Results from the HST/COS FUV detector "lifetime move"

We describe the planning, implementation, and initial results of the first planned move of the default position of spectra on the Hubble Space Telescope's Cosmic Origins Spectrograph (COS) Far Ultraviolet (FUV) cross-delay line detector. This was motivated by the limited amount of charge that can be extracted from the microchannel plate due to gain sag at any one position. Operations at a new location began on July 23, 2012, with a shift of the spectrum by +3.5"(corresponding to ~ 41 pixels or ~ 1 mm) in a direction orthogonal to the spectral dispersion. Operation at this second "lifetime position" allows for spectra to be collected which are not affected by detector artifacts and loss of sensitivity due to gain sag. We discuss programs designed to enable operations at the new lifetime position; these include determinations of operational high voltage, measuring walk corrections and focus, confirming spectrum placement and aperture centering, and target acquisition performance. We also present results related to calibration of the new lifetime position, including measurements of spectral resolution and wavelength calibration, flux and flat field calibration, carryover of time-dependent sensitivity monitoring, and operations with the Bright Object Aperture (BOA).

Epidemiological aspects of American cutaneous leishmaniasis and phlebotomine sandfly population, in the municipality of Monte Negro, State of Rondônia, Brazil

INTRODUCTION: This work was carried out on the purpose of identifying the species of phlebotomine sandflies in the municipality of Monte Negro, state of Rondonia, Brazil, that may have been transmitting the American cutaneous leishmaniasis (ACL), and concisely describe epidemiological aspects of disease. METHODS: The epidemiologic and socioeconomical indicators were obtained from government institutions and the local Municipal Secretary of Health. Phlebotomine sandflies were captured using CDC light traps between July 2006 to July 2008. The total of 1,240 of female sandflies were examined by PCR method directed to k-DNA. RESULTS: There has been a significant decrease in the incidence of ACL of about 50% over the last ten years in the municipality. A total of 1,935 specimens of 53 sandfly species were captured, three of the genus Brumptomyia genus and 50 of the genus Lutzomyia. The predominant species was Lutzomyia acanthopharynx, Lutzomyia whitmani, Lutzomyia geniculata and Lutzomyia davisi. None were positive for Leishmania sp. CONCLUSIONS: Four sandflies species were found in the State of Rondonia for the first time: Brumptomyia brumpti, Lutzomyia tarapacaensis, Lutzomyia melloi and Lutzomyia lenti. The presence of Lutzomyia longipalpis, was also captured. Socioeconomical improvement of Brazilian economy and the increase of environmental surveillance in the last 15 years collaborated in the decrease of people exposed to vectors, reducing the incidence of ACL.

Origin of the heavy elements in HD 140283: measurement of europium abundance

Context. HD140283 is a nearby (V = 7:7) subgiant metal-poor star, extensively analysed in the literature. Although many spectra have been obtained for this star, none showed a signal-to-noise (S/N) ratio high enough to enable a very accurate derivation of abundances from weak lines. Aims. The detection of europium proves that the neutron-capture elements in this star originate in the r-process, and not in the s-process, as recently claimed in the literature. Methods. Based on the OSMARCS 1D LTE atmospheric model and with a consistent approach based on the spectrum synthesis code Turbospectrum, we measured the europium lines at 4129 Å and 4205 Å, taking into account the hyperfine structure of the transitions. The spectrum, obtained with a long exposure time of seven hours at the Canada-France-Hawaii Telescope (CFHT), has a resolving power of 81 000 and a S/N ratio of 800 at 4100 Å. Results. We were able to determine the abundance A(Eu) =

3C 273 variability at 7 mm: evidence of shocks and precession in the jet

We report on four years of observations of 3C 273 at 7mm obtained with the Itapetinga radio telescope, in Brazil, between 2009 and 2013. We detected a flare in 2010 March, when the flux density increased by 50 per cent and reached 35 Jy. After the flare, the flux density started to decrease and reached values lower than 10 Jy. We suggest that the 7-mm flare is the radio counterpart of the γ -ray flare observed by the Fermi Large Area Telescope in 2009 September, in which the flux density at high energies reached a factor of 50 of its average value. A delay of 170 d between the radio and γ -ray flares was revealed using the discrete correlation function (DCF) that can be interpreted in the context of a shock model, in which each flare corresponds to the formation of a compact superluminal component that expands and becomes optically thin at radio frequencies at latter epochs. The differences in flare intensity between frequencies and at different times are explained as a consequence of an increase in the Doppler factor δ, as predicted by the 16-yr precession model proposed by Abraham & Romero. This increase has a large effect on boosting at high frequencies while it does not affect the observed optically thick radio emission too much. We discuss other observable effects of the variation in δ, such as the increase in the formation rate of superluminal components, the variations in the time delay between flares and the periodic behaviour of the radio light curve that we have found to be compatible with changes in the Doppler factor.

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.

