, returns formulas passed as input.


Observation$terms()

Terms of model formulas

Usage
Observation$terms()

Observation$obs_var()

Data frame of response variables

Usage
Observation$obs_var(expand = FALSE)
Arguments
expand

If TRUE, then multivariate variables in observations are expanded to be univariate, creating extra columns.

Returns

Data frame of observation variables


Observation$known_states()

Vector of known states

Usage
Observation$known_states(mat = TRUE)
Arguments
mat

Logical.


Observation$fixpar()

Fixed parameters

Usage
Observation$fixpar(all = FALSE)
Arguments
all

Logical. If FALSE, only user-specified fixed parameters are returned, but not parameters that are fixed for some other reason (e.g., size of binomial distribution)


Observation$empty()

Empty model? (for simulation only)

Usage
Observation$empty()

Observation$gam_args()

Extra arguments for mgcv::gam (passed to make_matrices)

Usage
Observation$gam_args()

Observation$update_par()

Update parameters

Updates the 'par' attribute to the list passed as input, and updates the intercept elements of 'coeff_fe' using the list passed as input

Usage
Observation$update_par(par)
Arguments
par

New list of parameters


Observation$update_coeff_fe()

Update coefficients for fixed effect parameters

Usage
Observation$update_coeff_fe(coeff_fe)
Arguments
coeff_fe

New vector of coefficients for fixed effect parameters


Observation$update_coeff_re()

Update random effect parameters

Usage
Observation$update_coeff_re(coeff_re)
Arguments
coeff_re

New vector of coefficients for random effect parameters


Observation$update_X_fe()

Update fixed effect design matrix

Usage
Observation$update_X_fe(X_fe)
Arguments
X_fe

New fixed effect design matrix


Observation$update_X_re()

Update random effect design matrix

Usage
Observation$update_X_re(X_re)
Arguments
X_re

New random effect design matrix


Observation$update_lambda()

Update smoothness parameters

Usage
Observation$update_lambda(lambda)
Arguments
lambda

New smoothness parameter vector


Observation$update_data()

Update data

Usage
Observation$update_data(data)
Arguments
data

New data frame


Observation$update_fixpar()

Update information about fixed parameters

Usage
Observation$update_fixpar(fixpar)
Arguments
fixpar

New list of fixed parameters, in the same format expected by Observation$new()


Observation$make_mat()

Make model matrices

Usage
Observation$make_mat(new_data = NULL)
Arguments
new_data

Optional new data set, including covariates for which the design matrices should be created. If this argument is not specified, the design matrices are based on the original data frame.

Returns

A list with elements:

X_fe

Design matrix for fixed effects

X_re

Design matrix for random effects

S

Smoothness matrix for random effects

ncol_fe

Number of columns of X_fe for each parameter

ncol_re

Number of columns of X_re and S for each random effect


Observation$make_newdata_grid()

Design matrices for grid of covariates

Usage
Observation$make_newdata_grid(var, covs = NULL, n_grid = 1000)
Arguments
var

Name of variable

covs

Optional named list for values of covariates (other than 'var') that should be used in the plot (or dataframe with single row). If this is not specified, the mean value is used for numeric variables, and the first level for factor variables.

n_grid

Grid size (number of points). Default: 1000.

Returns

A list with the same elements as the output of make_mat, plus a data frame of covariates values.


Observation$n2w()

Natural to working parameter transformation

This function applies the link functions of the distribution parameters, to transform parameters from their natural scale to the working scale (i.e., linear predictor scale)

Usage
Observation$n2w(par)
Arguments
par

List of parameters on natural scale

Returns

Vector of parameters on working scale


Observation$w2n()

Working to natural parameter transformation

This function applies the inverse link functions of the distribution parameters, to transform parameters from the working scale (i.e., linear predictor scale) to their natural scale.

