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    Statistics of Solar Cycle–La Niña Connection: Correlation of Two Autocorrelated Time Series

    Source: Journal of the Atmospheric Sciences:;2012:;Volume( 069 ):;issue: 010::page 2934
    Author:
    Haam, Eddie
    ,
    Tung, Ka-Kit
    DOI: 10.1175/JAS-D-12-0101.1
    Publisher: American Meteorological Society
    Abstract: oth 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.
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      Statistics of Solar Cycle–La Niña Connection: Correlation of Two Autocorrelated Time Series

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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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    DSpace software copyright © 2002-2015  DuraSpace
    نرم افزار کتابخانه دیجیتال "دی اسپیس" فارسی شده توسط یابش برای کتابخانه های ایرانی | تماس با یابش
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