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1 Studies in the History of Statistics and Probability ... - Sheynin, Oscar

1 Studies in the History of Statistics and Probability ... - Sheynin, Oscar

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This is <strong>the</strong> celebrated model <strong>of</strong> autoregression (<strong>of</strong> <strong>the</strong> second order)which was applied by many statisticians deserv<strong>in</strong>g complete trust.Yule’s considerations lead<strong>in</strong>g to model (3.8) were, however, not quiteclear. In particular, for <strong>the</strong> case <strong>of</strong> <strong>the</strong> pendulum, {δ n } is not asequence <strong>of</strong> <strong>in</strong>dependent r<strong>and</strong>om variables but is ra<strong>the</strong>r describable bySlutsky’s mov<strong>in</strong>g average. However, <strong>in</strong>troduc<strong>in</strong>g additionalparameters <strong>of</strong> that average <strong>in</strong>to <strong>the</strong> model will mean hav<strong>in</strong>g too manyparameters <strong>and</strong> extremely complicated work <strong>in</strong> its application.Yule’s mistake certa<strong>in</strong>ly does not logically prove that <strong>the</strong> modelis not applicable to sunspots or some economic <strong>in</strong>dicator, but <strong>of</strong> courseit is a bad omen.Descartes noted that <strong>the</strong> world can be expla<strong>in</strong>ed <strong>in</strong> many differentmanners <strong>and</strong> <strong>the</strong> problem only is, to choose that which is really valid.Most chances to be valid certa<strong>in</strong>ly has that manner which is <strong>the</strong> mostnatural <strong>and</strong> harmonious <strong>and</strong> does not conta<strong>in</strong> contradictions. If,however, it occurs that <strong>the</strong> creator <strong>of</strong> a <strong>the</strong>ory committed a mistake at<strong>the</strong> very outset, even if only concern<strong>in</strong>g a particular case, our chances<strong>of</strong> success <strong>in</strong> o<strong>the</strong>r cases will sharply dim<strong>in</strong>ish.As to sunspots, Yule himself did not achieve a decisive positiveresult. He was compelled to change his model (3.8) by assum<strong>in</strong>g thatwe observe not <strong>the</strong> variables {ξ n } <strong>the</strong>mselves, but that our observationswere corrupted by an additional r<strong>and</strong>om error. He had to make thischange because his model did not pass a statistical check to which hesubjected it, as was supposed to be done. The change <strong>of</strong> <strong>the</strong> modelallows to make ends meet but <strong>in</strong> statistics <strong>in</strong>troduc<strong>in</strong>g an additionalparameter is very bad.In general, Yule’s contribution (1927) is an example <strong>of</strong> a statisticalmasterpiece which, however, provided a dubious (if not negative)result <strong>of</strong>ten happen<strong>in</strong>g exactly with masterpieces.The <strong>in</strong>terest emerged <strong>in</strong> forecast<strong>in</strong>g stochastic processes led ano<strong>the</strong>rrepresentative <strong>of</strong> <strong>the</strong> English school, Moran (1954), to study <strong>the</strong>possibilities <strong>of</strong> apply<strong>in</strong>g model (3.8) for predict<strong>in</strong>g solar activity. S<strong>in</strong>ceδ n does not depend on <strong>the</strong> previous behaviour <strong>of</strong> <strong>the</strong> process, that is, onvariables ξ n−1 , ξ n−2 , ..., <strong>the</strong> best possible method <strong>of</strong> forecast<strong>in</strong>g <strong>the</strong>estimate <strong>of</strong> ξ n from all <strong>the</strong> previous <strong>in</strong>formation is to assume thatˆξ = − ( a ξ + b ξ ).n n−1 n−2Moran did that <strong>and</strong> had showed his result to his friends among radiophysicists who told him that a forecast <strong>of</strong> such a quality could havebeen possible without any science, just by naked eye. And so it was, asproved by an experiment. That was <strong>the</strong> second failure <strong>of</strong> <strong>the</strong> model <strong>of</strong>autoregression.That model possesses, however, an excellent property: it is easilyapplied. Its parameters are easy to estimate , <strong>the</strong> correlation function is<strong>of</strong> <strong>the</strong> k<strong>in</strong>d <strong>of</strong> fad<strong>in</strong>g s<strong>in</strong>usoidal oscillations <strong>and</strong> is comparatively easyto be <strong>in</strong>terpreted. The spectral density is also expressed <strong>in</strong> a simpleway. It made sense <strong>the</strong>refore to test it many times on differ<strong>in</strong>g material<strong>and</strong> hope that cases <strong>in</strong> which it works well enough will be found. It isbest to read about <strong>the</strong> application <strong>of</strong> <strong>the</strong> autoregression model <strong>in</strong>Kendall & Stuart (1968).73

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