Usage
Observation$w2n(wpar)
Arguments
wpar

Vector of parameters on working scale

Returns

List of parameters on natural scale


Observation$linpred()

Compute linear predictor

Usage
Observation$linpred()

Observation$obs_probs()

Observation likelihoods

Usage
Observation$obs_probs(data = NULL)
Arguments
data

Optional dataframe to include in form of obs_var() output

Returns

Matrix of likelihoods of observations, with one row for each time step, and one column for each state.


Observation$cdf()

Cumulative probabilities of observations

Usage
Observation$cdf()
Returns

List of cumulative probabilities, with one element for each observed variable. Matrix rows correspond to time steps, and columns correspond to states.


Observation$suggest_initial()

Suggest initial observation parameters

The K-means algorithm is used to define clusters of observations (supposed to approximate the HMM states). Then, for each cluster, the parapprox function of the relevant Dist object is used to obtain parameter values.

Usage
Observation$suggest_initial()
Returns

List of initial parameters for each observation variable

Examples
# Load data set from MSwM package
data(energy, package = "MSwM")

# Initial observation parameters
par0 <- list(Price = list(mean = c(3, 6), sd = c(2, 2)))

# Model "energy" with normal distributions
obs <- Observation$new(data = energy, 
                       dists = list(Price = "norm"),
                       par = par0,
                       n_states = 2)

# Print observation parameters
obs$par()

# Suggest initial parameters
par0_new <- obs$suggest_initial()
par0_new

# Update model parameters to suggested
obs$update_par(par = par0_new)
obs$par()

Observation$plot_dist()

Plot histogram of data and pdfs

Plot histogram of observations for the variable specified by the argument name, overlaid with the pdf of the specified distribution for that data stream. Helpful to select initial parameter values for model fitting, or to visualise fitted state-dependent distributions.

Usage
Observation$plot_dist(var = NULL, weights = NULL, t = 1)
Arguments
var

Name of response variable for which the histogram and pdfs should be plotted.

weights

Optional vector of length the number of pdfs that are plotted. Useful to visualise a mixture of distributions weighted by the proportion of time spent in the different states.

t

Index of time step to use for covariates (default: 1).

Returns

A ggplot object


Observation$formulation()

Print model formulation

Usage
Observation$formulation()

Observation$print()

Print Observation object Check constructor arguments

Usage
Observation$print()

Observation$clone()

The objects of this class are cloneable with this method.

Usage
Observation$clone(deep = FALSE)
Arguments
deep

Whether to make a deep clone.

Examples


## ------------------------------------------------
## Method `Observation$new()`
## ------------------------------------------------

# Load data set from MSwM package
data(energy, package = "MSwM")

# Initial observation parameters
par0 <- list(Price = list(mean = c(3, 6), sd = c(2, 2)))

# Model "energy" with normal distributions
obs <- Observation$new(data = energy, 
                       dists = list(Price = "norm"),
                       par = par0)
                       
# Model "energy" with gamma distributions
obs <- Observation$new(data = energy, 
                       dists = list(Price = "gamma2"),
                       par = par0)
                       
# Model with non-linear effect of EurDol on mean price
f <- list(Price = list(mean = ~ s(EurDol, k = 5, bs = "cs")))
obs <- Observation$new(data = energy, 
                       dists = list(Price = "norm"),
                       par = par0, 
                       formula = f)

## ------------------------------------------------
## Method `Observation$par()`
## ------------------------------------------------

# Load data set from MSwM package
data(energy, package = "MSwM")

# Initial observation parameters
par0 <- list(Price = list(mean = c(3, 6), sd = c(2, 2)))

# Model with linear effect of EurDol on mean price
f <- list(Price = list(mean = ~ EurDol))
obs <- Observation$new(data = energy, 
                       dists = list(Price = "norm"),
                       par = par0,
                       n_states = 2, 
                       formula = f)

