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Applications of state space models in finance

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5.2 Stochastic volatility 67<br />

5.2.1.1 L<strong>in</strong>earized representation<br />

Harvey et al. (1994) proposed to l<strong>in</strong>earize the SV model by squar<strong>in</strong>g the returns and<br />

tak<strong>in</strong>g logarithms:<br />

log y 2 t = log σ2 ∗ + ht + log ɛ 2 t , (5.27)<br />

ht+1 = φht + ηt, (5.28)<br />

where the disturbance terms <strong>in</strong> the transformed model are assumed to be uncorrelated,<br />

contemporaneously and at all lags. The standard normality <strong>of</strong> ɛt <strong>in</strong> the orig<strong>in</strong>al mean<br />

equation (5.25) implies a log � χ2 �<br />

2<br />

1 distribution for log ɛt with mean −1.27 and variance<br />

π 2 /2 = 4.93. Tak<strong>in</strong>g logarithms <strong>of</strong> very small numbers leads to a heavily skewed distribution<br />

<strong>of</strong> log ɛ 2 t with a long left-hand tail. Another important issue <strong>of</strong> practical relevance<br />

is the so-called <strong>in</strong>lier problem, which arises when tak<strong>in</strong>g logarithms <strong>of</strong> returns that are<br />

equal to zero. In case where zero returns go back to irregular observations, deletion <strong>of</strong><br />

these observations avoids the <strong>in</strong>lier problem. For those <strong>in</strong>liers that cannot be assumed<br />

to result from data irregularities, Sandmann and Koopman (1998) describe various ways<br />

<strong>of</strong> deal<strong>in</strong>g with them. They recommend to cut <strong>of</strong>f any <strong>in</strong>liers by replac<strong>in</strong>g zeros by the<br />

value 0.001.<br />

Unfortunately, due to the non-Gaussianity <strong>of</strong> the observation disturbances, the prediction<br />

error decomposition <strong>in</strong> (3.58) does not yield the exact likelihood. Thus, a direct<br />

application <strong>of</strong> the Kalman filter us<strong>in</strong>g the QML method <strong>in</strong>troduced <strong>in</strong> ¢ 3.3.7, only yields<br />

m<strong>in</strong>imum mean square l<strong>in</strong>ear estimators. Even though the QML asymptotic theory is<br />

correct, it has been shown that due to the poor approximation <strong>of</strong> log ɛ2 t by a normal<br />

distribution, the correspond<strong>in</strong>g QML estimator has poor small sample properties (Kim<br />

et al. 1998). Therefore, the QML method for estimat<strong>in</strong>g SV <strong>models</strong> will not f<strong>in</strong>d any<br />

consideration hereafter.<br />

5.2.1.2 Statistical properties<br />

Accord<strong>in</strong>g to Shephard (1996) the properties <strong>of</strong> the SV model as represented by (5.26)<br />

and (5.26) can be easily derived. For φ be<strong>in</strong>g restricted to be positive and smaller than<br />

unity, the standard Gaussian autoregression ht will be strictly covariance stationary and<br />

follow a log-normal distribution with<br />

E(ht) = 0, (5.29)<br />

V ar(ht) = σ2 η<br />

. (5.30)<br />

1 − φ2 Stationarity <strong>of</strong> yt holds if and only if ɛt and ht are stationary processes. Given the<br />

properties <strong>of</strong> the log-normal distribution, for stationary ht all odd moments are zero.<br />

All even moments exist and are given by<br />

E(y r t ) = E(ɛ r � �<br />

r<br />

t )E exp<br />

2 ht<br />

��<br />

� � 2 2 r σ<br />

�<br />

h<br />

= r! exp /<br />

8<br />

2 r/2 � r<br />

2<br />

� �<br />

! , (5.31)

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