Reconstruction of grand minima of solar activity from radiocarbon data : linear and nonlinear signal analysis
- Using a special technique of data analysis, we have found out 34 grand minima of solar activity in a 7,700 years long C14 record. The method used rests on a proper filtering of the C14 record and the extrapolation of verifiable results for the later history back in time. Additionally, we have applied a method of nonlinear dynamics, the recurrence rate, to back up the results. Our findings are not contradictory to the record of grand minima by Eddy, but constitute a considerable extension. Hence, it has become possible to look closer at the validity of models. This way, we have tested esp. the model of Barnes et al. There are hints for that the grand minima might solely be driven by the 209--year period found in the C14 record.
| Verfasserangaben: | Henning U. Voss, Jürgen KurthsORCiDGND, Udo Schwarz |
|---|---|
| URL: | http://www.agnld.uni-potsdam.de/~shw/Paper/vks.ps.gz |
| Publikationstyp: | Wissenschaftlicher Artikel |
| Sprache: | Englisch |
| Jahr der Erstveröffentlichung: | 1996 |
| Erscheinungsjahr: | 1996 |
| Datum der Freischaltung: | 25.03.2017 |
| Quelle: | Journal of Geophysical Research : A, Space Physics. - 101 (1996), S. 15637 - 15643 |
| Organisationseinheiten: | Zentrale und wissenschaftliche Einrichtungen / Interdisziplinäres Zentrum für Dynamik komplexer Systeme |
| Name der Einrichtung zum Zeitpunkt der Publikation: | Zentrale und wissenschaftliche Einrichtungen / Interdisziplinäres Zentrum für Nichtlineare Dynamik |