# Set slope coefficients
obs$update_coeff_fe(coeff_fe = c(3, 2, 6, -2, log(2), log(2)))

# Observation parameter values for given data rows
obs$par(t = c(1, 10, 20))

## ------------------------------------------------
## Method `Observation$suggest_initial()`
## ------------------------------------------------

# Load data set from MSwM package
data(energy, package = "MSwM")

# Initial observation parameters
par0 <- list(Price = list(mean = c(3, 6), sd = c(2, 2)))

# Model "energy" with normal distributions
obs <- Observation$new(data = energy, 
                       dists = list(Price = "norm"),
                       par = par0,
                       n_states = 2)

# Print observation parameters
obs$par()

# Suggest initial parameters
par0_new <- obs$suggest_initial()
par0_new

# Update model parameters to suggested
obs$update_par(par = par0_new)
obs$par()

Read formula with as.character without splitting

Description

Read formula with as.character without splitting

Usage

as_character_formula(x, ...)

Arguments

x

R formula

...

Unused

Details

Citation: this function was taken from the R package formula.tools: Christopher Brown (2018). formula.tools: Programmatic Utilities for Manipulating Formulas, Expressions, Calls, Assignments and Other R Objects. R package version 1.7.1. https://CRAN.R-project.org/package=formula.tools


Transforms matrix to dgTMatrix

Description

Transforms matrix to dgTMatrix

Usage

as_sparse(x)

Arguments

x

Matrix or vector. If this is a vector, it is formatted into a single-column matrix.

Value

Sparse matrix of class dgTMatrix


Create block diagonal matrix (safe version)

Description

This version of bdiag checks whether the matrices passed as arguments are NULL. This avoids errors that would arise if using bdiag directly.

Usage

bdiag_check(...)

Arguments

...

Matrix or list of matrices (only the first argument is used)

Value

Block diagonal matrix


Check values in vector are contiguous

Description

Check values in vector are contiguous

Usage

check_contiguous(x)

Arguments

x

Vector of values (can be numeric, character, factor)

Value

Logical: are values contiguous?


Check that only supported smooths are used

Description

Currently, this raises an error message if tensor product smooths are used (te, ti, t2).

Usage

check_smooths(form)

Arguments

form

Model formula


Grid of covariates

Description

Grid of covariates

Usage

cov_grid(var, data = NULL, obj = NULL, covs = NULL, formulas, n_grid = 1000)

Arguments

var

Name of variable

data

Data frame containing the covariates. If not provided, data are extracted from obj

obj

HMM model object containing data and formulas

covs

Optional named list for values of covariates (other than 'var') that should be used in the plot (or dataframe with single row). If this is not specified, the mean value is used for numeric variables, and the first level for factor variables.

formulas

List of formulas used in the model

n_grid

Grid size (number of points). Default: 1000.

Value

Data frame of covariates, with 'var' defined over a grid, and other covariates fixed to their mean (numeric) or first level (factor).


Grid of covariate values over two covariates

Description

The two-dimensional counterpart of cov_grid, used by HMM$plot_2d(). Both var and var2 are varied over a regular n_grid by n_grid lattice spanning their ranges in the data, and every other covariate is held at one value, as in cov_grid: the one given in covs, otherwise the mean of a numeric covariate or the first level of a factor.

Usage

cov_grid_2d(
  var,
  var2,
  data = NULL,
  obj = NULL,
  covs = NULL,
  formulas,
  n_grid = 40,
  padding = 0
)

Arguments

var

Name of the first covariate, on the x axis

var2

Name of the second covariate, on the y axis

data

Data frame of covariate values

obj

HMM model object, used to find the covariates if data is not given

covs

Optional named list of values for the other covariates

formulas

List of model formulas

n_grid

Number of points along each axis, so the grid has n_grid^2 rows

padding

Numeric vector of length 1 or 2 giving the amount to pad the 'var' and 'var2' ranges beyond the data. A single value is recycled to both axes, and a length-2 vector is interpreted as (padding in var, padding in var2). Defaults to 0.

