Резюме
Было усmaновлено, чmо ¶rt;вuженuе Солнцa вокре
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ценmрa mяжесmu солнечноŭ сuсmемы сосmоum uз ¶rt;вух основных, nеременно nовmоряющuхся элеменmов — uз nеmлu u uз aркu. Двuженuе Солнцa в кaж¶rt;ом uз эmuх злеменmов ¶rt;лumся в сре¶rt;нем 9.93
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о¶rt;a. В рaбоmе былa усmaновленa связь меж¶rt;у ¶rt;вuженuем Солнцa u колебaнuем солнечноŭ aкmuвносmu: нa основе оmклоненuŭ оm nоря¶rt;кaЮnumер—Сamурн былa обнaруженa nрuблuзumельно maкaя же нерuо¶rt;uчносmь в ¶rt;вuженuu Солнцa в nре¶rt;eлaх 60–2200 леm, кaк u в солнечноŭ aкmuвносmu, a в mеченuе uнmервaлa ¶rt;лumельносmью 3100 леm было нaŭ¶rt;ено nолное совna¶rt;енuе ¶rt;ол
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овременных мuнuмумов солнечноŭ aкmuвносmu с nерuо¶rt;aмu мaксцuмaльных оmклоненuŭ оm nоря¶rt;кa Ю—С u нaобороm.
Summary
The Sun's motion round the barycentre of the solar system was found to consist of two basic alternately repeating elements of the noose and of the arc. The mean time for solar motion around each of these elements was found to be 9.93 yr. The relation between solar motion and solar variability was determined as follows: Approximately coincident periodicities ranging from 60 to 2200 yr were traced in both phenomena and a coincidence of all prolonged minima in solar activity with the epochs of the highest deviations from the Jupiter—Saturn order was found over a time interval of 3100 yr.
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Charvátová, I. On the relation between solar motion and the long term variability of solar activity. Stud Geophys Geod 33, 230–241 (1989). https://doi.org/10.1007/BF01633526
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DOI: https://doi.org/10.1007/BF01633526