Holocene variability of atmospheric dust and mercury in the southern hemisphere

The Southern westerly winds (SWW) play an important role in regulating Southern Ocean carbon budget by enhancing the absorbance of atmospheric CO2 or resurfacing deep ocean carbon. Changes in SWW intensity are thought to determine whether Southern Ocean acts as a net CO2 sink or source, thereby affe...

Full description

Bibliographic Details
Main Author: Li, Chuxian
Other Authors: Laboratoire Ecologie Fonctionnelle et Environnement (LEFE), Institut Ecologie et Environnement - CNRS Ecologie et Environnement (INEE-CNRS), Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Centre National de la Recherche Scientifique (CNRS)-Institut National Polytechnique (Toulouse) (Toulouse INP), Université de Toulouse (UT), Université Paul Sabatier - Toulouse III, François De Vleeschouwer, Jeroen Sonke
Format: Doctoral or Postdoctoral Thesis
Language:French
Published: HAL CCSD 2019
Subjects:
Online Access:https://theses.hal.science/tel-03215837
https://theses.hal.science/tel-03215837/document
https://theses.hal.science/tel-03215837/file/2019TOU30277.pdf
id ftmeteofrance:oai:HAL:tel-03215837v1
record_format openpolar
institution Open Polar
collection Météo-France: HAL
op_collection_id ftmeteofrance
language French
topic Southern westerly winds
Holocene
Dust
Mercury
Mercury isotope
Peat
Vents du sud
Holocène
Poussière
Mercure
Isotopique du mercure
Tourbière
[SDU.OCEAN]Sciences of the Universe [physics]/Ocean
Atmosphere
spellingShingle Southern westerly winds
Holocene
Dust
Mercury
Mercury isotope
Peat
Vents du sud
Holocène
Poussière
Mercure
Isotopique du mercure
Tourbière
[SDU.OCEAN]Sciences of the Universe [physics]/Ocean
Atmosphere
Li, Chuxian
Holocene variability of atmospheric dust and mercury in the southern hemisphere
topic_facet Southern westerly winds
Holocene
Dust
Mercury
Mercury isotope
Peat
Vents du sud
Holocène
Poussière
Mercure
Isotopique du mercure
Tourbière
[SDU.OCEAN]Sciences of the Universe [physics]/Ocean
Atmosphere
description The Southern westerly winds (SWW) play an important role in regulating Southern Ocean carbon budget by enhancing the absorbance of atmospheric CO2 or resurfacing deep ocean carbon. Changes in SWW intensity are thought to determine whether Southern Ocean acts as a net CO2 sink or source, thereby affecting atmospheric CO2 concentration and then global climate. SWW also affect Southern Hemisphere (SH) dust trajectory and mercury biogeochemical cycling, which in turn can be used to trace SWW dynamics. Less is known about the past SWW variabilities and historical mercury cycle. The aim of this PhD study is to improve our understanding of the SWW trend and mercury deposition in the Holocene at remote SH sites by using geochemical and isotopic proxies in peat archives. We investigated Amsterdam Island (AMS) peat record coupled with three other peatlands in the SH mid latitudes as long-term archives of atmospheric dust and/or mercury deposition. At the northern edge of SWW and free from anthropogenic disturbance, AMS is a key site to study SWW dynamics. We find that during the Holocene, dust and mercury deposition at AMS oscillated on millennial time scales. Mercury isotope signatures, which are sensitive to rainfall inputs, indicate that high dust, high mercury events correspond to low rainfall. We suggest that these events were caused by a poleward shift of the SWW at AMS. The peat mercury records also inform on recent, human perturbation of the natural mercury cycle in the SH. We find however that the 4-fold anthropogenic mercury enrichment we observe in the SH since 1450AD, is smaller than the 16-fold enrichment in the northern hemisphere. These scientific contributions should help improve global climate models and international environmental policy under the Minamata convention on mercury. Les vents de sud-ouest (VSO) de l'hémisphère sud (HS) régularisent les cycles biogéochimiques du carbone de l'océan Austral en augmentant l'absorption du CO2 atmosphérique ou en faisant remonter les éléments nutritifs et le ...
author2 Laboratoire Ecologie Fonctionnelle et Environnement (LEFE)
Institut Ecologie et Environnement - CNRS Ecologie et Environnement (INEE-CNRS)
Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université Toulouse III - Paul Sabatier (UT3)
Université de Toulouse (UT)-Université de Toulouse (UT)-Observatoire Midi-Pyrénées (OMP)
Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3)
Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Centre National de la Recherche Scientifique (CNRS)-Institut National Polytechnique (Toulouse) (Toulouse INP)
Université de Toulouse (UT)
Université Paul Sabatier - Toulouse III
François De Vleeschouwer
Jeroen Sonke
format Doctoral or Postdoctoral Thesis
author Li, Chuxian
author_facet Li, Chuxian
author_sort Li, Chuxian
title Holocene variability of atmospheric dust and mercury in the southern hemisphere
title_short Holocene variability of atmospheric dust and mercury in the southern hemisphere
