A influência da qualidade dos habitats sobre os polinizadores de berinjela e a produtividade dos cultivos

Pós-graduação em Ciências Biológicas (Zoologia) - IBRC

Qualidade da madeira de eucalipto em função do espaçamento, da adubação e da idade conduzida no sistema de curta rotação

Pós-graduação em Ciência Florestal - FCA

Atributos físicos e químicos do solo sob cultivos de outono-inverno em sistema de semeadura direta

Pós-graduação em Agronomia (Agricultura) - FCA

Absorção de nutrientes e alterações químicas em Latossolos cultivados com plantas de cobertura em rotação com soja e milho

The effects on soil chemical properties brought about by cover crops vary considerably. This study was conducted to evaluate nutrient uptake by five cover crops used for grain, seed and forage production at different seed densities per hectare, as well as uptake by spontaneous vegetation, and their effect on the chemical properties of two Oxisols when grown in rotation with soybean and corn. The experiments were set up in Votuporanga, SP, Brazil and Selvíria, MS, Brazil in March 2008 after conventional soil tillage. A randomized complete block experimental design was used with four replications with the following cover crops at different seed densities: Sorghum bicolor at 6, 7 and 8 kg ha-1; Pennisetum americanum at 10, 15 and 20 kg ha-1; Sorghum sudanense at 12, 15 and 18 kg ha-1; hybrid of Sorghum bicolor with Sorghum sudanense at 8, 9 and 10 kg ha-1; and Urochloa ruziziensis at 8, 12 and 16 kg ha-1. We also used a spontaneous vegetation control. After management of the cover crops, in the first year of study, soybean was sown in no-tillage system and, in the second year, corn was sown, also in a no-tillage system. We evaluated the dry matter yield of different cover crops, nutrient uptake by the cover crops, and the chemical changes in the soil. It was found that in clayey soils with high aluminum content, as in Selvíria, sudan grass at a seed density of 18 kg ha-1, and sorghum at a seed density of 6 kg ha-1, in combination with liming, contributed to reduction of aluminum content and high potential acidity and an increase in base saturation. The different seed densities of each cover crop did not affect the dry matter yield of the cover crop itself, but affected nitrogen uptake of the hybrid Sorghum bicolor with Sorghum sudanense at a seed density of 10 kg ha-1, with lower uptake than at a seed density of 8 kg ha-1. Seed density also affected the organic matter content in the soil with sudan grass, with the seed density of 15 kg ha-1 providing more organic matter content than a seed density of 18 kg ha-1.

Arbuscular mycorrhizal fungal communities and soil aggregation as affected by cultivation of various crops during the sugarcane fallow period

Management systems involving crop rotation, ground cover species and reduced soil tillage can improve the soil physical and biological properties and reduce degradation. The primary purpose of this study was to assess the effect of various crops grown during the sugarcane fallow period on the production of glomalin and arbuscular mycorrhizal fungi in two Latosols, as well as their influence on soil aggregation. The experiment was conducted on an eutroferric Red Latosol with high-clay texture (680 g clay kg-1) and an acric Red Latosol with clayey texture (440 g kg-1 clay) in Jaboticabal (São Paulo State, Brazil). A randomized block design involving five blocks and four crops [soybean (S), soybean/fallow/soybean (SFS), soybean/millet/soybean (SMS) and soybean/sunn hemp/soybean (SHS)] was used to this end. Soil samples for analysis were collected in June 2011. No significant differences in total glomalin production were detected between the soils after the different crops. However, total external mycelium length was greater in the soils under SMS and SHS. Also, there were differences in easily extractable glomalin, total glomalin and aggregate stability, which were all greater in the eutroferric Red Latosol than in the acric Red Latosol. None of the cover crops planted in the fallow period of sugarcane improved aggregate stability in either Latosol.

Ruzigrass affecting soil-phosphorus availability

The objective of this work was to evaluate the effectiveness of ruzigrass (Urochloaruziziensis) in enhancing soil-P availability in areas fertilized with soluble or reactive rock phosphates. The area had been cropped for five years under no-till, in a system involving soybean, triticale/black-oat, and pearl millet. Previously to the five-year cultivation period, corrective phosphorus fertilization was applied once on soil surface, at 0.0 and 80 kg ha-1 P2O5, as triple superphosphate or Arad rock phosphate. After this five-year period, plots received the same corrective P fertilization as before and ruzigrass was introduced to the cropping system in the stead of the other cover crops. Soil samples were taken (0-10 cm) after ruzigrass cultivation and subjected to soil-P fractionation. Soybean was grown thereafter without P application to seed furrow. Phosphorus availability in plots with ruzigrass was compared to the ones with spontaneous vegetation for two years. Ruzigrass cultivation increased inorganic (resin-extracted) and organic (NaHCO3) soil P, as well as P concentration in soybean leaves, regardless of the P source. However, soybean yield did not increase significantly due to ruzigrass introduction to the cropping system. Soil-P availability did not differ between soluble and reactive P sources. Ruzigrass increases soil-P availability, especially where corrective P fertilization is performed.

