939 resultados para Richter, Dave
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A comunidade de tubarões (Selachii:Galea) proveniente da Formação Pirabas pode ser considerada como uma das mais representativas e de maior diversidade entre as unidades do Neógeno da América do Sul. A presença de 8 gêneros permitiu elaborar hipóteses sobre a reconstrução da cadeia trófica envolvendo outros elementos da paleofauna de vertebrados, assim como também serviu como um indicador paleoecológico adicional que corrobora dados anteriores sobre a reconstituição dos parâmetros paleoambientais da unidade geológica. Foi realizado uma revisão taxonômica das espécies previamente conhecidos para a Formação Pirabas, cuja composição da paleocomun idade de tubarões foi a seguinte: Carcharhinus spl Carcharhinus sp2, Carcharhinus sp3, Carcharhinus priscus, Sphyma magna, Hemipristis serra, Carcharodon megalodon, Isurus sp, Ginglyrnostoma serra, Ginglymostoma obliquum. Novas coletas possibilitaram a expansão de 31 exemplares depositados em museus brasileiros para 231 novos indivíduos, incluindo material microscópico. Esta coleta serviu para aumentar o conhecimento sobre a diversidade e aspectos paleoecológicos dos grupos representados.
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Pós-graduação em Geografia - FCT
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O intervalo que compreende o final do Paleozóico e início do Mesozóico foi marcado por mudanças globais paleogeográficas e paleoclimáticas, em parte atribuídas a eventos catastróficos. A intensa continentalização do supercontinente Pangéia, com a implantação de extensos desertos, sucedeu os ambientes costeiros-plataformais do início do Permiano. Os registros desses eventos no norte do Brasil são encontrados nas bacias intracratônicas, particularmente na Bacia do Parnaíba, representados pela zona de contato entre as formações Motuca e Sambaíba. A Formação Motuca é constituída predominantemente por pelitos vermelhos laminados com lentes de gipsita, calcita e marga. Na porção leste da Bacia do Parnaíba, as fácies da Formação Motuca tornam-se mais arenosas com a ocorrência expressiva de arenitos com estratificação cruzada sigmoidal. A Formação Sambaíba consiste em arenitos de coloração creme alaranjada com estratificação plano-paralela e estratificação cruzada de médio a grande porte. Em geral, o contato entre as unidades é brusco, representado pela passagem de arenitos finos com laminação cruzada cavalgante e acamamento flaser/wavy da Formação Motuca para arenitos médios com falhas/microfalhas sinsedimentares e laminações convolutas da Formação Sambaíba. Foram individualizadas 14 fácies sedimentares, agrupadas em quatro associações: AF1 – Lacustre raso / Planície de lama (mudflat), AF2 – “Panela” salina (saline pan), AF3 – Lençol de areia e AF4 – Campo de dunas. A AF1 foi depositada dominantemente por processos de decantação em um extenso ambiente lacustre raso de baixa energia, influenciado por influxos esporádicos de areias oriundos de rios efêmeros. Este sistema lacustre foi, provavelmente, influenciado por períodos de contração e expansão, devido às variações das condições climáticas predominantemente áridas. Os mais expressivos períodos de contração ocorreram na porção oeste da Bacia do Parnaíba, representados pelo desenvolvimento de planícies de lama (mudflats) associadas a lagoas efêmeras saturadas em carbonatos e a “panelas” salinas (saline pans- AF2). Os lençóis de areia (AF3) são planícies arenosas extensas, localmente com área úmidas, intensamente retrabalhadas por processos eólicos. A AF4 é interpretada como parte de um erg composto por dunas/draas em zona saturada em areia, com interdunas secas subordinadas. Intervalos deformados lateralmente contínuos por centenas de quilômetros ocorrem na zona de contato entre as formações Motuca e Sambaíba. Pelitos com camadas contorcidas e brechadas (Formação Motuca) e arenitos com falhas/microfalhas sinsedimentares, laminação convoluta e diques de injeção preenchidos por argilitos (Formação Sambaíba) são interpretados como sismitos induzidos por terremotos de alta magnitude (>8 na escala Ritcher). Anomalias geoquímicas de elementos traços como Mn, Cr, Co, Cu e Ni na zona de contato entre as formações, juntamente com a presença de micropartículas de composição metálica na matriz argilosa dos sismitos, corroboram com impactos de meteoritos no limite c, possivelmente do astroblema Riachão.
