Perceived neighborhood problems: multilevel analysis to evaluate psychometric properties in a Southern adult Brazilian population

Abstract Background Physical attributes of the places in which people live, as well as their perceptions of them, may be important health determinants. The perception of place in which people dwell may impact on individual health and may be a more telling indicator for individual health than objective neighborhood characteristics. This paper aims to evaluate psychometric and ecometric properties of a scale on the perceptions of neighborhood problems in adults from Florianopolis, Southern Brazil. Methods Individual, census tract level (per capita monthly familiar income) and neighborhood problems perception (physical and social disorders) variables were investigated. Multilevel models (items nested within persons, persons nested within neighborhoods) were run to assess ecometric properties of variables assessing neighborhood problems. Results The response rate was 85.3%, (1,720 adults). Participants were distributed in 63 census tracts. Two scales were identified using 16 items: Physical Problems and Social Disorder. The ecometric properties of the scales satisfactory: 0.24 to 0.28 for the intra-class correlation and 0.94 to 0.96 for reliability. Higher values on the scales of problems in the physical and social domains were associated with younger age, more length of time residing in the same neighborhood and lower census tract income level. Conclusions The findings support the usefulness of these scales to measure physical and social disorder problems in neighborhoods.

Preserve and protect in a science museum

Reflections on the university campus usually focus on its relevancy as a research and teaching area; however, the need for preservation, protection, maintenance and cleaning only become visible in the event of inadequacy or lack thereof. The aim of this study is to address the characteristics of the preservation and security measures performed at the Science and Technology Park of the University of São Paulo (Parque de Ciência e Tecnologia da Universidade de São Paulo), agency subjected to the Dean’s Office for Culture and University Extension (Pró-Reitoria de Cultura e Extensão Universitária). Because of its history and location, the Park requires special care. The Park’s land formerly housed the Astronomical Observatory of São Paulo and the Institute of Astronomy and Geophysics of the University of São Paulo (Instituto de Astronomia e Geofísica – IAG-USP), within the Fontes do Ipiranga State Park (Parque Estadual das Fontes do Ipiranga – PEFI), in the city of São Paulo. Preservation and reconversion activities relative to historical buildings are developed at the Park. The institution’s location and its specificities require security in its borders, as well as in relation to the users of the park.

Introducing the CTA concept

The Cherenkov Telescope Array (CTA) is a new observatory for very high-energy (VHE) gamma rays. CTA has ambitions science goals, for which it is necessary to achieve full-sky coverage, to improve the sensitivity by about an order of magnitude, to span about four decades of energy, from a few tens of GeV to above 100 TeV with enhanced angular and energy resolutions over existing VHE gamma-ray observatories. An international collaboration has formed with more than 1000 members from 27 countries in Europe, Asia, Africa and North and South America. In 2010 the CTA Consortium completed a Design Study and started a three-year Preparatory Phase which leads to production readiness of CTA in 2014. In this paper we introduce the science goals and the concept of CTA, and provide an overview of the project.

Effects of ocean acidification on the brown alga "Padina pavonica": decalcification due to acute and chronic events

[EN] Since the industrial revolution, anthropogenic CO2 emissions have caused ocean acidification, which particularly affects calcified organisms. Given the fan-like calcified fronds of the brown alga Padina pavonica, we evaluated the acute (shortterm) effects of a sudden pH drop due to a submarine volcanic eruption (October 2011–early March 2012) affecting offshore waters around El Hierro Island (Canary Islands, Spain). We further studied the chronic (long-term) effects of the continuous decrease in pH in the last decades around the Canarian waters. In both the observational and retrospective studies (using herbarium collections of P. pavonica thalli from the overall Canarian Archipelago), the percent of surface calcium carbonate coverage of P. pavonica thalli were contrasted with oceanographic data collected either in situ (volcanic eruption event) or from the ESTOC marine observatory data series (herbarium study). Results showed that this calcified alga is sensitive to acute and chronic environmental pH changes. In both cases, pH changes predicted surface thallus calcification, including a progressive decalcification over the last three decades. This result concurs with previous studies where calcareous organisms decalcify under more acidic conditions. Hence, Padina pavonica can be implemented as a bio-indicator of ocean acidification (at short and long time scales) for monitoring purposes over wide geographic ranges, as this macroalga is affected and thrives (unlike strict calcifiers) under more acidic conditions

