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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Dumonteil E., Barre H. & Meissner G. (1994). Effect of palmitol carnitine and related metabolites on the avian ca²+-AtPase and Ca²+ release channel. (Vol. 479). Bachelor's thesis, , .
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Abbadi I. (1995). Modélisation stochastique du cycle biologique de la truite – Application à la modélisation du cycle de la truite de mer de la baie Norvégienne aux Kerguelen..
Abstract: Diplôme d'Etudes Supérieures Spécialisées, Méthodes informatiques et modèles Mathématiques, Université Paul Sabatier
Programme: 123
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Nguyen B.C., Mihalopoulos N., Baboukas E. & Putaud J.P. (1995). Seasonal variation of methanesulfonic acid in precipitation in the southern Indian Ocean..
Abstract: Presented at the 20th General Assembly of the Europ.geophys.Soc.
Programme: 146
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Ropert Coudert Y., Bost C.A., Handrich Y., Bevan R.M., Butler P.J., Woakes A.J. & Le Maho Y. (2000). Impact of externally attached loggers on the diving behaviour of the king penguin. Physiol. Biochem. Zool., 73(4), 438–445.
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Goutail F., Pommereau J.P. & Sarkissian A. (1994). Four years of ground-based total ozone measurements by visible spectrometry in Antarctica. Proc. Quad Ozone Symp, 3266(2), 602–605.
Abstract: Proc. Quad Ozone Symp., 602, NASA Conf. Pub. 3266, Part 2, 602, 605
Programme: 209
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