949 resultados para Angular kinematics


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Experimentos de longa duração constituem ferramenta valiosa para o estudo da dinâmica da matéria orgânica no solo. Com esse objetivo, realizou-se a presente pesquisa a qual foi baseada em experimento instalado, em 1985, em um Argissolo Vermelho degradado pelo cultivo inadequado por 16 anos. O experimento está localizado na Estação Experimental Agronômica da UFRGS, em Eldorado do Sul (RS), e consiste em três sistemas de preparo de solo (preparo convencional-PC, preparo reduzido-PR, e plantio direto-PD) em parcelas principais, três sistemas de culturas (aveia/milho-A/M, ervilhaca/milho-E/M, e aveia + ervilhaca/ milho + caupi-A + E/M + C), em subparcelas, e duas doses de N mineral na cultura do milho (0 e 139 kg ha-1), em subblocos, distribuídos segundo um delineamento de blocos ao acaso, com três repetições. As adições de C e N pelas culturas foram estimadas para o período experimental de 13 anos; o solo foi amostrado, em setembro de 1998, em seis camadas, até à profundidade de 0,30 m, analisado em relação aos teores de carbono orgânico total (COT) e nitrogênio total (NT), tendo sido calculados os estoques desses elementos nas camadas de 0-0,175 e 0,175-0,30 m. As leguminosas contribuíram para a maior adição anual de C e N ao solo pelos sistemas de culturas, que variaram de 4,17 a 8,39 Mg ha-1 e de -21 a 178 kg ha-1, respectivamente. As maiores adições de C e N refletiram-se num maior acúmulo de COT e NT na camada de 0-0,175 m do solo em PD e em gradativa elevação do rendimento do milho nos três sistemas de preparo. A adição anual de C (A) necessária para manter o estoque inicial de COT (dC/dt = zero) foi estimada em 4,2 Mg ha-1 em PD, 7,3 Mg ha-1 em PR e 8,9 Mg ha-1 em PC. De forma similar, a adição anual de N necessária para manter os estoques iniciais (dN/dt = zero) foi estimada em 5 kg ha-1 para o PD, 31 kg ha-1 para o PR e 94 kg ha-1 para o PC. Estimou-se, pelo coeficiente angular da regressão linear que relaciona as taxas anuais de adição de C (A) e a variação anual nos estoques de COT na camada de 0-0,175 m do solo (dC/dt), que 12,9, 8,1 e 11,5 % do C adicionado ao solo foi retido na matéria orgânica do solo em PD, PR e PC, respectivamente, o que corresponde a uma estimativa aproximada do coeficiente de humificação (k1). Analogamente, estimou-se que 49,7, 21,0 e 33,1 % da quantidade líquida de N adicionada foi retida como NT no solo em PD, PR e PC, respectivamente. A taxa de perda de COT do solo (k2), calculada para a condição dC/dt = zero, foi de 0,0166 ano-1 no solo em PD, 0,0182 ano-1 no solo em PR, e 0,0314 ano-1 no solo em PC. O plantio direto, pela diminuição da taxa de perda de matéria orgânica (k2), e os sistemas de culturas com leguminosas, pela alta adição de C fotossintetizado e de N fixado simbioticamente, são boas alternativas para recuperar os estoques de COT e NT do solo e aumentar o rendimento do milho na região subtropical do Sul do Brasil.

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O presente trabalho teve como objetivo estabelecer um método para a utilização de dados espectrais, obtidos em laboratório e imagens do Landsat 5, no reconhecimento e discriminação de três classes de solos do estado de São Paulo. Foram coletadas amostras de solo e obtidos os dados de reflectância por espectrorradiômetro em laboratório como padrão de um Latossolo Vermelho distroférrico (LVdf), um Argissolo Vermelho-Amarelo (PVA) e Neossolo Quartzarênico (RQ). Foram extraídos dados de reflectância das imagens, com os quais se efetuou a classificação digital pelo classificador Spectral Angular Mapper. As curvas espectrais obtidas por espectrorradiômetro em laboratório mostraram três padrões distintos de comportamento espectral, baseados nas diferenças da forma das curvas, feições de absorção dos minerais do solo e na intensidade de reflectância. O LVdf apresentou menor albedo em virtude da textura argilosa e maiores teores de Fe, ao contrário dos solos mais arenosos PVA e RQ. As bandas de absorção características da caulinta (2.200 nm), OH- e água (1.400 e 1.900 nm) ocorreram em todos os solos. Solos arenosos, como o RQ, apresentaram uma curva espectral com tendência positiva. A linha do solo mostrou distinção espectral, tanto com dados orbitais como terrestres, indicando que cada solo tem uma tendência individual. Os padrões espectrais obtidos em laboratório foram importantes para a eficiência do método na detecção dos mesmos nas imagens de satélite. Os solos avaliados podem ser discriminados e reconhecidos pela interpretação quantitativa em imagens. O método mostrou-se eficiente como auxílio no mapeamento de solos no nível semidetalhado de alta intensidade.

