Efeito da aplicação de ondas de choque extracorpóreas na placa epifisária da tíbia de coelhos

Pós-graduação em Medicina Veterinária - FMVZ

Ocorrência de ostras perlíferas no Marajó, rio Pará

Ostras perlíferas foram encontradas em águas que circundam a parte sul da ilha do Marajó, próxima à confluência dos rios Tocantins e Pará. As conchas das ostras possuem uma camada espessa de conchiolina, que lhes confere qualidades de madrepérola. Um lote de 12 pérolas naturais apresentou as seguintes características: cores variadas do branco rosa ao cinza escuro; tamanhos de 3 a 11 mm; formas esféricas a subesféricas, cilíndricas (algumas cinturadas) a barrocas. Sob irradiação UV de onda longa, duas amostras apresentaram cor azul forte e uma cor azul média. Respectivamente cores azuis mais fracas são obtidas por UV de onda curta. A parte interna da concha da ostra apresenta cor azul fraca, tanto sob irradiação UV de onda longa quanto de onda curta. A superfície externa das pérolas é lisa com brilho nacarado característico, sendo que algumas apresentam um tom metálico dourado. Essa é, provavelmente, a primeira região brasileira mais importante com ocorrência de pérolas naturais atuais, abrindo perspectivas para a produção de pérolas cultivadas em água doce.

Modelos de estimativa da radiação atmosférica em função da temperatura, umidade e dos índices radiométricos Kt e Kd para Botucatu - SP

Pós-graduação em Agronomia (Energia na Agricultura) - FCA

Modelling the surface circulation and thermal structure of a tropical reservoir using three-dimensional hydrodynamic lake model and remote-sensing data

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

Index of thermal stress for cows (ITSC) under high solar radiation in tropical environments

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

Carlosbarbosaite, ideally (UO2)(2)Nb2O6(OH)(2)center dot 2H(2)O, a new hydrated uranyl niobate mineral with tunnels from Jaguaracu, Minas Gerais, Brazil: description and crystal structure

Carlosbarbosaite, ideally (UO2)(2)Nb2O6(OH)(2)center dot 2H(2)O, is a new mineral which occurs as a late cavity filling in albite in the Jaguaracu pegmatite, Jaguaracu municipality, Minas Gerais, Brazil. The name honours Carlos do Prado Barbosa (1917-2003). Carlosbarbosaite forms long flattened lath-like crystals with a very simple orthorhombic morphology. The crystals are elongated along [001] and flattened on (100); they are up to 120 mu m long and 2-5 mu m thick. The colour is cream to pale yellow, the streak yellowish white and the lustre vitreous. The mineral is transparent (as individual crystals) to translucent (massive). It is not fluorescent under either long-wave or short-wave ultraviolet radiation. Carlosbarbosaite is biaxial(+) with alpha = 1.760(5), beta = 1.775(5), gamma = 1.795(5), 2V(meas) = 70(1)degrees, 2V(calc) = 83 degrees. The orientation is X parallel to a, Y parallel to b, Z parallel to c. Pleochroism is weak, in yellowish green shades, which are most intense in the Z direction. Two samples were analysed. For sample I, the composition is: UO3 54.52, CaO 2.07, Ce2O3 0.33, Nd2O3 0.49, Nb2O5 14.11, Ta2O5 15.25, TiO2 2.20, SiO2 2.14, Fe2O3 1.08, Al2O3 0.73, H2O (calc.) 11.49, total 104.41 wt.%; the empirical formula is (square 0.68Ca0.28Nd0.02Ce0.02)(Sigma=1.00)[U-1.44 square O-0.56(2.88)(H2O)(1.12)](Nb0.80Ta0.52Si0.27Ti0.21Al0.11Fe0.10)(Sigma=2.01) O-4.72(OH)(3.20)(H2O)(2.08). For sample 2, the composition is: UO3 41.83, CaO 2.10, Ce2O3 0.31, Nd2O3 1.12, Nb2O5 14.64, Ta2O5 16.34, TiO2 0.95, SiO2 3.55, Fe2O3 0.89, Al2O3 0.71, H2O (calc.) 14.99, total 97.43 wt.%; the empirical formula is (square 0.67Ca0.27Nd0.05Ce0.01)(Sigma=1.00)[U-1.04 square O-0.96(2.08)(H2O)(1.92)] (Nb0.79Ta0.53Si0.42Ti0.08Al0.10Fe0.08)(Sigma=2.00)O-4.00(OH)(3.96)(H2O)(2.04). The ideal endmember formula is (UO2)(2)Nb2O6(OH)(2)center dot 2H(2)O. Calculated densities are 4.713 g cm(-3) (sample 1) and 4.172 g cm(-3) (sample 2). Infrared spectra show that both (OH) and H2O are present. The strongest eight X-ray powder-diffraction lines [listed as d in angstrom(I)(hkl)] are: 8.405(8)(110), 7.081(10)(200), 4.201(9)(220), 3.333(6)(202), 3.053(8)(022), 2.931(7)(420), 2.803(6)(222) and 2.589(5)(040,402). The crystal structure was solved using single-crystal X-ray diffraction (R = 0.037) which gave the following data: orthorhombic, Cmem, a = 14.150(6), b = 10.395(4), c = 7.529(3) angstrom, V = 1107(1) angstrom(3), Z = 4. The crystal structure contains a single U site with an appreciable deficiency in electron scattering, which is populated by U atoms and vacancies. The U site is surrounded by seven 0 atoms in a pentagonal bipyramidal arrangemet. The Nb site is coordinated by four 0 atoms and two OH groups in an octahedral arrangement. The half-occupied tunnel Ca site is coordinated by four 0 atoms and four H2O groups. Octahedrally coordinated Nb polyhedra share edges and comers to form Nb2O6(OH)(2) double chains, and edge-sharing pentagonal bipyramidal U polyhedra form UO5 chains. The Nb2O6(OH)(2) and UO5 chains share edges to form an open U-Nb-phi framework with tunnels along [001] that contain Ca(H2O)(4) clusters. Carlosbarbosaite is closely related to a family of synthetic U-Nb-O framework tunnel structures, it differs in that is has an (OH)-bearing framework and Ca(H2O)(4) tunnel occupant. The structure of carlosbarbosaite resembles that of holfertite.