Estrutura de populações e inoculações recíprocas de Xylella fastidiosa subsp. pauca com ocorrência em cultivos vizinhos de Citrus sinensis e Coffea arabica sob condições do estado de São Paulo

Pós-graduação em Agronomia (Genética e Melhoramento de Plantas) - FCAV

Análise econômica do plantio e condução do eucalipto de curta rotação para fins energéticos

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

Comportamento dos músculos estabilizadores da escápula durante rotação de ombro em indivíduos com síndrome do impacto

Devido à grande diversidade de problemas no ombro e da alta incidência da Síndrome do Impacto (SI) torna-se de grande interesse e importância para a reabilitação o comportamento dos músculos da cintura escapular. O objetivo deste estudo foi analisar a ação simultânea dos músculos serrátil anterior e trapézio durante o movimento de rotação do braço na SI. Participaram do estudo 8 indivíduos com SI unilateral, e 8 indivíduos saudáveis, de ambos os sexos, constituindo 3 grupos: Grupo saúdavel (G1-S), Grupo com SI lado acometido (G2-LA) e Grupo com SI lado não acometido (G2-LNA). Este estudo comparou a atividade eletromiográfica dos músculos estabilizadores da escápula durante os movimentos de rotação interna (RI) e rotação externa (RE), por meio de parâmetros que quantificam a co-contração dos pares de músculos TA/TT, TA/TD, TA/SA, TT/TD, TT/SA, TD/SA, normalizados pela CIVM do movimento de RI e RE dos músculos trapézio ascendente (TA), trapézio transverso (TT), trapézio descendente (TD) e serrátil anterior (SA) entre os voluntários com SI unilateral grau I ou II e indivíduos assintomáticos. Os resultados encontrados para a co-contração dos pares de músculos TA/TT, TA/SA, TT/SA e TD/SA do grupo G2 – LA é maior que dos grupos G1 e G2 - LNA no movimento de RE. No movimento de RI não foi observada diferença que fosse decorrente da SI entre os pares musculares. Como os ombros acometidos pela SI apresentaram co-contração dos pares de músculos significativamente maior durante todo o movimento de RE, o exame da cintura escapular na prescrição de tratamento para SI parece ser aspecto importante para ser considerado, tanto na abordagem desses indivíduos quanto no estudo dos fatores etiológicos e de evolução da SI grau I ou II

Introdução à dinâmica de rotação clássica

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Satélites estabilizados por rotação e torque de radiação solar direta

The aims of this work are to analyze the direct solar radiation pressure torque (TPRS) in the rotational motion of spin-stabilized artificial satellites, to numerically implement these solutions and to compare the results with real data of the Brazilian Satellite Data Collection – SCD1 and SCD2, supplied by INPE. The mathematical model for this torque is determined for a cylindrical satellite, and the components of this torque are determined in a fixed system in the satellite. An analytical solution for the spin motion equations is proposed, in which TPRSD does not affect the spin velocity of the satellite. Two approaches are adopted in the numerical implementation of the developed theory: the first one considers the proposed theory and the second introduces a variation in the spin velocity based on its real variation. The results obtained indicate that the solar radiation pressure torque has little influence in the right ascension and declination axis of rotation due to the small dimension of the satellite and altitude in which it is found. To better validate the application of the presented theory, the angular deviation of the spin axis and solar aspect angle were also analyzed. The comparison of the results of the approaches conducted with real data show good precision in the theory, which can be applied in the prediction of the rotational motion of the spin-stabilized artificial satellites, when others external torques are considered besides the direct solar radiation pressure torque

Ecologia de cultivos: caracterização dos aspectos ecológicos dos diferentes cultivos no município de Cristais Paulistas-SP

