A comparative analysis of the relative efficacy of vector-control strategies against dengue fever

Dengue is considered one of the most important vector-borne infection, affecting almost half of the world population with 50 to 100 million cases every year. In this paper, we present one of the simplest models that can encapsulate all the important variables related to vector control of dengue fever. The model considers the human population, the adult mosquito population and the population of immature stages, which includes eggs, larvae and pupae. The model also considers the vertical transmission of dengue in the mosquitoes and the seasonal variation in the mosquito population. From this basic model describing the dynamics of dengue infection, we deduce thresholds for avoiding the introduction of the disease and for the elimination of the disease. In particular, we deduce a Basic Reproduction Number for dengue that includes parameters related to the immature stages of the mosquito. By neglecting seasonal variation, we calculate the equilibrium values of the model’s variables. We also present a sensitivity analysis of the impact of four vector-control strategies on the Basic Reproduction Number, on the Force of Infection and on the human prevalence of dengue. Each of the strategies was studied separately from the others. The analysis presented allows us to conclude that of the available vector control strategies, adulticide application is the most effective, followed by the reduction of the exposure to mosquito bites, locating and destroying breeding places and, finally, larvicides. Current vector-control methods are concentrated on mechanical destruction of mosquitoes’ breeding places. Our results suggest that reducing the contact between vector and hosts (biting rates) is as efficient as the logistically difficult but very efficient adult mosquito’s control.

Referencing geostrophic velocities using ADCP data at 24.5 ºN

Diploma de Estudios Avanzados

Referencing geostrophic velocities using ADCP data at 24.5°N (North Atlantic)

[EN] Acoustic Doppler Current Profilers (ADCPs) have proven to be a useful oceanographic tool in the study of ocean dynamics. Data from D279, a transatlantic hydrographic cruise carried out in spring 2004 along 24.5°N, were processed, and lowered ADCP (LADCP) bottom track data were used to assess the choice of reference velocity for geostrophic calculations. The reference velocities from different combinations of ADCP data were compared to one another and a reference velocity was chosen based on the LADCP data. The barotropic tidal component was subtracted to provide a final reference velocity estimated by LADCP data. The results of the velocity fields are also shown. Further studies involving inverse solutions will include the reference velocity calculated here.

The relative influence of local to regional drivers of variation in reef fishes

La versión definitiva del documento en www3.interscience.wiley.com

Analisi della domanda di sosta veicolare e delle relative ripercussioni sulla mobilità urbana

