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Vogel, N., Dommergue, A., Ferrari, C., Preunkert, S., Jourdain, B., Legrand, M. (2011).
Abstract: The 10th International Conference on Mercury as a Global Pollutant (ICMGP),Halifax (Canada), 24-29 July
Programme: 1028
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Roscoe H.K., Squires J.A.C., Oldham D.J., Pommereau J.P. & Goutail F. (1994). Proc. Quad. Ozone Symp., NASA Conf. Pub., 3266, 569–572.
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. (2011).
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. (2010).
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. (2009). Bachelor's thesis, , .
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Hochstrasser-Petit Ch., Romanova L., Duchesne S., Melnichuk O., Gérard P. (2020). Yakut clothes of the 17th and 18th centuries, archaeology and restitution. (Vol. 4).
Abstract: 40 Frozen Yakutian Graves, From The 17th To The 19th Century Allow The Reconstitution Of Clothes. At The End Of the 17th Century, New Fashions Are Emerging With The Ostentatious Use Of Imported Goods And The Influences Of russian Noble Circles And Chinese And/or Mongol And/or Buriat Fashions. The Garment Does Not Only Seem To Be any More An Element Of Protection Against The Cold And A Utilitarian Object But Becomes A Way To Marking The Socialization of The Individual.
Programme: 1038
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Collins T., Gerday C. & Feller G. (2004). Xylanases, xylanase families and extremophilic xylanases. FEMS Microbiol. Rev., 29, 3–23.
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Petrescu I., Lamotte Brasseur J., Chessa J.P., Ntarima P., Claeyssens M., Devreese B., Marino G. & Gerday C. (2000). Xylanase from the psychrophilic yeast Crytococcus adeliae. Extremophiles, 4, 137–144.
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Gregoire M., Lorand J.P., Cottin J.Y., Giret A., Mattielli N. & Weis D. (1997). Xenoliths evidence for a refractory oceanic mantle percolated by basaltic melts beneath the Kerguelen archipelago. European journal of mineralogy, 9, 1085–1100.
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. (2017). X-Ray, Radio and SEP Observations of Relativistic Gamma-Ray Events.
Abstract: The rather frequent occurrence, and sometimes long duration, of ?-ray events at photon energies above 100 MeV challenges our understanding of particle acceleration processes at the Sun. The emission is ascribed to pion-decay photons due to protons with energies above 300 MeV. We study the X-ray and radio emissions and the solar energetic particles (SEPs) in space for a set of 25 Fermi ?-ray events. They are accompanied by strong SEP events, including, in most cases where the parent activity is well-connected, protons above 300 MeV. Signatures of energetic electron acceleration in the corona accompany the impulsive and early post-impulsive ?-ray emission. ?-ray emission lasting several hours accompanies in general the decay phase of long-lasting soft X-ray bursts and decametric-to-kilometric type II bursts. We discuss the impact of these results on the origin of the ?-ray events.
Programme: 227
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