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See detailLe plan de la Domus aux Bucranes et son système décoratif : pavements - parois peintes - stucs - plafonds.
Morard, Thomas ULg

in Perrier, Bertrand (Ed.) Colloque de Saint-Romain-en-Gal "Villas, maisons, sanctuaires et tombeaux tardo-républicains. Découvertes et relectures récentes." En l'honneur d'A. Gallina Zevi. (2007)

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See detailPlan éolien wallon et Paysage
Feltz, Claude ULg; Lejeune, Philippe ULg; Cuvelier, M. et al

in Collectif Ministère de la région wallonne; Mardaga (Eds.) Cahiers de l'urbanisme (Les), n° 52 Les éoliennes (2004)

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See detailPlan loutre 2011-2021 en Wallonie et au Grand-Duché de Luxembourg
Nederlandt, Nicolas; Schmidt, Gérard; Leclercq, Christine et al

Report (2011)

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See detailLe plan Marshall doit être complété
Nondonfaz, Robert ULg

Article for general public (2007)

Le plan Marshall développé par la Région Wallonne a sélectionné la logistique comme étant un des pôles de re-développement de la Région. L'auteur pense qu'il faudrait ajouter quelques ouvertures pour l ... [more ▼]

Le plan Marshall développé par la Région Wallonne a sélectionné la logistique comme étant un des pôles de re-développement de la Région. L'auteur pense qu'il faudrait ajouter quelques ouvertures pour l'améliorer. [less ▲]

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See detailPlan pour une restauration de la population de tétras lyres en Wallonie. Rapport final
Keulen, C.; Charlet, O.; Poncin, Pascal ULg et al

Report (2003)

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See detailLe plan régional d'aménagement du territoire wallon
Delnoy, Michel ULg; Pâques, Michel ULg

in Aménagement - Environnement (1994), n° spécial

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See detailPlan Simple de Gestion : un outil de gestion de la ressource bois énergie dans les espaces périurbains
Dubiez, Emilien; Vermeulen, Cédric ULg; Larzillière, Adélaïde et al

Scientific conference (2013)

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See detailPlan Simple de Gestion à vocation de production de bois énergie
Dubiez, Emilien; Vermeulen, Cédric ULg; Larzilière, Adélaïde

E-print/Working paper (2012)

Les zones d’interventions du Projet Makala présentent des contextes différents liés à l’occupation spatiale coutumière, l’organisation des structures sociales traditionnelles (lignage, clan, chefferie ... [more ▼]

Les zones d’interventions du Projet Makala présentent des contextes différents liés à l’occupation spatiale coutumière, l’organisation des structures sociales traditionnelles (lignage, clan, chefferie coutumière), les types de formations végétales présentes dans la zone et les activités principales des populations. L’ensemble de ces éléments structure l’intervention du projet dans son objectif d’aménagement des espaces forestiers périurbains dégradés. Des enquêtes d’identification du finage et des terroirs villageois partenaires ont d’abord été réalisées pour caractériser le contexte social et environnemental d’intervention. Les données recueillies ont constituées la base de travail de la construction du processus d’élaboration des Plans Simples de Gestion (PSG). Le présent document présente les étapes structurant le PSG, l’outil de démarche participatif permettant une appropriation collective du processus et les activités techniques développées pour la reconstitution des espaces forestiers dégradés. [less ▲]

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See detailPlan stratégique
Pagnoulle, Christine ULg

in Durand, Pascal (Ed.) Les nouveaux mots du pouvoir, Abécédaire critique (2007)

This is but a very limited contribution to a major critical enterprise, a systematic debunking of smokescreen words such as governance, civil society or expertise.

