Tous les articles par Célia Eschstruth

Le raid scientifique EAIIST est parti de Concordia

Après quelques jours à Concordia pour les derniers réglages des instruments, le raid EAIIST est parti samedi en direction de Pole Sud, vers les zones de megadunes. Mathieu a fait le voyage de 10 jours entre Cap Prudhomme et Concordia pour vérifier que tout se passe bien avec l’instrument de mesure de la composition isotopique de la vapeur d’eau en continu sur le raid. Il a effectué quelques calibrations à Concordia et il reste à Concordia pour d’autres expériences scientifiques.

Installation de l’instrument de mesure de la composition isotopique de la vapeur d’eau dans la caravane scientifique
Le raid en route

Assessing the robustness of Antarctic temperature reconstructions over the past 2 millennia using pseudoproxy and data assimilation

The Antarctic temperature changes over the past millennia remain more uncertain than in many other continental regions. This has several origins: (1) the number of high-resolution ice cores is small, in particular on the East Antarctic plateau and in some coastal areas in East Antarctica; (2) the short and spatially sparse instrumental records limit the calibration period for reconstructions and the assessment of the methodologies; (3) the link between isotope records from ice cores and local climate is usually complex and dependent on the spatial scales and timescales investigated. Here, we use climate model results, pseudoproxy experiments and data assimilation experiments to assess the potential for reconstructing the Antarctic temperature over the last 2 millennia based on a new database of stable oxygen isotopes in ice cores compiled in the framework of Antarctica2k (Stenni et al.2017).

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Limited increase in tropospheric ozone since 1850 C.E

Tropospheric ozone (O3) is key component of air pollution and an important anthropogenic greenhouse gas. During the 20th century, proliferation of the internal combustion engine, rapid industrialization, and land-use change led to a global-scale increase in its concentrations, but the magnitude of this increase is not known. Atmospheric chemistry models typically predict an increase in the tropospheric O3 burden of less than 50% since 1900,1,2 while direct measurements made in the late 19th century imply that surface O3 mixing ratios increased by much more, up to 300%3-5.

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Estimation of the Antarctic surface mass balance using the regional climate model MAR (1979–2015) and identification of dominant processes

The Antarctic ice sheet mass balance is a major component of the sea level budget and results from the difference of two fluxes of a similar magnitude: ice flow discharging in the ocean and net snow accumulation on the ice sheet surface, i.e. the surface mass balance (SMB). Separately modelling ice dynamics and SMB is the only way to project future trends. In addition, mass balance studies frequently use regional climate models (RCMs) outputs as an alternative to observed fields because SMB observations are particularly scarce on the ice sheet.

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Prochaine saison en Antarctique Novembre 2019 – Janvier 2020

Aymeric Antoine et Mathieu partiront pour l’Antarctique de novembre à janvier.

Aymeric s’occupera de la calibration et de l’entretien de l’instrument de de mesure en continu de la composition isotopique de la vapeur installé sur le site de Dumont d’Urville en 2018-2019

Antoine fera de la découpe de glace de la carotte EPICA Dôme C stockée dans la cave de stockage (-50°C) de la station Concordia et mesurera ensuite ces échantillons dans le cadre de sa thèse qui débute en Octobre 2019

Quant à Mathieu, il installera un premier instrument de mesure en continu de la composition isotopique de la vapeur sur le raid EAIIST puis un deuxième instrument de mesure de la composition isotopique de la vapeur sur le site de Concordia (premier instrument installé en 2018-2019). Aussi prélèvera t-il des échantillons de surface et de subsurface

Unveiling the anatomy of Termination 3 using water and air isotopes in the Dome C ice core, East Antarctica

Each glacial – interglacial transition of the Quaternary occurs in a different orbital context leading to various timing for the deglaciation and sequence of high vs low latitudes events. Termination 3, 250 kiloyears before present (ka), is an unusual deglaciation in the context of the last 9 deglaciations recorded in the old EPICA Dome C (EDC) Antarctic ice core: it exhibits a three–phase sequence, two warming phases separated by a small cooling, the last phase suggesting a particularly rapid temperature increase. We present here new high resolution d15N and deuterium excess (d–excess) data from the EDC ice core to provide a detailed temperature change estimate during this termination. Then, we combined the dD and d18O to discuss the relationship between high and low latitude changes through the d-excess. We also provide the high vs low latitude sequence of events over this deglaciation without chronological uncertainty using low latitude ice core proxies. In agreement with previous studies based on speleothem analyses, we show that the first phase of Termination 3 (256 to 249 ka) is associated with small Heinrich like events linked to changes in ITCZ position, monsoon activity and teleconnections with Antarctica. In a context of minimum Northern Hemisphere insolation, this leads to a rather strong Antarctic warming, as observed in the d15N record in contrast to the relatively small dD increase. The second warming phase occurs during the rise of the Northern hemisphere insolation, with a large Heinrich like event leading to the characteristic Antarctic warming observed in the d15N and dD increase as for the more recent terminations.

Figure: Millennial variability during the Terminations 3.a: EDC dD record. b: measured EDC d15N. c: EDC DTsite (dark green) and DTsource (green) reconstructions. d: EDC CH4. e: d18Ocalcite from East Asian speleothems in red and EDC d18Oatm in yellow. f: IRD percentage from site ODP980 in black and June 21st insolation at 65°N in grey. g: d18Oplanktonic of core MD97-2120.

Auteurs : C. Bréant, A. Landais, A. Orsi, P. Martinerie, T. Extier, F. Prié, V. Masson-Delmotte, J. Jouzel, M. Leuenberger

Ref. : Quaternary Science Reviews, 211, 156-165, 2019

Projet/financement: ERC Combiniso, LEFE NEVE/CLIMAT

 

Coastal water vapor isotopic composition driven by katabatic wind variability in summer at Dumont d’Urville, coastal East Antarctica

Dumont d’Urville station, located on the East coast of Antarctica in Adélie Land, is in one of the windiest coastal region on Earth, due to katabatic winds downslope from the East Antarctic ice sheet. In summer, the season of interest in this study, coastal weather is characterized by well-marked diel cycles in temperature and wind patterns.

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Estimation of the Antarctic surface mass balance using the regional climate model MAR (1979–2015) and identification of dominant processes

The Antarctic ice sheet mass balance is a major component of the sea level budget and results from the difference of two fluxes of a similar magnitude: ice flow discharging in the ocean and net snow accumulation on the ice sheet surface, i.e. the surface mass balance (SMB). Separately modelling ice dynamics and SMB is the only way to project future trends.

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Le logement à Dome C (message d’Amaëlle)

Nous sommes maintenant plus de 80 personnes sur la station. Heureusement, il y a plusieurs bâtiments qui ont été construits au fil du temps et qui permettent d’accueillir tout le monde.

D’abord, la première caravane amenée lors de la création de la station dans les années 1990 peut accueillir 6 personnes. Ensuite, le camp d’été a été construit et il a accueilli pendant plus de 10 ans les quelques dizaines de personnes qui ont assuré la logistique (médecin, cuisinier, chauffagiste, électricien, plombier), les expériences scientifiques et la construction des deux tours de la station permanente jusqu’à son ouverture en 2005 pour le premier hivernage. 20 personnes peuvent y être logées par chambre de deux. 4 tentes montées à la même époque permettent de loger 6 personnes chacune. Enfin, il reste 32 places par chambre de deux dans la tour calme de la station. Quand la traverse arrive, les conducteurs dorment dans leur caravane. Quant aux pilotes d’avion qui doivent rester parfois plusieurs nuits entre deux vols, ils installent des matelas dans la salle vidéo de la station permanente.

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