Autophagic programmed cell death in the suspensor and endosperm of Vicia faba : An ultrastructural study

Programmed cell death (PCD) is a widely spread phenomenon among multi-cellular organisms. Without the deletion of cells no longer needed, the organism will not be able to develop in a predicted way. It is now belived that all cells have the capacity to self-destruct and that the survival of the cells is depending on the repression of this suicidal programme. PCD has turned out to show similarities in many different species and there are strong indications that the mechanisms running the programme might, at least in some parts, be evolutionarily conserced. PCD is a generic term for different programmes of cell destruction, such as apoptosis and autophagic PCD. An important tool to determine if a cell is undergoing PCD is the transmitting electron microscope. The aims of my study were to find out if, and in what way, the suspensor and endosperm in Vicia faba (Broad bean), which are short-lived structures, undergoes PCD. The endosperm degradation preceed the suspensor cell death and they differ to some extent ultrastructurally. The cell death occurs in both tissues about 13-14 days after pollination when the embryo proper is mature enough to support itself. It was found that both tissues are committed to autophagic PCD, a cell death characteristic of conspicuous formations of autophagic vacuoles. It was shown by histochemical staining that acid phosphatases are accumulated in these vacuoles but are also present in the cytoplasm. These vacuoles are similar to autophagic vacuoles formed in rat liver cells, indicating that autophagy is a widely spread phenomenon. DNA fragmentation is the first visible sign of PCD in both tissues and it is demonstrated by a labelling technique (TUNEL). In the endosperm nuclei the heterochromatin subsequently appears in the form of a network, while in the suspensor it is more conspicuous, with heterochromatin that forms large electron dense aggregates located close to the nuclear envelope. In the suspensor, the plastids develop into chromoplasts with lycopene crystals at the same time or shortly after DNA fragmentation. This is probably due to the fact that the suspensor plastids function as hormone producing organelles and support the embryo proper with indispensable growth factors. Later the embryo will be able to produce its own growth factors and the synthesis of these, in particular gibberelines, might be suppressed in the suspensor. The precursors can then be used for synthesis of lycopene instead. Both the suspensor and endosperm are going through autophagic PCD, but the process differs in some respects. This is probably due the the different function of the two tissues, and that the signals that trigger the process presumably are different. The embryo proper is probably the source of the death signal affecting the suspensor. The endosperm, which has a different origin and function, might be controlling the death signal within its own cell. The death might in this case be related to the age of the cell.

Molecular gas in the galaxy M83 : Its distribution, kinematics, and relation to star formation

The barred spiral galaxy M83 (NGC5236) has been observed in the 12CO J=1–0 and J=2–1 millimetre lines with the Swedish-ESO Submillimetre Telescope (SEST). The sizes of the CO maps are 100×100, and they cover the entire optical disk. The CO emission is strongly peaked toward the nucleus. The molecular spiral arms are clearly resolved and can be traced for about 360º. The total molecular gas mass is comparable to the total Hi mass, but H2 dominates in the optical disk. Iso-velocity maps show the signature of an inclined, rotating disk, but also the effects of streaming motions along the spiral arms. The dynamical mass is determined and compared to the gas mass. The pattern speed is determined from the residual velocity pattern, and the locations of various resonances are discussed. The molecular gas velocity dispersion is determined, and a trend of decreasing dispersion with increasing galactocentric radius is found. A total gas (H2+Hi+He) mass surface density map is presented, and compared to the critical density for star formation of an isothermal gaseous disk. The star formation rate (SFR) in the disk is estimated using data from various star formation tracers. The different SFR estimates agree well when corrections for extinctions, based on the total gas mass map, are made. The radial SFR distribution shows features that can be associated with kinematic resonances. We also find an increased star formation efficiency in the spiral arms. Different Schmidt laws are fitted to the data. The star formation properties of the nuclear region, based on high angular resolution HST data, are also discussed.

A Dark Matter Search with AMANDA : Limits on the Muon Flux from Neutralino Annihilations at the Centre of the Earth with 1997-99 Data

The nature of the dark matter in the Universe is one of the greatest mysteries in modern astronomy. The neutralino is a nonbaryonic dark matter candidate in minimal supersymmetric extensions to the standard model of particle physics. If the dark matter halo of our galaxy is made up of neutralinos some would become gravitationally trapped inside massive bodies like the Earth. Their pair-wise annihilation produces neutrinos that can be detected by neutrino experiments looking in the direction of the centre of the Earth. The AMANDA neutrino telescope, currently the largest in the world, consists of an array of light detectors buried deep in the Antarctic glacier at the geographical South Pole. The extremely transparent ice acts as a Cherenkov medium for muons passing the array and using the timing information of detected photons it is possible to reconstruct the muon direction. A search has been performed for nearly vertically upgoing neutrino induced muons with AMANDA-B10 data taken over the three year period 1997-99. No excess above the atmospheric neutrino background expectation was found. Upper limits at the 90 % confidence level has been set on the annihilation rate of neutralinos at the centre of the Earth and on the muon flux induced by neutrinos created by the annihilation products.

