2016 International Conference on Computational Science and Computational Intelligence (CSCI) 2016
DOI: 10.1109/csci.2016.0227
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Closest History Flow Field Forecasting for IEEE CSCI-ISCS

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Cited by 2 publications
(6 citation statements)
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“…Because different history structures () have a different numbers of predictors, the distances are computed in spaces with different dimensions. In (Caudle and Fleming (2016)), we show that the Manhattan distance computed in different dimensional spaces have different distributions and different quantiles. So, direct comparison of distances is not appropriate.…”
Section: Bivariate Ff Forecastingmentioning
confidence: 87%
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“…Because different history structures () have a different numbers of predictors, the distances are computed in spaces with different dimensions. In (Caudle and Fleming (2016)), we show that the Manhattan distance computed in different dimensional spaces have different distributions and different quantiles. So, direct comparison of distances is not appropriate.…”
Section: Bivariate Ff Forecastingmentioning
confidence: 87%
“…For bivariate data, we start with a set of candidate predictors (scriptP). We then search over all history structures () obtained from all the power sets of scriptP (Caudle & Fleming, 2016). Although this is computationally expensive, for bivariate data, it does not overload the computing resources on standard desktop computers.…”
Section: Bivariate Ff Forecastingmentioning
confidence: 99%
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