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Enstip, M. R.; Daunt, F.; Wanless, S.; Humphreys, E. M.; Hamer, K. C.; Benvenuti, S.; Gremillet, D. (2006). Foraging energetics of North Sea birds confronted with fluctuating prey availability.
Abstract: In: Boyd, S.; Wanless, S.; Camphuysen, C.J., (eds.) Top predators in marine ecosystems: their role in monitoring and management. Cambridge, Cambridge University Press
Programme: 388
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Lambotte S. and L. Rivera and J. Hinderer. (2006). Constraining the overall kinematics of the 2004 Sumatra and the 2005 Nias earthquakes using the Earth's gravest free oscillations. Bulletin of the seismological society of america, 97, S128–S138.
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Morin, S.; Marion, G.M.; von Glasow, R.; Voisin, D.; Bouchez, J.; Savarino, J. (2008). Precipitation of salts in freezing seawater and ozone depletion events: a status report. Atmospheric chemistry and physics, 8(23), 7317–7324.
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Zorn, S.R.; Drewnick, F.; Schott, M.; Hoffmann, T.; Borrmann, S. (2008). Characterization of the South Atlantic marine boundary layer aerosol using an aerodyne aerosol mass spectrometer. Atmospheric chemistry and physics, 8(16), 4711–4728.
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David, C.; Keckhut, P.; Armetta, A.; Jumelet, J.; Snels, M.; Marchand, M.; Bekki, S. (2010). Radiosonde stratospheric temperatures at Dumont d'Urville (Antarctica): trends and link with polar stratospheric clouds. ACP, 10(8), 3813–3825.
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Fouillen L., T. Raclot, A. Van Dorsselaer and F. Bertile. (2008). Biodiversity exploration using MS-based proteomics for the improved understanding of extreme physiopathological situation adaptations..
Abstract: Denver, Colorado, USA, June 1 – 5, 2008.
Programme: 137
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. (2011). Polarisation in the auroral red line during coordinated EISCAT Svalbard Radar/optical experiments. ANGEO, 29(6), 1101–1112.
Abstract: The polarisation of the atomic oxygen red line in the Earth's thermosphere is observed in different configurations with respect to the magnetic field line at high latitude during several coordinated Incoherent Scatter radar/optical experiment campaigns. When pointing northward with a line-of-sight nearly perpendicular to the magnetic field, we show that, as expected, the polarisation is due to precipitated electrons with characteristic energies of a few hundreds of electron Volts. When pointing toward the zenith or southward with a line-of-sight more parallel to the magnetic field, we show that the polarisation practically disappears. This confirms experimentally the predictions deduced from the recent discovery of the red line polarisation. We show that the polarisation direction is parallel to the magnetic field line during geomagnetic activity intensification and that these results are in agreement with theoretical work.
Programme: 1026
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Favier V. and C. Genthon. (2009). Rapport de mission glacioclim.
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. (2005).
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Six D., Lemeur E., Genthon C. (2007). Rapport de mission glacioclim.
Abstract: Consultable sur http://www-lgge.obs.ujf-grenoble.fr/~christo/glacioclim/samba/
Programme: 411
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