Multiwavelenght study of cluster mergers and consequences for the radio emission properties of galaxy clusters

In the present thesis a thourough multiwavelength analysis of a number of galaxy clusters known to be experiencing a merger event is presented. The bulk of the thesis consists in the analysis of deep radio observations of six merging clusters, which host extended radio emission on the cluster scale. A composite optical and X–ray analysis is performed in order to obtain a detailed and comprehensive picture of the cluster dynamics and possibly derive hints about the properties of the ongoing merger, such as the involved mass ratio, geometry and time scale. The combination of the high quality radio, optical and X–ray data allows us to investigate the implications of the ongoing merger for the cluster radio properties, focusing on the phenomenon of cluster scale diffuse radio sources, known as radio halos and relics. A total number of six merging clusters was selected for the present study: A3562, A697, A209, A521, RXCJ 1314.4–2515 and RXCJ 2003.5–2323. All of them were known, or suspected, to possess extended radio emission on the cluster scale, in the form of a radio halo and/or a relic. High sensitivity radio observations were carried out for all clusters using the Giant Metrewave Radio Telescope (GMRT) at low frequency (i.e. ≤ 610 MHz), in order to test the presence of a diffuse radio source and/or analyse in detail the properties of the hosted extended radio emission. For three clusters, the GMRT information was combined with higher frequency data from Very Large Array (VLA) observations. A re–analysis of the optical and X–ray data available in the public archives was carried out for all sources. Propriety deep XMM–Newton and Chandra observations were used to investigate the merger dynamics in A3562. Thanks to our multiwavelength analysis, we were able to confirm the existence of a radio halo and/or a relic in all clusters, and to connect their properties and origin to the reconstructed merging scenario for most of the investigated cases. • The existence of a small size and low power radio halo in A3562 was successfully explained in the theoretical framework of the particle re–acceleration model for the origin of radio halos, which invokes the re–acceleration of pre–existing relativistic electrons in the intracluster medium by merger–driven turbulence. • A giant radio halo was found in the massive galaxy cluster A209, which has likely undergone a past major merger and is currently experiencing a new merging process in a direction roughly orthogonal to the old merger axis. A giant radio halo was also detected in A697, whose optical and X–ray properties may be suggestive of a strong merger event along the line of sight. Given the cluster mass and the kind of merger, the existence of a giant radio halo in both clusters is expected in the framework of the re–acceleration scenario. • A radio relic was detected at the outskirts of A521, a highly dynamically disturbed cluster which is accreting a number of small mass concentrations. A possible explanation for its origin requires the presence of a merger–driven shock front at the location of the source. The spectral properties of the relic may support such interpretation and require a Mach number M < ∼ 3 for the shock. • The galaxy cluster RXCJ 1314.4–2515 is exceptional and unique in hosting two peripheral relic sources, extending on the Mpc scale, and a central small size radio halo. The existence of these sources requires the presence of an ongoing energetic merger. Our combined optical and X–ray investigation suggests that a strong merging process between two or more massive subclumps may be ongoing in this cluster. Thanks to forthcoming optical and X–ray observations, we will reconstruct in detail the merger dynamics and derive its energetics, to be related to the energy necessary for the particle re–acceleration in this cluster. • Finally, RXCJ 2003.5–2323 was found to possess a giant radio halo. This source is among the largest, most powerful and most distant (z=0.317) halos imaged so far. Unlike other radio halos, it shows a very peculiar morphology with bright clumps and filaments of emission, whose origin might be related to the relatively high redshift of the hosting cluster. Although very little optical and X–ray information is available about the cluster dynamical stage, the results of our optical analysis suggest the presence of two massive substructures which may be interacting with the cluster. Forthcoming observations in the optical and X–ray bands will allow us to confirm the expected high merging activity in this cluster. Throughout the present thesis a cosmology with H0 = 70 km s−1 Mpc−1, m=0.3 and =0.7 is assumed.

Nonlinear/electromagnetic co-simulation of microwaves and millimeter-waves links

The Ph.D. thesis describes the simulations of different microwave links from the transmitter to the receiver intermediate-frequency ports, by means of a rigorous circuit-level nonlinear analysis approach coupled with the electromagnetic characterization of the transmitter and receiver front ends. This includes a full electromagnetic computation of the radiated far field which is used to establish the connection between transmitter and receiver. Digitally modulated radio-frequency drive is treated by a modulation-oriented harmonic-balance method based on Krylov-subspace model-order reduction to allow the handling of large-size front ends. Different examples of links have been presented: an End-to-End link simulated by making use of an artificial neural network model; the latter allows a fast computation of the link itself when driven by long sequences of the order of millions of samples. In this way a meaningful evaluation of such link performance aspects as the bit error rate becomes possible at the circuit level. Subsequently, a work focused on the co-simulation an entire link including a realistic simulation of the radio channel has been presented. The channel has been characterized by means of a deterministic approach, such as Ray Tracing technique. Then, a 2x2 multiple-input multiple-output antenna link has been simulated; in this work near-field and far-field coupling between radiating elements, as well as the environment factors, has been rigorously taken into account. Finally, within the scope to simulate an entire ultra-wideband link, the transmitting side of an ultrawideband link has been designed, and an interesting Front-End co-design technique application has been setup.

