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Lecointre G. & Ozouf-Costaz C. (2004). Pour la science, 320, 56–61.
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Rousseau D.D., Schevin P., Duzer D., Jolly D., Cambon G. & Ferrier J. (2005). Long distance pollen transport to southern Greenland: Is there a regular pattern? Biogeosciences discussions, 2, 829–847.
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Mercier D. (2003).4, 407–416.
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Roussel E. (2005). Norois, 194, 85–96.
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. (2003).3, 177–190.
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. (2008). Applied comparisons between SCHA and R-SCHA regional modeling techniques. Geochem. Geophys. Geosyst., 9.
Keywords: regional modeling; SCHA; R-SCHA; 1517 Geomagnetism and Paleomagnetism: Magnetic anomalies: modeling and interpretation; 1541 Geomagnetism and Paleomagnetism: Satellite magnetics: main field, crustal field, external field
Programme: 139
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Lang M., Glasmacher U., Moine B.N., Neumann R. & Wagner G.A. (2004). Etch-pit morphology of tracks caused by swift heavy ions in natural dark mica. Nuclear instruments and methods in physics research b, 218, 466–471.
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Bost C.A. & Weimerskirch H. (2005). Le courrier de la nature, 220, 30–38.
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Agabi, A.; Aristidi, E.; Azouit, M.; Fossat, E.; Martin, F.; Sadibekova, T.; Vernin, J.; Ziad, A. (2006). First Whole Atmosphere Nighttime Seeing Measurements at Dome C, Antarctica. Publ. Astron. Soc. Pac., 118(840), 344–348.
Abstract: We report site-testing results obtained in the nighttime during the polar autumn and winter at Dome C. These results were collected during the first Concordia winterover by A. Agabi. They are based on seeing and isoplanatic angle monitoring, as well as in situ balloon measurements of the refractive index structure constant profiles C2n(h). Atmosphere is divided into two regions: (1) a 36 m high surface layer responsible for 87% of the turbulence, and (2) a very stable free atmosphere above, with a median seeing of 0.36“ +/- 0.19” at an elevation of h=30 m. The median seeing measured with a differential image motion monitor placed on top of an 8.5 m high tower is 1.3“ +/- 0.8”.
Keywords: Site Testing
Programme: 908
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Rochette P., Gattacceca J., Eisenlohr P. & Folco L. (2004). In situ magnetic identification and classification of meteorites in Antarctica. Lunar and planetary science, .
Abstract: We present the results of the use of magnetic methods (susceptibility, magnetic anomalies) applied to meteorite identification and partial classification. These methods were successfully tested during a meteorite collection expedition in Antarctica.
Programme: 412
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