A spectroscopic and photometric study of MSP companions in Galactic Globular Clusters

This Thesis is devoted to the study of the optical companions of Millisecond Pulsars in Galactic Globular Clusters (GCs) as a part of a large project started at the Department of Astronomy of the Bologna University, in collaboration with other institutions (Astronomical Observatory of Cagliari and Bologna, University of Virginia), specifically dedicated to the study of the environmental effects on passive stellar evolution in galactic GCs. Globular Clusters are very efficient “Kilns” for generating exotic object, such as Millisecond Pulsars (MSP), low mass X-ray binaries(LMXB) or Blue Straggler Stars (BSS). In particular MSPs are formed in binary systems containing a Neutron Star which is spun up through mass accretion from the evolving companion (e.g. Bhattacharia & van den Heuvel 1991). The final stage of this recycling process is either the core of a peeled star (generally an Helium white dwarf) or a very light almos exhausted star, orbiting a very fast rotating Neutron Star (a MSP). Despite the large difference in total mass between the disk of the Galaxy and the Galactic GC system (up a factor 103), the percentage of fast rotating pulsar in binary systems found in the latter is very higher. MSPs in GCs show spin periods in the range 1.3 ÷ 30ms, slowdown rates ˙P 1019 s/s and a lower magnetic field, respect to ”normal” radio pulsars, B 108 gauss . The high probability of disruption of a binary systems after a supernova explosion, explain why we expect only a low percentage of recycled millisecond pulsars respect to the whole pulsar population. In fact only the 10% of the known 1800 radio pulsars are radio MSPs. Is not surprising, that MSP are overabundant in GCs respect to Galactic field, since in the Galactic Disk, MSPs can only form through the evolution of primordial binaries, and only if the binary survives to the supernova explosion which lead to the neutron star formation. On the other hand, the extremely high stellar density in the core of GCs, relative to most of the rest of the Galaxy, favors the formation of several different binary systems, suitable for the recycling of NSs (Davies at al. 1998). In this thesis we will present the properties two millisecond pulsars companions discovered in two globular clusters, the Helium white dwarf orbiting the MSP PSR 1911-5958A in NGC 6752 and the second case of a tidally deformed star orbiting an eclipsing millisecond pulsar, PSR J1701-3006B in NGC6266

Aumento della risoluzione spaziale per il sondaggio di temperatura e umidità da satellite geostazionario mediante radiometria ad onde millimetriche e submillimetriche

The purpose of this study is to develop and evaluate techniques that improve the spatial resolution of the channels already selected in the preliminary studies for Geostationary Observatory for Microwave Atmospheric Soundings (GOMAS). Reference high resolution multifrequency brightness temperatures scenarios have been derived by applying radiative transfer calculation to the spatially and microphysically detailed output of meteorological events simulated by the University of Wisconsin - Non-hydrostatic Model System (UW-NMS). Three approaches, Wiener filter, Super-Resolution and Image Fusion have been applied to some representative GOMAS frequency channels to enhance the resolution of antenna temperatures. The Wiener filter improved resolution of the largely oversampled images by a factor 1.5- 2.0 without introducing any penalty in the radiometric accuracy. Super-resolution, suitable for not largely oversampled images, improved resolution by a factor ~1.5 but introducing an increased radiometric noise by a factor 1.4-2.5. The image fusion allows finally to further increase the spatial frequency of the images obtained by the Wiener filter increasing the total resolution up to a factor 5.0 with an increased radiometric noise closely linked to the radiometric frequency and to the examined case study.

Formazione, apprendimento e nuove prospettive e-learning. Lo sviluppo delle nuove tecnologie didattiche e la creazione di sistemi di apprendimento lungo l’intero arco della vita

