946 resultados para 2.0 Web
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In der Überprüfung von Kernmodellen stellt der elektrische Formfaktor des Neutrons Gen eine wichtige Eingangsgröße dar. Im Rahmen dieser Arbeit wurde am polarisierten Elektronenstrahl des Mainzer Mikrotrons MAMI der elektrische Formfaktor des Neutrons in der Reaktion 3He(e,e'n) bestimmt. Aus dem Verhältnis der Asymmetrien respektive der Helizitätsumkehr der Elektronenpolarisation mit Targetspin senkrecht und parallel zum Impulsübertrag konnte in einer integralen Analyse Gen bestimmt werden. Zusammengefasst ergab sich Gen(Q2=0.67 (GeV/c)2) = 0.0468 +- 0.0064(stat} +- 0.0027(syst}. Um den Einfluß von Kernbindungseffekten, die z. Zt. von der Gruppe um Prof. Glöckle in Bochum theoretisch gerechnet werden, auch experimentell abzusichern, wurden parallel zur Gen-Messung die Targetasymmetrie Ay0 3He(e,e'n) und Protonenasymmetrie 3He(e,e'p) bestimmt. Die Empfindlichkeit dieser Observablen auf FSI und D-Wellenbeiträge schafft Redundanzen, aus denen auf die Eigenschaften des freien Neutrons im gebundenen System geschlossen werden kann.
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Oggetto di questa tesi è la riqualificazione sostenibile dell’edificio ospitante la Scuola secondaria di I grado “Il Guercino”, sita all’interno del quartiere Savena, nel Comune di Bologna, ai confini con quello di San Lazzaro di Savena. L’edificio, esito di un modo di fare architettura legato ad un contesto storico e professionale precisamente definito (quello dell’amministrazione pubblica bolognese nel quindicennio 1970-’85), presenta principi compositivi e soluzioni tecnologiche non scontate e per certi versi pregevoli, se contestualizzate nel momento della sua realizzazione. L’intervento di riqualificazione progettato affronta in primo luogo la riorganizzazione funzionale dell’edificio (anche attraverso un ampliamento) e del sistema delle accessibilità, oggi inadeguati rispetto alle esigenze degli utenti e alle prescrizioni normative. Particolare attenzione è stata dedicata alla possibilità di rendere l’edificio il più possibile fruibile ai portatori di handicap, aspetto non più trascurabile, soprattutto all’interno di un istituto scolastico. In secondo luogo il progetto si occupa del retrofit energetico realizzato tramite alcuni interventi mirati, quali la sostituzione del sistema di involucro verticale e di quello impiantistico: in tal modo si è passati da una classe di prestazione energetica F ad una classe di prestazione energetica A, rendendo sostenibile il consumo energetico e migliorando sensibilmente il livello di comfort degli occupanti.
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In this contribution the experiences with e-Learning 2.0 applications by using a Wiki for the education in hydraulic engineering are shown. Up to now important information for the students has been prepared by the instructor. For this project the students were asked to collaborate and search on their own for the information they needed. Therefore a Wiki-system was used. For the engineering practice a self dependent realisation of tasks is an important requirement which students should be prepared for. With the help of online communication there should be shown the possibilities for students for working together in an interdisciplinary team. The positive experiences as well as the results of the evaluation of this project plead for a continuation of the application of e-Learning 2.0 for education. The comparison of results of tests without using Wiki and with using Wiki shows a qualitative tendency of better marks. In this contribution we present the application of Wiki in hydraulic engineering but the results can also be used for other engineering disciplines.
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Einzelne Projekte bildeten den Anfang für die E-Learning-Integration im Hochschulbereich. Heute, nach dem Ende der großen E-Learning-Förderprojekte, haben sich an vielen Hochschulen feste E-Learning-Einrichtungen etabliert. Learning Management Systeme (LMS) sind flächendeckend Realität. Die Pädagogische Hochschule Ludwigsburg war in der Lage, E-Learning auch strukturell fest in der Hochschulorganisation zu verankern – ein ‚luxuriöser‘ und beruhigend zukunftsfähiger, nachhaltiger Zustand. Didaktische Konzepte sind erprobt, der Einsatz von E-Learning in den Hochschulveranstaltungen vielzählig in allen Fachgebieten etabliert; die technische Realisation stellt kein Problem mehr dar. Das ‚klassische E-Learning‘ sozusagen haben wir hinter uns – was bringt die mobile Zukunft? Genau jetzt ist der richtige Zeitpunkt festzuhalten, welche Umsetzungen und Anwendungen es für E-Learning an der Pädagogischen Hochschule Ludwigsburg gibt – und dies sicher beispielhaft für viele Hochschulen. Welche Projekte bewegen die Hochschule auf diesem Feld, welche Partner wurden gefunden und welche Antworten auf die Grundfragen des E-Learning? UND: Wie soll es weiter gehen auf dem elektronischen Weg der individualisierten Lernumgebungen; welchen Anforderungen stellen wir uns?