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A new statistical parallax method using the Maximum Likelihood principle is presented, allowing the simultaneous determination of a luminosity calibration, kinematic characteristics and spatial distribution of a given sample. This method has been developed for the exploitation of the Hipparcos data and presents several improvements with respect to the previous ones: the effects of the selection of the sample, the observational errors, the galactic rotation and the interstellar absorption are taken into account as an intrinsic part of the formulation (as opposed to external corrections). Furthermore, the method is able to identify and characterize physically distinct groups in inhomogeneous samples, thus avoiding biases due to unidentified components. Moreover, the implementation used by the authors is based on the extensive use of numerical methods, so avoiding the need for simplification of the equations and thus the bias they could introduce. Several examples of application using simulated samples are presented, to be followed by applications to real samples in forthcoming articles.

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We present Stroemgren uvby and Hbeta_ photometry for a set of 575 northern main sequence A type stars, most of them belonging to the Hipparcos Input Catalogue, with V from 5mag to 10mag and with known radial velocities. These observations enlarge the catalogue we began to compile some years ago to more than 1500 stars. Our catalogue includes kinematic and astrophysical data for each star. Our future goal is to perform an accurate analysis of the kinematical behaviour of these stars in the solar neighbourhood.

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Our procedure to detect moving groups in the solar neighbourhood (Chen et al., 1997) in the four-dimensional space of the stellar velocity components and age has been improved. The method, which takes advantadge of non-parametric estimators of density distribution to avoid any a priori knowledge of the kinematic properties of these stellar groups, now includes the effect of observational errors on the process to select moving group stars, uses a better estimation of the density distribution of the total sample and field stars, and classifies moving group stars using all the available information. It is applied here to an accurately selected sample of early-type stars with known radial velocities and Strömgren photometry. Astrometric data are taken from the HIPPARCOS catalogue (ESA, 1997), which results in an important decrease in the observational errors with respect to ground-based data, and ensures the uniformity of the observed data. Both the improvement of our method and the use of precise astrometric data have allowed us not only to confirm the existence of classical moving groups, but also to detect finer structures that in several cases can be related to kinematic properties of nearby open clusters or associations.

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The absolute K magnitudes and kinematic parameters of about 350 oxygen-rich Long-Period Variable stars are calibrated, by means of an up-to-date maximum-likelihood method, using HIPPARCOS parallaxes and proper motions together with radial velocities and, as additional data, periods and V-K colour indices. Four groups, differing by their kinematics and mean magnitudes, are found. For each of them, we also obtain the distributions of magnitude, period and de-reddened colour of the base population, as well as de-biased period-luminosity-colour relations and their two-dimensional projections. The SRa semiregulars do not seem to constitute a separate class of LPVs. The SRb appear to belong to two populations of different ages. In a PL diagram, they constitute two evolutionary sequences towards the Mira stage. The Miras of the disk appear to pulsate on a lower-order mode. The slopes of their de-biased PL and PC relations are found to be very different from the ones of the Oxygen Miras of the LMC. This suggests that a significant number of so-called Miras of the LMC are misclassified. This also suggests that the Miras of the LMC do not constitute a homogeneous group, but include a significant proportion of metal-deficient stars, suggesting a relatively smooth star formation history. As a consequence, one may not trivially transpose the LMC period-luminosity relation from one galaxy to the other.