The thesis of this paper is based on the assumption that the socio-economic system in which we are living is characterised by three great trends: growing attention to the promotion of human capital; extremely rapid technological progress, based above all on the information and communication technologies (ICT); the establishment of new production and organizational set-ups. These transformation processes pose a concrete challenge to the training sector, which is called to satisfy the demand for new skills that need to be developed and disseminated. Hence the growing interest that the various training sub-systems devote to the issues of lifelong learning and distance learning. In such a context, the so-called e-learning acquires a central role. The first chapter proposes a reference theoretical framework for the transformations that are shaping post-industrial society. It analyzes some key issues such as: how work is changing, the evolution of organizational set-ups and the introduction of learning organization, the advent of the knowledge society and of knowledge companies, the innovation of training processes, and the key role of ICT in the new training and learning systems. The second chapter focuses on the topic of e-learning as an effective training model in response to the need for constant learning that is emerging in the knowledge society. This chapter starts with a reflection on the importance of lifelong learning and introduces the key arguments of this thesis, i.e. distance learning (DL) and the didactic methodology called e-learning. It goes on with an analysis of the various theoretic and technical aspects of e-learning. In particular, it delves into the theme of e-learning as an integrated and constant training environment, characterized by customized programmes and collaborative learning, didactic assistance and constant monitoring of the results. Thus, all the aspects of e-learning are taken into exam: the actors and the new professionals, the virtual communities as learning subjects, the organization of contents in learning objects, the conformity to international standards, the integrated platforms and so on. The third chapter, which concludes the theoretic-interpretative part, starts with a short presentation of the state-of-the-art e-learning international market that aims to understand its peculiarities and its current trends. Finally, we focus on some important regulation aspects related to the strong impulse given by the European Commission first, and by the Italian governments secondly, to the development and diffusion of e-learning. The second part of the thesis (chapters 4, 5 and 6) focus on field research, which aims to define the Italian scenario for e-learning. In particular, we have examined some key topics such as: the challenges of training and the instruments to face such challenges; the new didactic methods and technologies for lifelong learning; the level of diffusion of e-learning in Italy; the relation between classroom training and online training; the main factors of success as well as the most critical aspects of the introduction of e-learning in the various learning environments. As far as the methodological aspects are concerned, we have favoured a qualitative and quantitative analysis. A background analysis has been done to collect the statistical data available on this topic, as well as the research previously carried out in this area. The main source of data is constituted by the results of the Observatory on e-learning of Aitech-Assinform, which covers the 2000s and four areas of implementation (firms, public administration, universities, school): the thesis has reviewed the results of the last three available surveys, offering a comparative interpretation of them. We have then carried out an in-depth empirical examination of two case studies, which have been selected by virtue of the excellence they have achieved and can therefore be considered advanced and emblematic experiences (a large firm and a Graduate School).

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.

LBT AO system: tests and calibration

An Adaptive Optic (AO) system is a fundamental requirement of 8m-class telescopes. We know that in order to obtain the maximum possible resolution allowed by these telescopes we need to correct the atmospheric turbulence. Thanks to adaptive optic systems we are able to use all the effective potential of these instruments, drawing all the information from the universe sources as best as possible. In an AO system there are two main components: the wavefront sensor (WFS) that is able to measure the aberrations on the incoming wavefront in the telescope, and the deformable mirror (DM) that is able to assume a shape opposite to the one measured by the sensor. The two subsystem are connected by the reconstructor (REC). In order to do this, the REC requires a “common language" between these two main AO components. It means that it needs a mapping between the sensor-space and the mirror-space, called an interaction matrix (IM). Therefore, in order to operate correctly, an AO system has a main requirement: the measure of an IM in order to obtain a calibration of the whole AO system. The IM measurement is a 'mile stone' for an AO system and must be done regardless of the telescope size or class. Usually, this calibration step is done adding to the telescope system an auxiliary artificial source of light (i.e a fiber) that illuminates both the deformable mirror and the sensor, permitting the calibration of the AO system. For large telescope (more than 8m, like Extremely Large Telescopes, ELTs) the fiber based IM measurement requires challenging optical setups that in some cases are also impractical to build. In these cases, new techniques to measure the IM are needed. In this PhD work we want to check the possibility of a different method of calibration that can be applied directly on sky, at the telescope, without any auxiliary source. Such a technique can be used to calibrate AO system on a telescope of any size. We want to test the new calibration technique, called “sinusoidal modulation technique”, on the Large Binocular Telescope (LBT) AO system, which is already a complete AO system with the two main components: a secondary deformable mirror with by 672 actuators, and a pyramid wavefront sensor. My first phase of PhD work was helping to implement the WFS board (containing the pyramid sensor and all the auxiliary optical components) working both optical alignments and tests of some optical components. Thanks to the “solar tower” facility of the Astrophysical Observatory of Arcetri (Firenze), we have been able to reproduce an environment very similar to the telescope one, testing the main LBT AO components: the pyramid sensor and the secondary deformable mirror. Thanks to this the second phase of my PhD thesis: the measure of IM applying the sinusoidal modulation technique. At first we have measured the IM using a fiber auxiliary source to calibrate the system, without any kind of disturbance injected. After that, we have tried to use this calibration technique in order to measure the IM directly “on sky”, so adding an atmospheric disturbance to the AO system. The results obtained in this PhD work measuring the IM directly in the Arcetri solar tower system are crucial for the future development: the possibility of the acquisition of IM directly on sky means that we are able to calibrate an AO system also for extremely large telescope class where classic IM measurements technique are problematic and, sometimes, impossible. Finally we have not to forget the reason why we need this: the main aim is to observe the universe. Thanks to these new big class of telescopes and only using their full capabilities, we will be able to increase our knowledge of the universe objects observed, because we will be able to resolve more detailed characteristics, discovering, analyzing and understanding the behavior of the universe components.

