Architettura e verità. Emil Steffann architetto di chiese

La ricerca pone al suo centro lo studio dell'opera architettonica di Emil Steffann (1899-1968) la cui produzione realizzata consta, nel breve arco temporale che va dal 1950 al 1968, del ragguardevole numero di trentanove chiese, rappresentando un caso emblematico di progettazione e costruzione di edifici per il culto cristiano in grado di raffigurarne concretamente i principi fondativi liturgici, estetici e morfologici. L'architettura di Steffann, profondamente ispirata dallo spirito religioso, legata a figure primigenie che plasmano lo stare-insieme della comunità nella qualità corporea della materia, dove la presenza liturgica e monumentale si esprime nel silenzio e nella disponibilità di uno spazio circoscritto dai muri e direzionato dalla luce, concorre a definire nell'oggettivo amore per il vero la percezione estetico-teologica e la poetica formativa che connaturano, a nostro parere, progetto e segno della chiesa. Il testo concretizza il primo studio monografico completo di questo corpus architettonico e si basa sulla ricognizione diretta delle opere di Steffann; ne è derivata una narrazione non conseguente a un ordine cronologico o di presupposta importanza degli edifici, bensì che ricerca ed evidenzia corrispondenze tra nodi di una rete ideativa la quale, con diversi gradi di finitezza, in punti non sempre omogenei del tempo e dello spazio, denota un'esperienza autentica del comporre e del costruire. Il racconto individua gli oggetti architettonici, ne discute la consistenza aprendosi a riferimenti altri (in particolare il pensiero ecclesiologico-liturgico di Romano Guardini e quello estetico-teologico di Hans Urs von Balthasar) in grado di illuminarne la genesi e la manifestazione, li lega infine in sequenze analogiche. Una serie di tavole fotografiche originali, parte ineludibile e integrante della ricerca, testimonia dello stato attuale dei luoghi, connotando ulteriormente l'aspetto info-rappresentativo della loro composizione architettonica. In chiusura, la sintesi architetturale vuole essere uno strumento di verifica e progetto, quindi di trasposizione futura, correlato all'elaborazione documentaria.

Astronomical site testing in the era of the extremely large telescopes

The quality of astronomical sites is the first step to be considered to have the best performances from the telescopes. In particular, the efficiency of large telescopes in UV, IR, radio etc. is critically dependent on atmospheric transparency. It is well known that the random optical effects induced on the light propagation by turbulent atmosphere also limit telescope’s performances. Nowadays, clear appears the importance to correlate the main atmospheric physical parameters with the optical quality reachable by large aperture telescopes. The sky quality evaluation improved with the introduction of new techniques, new instrumentations and with the understanding of the link between the meteorological (or synoptical parameters and the observational conditions thanks to the application of the theories of electromagnetic waves propagation in turbulent medias: what we actually call astroclimatology. At the present the site campaigns are evolved and are performed using the classical scheme of optical seeing properties, meteorological parameters, sky transparency, sky darkness and cloudiness. New concept are added and are related to the geophysical properties such as seismicity, microseismicity, local variability of the climate, atmospheric conditions related to the ground optical turbulence and ground wind regimes, aerosol presence, use of satellite data. The purpose of this project is to provide reliable methods to analyze the atmospheric properties that affect ground-based optical astronomical observations and to correlate them with the main atmospheric parameters generating turbulence and affecting the photometric accuracy. The first part of the research concerns the analysis and interpretation of longand short-time scale meteorological data at two of the most important astronomical sites located in very different environments: the Paranal Observatory in the Atacama Desert (Chile), and the Observatorio del Roque de Los Muchachos(ORM) located in La Palma (Canary Islands, Spain). The optical properties of airborne dust at ORM have been investigated collecting outdoor data using a ground-based dust monitor. Because of its dryness, Paranal is a suitable observatory for near-IR observations, thus the extinction properties in the spectral range 1.00-2.30 um have been investigated using an empirical method. Furthermore, this PhD research has been developed using several turbulence profilers in the selection of the site for the European Extremely Large Telescope(E-ELT). During the campaigns the properties of the turbulence at different heights at Paranal and in the sites located in northern Chile and Argentina have been studied. This given the possibility to characterize the surface layer turbulence at Paranal and its connection with local meteorological conditions.

Numerical models of trench migration for lateral heterogeneous subducting plates

The aim of this Thesis is to investigate the effect of heterogeneities within the subducting plate on the dynamics of subduction. In particular, I study the motion of the trench for oceanic and continental subduction, first, separately, and, then, together in the same system to understand how they interact. The understanding of these features is fundamental to reconstruct the evolution of complex subduction zones, such as the Central Mediterranean. For this purpose, I developed 2D and 3D numerical models of oceanic and continental subduction where the rheological, geometrical and compositional properties of the plates are varied. In these models, the trench and the overriding plate move self-consistently as a function of the dynamics of the system. The effect of continental subduction on trench migration is largely investigated. Results from a parametric study showed that despite different rheological properties of the plates, all models with a uniform continental crust share the same kinematic behaviour: the trench starts to advance once the continent arrives at the subduction zone. Hence, the advancing mode in continental collision scenarios is at least partly driven by an intrinsic feature of the system. Moreover, the presence of a weak lower crust within the continental plate can lead to the occurrence of delamination. Indeed, by changing the viscosity of the lower crust, both delamination and slab detachment can occur. Delamination is favoured by a low viscosity value of the lower crust, because this makes the mechanical decoupling easier between crust and lithospheric mantle. These features are observed both in 2D and 3D models, but the numerical results of the 3D models also showed that the rheology of the continental crust has a very strong effect on the dynamics of the whole system, since it influences not only the continental part of plate but also the oceanic sides.