Quantificação do carbono das substâncias húmicas em diferentes sistemas de uso do solo e épocas de avaliação.

A quantificação do carbono nas diferentes frações da matéria orgânica do solo (MOS) torna-se necessária devido ao interesse de se conhecer o potencial de captura e armazenamento do carbono nos diferentes sistemas de uso do solo. O objetivo deste trabalho foi quantificar o carbono das substâncias húmicas em diferentes sistemas de uso do solo e épocas de avaliação e correlacioná-lo com algumas propriedades químicas e físicas do solo. Os sistemas selecionados foram: preparo convencional (PC-milho/feijão), plantio direto (PD-berinjela/milho), consórcio maracujá/Desmodium sp, cultivo com figo e sistema agroflorestal. As amostras de solo foram coletadas em duas profundidades (0-5 e 5-10 cm) e épocas (17/11/2005–verão e 23/6/2006-inverno). Foi determinado o carbono orgânico total (COT) e realizado o fracionamento químico da MOS, quantificando-se o carbono da fração humina (C-HUM), fração ácido húmico (C-FAH) e fração ácido fúlvico (C-FAF). O C-HUM constituiu a maior parte do COT, havendo correlação significativa com o COT em todos os sistemas avaliados e estações. Analisando o C-FAH foi possível identificar alterações no solo relacionadas aos sistemas de uso, na profundidade de 0-5 cm e no verão, destacando-se o PD com os maiores teores. Com o C-FAF ocorreu este mesmo comportamento, mas na profundidade de 5-10 cm e no inverno, destacando-se o PC com maiores valores. Foram verificadas correlações significativas entre Valor S, Valor T e DMP em todos os sistemas, com exceção da área de PC. O PD aumenta os teores de C-FAH, nas duas profundidades e nas duas estações, quando comparado ao PC do solo

CORRELAÇÃO GENÉTICA, FENOTÍPICA E AMBIENTAL EM CARACTERÍSTICAS DE CRESCIMENTO DE BOVINOS DA RAÇA NELORE VARIEDADE MOCHA

The objective of this work was estimate the genetic correlations, environmental and phenotypic on the birth weight (WB) and on the 205 (W205), 365 (W365) and 550 (W550) days of age, in animals of the polled nellore breed from Bahia state. The analyses were carried out by software MTDFREML. The genetic correlations were 0.08 (WB and W205), 0.00 (WB and W365), - 0.14 (WB and W550), 0.90 (W205 and W365), 0.81 (W205 and W550) and 0.97 (W205 and W550). The environmental correlations were 0.12 (WB and W205), 0.11 (WB and W365) and 0.16 (WB and W550), 0.35 (W205 and W365), 0.13 (W205 and W550) and 0.54 (W365 and W550). The phenotypic correlations were 0.09 (WB and W205), 0.05 (WB and W365), 0.00 (WB and W550), 0.75 (W205 and W365), 0.65 (W205 and W550) and 0.87 (W365 and W550). The birth weight presented weak genetic, environmental, and phenotypic associations with the others weighting. On the other hand, the values gotten for the genetic correlations between the other weighting, indicates that the selection for weight in young ages will promote changes on the future weights of the animal.O objetivo deste trabalho foi estimar as correlações genéticas, fenotípicas e ambientais sobre os pesos ao nascimento (PN) e aos 205 (P205), 365 (P365) e 550 (P550) dias de idade, em animais da raça Nelore Mocha, criados no estado da Bahia. As análises bi-características foram realizadas através do programa MTDFREML. As correlações genéticas foram iguais a 0,08 (PN e P205), 0,00 (PN e P365), - 0,14 (PN e P550), 0,90 (P205 e P365), 0,81, (P205 e P550) e 0,97 (P365 e P550). As correlações ambientais foram 0,12 (PN e P205), 0,11 (PN e P365), 0,16 (PN e P550), 0,35 (P205 e P365), 0,13 (P205 e P550) e 0,54 (P365 e P550). Os valores obtidos para as correlações fenotípicas foram 0,09 (PN e P205), 0,05 (PN e P365), 0,00 (PN e P550), 0,75 (P205 e P365) 0,65 (P205 e P550) e 0,87 (P365 e P550). O peso ao nascimento apresentou ausência de associações genéticas, ambientais e fenotípicas com as demais pesagens. Por outro lado, os valores obtidos para as correlações genéticas entre as outras pesagens, indicam que a seleção para peso em idades jovens deverá promover mudanças nos pesos posteriores dos animais

