389 Spatio-Temporal Modeling for Small Area Health Analysis
mechanism of disease occurrence within the model. These latter models are often assumed
for infectious diseases where transmission from one time period to the next can be directly
modeled (see Section 18.4.2). Descriptive models often use random effects to provide a
parsimonious summary description of the risk variation. These are often most appro-
priate for noninfectious diseases. In what follows, we will discuss models for the rela-
tive risk under the Poisson model. Specication can be easily modied for a binomial
likelihood.
18.2.1 Descriptive Models
A basic description of space-time variation would consist of a separate spatial and temporal
effect model with a possible effect for the residual space-time interaction. Assume that
log(θ
it
) = α
0
+ S
i
+ T
t
+ ST
it
(18.1)
where S
i
, T
t
,and ST
it
represent the spatial, temporal, and space-time interaction terms,
respectively. Here, exp(α
0
) represents the overall rate in space-time.
Some simple spatial models could consist of (1) spatial trend (e.g., S
i
= α
1
s
1i
+ α
2
s
2i
where (s
1i
, s
2i
) is a coordinate pair for the geographic centroid of the ith small area), (2)
uncorrelated heterogeneity (e.g., S
i
= v
i
where v
i
is an uncorrelated heterogeneity term),
or (3) as for (2) but with correlated heterogeneity added (e.g., S
i
= v
i
+ u
i
where u
i
is a
spatially correlated heterogeneity term). This latter model is sometimes called a convolu-
tion model. The temporal effect T
t
can also take a variety of forms: (1) simple linear time
trend, that is, T
t
= βγ
t
where γ
t
is the actual time of the tth period and (2) a random time
−1
effect such as an autoregressive lag 1 model (i.e., T
t
∼ N(φT
t−1
, τ
T
)) or a random walk
(when φ = 1). A simpler uncorrelated time effect could also be considered where T
t
∼ N(0,
−1
τ
T
), τ
∗
being the precision of the respective Gaussian distribution. Combinations of
uncorrelated and correlated effects could also be considered for the time component.
Finally, as a form of residual interaction, the space-time interaction term (ST
it
) can also
be included. Often, the specication of
log(θ
it
) = α
0
+ v
i
+ u
i
+ γ
t
+ ψ
it
, (18.2)
−1
where the interaction is assumed to be dened as ψ
it
∼ N(0, τ
ψ
) is found to be a robust
and appropriate model for disease variation (see, e.g., Knorr-Held, 2000; Lawson, 2013,
ch 12). More sophisticated models with nonseparable space-time variation are also pos-
sible (see, e.g., Cai et al., 2012, 2013). These models can sometimes be more effective in
describing the space-time variation but are less immediately interpretable than separable
models. In terms of inferential paradigms, it is commonly found that a Bayesian approach
is adopted to the formulation of the hierarchical model structure and the ensuing estima-
tion methods focus on posterior sampling via Markov chain Monte Carlo (MCMC). For
the model specication in (18.2), the model hierarchy with suitable prior distributions
could be