5,433 research outputs found
Villa de l'architecte J. Mauri à Port aux Poules (Oran)
No full textMauri Marcel Joseph. Villa de l'architecte J. Mauri à Port aux Poules (Oran). In: Chantiers. Revue illustrée de la construction en Afrique du Nord, N°21, 1955. Lotissements et villas. p. 37
Mauri Hono: A Mauri sensory methodology
No full textWithin a Māori cultural context, the manifestation of mauri instilled in all living things, both animate and inanimate gives life. Previous research suggests Māori can experience somatic exchanges of energy such as mauri from both other people, as well as within the natural environment. Accordingly, Mauri Hono: A Mauri Sensory Methodology provides a foundation to understanding knowledge by tuning into our senses and using mauri states to help elicit meaning about ourselves and our relationships with natural environments when immersed in those environments. In this study, four key phases of the methodology are detailed; Rongo, Mōhio, Mārama and Mātau and applied to a case study which sought to understand how Māori draw meaning from their experience of being immersed in a natural environment. Ten participants undertook a hīkoi (walk) within a national forest park of regenerating, native, bush. Findings revealed the importance of tuning into one’s senses and having the time and space to interpret different experiences. Furthermore, Mauri Hono, as a Māori methodology is predicated on the belief that experiential knowledge aids in providing a more complete understanding of phenomena than theoretical knowledge alone. It further highlights that whilst knowledge can come into fruition within the timeframe of the project, there is opportunity for insights to arise afterwards, comprising various layers of knowing.fals
Obiettivi, metodi e strumenti della tipologia
No full textIn questo capitolo ci occuperemo di delineare il percorso di ricerca che segue il tipologo, concentrando l’attenzione sulle prime fasi che lo caratterizzano, dall’individuazione degli obiettivi e degli interrogativi di ricerca al reperimento dei dati, chiarendo gli aspetti metodologici necessari per costruire una base empirica solida
Le parti del discorso
No full textLe classi lessicali, che tradizionalmente vengono individuate sotto eti- chette come nomi, verbi, aggettivi o avverbi, sono concetti profonda- mente problematici sia in un’ottica intralinguistica sia in prospettiva interlinguistica, perché sembrano sfuggire tanto a rigide definizioni semantiche quanto a univoche caratterizzazioni morfosintattiche. Questa difficoltà classificatoria mette in dubbio il carattere universale delle parti del discorso: se, infatti, è ben noto che non tutte le lingue possiedono gli articoli o le preposizioni, non è altrettanto noto che i problemi emergono anche con quelle che vengono considerate le classi lessicali maggiori, che coprono la stragrande maggioranza delle parole di una lingua, cioè i nomi, i verbi, gli aggettivi e, in misura minore, gli avverbi1. In questo capitolo, cercheremo di capire se sia possibile trovare dei criteri definitori universali, validi per tutte le lingue del mondo, oppure se le classi di nome, verbo e aggettivo debbano essere definite unicamente in base a parametri specifici per ogni lingua, e ci chiedere- mo se esistano dei modelli di variazione in qualche misura prevedibili
Measurement of the TeV atmospheric muon charge ratio with the full OPERA data set
No full textAbstractThe OPERA detector, designed to search for νμ→ντ oscillations in direct appearance mode, is located in the underground Gran Sasso laboratory, a privileged location to study TeV-scale cosmic rays. Given the large rock depth and the detector's wide acceptance, the apparatus was used to measure the atmospheric muon charge ratio in the TeV energy region. The muon charge ratio, defined as the number of positive over negative charged muons, provides an understanding of the mechanism of multiparticle production in the atmosphere in kinematic regions not accessible to accelerators, as well as information on the primary cosmic ray composition. We present the results obtained with the full statistics collected by OPERA from 2008 to 2012. The combination of two data sets with opposite magnet polarities allows minimizing systematic uncertainties and reaching an accurate determination of the muon charge ratio. Relevant parameters on the composition of primary cosmic rays and the associated kaon production in the forward fragmentation region are obtained
Results from the OPERA experiment at the CNGS beam
