fitHMM | R Documentation |
Fit a (multivariate) hidden Markov model to the data provided, using numerical optimization of the log-likelihood function.
fitHMM(data, ...) ## S3 method for class 'momentuHMMData' fitHMM( data, nbStates, dist, Par0, beta0 = NULL, delta0 = NULL, estAngleMean = NULL, circularAngleMean = NULL, formula = ~1, formulaDelta = NULL, stationary = FALSE, mixtures = 1, formulaPi = NULL, nlmPar = list(), fit = TRUE, DM = NULL, userBounds = NULL, workBounds = NULL, betaCons = NULL, betaRef = NULL, deltaCons = NULL, mvnCoords = NULL, stateNames = NULL, knownStates = NULL, fixPar = NULL, retryFits = 0, retrySD = NULL, optMethod = "nlm", control = list(), prior = NULL, modelName = NULL, ... ) ## S3 method for class 'momentuHierHMMData' fitHMM( data, hierStates, hierDist, Par0, hierBeta = NULL, hierDelta = NULL, estAngleMean = NULL, circularAngleMean = NULL, hierFormula = NULL, hierFormulaDelta = NULL, mixtures = 1, formulaPi = NULL, nlmPar = list(), fit = TRUE, DM = NULL, userBounds = NULL, workBounds = NULL, betaCons = NULL, deltaCons = NULL, mvnCoords = NULL, knownStates = NULL, fixPar = NULL, retryFits = 0, retrySD = NULL, optMethod = "nlm", control = list(), prior = NULL, modelName = NULL, ... )
data |
A |
... |
further arguments passed to or from other methods |
nbStates |
Number of states of the HMM. |
dist |
A named list indicating the probability distributions of the data streams. Currently
supported distributions are 'bern', 'beta', 'cat', exp', 'gamma', 'lnorm', 'logis', 'negbinom', 'norm', 'mvnorm2' (bivariate normal distribution), 'mvnorm3' (trivariate normal distribution),
'pois', 'rw_norm' (normal random walk), 'rw_mvnorm2' (bivariate normal random walk), 'rw_mvnorm3' (trivariate normal random walk), 'vm', 'vmConsensus', 'weibull', and 'wrpcauchy'. For example,
|
Par0 |
A named list containing vectors of initial state-dependent probability distribution parameters for
each data stream specified in If |
beta0 |
Initial matrix of regression coefficients for the transition probabilities (more
information in 'Details').
Default: |
delta0 |
Initial value for the initial distribution of the HMM. Default: |
estAngleMean |
An optional named list indicating whether or not to estimate the angle mean for data streams with angular
distributions ('vm' and 'wrpcauchy'). For example, |
circularAngleMean |
An optional named list indicating whether to use circular-linear (FALSE) or circular-circular (TRUE)
regression on the mean of circular distributions ('vm' and 'wrpcauchy') for turning angles. For example,
Alternatively, |
formula |
Regression formula for the transition probability covariates. Default: |
formulaDelta |
Regression formula for the initial distribution. Default for |
stationary |
|
mixtures |
Number of mixtures for the state transition probabilities (i.e. discrete random effects *sensu* DeRuiter et al. 2017). Default: |
formulaPi |
Regression formula for the mixture distribution probabilities. Default: |
nlmPar |
List of parameters to pass to the optimization function |
fit |
|
DM |
An optional named list indicating the design matrices to be used for the probability distribution parameters of each data
stream. Each element of Design matrices specified using formulas allow standard functions in R formulas
(e.g., |
userBounds |
An optional named list of 2-column matrices specifying bounds on the natural (i.e, real) scale of the probability
distribution parameters for each data stream. For each matrix, the first column pertains to the lower bound and the second column the upper bound. For example, for a 2-state model using the wrapped Cauchy ('wrpcauchy') distribution for
a data stream named 'angle' with |
workBounds |
An optional named list of 2-column matrices specifying bounds on the working scale of the probability distribution, transition probability, and initial distribution parameters. For each matrix, the first column pertains to the lower bound and the second column the upper bound.