Details

The lattice is regular because that is what ggplot2::geom_raster() needs, and var varies fastest, so that the result can be reshaped into a matrix column by column.

Value

Data frame with n_grid^2 rows and one column for each covariate


Covariate names that are columns of the data

Description

all.vars() on a model formula returns every symbol in it, including objects a smooth refers to through its xt argument – the mesh of an SPDE field, say – which are not covariates and are not columns of the data. Those have to be dropped before the data are indexed by name.

Usage

cov_names_in_data(var_names, data)

Arguments

var_names

Character vector of names found in the formulas

data

Data frame

Details

A covariate that is genuinely missing from the data is dropped here too, rather than raising an error. mgcv::gam() reports it when the design matrices are built, which is a better place to say so.

Value

The subset of var_names naming columns of data


Density function of von Mises distribution

Description

Density function of von Mises distribution

Usage

dvm(x, mu, kappa, log = FALSE)

Arguments

x

Angle

mu

Mean parameter

kappa

Concentration parameter

log

Should log-density be returned?

Value

Von Mises density


Density function of wrapped Cauchy distribution

Description

Density function of wrapped Cauchy distribution

Usage

dwrpcauchy(x, mu, rho, log = FALSE)

Arguments

x

Angle

mu

Mean parameter

rho

Concentration parameter

log

Should log-density be returned?

Value

Wrapped Cauchy density


Find s(, bs = "re") terms in formula

Description

This function is used to identify the variables "x" which are included as s(x, bs = "re") in the formula, in particular to check that they are factors.

Usage

find_re(form)

Arguments

form

Model formula

Value

Vector of names of variables for which a random effect term is included in the model.


Shell gam object for building prediction matrices

Description

mgcv::predict.gam() with type = "lpmatrix" uses only the model frame, the terms objects, the factor levels and contrasts, and the smooth objects – all of which mgcv::gam(fit = FALSE) already produces. This wraps that unfitted setup in something predict.gam() accepts, so that a prediction matrix can be built without fitting anything.

Usage

gam_shell(G)

Arguments

G

Output of mgcv::gam() called with fit = FALSE

Details

The coefficients are set to zero. predict.gam() requires the slot to exist and to have the right length, but for type = "lpmatrix" it returns the design matrix itself and never multiplies by them.

Value

An object of class "gam", only usable for predict(type = "lpmatrix")


Generalized matrix determinant

Description

Generalized determinant = product of non-zero eigenvalues (see e.g., Wood 2017). Used for (log)determinant of penalty matrices, required in log-likelihood function.

Usage

gdeterminant(x, eps = 1e-10, log = TRUE)

Arguments

x

Numeric matrix

eps

Threshold below which eigenvalues are ignored (default: 1e-10)

log

Logical: should the log-determinant be returned?

Value

Generalized determinant of input matrix


hmmTMB colour palette

Description

hmmTMB colour palette

Usage

hmmTMB_cols

Multivarite inverse logit function

Description

Multivarite inverse logit function

Usage

invmlogit(x)

Arguments

x

Numeric vector


Check if number of whole number

Description

Check if number of whole number

Usage

is_whole_number(x, tol = 1e-10)

Arguments

x

number to check or vector of numbers

tol

how far away from whole number is ok?

Value

TRUE if it is a whole number within tolerance


logLik function for SDE objects

Description

This function makes it possible to call generic R methods such as AIC and BIC on HMM objects. It is based on the number of degrees of freedom of the *conditional* AIC (rather than marginal AIC), i.e., including degrees of freedom from the smooth/random effect components of the model.

Usage

## S3 method for class 'HMM'
logLik(object, ...)

Arguments

object

HMM model object

...