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See detailLe Plan « Horizon 97 » à la R.T.B.F.
Hermans, Michel ULg

Report (1995)

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See detailThe planar optics phase sensor: a study for the VLTI 2nd generation fringe tracker
Blind, Nicolas; Le Bouquin, Jean-Baptiste; Absil, Olivier ULg et al

in Danchi, W. C.; Delplancke, F.; Rajagopal, J. K. (Eds.) Optical and Infrared Interferometry II (2010, July)

In a few years, the second generation instruments of the Very Large Telescope Interferometer (VLTI) will routinely provide observations with 4 to 6 telescopes simultaneously. To reach their ultimate ... [more ▼]

In a few years, the second generation instruments of the Very Large Telescope Interferometer (VLTI) will routinely provide observations with 4 to 6 telescopes simultaneously. To reach their ultimate performance, they will need a fringe sensor capable to measure in real time the randomly varying optical paths differences. A collaboration between LAOG (PI institute), IAGL, OCA and GIPSA-Lab has proposed the Planar Optics Phase Sensor concept to ESO for the 2[SUP]nd[/SUP] Generation Fringe Tracker. This concept is based on the integrated optics technologies, enabling the conception of extremely compact interferometric instruments naturally providing single-mode spatial filtering. It allows operations with 4 and 6 telescopes by measuring the fringes position thanks to a spectrally dispersed ABCD method. We present here the main analysis which led to the current concept as well as the expected on-sky performance and the proposed design. [less ▲]

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See detailPlanatophyton gen. nov., a late Early or Middle Devonian euphyllophyte from Xinjiang, North-West China
Gerrienne, Philippe ULg; Meyer-Berthaud; Yang, N. et al

in Review of Palaeobotany and Palynology (2014)

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See detailUne planche de Manuel. Lecture sémiotique
Badir, Sémir ULg

in Groupe ACME (Ed.) L’Association. Une utopie éditoriale et esthétique (2011)

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See detailPlanck pre-launch status: The Planck mission
Tauber, Jan; Banos, Thierry; Roose, Stéphane ULg et al

in Astronomy and Astrophysics (2010), 520

The European Space Agency’s Planck satellite, launched on 14 May 2009, is the third-generation space experiment in the field of cosmic microwave background (CMB) research. It will image the anisotropies ... [more ▼]

The European Space Agency’s Planck satellite, launched on 14 May 2009, is the third-generation space experiment in the field of cosmic microwave background (CMB) research. It will image the anisotropies of the CMB over the whole sky, with unprecedented sensitivity ( ΔT T ∼ 2 × 10−6) and angular resolution (∼5 arcmin). Planck will provide a major source of information relevant to many fundamental cosmological problems and will test current theories of the early evolution of the Universe and the origin of structure. It will also address a wide range of areas of astrophysical research related to the Milky Way as well as external galaxies and clusters of galaxies. The ability of Planck to measure polarization across a wide frequency range (30−350 GHz), with high precision and accuracy, and over the whole sky, will provide unique insight, not only into specific cosmological questions, but also into the properties of the interstellar medium. This paper is part of a series which describes the technical capabilities of the Planck scientific payload. It is based on the knowledge gathered during the on-ground calibration campaigns of the major subsystems, principally its telescope and its two scientific instruments, and of tests at fully integrated satellite level. It represents the best estimate before launch of the technical performance that the satellite and its payload will achieve in flight. In this paper, we summarise the main elements of the payload performance, which is described in detail in the accompanying papers. In addition, we describe the satellite performance elements which are most relevant for science, and provide an overview of the plans for scientific operations and data analysis. [less ▲]

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See detailPlane strain test for metal sheet characterization
Flores, Paulo; Bonnet, Félix; Habraken, Anne ULg

in Key Engineering Materials [=KEM] (2007), 344

This article shows the influence of a plane strain test specimen geometry on the measurable strain field and the influence of free edge effects over the stress computation. The experimental strain field ... [more ▼]

This article shows the influence of a plane strain test specimen geometry on the measurable strain field and the influence of free edge effects over the stress computation. The experimental strain field distribution is measured over the whole deformable zone of a plane strain test specimen by an optical strain gauge. The chosen material is the DC06 IF steel of 0.8 mm thickness. The stress field is computed for several geometries at different strain levels by a Finite Element (FE) commercial code (Samcef ®). The results show that the stress field is sensitive to the specimen’s geometry and also to the tested material (strain field behavior is independent of material) and, based on results, an optimal specimen geometry is proposed in order to minimized the stress computation error. [less ▲]

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