Massenspektrometrische in-situ Messungen zur Bestimmung der chemischen Zusammensetzung von natürlichem und anthropogenem Aerosol

Für die vorliegende Arbeit wurde die chemische Zusammensetzung von natürlichen und anthropogenen Aerosolpartikeln untersucht. Zu diesem Zweck wurde das Aerosolmassenspektrometer (AMS) der Firma Aerodyne, Inc. eingesetzt, womit neben den chemischen Substanzen auch die Massengrößenverteilungen der einzelnen Komponenten der Aerosolpartikel in einem Größenbereich zwischen 20 und 1500 nm quantitativ gemessen werden können. Im Rahmen der HAZE2002-Messkampagne am Meteorologischen Observatorium Hohenpeißenberg wurden die Aerosolpartikel aus natürlichen Quellen untersucht. Diese Partikel bestanden aus Sulfat, Nitrat, Ammonium und organischen Komponenten (Organics). Sulfat, Nitrat und Ammonium wiesen den gleichen Durchmesser auf, was auf eine interne Mischung dieser drei chemischen Substanzen in den Partikeln hinwies. Die Organics hatten einen kleineren Durchmesser, was auf jüngere Partikel hindeutete. Die Analyse der organischen Substanzen in den Aerosolpartikeln zeigte, dass diese zu einem großen Teil aus oxidierten Kohlenwasserstoffen bestanden, die während den Nachmittagsstunden gebildet wurden. Die thermische Abhängigkeit der Bildung von Ammoniumnitrat konnte sowohl gemessen als auch mit Hilfe Konzentrationsberechnungen nach [Seinfeld und Pandis, 1998] nachvollzogen werden. Die gemessene Partikelneubildung konnte auf die ternäre Nukleation aus H2SO4/H2O/NH3 zurückgeführt werden. Aerosolpartikel aus anthropogenen Quellen, wie z.B. der motorischen Verbrennung, wurden während der Messungen in Zusammenarbeit mit dem Ford Forschungszentrum in Aachen (FFA) untersucht. Nukleationspartikel (D 45 nm) konnten bei Experimenten auf dem Rollenprüfstand nur bei einer ausreichend hohen Verdünnung, einem hohen Schwefelgehalt im Kraftstoff und einem hohen Lastzustand nachgewiesen werden. Die Messungen an der Autobahn A4 ergaben eine bimodale Massengrößenverteilung der organischen Partikel, wobei die erste Mode Partikeln aus der motorischen Verbrennungen zugeschrieben werden konnte. Aufgrund der guten Charakterisierung stellt das AMS ein vielseitig einsetzbares Aerosolmessgerät dar, welches in einer hohen Zeitauflösung eine quantitative, größenaufgelöste chemische Analyse der zu messenden Aerosolpartikel bereitstellt.

Application of comprehensive gas chromatography (GCxGC) to measurements of volatile organic species in ambient air