For data streams, each element of |
betaCons |
Matrix of the same dimension as |
betaRef |
Numeric vector of length |
deltaCons |
Matrix of the same dimension as |
mvnCoords |
Character string indicating the name of location data that are to be modeled using a multivariate normal distribution. For example, if |
stateNames |
Optional character vector of length nbStates indicating state names. |
knownStates |
Vector of values of the state process which are known prior to fitting the model (if any). Default: NULL (states are not known). This should be a vector with length the number of rows of 'data'; each element should either be an integer (the value of the known states) or NA if the state is not known. |
fixPar |
An optional list of vectors indicating parameters which are assumed known prior to fitting the model. Default: NULL
(no parameters are fixed). For data streams, each element of |
retryFits |
Non-negative integer indicating the number of times to attempt to iteratively fit the model using random perturbations of the current parameter estimates as the
initial values for likelihood optimization. Normal(0, |
retrySD |
An optional list of scalars or vectors indicating the standard deviation to use for normal perturbations of each working scale parameter when |
optMethod |
The optimization method to be used. Can be “nlm” (the default; see |
control |
A list of control parameters to be passed to |
prior |
A function that returns the log-density of the working scale parameter prior distribution(s). See 'Details'. |
modelName |
An optional character string providing a name for the fitted model. If provided, |
hierStates |
A hierarchical model structure |
hierDist |
A hierarchical data structure |
hierBeta |
A hierarchical data structure |
hierDelta |
A hierarchical data structure |
hierFormula |
A hierarchical formula structure for the transition probability covariates for each level of the hierarchy ('formula'). Default: |
hierFormulaDelta |
A hierarchical formula structure for the initial distribution covariates for each level of the hierarchy ('formulaDelta'). Default: |
By default the matrix beta0
of regression coefficients for the transition probabilities has
one row for the intercept, plus one row for each covariate, and one column for
each non-diagonal element of the transition probability matrix. For example, in a 3-state
HMM with 2 formula
covariates, the matrix beta
has three rows (intercept + two covariates)
and six columns (six non-diagonal elements in the 3x3 transition probability matrix -
filled in row-wise).
In a covariate-free model (default), beta0
has one row, for the intercept. While the diagonal elements are by default the reference elements, other elements can serve as the reference
using the betaRef
argument. For example, in a 3-state model, setting betaRef=c(3,2,3)
changes the reference elements to state transition 1 -> 3 for state 1 (instead of 1 -> 1), state
transition 2 -> 2 for state 2 (same as default), and state transition 3 -> 3 for state 3 (same as default).
When covariates are not included in formulaDelta
(i.e. formulaDelta=NULL
), then delta0
(and fixPar$delta
) are specified as a vector of length nbStates
that
sums to 1. When any formula is specified for formulaDelta
(e.g. formulaDelta=~1
, formulaDelta=~cov1
), then delta0
(and fixPar$delta
) must be specified
as a k x (nbStates
-1) matrix of working parameters, where k is the number of regression coefficients and the columns correspond to states 2:nbStates
. For example, in a 3-state
HMM with formulaDelta=~cov1+cov2
, the matrix delta0
has three rows (intercept + two covariates)
and 2 columns (corresponding to states 2 and 3). The initial distribution working parameters are transformed to the real scale as exp(covsDelta*Delta)/rowSums(exp(covsDelta*Delta))
, where covsDelta
is the N x k design matrix, Delta=cbind(rep(0,k),delta0)
is a k x nbStates
matrix of working parameters,
and N=length(unique(data$ID))
.
The choice of initial parameters (particularly Par0
and beta0
) is crucial to fit a model. The algorithm might not find
the global optimum of the likelihood function if the initial parameters are poorly chosen.
If DM
is specified for a particular data stream, then the initial values are specified on
the working (i.e., beta) scale of the parameters. The working scale of each parameter is determined by the link function used.
