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Orbital tuning, eccentricity, and the frequency modulation of climatic precession

Huybers, Peter and Aharonson, Oded (2010) Orbital tuning, eccentricity, and the frequency modulation of climatic precession. Paleoceanography, 25 . Art. no. PA4228. ISSN 0883-8305. http://resolver.caltech.edu/CaltechAUTHORS:20110131-102315353

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Abstract

The accuracy of geologic chronologies can, in principle, be improved through orbital tuning, the systematic adjustment of a chronology to bring the associated record into greater alignment with an orbitally derived signal. It would be useful to have a general test for the success of orbital tuning, and one proposal has been that eccentricity ought to covary with the amplitude envelope associated with precession variability recorded in tuned geologic records. A common procedure is to filter a tuned geologic record so as to pass precession period variability and compare the amplitude modulation of the resulting signal against eccentricity. There is a reasonable expectation for such a relationship to be found in paleoclimate records because the amplitude of precession forcing depends upon eccentricity. However, there also exists a relationship between eccentricity and the frequency of precession such that orbital tuning generates eccentricity-like amplitude modulation in filtered signals, regardless of the accuracy of the chronology or the actual presence of precession. This relationship results from the celestial mechanics governing eccentricity and precession and from the interaction between frequency modulation and amplitude modulation caused by filtering. When the eccentricity of Earth's orbit is small, the frequency of climatic precession undergoes large variations and less precession energy is passed through a narrow-band filter. Furthermore, eccentricity-like amplitude modulation is routinely obtained from pure noise records that are orbitally tuned to precession and then filtered. We conclude that the presence of eccentricity-like amplitude modulation in precession-filtered records does not support the accuracy of orbitally tuned time scales.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1029/2010PA001952DOIArticle
ORCID:
AuthorORCID
Aharonson, Oded0000-0001-9930-2495
Additional Information:© 2010 American Geophysical Union. Received 23 February 2010; accepted 23 September 2010; published 23 December 2010. R. Sari (Hebrew University of Jerusalem) provided helpful discussion regarding orbital mechanics; C. Wunsch (MIT) and B. Bills (JPL) gave useful feedback on earlier drafts of this paper; and insightful reviews were provided by L. Lourens (Utrecht University), M. Crucifix (Université catholique de Louvain), and an anonymous reviewer.
Subject Keywords:orbital tuning; precession; eccentricity
Record Number:CaltechAUTHORS:20110131-102315353
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20110131-102315353
Official Citation:Huybers, P., and O. Aharonson (2010), Orbital tuning, eccentricity, and the frequency modulation of climatic precession, Paleoceanography, 25, PA4228, doi:10.1029/2010PA001952
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:21933
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:11 Feb 2011 19:11
Last Modified:27 Apr 2017 21:11

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