Retrieval of trace gases vertical profile in the lower atmosphere combining. Differential Optical Absorption Spectroscopy with radiative transfer models

The motivation for the work presented in this thesis is to retrieve profile information for the atmospheric trace constituents nitrogen dioxide (NO2) and ozone (O3) in the lower troposphere from remote sensing measurements. The remote sensing technique used, referred to as Multiple AXis Differential Optical Absorption Spectroscopy (MAX-DOAS), is a recent technique that represents a significant advance on the well-established DOAS, especially for what it concerns the study of tropospheric trace consituents. NO2 is an important trace gas in the lower troposphere due to the fact that it is involved in the production of tropospheric ozone; ozone and nitrogen dioxide are key factors in determining the quality of air with consequences, for example, on human health and the growth of vegetation. To understand the NO2 and ozone chemistry in more detail not only the concentrations at ground but also the acquisition of the vertical distribution is necessary. In fact, the budget of nitrogen oxides and ozone in the atmosphere is determined both by local emissions and non-local chemical and dynamical processes (i.e. diffusion and transport at various scales) that greatly impact on their vertical and temporal distribution: thus a tool to resolve the vertical profile information is really important. Useful measurement techniques for atmospheric trace species should fulfill at least two main requirements. First, they must be sufficiently sensitive to detect the species under consideration at their ambient concentration levels. Second, they must be specific, which means that the results of the measurement of a particular species must be neither positively nor negatively influenced by any other trace species simultaneously present in the probed volume of air. Air monitoring by spectroscopic techniques has proven to be a very useful tool to fulfill these desirable requirements as well as a number of other important properties. During the last decades, many such instruments have been developed which are based on the absorption properties of the constituents in various regions of the electromagnetic spectrum, ranging from the far infrared to the ultraviolet. Among them, Differential Optical Absorption Spectroscopy (DOAS) has played an important role. DOAS is an established remote sensing technique for atmospheric trace gases probing, which identifies and quantifies the trace gases in the atmosphere taking advantage of their molecular absorption structures in the near UV and visible wavelengths of the electromagnetic spectrum (from 0.25 μm to 0.75 μm). Passive DOAS, in particular, can detect the presence of a trace gas in terms of its integrated concentration over the atmospheric path from the sun to the receiver (the so called slant column density). The receiver can be located at ground, as well as on board an aircraft or a satellite platform. Passive DOAS has, therefore, a flexible measurement configuration that allows multiple applications. The ability to properly interpret passive DOAS measurements of atmospheric constituents depends crucially on how well the optical path of light collected by the system is understood. This is because the final product of DOAS is the concentration of a particular species integrated along the path that radiation covers in the atmosphere. This path is not known a priori and can only be evaluated by Radiative Transfer Models (RTMs). These models are used to calculate the so called vertical column density of a given trace gas, which is obtained by dividing the measured slant column density to the so called air mass factor, which is used to quantify the enhancement of the light path length within the absorber layers. In the case of the standard DOAS set-up, in which radiation is collected along the vertical direction (zenith-sky DOAS), calculations of the air mass factor have been made using “simple” single scattering radiative transfer models. This configuration has its highest sensitivity in the stratosphere, in particular during twilight. This is the result of the large enhancement in stratospheric light path at dawn and dusk combined with a relatively short tropospheric path. In order to increase the sensitivity of the instrument towards tropospheric signals, measurements with the telescope pointing the horizon (offaxis DOAS) have to be performed. In this circumstances, the light path in the lower layers can become very long and necessitate the use of radiative transfer models including multiple scattering, the full treatment of atmospheric sphericity and refraction. In this thesis, a recent development in the well-established DOAS technique is described, referred to as Multiple AXis Differential Optical Absorption Spectroscopy (MAX-DOAS). The MAX-DOAS consists in the simultaneous use of several off-axis directions near the horizon: using this configuration, not only the sensitivity to tropospheric trace gases is greatly improved, but vertical profile information can also be retrieved by combining the simultaneous off-axis measurements with sophisticated RTM calculations and inversion techniques. In particular there is a need for a RTM which is capable of dealing with all the processes intervening along the light path, supporting all DOAS geometries used, and treating multiple scattering events with varying phase functions involved. To achieve these multiple goals a statistical approach based on the Monte Carlo technique should be used. A Monte Carlo RTM generates an ensemble of random photon paths between the light source and the detector, and uses these paths to reconstruct a remote sensing measurement. Within the present study, the Monte Carlo radiative transfer model PROMSAR (PROcessing of Multi-Scattered Atmospheric Radiation) has been developed and used to correctly interpret the slant column densities obtained from MAX-DOAS measurements. In order to derive the vertical concentration profile of a trace gas from its slant column measurement, the AMF is only one part in the quantitative retrieval process. One indispensable requirement is a robust approach to invert the measurements and obtain the unknown concentrations, the air mass factors being known. For this purpose, in the present thesis, we have used the Chahine relaxation method. Ground-based Multiple AXis DOAS, combined with appropriate radiative transfer models and inversion techniques, is a promising tool for atmospheric studies in the lower troposphere and boundary layer, including the retrieval of profile information with a good degree of vertical resolution. This thesis has presented an application of this powerful comprehensive tool for the study of a preserved natural Mediterranean area (the Castel Porziano Estate, located 20 km South-West of Rome) where pollution is transported from remote sources. Application of this tool in densely populated or industrial areas is beginning to look particularly fruitful and represents an important subject for future studies.