If a parameter P is bound by (0,Inf) then the working scale is the log(P) scale. If the parameter bounds are (-pi,pi) then the working
scale is tan(P/2) unless circular-circular regression is used. Otherwise if the parameter bounds are finite then logit(P) is the working scale. However, when both
zero- and one-inflation are included, then a multinomial logit link is used because the sum of the zeromass and onemass probability parameters cannot exceed 1.
The function getParDM
is intended to help with obtaining initial values on the working scale when specifying a design matrix and other
parameter constraints (see example below). When circular-circular regression is specified using circularAngleMean
, the working scale
for the mean turning angle is not as easily interpretable, but the
link function is atan2(sin(X)*B,1+cos(X)*B), where X are the angle covariates and B the angle coefficients (see Duchesne et al. 2015).
Under this formulation, the reference turning angle is 0 (i.e., movement in the same direction as the previous time step).
In other words, the mean turning angle is zero when the coefficient(s) B=0.
Circular-circular regression in momentuHMM
is designed for turning angles (not bearings) as computed by simData
and prepData
.
Any circular-circular regression angle covariates for time step t should therefore be relative to the previous
direction of movement for time step t-1. In other words, circular-circular regression covariates for time step t should be the turning angle
between the direction of movement for time step t-1 and the standard direction of the covariate relative to the x-axis for time step t. If provided standard directions in radians relative to the x-axis
(where 0 = east, pi/2 = north, pi = west, and -pi/2 = south), circAngles
or prepData
can perform this calculation for you.
When the circular-circular regression model is used, the special function angleFormula(cov,strength,by)
can be used in DM
for the mean of angular distributions (i.e. 'vm', 'vmConsensus', and 'wrpcauchy'),
where cov
is an angle covariate (e.g. wind direction), strength
is an optional positive real covariate (e.g. wind speed), and by
is an optional factor variable for individual- or group-level effects (e.g. ID, sex). The strength
argument allows angle covariates to be weighted based on their relative strength or importance at time step t as in
Rivest et al. (2016). In this case, the link function for the mean angle is atan2((Z * sin(X)) %*% B,1+(Z * cos(X)) %*% B), where X are the angle covariates, Z the strength covariates, and B the angle coefficients (see Rivest et al. 2016).
State-specific formulas can be specified in DM
using special formula functions. These special functions can take
the names paste0("state",1:nbStates)
(where the integer indicates the state-specific formula). For example,
DM=list(step=list(mean=~cov1+state1(cov2),sd=~cov2+state2(cov1)))
includes cov1
on the mean parameter for all states, cov2
on the mean parameter for state 1, cov2
on the sd parameter for all states, and cov1
on the sd parameter for state 2.
State- and parameter-specific formulas can be specified for transition probabilities in formula
using special formula functions.
These special functions can take the names paste0("state",1:nbStates)
(where the integer indicates the current state from which transitions occur),
paste0("toState",1:nbStates)
(where the integer indicates the state to which transitions occur),
or paste0("betaCol",nbStates*(nbStates-1))
(where the integer indicates the column of the beta
matrix). For example with nbStates=3
,
formula=~cov1+betaCol1(cov2)+state3(cov3)+toState1(cov4)
includes cov1
on all transition probability parameters, cov2
on the beta
column corresponding
to the transition from state 1->2, cov3
on transition probabilities from state 3 (i.e., beta
columns corresponding to state transitions 3->1 and 3->2),
and cov4
on transition probabilities to state 1 (i.e., beta
columns corresponding to state transitions 2->1 and 3->1).
betaCons
can be used to impose equality constraints among the t.p.m. parameters. It must be a matrix of the same dimension as beta0
and be composed of integers, where each beta parameter is sequentially indexed in a column-wise fashion (see checkPar0
). Parameter indices in betaCons
must therefore be integers between 1
and nbStates*(nbStates-1)
.