Prospects for asteroseismology

The observational basis for asteroseismology is being dramatically strengthened, through more than two years of data from the CoRoT satellite, the flood of data coming from the Kepler mission and, in the slightly longer term, from dedicated ground-based facilities. Our ability to utilize these data depends on further development of techniques for basic data analysis, as well as on an improved understanding of the relation between the observed frequencies and the underlying properties of the stars. Also, stellar modelling must be further developed, to match the increasing diagnostic potential of the data. Here we discuss some aspects of data interpretation and modelling, focussing on the important case of stars with solar-like oscillations.Comment: Proc. HELAS Workshop on 'Synergies between solar and stellar modelling', eds M. Marconi, D. Cardini & M. P. Di Mauro, Astrophys. Space Sci., in the press Revision: correcting abscissa labels on Figs 1 and

Fitting the integrated Spectral Energy Distributions of Galaxies

Fitting the spectral energy distributions (SEDs) of galaxies is an almost universally used technique that has matured significantly in the last decade. Model predictions and fitting procedures have improved significantly over this time, attempting to keep up with the vastly increased volume and quality of available data. We review here the field of SED fitting, describing the modelling of ultraviolet to infrared galaxy SEDs, the creation of multiwavelength data sets, and the methods used to fit model SEDs to observed galaxy data sets. We touch upon the achievements and challenges in the major ingredients of SED fitting, with a special emphasis on describing the interplay between the quality of the available data, the quality of the available models, and the best fitting technique to use in order to obtain a realistic measurement as well as realistic uncertainties. We conclude that SED fitting can be used effectively to derive a range of physical properties of galaxies, such as redshift, stellar masses, star formation rates, dust masses, and metallicities, with care taken not to over-interpret the available data. Yet there still exist many issues such as estimating the age of the oldest stars in a galaxy, finer details ofdust properties and dust-star geometry, and the influences of poorly understood, luminous stellar types and phases. The challenge for the coming years will be to improve both the models and the observational data sets to resolve these uncertainties. The present review will be made available on an interactive, moderated web page (sedfitting.org), where the community can access and change the text. The intention is to expand the text and keep it up to date over the coming years.Comment: 54 pages, 26 figures, Accepted for publication in Astrophysics & Space Scienc

Hydrothermal vents and methane seeps: rethinking the sphere of influence

Although initially viewed as oases within a barren deep ocean, hydrothermal vents and methane seep chemosynthetic communities are now recognized to interact with surrounding ecosystems on the sea floor and in the water column, and to affect global geochemical cycles. The importance of understanding these interactions is growing as the potential rises for disturbance of the systems from oil and gas extraction, seabed mining and bottom trawling. Here we synthesize current knowledge of the nature, extent and time and space scales of vent and seep interactions with background systems. We document an expanded footprint beyond the site of local venting or seepage with respect to elemental cycling and energy flux, habitat use, trophic interactions, and connectivity. Heat and energy are released, global biogeochemical and elemental cycles are modified, and particulates are transported widely in plumes. Hard and biotic substrates produced at vents and seeps are used by "benthic background" fauna for attachment substrata, shelter, and access to food via grazing or through position in the current, while particulates and fluid fluxes modify planktonic microbial communities. Chemosynthetic production provides nutrition to a host of benthic and planktonic heterotrophic background species through multiple horizontal and vertical transfer pathways assisted by flow, gamete release, animal movements, and succession, but these pathways remain poorly known. Shared species, genera and families indicate that ecological and evolutionary connectivity exists among vents, seeps, organic falls and background communities in the deep sea: the genetic linkages with inactive vents and seeps and background assemblages however, are practically unstudied. The waning of venting or seepage activity generates major transitions in space and time that create links to surrounding ecosystems, often with identifiable ecotones or successional stages. The nature of all these interactions is dependent on water depth, as well as regional oceanography and biodiversity. Many ecosystem services are associated with the interactions and transitions between chemosynthetic and background ecosystems, for example carbon cycling and sequestration, fisheries production, and a host of non-market and cultural services. The quantification of the sphere of influence of vents and seeps could be beneficial to better management of deep-sea environments in the face of growing industrialization

