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contributor authorHaam, Eddie
contributor authorTung, Ka-Kit
date accessioned2017-06-09T16:55:08Z
date available2017-06-09T16:55:08Z
date copyright2012/10/01
date issued2012
identifier issn0022-4928
identifier otherams-76490.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4218942
description abstractoth the 11-yr solar cycle and the El Niño?Southern Oscillation (ENSO) phenomena are quasi periodic, with periods of 9?11 and 3?4 yr, respectively. There have been claims that the two are correlated, with the sun at its peak in sunspot number presumably forcing a cold event in the equatorial Pacific. However, both phenomena are also highly autocorrelated. Caution should be exercised when testing for the statistical significance of the correlation of two autocorrelated time series. The solar peak years can coincide with cold ENSO by chance, even if the two time series are independent, and the coincidence then persists for many cycles due to their autocorrelation, before drifting apart. This study demonstrates that this is indeed the case using the Quinn El Niño index (1525?1987), which is a chronicle of observations of El Niño?related events, and the sunspot number (SSN) series going back to 1750. Appropriate statistical tests are suggested that can test for correlation, taking into account autocorrelation applicable to the shorter instrumental records. There is so far no solar peak?La Niña connection found that is statistically significant.
publisherAmerican Meteorological Society
titleStatistics of Solar Cycle–La Niña Connection: Correlation of Two Autocorrelated Time Series
typeJournal Paper
journal volume69
journal issue10
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/JAS-D-12-0101.1
journal fristpage2934
journal lastpage2939
treeJournal of the Atmospheric Sciences:;2012:;Volume( 069 ):;issue: 010
contenttypeFulltext


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