advanced spectral methods for climatic time series - Atmospheric ...
advanced spectral methods for climatic time series - Atmospheric ...
advanced spectral methods for climatic time series - Atmospheric ...
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40, 1 / REVIEWS OF GEOPHYSICS Ghil et al.: CLIMATIC TIME SERIES ANALYSIS ● 3-3<br />
TABLE 1. (continued)<br />
Symbol Definition Method Section<br />
nt discretely sampled <strong>time</strong> 1<br />
Uk(f) W<br />
discrete Fourier trans<strong>for</strong>m of wk(t) sliding-window length of wavelet<br />
MTM<br />
SSA<br />
3.4<br />
2.4<br />
W(a, b)<br />
W(k) Wm(k) wk(t) Xˆ (t)<br />
wavelet trans<strong>for</strong>m of {X(t)} using b-translated and a-dilated ((t b)/a)<br />
lag window <strong>for</strong> S<br />
X(f) with smoothing parameter <br />
Bartlett window <strong>for</strong> S<br />
X(f) with window length m<br />
kth taper<br />
observed <strong>time</strong> <strong>series</strong><br />
SSA<br />
BT<br />
BT<br />
MTM<br />
2.4<br />
3.2<br />
3.2<br />
3.4<br />
1<br />
Xn X<br />
X(nt) 1<br />
(p)<br />
pth-order differentiation of X(t) with respect to <strong>time</strong> t, d p X/dt p<br />
1<br />
{X(t)} univariate <strong>time</strong> <strong>series</strong> in t or t <br />
X˜(t) M-dimensional augmented vector of X(t)<br />
1<br />
2.1<br />
X0 XI(t) X˜(t), X˜(nt)<br />
mean of {X(t)}<br />
reconstructed X(t)<br />
continuous- and discrete-<strong>time</strong> reconstructed signal<br />
SSA<br />
WLTs<br />
MTM<br />
2.3<br />
2.4<br />
3.4<br />
{X(t)} multivariate <strong>time</strong> <strong>series</strong> in t or t <br />
{X˜<br />
l}<br />
Yˆ<br />
k(f)<br />
<br />
multichannel augmented vector of {X˜(t)}<br />
discrete Fourier trans<strong>for</strong>m of {X(t)w k(t)}<br />
<strong>time</strong>-scale ratio<br />
POP<br />
SSA<br />
MTM<br />
SSA<br />
4.1<br />
4.2<br />
3.4<br />
2.4<br />
(t) additive noise MTM 3.4<br />
explained contribution to variance MTM 3.4<br />
k, X R k <br />
kth eigenvalue and eigenvalue matrix of CX projection of CR onto EX weight of kth taper<br />
number of degrees of freedom of spectrum<br />
SSA<br />
SSA<br />
MTM<br />
MTM<br />
2.2<br />
2.3<br />
3.4<br />
3.4<br />
(t) random <strong>for</strong>cing 1<br />
k, EX kth eigenvector and eigenvector matrix of CX SSA 2.2<br />
2<br />
variance of random <strong>for</strong>cing 1<br />
<br />
X(k), ˆ<br />
X(k)<br />
(x)<br />
characteristic delay <strong>time</strong><br />
true and estimated lag k autocorrelation function of X(t)<br />
mother wavelet of variable x<br />
SSA<br />
BT<br />
WLTs<br />
2.3<br />
3.2<br />
2.4<br />
unexplained contribution to variance MTM 3.4<br />
a Method and section number correspond to where the symbol appears first or is used differently from previous sections.<br />
tifying certain features of the <strong>time</strong> <strong>series</strong>. These properties<br />
can then help understand the system’s behavior and<br />
predict its future.<br />
[3] To illustrate the ideas and <strong>methods</strong> reviewed here,<br />
we shall turn to one of the best known <strong>climatic</strong> <strong>time</strong><br />
<strong>series</strong>. This <strong>time</strong> <strong>series</strong> is made up of monthly values of<br />
the Southern Oscillation Index (SOI). It will be introduced<br />
in section 2.2 and is shown in Figure 2 there.<br />
[4] At this point we merely note that physical processes<br />
usually operate in continuous <strong>time</strong>. Most measurements,<br />
though, are done and recorded in discrete<br />
<strong>time</strong>. Thus the SOI <strong>time</strong> <strong>series</strong>, as well as most <strong>climatic</strong><br />
and other geophysical <strong>time</strong> <strong>series</strong>, are available in discrete<br />
<strong>time</strong>.<br />
1.1. Analysis in the Time Domain Versus the<br />
Spectral Domain<br />
[5] Two basic approaches to <strong>time</strong> <strong>series</strong> analysis are<br />
associated with the <strong>time</strong> domain or the <strong>spectral</strong> domain.<br />
We present them at first in the linear context in which<br />
the physical sciences have operated <strong>for</strong> most of the last<br />
two centuries. In this context the physical system can be<br />
described by a linear ordinary differential equation<br />
(ODE), or a system of such equations, subject to additive<br />
random <strong>for</strong>cing.<br />
[6] It goes well beyond the scope of this review paper<br />
to introduce the concepts of random variables, stochastic<br />
processes, and stochastic differential equations. We refer<br />
the interested reader to Feller [1968, 1971] <strong>for</strong> the<br />
<strong>for</strong>mer two concepts and to Arnold [1974] and Schuss<br />
[1980] <strong>for</strong> the latter. Many of the standard books on<br />
classical <strong>spectral</strong> <strong>methods</strong> that are cited in sections 3.1<br />
and 3.2 also contain good elementary introductions to<br />
stochastic processes in discrete and, some<strong>time</strong>s, continuous<br />
<strong>time</strong>.<br />
[7] We concentrate here on <strong>time</strong> <strong>series</strong> in discrete<br />
<strong>time</strong> and consider there<strong>for</strong>e first the simple case of a<br />
scalar, linear ordinary difference equation with random<br />
<strong>for</strong>cing,<br />
M<br />
Xt 1 aj Xt M j t. (1)<br />
j1<br />
Its constant coefficients a j determine the solutions X(t)<br />
at discrete <strong>time</strong>s t 0, 1, , n, . In (1) the random<br />
<strong>for</strong>cing (t) is assumed to be white in <strong>time</strong>, i.e., uncor-