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Correlation of Time Series of Wolf Numbers and their Derivatives
The results of the study of the correlation of the mean annual Wolf numbers W and their time derivatives W ' for time shifts of fragments of series W and W ' relative to each other are presented. The most significant (up to 0.88 and –0.85) correlation and anticorrelation coefficients are...
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Published in: | Geomagnetism and Aeronomy 2022-12, Vol.62 (6), p.685-693 |
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description | The results of the study of the correlation of the mean annual Wolf numbers
W
and their time derivatives
W
' for time shifts of fragments of series
W
and
W
' relative to each other are presented. The most significant (up to 0.88 and –0.85) correlation and anticorrelation coefficients are obtained with shifts of 2 or 3 years for fragments covering two 11-year cycles. For longer fragments, the coefficients remain significant (at levels of approximately ±0.8) at the same shifts. Therefore, the phase shift between
W
and
W
' is approximately one-quarter of the solar cycle, which physically corresponds to the predominant connection of spots with magnetic energy. At the same time, there is also a significant shift by 8–9 years, which corresponds to correlation coefficients at levels of approximately ±0.75 associated with the magnetic energy variability. The prognostic potentials of the obtained correlation dependences are discussed. |
doi_str_mv | 10.1134/S0016793222050164 |
format | article |
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W
and their time derivatives
W
' for time shifts of fragments of series
W
and
W
' relative to each other are presented. The most significant (up to 0.88 and –0.85) correlation and anticorrelation coefficients are obtained with shifts of 2 or 3 years for fragments covering two 11-year cycles. For longer fragments, the coefficients remain significant (at levels of approximately ±0.8) at the same shifts. Therefore, the phase shift between
W
and
W
' is approximately one-quarter of the solar cycle, which physically corresponds to the predominant connection of spots with magnetic energy. At the same time, there is also a significant shift by 8–9 years, which corresponds to correlation coefficients at levels of approximately ±0.75 associated with the magnetic energy variability. The prognostic potentials of the obtained correlation dependences are discussed.</description><identifier>ISSN: 0016-7932</identifier><identifier>EISSN: 1555-645X</identifier><identifier>EISSN: 0016-7940</identifier><identifier>DOI: 10.1134/S0016793222050164</identifier><language>eng</language><publisher>Moscow: Pleiades Publishing</publisher><subject>Correlation coefficient ; Correlation coefficients ; Earth and Environmental Science ; Earth Sciences ; Fragments ; Geophysics/Geodesy ; Solar cycle ; Sunspot numbers</subject><ispartof>Geomagnetism and Aeronomy, 2022-12, Vol.62 (6), p.685-693</ispartof><rights>Pleiades Publishing, Ltd. 2022. ISSN 0016-7932, Geomagnetism and Aeronomy, 2022, Vol. 62, No. 6, pp. 685–693. © Pleiades Publishing, Ltd., 2022. Russian Text © The Author(s), 2022, published in Geomagnetizm i Aeronomiya, 2022, Vol. 62, No. 6, pp. 693–701.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-LOGICAL-c198t-b1962513cedf10a4fdcc478e32ad783ffb5a08f08dfb427fe6963358835bbee13</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids></links><search><creatorcontrib>Starchenko, S. V.</creatorcontrib><creatorcontrib>Yakovleva, S. V.</creatorcontrib><title>Correlation of Time Series of Wolf Numbers and their Derivatives</title><title>Geomagnetism and Aeronomy</title><addtitle>Geomagn. Aeron</addtitle><description>The results of the study of the correlation of the mean annual Wolf numbers
W
and their time derivatives
W
' for time shifts of fragments of series
W
and
W
' relative to each other are presented. The most significant (up to 0.88 and –0.85) correlation and anticorrelation coefficients are obtained with shifts of 2 or 3 years for fragments covering two 11-year cycles. For longer fragments, the coefficients remain significant (at levels of approximately ±0.8) at the same shifts. Therefore, the phase shift between
W
and
W