The focus of this thesis was the in-situ application of the new analytical technique "GCxGC" in both the marine and continental boundary layer, as well as in the free troposphere. Biogenic and anthropogenic VOCs were analysed and used to characterise local chemistry at the individual measurement sites. The first part of the thesis work was the characterisation of a new set of columns that was to be used later in the field. To simplify the identification, a time-of-flight mass spectrometer (TOF-MS) detector was coupled to the GCxGC. In the field the TOF-MS was substituted by a more robust and tractable flame ionisation detector (FID), which is more suitable for quantitative measurements. During the process, a variety of volatile organic compounds could be assigned to different environmental sources, e.g. plankton sources, eucalyptus forest or urban centers. In-situ measurements of biogenic and anthropogenic VOCs were conducted at the Meteorological Observatory Hohenpeissenberg (MOHP), Germany, applying a thermodesorption-GCxGC-FID system. The measured VOCs were compared to GC-MS measurements routinely conducted at the MOHP as well as to PTR-MS measurements. Furthermore, a compressed ambient air standard was measured from three different gas chromatographic instruments and the results were compared. With few exceptions, the in-situ, as well as the standard measurements, revealed good agreement between the individual instruments. Diurnal cycles were observed, with differing patterns for the biogenic and the anthropogenic compounds. The variability-lifetime relationship of compounds with atmospheric lifetimes from a few hours to a few days in presence of O3 and OH was examined. It revealed a weak but significant influence of chemistry on these short-lived VOCs at the site. The relationship was also used to estimate the average OH radical concentration during the campaign, which was compared to in-situ OH measurements (1.7 x 10^6 molecules/cm^3, 0.071 ppt) for the first time. The OH concentration ranging from 3.5 to 6.5 x 10^5 molecules/cm^3 (0.015 to 0.027 ppt) obtained with this method represents an approximation of the average OH concentration influencing the discussed VOCs from emission to measurement. Based on these findings, the average concentration of the nighttime NO3 radicals was estimated using the same approach and found to range from 2.2 to 5.0 x 10^8 molecules/cm^3 (9.2 to 21.0 ppt). During the MINATROC field campaign, in-situ ambient air measurements with the GCxGC-FID were conducted at Tenerife, Spain. Although the station is mainly situated in the free troposphere, local influences of anthropogenic and biogenic VOCs were observed. Due to a strong dust event originating from Western Africa it was possible to compare the mixing ratios during normal and elevated dust loading in the atmosphere. The mixing ratios during the dust event were found to be lower. However, this could not be attributed to heterogeneous reactions as there was a change in the wind direction from northwesterly to southeasterly during the dust event.

HCHO, H 2 O 2 und CH 3 OOH in der Troposphäre

In dieser Arbeit wurden im Rahmen der UTOPIHAN- und HOHPEX04-Projekte Peroxid- und Formaldehydmessungen in der Troposphäre durchgeführt und wissenschaftlich interpretiert. Die Messungen während UTOPIHAN fanden dabei an Bord eines für Forschungszwecke umgerüsteten Flugzeuges (Learjet 35A) im Wesentlichen in der freien, insbesondere in der oberen Troposphäre über Europa statt. Die Messungen während HOHPEX04 waren hingegen als Bodenmessungen an der sich abwechselnd in der bodennahen Grenzschicht und in von dieser Schicht entkoppelten Luftmassen liegenden Bergstation Hohenpeißenberg (bayerisches Voralpenland) konzipiert. Um eine quantitative Auswertbarkeit der Messungen sicherzustellen, wurden die verwendeten, auf chemischer Derivatisierung und fluorimetrischer Detektion basierenden Messgeräte AL 2001CA (Peroxide) und AL 4021 (Formaldehyd) (AEROLASER) genau charakterisiert. Dabei wurde speziell die bekannte Ozoninterferenz beider Geräte in einer großen Zahl von Laborexperimenten mit unterschiedlichen Randbedingungen bezüglich Wasserdampf- und Kohlenwasserstoffgehalt der Luft untersucht. Für beide Verbindungen wurden Höhen- sowie Breitenprofile erstellt und mit Ergebnissen eines 3D-Chemie-Transport-Modells (CTM) sowie früherer Studien verglichen. In einem weiteren Kapitel werden Ergebnisse einer quantitativen Studie zum Einfluss hochreichender Konvektion auf das HCHO-Budget in der mittleren und oberen Troposphäre präsentiert. Diese Studie kommt zu dem Schluss, dass der rasche Aufwärtstransport von Vorläufergasen von HCHO und HOx wie Methanol, Aceton und sogar gut löslicher Spurengase wie CH3OOH beziehungsweise H2O2 aus der Grenzschicht einen signifikanten, auf Grund der längeren Lebensdauer von NOx über mehrere Tage andauernden und damit großräumigen Einfluss auf die Budgets von HCHO, HOx und auch O3 in der oberen Troposphäre haben kann. Die Befunde der Studie legen desweiteren nahe, dass fehlerhafte Modellvorhersagen für die NO-Mischungsverhältnisse in der Tropopausenregion, die zum Beispiel mit Mängeln des Modells bezüglich der Höhe der Konvektion und des Stratosphären-Troposphären-Austauschs zu tun haben, hauptverantwortlich sind für gefundene Differenzen zwischen Messdaten und dem verwendeten 3D-Chemie-Transport-Modell. Um die Signifikanz der Aussagen zu erhöhen, wurde eine Sensitivitätsstudie durchgeführt, in der die Konzentration einiger chemischer Verbindungen sowie die Photolyseraten variiert wurden. Eine weitere Studie zum Einfluss verschiedener Parameter auf das CH3OOH/H2O2-Verhältnis kommt zu dem Schluss, dass dieses Verhältnis keinen idealen Indikator für Wolkenprozessierung von Luftmassen darstellt, während eine signifikant positive Abweichung vom H2O2/H2O-Verhältnis in der oberen Troposphäre ein guter Indikator für rasch aufwärts transportierte Luftmassen sein kann. Im Rahmen dieser Studie werden auch Höhen- und Breitenprofile des CH3OOH/H2O2-Verhältnisses diskutiert. In einer letzten Untersuchung zu HCHO-Messungen am Observatorium Hohenpeißenberg im Sommer 2004 werden für die in zwei Windrichtungssektoren eingeteilten Daten Korrelationen anderer Spurengase wie O3, PAN, CO, NOy und Isopren mit HCHO interpretiert. In diesem Zusammenhang wird auch versucht, den beobachteten Tagesgang von HCHO zu erklären.

