Quantitative impact of astronomical and sun-related cycles on the Pleistocene climate system from Antarctica records

We use the benefits of the full-resolution methodology for time-series decomposition singular spectrum analysis to assess the quantitative impact of orbital and, for the first time, millennial-scale Sun-related climate responses from EPICA records. The quantitative impact of the three Sun-related cy...

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Main Author: Paolo Viaggi
Format: Article
Language:English
Published: Elsevier 2021-10-01
Series:Quaternary Science Advances
Subjects:
Online Access:http://www.sciencedirect.com/science/article/pii/S2666033421000162
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spelling doaj-c3699c6ad5494079a2eacdce6e10fb542021-07-05T04:14:44ZengElsevierQuaternary Science Advances2666-03342021-10-014100037Quantitative impact of astronomical and sun-related cycles on the Pleistocene climate system from Antarctica recordsPaolo Viaggi0Museo Geologico Giovanni Capellini, Bologna University, Via Zamboni 63, I-40126, Bologna, ItalyWe use the benefits of the full-resolution methodology for time-series decomposition singular spectrum analysis to assess the quantitative impact of orbital and, for the first time, millennial-scale Sun-related climate responses from EPICA records. The quantitative impact of the three Sun-related cycles (unnamed ~9.7-kyr; proposed ‘Heinrich-Bond’ ~6.0-kyr; Hallstatt ~2.5-kyr), cumulatively explain ~4.0% (δD), 2.9% (CO2), and 6.6% (CH4) in variance, demonstrating for the first time the minor role of solar activity in the regional budget of Earth's climate forcing. A cycle of ~3.6 kyr, which is little known in literature, results in a mean variance of 0.6% only, does not seem to be Sun-related, although a gravitational origin cannot be ruled out. According to the recurrence analysis of Heinrich events (6.03 ± 1.4 kyr) and their correlation with EPICA stack ~6.0-kyr cycle, it is proposed that this band of solar activity be named the ‘Heinrich-Bond cycle’. On these basis, it is deemed that the ‘Heinrich-Bond’ solar cycle may act on the ice-sheet as an external instability factor both related to excess ice leading to calving process and IRD-layers (‘cold-related’ Heinrich events), and surface heating with meltwater streams (‘warm-related’ Heinrich events). The Hallstatt cycle is found in a number of solar proxies, geomagnetic secular variations, paleoclimatic oscillations, combination tones of Milankovitch forcings and resonant planetary beats, indicating an apparent ‘multi-forcing’ origin possibly related to planetary beat hypothesis. The orbital components consistently reflects the post-Mid-Pleistocene transition nature of the EPICA records in which the short eccentricity results in most of the variance (51.6%), followed by obliquity (19.0%) and precession (8.4%). Beyond the Milankovitch theory, evidence is emerging of a multiple-forcing cosmoclimatic system with stochastic interactions between external (gravitational resonances, orbitals, solar activity) and Earth's internal (geodynamics, atmosphere composition, feedback mechanisms) climate components, each having a strong difference in terms of the relative quantitative impact on Earth's climate.http://www.sciencedirect.com/science/article/pii/S2666033421000162Quantitative impactPlanetary beat hypothesisSingular spectrum analysisSolar cyclesHeinrich-bondHallstatt
collection DOAJ
language English
format Article
sources DOAJ
author Paolo Viaggi
spellingShingle Paolo Viaggi
Quantitative impact of astronomical and sun-related cycles on the Pleistocene climate system from Antarctica records
Quaternary Science Advances
Quantitative impact
Planetary beat hypothesis
Singular spectrum analysis
Solar cycles
Heinrich-bond
Hallstatt
author_facet Paolo Viaggi
author_sort Paolo Viaggi
title Quantitative impact of astronomical and sun-related cycles on the Pleistocene climate system from Antarctica records
title_short Quantitative impact of astronomical and sun-related cycles on the Pleistocene climate system from Antarctica records
title_full Quantitative impact of astronomical and sun-related cycles on the Pleistocene climate system from Antarctica records
title_fullStr Quantitative impact of astronomical and sun-related cycles on the Pleistocene climate system from Antarctica records
title_full_unstemmed Quantitative impact of astronomical and sun-related cycles on the Pleistocene climate system from Antarctica records
title_sort quantitative impact of astronomical and sun-related cycles on the pleistocene climate system from antarctica records
publisher Elsevier
series Quaternary Science Advances
issn 2666-0334
publishDate 2021-10-01
description We use the benefits of the full-resolution methodology for time-series decomposition singular spectrum analysis to assess the quantitative impact of orbital and, for the first time, millennial-scale Sun-related climate responses from EPICA records. The quantitative impact of the three Sun-related cycles (unnamed ~9.7-kyr; proposed ‘Heinrich-Bond’ ~6.0-kyr; Hallstatt ~2.5-kyr), cumulatively explain ~4.0% (δD), 2.9% (CO2), and 6.6% (CH4) in variance, demonstrating for the first time the minor role of solar activity in the regional budget of Earth's climate forcing. A cycle of ~3.6 kyr, which is little known in literature, results in a mean variance of 0.6% only, does not seem to be Sun-related, although a gravitational origin cannot be ruled out. According to the recurrence analysis of Heinrich events (6.03 ± 1.4 kyr) and their correlation with EPICA stack ~6.0-kyr cycle, it is proposed that this band of solar activity be named the ‘Heinrich-Bond cycle’. On these basis, it is deemed that the ‘Heinrich-Bond’ solar cycle may act on the ice-sheet as an external instability factor both related to excess ice leading to calving process and IRD-layers (‘cold-related’ Heinrich events), and surface heating with meltwater streams (‘warm-related’ Heinrich events). The Hallstatt cycle is found in a number of solar proxies, geomagnetic secular variations, paleoclimatic oscillations, combination tones of Milankovitch forcings and resonant planetary beats, indicating an apparent ‘multi-forcing’ origin possibly related to planetary beat hypothesis. The orbital components consistently reflects the post-Mid-Pleistocene transition nature of the EPICA records in which the short eccentricity results in most of the variance (51.6%), followed by obliquity (19.0%) and precession (8.4%). Beyond the Milankovitch theory, evidence is emerging of a multiple-forcing cosmoclimatic system with stochastic interactions between external (gravitational resonances, orbitals, solar activity) and Earth's internal (geodynamics, atmosphere composition, feedback mechanisms) climate components, each having a strong difference in terms of the relative quantitative impact on Earth's climate.
topic Quantitative impact
Planetary beat hypothesis
Singular spectrum analysis
Solar cycles
Heinrich-bond
Hallstatt
url http://www.sciencedirect.com/science/article/pii/S2666033421000162
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