Il passato nell’epoca della sua (ri)producibilità digitale. Torino 1943 - 45. Metodologia della ricerca con tecnologie informatiche. Sistema storico-territoriale di informazione multimediale

Se il lavoro dello storico è capire il passato come è stato compreso dalla gente che lo ha vissuto, allora forse non è azzardato pensare che sia anche necessario comunicare i risultati delle ricerche con strumenti propri che appartengono a un'epoca e che influenzano la mentalità di chi in quell'epoca vive. Emergenti tecnologie, specialmente nell’area della multimedialità come la realtà virtuale, permettono agli storici di comunicare l’esperienza del passato in più sensi. In che modo la storia collabora con le tecnologie informatiche soffermandosi sulla possibilità di fare ricostruzioni storiche virtuali, con relativi esempi e recensioni? Quello che maggiormente preoccupa gli storici è se una ricostruzione di un fatto passato vissuto attraverso la sua ricreazione in pixels sia un metodo di conoscenza della storia che possa essere considerato valido. Ovvero l'emozione che la navigazione in una realtà 3D può suscitare, è un mezzo in grado di trasmettere conoscenza? O forse l'idea che abbiamo del passato e del suo studio viene sottilmente cambiato nel momento in cui lo si divulga attraverso la grafica 3D? Da tempo però la disciplina ha cominciato a fare i conti con questa situazione, costretta soprattutto dall'invasività di questo tipo di media, dalla spettacolarizzazione del passato e da una divulgazione del passato parziale e antiscientifica. In un mondo post letterario bisogna cominciare a pensare che la cultura visuale nella quale siamo immersi sta cambiando il nostro rapporto con il passato: non per questo le conoscenze maturate fino ad oggi sono false, ma è necessario riconoscere che esiste più di una verità storica, a volte scritta a volte visuale. Il computer è diventato una piattaforma onnipresente per la rappresentazione e diffusione dell’informazione. I metodi di interazione e rappresentazione stanno evolvendo di continuo. Ed è su questi due binari che è si muove l’offerta delle tecnologie informatiche al servizio della storia. Lo scopo di questa tesi è proprio quello di esplorare, attraverso l’utilizzo e la sperimentazione di diversi strumenti e tecnologie informatiche, come si può raccontare efficacemente il passato attraverso oggetti tridimensionali e gli ambienti virtuali, e come, nel loro essere elementi caratterizzanti di comunicazione, in che modo possono collaborare, in questo caso particolare, con la disciplina storica. La presente ricerca ricostruisce alcune linee di storia delle principali fabbriche attive a Torino durante la seconda guerra mondiale, ricordando stretta relazione che esiste tra strutture ed individui e in questa città in particolare tra fabbrica e movimento operaio, è inevitabile addentrarsi nelle vicende del movimento operaio torinese che nel periodo della lotta di Liberazione in città fu un soggetto politico e sociale di primo rilievo. Nella città, intesa come entità biologica coinvolta nella guerra, la fabbrica (o le fabbriche) diventa il nucleo concettuale attraverso il quale leggere la città: sono le fabbriche gli obiettivi principali dei bombardamenti ed è nelle fabbriche che si combatte una guerra di liberazione tra classe operaia e autorità, di fabbrica e cittadine. La fabbrica diventa il luogo di "usurpazione del potere" di cui parla Weber, il palcoscenico in cui si tengono i diversi episodi della guerra: scioperi, deportazioni, occupazioni .... Il modello della città qui rappresentata non è una semplice visualizzazione ma un sistema informativo dove la realtà modellata è rappresentata da oggetti, che fanno da teatro allo svolgimento di avvenimenti con una precisa collocazione cronologica, al cui interno è possibile effettuare operazioni di selezione di render statici (immagini), di filmati precalcolati (animazioni) e di scenari navigabili interattivamente oltre ad attività di ricerca di fonti bibliografiche e commenti di studiosi segnatamente legati all'evento in oggetto. Obiettivo di questo lavoro è far interagire, attraverso diversi progetti, le discipline storiche e l’informatica, nelle diverse opportunità tecnologiche che questa presenta. Le possibilità di ricostruzione offerte dal 3D vengono così messe a servizio della ricerca, offrendo una visione integrale in grado di avvicinarci alla realtà dell’epoca presa in considerazione e convogliando in un’unica piattaforma espositiva tutti i risultati. Divulgazione Progetto Mappa Informativa Multimediale Torino 1945 Sul piano pratico il progetto prevede una interfaccia navigabile (tecnologia Flash) che rappresenti la pianta della città dell’epoca, attraverso la quale sia possibile avere una visione dei luoghi e dei tempi in cui la Liberazione prese forma, sia a livello concettuale, sia a livello pratico. Questo intreccio di coordinate nello spazio e nel tempo non solo migliora la