For compatibility with S3 method

Value

Maximum log-likelihood value for the model, with attributes df (degrees of freedom) and nobs (number of observations)


Log of sum of exponentials

Description

Log of sum of exponentials

Usage

logsumexp(x)

Arguments

x

Numeric vector


Make covariance matrix from standard deviations and correlations

Description

Make covariance matrix from standard deviations and correlations

Usage

make_cov(sds, corr)

Arguments

sds

Vector of standard deviations

corr

Vector of correlations (must be of length m*(m-1)/2 if sds is of length m)

Value

An m by m covariance matrix


Process formulas and store in nested list

Description

Process formulas and store in nested list

Usage

make_formulas(input_forms, var_names, par_names, n_states)

Arguments

input_forms

Nested list of formulas, with two levels: observed variable, and parameter of the observation distribution. The formulas can contain state-specific terms, e.g. "~ state1(x1) + x2".

var_names

character vector name of each observation variable

par_names

list with element for each observation variable that contains character vector of name of each parameter in its distribution

n_states

Number of states

Details

Formulas for the observation parameters can be different for the different states, using special functions of the form "state1", "state2", etc. This method processes the list of formulas passed by the user to extract the state-specific formulas. Missing formulas are assumed to be intercept-only ~1.

Value

Nested list of formulas, with three levels: observed variable, parameter of the observation distribution, and state.

Examples

input_forms <- list(step = list(shape = ~ state1(x1) + x2,
                                scale = ~ x1),
                    count = list(lambda = ~ state1(x1) + state2(s(x2, bs = "cs"))))

make_formulas(input_forms = input_forms, 
              var_names = names(input_forms), 
              par_names = lapply(input_forms, names), 
              n_states = 2)
              

Create model matrices

Description

Create model matrices

Usage

make_matrices(formulas, data, new_data = NULL, gam_args = NULL)

Arguments

formulas

List of formulas (possibly nested, e.g. for use within Observation)

data

Data frame including covariates

new_data

Optional new data set, including covariates for which the design matrices should be created. This needs to be passed in addition to the argument 'data', for cases where smooth terms or factor covariates are included, and the original data set is needed to determine the full range of covariate values.

gam_args

Named list of additional arguments for mgcv::gam(), such as knots.

Details

Note the two indices: ncol_re, log_det_S and gmrf have one entry per penalty, while L, sp_names, sp_gmrf and theta_start have one per smoothing parameter. The two coincide for an ordinary smooth, which has one of each, but an SPDE field has three penalties and two parameters.

Value

A list of


Multivariate logit function

Description

Multivariate logit function

Usage

mlogit(x)

Arguments

x

Numeric vector


Description

Multivariate Normal inverse link function

Usage

mvnorm_invlink(x)

Arguments

x

Vector of parameters on linear predictor scale (in the order: means, SDs, correlations)


Description

Multivariate Normal link function

Usage

mvnorm_link(x)

Arguments

x

Vector of parameters on natural scale (in the order: means, SDs, correlations)


Fill in NAs

Description

Replace NA entries in a vector by the last non-NA value. If the first entry of the vector is NA, it is replaced by the first non-NA value. If the vector passed as input doesn't contain NAs, it is returned as is.

Usage

na_fill(x)

Arguments

x

Vector in which NAs should be removed

Value

Copy of x in which NAs have been replaced by nearest available value.


Get covariance matrix from precision matrix

Description

The covariance matrix is the inverse of the precision matrix. By default, the function solve is used for inversion. If it fails (e.g., singular system), then MASS::ginv is used instead, and returns the Moore-Penrose generalised inverse of the precision matrix.

Usage

prec_to_cov(prec_mat)

Arguments

prec_mat

Precision matrix (either of 'matrix' type or sparse matrix on which as.matrix can be used)

Value

Precision matrix


Solve for positive root of quadratic ax^2 + bx + c = 0 when it exists

Description

Solve for positive root of quadratic ax^2 + bx + c = 0 when it exists

Usage

quad_pos_solve(a, b, c)

Arguments

a

coefficient of x^2

b

coefficient of x

c

scalar coefficient

Value

real positive root if it exists


Sample from a multivariate normal given its precision matrix

Description

Draws from N(mu, Q^-1) through a sparse Cholesky factorisation of the precision, Q = P' L L' P, as x = mu + P' L^-T z with z standard normal. Nothing is inverted, and the Cholesky factor keeps the sparsity of Q, so the cost is that of the factorisation rather than of a dense inverse followed by a dense n-by-n Cholesky of it. A dense precision is simply a sparse matrix with no zeros, and costs no more this way than the old route did.