Use of betaCons
is perhaps best demonstrated by example. If no constraints are imposed (the default), then betaCons=matrix(1:length(beta0),nrow(beta0),ncol(beta0))
such that
each beta parameter is (column-wise) sequentially identified by a unique integer. Suppose we wish to fit a model with nbStates=3
states and a covariate (‘cov1’) on the t.p.m. With no constraints on the t.p.m., we would have
betaCons=matrix(1:(2*(nbStates*(nbStates-1))),nrow=2,ncol=nbStates*(nbStates-1),dimnames=list(c("(Intercept)","cov1"),c("1 -> 2","1 -> 3","2 -> 1","2 -> 3","3 -> 1","3 -> 2")))
. If we then wanted to constrain the t.p.m. such that the covariate effect is identical for transitions from state 1 to states 2 and 3 (and vice versa), we have
betaCons=matrix(c(1,2,3,2,5,6,7,8,9,6,11,12),nrow=2,ncol=nbStates*(nbStates-1),dimnames=list(c("(Intercept)","cov1"),c("1 -> 2","1 -> 3","2 -> 1","2 -> 3","3 -> 1","3 -> 2")))
; this results in 10 estimated beta parameters (instead of 12), the “cov1” effects indexed by a “2” (“1 -> 2” and “1 -> 3”) constrained to be equal, and
the “cov1” effects indexed by a “6” (“2 -> 1” and “3 -> 1”) constrained to be equal.
Now suppose we instead wish to constrain these sets of state transition probabilities to be equal, i.e., Pr(1 -> 2) = Pr(1 -> 3) and Pr(2 -> 1) = Pr(3 -> 1); then we have betaCons=matrix(c(1,2,1,2,5,6,7,8,5,6,11,12),nrow=2,ncol=nbStates*(nbStates-1),dimnames=list(c("(Intercept)","cov1"),c("1 -> 2","1 -> 3","2 -> 1","2 -> 3","3 -> 1","3 -> 2")))
Cyclical relationships (e.g., hourly, monthly) may be modeled in DM
or formula
using the cosinor(x,period)
special formula function for covariate x
and sine curve period of time length period
. For example, if
the data are hourly, a 24-hour cycle can be modeled using ~cosinor(cov1,24)
, where the covariate cov1
is a repeating sequential series
of integers indicating the hour of day (0,1,...,23,0,1,...,23,0,1,...
) (note that fitHMM
will not do this for you, the appropriate covariate must be included in data
; see example below).
The cosinor(x,period)
function converts x
to 2 covariates cosinorCos(x)=cos(2*pi*x/period)
and cosinorSin(x)=sin(2*pi*x/period
for inclusion in the model (i.e., 2 additional parameters per state). The amplitude of the sine wave
is thus sqrt(B_cos^2 + B_sin^2)
, where B_cos
and B_sin
are the working parameters correponding to cosinorCos(x)
and cosinorSin(x)
, respectively (e.g., see Cornelissen 2014).
Similar to that used in crawlWrap
, the prior
argument is a user-specified function that returns the log-density of the working scale parameter prior distribution(s). In addition to including prior information about parameters, one area where priors can be particularly useful is for handling numerical issues that can arise when parameters are near a boundary.
When parameters are near boundaries, they can wander into the “nether regions” of the parameter space during optimization. For example, setting prior=function(par) {sum(dnorm(par,0,sd,log=TRUE))}
with a reasonably large sd
(e.g. 100 or 1000) can help prevent working parameters
from straying too far along the real line. Here par
is the vector of working scale parameters (as returned by fitHMM
, e.g., see example$m$mod$estimate
) in the following order: data stream working parameters (in order names(dist)
), beta working parameters, and delta working parameters. Instead of specifying the same prior on all parameters, different priors could be specified on different parameters (and not all parameters must have user-specified priors). For example,
prior=function(par){dnorm(par[3],0,100,log=TRUE)}
would only specify a prior for the third working parameter. Note that the prior
function must return a scalar on the log scale. See 'harbourSealExample.R' in the “vignettes” source directory for an example using the prior
argument.
fitHMM.momentuHierHMMData
is very similar to fitHMM.momentuHMMData
except that instead of simply specifying the number of states (nbStates
), distributions (dist
), and a single t.p.m. formula (formula
), the hierStates
argument specifies the hierarchical nature of the states,
the hierDist
argument specifies the hierarchical nature of the data streams, and the hierFormula
argument specifies a t.p.m. formula for each level of the hierarchy. All are specified as
Node
objects from the data.tree
package.