La Ricostruzione 3D di Bologna nel XVI Secolo

Il lavoro presentato ha come oggetto la ricostruzione tridimensionale della città di Bologna nella sua fase rinascimentale. Tale lavoro vuole fornire un modello 3D delle architetture e degli spazi urbani utilizzabile sia per scopi di ricerca nell’ambito della storia delle città sia per un uso didattico-divulgativo nel settore del turismo culturale. La base del lavoro è una fonte iconografica di grande importanza: l’affresco raffigurante Bologna risalente al 1575 e situato in Vaticano; questa è una veduta a volo d’uccello di grandi dimensioni dell’intero tessuto urbano bolognese all’interno della terza cerchia di mura. In esso sono rappresentate in maniera particolareggiata le architetture civili e ecclesiastiche, gli spazi ortivi e cortilivi interni agli isolati e alcune importanti strutture urbane presenti in città alla fine del Cinquecento, come l’area portuale e i canali interni alla città, oggi non più visibili. La ricostruzione tridimensionale è stata realizzata tramite Blender, software per la modellazione 3D opensource, attraverso le fasi di modellazione, texturing e creazione materiali (mediante campionamento delle principali cromie presenti nell’affresco), illuminazione e animazione. Una parte della modellazione è stata poi testata all’interno di un GIS per verificare l’utilizzo delle geometrie 3D come elementi collegabili ad altre fonti storiche relative allo sviluppo urbano e quindi sfruttabili per la ricerca storica. Grande attenzione infine è stata data all’uso dei modelli virtuali a scopo didattico-divulgativo e per il turismo culturale. La modellazione è stata utilizzata all’interno di un motore grafico 3D per costruire un ambiente virtuale interattivo nel quale un utente anche non esperto possa muoversi per esplorare gli spazi urbani della Bologna del Cinquecento. In ultimo è stato impostato lo sviluppo di un’applicazione per sistemi mobile (Iphone e Ipad) al fine di fornire uno strumento per la conoscenza della città storica in mobilità, attraverso la comparazione dello stato attuale con quello ricostruito virtualmente.

