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Taking the pulse of the Sun during the Holocene by joint analysis of 14 C and 10 Be
Author(s) -
Knudsen Mads Faurschou,
Riisager Peter,
Jacobsen Bo Holm,
Muscheler Raimund,
Snowball Ian,
Seidenkrantz MaritSolveig
Publication year - 2009
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/2009gl039439
Subject(s) - holocene , amplitude , spectral line , geology , dipole , spectral analysis , cosmogenic nuclide , joint (building) , astrophysics , climatology , physics , atmospheric sciences , astronomy , paleontology , spectroscopy , optics , architectural engineering , engineering , quantum mechanics , cosmic ray
We have studied solar variations during the Holocene (i.e., last ∼11,700 yr) by combining a new model of the Earth's dipole moment with 14 C data from the IntCal04 record and 10 Be data from the GRIP ice core. Joint spectral analysis of the two nuclide records suggests that the periodic behavior of the Sun was particularly pronounced between 6000–4500 yr BP and 3000–2000 yr BP, with dominating periodicities of ∼88, ∼150, ∼220, and ∼400 years, while this rhythmic behavior faded during other time intervals. The fact that the two reconstructions, based on radionuclides with distinct geochemical properties, agree with respect to both the frequency and timing of the periodic behavior, strongly suggests that they reflect the actual behavior of the Sun. Subtle but systematic differences between the amplitude spectra may point to an interplay between the climate system and the ∼220‐ and ∼400‐year solar cycles during intervals when these were particularly prominent.