No full textThe OPERA experiment at the Gran Sasso underground laboratory was designed to study vμ → vτ oscillations in appearance mode in the CNGS neutrino beam. Five vτ candidate events have been observed, allowing to assess the discovery of vμ → vτ transitions in the atmospheric sector with a significance of 5.1σ. In this paper the vτ data analysis will be discussed, with emphasis on the background constraints obtained using dedicated data-driven control samples. Results on the search for vμ → vτ oscillations, on the search for sterile neutrino mixing and on the atmospheric muon charge ratio will also be presented
Experimental results on the atmospheric muon charge ratio
No full textThe atmospheric muon charge ratio, defined as the number of positive over negative charged muons, is a highly informative observable both for cosmic rays and particle physics. It allows studying the features of high-energy hadronic interactions in the forward region and the composition of primary cosmic rays. In this review results from underground experiments measuring the charge ratio around 1 TeV are discussed. The measurements in the TeV energy region constrain the associated kaon production, which is particularly important e.g. for the calculation of the atmospheric neutrino flux
Search for sterile neutrino mixing in the νμ → ντ appearance channel with the OPERA detector
No full textThe OPERA experiment has observed muon neutrino to tau neutrino oscillations in the atmospheric sector in appearance mode. Five ντ candidate events have been detected, a number consistent with the expectation from the “standard” 3ν framework. Based on this result new limits on the mixing parameters of a massive sterile neutrino have been set. The analysis is performed in the 3+1 neutrino model
Qui sont les Dii mauri ?
No full textThe author reviews the various but rare interpretations of the divine collectivity referred to by the name of Dii Mauri. From a re-examination of the literary or epigraphic mentions of the 50 specifically African local or regional divinities, and of the 20 dedications to the Dii Mauri known to this day, he believes he can propose the relationship, even the identity, between the local gods and the Dii Mauri. The comparison between the authors of the dedications shows that the worship of the local gods principally concerned « civilians » (82,5 %), whereas the Dii Mauri were invoked by governors, imperial procurators, soldiers (81,25 %). Moreover the Dii Mauri are invoked as often in Numidia and in Africa as in Caesarian Mauretania (they are unknown in Tingitana). Therefore the term of "maurus" is not linked to the Roman administrative carving, it applies to what is rebellious to Latin culture, to what is specifically native and unassimilable. Dii Mauri and African gods are the same divinities, only the dedicators change.The author reviews the various but rare interpretations of the divine collectivity referred to by the name of Dii Mauri. From a re-examination of the literary or epigraphic mentions of the 50 specifically African local or regional divinities, and of the 20 dedications to the Dii Mauri known to this day, he believes he can propose the relationship, even the identity, between the local gods and the Dii Mauri. The comparison between the authors of the dedications shows that the worship of the local gods principally concerned « civilians » (82,5 %), whereas the Dii Mauri were invoked by governors, imperial procurators, soldiers (81,25 %). Moreover the Dii Mauri are invoked as often in Numidia and in Africa as in Caesarian Mauretania (they are unknown in Tingitana). Therefore the term of "maurus" is not linked to the Roman administrative carving, it applies to what is rebellious to Latin culture, to what is specifically native and unassimilable. Dii Mauri and African gods are the same divinities, only the dedicators change.Camps Gabriel. Qui sont les Dii mauri ?. In: Antiquités africaines, 26,1990. pp. 131-153
The OPERA experiment at Gran Sasso
No full textOPERA (Oscillation Project with Emulsion tRacking Apparatus) is a long baseline neutrino experiment aiming to detect for the first time the appearance of tau neutrinos in a pure muon neutrino beam. The OPERA detector is exposed to the CNGS beam (CERN Neutrinos to Gran Sasso), a high-intensity and high-energy beam of muon neutrinos produced at the CERN SPS and directed toward the Gran Sasso underground laboratory (LNGS), 730 km away. The LNGS laboratory is situated under an average depth of 3800 meters water equivalent, making OPERA the deepest experiment able to measure cosmic ray muons with a magnetized detector, e.g. the cosmic ray muon charge ratio. Cosmic ray events were observed, together with the first neutrino beam events, during the 2007 and 2008 CNGS runs. This paper reviews the experimental apparatus, presents the first results for neutrino data and describes the analysis of cosmic ray data. © 2009 Elsevier B.V. All rights reserved
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