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Ellis L.T., Alegro A., Šegota, Bakalin V.A., Barone R., Borovichev E.A., Hugonnot V., Lebouvier M., Nobis M., Nowak A., Ochyra R., Papp B., Szurdoki E., Piwowarczyk R., Plášek V., Číhal L., Ren Z.J., Sabovljević M.S., Sérgio S., Garcia C.A., Melo I., Sawicki J., Stebel A., Ştefănuţ S., Ion R., Manole A., Tzioptzis I., Xiong Y., Zhao Z.-T. (2015). New national and regional bryophyte records, 44. J. Bryol., 37, 228–242.
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Hejun Zhu, Ebru Bozda, and Jeroen Tromp. (2015). Seismic structure of the European upper mantle based on adjoint tomography. Geophys J Int, 201(1), 18–52.
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C.P. Legendre, L. Zhao and Q.-F. Chen. (2015). Upper-mantle shear-wave structure under East and Southeast Asia from Automated Multimode Inversion of waveforms. Geophys J Int, 203(1), 707–719 .
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Viblanc V. A., Saraux C., Smith A. D., Gineste B., Robin J. P. et R. Groscolas . (2015). Quantifying seabird disturbance in the wild: physiological and behavioral measures in breeding king penguin. 2th World Seabird Conference. Cape Town (Afrique du Sud), 26-30 Octobre..
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Stier A., Viblanc V. A., de Margerie E., Zahn S., Handrich Y., de Buffrénil V., Erbrech A., Guérin N., Martrette J. M., Groscolas R., Criscuolo F., Bize P. et J. P. Robin . (2015). How do adults and chicks of king penguins (Aptenodytes patagonicus) face nutritional constraints while breeding or growing? 1st Congress of Physiology and Integrative Biology (CPBI) and 84th Congress of French Physiological Society (SFP). Strasbourg (France), 4-6 Mai. Acta Physiologica 214, Supplément S700: pp87..
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Merieme Chadid . (2015). A new way to study the stellar pulsation; First Polar mission PAIX (Vol. SF2A-2015: Proceedings of the Annual meeting of th).
Abstract: In the context of long and continuous time–series photometry and after the MOST, CoRoT, KEPLER space missions and large geographic longitude ground–based networks, a new method is offered by the polar location helping to cope with the problem associated with the Earth’s day–night cycle. In this talk, we present the first long time–series photometry from the heart of Antarctica -Dome Charlie- and we discuss briefly our new results and perspective on the pulsating stars from Antarctica, especially the connection between temporal hydrodynamic phenomena and cyclic modulations. Finally, we highlight the impact of PAIX -the robotic Antarctica photometer- on the stellar pulsation study.
Programme: 1096
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Hennion F., Labarrere B., Prinzing A., Siljak-Yakovlev S., Robert T., Lamy F., Nadot S., Colas B., D’hont A. (2015). PLANTEVOL : Biodiversité des plantes dans les îles subantarctiques: évolution, passé, et avenir dans des environnements changeants. 3ème Colloque Biennal des Zones Atelier du CNRS, 14 – 16 octobre, CNRS Campus Michel-Ange, Paris, France..
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Maupin, V., and J. Park. (2015). Theory and Observations-Seismic Anisotropy. (Vol. 1.09).
Abstract: Treatise on Geophysics
Programme: 133
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Labarrere B., Prinzing A., Renaudon M. & Hennion F. (2015). Influence of phenotypic integration on plant plasticity. 1ère réunion du GDR PlasPhen, 4 et 5 novembre, Paris, France..
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Meijian An, Douglas A. Wiens, Yue Zhao, Mei Feng, Andrew Nyblade, Masaki Kanao, Yuansheng Li, Alessia Maggi, and Jean-Jacques Lévêque. (2015). S-velocity model and inferred Moho topography beneath the Antarctic Plate from Rayleigh waves. J. Geophys. Res., 120, 8720–8742.
Abstract: Since 2007/2008, seismographs were deployed in many new locations across much of Antarctica. Using the records from 122 broadband seismic stations, over 10,000 Rayleigh wave fundamental-mode dispersion curves have been retrieved from earthquake waveforms and from ambient noise. Using the processed data set, a 3-D S-velocity model for the Antarctic lithosphere was constructed using a single-step surface wave tomographic method, and a Moho depth map was estimated from the model. Using the derived crustal thicknesses, the average ratio of lithospheric mantle and crustal densities of Antarctica was calculated. The calculated density ratio indicates that the average crustal density for Antarctica is much higher than the average values for continental crust or the average density of lithospheric mantle is so low as to be equal to low-density bound of Archean lithosphere. The latter implies that the lithospheric mantle in much of Antarctica should be old and of Archean age. The East Antarctic Mountain Ranges (EAMOR) represent a thick crustal belt, with the thickest crust (~60 km) located close to Dome A. Very high velocities can be found at depths greater than 200 km beneath parts of East Antarctica, demonstrating that the continental lithosphere extends deeper than 200 km. The very thick crust beneath the EAMOR may represent the collision suture of East Gondwana with Indo-Antarctica and West Gondwana during the Pan-African orogeny.
Programme: 133
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