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| Titel |
Can origin of the 2400-year cycle of solar activity be caused by solar inertial motion? |
| VerfasserIn |
I. Charvátová |
| Medientyp |
Artikel
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| Sprache |
Englisch
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| ISSN |
0992-7689
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| Digitales Dokument |
URL |
| Erschienen |
In: Annales Geophysicae ; 18, no. 4 ; Nr. 18, no. 4, S.399-405 |
| Datensatznummer |
250013950
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| Publikation (Nr.) |
 copernicus.org/angeo-18-399-2000.pdf |
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| Zusammenfassung |
A solar activity cycle of about 2400 years
has until now been of uncertain origin. Recent results indicate it is caused by
solar inertial motion. First we describe the 178.7-year basic cycle of solar
motion. The longer cycle, over an 8000 year interval, is found to average 2402.2
years. This corresponds to the Jupiter/Heliocentre/Barycentre alignments (9.8855
× 243). Within each cycle an exceptional segment of 370 years has been found
characterized by a looping pattern by a trefoil or quasitrefoil geometry. Solar
activity, evidenced by 14C tree-ring proxies, shows the same pattern.
Solar motion is computable in advance, so this provides a basis for future
predictive assessments. The next 370-year segment will occur between AD 2240 and
2610.
Key words: Solar physics (celestial mechanics) |
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