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This chapter explores cultural protectionism 2.0, i.e. the normative dimensions of cultural diversity policies in the global digital space, asking what adjustments are needed and in fact, how feasible the entire project of diversity regulation in this environment may be. The complexities of the shift from offline to online and from analogue to digital, and the inherent policy challenges are illustrated with some (positive and negative) instances of existing media initiatives. Taking into account the specificities of cyberspace and in a forward-looking manner, the chapter suggests some adjustments to current media policy practices in order to better serve the goal of sustainably diverse cultural environment.
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PLATO 2.0 has recently been selected for ESA’s M3 launch opportunity (2022/24). Providing accurate key planet parameters (radius, mass, density and age) in statistical numbers, it addresses fundamental questions such as: How do planetary systems form and evolve? Are there other systems with planets like ours, including potentially habitable planets? The PLATO 2.0 instrument consists of 34 small aperture telescopes (32 with 25 s readout cadence and 2 with 2.5 s candence) providing a wide field-of-view (2232 deg 2) and a large photometric magnitude range (4–16 mag). It focusses on bright (4–11 mag) stars in wide fields to detect and characterize planets down to Earth-size by photometric transits, whose masses can then be determined by ground-based radial-velocity follow-up measurements. Asteroseismology will be performed for these bright stars to obtain highly accurate stellar parameters, including masses and ages. The combination of bright targets and asteroseismology results in high accuracy for the bulk planet parameters: 2 %, 4–10 % and 10 % for planet radii, masses and ages, respectively. The planned baseline observing strategy includes two long pointings (2–3 years) to detect and bulk characterize planets reaching into the habitable zone (HZ) of solar-like stars and an additional step-and-stare phase to cover in total about 50 % of the sky. PLATO 2.0 will observe up to 1,000,000 stars and detect and characterize hundreds of small planets, and thousands of planets in the Neptune to gas giant regime out to the HZ. It will therefore provide the first large-scale catalogue of bulk characterized planets with accurate radii, masses, mean densities and ages. This catalogue will include terrestrial planets at intermediate orbital distances, where surface temperatures are moderate. Coverage of this parameter range with statistical numbers of bulk characterized planets is unique to PLATO 2.0. The PLATO 2.0 catalogue allows us to e.g.: - complete our knowledge of planet diversity for low-mass objects, - correlate the planet mean density-orbital distance distribution with predictions from planet formation theories,- constrain the influence of planet migration and scattering on the architecture of multiple systems, and - specify how planet and system parameters change with host star characteristics, such as type, metallicity and age. The catalogue will allow us to study planets and planetary systems at different evolutionary phases. It will further provide a census for small, low-mass planets. This will serve to identify objects which retained their primordial hydrogen atmosphere and in general the typical characteristics of planets in such low-mass, low-density range. Planets detected by PLATO 2.0 will orbit bright stars and many of them will be targets for future atmosphere spectroscopy exploring their atmosphere. Furthermore, the mission has the potential to detect exomoons, planetary rings, binary and Trojan planets. The planetary science possible with PLATO 2.0 is complemented by its impact on stellar and galactic science via asteroseismology as well as light curves of all kinds of variable stars, together with observations of stellar clusters of different ages. This will allow us to improve stellar models and study stellar activity. A large number of well-known ages from red giant stars will probe the structure and evolution of our Galaxy. Asteroseismic ages of bright stars for different phases of stellar evolution allow calibrating stellar age-rotation relationships. Together with the results of ESA’s Gaia mission, the results of PLATO 2.0 will provide a huge legacy to planetary, stellar and galactic science.
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This paper presents a software prototype of a personal digital assistant 2.0. Based on soft computing methods and cognitive computing this mobile application prototype improves calendar and mobility management in cognitive cities. Applying fuzzy cognitive maps and evolutionary algorithms, the prototype represents a next step towards the realization of cognitive cities (i.e., smart cities enhanced with cognition). A user scenario and a test version of the prototype are included for didactical reasons.
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Robert Sanborn and Angelo Giardino's introduction for Volume 4, Issue 1: New Morbdities 2.0