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Titre du document / Document title

Can origin of the 2400-year cycle of solar activity be caused by solar inertial motion?

Auteur(s) / Author(s)

CHARVATOVA I. (1) ;

Affiliation(s) du ou des auteurs / Author(s) Affiliation(s)

(1) Geophysical Institute AS CR, Boční II, 141 31 Praha, TCHEQUE, REPUBLIQUE

Résumé / Abstract

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 x 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.

Revue / Journal Title

Annales geophysicae    ISSN  0992-7689 

Source / Source

2000, vol. 18, no4, pp. 399-405 (35 ref.)

Langue / Language

Anglais

Editeur / Publisher

Copernicus, Göttingen, ALLEMAGNE  (1988) (Revue)

Mots-clés anglais / English Keywords

Solar activity

;

Solar cycle

;

Carbon 14

;

Tree rings

;

Mots-clés français / French Keywords

Activité solaire

;

Cycle solaire

;

Carbone 14

;

Cerne bois

;

Localisation / Location

INIST-CNRS, Cote INIST : 19920, 35400008838691.0010

Nº notice refdoc (ud4) : 1355096



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