Adubação nitrogenada em soja na implantação do sistema plantio direto

The vegetal residues maintenance on soil surface, characteristic of no-tillage system have changing the nutrients availability. So, in this sense, the aim of this work was to evaluate the effect of times of N application on corn sowed in no tillage system under vegetable residues of different species used for soil covering and straw supply in the cerrado area. The experiment was carried out in field conditions, in an Oxisol characteristic of this area. The treatments were constituted by the combination of different times of N application: (43+23+20+00); (00+70+20+00); (00+00+90+00); (00+00+20+70); (00+00+00+90) with an control treatment (absence of nitrogen), in kg ha(-1), respectively 30 days before the desiccation, at desiccation, at sowing and at sidedress of corn, sowed directly on Penisetum americanum and Brachiaria decumbens residues. By the results it can be concluded that nitrogen application in soybean, independent of time, does not increase productivity in relation to the treatment without nitrogen application.

Institucionalização da publicidade registral imobiliária no ordenamento jurídico brasileiro

Pós-graduação em Direito - FCHS

Metaheurísticas em um problema de rotação de culturas

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

Chiquinha Gonzaga e o Maxixe

Pós-graduação em Música - IA

Avaliação sazonal dos efeitos do enriquecimento por N e P sobre o perifíton em represa tropical rasa mesotrófica (Lago das Ninféias, São Paulo)

Pós-graduação em Ciências Biológicas (Biologia Vegetal) - IBRC

Literatura, ensino e educação liberal

Pós-graduação em Letras - FCLAS

Analisando a possibilidade de um anel ao redor de um satélite

On November 26 th, 2005, Rhea, one of Saturn's moons, is found by Cassini spacecraft approximately at 5.105 km from Saturn. Observations in situ reveal that electrons are depleted in the moon's vicinity. However, Rhea is considered massive enough to retain a thin atmosphere. Assumption was that the atmosphere of Rhea was not composed exclusively of gas, its likely contains solid material that can absorb magnetospheric particles. According to Jones et al. (2008), these particles were in a speci c position so that at the moment of observation the electrons could not be detected. In opposition to this idea there is a group, Tiscareno et al. 2010, Cornell University Library, that underwent intensive search for any material that might be orbiting Rhea using Cassini images, however the could not identify any. Second recommendation made by American researchers and other countries, and accepted by the National Board of Research the Cassini Equinox Mission will continue in orbit around Saturn until 2016.The probe will perform several maneuvers with high inclination to delve into the main ring system, and then enter in Saturn's atmosphere and collide with planet. This research is of great importance because until today no rings were found orbiting satellites. The goal of this work is to analyze the orbital evolution of a set of particles around Rhea disturbance of Saturn, J2 e J4 and check results by the numerical simulations and the possibility of a stable ring orbiting Rhea.