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. (2004). AMS measurement of 24Mg(3He,p)26Al cross section, implications for the 26Al production in the early Solar System. Lunar and planetary science, 35, 1586.
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Maurette M., Brack A., Duprat J., Engrand C. & Kurat G. (2004). High input rates of micrometeoritic sulfur, smoke“ particles and oligo-elements on the early Earth.”. Lunar and planetary science, 35, 1625.
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Swain, M.; Lloyd, J.; Traub, W.; Walker, C.; Stark, A.; Lawson, P.; Storey, J.; Coude du Foresto, V.; Fossat, E.; Ireland, M.; Burrows, A.; Vakili, F. (2003). The Antarctic Planet Interferometer. Bulletin of the american astronomical society, 35, 1262.
Abstract: American Astronomical Society Meeting 203, #38.15;
Programme: 908
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JOLY D., NILSEN L., ELVEBAKK A., BROSSARD T.,. (2006).35, 255–270.
Abstract: Climate change is a key issue, especially in the Arctic. However, this general observation is not sufficient to determine the consequences of this phenomenon since the impact of climate change varies with geographical position and local conditions in different environmental contexts. The study area is located at 79?N, in Kongsfjorden (Svalbard). Botanical observations and temperature measurements, remote sensing and topographical indices are input into a Geographical Information System. These GIS layers are then computed to provide variables that can give a statistical explanation of the temperature and vegetation distribution at high resolution.
Keywords: arctic; bioclimatology; interpolation; spatial modelling
Programme: 304
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Spracklen, D.V.; Arnold, S.R.; Sciare, J.; Carslaw, K.S.; Pio, C. (2008). Globally significant oceanic source of organic carbon aerosol. Geophysical research letters, 35.
Keywords: organic carbon; ocean; aerosol; 0305 Atmospheric Composition and Structure: Aerosols and particles; 0315 Atmospheric Composition and Structure: Biosphere/atmosphere interactions; 0312 Atmospheric Composition and Structure: Air/sea constituent fluxes
Programme: 414;415
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Heikkila U., Beer J., Jouzel J., Feitcher J., Kubik P. (2008). Be-10 measured in a GRIP snow pit and modeled using the ECHAM5-HAM general circulation model. Geophysical research letters, 35, L05817.
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. (2008). Polarization in aurorae: A new dimension for space environments studies, ., 35, L08804. GEOGRAPHICAL RESEARCH, 35(L08804).
Abstract: The polarization of emission lines is a noteworthy
observational parameter in astronomy. However, it has
never been detected without ambiguity in planetary upper
atmospheres. Theoretical considerations have suggested that
the polarization of the thermospheric oxygen red line
(630 nm) could exist in the polar cap region. We present
here its first successful measurement at Svalbard in January
2007, during active geophysical conditions. We assign its
origin and variability to complementary effects between
permanent low-energy electron precipitation and sporadic
auroral events. Implications in physics, geophysics and
planetary science are foreseen. In physics, it raises the
question of the polarization of a forbidden transition by
electron impact which is still unknown. In geophysics, it
provides a new parameter to constrain the thermospheric
models. In planetary science, it makes it possible to derive
the local configuration of the magnetic fields. It therefore
opens new perspectives for future space missions towards
other planets.
Programme: 1026
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Salamatin A.N.. & Duval P. (1997). Creep flow and pressure relaxation in bubbly medium. International journal of solid structures, 34(1), 61–78.
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Pinglot J.F. (1993). Canberra in the arctic. NPGNEWS, 34.
Abstract: NPGNEWS a publication of the Canberra Nuclear Products group
Programme: 265
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Jouventin P. (2002). La communication animale aux carrefours de la naissance. Pour la science, 34.
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