A momentuHMM
or momentuHierHMM
object, i.e. a list of:
mle |
A named list of the maximum likelihood estimates of the parameters of the model (if the numerical algorithm
has indeed identified the global maximum of the likelihood function). Elements are included for the parameters of each
data strea, as well as |
CIreal |
Standard errors and 95% confidence intervals on the real (i.e., natural) scale of parameters |
CIbeta |
Standard errors and 95% confidence intervals on the beta (i.e., working) scale of parameters |
data |
The momentuHMMData or momentuHierHMMData object |
mod |
List object returned by the numerical optimizer |
conditions |
Conditions used to fit the model, e.g., |
rawCovs |
Raw covariate values for transition probabilities, as found in the data (if any). Used in |
stateNames |
The names of the states. |
knownStates |
Vector of values of the state process which are known. |
covsDelta |
Design matrix for initial distribution. |
Cornelissen, G. 2014. Cosinor-based rhythmometry. Theoretical Biology and Medical Modelling 11:16.
Duchesne, T., Fortin, D., Rivest L-P. 2015. Equivalence between step selection functions and biased correlated random walks for statistical inference on animal movement. PLoS ONE 10 (4): e0122947.
Langrock R., King R., Matthiopoulos J., Thomas L., Fortin D., Morales J.M. 2012. Flexible and practical modeling of animal telemetry data: hidden Markov models and extensions. Ecology, 93 (11), 2336-2342.
Leos-Barajas, V., Gangloff, E.J., Adam, T., Langrock, R., van Beest, F.M., Nabe-Nielsen, J. and Morales, J.M. 2017. Multi-scale modeling of animal movement and general behavior data using hidden Markov models with hierarchical structures. Journal of Agricultural, Biological and Environmental Statistics, 22 (3), 232-248.
Maruotti, A., and T. Ryden. 2009. A semiparametric approach to hidden Markov models under longitudinal observations. Statistics and Computing 19: 381-393.
McClintock B.T., King R., Thomas L., Matthiopoulos J., McConnell B.J., Morales J.M. 2012. A general discrete-time modeling framework for animal movement using multistate random walks. Ecological Monographs, 82 (3), 335-349.
McClintock B.T., Russell D.J., Matthiopoulos J., King R. 2013. Combining individual animal movement and ancillary biotelemetry data to investigate population-level activity budgets. Ecology, 94 (4), 838-849.
Patterson T.A., Basson M., Bravington M.V., Gunn J.S. 2009. Classifying movement behaviour in relation to environmental conditions using hidden Markov models. Journal of Animal Ecology, 78 (6), 1113-1123.
Rivest, LP, Duchesne, T, Nicosia, A, Fortin, D, 2016. A general angular regression model for the analysis of data on animal movement in ecology. Journal of the Royal Statistical Society: Series C (Applied Statistics), 65(3):445-463.