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Aims.We revisit the vicinity of the microquasar Cygnus X-3 at radio wavelengths. We aim to improve our previous search for possible associated extended radio features/hot spots in the position angle of the Cygnus X-3 relativistic jets focusing on shorter angular scales than previously explored. Methods.Our work is mostly based on analyzing modern survey and archive radio data, mainly including observations carried out with the Very Large Array and the Ryle Telescopes. We also used deep near-infrared images that we obtained in 2005. Results.We present new radio maps of the Cygnus X-3 field computed after combining multi-configuration Very Large Array archive data at 6 cm and different observing runs at 2 cm with the Ryle Telescope. These are probably among the deepest radio images of Cygnus X-3 reported to date at cm wavelengths. Both interferometers reveal an extended radio feature within a few arc-minutes of the microquasar position, thus making our detection more credible. Moreover, this extended emission is possibly non-thermal, although this point still needs confirmation. Its physical connection with the microquasar is tentatively considered under different physical scenarios. We also report on the serendipitous discovery of a likely Fanaroff-Riley type II radio galaxy only away from Cygnus X-3.

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Dezenove amostras de horizontes B latossólicos, uma de B plíntico, uma de B incipiente e uma de horizonte Cr foram submetidas a dissoluções seletivas da goethita e da hematita por ditionito-citratro-bicarbonato de sódio a 20 ºC em intervalos de tempo entre 5 e 3.840 minutos. O diâmetro médio do cristal (DMC), área superficial específica (ASE) e substituição do ferro por Al (substituição por Al3+) da goethita e da hematita nas amostras foram estimados, por difratometria de raios X (DRX), em subamostras não tratadas e em subamostras tratadas selecionadas ao longo das dissoluções seletivas. O controle das fases de goethita e hematita que persistiram após cada etapa da dissolução seletiva foi realizado pelo método da difratometria diferencial de raios X (DDRX). A cinética dissolutiva dos cristais foi descrita por meio da segmentação das curvas de dissolução do ferro no tempo em intervalos em que o comportamento dissolutivo foi linear. As taxas de dissolução nos diferentes segmentos lineares foram estimadas a partir do coeficiente angular da reta relativa a cada segmento. Em amostras goethíticas latossólicas, a metodologia discriminou diferentes fases de goethita (populações heterogêneas) quanto à substituição por Al3+, DMC e ASE e ofereceu condições para classificar o grau de estabilidade da goethita em baixa, média, alta e muito alta estabilidade. Amostras goethíticas oriundas de ambientes pedogênicos jovens e amostras hematíticas latossólicas caracterizaram-se pela maior homogeneidade de seus cristais, classificados como de baixa e média estabilidade. Nas amostras goethíticas, a proporção de cristais com maior estabilidade (alta substituição por Al3+ e cristalinidade) em cada população mostrou associação positiva com a proporção de gibbsita em relação a caulinita nas amostras. A hematita apresentou menor resistência à dissolução por redução em relação à goethita, exceto quando a última combinou baixa substituição por Al3+ e alta ASE. A caracterização de populações heterogêneas de goethita pode ampliar a utilização deste óxido como indicador de processos pedogênicos em solos poligenéticos, bem como contribuir para um melhor entendimento do comportamento químico e físico desses solos.

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Background: Variable definitions of outcome (Constant score, Simple Shoulder Test [SST]) have been used to assess outcome after shoulder treatment, although none has been accepted as the universal standard. Physicians lack an objective method to reliably assess the activity of their patients in dynamic conditions. Our purpose was to clinically validate the shoulder kinematic scores given by a portable movement analysis device, using the activities of daily living described in the SST as a reference. The secondary objective was to determine whether this device could be used to document the effectiveness of shoulder treatments (for glenohumeral osteoarthritis and rotator cuff disease) and detect early failures.Methods: A clinical trial including 34 patients and a control group of 31 subjects over an observation period of 1 year was set up. Evaluations were made at baseline and 3, 6, and 12 months after surgery by 2 independent observers. Miniature sensors (3-dimensional gyroscopes and accelerometers) allowed kinematic scores to be computed. They were compared with the regular outcome scores: SST; Disabilities of the Arm, Shoulder and Hand; American Shoulder and Elbow Surgeons; and Constant.Results: Good to excellent correlations (0.61-0.80) were found between kinematics and clinical scores. Significant differences were found at each follow-up in comparison with the baseline status for all the kinematic scores (P < .015). The kinematic scores were able to point out abnormal patient outcomes at the first postoperative follow-up.Conclusion: Kinematic scores add information to the regular outcome tools. They offer an effective way to measure the functional performance of patients with shoulder pathology and have the potential to detect early treatment failures.Level of evidence: Level II, Development of Diagnostic Criteria, Diagnostic Study. (C) 2011 Journal of Shoulder and Elbow Surgery Board of Trustees.