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O intervalo que compreende o final do Paleozoico e início do Mesozoico foi marcado por mudanças globais paleogeográficas e paleoclimáticas, em parte atribuídas a eventos catastróficos. A intensa continentalização do supercontinente Pangeia, com a implantação de extensos desertos, sucedeu os ambientes costeiro-plataformais do início do Permiano. Os registros desses eventos no norte do Brasil são encontrados nas bacias intracratônicas, particularmente na sucessão Permotriássica da Bacia do Parnaíba. A análise de fácies e estratigráfica de afloramentos desta sucessão permitiu a individualização de 14 fácies sedimentares agrupadas em 4 associações de fácies (AF): AF1 e AF2, relacionadas aos depósitos da Formação Motuca, e AF3 e AF4, representativas da base da Formação Sambaíba. A AF1 - Lacustre raso/Mudflat consiste em pelitos vermelhos laminados com lentes de gipsita, calcita e marga, além de lobos de arenitos sigmoidais. A AF2 - Saline pan é constituída por corpos lenticulares de gipso laminado, gipso nodular e gipsarenito, sobrepostos por pelitos esverdeados com nódulos de dolomita e palygorskita. A AF3 - Lençol de areia e AF4 - Campo de dunas são formadas, respectivamente, por arenitos de coloração creme alaranjada com estratificação plano-paralela e estratificação cruzada de médio a grande porte. Destaca-se o registro de intervalos deformados lateralmente contínuos por centenas de quilômetros na zona de contato entre as formações Motuca e Sambaíba. Nestes, ocorrem pelitos com camadas contorcidas e brechadas (Formação Motuca) e arenitos com falhas/microfalhas sinsedimentares, laminação convoluta e diques de injeção preenchidos por argilitos (Formação Sambaíba), interpretados como sismitos induzidos por terremotos de alta magnitude (> 8 na escala Richter).
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Pós-graduação em Ciências Biológicas (Zoologia) - IBRC
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A proposta de Denis Richter neste livro - fruto de pesquisa de campo realizada com alunos da 3.a série do ensino médio de Presidente Prudente (SP) - é investigar o raciocínio geográfico desenvolvido pelos estudantes a partir do ensino da Geografia em unidades de ensino públicas e privadas. Partindo da construção de mapas mentais da cidade, Richter analisou e interpretou o raciocínio geográfico formado ao longo da educação básica, identificou e avaliou os conteúdos que os alunos possuíam de Geografia e levantou como eles utilizavam a linguagem espacial para expressar seus conceitos espontâneos e científicos. A produção desses mapas mentais revelou ainda os conceitos que os alunos desenvolvem sobre a organização e a estrutura da cidade, bem como sobre os processos que, no entender deles, determinam os diferentes contextos do espaço urbano. O objetivo de fundo do livro de Richter é oferecer subsídios para que o ensino da Geografia proporcione um novo olhar sobre seu contexto sócio-cultural. Citando Milton Santos, o autor afirma que esse olhar está relacionado ao estudo do espaço, ou seja, ao estabelecimento de relações com os objetos e arranjos espaciais que compõem a sociedade - a totalidade.
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A Scientific Committee on Problems of the Environment Rapid Assessment (SCOPE-RAP) workshop was held on 18-22 March 2013. This workshop was hosted by the European Commission, JRC Centre at Ispra, Italy, and brought together 40 leading experts from Africa, Asia, Europe and North and South America to create four synthesis chapters aimed at identifying knowledge gaps, research requirements, and policy innovations. Given the forthcoming publication by CABI of a book volume of the outcomes of the SCOPE-RAP in 2014, this workshop report provides an update on the global societal challenge of soil carbon management and some of the main issues and solutions that were identified in the four working sessions.
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In this paper we present the results of a coherent narrow-band search for continuous gravitational-wave signals from the Crab and Vela pulsars conducted on Virgo VSR4 data. In order to take into account a possible small mismatch between the gravitational-wave frequency and two times the star rotation frequency, inferred from measurement of the electromagnetic pulse rate, a range of 0.02 Hz around two times the star rotational frequency has been searched for both the pulsars. No evidence for a signal has been found and 95% confidence level upper limits have been computed assuming both that polarization parameters are completely unknown and that they are known with some uncertainty, as derived from x-ray observations of the pulsar wind torii. For Vela the upper limits are comparable to the spin-down limit, computed assuming that all the observed spin-down is due to the emission of gravitational waves. For Crab the upper limits are about a factor of 2 below the spin-down limit, and represent a significant improvement with respect to past analysis. This is the first time the spin-down limit is significantly overcome in a narrow-band search.
