MCAO for Extremely Large Telescopes: the cases of LBT and E-ELT

Several MCAO systems are under study to improve the angular resolution of the current and of the future generation large ground-based telescopes (diameters in the 8-40 m range). The subject of this PhD Thesis is embedded in this context. Two MCAO systems, in dierent realization phases, are addressed in this Thesis: NIRVANA, the 'double' MCAO system designed for one of the interferometric instruments of LBT, is in the integration and testing phase; MAORY, the future E-ELT MCAO module, is under preliminary study. These two systems takle the sky coverage problem in two dierent ways. The layer oriented approach of NIRVANA, coupled with multi-pyramids wavefront sensors, takes advantage of the optical co-addition of the signal coming from up to 12 NGS in a annular 2' to 6' technical FoV and up to 8 in the central 2' FoV. Summing the light coming from many natural sources permits to increase the limiting magnitude of the single NGS and to improve considerably the sky coverage. One of the two Wavefront Sensors for the mid- high altitude atmosphere analysis has been integrated and tested as a stand- alone unit in the laboratory at INAF-Osservatorio Astronomico di Bologna and afterwards delivered to the MPIA laboratories in Heidelberg, where was integrated and aligned to the post-focal optical relay of one LINC-NIRVANA arm. A number of tests were performed in order to characterize and optimize the system functionalities and performance. A report about this work is presented in Chapter 2. In the MAORY case, to ensure correction uniformity and sky coverage, the LGS-based approach is the current baseline. However, since the Sodium layer is approximately 10 km thick, the articial reference source looks elongated, especially when observed from the edge of a large aperture. On a 30-40 m class telescope, for instance, the maximum elongation varies between few arcsec and 10 arcsec, depending on the actual telescope diameter, on the Sodium layer properties and on the laser launcher position. The centroiding error in a Shack-Hartmann WFS increases proportionally to the elongation (in a photon noise dominated regime), strongly limiting the performance. To compensate for this effect a straightforward solution is to increase the laser power, i.e. to increase the number of detected photons per subaperture. The scope of Chapter 3 is twofold: an analysis of the performance of three dierent algorithms (Weighted Center of Gravity, Correlation and Quad-cell) for the instantaneous LGS image position measurement in presence of elongated spots and the determination of the required number of photons to achieve a certain average wavefront error over the telescope aperture. An alternative optical solution to the spot elongation problem is proposed in Section 3.4. Starting from the considerations presented in Chapter 3, a first order analysis of the LGS WFS for MAORY (number of subapertures, number of detected photons per subaperture, RON, focal plane sampling, subaperture FoV) is the subject of Chapter 4. An LGS WFS laboratory prototype was designed to reproduce the relevant aspects of an LGS SH WFS for the E-ELT and to evaluate the performance of different centroid algorithms in presence of elongated spots as investigated numerically and analytically in Chapter 3. This prototype permits to simulate realistic Sodium proles. A full testing plan for the prototype is set in Chapter 4.

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.

Mediterranean brachiopods: morphological, ecological and phylogenetic aspects

The Brachiopoda of the Marine Protected Area “Secche di Tor Paterno”, Central Tyrrhenian Sea, have been investigated in order to give a first glance of the diversity of the brachiopods of this area and provide a new report on the Mediterranean Brachiopod fauna. Four species were reported: Novocrania anomala (Müller, 1776), Megathiris detruncata (Gmelin, 1790), Joania cordata (Risso,1826) and Argyrotheca cuneata (Risso,1826). For all the four species a morphological analysis was carried out. For the two most abundant species, J.cordata and A. cuneata, a morphometric study, based on thickness/width and length/width scattergrams, was carried out, in order to investigate their variability. Size-frequency distributions relative to the three dimensions of the shell were also computed, aimed at a evaluation of population dynamics of these two species. The results showed that, for both species, the parameters which most determine the rise of the shell during the growth of animal are width and length and that frequency distributions are mainly bi- or plurymodal and that they are difficult to interpret, as reported by other studies. Analysis of drill holes found on the shell of some specimens of the two same species revealed a predatory origin and that three different predators are responsible for them. Partial sequences of two different genetic markers, the Internal Transcribed Spacer 1 (ITS1) and the cytochrome oxidase subunit 1 (COI), were used to investigate the phylogenetic relationship between two populations of the eurybathic brachiopod species Gryphus vitreus (Born,1778) across the strait of Gibraltar. This represents the first genetic population study on brachiopods. Results from AMOVA and Bayesian analysis performed on 31 specimens highlighted no genetic differentiation indicating a likely panmixia, dispite the lecitotrophic development of the species.