Usage

rmvn_prec(n, mu, prec_mat)

Arguments

n

Number of samples

mu

Mean vector

prec_mat

Precision matrix, sparse or dense

Details

If prec_mat is not positive definite – a fit that has not converged, or a singular Hessian – there is no Cholesky factor to be had, and this falls back on prec_to_cov, which uses a generalised inverse and warns.

Value

Matrix with one row for each sample and one column for each element of mu


Sample from von Mises distribution

Description

Sample from von Mises distribution

Usage

rvm(n, mu, kappa)

Arguments

n

Number of samples

mu

Mean parameter

kappa

Concentration parameter

Details

Uses basic rejection sampling, based on dvm(), which might be inefficient for large kappa. Could be improved following Best & Fisher (1979), Efficient simulation of the von Mises distribution, JRSSC, 28(2), 152-157.

Value

Vector of n samples from vm(mu, kappa)


Sample from wrapped Cauchy distribution

Description

Sample from wrapped Cauchy distribution

Usage

rwrpcauchy(n, mu, rho)

Arguments

n

Number of samples

mu

Mean parameter

rho

Concentration parameter

Details

Uses basic rejection sampling, based on dwrpcauchy(), which might be inefficient for large rho.

Value

Vector of n samples from wrpcauchy(mu, rho)


Matern SPDE smooth

Description

A smooth term for a spatially (or temporally) continuous Gaussian random field, usable as s(x, y, bs = "spde", xt = list(mesh = mesh)) in any hmmTMB formula, and so on any transition probability or any parameter of any observation distribution.

Usage

## S3 method for class 'spde.smooth.spec'
smooth.construct(object, data, knots)

## S3 method for class 'spde.smooth'
Predict.matrix(object, data)

Arguments

object, data, knots

As mgcv::smooth.construct(); for Predict.matrix, knots is absent and the rest are as mgcv::Predict.matrix().

Value

A smoothCon object of class spde.smooth, with sparse X and sparse penalties.

The mesh in one dimension

A one-dimensional field needs no mesh: s(x, bs = "spde") builds one by default, as k quadratic B-spline basis functions on evenly spaced knots, so

f <- ~ s(x, bs = "spde")          # and s(x, bs = "spde", k = 40) for a finer one

is the whole of it. The knots are spread over the range of the covariate widened by a fifth on each side, which is the one-dimensional version of the outer extension of a two-dimensional mesh: with the knots stopping at the data, the boundary condition inflates the field's variance at the two ends by a third or more.

k is a resolution, not a smoothing parameter, and this is the one place where a field does not behave like the smooths around it. The range is estimated and is what does the smoothing, so k is not a cap on wiggliness that the penalty then pulls back from: it only has to be large enough to resolve the range the data ask for, knots about a third of a range apart as in two dimensions. That is why the default is k = 15 rather than mgcv's 10 – with the widening, 15 knots put the knot spacing at about half the range the smoother starts from, which is a fifth of the spread of the covariate.

Too small a k does not simply oversmooth. Once the knots are further apart than the range the data want, the weights are near enough independent that the likelihood cannot tell one short range from another, and the range collapses towards zero while the standard deviation grows to compensate. The fitted curve can still look right when that happens, because the basis is then doing the smoothing on its own, but the two parameters are meaningless. So read lambda() before reading the curve: a range far below the knot spacing, or a standard deviation orders of magnitude above the scale of the linear predictor, means raise k and refit.