' is approximately one-quarter of the solar cycle, which physically corresponds to the predominant connection of spots with magnetic energy. At the same time, there is also a significant shift by 8–9 years, which corresponds to correlation coefficients at levels of approximately ±0.75 associated with the magnetic energy variability. The prognostic potentials of the obtained correlation dependences are discussed.</description><subject>Correlation coefficient</subject><subject>Correlation coefficients</subject><subject>Earth and Environmental Science</subject><subject>Earth Sciences</subject><subject>Fragments</subject><subject>Geophysics/Geodesy</subject><subject>Solar cycle</subject><subject>Sunspot numbers</subject><issn>0016-7932</issn><issn>1555-645X</issn><issn>0016-7940</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><recordid>eNp1kE9Lw0AQxRdRMFY_gLcFz9Gd_ZNsbkq0KhQ9tKK3sElmNaXN1t204Ld3QwUP4mlmeL_3Bh4h58AuAYS8mjMGWV4IzjlTcZUHJAGlVJpJ9XZIklFOR_2YnISwZEwwpSAh16XzHldm6FxPnaWLbo10jr7DMJ6vbmXp03Zdow_U9C0dPrDz9DYCu-jZYTglR9asAp79zAl5md4tyod09nz_WN7M0gYKPaQ1FBlXIBpsLTAjbds0MtcouGlzLaytlWHaMt3aWvLcYlZkQiithaprRBATcrHP3Xj3ucUwVEu39X18WfFcScW1KHSkYE813oXg0VYb362N_6qAVWNR1Z-ioofvPSGy_Tv63-T_Td9sFWk-</recordid><startdate>20221201</startdate><enddate>20221201</enddate><creator>Starchenko, S. V.</creator><creator>Yakovleva, S. V.</creator><general>Pleiades Publishing</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>8FD</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope></search><sort><creationdate>20221201</creationdate><title>Correlation of Time Series of Wolf Numbers and their Derivatives</title><author>Starchenko, S. V. ; Yakovleva, S. V.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c198t-b1962513cedf10a4fdcc478e32ad783ffb5a08f08dfb427fe6963358835bbee13</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><topic>Correlation coefficient</topic><topic>Correlation coefficients</topic><topic>Earth and Environmental Science</topic><topic>Earth Sciences</topic><topic>Fragments</topic><topic>Geophysics/Geodesy</topic><topic>Solar cycle</topic><topic>Sunspot numbers</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Starchenko, S. V.</creatorcontrib><creatorcontrib>Yakovleva, S. V.</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Geomagnetism and Aeronomy</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Starchenko, S. V.</au><au>Yakovleva, S. V.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Correlation of Time Series of Wolf Numbers and their Derivatives</atitle><jtitle>Geomagnetism and Aeronomy</jtitle><stitle>Geomagn. Aeron</stitle><date>2022-12-01</date><risdate>2022</risdate><volume>62</volume><issue>6</issue><spage>685</spage><epage>693</epage><pages>685-693</pages><issn>0016-7932</issn><eissn>1555-645X</eissn><eissn>0016-7940</eissn><abstract>The results of the study of the correlation of the mean annual Wolf numbers
W
and their time derivatives
W
' for time shifts of fragments of series
W
and
W
' relative to each other are presented. The most significant (up to 0.88 and –0.85) correlation and anticorrelation coefficients are obtained with shifts of 2 or 3 years for fragments covering two 11-year cycles. For longer fragments, the coefficients remain significant (at levels of approximately ±0.8) at the same shifts. Therefore, the phase shift between
W
and
W
' is approximately one-quarter of the solar cycle, which physically corresponds to the predominant connection of spots with magnetic energy. At the same time, there is also a significant shift by 8–9 years, which corresponds to correlation coefficients at levels of approximately ±0.75 associated with the magnetic energy variability. The prognostic potentials of the obtained correlation dependences are discussed.</abstract><cop>Moscow</cop><pub>Pleiades Publishing</pub><doi>10.1134/S0016793222050164</doi><tpages>9</tpages></addata></record> |
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identifier | ISSN: 0016-7932 |
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source | Springer Nature |
subjects | Correlation coefficient Correlation coefficients Earth and Environmental Science Earth Sciences Fragments Geophysics/Geodesy Solar cycle Sunspot numbers |
title | Correlation of Time Series of Wolf Numbers and their Derivatives |
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