Questa si ripropone in prima istanza di analizzare le origini e l’evoluzione del concetto di sostenibilità e successivamente di prendere in considerazione uno dei tanti mezzi che consentono di perseguirla: la gestione della sosta. Per molti anni infatti, a partire dal momento in cui sono iniziate ad emergere le esternalità negative legate al traffico, si è pensato che quello dei parcheggi fosse solo un ulteriore problema. Solo di recente, dalla fine degli anni ’90, fatta eccezione per il caso della Gran Bretagna che ha fatto da capofila già a partire dagli anni ’80, si è iniziato a considerare la sosta come parte della soluzione dei problemi di congestione, inquinamento e di vivibilità delle città. Verrà analizzata perciò nel secondo capitolo l’evoluzione delle politiche della sosta a livello europeo, con particolare attenzione all’operato svolto dall’EPA (European Parking Association) associazione leader nel settore riconosciuta dall’Unione Europea e sostenuta da 18 Paesi membri tra cui anche l’Italia. Il lavoro svolto da quest’associazione, nata nei primi anni ’80, è quello di decidere insieme agli associati delle linee comuni da seguire per migliorare le politiche a livello europeo riguardo la gestione della sosta. Si tratta nella pratica di studi, convegni e analisi degli effetti prodotti da provvedimenti intrapresi nelle varie città che hanno iniziato ad introdurre la regolamentazione della sosta. Sempre nel secondo capitolo saranno quindi presentate le linee guida europee nell’ambito dei parcheggi e si analizzeranno casi di “Best Practices” di alcuni Paesi che hanno introdotto provvedimenti per la gestione della sosta. Nel terzo capitolo invece viene considerata la situazione in Italia parlando in principio di Aipark, l’associazione italiana operatori nel settore dei parcheggi che partecipa alle attività dell’Epa e prendendo in esame in seguito le politiche adottate a livello nazionale e nello specifico in alcune tra le più importanti città italiane. Si vedrà come sia ancora troppo marcata la distanza del nostro Paese dai progressi registrati in altri Paesi dell’UE, con le dovute eccezioni. Per quel che riguarda l’aspetto normativo è significativo il fatto che, nonostante il riconoscimento della forte influenza che le politiche della sosta hanno sulla regolazione del traffico, ci siano ancora molte lacune legislative e che spesso la sosta non compaia tra i soggetti delle leggi in tale settore. La legislazione italiana nell’ambito dei parcheggi verrà analizzata nel quarto capitolo. Successivamente, nei capitoli 5 e 6 si parlerà delle fasi preliminari della redazione del Piano della Sosta di Casalecchio di Reno. Il Piano della Sosta è uno dei Piani Particolareggiati che costituiscono il 2° livello di progettazione del PUT (Piano Urbano del Traffico) e rappresenta uno strumento di pianificazione utile ad analizzare lo stato di fatto del sistema dei parcheggi di una città in modo da coglierne le criticità e fornire eventualmente le soluzioni per ovviare ad esse. Nel quinto capitolo viene effettuato un inquadramento territoriale di Casalecchio e si parlerà delle problematiche della sosta emerse nel PGTU (Piano Generale del Traffico Urbano) che costituisce il progetto preliminare o Piano Quadro del PUT. Le fasi attraverso le quali viene elaborato un Piano della sosta si possono sintetizzare nei seguenti punti: - Studio della normativa nazionale e locale e di esempi significativi di altre realtà nell’ambito della sosta. - Analisi dello stato di fatto in termini di domanda e offerta. - Indagini mediante incontri pubblici, distribuzione di questionari o interviste dirette, per cogliere le esigenze degli utenti che usufruiscono del servizio. - Analisi delle eventuali criticità emerse. - Progettazione del nuovo assetto della sosta. - Campagna di sensibilizzazione per fare “accettare” con più facilità i cambiamenti agli utenti. Nel sesto capitolo di questa tesi, e negli allegati si possono consultare i risultati delle indagini su domanda e offerta condotte da TPS (Transport Planning Service), azienda che svolge attività di pianificazione e progettazione, di fornitura software, oltre che indagini e rilievi nell’ambito dei trasporti. Verranno descritte le modalità di rilievo e verranno presentati i risultati ottenuti dall’elaborazione dei dati raccolti, con qualche accenno alle possibili soluzioni per risolvere le problematiche emerse. La fase di progettazione vera e propria degli interventi non verrà invece trattata in questa sede.

X-Ray studies of the physics of matter around super-massive black-holes in nearby Seyfert galaxies

