Space-temporal dynamics of limnological variables in a floodplain wetland located at Ribeira do Iguape Valley (São Paulo, Brazil) at different hydrological periods

AIM: The main goal of this research was to investigate the influence of the hydrological pulses on the space-temporal dynamics of physical and chemical variables in a wetland adjacent to Jacupiranguinha River (São Paulo, Brazil); METHODS: Eleven sampling points were distributed among the wetland, a tributary by its left side and the adjacent river. Four samplings were carried out, covering the rainy and the dry periods. Measures of pH, dissolved oxygen, electrical conductivity and redox potential were taken in regular intervals of the water column using a multiparametric probe. Water samples were collected for the nitrogen and total phosphorus analysis, as well as their dissolved fractions (dissolved inorganic phosphorus, total dissolved phosphorus, ammoniacal nitrogen and nitrate). Total alkalinity and suspended solids were also quantified; RESULTS: The Multivariate Analysis of Variance showed the influence of the seasonality on the variability of the investigated variables, while the Principal Component Analysis gave rise in two statistical significant axes, which delimited two groups representative of the rainy and dry periods. Hydrological pulses from Jacupiranguinha River, besides contributing to the inputs of nutrients and sediments during the period of connectivity, accounted for the decrease in spatial gradients in the wetland. This "homogenization effect" was evidenced by the Cluster Analysis. The research also showed an industrial raw effluent as the main point source of phosphorus to the Jacupiranguinha River and, indirectly, to the wetland; CONCLUSIONS: Therefore, considering the scarcity of information about the wetlands in the study area, this research, besides contributing to the understanding of the influence of hydrological pulses on the investigated environmental variables, showed the need for adoption of conservation policies of these ecosystems face the increase anthropic pressures that they have been submitted, which may result in lack of their ecological, social and economic functions.

Minka - The houses of Japanese imigrants in Ribeira valley, São Paulo,Brazil

O artigo analisa o processo de produção de moradia do imigrante japonês no Vale do Ribeira, na região sul do estado de São Paulo, ocorrido no início do século XX. Partindo do contexto histórico do início da colonização da região e as condicionantes que possibilitaram a criação da colônia, o trabalho busca verificar como foram construídas as casas que, baseados na autoconstrução e tendo a terra e madeira formaram o repertório de quase 500 casas. Põe foco em dois exemplares onde são analisadas a técnica do tsuchikabe e as sambladuras; verificando que mesmo diante das adversidades encontradas na natureza distinta de sua origem construíram casas de elevada qualidade. Os saberes trazidos do extremo oriente foram aplicados e se mesclaram às influências, cabocla, quilombola e europeia que hoje, após um século, representam uma categoria expressiva e variada sob os aspectos construtivo, tipológico e programático.

The Gemini planet-finding campaign: the frequency of giant planets aroud debris disk stars

We have completed a high-contrast direct imaging survey for giant planets around 57 debris disk stars as part of the Gemini NICI Planet-Finding Campaign. We achieved median H-band contrasts of 12.4 mag at 0.''5 and 14.1 mag at 1'' separation. Follow-up observations of the 66 candidates with projected separation <500 AU show that all of them are background objects. To establish statistical constraints on the underlying giant planet population based on our imaging data, we have developed a new Bayesian formalism that incorporates (1) non-detections, (2) single-epoch candidates, (3) astrometric and (4) photometric information, and (5) the possibility of multiple planets per star to constrain the planet population. Our formalism allows us to include in our analysis the previously known β Pictoris and the HR 8799 planets. Our results show at 95% confidence that <13% of debris disk stars have a ≥5 M Jup planet beyond 80 AU, and <21% of debris disk stars have a ≥3 M Jup planet outside of 40 AU, based on hot-start evolutionary models. We model the population of directly imaged planets as d 2 N/dMdavpropm α a β, where m is planet mass and a is orbital semi-major axis (with a maximum value of a max). We find that β < –0.8 and/or α > 1.7. Likewise, we find that β < –0.8 and/or a max < 200 AU. For the case where the planet frequency rises sharply with mass (α > 1.7), this occurs because all the planets detected to date have masses above 5 M Jup, but planets of lower mass could easily have been detected by our search. If we ignore the β Pic and HR 8799 planets (should they belong to a rare and distinct group), we find that <20% of debris disk stars have a ≥3 M Jup planet beyond 10 AU, and β < –0.8 and/or α < –1.5. Likewise, β < –0.8 and/or a max < 125 AU. Our Bayesian constraints are not strong enough to reveal any dependence of the planet frequency on stellar host mass. Studies of transition disks have suggested that about 20% of stars are undergoing planet formation; our non-detections at large separations show that planets with orbital separation >40 AU and planet masses >3 M Jup do not carve the central holes in these disks.