Análise de diversidade genética do gene da osteopontina em bovinos da raça girolando

Objetivou-se obter os índices de diversidade genética para o SNP (single nucleotide polymorphism) do íntron 4 do gene da osteopontina (OPN) para 434 animais (87 touros e 347 vacas) participantes do Teste de Progênie da raça girolando no Brasil. Para a amplificação, foram utilizados primers descritos para a raça holandesa, e a diferenciação dos alelos C/T desse SNP foi obtida por meio da técnica de PCR-RFLP. As frequências genotípicas TT (52,53%), CT (38,71%) e CC (8,76%) e as frequências alélicas de T (71,9%) e C (28,1%) indicam que a população encontra-se em Equilíbrio de Hardy-Weinberg (EHW). Apesar de o loco do gene OPN estar em EHW, a frequência superior do alelo T do SNP nesses animais pode sugerir uma tendência de fixação do alelo T na raça. Não foi observada diferenciação entre o grupo de touros e vacas (F ST = -0,018), corroborando a estimativa de equilíbrio da população. Considerando os valores estimados pelo F IS (0,043), é possível que ocorram altos números de indivíduos homozigotos para o alelo T observados na população, em virtude da provável herança desse alelo vindo da raça zebuína, e não a endogamia. Assim, para melhor caracterização do polimorfismo do gene OPN, devem ser realizadas avaliações em maior número de animais, uma vez que só foram avaliados animais participantes do teste de progênie.The objective was to obtain the indices of genetic diversity for the SNP (single nucleotide polymorphism) of the 4 intron osteopontin gene (OPN) for 434 animals (87 bulls and 347 cows) participants in the Teste de Progênie da raça girolando (Girolando Progeny Test) in Brazil. For amplification, primers used were described for the Holstein breed, and differentiation of alleles C/T SNP that was obtained by PCR-RFLP. Genotype frequencies of TT (52.53%), CT (38.71%) and CC (8.76%) and allele frequencies of T (71.9%) and C (28.1%) indicate that the population is in Hardy-Weinberg principle (HWP). Although the OPN gene locus is in HWP, the higher frequency of allele T of SNP in these animals may suggest a setting-trend of allele T in the race. No difference was observed between the group of bulls and cows (F ST = -0.018), supporting the estimate of population balance. Considering the values estimated by the F IS (0.043), it is likely that high numbers of individuals homozygous for the T allele observed in the population occur because of possible inheritance of this allele coming from the zebu breed, rather than inbreeding. Thus, to better characterize the OPN gene polymorphism, assessments in a larger number of animals must be performed, since only animals that participated in the Progeny Test were assessed

Soybean crop area estimation by Modis/Evi data

The objective of this work was to develop a procedure to estimate soybean crop areas in Rio Grande do Sul state, Brazil. Estimations were made based on the temporal profiles of the enhanced vegetation index (Evi) calculated from moderate resolution imaging spectroradiometer (Modis) images. The methodology developed for soybean classification was named Modis crop detection algorithm (MCDA). The MCDA provides soybean area estimates in December (first forecast), using images from the sowing period, and March (second forecast), using images from the sowing and maximum crop development periods. The results obtained by the MCDA were compared with the official estimates on soybean area of the Instituto Brasileiro de Geografia e Estatística. The coefficients of determination ranged from 0.91 to 0.95, indicating good agreement between the estimates. For the 2000/2001 crop year, the MCDA soybean crop map was evaluated using a soybean crop map derived from Landsat images, and the overall map accuracy was approximately 82%, with similar commission and omission errors. The MCDA was able to estimate soybean crop areas in Rio Grande do Sul State and to generate an annual thematic map with the geographic position of the soybean fields. The soybean crop area estimates by the MCDA are in good agreement with the official agricultural statistics