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The purpose of this study was to examine the physiological and biomechanical changes occurring in a subject after running 8,500 km in 161 days (i.e. 52.8 km daily). Three weeks before, 3 weeks after (POST) and 5 months after (POST+5) running from Paris to Beijing, energy cost of running (Cr), knee flexor and extensor isokinetic strength and biomechanical parameters (using a treadmill dynamometer) at different velocities were assessed in an experienced ultra-runner. At POST, there was a tendency toward a 'smoother' running pattern, as shown by (a) a higher stride frequency and duty factor, and a reduced aerial time without a change in contact time, (b) a lower maximal vertical force and loading rate at impact and (c) a decrease in both potential and kinetic energy changes at each step. This was associated with a detrimental effect on Cr (+6.2%) and a loss of strength at all angular velocities for both knee flexors and extensors. At POST+5, the subject returned to his original running patterns at low but not at high speeds and maximal strength remained reduced at low angular velocities (i.e. at high levels of force). It is suggested that the running pattern changes observed in the present study were a strategy adopted by the subject to reduce the deleterious effects of long distance running. However, the running pattern changes could partly be linked to the decrease in maximal strength.

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The oxidation of GaAs and AlGaAs targets subjected to O2+ bombardment has been analyzed, using in situ x¿ray photoelectron spectroscopy, as a function of time until steady state is reached. The oxides formed by the O2+ bombardment have been characterized in terms of composition and binding energy. A strong energy and angular dependence for the oxidation of As relative to Ga is found. Low energies as well as near normal angles of incidence favor the oxidation of As. The difference between Ga and As can be explained in terms of the formation enthalpy for the oxide and the excess supply of oxygen. In an AlGaAs target the Al is very quickly completely oxidized irrespective of the experimental conditions. The steady state composition of the altered layers show in all cases a preferential removal of As.

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This paper focuses on new paleontological discoveries that have come to light while working on a Permian "paieobotanical" transect. from Oman to Central Morocco, In the Huqf area, the continental plant bearing "Gharif" Formation is bracketed by two welt dated marine Formations, providing new age constraint for the discovered "mixed" paleoHora, The newly named KubergarH;Jian'Murgabian "Gharif Paleoflora" is of outstanding paleogeographic .ignificance, Gondwanan, Cathaysian and Euramerian elements are found to be associated, The understanding of the kinematics of the Permian vegetal cover lead us to test the proposed Peri-Tethyan paleogeographical contours

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High-speed running accounts for the majority of hamstring strains in many sports. The terminal swing phase is believed to be the most hazardous as the hamstrings are undergoing an active lengthening contraction in a long muscle length position. Prevention-based strength training mainly focuses on eccentric exercises. However, it appears crucial to integrate other parameters than the contraction type. Therefore, the aim of this study is to present a conceptual framework based on six key parameters (contraction type, load, range of motion, angular velocity, uni-/bilateral exercises, kinetic chain) for the hamstring's strength exercise for strain prevention. Based on the biomechanical parameters of sprinting, it is proposed to use high-load eccentric contractions. The movement should be performed at a slow to moderate angular velocity and focused at the knee joint, while the hip is kept in a large flexion position in order to reach a greater elongation stress of the hamstrings than in the terminal swing phase. In this way, we believe that, during sprinting, athletes would be better trained to brake the knee extension effectively in the whole range of motion without overstretch of the hamstrings. Finally, based on its functional application, unilateral open kinetic chain should be preferred.

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Within current-density-functional theory, we have studied a quantum dot made of 210 electrons confined in a disk geometry. The ground state of this large dot exhibits some features as a function of the magnetic field (Beta) that can be attributed in a clear way to the formation of compressible and incompressible states of the system. The orbital and spin angular momenta, the total energy, ionization and electron chemical potentials of the ground state, as well as the frequencies of far-infrared edge modes are calculated as a function of Beta, and compared with available experimental and theoretical results.

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We have employed time-dependent local-spin density-functional theory to analyze the multipole spin and charge density excitations in GaAs-AlxGa1-xAs quantum dots. The on-plane transferred momentum degree of freedom has been taken into account, and the wave-vector dependence of the excitations is discussed. In agreement with previous experiments, we have found that the energies of these modes do not depend on the transferred wave vector, although their intensities do. Comparison with a recent resonant Raman scattering experiment [C. Schüller et al., Phys. Rev. Lett. 80, 2673 (1998)] is made. This allows us to identify the angular momentum of several of the observed modes as well as to reproduce their energies