getParDM
, prepData
, simData
simHierData
nbStates <- 2 stepDist <- "gamma" # step distribution angleDist <- "vm" # turning angle distribution # extract data from momentuHMM example data <- example$m$data ### 1. fit the model to the simulated data # define initial values for the parameters mu0 <- c(20,70) sigma0 <- c(10,30) kappa0 <- c(1,1) stepPar <- c(mu0,sigma0) # no zero-inflation, so no zero-mass included anglePar <- kappa0 # not estimating angle mean, so not included formula <- ~cov1+cos(cov2) m <- fitHMM(data=data,nbStates=nbStates,dist=list(step=stepDist,angle=angleDist), Par0=list(step=stepPar,angle=anglePar),formula=formula) print(m) ## Not run: ### 2. fit the exact same model to the simulated data using DM formulas # Get initial values for the parameters on working scale Par0 <- getParDM(data=data,nbStates=nbStates,dist=list(step=stepDist,angle=angleDist), Par=list(step=stepPar,angle=anglePar), DM=list(step=list(mean=~1,sd=~1),angle=list(concentration=~1))) mDMf <- fitHMM(data=data,nbStates=nbStates,dist=list(step=stepDist,angle=angleDist), Par0=Par0,formula=formula, DM=list(step=list(mean=~1,sd=~1),angle=list(concentration=~1))) print(mDMf) ### 3. fit the exact same model to the simulated data using DM matrices # define DM DMm <- list(step=diag(4),angle=diag(2)) # user-specified dimnames not required but are recommended dimnames(DMm$step) <- list(c("mean_1","mean_2","sd_1","sd_2"), c("mean_1:(Intercept)","mean_2:(Intercept)", "sd_1:(Intercept)","sd_2:(Intercept)")) dimnames(DMm$angle) <- list(c("concentration_1","concentration_2"), c("concentration_1:(Intercept)","concentration_2:(Intercept)")) mDMm <- fitHMM(data=data,nbStates=nbStates,dist=list(step=stepDist,angle=angleDist), Par0=Par0,formula=formula, DM=DMm) print(mDMm) ### 4. fit step mean parameter covariate model to the simulated data using DM stepDMf <- list(mean=~cov1,sd=~1) Par0 <- getParDM(data,nbStates,list(step=stepDist,angle=angleDist), Par=list(step=stepPar,angle=anglePar), DM=list(step=stepDMf,angle=DMm$angle)) mDMfcov <- fitHMM(data=data,nbStates=nbStates,dist=list(step=stepDist,angle=angleDist), Par0=Par0, formula=formula, DM=list(step=stepDMf,angle=DMm$angle)) print(mDMfcov) ### 5. fit the exact same step mean parameter covariate model using DM matrix stepDMm <- matrix(c(1,0,0,0,"cov1",0,0,0,0,1,0,0,0,"cov1",0,0, 0,0,1,0,0,0,0,1),4,6,dimnames=list(c("mean_1","mean_2","sd_1","sd_2"), c("mean_1:(Intercept)","mean_1:cov1","mean_2:(Intercept)","mean_2:cov1", "sd_1:(Intercept)","sd_2:(Intercept)"))) Par0 <- getParDM(data,nbStates,list(step=stepDist,angle=angleDist), Par=list(step=stepPar,angle=anglePar), DM=list(step=stepDMm,angle=DMm$angle)) mDMmcov <- fitHMM(data=data,nbStates=nbStates,dist=list(step=stepDist,angle=angleDist), Par0=Par0, formula=formula, DM=list(step=stepDMm,angle=DMm$angle)) print(mDMmcov) ### 6. fit circular-circular angle mean covariate model to the simulated data using DM # Generate fake circular covariate using circAngles data$cov3 <- circAngles(refAngle=2*atan(rnorm(nrow(data))),data) # Fit circular-circular regression model for angle mean # Note no intercepts are estimated for angle means because these are by default # the previous movement direction (i.e., a turning angle of zero) mDMcircf <- fitHMM(data=data,nbStates=nbStates,dist=list(step=stepDist,angle=angleDist), Par0=list(step=stepPar,angle=c(0,0,Par0$angle)), formula=formula, estAngleMean=list(angle=TRUE), circularAngleMean=list(angle=TRUE), DM=list(angle=list(mean=~cov3,concentration=~1))) print(mDMcircf) ### 