Passing your own fmesher::fm_mesh_1d() overrides all of this, and is worth doing when the covariate is unevenly spread and you want the knots placed accordingly.

Building a mesh in two dimensions

In two dimensions the mesh is yours to build and pass in, because a good one depends on the domain, the data and the range you expect. fmesher::fm_mesh_2d() takes locations, a maximum triangle edge length inside the domain and in the outer extension, and a cutoff below which nearby points are merged:

mesh <- fmesher::fm_mesh_2d(loc = cbind(data$x, data$y),
                            max.edge = c(0.1, 0.3),
                            cutoff = 0.05, offset = c(0.1, 0.3))
f <- ~ s(x, y, bs = "spde", xt = list(mesh = mesh))

A rule of thumb is max.edge no larger than a third of the range you expect, and an offset about equal to the range; without the outer extension the field's variance is inflated at the boundary.

The field is evaluated at every time step, so missing covariates are replaced by the last non-missing value as elsewhere in hmmTMB. If that is too crude for locations, interpolate them before fitting.

Parameterisation

The precision is

Q(\tau, \kappa) = \tau^2(\kappa^4 C + 2\kappa^2 G_1 + G_2)

with C, G_1, G_2 the finite element matrices from fmesher::fm_fem(). alpha = 2 throughout, so the Matern smoothness is \nu = 2 - d/2: \nu = 1 in two dimensions and \nu = 3/2 in one. The range is \rho = \sqrt{8\nu}/\kappa and the marginal variance is \sigma^2 = \Gamma(\nu) / (\Gamma(2)(4\pi)^{d/2}\kappa^{2\nu}\tau^2), which is 1/(\tau^2\kappa^2 4\pi) in two dimensions and 1/(4\tau^2\kappa^3) in one. Both constants depend on d, so the one- and two-dimensional smoothers do not share them.

The two estimated parameters are \log\sigma and \log\rho, not \log\tau and \log\kappa, and appear as sd and range in lambda(). The change is exact – a linear map of the log parameters, absorbed into the constants in front of the three matrices – and worth making: the parameters mean something on their own, and the likelihood's long ridge along constant marginal variance runs diagonally in (\tau, \kappa) but along an axis in (\sigma, \rho), which the optimiser finds much easier.

Both are estimated freely, with no prior. A single realisation identifies them only loosely, and a field whose range approaches the size of the domain is close to improper: the range then runs off and the standard deviation follows it, with the fitted surface barely changing. The fit is still usable if that happens, but the two parameters are not, and a finer mesh will not help – it is the data that are uninformative.

The field is proper for any positive \kappa, so no identifiability constraint is imposed, as in INLA. It is not centred, and its level is only weakly separated from the intercept when the range is large.

Bandwidth

A model containing this smooth is fitted with the banded forward algorithm, because the exact one makes the Hessian with respect to the field weights dense and so defeats the sparsity the SPDE representation exists to provide. See HMM$update_bw() and HMM$check_bw().

References

Lindgren, F., Rue, H. and Lindstrom, J. (2011). An explicit link between Gaussian fields and Gaussian Markov random fields. JRSS-B 73, 423-498.

Miller, D. L., Glennie, R., & Seaton, A. E. (2020). Understanding the stochastic partial differential equation approach to smoothing. Journal of Agricultural, Biological and Environmental Statistics, 25(1), 1-16.

Fischer, J.-O. (2026). Fast and scalable inference in hidden Markov models with Gaussian fields.

Examples

# A one-dimensional field over a covariate, with a default mesh
if(requireNamespace("fmesher", quietly = TRUE)) {
  d <- data.frame(x = runif(100))
  sm <- mgcv::smoothCon(mgcv::s(x, bs = "spde"), data = d)[[1]]
  c(k = ncol(sm$X), sm$theta.names)
}


A length scale for the meshed domain, for starting values

Description

The larger side of the bounding box of the mesh nodes that carry basis weight, which is the region the data occupy rather than the outer extension. A one-dimensional mesh stores its knots in 'loc' and the midpoints of its basis functions in 'mid', and only the latter are one per column of X, so 'mid' is the one to use where there is a choice.