title_full Holocene variability of atmospheric dust and mercury in the southern hemisphere
title_fullStr Holocene variability of atmospheric dust and mercury in the southern hemisphere
title_full_unstemmed Holocene variability of atmospheric dust and mercury in the southern hemisphere
title_sort holocene variability of atmospheric dust and mercury in the southern hemisphere
publisher HAL CCSD
publishDate 2019
url https://theses.hal.science/tel-03215837
https://theses.hal.science/tel-03215837/document
https://theses.hal.science/tel-03215837/file/2019TOU30277.pdf
geographic Austral
Southern Ocean
geographic_facet Austral
Southern Ocean
genre Amsterdam Island
Southern Ocean
genre_facet Amsterdam Island
Southern Ocean
op_source https://theses.hal.science/tel-03215837
Océan, Atmosphère. Université Paul Sabatier - Toulouse III, 2019. Français. ⟨NNT : 2019TOU30277⟩
op_relation NNT: 2019TOU30277
tel-03215837
https://theses.hal.science/tel-03215837
https://theses.hal.science/tel-03215837/document
https://theses.hal.science/tel-03215837/file/2019TOU30277.pdf
op_rights info:eu-repo/semantics/OpenAccess
_version_ 1798837530468024320
spelling ftmeteofrance:oai:HAL:tel-03215837v1 2024-05-12T07:52:44+00:00 Holocene variability of atmospheric dust and mercury in the southern hemisphere Variabilité Holocène des poussières atmosphériques et du mercure dans l’hémisphère Sud Li, Chuxian Laboratoire Ecologie Fonctionnelle et Environnement (LEFE) Institut Ecologie et Environnement - CNRS Ecologie et Environnement (INEE-CNRS) Centre National de la Recherche Scientifique (CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université Toulouse III - Paul Sabatier (UT3) Université de Toulouse (UT)-Université de Toulouse (UT)-Observatoire Midi-Pyrénées (OMP) Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3) Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France-Centre National de la Recherche Scientifique (CNRS)-Institut National Polytechnique (Toulouse) (Toulouse INP) Université de Toulouse (UT) Université Paul Sabatier - Toulouse III François De Vleeschouwer Jeroen Sonke 2019-09-17 https://theses.hal.science/tel-03215837 https://theses.hal.science/tel-03215837/document https://theses.hal.science/tel-03215837/file/2019TOU30277.pdf fr fre HAL CCSD NNT: 2019TOU30277 tel-03215837 https://theses.hal.science/tel-03215837 https://theses.hal.science/tel-03215837/document https://theses.hal.science/tel-03215837/file/2019TOU30277.pdf info:eu-repo/semantics/OpenAccess https://theses.hal.science/tel-03215837 Océan, Atmosphère. Université Paul Sabatier - Toulouse III, 2019. Français. ⟨NNT : 2019TOU30277⟩ Southern westerly winds Holocene Dust Mercury Mercury isotope Peat Vents du sud Holocène Poussière Mercure Isotopique du mercure Tourbière [SDU.OCEAN]Sciences of the Universe [physics]/Ocean Atmosphere info:eu-repo/semantics/doctoralThesis Theses 2019 ftmeteofrance 2024-04-18T00:26:46Z The Southern westerly winds (SWW) play an important role in regulating Southern Ocean carbon budget by enhancing the absorbance of atmospheric CO2 or resurfacing deep ocean carbon. Changes in SWW intensity are thought to determine whether Southern Ocean acts as a net CO2 sink or source, thereby affecting atmospheric CO2 concentration and then global climate. SWW also affect Southern Hemisphere (SH) dust trajectory and mercury biogeochemical cycling, which in turn can be used to trace SWW dynamics. Less is known about the past SWW variabilities and historical mercury cycle. The aim of this PhD study is to improve our understanding of the SWW trend and mercury deposition in the Holocene at remote SH sites by using geochemical and isotopic proxies in peat archives. We investigated Amsterdam Island (AMS) peat record coupled with three other peatlands in the SH mid latitudes as long-term archives of atmospheric dust and/or mercury deposition. At the northern edge of SWW and free from anthropogenic disturbance, AMS is a key site to study SWW dynamics. We find that during the Holocene, dust and mercury deposition at AMS oscillated on millennial time scales. Mercury isotope signatures, which are sensitive to rainfall inputs, indicate that high dust, high mercury events correspond to low rainfall. We suggest that these events were caused by a poleward shift of the SWW at AMS. The peat mercury records also inform on recent, human perturbation of the natural mercury cycle in the SH. We find however that the 4-fold anthropogenic mercury enrichment we observe in the SH since 1450AD, is smaller than the 16-fold enrichment in the northern hemisphere. These scientific contributions should help improve global climate models and international environmental policy under the Minamata convention on mercury. Les vents de sud-ouest (VSO) de l'hémisphère sud (HS) régularisent les cycles biogéochimiques du carbone de l'océan Austral en augmentant l'absorption du CO2 atmosphérique ou en faisant remonter les éléments nutritifs et le ... Doctoral or Postdoctoral Thesis Amsterdam Island Southern Ocean Météo-France: HAL Austral Southern Ocean