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We present results of a search for continuously emitted gravitational radiation, directed at the brightest low-mass x-ray binary, Scorpius X-1. Our semicoherent analysis covers 10 days of LIGO S5 data ranging from 50-550 Hz, and performs an incoherent sum of coherent F-statistic power distributed amongst frequency-modulated orbital sidebands. All candidates not removed at the veto stage were found to be consistent with noise at a 1% false alarm rate. We present Bayesian 95% confidence upper limits on gravitational-wave strain amplitude using two different prior distributions: a standard one, with no a priori assumptions about the orientation of Scorpius X-1; and an angle-restricted one, using a prior derived from electromagnetic observations. Median strain upper limits of 1.3 x 10(-24) and 8 x 10(-25) are reported at 150 Hz for the standard and angle-restricted searches respectively. This proof-of-principle analysis was limited to a short observation time by unknown effects of accretion on the intrinsic spin frequency of the neutron star, but improves upon previous upper limits by factors of similar to 1.4 for the standard, and 2.3 for the angle-restricted search at the sensitive region of the detector.
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The Advanced LIGO gravitational wave detectors are second-generation instruments designed and built for the two LIGO observatories in Hanford, WA and Livingston, LA, USA. The two instruments are identical in design, and are specialized versions of a Michelson interferometer with 4 km long arms. As in Initial LIGO, Fabry-Perot cavities are used in the arms to increase the interaction time with a gravitational wave, and power recycling is used to increase the effective laser power. Signal recycling has been added in Advanced LIGO to improve the frequency response. In the most sensitive frequency region around 100 Hz, the design strain sensitivity is a factor of 10 better than Initial LIGO. In addition, the low frequency end of the sensitivity band is moved from 40 Hz down to 10 Hz. All interferometer components have been replaced with improved technologies to achieve this sensitivity gain. Much better seismic isolation and test mass suspensions are responsible for the gains at lower frequencies. Higher laser power, larger test masses and improved mirror coatings lead to the improved sensitivity at mid and high frequencies. Data collecting runs with these new instruments are planned to begin in mid-2015.
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A survey to determine population trends and entomopathogenic fungi associated with the red palm mite (RPM), Raoiella indica, was conducted in Trinidad, Antigua, St. Kitts and Nevis and Dominica. RPM population density was evaluated by sampling a total of ten coconut palms per site in Antigua, St. Kitts and Nevis, Dominica, and Trinidad (Manzanilla and Icacos). Mites from the four islands were either surface sterilized or left unsterilized before being cultured on Tap Water Agar (TWA). A total of 318 fungal colonies were retrieved. A further 96 mites from Dominica were kept on sterile moist filter paper in a humidity chamber and a further 85 colonies were isolated. Based on morphological observations of all 403 isolates, a sample consisting of 32 colonies (8 %) was sent for identification at CABI-UK. Of the 27 fungi positively identified, 15 isolates belonged to the genera Cladosporium, three to Simplicillium spp., and one to Penicillium. Other fungi genera with limited or no entomopathogenic potential included: Aspergillus, Cochliobolus, Fusarium, Pestalotiopsis and Pithomyces. The results show a potential use of entomopathogenic fungi for population management of the red palm mite in the Caribbean region.
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The development of a new methodology for the construction of very efficient flow cells for mercury detection by potentiometric stripping analysis, employing the thin gold layer of recordable CDs as working electrode is reported. This new source of electrodes (CDtrodes) show very attractive performance, similar to that obtained with commercial gold electrodes, with superior versatility. The low cost of this new source of gold electrodes allows a frequent replacement of the electrode, avoiding cumbersome clean-up treatments. Various experimental parameters have been optimized to yield low detection limits (0.25 ng/mL of mercury for 5 min deposition at 0.3 V) and good precision (standard deviation of 1.9% was obtained for 15 repetitive measurements using 10 ng/mL of mercury). Standard curves were found to be linear over the range of 0.5-100 μg L-1 of mercury. The flow cells developed were used for the quantification of mercury in oceanic and tap water. © Springer-Verlag 2000.