Seyfert galaxies are the closest active galactic nuclei. As such, we can use them to test the physical properties of the entire class of objects. To investigate their general properties, I took advantage of different methods of data analysis. In particular I used three different samples of objects, that, despite frequent overlaps, have been chosen to best tackle different topics: the heterogeneous BeppoS AX sample was thought to be optimized to test the average hard X-ray (E above 10 keV) properties of nearby Seyfert galaxies; the X-CfA was thought the be optimized to compare the properties of low-luminosity sources to the ones of higher luminosity and, thus, it was also used to test the emission mechanism models; finally, the XMM–Newton sample was extracted from the X-CfA sample so as to ensure a truly unbiased and well defined sample of objects to define the average properties of Seyfert galaxies. Taking advantage of the broad-band coverage of the BeppoS AX MECS and PDS instruments (between ~2-100 keV), I infer the average X-ray spectral propertiesof nearby Seyfert galaxies and in particular the photon index (~1.8), the high-energy cut-off (~290 keV), and the relative amount of cold reflection (~1.0). Moreover the unified scheme for active galactic nuclei was positively tested. The distribution of isotropic indicators used here (photon index, relative amount of reflection, high-energy cut-off and narrow FeK energy centroid) are similar in type I and type II objects while the absorbing column and the iron line equivalent width significantly differ between the two classes of sources with type II objects displaying larger absorbing columns. Taking advantage of the XMM–Newton and X–CfA samples I also deduced from measurements that 30 to 50% of type II Seyfert galaxies are Compton thick. Confirming previous results, the narrow FeK line is consistent, in Seyfert 2 galaxies, with being produced in the same matter responsible for the observed obscuration. These results support the basic picture of the unified model. Moreover, the presence of a X-ray Baldwin effect in type I sources has been measured using for the first time the 20-100 keV luminosity (EW proportional to L(20-100)^(−0.22±0.05)). This finding suggests that the torus covering factor may be a function of source luminosity, thereby suggesting a refinement of the baseline version of the unifed model itself. Using the BeppoSAX sample, it has been also recorded a possible correlation between the photon index and the amount of cold reflection in both type I and II sources. At a first glance this confirms the thermal Comptonization as the most likely origin of the high energy emission for the active galactic nuclei. This relation, in fact, naturally emerges supposing that the accretion disk penetrates, depending to the accretion rate, the central corona at different depths (Merloni et al. 2006): the higher accreting systems hosting disks down to the last stable orbit while the lower accreting systems hosting truncated disks. On the contrary, the study of the well defined X–C f A sample of Seyfert galaxies has proved that the intrinsic X-ray luminosity of nearby Seyfert galaxies can span values between 10^(38−43) erg s^−1, i.e. covering a huge range of accretion rates. The less efficient systems have been supposed to host ADAF systems without accretion disk. However, the study of the X–CfA sample has also proved the existence of correlations between optical emission lines and X-ray luminosity in the entire range of L_(X) covered by the sample. These relations are similar to the ones obtained if high-L objects are considered. Thus the emission mechanism must be similar in luminous and weak systems. A possible scenario to reconcile these somehow opposite indications is assuming that the ADAF and the two phase mechanism co-exist with different relative importance moving from low-to-high accretion systems (as suggested by the Gamma vs. R relation). The present data require that no abrupt transition between the two regimes is present. As mentioned above, the possible presence of an accretion disk has been tested using samples of nearby Seyfert galaxies. Here, to deeply investigate the flow patterns close to super-massive black-holes, three case study objects for which enough counts statistics is available have been analysed using deep X-ray observations taken with XMM–Newton. The obtained results have shown that the accretion flow can significantly differ between the objects when it is analyzed with the appropriate detail. For instance the accretion disk is well established down to the last stable orbit in a Kerr system for IRAS 13197-1627 where strong light bending effect have been measured. The accretion disk seems to be formed spiraling in the inner ~10-30 gravitational radii in NGC 3783 where time dependent and recursive modulation have been measured both in the continuum emission and in the broad emission line component. Finally, the accretion disk seems to be only weakly detectable in rk 509, with its weak broad emission line component. Finally, blueshifted resonant absorption lines have been detected in all three objects. This seems to demonstrate that, around super-massive black-holes, there is matter which is not confined in the accretion disk and moves along the line of sight with velocities as large as v~0.01-0.4c (whre c is the speed of light). Wether this matter forms winds or blobs is still matter of debate together with the assessment of the real statistical significance of the measured absorption lines. Nonetheless, if confirmed, these phenomena are of outstanding interest because they offer new potential probes for the dynamics of the innermost regions of accretion flows, to tackle the formation of ejecta/jets and to place constraints on the rate of kinetic energy injected by AGNs into the ISM and IGM. Future high energy missions (such as the planned Simbol-X and IXO) will likely allow an exciting step forward in our understanding of the flow dynamics around black holes and the formation of the highest velocity outflows.