Atmospheric radiative transfer in multiple scattering conditions. Application to NWP models.

High spectral resolution radiative transfer (RT) codes are essential tools in the study of the radiative energy transfer in the Earth atmosphere and a support for the development of parameterizations for fast RT codes used in climate and weather prediction models. Cirrus clouds cover permanently 30% of the Earth's surface, representing an important contribution to the Earth-atmosphere radiation balance. The work has been focussed on the development of the RT model LBLMS. The model, widely tested in the infra-red spectral range, has been extended to the short wave spectrum and it has been used in comparison with airborne and satellite measurements to study the optical properties of cirrus clouds. A new database of single scattering properties has been developed for mid latitude cirrus clouds. Ice clouds are treated as a mixture of ice crystals with various habits. The optical properties of the mixture are tested in comparison to radiometric measurements in selected case studies. Finally, a parameterization of the mixture for application to weather prediction and global circulation models has been developed. The bulk optical properties of ice crystals are parameterized as functions of the effective dimension of measured particle size distributions that are representative of mid latitude cirrus clouds. Tests with the Limited Area Weather Prediction model COSMO have shown the impact of the new parameterization with respect to cirrus cloud optical properties based on ice spheres.

Phylogenetische Charakterisierung von Mikroorganismen aus dem Intestinaltrakt von Insekten

Zusammenfassung Die komplexe Lebensgemeinschaft des Termitendarms fasziniert die Biologen schon seit langem. Es ist bekannt, dass Termiten ihre Nahrung mit Hilfe von symbiontischen Bakterien und Protozoen verdauen können. Ohne ihre Symbionten würden sie verhungern. Das Zusammenspiel von Termiten und darmbewohnenden Mikroorganismen, zu denen Flagellaten, Bakterien, Archaebakterien und Hefen gehören, ist trotz moderner Untersuchungstechniken keineswegs vollständig aufgeklärt. In der vorliegenden Arbeit wurden:1) Einige kultivierte und nicht-kultivierte Bakterien charakterisiert, die an der Darmwand von Mastotermes darwiniensis lokalisiert sind. Die Darmwandbakterien wurden entweder nach Kultivierung oder direkt von der Darmwand für die Analyse der 16S rDNA verwendet. Die Sequenzierung erfolgte entweder nach DGGE oder nach Klonierung der PCR-Produkte. Die identifizierten Bakterien kann man in 7 Gruppen teilen:1: Gram-positive Bakterien mit hohem GC-Gehalt 2: Gram-positive Bakterien mit niedrigem GC-Gehalt 3: Fusobakterien-ähnliche Bakterien 4: ß-Proteobakterien5: Verrucomicrobien6: Bacteroides-ähnliche Bakterien7: Methanogene Bakterien 2) Aufgrund des Vorhandenseins des Coenzyms Deazaflavin-Derivats F420, kann man Methanbakterien mikroskopisch identifizieren und von anderen Bakterien unterscheiden, weil Methanbakterien im kurzwelligen Blaulicht blaugrün aufleuchten. Untersuchungen haben gezeigt, dass mindestens zwei Morphotypen von Methanbakterien an der Darmwand von M. darwiniensis vorkommen. Sie wurden auch über 16S rDNA Sequenzanalyse identifiziert. Ihre Lokalisierung an der Darmwand wurde durch Fluoreszenz-in-situ-Hybridsierung mit spezifischen Oligonukleotiden nachgewiesen. Schließlich konnte gezeigt werden, dass pro Gramm Termite 2,6 µg Methan pro Stunde produziert werden. 3) Bis jetzt wurden aus verschiedenen Termiten sulfatreduzierende Bakterien (SRB) isoliert. Deshalb wurde in dieser Arbeit die Verbreitung der SRB in verschiedenen Insekten untersucht. Insgesamt wurden zwei Sequenzen aus Libellenlarven (FSBO4 und FSBRO2), drei Sequenzen aus Zuckmückenlarven (FSCI, FSCII und FSC4), eine Sequenz aus Rosenkäfern (FSPa4-5) und ebenfalls eine Sequenz aus Eintagsfliegenlarven (FSB6) identifiziert. Alle identifizierten Bakterien ausser Klon FSB6, gehören zur Gattung Desulfovibrio. Klon FSB6 gehört zu der Gram-positiven Gattung Desulfotomaculum.Außerdem wurde die Sulfatreduktionsrate der SRB im Darm von Rosenkäfern (Pachnoda marginata), Holz- bzw. Sulfat-gefütterten Termiten (Mastotermes darwiniensis) und einer Reinkultur von Desulfovibrio intestinalis gemessen. Dabei konnte gezeigt werden, dass die Aktivität pro Zelle in Holz-gefütterten Termite am höchsten ist (4,9 nmol/107 Bakterien x h).

