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See detailAulu-Gelle et Favorinos, lecteur et ‘philologue’ des textes latins
Scappaticcio, Maria Chiara ULg

Scientific conference (2012, February 24)

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See detailAura
Durand, Pascal ULg

E-print/Working paper (in press)

Entrée du Lexique Socius sur le concept d'Aura chez Walter Benjamin

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See detailL’aura et la chose écrite. Une mise au point
Durand, Pascal ULg

in Piret, Pierre (Ed.) La littérature à l’ère de la reproductibilité technique. Réponses littéraires aux nouveaux dispositifs représentatifs créés par les médias modernes (2007)

Detailed reference viewed: 39 (16 ULg)
See detailAURA validation by the baloon-borne MkIV Interferometer.
Toon, G. C.; Kleinboehl, A.; Salawitch, R. J. et al

Scientific conference (2006)

Detailed reference viewed: 7 (1 ULg)
See detailAuralias
Leclercq, Pierre ULg; Stevens, Benjamin ULg; Demaret, Jean-Noël ULg et al

Software (2010)

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See detailAURALIAS: an audio-immersive system for auralizing room acoustics projects
Embrechts, Jean-Jacques ULg

Conference (2011, December)

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See detailAuralization in Room Acoustics using Directional Impulse Responses Computed by Sound Ray Techniques
Embrechts, Jean-Jacques ULg; Werner, Nicolas; Lesoinne, Stéphane ULg

in Proceedings of the 4th Forum Acusticum Congress (2005)

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See detailThe Aurignacian in Eastern Europe
Noiret, Pierre ULg

in Anatolia (2005), 29

In Eastern Europe, a few sites have yielded industries attributed to the Early Aurignacian between 33,000 and 29.000 BP, characterized by bladelet production from bladelet cores and/or from carinated core ... [more ▼]

In Eastern Europe, a few sites have yielded industries attributed to the Early Aurignacian between 33,000 and 29.000 BP, characterized by bladelet production from bladelet cores and/or from carinated core-tools. These industries have affinities with other local industries south of the expansion zone of this Early Aurignacian, but problems with relative and absolute chronologies currently prevented a satisfactory "historical" interpretation of the Aurignacian phenomenon. [less ▲]

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See detailThe Aurignacian in the Zagros Region: new research at Yafteh Cave, Lorestan, Iran
Otte, Marcel ULg; Biglari, Fereidoun; Flas, Damien ULg et al

in Antiquity (2007), 81(311), 82-96

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See detailL'Aurignacien de Siuren I (Crimée): fouilles 1994-1995
Otte, Marcel ULg; Noiret, Pierre ULg; Tatartsev, Serguei et al

in Montet-White, Anta; Palma di Cesnola, Arturo; Valoch, Karel (Eds.) The Upper Palaeolithic. Colloquium XI: The Late Aurignacian (1996)

New excavations undertaken in Siuren I shelter add to our knowledge on Eastern Aurignacian dispersal.

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See detailL'Aurignacien de Siuren I (Crimée, Ukraine)
Otte, Marcel ULg; Noiret, Pierre ULg; Tatartsev, Serguei et al

in Anthropologica et Praehistorica : Bulletin de la Société Royale Belge d'Anthropologie et de Préhistoire (1996), 107

New excavations at Siuren I allowed to control the stratigraphy of the site, to give radiometric dating to the two main layers encountered and to reevaluate the lithic and faunal materials. The new dates ... [more ▼]

New excavations at Siuren I allowed to control the stratigraphy of the site, to give radiometric dating to the two main layers encountered and to reevaluate the lithic and faunal materials. The new dates show that a real Aurignacian is present at Siuren I around 28000-29000 BP. These occupations were probably a late extension of this culture through Eastern Europe. [less ▲]

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See detailAurora : Global features
Gérard, Jean-Claude ULg

Conference (2011, July)

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See detailAurora at Earth, Jupiter and Saturn: a comparative view
Gérard, Jean-Claude ULg

Conference (2009, August)

The interaction of the solar wind with the magnetospheres of the giant planets is different from that with the terrestrial magnetosphere in several respects bearing consequences on the morphology and ... [more ▼]

The interaction of the solar wind with the magnetospheres of the giant planets is different from that with the terrestrial magnetosphere in several respects bearing consequences on the morphology and dynamics of the aurora: - the magnetospheres of the outer planets are dominated by the planetary rotation that can provide much of the energy for the processes acting within these magnetospheres. - the circulation of plasma may be driven by mass loading of the giant magnetospheres by moons and rings rather than by reconnection with the IMF. - the magnitude and orientation of the interplanetary magnetic field plays a key role in controlling the Earth’s auroral dynamics whereas the solar wind dynamic pressure appears as a key factor in triggering auroral intensification on Saturn. - The combination of imaging and spectral techniques indicates the characteristic energy of the auroral electrons is comparable on Earth and Saturn, but higher energies are associated with the Jovian aurora. As a consequence, Jupiter’s aurora appears relatively shielded from solar wind influences, except inside the auroral oval where transient bright emission has been observed following sudden compressions of the magnetosphere. The size and brightness of the main oval shows only a week dependence on solar wind conditions. By contrast, Saturn’s aurora is quite responsive to solar wind perturbations, as was observed during campaigns of concurrent observations between HST and Cassini. Auroral intensification events that are reminiscent of shock-induced Earth aurora appear to be triggered by sudden increases of the solar dynamic pressure more than by changes in the IMF orientation. However, simultaneous HST-Cassini observations indicate that localised auroral brightenings and ENA acceleration events may be observed under quiet solar wind conditions. The occurrence of substorms is a key characteristics of the Earth’s auroral dynamics. Localized auroral enhancements have also been observed on Jupiter and Saturn. They have been associated to reconnection events causing events similar to substorms. [less ▲]

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See detailThe aurora of giant planets: 20 years of observations with the Hubble Space Telescope
Gérard, Jean-Claude ULg

Scientific conference (2013, May)

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See detailAurorae at Jupiter: a selection of recent results
Bonfond, Bertrand ULg

Scientific conference (2013, December 17)

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See detailAurorae at Jupiter: Recent Findings
Bonfond, Bertrand ULg

Scientific conference (2013, April 30)

In this seminar I review the recent results concerning the aurora at Jupiter, based on Hubble Space Telescope Far-UV images.

Detailed reference viewed: 17 (5 ULg)