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The College of Arts and Sciences proudly presents the seventh Book of Abstracts, highlighting the undergraduate scholarship conducted by students in collaboration with faculty mentors. This collection of abstracts represents many hours of scholarly activity in which students further developed their research, critical thinking, and writing skills and engaged in learning well beyond the classroom. We congratulate the students and their faculty mentors for the quality of their work and their willingness to share it with the academic community through publications in refereed journals and presentations at regional, national, and international meetings. We also thank Evan Adams for editing the abstracts and Chris Richter, a visual communication design major, for designing the cover and producing the book.
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This State of the Arctic Report presents a review of recent data by an international group of scientists who developed a consensus on the information content and reliability. The report highlights data primarily from 2000 to 2005 with a first look at winter 2006, providing an update to some of the records of physical processes discussed in the Arctic Climate Impact Assessment (ACIA, 2004, 2005). Of particular note: • Atmospheric climate patterns are shifting (Fig. 1). The late winter/spring pattern for 2000–2005 had new hot spots in northeast Canada and the East Siberian Sea relative to 1980–1999. Late winter 2006, however, shows a return to earlier climate patterns, with warm temperatures in the extended region near Svalbard. • Ocean salinity and temperature profiles at the North Pole and in the Beaufort Sea, which changed abruptly in the 1990s, show that conditions since 2000 have relaxed toward the pre-1990 climatology, although 2001–2004 has seen an increase in northward ocean heat transport through Bering Strait (Fig. 2), which is thought to impact sea ice loss. • Sea ice extent continues to decrease. The sea ice extent in September 2005 was the minimum observed in summer during the satellite era (beginning in 1979), marking an unprecedented series of extreme ice extent minima beginning in 2002 (Fig. 3). The sea ice extent in March 2006 was also the minimum observed in winter during the satellite era. • Tundra vegetation greenness increased, primarily due to an increase in the abundance of shrubs. Boreal forest vegetation greenness decreased, possibly due to drought conditions (Fig. 4). • There is increasing interest in the stability of the Greenland ice sheet. The velocity of outlet glaciers increased in 2005 relative to 2000 and 1995, but uncertainty remains with regard to the total mass balance. • Permafrost temperatures continue to increase. However, data on changes in the active layer thickness (the relatively thin layer of ground between the surface and permafrost that undergoes seasonal freezing and thawing) are less conclusive. While some of the sites show a barely noticeable increasing trend in the thickness of the active layer, most of them do not. • Globally, 2005 was the warmest year in the instrumental record (beginning in 1880), with the Arctic providing a large contribution toward this increase. Many of the trends documented in the ACIA are continuing, but some are not. Taken collectively, the observations presented in this report indicate that during 2000–2005 the Arctic system showed signs of continued warming. However, there are a few indications that certain elements may be recovering and returning to recent climatological norms (for example, the central Arctic Ocean and some wind patterns). These mixed tendencies further illustrate the sensitivity and complexity of the Arctic physical system. They underline the importance of maintaining and expanding efforts to observe and better understand this important component of the climate system to provide accurate predictions of its future state.
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Collectively, the observations indicate that the overall warming of the Arctic system continued in 2007. There are some elements that are stabilizing or returning to climatological norms. These mixed tendencies illustrate the sensitivity and complexity of the Arctic System. Atmosphere: Hot spot shifts toward Europe Ocean: North Pole Temperatures at depth returning to 1990s values Sea Ice: Summer extent at record minimum Greenland: Recent warm temperatures associated with net ice loss Biology: increasing tundra shrub cover and variable treeline advance; up to 80% declines in some caribou herds while goose populations double Land: Increase in permafrost temperatures The Arctic Report Card 2007 is introduced as a means of presenting clear, reliable and concise information on recent observations of environmental conditions in the Arctic, relative to historical time series records. It provides a method of updating and expanding the content of the State of the Arctic Report, published in fall 2006, to reflect current conditions. Material presented in the Report Card is prepared by an international team of scientists and is peer-reviewed by topical experts nominated by the US Polar Research Board. The audience for the Arctic Report Card is wide, including scientists, students, teachers, decision makers and the general public interested in Arctic environment and science. The web-based format will facilitate future timely updates of the content.