Barragem subterrânea: água para uso na agricultura.

Introdução; Considerações gerais e recomendações técnicas; Benefícios e cuidados no uso da tecnologia.bitstream/item/17368/1/Barbosa.pd

Personalised trails and learner profiling within e-learning environments

This deliverable focuses on personalisation and personalised trails. We begin by introducing and defining the concepts of personalisation and personalised trails. Personalisation requires that a user profile be stored, and so we assess currently available standard profile schemas and discuss the requirements for a profile to support personalised learning. We then review techniques for providing personalisation and some systems that implement these techniques, and discuss some of the issues around evaluating personalisation systems. We look especially at the use of learning and cognitive styles to support personalised learning, and also consider personalisation in the field of mobile learning, which has a slightly different take on the subject, and in commercially available systems, where personalisation support is found to currently be only at quite a low level. We conclude with a summary of the lessons to be learned from our review of personalisation and personalised trails

Relações entre medidas da produção de leite nas raças Canchim e Nelore.

Relação da produção de leite pela manha/produção de leite durante todo o dia (RMD) e correlação entre produções de leite parciais e produção total em 210 dias de lactação (L200), nas raças Canchim (Ca) e Nelore (Ne); Os resultados sugerem que três medidas mensais estimam razoavelmente bem a produção de leite durante toda a lactação em gado de corte

Quantifying the Drivers of Star Formation on Galactic Scales. I. The Small Magellanic Cloud

We use the star formation history of the Small Magellanic Cloud (SMC) to place quantitative limits on the effect of tidal interactions and gas infall on the star formation and chemical enrichment history of the SMC. The coincident timing of two recent (< 4 Gyr) increases in the star formation rate and SMC/Milky Way(MW) pericenter passages suggests that global star formation in the SMC is driven at least in part by tidal forces due to the MW. The Large Magellanic Cloud (LMC) is the other potential driver of star formation, but is only near the SMC during the most recent burst. The poorly constrained LMC-SMC orbit is our principal uncertainty. To explore the correspondence between bursts and MW pericenter passages further, we model star formation in the SMC using a combination of continuous and tidally-triggered star formation. The behavior of the tidally-triggered mode is a strong inverse function of the SMC-MW separation (preferred behavior ~ r^-5, resulting in a factor of ~100 difference in the rate of tidally-triggered star formation at pericenter and apocenter). Despite the success of these closed-box evolutionary models in reproducing the recent SMC star formation history and current chemical abundance, they have some systematic shortcomings that are remedied by postulating that a sizable infall event (~ 50% of the total gas mass) occured about 4 Gyr ago. Regardless of whether this infall event is included, the fraction of stars in the SMC that formed via a tidally triggered mode is > 10% and could be as large as 70%.Comment: Accepted for publication in Ap

Qualidade do solo em áreas de plantio convencional sob latossolos do cerrado.

O cultivo convencional envolve o revolvimento e pulverização do solo, aplicação de corretivos e fertilizantes e exposição das partículas de solo. Este cultivo pode alterar a estrutura do solo, o que reflete no índice de qualidade do solo. Assim, o objetivo do presente estudo foi estabelecer índices que expressam a qualidade do solo em áreas de manejo com cultivo convencional em Latossolos sob Cerrado, através da avaliação de atributos físicos e químicos dos solos