comprensione dei fenomeni, ma crea un maggiore interesse sull’argomento attraverso l’utilizzo di strumenti divulgativi di grande efficacia (e appeal) senza perdere di vista la necessità di valicare le tesi storiche proponendosi come piattaforma didattica. Un tale contesto richiede uno studio approfondito degli eventi storici al fine di ricostruire con chiarezza una mappa della città che sia precisa sia topograficamente sia a livello di navigazione multimediale. La preparazione della cartina deve seguire gli standard del momento, perciò le soluzioni informatiche utilizzate sono quelle fornite da Adobe Illustrator per la realizzazione della topografia, e da Macromedia Flash per la creazione di un’interfaccia di navigazione. La base dei dati descrittivi è ovviamente consultabile essendo contenuta nel supporto media e totalmente annotata nella bibliografia. È il continuo evolvere delle tecnologie d'informazione e la massiccia diffusione dell’uso dei computer che ci porta a un cambiamento sostanziale nello studio e nell’apprendimento storico; le strutture accademiche e gli operatori economici hanno fatto propria la richiesta che giunge dall'utenza (insegnanti, studenti, operatori dei Beni Culturali) di una maggiore diffusione della conoscenza storica attraverso la sua rappresentazione informatizzata. Sul fronte didattico la ricostruzione di una realtà storica attraverso strumenti informatici consente anche ai non-storici di toccare con mano quelle che sono le problematiche della ricerca quali fonti mancanti, buchi della cronologia e valutazione della veridicità dei fatti attraverso prove. Le tecnologie informatiche permettono una visione completa, unitaria ed esauriente del passato, convogliando tutte le informazioni su un'unica piattaforma, permettendo anche a chi non è specializzato di comprendere immediatamente di cosa si parla. Il miglior libro di storia, per sua natura, non può farlo in quanto divide e organizza le notizie in modo diverso. In questo modo agli studenti viene data l'opportunità di apprendere tramite una rappresentazione diversa rispetto a quelle a cui sono abituati. La premessa centrale del progetto è che i risultati nell'apprendimento degli studenti possono essere migliorati se un concetto o un contenuto viene comunicato attraverso più canali di espressione, nel nostro caso attraverso un testo, immagini e un oggetto multimediale. Didattica La Conceria Fiorio è uno dei luoghi-simbolo della Resistenza torinese. Il progetto è una ricostruzione in realtà virtuale della Conceria Fiorio di Torino. La ricostruzione serve a arricchire la cultura storica sia a chi la produce, attraverso una ricerca accurata delle fonti, sia a chi può poi usufruirne, soprattutto i giovani, che, attratti dall’aspetto ludico della ricostruzione, apprendono con più facilità. La costruzione di un manufatto in 3D fornisce agli studenti le basi per riconoscere ed esprimere la giusta relazione fra il modello e l’oggetto storico. Le fasi di lavoro attraverso cui si è giunti alla ricostruzione in 3D della Conceria: . una ricerca storica approfondita, basata sulle fonti, che possono essere documenti degli archivi o scavi archeologici, fonti iconografiche, cartografiche, ecc.; . La modellazione degli edifici sulla base delle ricerche storiche, per fornire la struttura geometrica poligonale che permetta la navigazione tridimensionale; . La realizzazione, attraverso gli strumenti della computer graphic della navigazione in 3D. Unreal Technology è il nome dato al motore grafico utilizzato in numerosi videogiochi commerciali. Una delle caratteristiche fondamentali di tale prodotto è quella di avere uno strumento chiamato Unreal editor con cui è possibile costruire mondi virtuali, e che è quello utilizzato per questo progetto. UnrealEd (Ued) è il software per creare livelli per Unreal e i giochi basati sul motore di Unreal. E’ stata utilizzata la versione gratuita dell’editor. Il risultato finale del progetto è un ambiente virtuale navigabile raffigurante una ricostruzione accurata della Conceria Fiorio ai tempi della Resistenza. L’utente può visitare l’edificio e visualizzare informazioni specifiche su alcuni punti di interesse. La navigazione viene effettuata in prima persona, un processo di “spettacolarizzazione” degli ambienti visitati attraverso un arredamento consono permette all'utente una maggiore immersività rendendo l’ambiente più credibile e immediatamente codificabile. L’architettura Unreal Technology ha permesso di ottenere un buon risultato in un tempo brevissimo, senza che fossero necessari interventi di programmazione. Questo motore è, quindi, particolarmente adatto alla realizzazione rapida di prototipi di una discreta qualità, La presenza di un certo numero di bug lo rende, però, in parte inaffidabile. Utilizzare un editor da videogame per questa ricostruzione auspica la possibilità di un suo impiego nella didattica, quello che le simulazioni in 3D permettono nel caso