Edificio-Impianto: ruolo dell'involucro e dell'impiantistica. Miglioramento delle prestazioni energetiche degli edifici attraverso progetti innovativi che anticipano l'applicazione della Direttiva CE 2010/31

La tematica del presente scritto è l’analisi teorico-sperimentale del sistema edificio-impianto, che è funzione delle soluzioni progettuali adottate, dei componenti scelti e del tipo di conduzione prevista. La Direttiva 2010/31/CE sulle prestazioni energetiche degli edifici, entrata in vigore l’8 luglio 2010, pubblicata sulla Gazzetta Europea del 18 giugno 2010, sostituirà, dal 1º febbraio 2012, la direttiva 2002/91/CE. La direttiva prevede che vengano redatti piani nazionali destinati ad aumentare il numero di “edifici a energia quasi zero” e che entro il 31 dicembre 2020 tutti gli edifici di nuova costruzione dovranno essere “edifici a energia quasi zero”, per gli edifici pubblici questa scadenza è anticipata al 31 dicembre 2018. In questa prospettiva sono stati progettati due “edifici a energia quasi zero”, una villa monofamiliare e un complesso scolastico (scuola dell’infanzia, elementare, media inferiore) attualmente in via di realizzazione, con l’obiettivo principale di fornire un caso studio unico per ogni tipologia in quanto anche modulare e replicabile nella realtà del nostro territorio, che anticipano gli obiettivi fissati dalla Direttiva 2010/31/CE. I risultati ottenibili dai suddetti progetti, esposti nella tesi, sono il frutto di un attenta e proficua progettazione integrata, connubio tra progettazione architettonica ed energetico/impiantistica. La stessa progettazione ha esaminato le tecnologie, i materiali e le soluzioni tecniche “mirate” ai fini del comfort ambientale e di un’elevata prestazione energetica dell’edificio. Inoltre è stato dedicato ampio rilievo alla diagnosi energetica degli edifici esistenti attraverso 4 casi studio, i principali svolti durante i tre anni di dottorato di ricerca, esemplari del patrimonio edilizio italiano. Per ogni caso studio è stata condotta una diagnosi energetica dell’edificio, valutati i risultati e definita la classe energetica, ed in seguito sono stati presi in considerazione i possibili interventi migliorativi sia da un punto di vista qualitativo sia economico tenendo conto degli incentivi statali per l’incremento dell’efficienza energetica.

La scrittura dell'interpretazione: Teoria e pratica della trascrizione musicale durante gli ‘anni veneziani’ di Bruno Maderna (1946-1952)

La definizione di «scrittura dell’interpretazione» comprime in una sola locuzione la descrizione dell’oggetto principale del nostro studio, ovvero il problema della trascrizione musicale, descritta, non tanto come un determinato genere musicale, quanto come una ragione di osmosi e interferenze tra il fatto compositivo e quello interpretativo. Ad una traversata di quel territorio ci si appresta incentrando la trattazione intorno alla figura e all’opera del giovane compositore e direttore Bruno Maderna, autore di diverse trascrizioni della cosiddetta musica antica (dall’Odhecaton A, Monteverdi, Viadana, Frescobaldi, Legrenzi, ed altri ancora). Attraverso gli esempi presentati si intende mostrare come l’approccio maderniano alla trascrizione musicale si giustifichi a partire dalla sua stessa teoria e pratica dell’interpretazione musicale, più che in base a concetti forti definiti sul versante della scrittura, quali ad esempio quelli di analisi e parodia. Pari attenzione si offre al contesto storico degli anni in cui egli gravita, opera e si afferma come musicista (1946-1952 circa), dedicando ampio spazio alle figure di Gian Francesco Malipiero, Angelo Ephrikian e Luigi Nono, autori a loro volta di trascrizioni e revisioni di opere del Cinquecento, del Seicento e del Settecento. Intorno ai loro rapporti viene fornita una documentazione significativa, in buona parte inedita o poco conosciuta dagli studiosi, resa disponibile grazie alle ricerche d’archivio di cui si avvantaggia la nostra trattazione.