Untersuchungen zur troposphärischen Photochemie am GAW-Observatorium Izana

Im Rahmen dieser Promotionsarbeit wurden Fragestellungen der troposphärischen Ozonproduktion, des photostationären Gleichgewicht des NO2-NO-O3-ROx-Systems, des Einflusses von heterogenen Reaktionen an Mineralstauboberflächen und der Bedeutung lokaler anthropogener Emissionen für Spurengasmessungen an einem Gebirgsobservatorium untersucht. Dazu wurde insbesondere ein atmosphärenchemisch-meteorologischer Datensatz ausgewertet, welcher während der Feldmesskampagne MINATROC II im Juli/August 2002 am Global Atmosphere Watch (GAW) Observatorium Izana (2360m über NN) auf Teneriffa gewonnen wurde. Der Datensatz enthält Messdaten von Aerosolen, Spurengasen, Strahlungsgrößen und meteorologischen Parametern. Eine dichte Sahara-Staubwolke passierte die Messstation zwischen dem 28. und 31.07.2002. Die Mischungsverhältnisse von O3, H2O2, NOx und ROx zeigten während dieses Ereignisses Abnahmen zwischen 10% und 50%. Insbesondere infolge der Reduktion von NO und HO2 wurde eine deutliche Verringerung der Netto-Ozon-Produktion in der Staubwolke berechnet. Die Bewertung der verschiedenen Terme der Ozonproduktion bzw. –vernichtung zeigte relativ geringe Beiträge der einzelnen photochemischen Verlustreaktionen am Ozonbudget. Im Rahmen einer Boxmodellstudie, welche die Eingangsdaten von MINATROC II verwendete, wurde ein Vergleich zwischen Simulation und Messung kurzlebiger Spurengase angestellt. Die Modellrechnungen weisen darauf hin, dass die reduzierten H2O2-Mischungsverhältnisse in der Sahara-Staubwolke unter Berücksichtigung heterogener Reaktionen von HO2 bzw. H2O2 an Stauboberflächen erklärt werden können. Die Betrachtungen zum photostationären Gleichgewicht des NO2-NO-O3-ROx-Systems ergeben hauptsächlich stark überhöhte Leighton-Verhältnisse. Die Abweichungen der Messdaten vom photostationären Gleichgewichtszustand sind dabei zum Verschmutzungsgrad der Atmosphäre antikorreliert. Eine Reihe potentieller Einflüsse auf das NO2-NO-O3-ROx-System wurde diskutiert, wobei gezeigt werden konnte, dass das bisherige Betrachtungsmodell nicht ausreicht, um die beobachteten Abweichungen vom photostationären Gleichgewicht zu erklären. Während für die Nachtmessungen von MINATROC II Bedingungen der freien Troposphäre vorlagen, waren die Messungen am Tage von der Kopplung zwischen photochemischer Aktivität und thermisch getriebener Hangströmung betroffen. Die zum Messort gelangte anthropogen beeinflusste Grenzschichtluft konnte dabei auf maximalen Mischungsanteilen zwischen 15% und 85% quantifiziert werden. Abschließend wurden verschiedene Aspekte der Quellen und der Verteilung anthropogener Verschmutzungen auf Teneriffa im Zusammenhang der zuvor behandelten Fragen diskutiert.

L’esperienza turistica tra pratica di consumo e fattore di sviluppo locale sostenibile

La società dei consumi ha reso ogni ambito vitale suscettibile di mercificazione. Il capitalismo ha da tempo svestito la prassi produttiva dei suoi elementi più pesanti per vestire i panni della dimensione simbolica e culturale. Il consumo fattosi segno, dimensione immateriale delle nostre vite materiali, ha finito per colonizzare l'ambito dell'esperienza e, quindi, della vita stessa. Il consumo diventa, innanzitutto, esperienza di vita. Una esperienza continuamente cangiante che ci permette di vivere numerose vite, ognuna diversa. Ciò che è stabile è il paradigma consumistico che investe la nostra stessa identità, l'identità dei luoghi, l'identità del mondo. Il nomadismo è la dimensione più tipica del consumo, così come la perenne mobilità della vita è la dimensione propria dell'epoca globale. Tuttavia, le nuove forme di consumerismo politico, etico e responsabile, conseguenti al montare dei rischi globali, investendo proprio l’ambito dell’esperienza e del consumo, contribuiscono a modificare i comportamenti in senso “riflessivo” e “glocale”. L’ambito turistico, rappresentando al contempo il paradigma esperienziale e quello della mobilità globale, può diventare allora l’osservatorio privilegiato per indagare queste stesse forme riflessive di consumo, le quali forniscono un significato del tutto nuovo tanto all’esperienza quanto al consumo stesso. Il lavoro di tesi vuole allora approfondire, attraverso lo studio di caso, il modo in cui nuove forme emergenti di turismo responsabile possano rappresentare una chiave d’accesso a nuove forme di sviluppo sostenibile dei territori locali in contesti di prima modernizzazione.