Become an expert in R — Interactive courses, Cheat Sheets, certificates and more!
Get Started for Free

ssm_ulg

General univariate linear-Gaussian state space models


Description

Construct an object of class ssm_ulg by directly defining the corresponding terms of the model.

Usage

ssm_ulg(
  y,
  Z,
  H,
  T,
  R,
  a1,
  P1,
  init_theta = numeric(0),
  D,
  C,
  state_names,
  update_fn = default_update_fn,
  prior_fn = default_prior_fn
)

Arguments

y

Observations as time series (or vector) of length n.

Z

System matrix Z of the observation equation as m x 1 or m x n matrix.

H

Vector of standard deviations. Either a scalar or a vector of length n.

T

System matrix T of the state equation. Either a m x m matrix or a m x m x n array.

R

Lower triangular matrix R the state equation. Either a m x k matrix or a m x k x n array.

a1

Prior mean for the initial state as a vector of length m.

P1

Prior covariance matrix for the initial state as m x m matrix.

init_theta

Initial values for the unknown hyperparameters theta.

D

Intercept terms for observation equation, given as a length n vector.

C

Intercept terms for state equation, given as m x n matrix.

state_names

Names for the states.

update_fn

Function which returns list of updated model components given input vector theta. See details.

prior_fn

Function which returns log of prior density given input vector theta.

Details

The general univariate linear-Gaussian model is defined using the following observational and state equations:

y_t = D_t + Z_t α_t + H_t ε_t, (\textrm{observation equation})

α_{t+1} = C_t + T_t α_t + R_t η_t, (\textrm{transition equation})

where ε_t \sim N(0, 1), η_t \sim N(0, I_k) and α_1 \sim N(a_1, P_1) independently of each other. Here k is the number of disturbance terms which can be less than m, the number of states.

The update_fn function should take only one vector argument which is used to create list with elements named as Z, H T, R, a1, P1, D, and C, where each element matches the dimensions of the original model. If any of these components is missing, it is assumed to be constant wrt. theta. Note that while you can input say R as m x k matrix for ssm_ulg, update_fn should return R as m x k x 1 in this case. It might be useful to first construct the model without updating function and then check the expected structure of the model components from the output.

Value

Object of class ssm_ulg.

Examples

# Regression model with time-varying coefficients
set.seed(1)
n <- 100
x1 <- rnorm(n)
x2 <- rnorm(n)
b1 <- 1 + cumsum(rnorm(n, sd = 0.5))
b2 <- 2 + cumsum(rnorm(n, sd = 0.1))
y <- 1 + b1 * x1 + b2 * x2 + rnorm(n, sd = 0.1)

Z <- rbind(1, x1, x2)
H <- 0.1
T <- diag(3)
R <- diag(c(0, 1, 0.1))
a1 <- rep(0, 3)
P1 <- diag(10, 3)

# updates the model given the current values of the parameters
update_fn <- function(theta) {
  R <- diag(c(0, theta[1], theta[2]))
  dim(R) <- c(3, 3, 1)
  list(R = R, H = theta[3])
}
# prior for standard deviations as half-normal(1)
prior_fn <- function(theta) {
  if(any(theta < 0)){
  log_p <- -Inf 
  } else {
  log_p <- sum(dnorm(theta, 0, 1, log = TRUE))
  }
  log_p
}

model <- ssm_ulg(y, Z, H, T, R, a1, P1, 
  init_theta = c(1, 0.1, 0.1), 
  update_fn = update_fn, prior_fn = prior_fn)

out <- run_mcmc(model, iter = 10000)
out
sumr <- summary(out, variable = "state")
ts.plot(sumr$Mean, col = 1:3)
lines(b1, col= 2, lty = 2)
lines(b2, col= 3, lty = 2)

# Perhaps easiest way to construct a general SSM for bssm is to use the 
# model building functionality of KFAS:
library("KFAS")

model_kfas <- SSModel(log(drivers) ~ SSMtrend(1, Q = 5e-4)+
  SSMseasonal(period = 12, sea.type = "trigonometric", Q = 0) +
 log(PetrolPrice) + law, data = Seatbelts, H = 0.005)

# use as_bssm function for conversion, kappa defines the 
# prior variance for diffuse states
model_bssm <- as_bssm(model_kfas, kappa = 100)

# define updating function for parameter estimation
# we can use SSModel and as_bssm functions here as well
# (for large model it is more efficient to do this 
# "manually" by constructing only necessary matrices,
# i.e., in this case  a list with H and Q)

updatefn <- function(theta){
  
  model_kfas <- SSModel(log(drivers) ~ SSMtrend(1, Q = theta[1]^2)+
    SSMseasonal(period = 12, 
      sea.type = "trigonometric", Q = theta[2]^2) +
    log(PetrolPrice) + law, data = Seatbelts, H = theta[3]^2)
  
  as_bssm(model_kfas, kappa = 100)
}

prior <- function(theta) {
  if(any(theta < 0)) -Inf else sum(dnorm(theta, 0, 0.1, log = TRUE))
}
init_theta <- rep(1e-2, 3)
c("sd_level", "sd_seasonal", "sd_y")
model_bssm <- as_bssm(model_kfas, kappa = 100, 
  init_theta = init_theta, 
  prior_fn = prior, update_fn = updatefn)

## Not run: 
out <- run_mcmc(model_bssm, iter = 10000, burnin = 5000) 
out

# Above the regression coefficients are modelled as time-invariant latent states. 
# Here is an alternative way where we use variable D so that the
# coefficients are part of parameter vector theta:

updatefn2 <- function(theta) {
  # note no PetrolPrice or law variables here
  model_kfas2 <- SSModel(log(drivers) ~ SSMtrend(1, Q = theta[1]^2)+
    SSMseasonal(period = 12, sea.type = "trigonometric", Q = theta[2]^2), 
    data = Seatbelts, H = theta[3]^2)
  
  X <- model.matrix(~ -1 + law + log(PetrolPrice), data = Seatbelts)
  D <- t(X %*% theta[4:5])
  as_bssm(model_kfas2, D = D, kappa = 100)
}
prior2 <- function(theta) {
 if(any(theta[1:3] < 0)) {
  -Inf
 } else {
   sum(dnorm(theta[1:3], 0, 0.1, log = TRUE)) +
   sum(dnorm(theta[4:5], 0, 10, log = TRUE))
 }
}
init_theta <- c(rep(1e-2, 3), 0, 0)
names(init_theta) <- c("sd_level", "sd_seasonal", "sd_y", "law", "Petrol")
model_bssm2 <- updatefn2(init_theta)
model_bssm2$theta <- init_theta
model_bssm2$prior_fn <- prior2
model_bssm2$update_fn <- updatefn2

out2 <- run_mcmc(model_bssm2, iter = 10000, burnin = 5000) 
out2

## End(Not run)

bssm

Bayesian Inference of Non-Linear and Non-Gaussian State Space Models

v1.1.4
GPL (>= 2)
Authors
Jouni Helske [aut, cre] (<https://orcid.org/0000-0001-7130-793X>), Matti Vihola [aut] (<https://orcid.org/0000-0002-8041-7222>)
Initial release
2021-04-13

We don't support your browser anymore

Please choose more modern alternatives, such as Google Chrome or Mozilla Firefox.