Planning is an essential instrument for the agricultural occupation of the lands, because it supports the activities of food production and raw materials. It must be driven by techniques that provide the sustainability of these activities, so that also ensures the environmental balance of agroecosystems. Lands misuse can be considered as one of the causes of frustration of agricultural activities. Thus, the occurrence of discrepancies between the effective use (real use) of the land and its agricultural aptitude can compete, in many cases, to the decrease of productivity, as well as for soil degradation. In this way, this research intends to study the relationship between the temporary cultivations, halfperennial cultures, perennial and its developmental environment, determining the edaphoclimatic characteristics of landscapes. From then on, a letter shall be subject to the use and occupation of the soil for agriculture in the municipality of Cristais Paulista-SP, aiming to describe the spatial organization of land use and vegetation cover, and emphasizing management and conservative practices. For that, climatic factors were characterized, fundamentally humidity, temperature and luminosity; edaphics, including parental material, chemical and physical properties, fertility, soil temperature and climatic zoning; biotic, referring to the suitability of different cultures or to be implanted; physical, such as geomorphology, slope, geology, hypsometry and hydrology; socioeconomic, in particular production and marketing seasons; and the way they all, together, affect the adaptation, distribution and production of crops. Using this information, the zoning of the area of study was done based on the 21 nominated groups obtained, in addition to recommendations and suggestions for handling each type of cultivation... (Complete abstract click electronic access below)

Estudo do comportamento dos músculos estabilizadores da escápula durante exercícios de rotação do ombro

A função normal dos músculos escapulotorácicos é um dos componentes vitais para a estabilidade dinâmica do complexo do ombro. A maioria dos estudos aborda o controle dinâmico da escápula, porém o comportamento muscular no controle estático da mesma tem sido menos frequente. O objetivo do estudo foi analisar a ação simultânea dos músculos serrátil anterior e as três porções do trapézio durante o movimento de rotação interna e externa do ombro, entre voluntários assintomáticos. 10 indivíduos com idade entre 20 e 40 anos foram avaliados com testes de movimentos de rotação do ombro direito e esquerdo, contra uma resistência elástica (40% da CIVM), para captação de EMG por meio de eletrodos de superfície nos músculos: trapézio ascendente (TA), trapézio transverso (TT), trapézio descendente (TD) e serrátil anterior (SA). Foram obtidos valores de Contração Isométrica Voluntária Máxima (CIVM) para os músculos rotadores do ombro e TA, TT, TD e SA. Os sinais foram normalizados pela CIVM e processados no software Matlab, gerando curvas médias de ativação simultânea para cada par muscular (TA/TT; TA/TD; TA/SA; TT/TD; TT/SA; e TD/SA). A quantidade de cocontração dos pares musculares foi baixa (variação média de 2,3% a 11% da CIVM), e os pares em combinação com o SA tiveram tendência de maiores valores; a variabilidade encontrada foi baixa e a confiabilidade foi adequada (ICC > 0,70). Os baixos valores de co-contração encontrados neste estudo eram esperados, concordando com a biomecânica do movimento utilizado e com os estudos que avaliaram os mesmos músculos em outras condições; o movimento de RE apresentou co-contração levemente maior que a RI e isto sugere que a RE é um movimento mais instável, além de ser considerado o movimento mais fraco do ombro. Diante dos resultados encontrados, conclui-se que a metodologia utilizada foi... (Resumo completo, clicar acesso eletrônico abaixo)

Dinâmica de rotação de exoplanetas tipo terrestre com perturbação de terceiro corpo

In this work we study some topics of Celestial Mechanics, namely the problem of rigid body rotation and “spin-orbit” resonances. Emphasis is placed on the problem formulation and applications to some exoplanets with physical parameters (e.g. mass and radius) compatible with a terrestrial type constitution (e.g. rock) belonging to multiple planetary systems. The approach is both analytical and numerical. The analytical part consists of: i) the deduction of the equation of motion for the rotation problem of a spherical body with no symmetry, disturbed by a central body; ii) modeling the same problem by including a third-body in the planet-star system; iii) formulation of the concept of “spin-orbit” resonance in which the orbital period of the planet is an integer multiple of the rotation’s period. Topics of dynamical systems (e.g. equilibrium points, chaos, surface sections, etc.) will be included at this stage. In the numerical part simulations are performed with numerical models developed in the previous analytical section. As a first step we consider the orbit of the planet not perturbed by a third-body in the star-planet system. In this case the eccentricity and orbital semi-major axis of the planet are constants. Here the technique of surface sections, widely used in dynamical systems are applied. Next, we consider the action of a third body, developing a more realistic model for planetary rotation. The results in both cases are compared. Since the technique of disturbed surface sections is no longer applicable, we quantitatively evaluate the evolution of the characteristic angles of rotation (e.g. physical libration) by studying the evolution of individual orbits in the dynamically important regions of phase space, the latter obtained in the undisturbed case