The Gemini NICI planet-finding campaign: the frequency of giant planets around young B and A stars

We have carried out high contrast imaging of 70 young, nearby B and A stars to search for brown dwarf and planetary companions as part of the Gemini NICI Planet-Finding Campaign. Our survey represents the largest, deepest survey for planets around high-mass stars (≈1.5-2.5 M ☉) conducted to date and includes the planet hosts β Pic and Fomalhaut. We obtained follow-up astrometry of all candidate companions within 400 AU projected separation for stars in uncrowded fields and identified new low-mass companions to HD 1160 and HIP 79797. We have found that the previously known young brown dwarf companion to HIP 79797 is itself a tight (3 AU) binary, composed of brown dwarfs with masses 58$^{+21}_{-20}$ M Jup and 55$^{+20}_{-19}$ M Jup, making this system one of the rare substellar binaries in orbit around a star. Considering the contrast limits of our NICI data and the fact that we did not detect any planets, we use high-fidelity Monte Carlo simulations to show that fewer than 20% of 2 M ☉ stars can have giant planets greater than 4 M Jup between 59 and 460 AU at 95% confidence, and fewer than 10% of these stars can have a planet more massive than 10 M Jup between 38 and 650 AU. Overall, we find that large-separation giant planets are not common around B and A stars: fewer than 10% of B and A stars can have an analog to the HR 8799 b (7 M Jup, 68 AU) planet at 95% confidence. We also describe a new Bayesian technique for determining the ages of field B and A stars from photometry and theoretical isochrones. Our method produces more plausible ages for high-mass stars than previous age-dating techniques, which tend to underestimate stellar ages and their uncertainties.

Zooplankton metabolic activity (respiration and ETS) from three stages of the Malaspina 2010 campaign

Máster Oceanografía Biológica. Primera Tesis de Máster con resultados de la Campaña de Circunnavegación Malaspina 2010

Ecological tools for assessing rock-art conservation in the Côa Valley Archaeological Park (V.N. Foz Côa, Northeast Portugal)

Centro de Investigação em Biodiversidade e Recursos Genéticos da Universidade do Porto. Departamento de Biologia, Faculdade de Ciências da Universidade do Porto. EscolaUniversitaria de Enxeñeria Forestal, Universidade de Vigo

Web Marketing e promozione del territorio - Il caso Motor Valley

L’oggetto della presente tesi progettuale riguarda l’analisi di funzionalità e usabilità per il sito www.motorvalley.it e il conseguente supporto dello sviluppo di una nuova release. Si tratta di un lavoro atto sia ad aumentare i visitatori e il volume di traffico verso il sito, sia a vendere più pacchetti turistici e promuovere eventi legati al circuito Motor Valley.

Struttura e dinamica di popolazione di Axinella polypoides (Schmidt, 1862) (Porifera, Demospongiae) presso l’Isola Gallinara (SV)

I poriferi rappresentano un importante campo di ricerca anche in ambito applicativo in quanto potenzialmente utili come fonte di metaboliti secondari da impiegarsi in ambito clinico (antitumorali, antibiotici, antivirali, ecc.) e industriale (antifouling). I processi di biosilicificazione interessano invece per aspetti legati alle biotecnologie marine. Questo Phylum ha un importante ruolo strutturale e funzionale nell’ecologia dei popolamenti bentonici, in quanto può essere dominante in numerosi habitat e svolgere un ruolo ecologico fondamentale nelle dinamiche degli ecosistemi marini. Per questo, la variazione spaziale e temporale della loro abbondanza può avere effetti considerevoli su altri membri della comunità. Lo studio delle dinamiche di popolazione e del ciclo riproduttivo dei poriferi potrebbe permettere di valutare come i cambiamenti climatici ne influenzino la crescita e la riproduzione e potrebbe quindi fornire una base per lo sviluppo di corrette tecniche di gestione ambientale. La spugna Axinella polypoides è inserita all’interno delle liste di protezione della Convenzione di Berna e di Barcellona, dove sono elencate le specie da proteggere perché minacciate o in pericolo di estinzione. Questa specie, avendo una morfologia eretta, è fortemente minacciata soprattutto da attività antropiche quali pesca e ancoraggi, ma nonostante questo la letteratura relativa ad essa è scarsa, La sua importanza è legata soprattutto al recente utilizzo come modello per numerosi esperimenti. A. polypoides rappresenta, infatti, il più basso livello nella scala evolutiva in cui sono stati rinvenuti meccanismi biochimici cellulari di reazione all’aumento di temperatura (incremento dell’attività ADP-ribosil ciclasica, sintesi di ossido nitrico) tipici degli organismi superiori. Lo scopo di questa tesi è di aumentare le conoscenze sull’ecologia e sulla biologia di questo porifero, al fine di consentire una migliore predisposizione di eventuali piani di tutela. Dallo studio delle colonie effettuato presso l’Isola Gallinara (SV), emerge una dinamica di crescita lenta ed un ciclo riproduttivo estivo, coerentemente con quanto osservato per altre specie mediterranee del genere Axinella. Le analisi istologiche effettuate hanno mostrato variabilità temporale nella densità e nella dimensione di particolari cellule sferulose, che si ipotizza siano collegate a fenomeni di proliferazione cellulare e rigenerazione in seguito a danni. È stata individuata inoltre la presenza di una particolare tipologia cellulare dendritica la cui funzione si ritiene abbia affinità con le funzioni sensoriali di Phyla superiori. Queste osservazioni, e l’evidente vulnerabilità della specie agli impatti antropici, hanno evidenziato la necessità di sviluppare adeguati piani di monitoraggio e di conservazione.