The effect of high-energy extracorporeal shock waves on hyaline cartilage of adult rats in vivo

The aim of this study was to determine if extracorporeal shock wave therapy (ESWT) in vivo affects the structural integrity of articular cartilage. A single bout of ESWT (1500 shock waves of 0.5 mJ/mm(2)) was applied to femoral heads of 18 adult Sprague-Dawley rats. Two sham-treated animals served as controls. Cartilage of each femoral head was harvested at 1, 4, or 10 weeks after ESWT (n = 6 per treatment group) and scored on safranin-O-stained sections. Expression of tenascin-C and chitinase 3-like protein 1 (Chi3L1) was analyzed by immunohistochemistry. Quantitative real-time polymerase chain reaction (PCR) was used to examine collagen (II)alpha(1) (COL2A1) expression and chondrocyte morphology was investigated by transmission electron microscopy no changes in Mankin scores were observed after ESWT. Positive immunostaining for tenascin-C and Chi3L1 was found up to 10 weeks after ESWT in experimental but not in control cartilage. COL2A1 mRNA was increased in samples 1 and 4 weeks after ESWT. Alterations found on the ultrastructural level showed expansion of the rough-surfaced endoplasmatic reticulum, detachment of the cell membrane and necrotic chondrocytes. Extracorporeal shock waves caused alterations of hyaline cartilage on a molecular and ultrastructural level that were distinctly different from control. Similar changes were described before in the very early phase of osteoarthritis (OA). High-energy ESWT might therefore cause degenerative changes in hyaline cartilage as they are found in initial OA.

Biaxial extensional motion of an inertially driven radially expanding liquid sheet

We consider the inertially driven, time-dependent biaxial extensional motion of inviscid and viscous thinning liquid sheets. We present an analytic solution describing the base flow and examine its linear stability to varicose (symmetric) perturbations within the framework of a long-wave model where transient growth and long-time asymptotic stability are considered. The stability of the system is characterized in terms of the perturbation wavenumber, Weber number, and Reynolds number. We find that the isotropic nature of the base flow yields stability results that are identical for axisymmetric and general two-dimensional perturbations. Transient growth of short-wave perturbations at early to moderate times can have significant and lasting influence on the long-time sheet thickness. For finite Reynolds numbers, a radially expanding sheet is weakly unstable with bounded growth of all perturbations, whereas in the inviscid and Stokes flow limits sheets are unstable to perturbations in the short-wave limit.

CH4, CO, and H2O spectroscopy for the Sentinel-5 Precursor mission: an assessment with the Total Carbon Column Observing Network measurements

The TROPOspheric Monitoring Instrument (TROPOMI) will be part of ESA's Sentinel-5 Precursor (S5P) satellite platform scheduled for launch in 2015. TROPOMI will monitor methane and carbon monoxide concentrations in the Earth's atmosphere by measuring spectra of back-scattered sunlight in the short-wave infrared (SWIR). S5P will be the first satellite mission to rely uniquely on the spectral window at 4190–4340 cm−1 (2.3 μm) to retrieve CH4 and CO. In this study, we investigated if the absorption features of the three relevant molecules CH4, CO, and H2O are adequately known. To this end, we retrieved total columns of CH4, CO, and H2O from absorption spectra measured by two ground-based Fourier transform spectrometers that are part of the Total Carbon Column Observing Network (TCCON). The retrieval results from the 4190–4340 cm−1 range at the TROPOMI resolution (0.45 cm−1) were then compared to the CH4 results obtained from the 6000 cm−1 region, and the CO results obtained from the 4190–4340 cm−1 region at the higher TCCON resolution (0.02 cm−1). For TROPOMI-like settings, we were able to reproduce the CH4 columns to an accuracy of 0.3% apart from a constant bias of 1%. The CO retrieval accuracy was, through interference, systematically influenced by the shortcomings of the CH4 and H2O spectroscopy. In contrast to CH4, the CO column error also varied significantly with atmospheric H2O content. Unaddressed, this would introduce seasonal and latitudinal biases to the CO columns retrieved from TROPOMI measurements. We therefore recommend further effort from the spectroscopic community to be directed at the H2O and CH4 spectroscopy in the 4190–4340 cm−1 region.