7. fit the exact same circular-circular angle mean model using DM matrices # Note no intercept terms are included in DM for angle means because the intercept is # by default the previous movement direction (i.e., a turning angle of zero) mDMcircm <- fitHMM(data=data,nbStates=nbStates,dist=list(step=stepDist,angle=angleDist), Par0=list(step=stepPar,angle=c(0,0,Par0$angle)), formula=formula, estAngleMean=list(angle=TRUE), circularAngleMean=list(angle=TRUE), DM=list(angle=matrix(c("cov3",0,0,0,0,"cov3",0,0,0,0,1,0,0,0,0,1),4,4))) print(mDMcircm) ### 8. Cosinor and state-dependent formulas nbStates<-2 dist<-list(step="gamma") Par<-list(step=c(100,1000,50,100)) # include 24-hour cycle on all transition probabilities # include 12-hour cycle on transitions from state 2 formula=~cosinor(hour24,24)+state2(cosinor(hour12,12)) # specify appropriate covariates covs<-data.frame(hour24=0:23,hour12=0:11) beta<-matrix(c(-1.5,1,1,NA,NA,-1.5,-1,-1,1,1),5,2) # row names for beta not required but can be helpful rownames(beta)<-c("(Intercept)", "cosinorCos(hour24, 24)", "cosinorSin(hour24, 24)", "cosinorCos(hour12, 12)", "cosinorSin(hour12, 12)") data.cos<-simData(nbStates=nbStates,dist=dist,Par=Par, beta=beta,formula=formula,covs=covs) m.cosinor<-fitHMM(data.cos,nbStates=nbStates,dist=dist,Par0=Par,formula=formula) m.cosinor ### 9. Piecewise constant B-spline on step length mean and angle concentration nObs <- 1000 # length of simulated track cov <- data.frame(time=1:nObs) # time covariate for splines dist <- list(step="gamma",angle="vm") stepDM <- list(mean=~splines2::bSpline(time,df=2,degree=0),sd=~1) angleDM <- list(mean=~1,concentration=~splines2::bSpline(time,df=2,degree=0)) DM <- list(step=stepDM,angle=angleDM) Par <- list(step=c(log(1000),1,-1,log(100)),angle=c(0,log(10),2,-5)) data.spline<-simData(obsPerAnimal=nObs,nbStates=1,dist=dist,Par=Par,DM=DM,covs=cov) Par0 <- list(step=Par$step,angle=Par$angle[-1]) m.spline<-fitHMM(data.spline,nbStates=1,dist=dist,Par0=Par0, DM=list(step=stepDM, angle=angleDM["concentration"])) ### 10. Initial state (delta) based on covariate nObs <- 100 dist <- list(step="gamma",angle="vm") Par <- list(step=c(100,1000,50,100),angle=c(0,0,0.01,0.75)) # create sex covariate cov <- data.frame(sex=factor(rep(c("F","M"),each=nObs))) # sex covariate formulaDelta <- ~ sex + 0 # Female begins in state 1, male begins in state 2 delta <- matrix(c(-100,100),2,1,dimnames=list(c("sexF","sexM"),"state 2")) data.delta<-simData(nbAnimals=2,obsPerAnimal=nObs,nbStates=2,dist=dist,Par=Par, delta=delta,formulaDelta=formulaDelta,covs=cov) Par0 <- list(step=Par$step, angle=Par$angle[3:4]) m.delta <- fitHMM(data.delta, nbStates=2, dist=dist, Par0 = Par0, formulaDelta=formulaDelta) ### 11. Two mixtures based on covariate nObs <- 100 nbAnimals <- 20 dist <- list(step="gamma",angle="vm") Par <- list(step=c(100,1000,50,100),angle=c(0,0,0.1,2)) # create sex covariate cov <- data.frame(sex=factor(rep(c("F","M"),each=nObs*nbAnimals/2))) formulaPi <- ~ sex + 0 # Females more likely in mixture 1, males more likely in mixture 2 beta <- list(beta=matrix(c(-1.5,-0.5,-1.5,-3),2,2), pi=matrix(c(-2,2),2,1,dimnames=list(c("sexF","sexM"),"mix2"))) data.mix<-simData(nbAnimals=nbAnimals,obsPerAnimal=nObs,nbStates=2,dist=dist,Par=Par, beta=beta,formulaPi=formulaPi,mixtures=2,covs=cov) Par0 <- list(step=Par$step, angle=Par$angle[3:4]) m.mix <- fitHMM(data.mix, nbStates=2, dist=dist, Par0 = Par0, beta0=beta,formulaPi=formulaPi,mixtures=2) ## End(Not run)
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