Salamolard M. (1992). Adaptations des stratégies de recherche alimentaire aux contraintes environnementales et énergétiques au cours de la reproduction..
Abstract: D.E.A. 'Adaptations et Survie en Environnements Extrêmes'
Programme: 109
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Walter J., Kurat G., Brandstatter F., Presper T., Koeberl C. & Maurette M. (1994). The chemical composition of olivine and pyroxenes from Antarctic micrometeorites. Meteoritics, 29, 545.
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Raymond C.A. & Giret A. (1997). Southern Ocean Evolution: Introduction. Terra antarctica, 3(2), 650–652.
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Bureau Central De Magnetisme Terrestre. (1995). Réseaux magnétiques de répétition, France Métropolitaine 1987, Terres Australes et Antarctiques Françaises 1981-1989, Afrique de l'Ouest 1983-1986. Bulletin, 5.
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Guinet C., Jouventin P. & Weimerskirch H. (1999). Recent population change of the southern elephant seal at îles Crozet and Kerguelen: the end of the decrease? Antarct. Sci., 11(2), 193–197.
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Iyemori T., Araki T., Kamei T. & Takeda M. (1997). Mid-latitude geomagnetic indices ASY and SYM. Data Analysis Center for Geomagnetic and Space Magnetism, 7.
Abstract: Publication annuelle du Data Analysis Center for Geomagnetic and Space Magnetism
Programme: 139
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Lambert Van Roozendael Simon De Maziere Pommereau Goutail Sarkissian Denis Dorokhov Eriksen Kyro Leveau Roscoe Vaughan Wahlstrom. (1996). Validation of the ERS-2 GOME products with the SAOZ network. (Vol. 108). Bachelor's thesis, , .
Abstract: Proc. Workshop on Gome validation, ESA WWPP
Programme: 209
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Démoulin, P.; Klein, K.-L.; Goff, C.; van Driel-Gesztelyi, L.; Culhane, J.; Mandrini, C.; Matthews, S.; Harra, L. (2007). Decametric N Burst: A Consequence of the Interaction of Two Coronal Mass Ejections. Solar physics, 240(2), 301–313.
Abstract: Abstract Radio emissions of electron beams in the solar corona and interplanetary space are tracers of the underlying magnetic configuration and of its evolution. We analyse radio observations from the Culgoora and WIND/WAVES spectrographs, in combination with SOHO/LASCO and SOHO/MDI data, to understand the origin of a type N burst originating from NOAA AR 10540 on January 20, 2004, and its relationship with type II and type III emissions. All bursts are related to the flares and the CME analysed in a previous paper (Goff et al., 2007). A very unusual feature of this event was a decametric type N burst, where a type III-like burst, drifting towards low frequencies (negative drift), changes drift first to positive, then again to negative. At metre wavelengths, i.e., heliocentric distances ?1.5R ?, these bursts are ascribed to electron beams bouncing in a closed loop. Neither U nor N bursts are expected at decametric wavelengths because closed quasi-static loops are not thought to extend to distances ?1.5R ?. We take the opportunity of the good multi-instrument coverage of this event to analyse the origin of type N bursts in the high corona. Reconnection of the expanding ejecta with the magnetic structure of a previous CME, launched about 8 hours earlier, injects electrons in the same manner as with type III bursts but into open field lines having a local dip and apex. The latter shape was created by magnetic reconnection between the expanding CME and neighbouring (open) streamer field lines. This particular flux tube shape in the high corona, between 5R ? and 10R ?, explains the observed type N burst. Since the required magnetic configuration is only a transient phenomenon formed by reconnection, severe timing and topological constraints are present to form the observed decametric N burst. They are therefore expected to be rare features.
Programme: 227
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Cherel Y., Charrassin J.B. & Handrich Y. (1993). Comparison of Body Reserve Buildup in Prefasting Chicks and Adults of King penguins(Aptenodytes patagonicus). Physiological zoology, 66(5), 750–770.
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Milan S.E., Lester M., Sato N., Takizawa H. & Villain J.P. (2000). Investigation of the relationship between optical auroral forms and HF radar E region backscatter. Annales geophysicae, 18, 608–617.
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