Usage

spde_extent(mesh, X)

Arguments

mesh

An fmesher mesh

X

The smooth's design matrix

Value

A positive number


Observation locations for an SPDE smooth

Description

Observation locations for an SPDE smooth

Usage

spde_loc(term, data)

Arguments

term

Character vector of one or two covariate names

data

Data frame containing those covariates

Value

Numeric vector (1d) or two-column matrix (2d) of locations


Default mesh for a one-dimensional SPDE smooth

Description

k quadratic B-spline basis functions on evenly spaced knots, over the range of the covariate widened by a fifth on each side. The widening is the one-dimensional counterpart of the outer extension of a two-dimensional mesh: fmesher's default boundary condition is Neumann, under which a field whose knots stop at the data has its variance inflated by a third or more at the two ends. A fifth of the spread of the covariate is about one range at the starting value used in smooth.construct.spde.smooth.spec(), which is the same rule of thumb used for the offset in two dimensions.

Usage

spde_mesh_1d(x, k)

Arguments

x

The covariate

k

Basis dimension, as passed to s(); negative when the user gave none, in which case 15 is used

Details

A degree-2 mesh has one basis function fewer than it has knots, so k knots would not give k of them; k keeps its mgcv meaning of a basis dimension here, and k + 1 knots are laid down.

The default of 15 is above mgcv's 10, because k is a resolution here and not a cap on wiggliness: with the widening, 15 knots put the knot spacing at about half the range the smoother starts from, in the spirit of max.edge in two dimensions. Ten of them leave the knots further apart than that range, and it collapses towards zero as a result.

Value

An fm_mesh_1d with k basis functions


Strip comments marked with a hash from a character vector

Description

Strip comments marked with a hash from a character vector

Usage

strip_comments(str)

Arguments

str

the character vector

Value

character vector with comments removed (and lines with only comments completely removed)


Update a model to a new model by changing one formula

Description

Update a model to a new model by changing one formula

Usage

## S3 method for class 'HMM'
update(object, type, i, j, change, fit = TRUE, silent = FALSE, ...)

Arguments

object

HMM model object

type

Character string for the part of the model that is updated (either "hid" or "obs")

i

If type = "hid" then i is the row of the formula containing the change. If type = "obs" then i is the observation variable name.

j

If type = "hid" then j is the column of the formula containing the change. If type = "obs" then j is the parameter whose formula is to be changed.

change

The change to make to the formula, see ?update.formula for details.

fit

If FALSE then change is made but model is not re-fit.

silent

If TRUE then no model fitting output is given

...

Additional arguments are ignored (for compatibility with generic S3 method)

Examples

# Load data set from MSwM package
data(energy, package = "MSwM")

# Create hidden state and observation models
hid <- MarkovChain$new(data = energy, n_states = 2)
par0 <- list(Price = list(mean = c(3, 6), sd = c(2, 3)))
obs <- Observation$new(data = energy, n_states = 2,
                       dists = list(Price = "norm"),
                       par = par0)

# Create HMM (no covariate effects)
hmm <- HMM$new(hid = hid, obs = obs)
hmm$hid()$formula()
hmm$obs()$formulas()

# Update transition probability formulas (one at a time)
hmm <- update(hmm, type = "hid", i = 1, j = 2, 
              change = ~ . + Oil, fit = FALSE)
hmm <- update(hmm, type = "hid", i = 2, j = 1, 
              change = ~ . + Gas + Coal, fit = FALSE)
hmm$hid()$formula()

# Update observation parameter formulas (one at a time)
hmm <- update(hmm, type = "obs", i = "Price", j = "mean", 
              change = ~ . + EurDol, fit = FALSE)
hmm$obs()$formulas()