specifico è di permettere agli studenti di sperimentare il lavoro della ricostruzione storica, con tutti i problemi che lo storico deve affrontare nel ricreare il passato. Questo lavoro vuole essere per gli storici una esperienza nella direzione della creazione di un repertorio espressivo più ampio, che includa gli ambienti tridimensionali. Il rischio di impiegare del tempo per imparare come funziona questa tecnologia per generare spazi virtuali rende scettici quanti si impegnano nell'insegnamento, ma le esperienze di progetti sviluppati, soprattutto all’estero, servono a capire che sono un buon investimento. Il fatto che una software house, che crea un videogame di grande successo di pubblico, includa nel suo prodotto, una serie di strumenti che consentano all'utente la creazione di mondi propri in cui giocare, è sintomatico che l'alfabetizzazione informatica degli utenti medi sta crescendo sempre più rapidamente e che l'utilizzo di un editor come Unreal Engine sarà in futuro una attività alla portata di un pubblico sempre più vasto. Questo ci mette nelle condizioni di progettare moduli di insegnamento più immersivi, in cui l'esperienza della ricerca e della ricostruzione del passato si intreccino con lo studio più tradizionale degli avvenimenti di una certa epoca. I mondi virtuali interattivi vengono spesso definiti come la forma culturale chiave del XXI secolo, come il cinema lo è stato per il XX. Lo scopo di questo lavoro è stato quello di suggerire che vi sono grosse opportunità per gli storici impiegando gli oggetti e le ambientazioni in 3D, e che essi devono coglierle. Si consideri il fatto che l’estetica abbia un effetto sull’epistemologia. O almeno sulla forma che i risultati delle ricerche storiche assumono nel momento in cui devono essere diffuse. Un’analisi storica fatta in maniera superficiale o con presupposti errati può comunque essere diffusa e avere credito in numerosi ambienti se diffusa con mezzi accattivanti e moderni. Ecco perchè non conviene seppellire un buon lavoro in qualche biblioteca, in attesa che qualcuno lo scopra. Ecco perchè gli storici non devono ignorare il 3D. La nostra capacità, come studiosi e studenti, di percepire idee ed orientamenti importanti dipende spesso dai metodi che impieghiamo per rappresentare i dati e l’evidenza. Perché gli storici possano ottenere il beneficio che il 3D porta con sè, tuttavia, devono sviluppare un’agenda di ricerca volta ad accertarsi che il 3D sostenga i loro obiettivi di ricercatori e insegnanti. Una ricostruzione storica può essere molto utile dal punto di vista educativo non sono da chi la visita ma, anche da chi la realizza. La fase di ricerca necessaria per la ricostruzione non può fare altro che aumentare il background culturale dello sviluppatore. Conclusioni La cosa più importante è stata la possibilità di fare esperienze nell’uso di mezzi di comunicazione di questo genere per raccontare e far conoscere il passato. Rovesciando il paradigma conoscitivo che avevo appreso negli studi umanistici, ho cercato di desumere quelle che potremo chiamare “leggi universali” dai dati oggettivi emersi da questi esperimenti. Da punto di vista epistemologico l’informatica, con la sua capacità di gestire masse impressionanti di dati, dà agli studiosi la possibilità di formulare delle ipotesi e poi accertarle o smentirle tramite ricostruzioni e simulazioni. Il mio lavoro è andato in questa direzione, cercando conoscere e usare strumenti attuali che nel futuro avranno sempre maggiore presenza nella comunicazione (anche scientifica) e che sono i mezzi di comunicazione d’eccellenza per determinate fasce d’età (adolescenti). Volendo spingere all’estremo i termini possiamo dire che la sfida che oggi la cultura visuale pone ai metodi tradizionali del fare storia è la stessa che Erodoto e Tucidide contrapposero ai narratori di miti e leggende. Prima di Erodoto esisteva il mito, che era un mezzo perfettamente adeguato per raccontare e dare significato al passato di una tribù o di una città. In un mondo post letterario la nostra conoscenza del passato sta sottilmente mutando nel momento in cui lo vediamo rappresentato da pixel o quando le informazioni scaturiscono non da sole, ma grazie all’interattività con il mezzo. La nostra capacità come studiosi e studenti di percepire idee ed orientamenti importanti dipende spesso dai metodi che impieghiamo per rappresentare i dati e l’evidenza. Perché gli storici possano ottenere il beneficio sottinteso al 3D, tuttavia, devono sviluppare un’agenda di ricerca volta ad accertarsi che il 3D sostenga i loro obiettivi di ricercatori e insegnanti. Le esperienze raccolte nelle pagine precedenti ci portano a pensare che in un futuro non troppo lontano uno strumento come il computer sarà l’unico mezzo attraverso cui trasmettere conoscenze, e dal punto di vista didattico la sua interattività consente coinvolgimento negli studenti come nessun altro mezzo di comunicazione moderno.