Eduard Study (1862-1930) - ein mathematischer Mephistopheles im geometrischen Gärtchen

Diese Arbeit befasst sich mit Eduard Study (1862-1930), einem der deutschen Geometer um die Jahrhundertwende, der seine Zeit zum Einen durch seine Kontakte zu Klein, Hilbert, Engel, Lie, Gordan, Halphen, Zeuthen, Einstein, Hausdorff und Weyl geprägt hat, zum Anderen in ihr aber auch für seine beißenden und stilistisch ausgefeilten Kritiken ebenso berühmt wie berüchtigt war. Da sich Study mit einer Vielzahl mathematischer Themen beschäftigt hat, führen wir zunächst in die von ihm bearbeiteten Gebiete der Geometrie des 19. Jahrhunderts ein (analytische und synthetische Geometrie im Sinne von Monge, Poncelet, Plücker und Reye, Invariantentheorie Clebsch-Gordan'scher Prägung, abzählende Geometrie von Chasles und Halphen, die Werke Lie's und Grassmann’s, Liniengeometrie sowie Axiomatik und Grundlagenkrise). In seiner darauf folgenden Biographie finden sich als zentrale Stellen seine Habilitation bei Klein über die Chasles’sche Vermutung, sein Streit mit Zeuthen darüber als eine der Debatten der Mathematischen Annalen (aus der er historisch zwar nicht, mathematisch aber tatsächlich als Gewinner hätte herausgehen müssen, wie wir an der Lösung des Problems durch van der Waerden sehen werden) und seine Auseinandersetzungen als etablierter Bonner Professor mit Engel über Lie, Weyl über Invariantentheorie, zahlreichen philosophischen Richtungen über das Raumproblem, Pasch’s Axiomatik, Hilbert’s Formalismus sowie Brouwer’s und Weyl’s Intuitionismus.

Tracking, photometry and spectroscopy of space debris: the Malindi, Loiano, Las Campanas and Cerro Tololo observation campaign results

The main purpose of my thesis has been the analysis of the space debris environment and their characterization through optical measurements. In particular I had the opportunity to contribute to the Italian Space Agency activities in space debris optical observation campaign and I cooperated directly with NASA Orbital Debris Program Office by working at the Astronomy Department of the University of Michigan for six months.

Land use management in mountainous areas: combining ground-based and EO (Earth Observation) data to investigate the shallow landsliding susceptibility in the Duron valley (Trento, Italy).

Throughout the alpine domain, shallow landslides represent a serious geologic hazard, often causing severe damages to infrastructures, private properties, natural resources and in the most catastrophic events, threatening human lives. Landslides are a major factor of landscape evolution in mountainous and hilly regions and represent a critical issue for mountainous land management, since they cause loss of pastoral lands. In several alpine contexts, shallow landsliding distribution is strictly connected to the presence and condition of vegetation on the slopes. With the aid of high-resolution satellite images, it's possible to divide automatically the mountainous territory in land cover classes, which contribute with different magnitude to the stability of the slopes. The aim of this research is to combine EO (Earth Observation) land cover maps with ground-based measurements of the land cover properties. In order to achieve this goal, a new procedure has been developed to automatically detect grass mantle degradation patterns from satellite images. Moreover, innovative surveying techniques and instruments are tested to measure in situ the shear strength of grass mantle and the geomechanical and geotechnical properties of these alpine soils. Shallow landsliding distribution is assessed with the aid of physically based models, which use the EO-based map to distribute the resistance parameters across the landscape.