Applications of High Speed Configurable Logic Devices in Modern Particle Physics Experiments

Several activities were conducted during my PhD activity. For the NEMO experiment a collaboration between the INFN/University groups of Catania and Bologna led to the development and production of a mixed signal acquisition board for the Nemo Km3 telescope. The research concerned the feasibility study for a different acquisition technique quite far from that adopted in the NEMO Phase 1 telescope. The DAQ board that we realized exploits the LIRA06 front-end chip for the analog acquisition of anodic an dynodic sources of a PMT (Photo-Multiplier Tube). The low-power analog acquisition allows to sample contemporaneously multiple channels of the PMT at different gain factors in order to increase the signal response linearity over a wider dynamic range. Also the auto triggering and self-event-classification features help to improve the acquisition performance and the knowledge on the neutrino event. A fully functional interface towards the first level data concentrator, the Floor Control Module, has been integrated as well on the board, and a specific firmware has been realized to comply with the present communication protocols. This stage of the project foresees the use of an FPGA, a high speed configurable device, to provide the board with a flexible digital logic control core. After the validation of the whole front-end architecture this feature would be probably integrated in a common mixed-signal ASIC (Application Specific Integrated Circuit). The volatile nature of the configuration memory of the FPGA implied the integration of a flash ISP (In System Programming) memory and a smart architecture for a safe remote reconfiguration of it. All the integrated features of the board have been tested. At the Catania laboratory the behavior of the LIRA chip has been investigated in the digital environment of the DAQ board and we succeeded in driving the acquisition with the FPGA. The PMT pulses generated with an arbitrary waveform generator were correctly triggered and acquired by the analog chip, and successively they were digitized by the on board ADC under the supervision of the FPGA. For the communication towards the data concentrator a test bench has been realized in Bologna where, thanks to a lending of the Roma University and INFN, a full readout chain equivalent to that present in the NEMO phase-1 was installed. These tests showed a good behavior of the digital electronic that was able to receive and to execute command imparted by the PC console and to answer back with a reply. The remotely configurable logic behaved well too and demonstrated, at least in principle, the validity of this technique. A new prototype board is now under development at the Catania laboratory as an evolution of the one described above. This board is going to be deployed within the NEMO Phase-2 tower in one of its floors dedicated to new front-end proposals. This board will integrate a new analog acquisition chip called SAS (Smart Auto-triggering Sampler) introducing thus a new analog front-end but inheriting most of the digital logic present in the current DAQ board discussed in this thesis. For what concern the activity on high-resolution vertex detectors, I worked within the SLIM5 collaboration for the characterization of a MAPS (Monolithic Active Pixel Sensor) device called APSEL-4D. The mentioned chip is a matrix of 4096 active pixel sensors with deep N-well implantations meant for charge collection and to shield the analog electronics from digital noise. The chip integrates the full-custom sensors matrix and the sparsifification/readout logic realized with standard-cells in STM CMOS technology 130 nm. For the chip characterization a test-beam has been set up on the 12 GeV PS (Proton Synchrotron) line facility at CERN of Geneva (CH). The collaboration prepared a silicon strip telescope and a DAQ system (hardware and software) for data acquisition and control of the telescope that allowed to store about 90 million events in 7 equivalent days of live-time of the beam. My activities concerned basically the realization of a firmware interface towards and from the MAPS chip in order to integrate it on the general DAQ system. Thereafter I worked on the DAQ software to implement on it a proper Slow Control interface of the APSEL4D. Several APSEL4D chips with different thinning have been tested during the test beam. Those with 100 and 300 um presented an overall efficiency of about 90% imparting a threshold of 450 electrons. The test-beam allowed to estimate also the resolution of the pixel sensor providing good results consistent with the pitch/sqrt(12) formula. The MAPS intrinsic resolution has been extracted from the width of the residual plot taking into account the multiple scattering effect.

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.

Studies of the atmospheric muon flux with the ANTARES detector

The thesis main topic is the determination of the vertical component of the atmospheric muon flux as a function of the sea depth at the ANTARES site. ANTARES is a Cherenkov neutrino telescope placed at 2500m depth in the Mediterranean Sea at 40 km from the southern cost of France. In order to retrieve back the physical flux from the experimental data a deconvolution algorithm has been perform which takes into consideration the trigger inefficiensies and the reconstruction errors on the zenith angle. The obtained results are in good agreement with other ANTARES indipendent analysis.