Long-range correlations and trends in Colombian seismic time series

We study long-range correlations and trends in time series extracted from the data of seismic events occurred from 1973 to 2011 in a rectangular region that contains mainly all the continental part of Colombia. The long-range correlations are detected by the calculation of the Hurst exponents for the time series of interevent intervals, separation distances, depth differences and magnitude differences. By using a modification of the classical $R/S$ method that has been developed to detect short-range correlations in time series, we find the existence of persistence for all the time series considered except for magnitude differences. We find also, by using the $DFA$ until the third order, that the studied time series are not influenced by trends. Additionally, an analysis of the Hurst exponent as a function of the number of events in the time and the maximum window size is presented.Comment: 21 pages, 6 figures, 2 figures added, types corrected, accepted to be published in Physica

Um estudo de caso: produção e mercado do Pinus.

bitstream/CNPF-2009-09/30395/1/com_tec53.pd

Análise econômica de sistemas agroflorestais na Amazônia Ocidental, Machadinho D'Oeste - RO.

O objetivo deste estudo foi realizar a análise financeira e a simulação de risco de investimento em sistemas agroflorestais (SAFs) implantados em 1987, no Campo Experimental da Embrapa Rondônia, localizado no município de Machadinho d’Oeste, RO. A análise financeira foi realizada mediante os métodos de avaliação de projetos florestais, e para a análise de risco utilizou-se a técnica de simulação de Monte Carlo, mediante o programa @RISK. Entre os arranjos testados, o SAF T1 Castanha-do-brasil-banana-pimenta-do-reino-cupuaçu apresentou o melhor desempenho financeiro em relação aos SAFs T2 Freijó-banana-pimenta-do-reino-cupuaçu e T3 Pupunha-banana-pimenta-do-reino-cupuaçu. Os custos com tratos culturais e colheita representaram mais de 70% da composição dos custos totais, e a participação da mão-de-obra foi superior a 50% nas fases de preparo da área e de manutenção (tratos culturais) dos SAFs. A simulação da análise de risco indicou que as variáveis que afetaram o Valor Presente Líquido no Horizonte Infinito (VPL*), de acordo com a ordem de importância (R), foram: taxa de desconto, preço do fruto de cupuaçu (Theobroma grandiflorum), custo de colheita, preço da madeira de castanha-do-brasil (Bertholletia excelsa) e o custo de tratos culturais. Apesar do alto custo de implantação e manutenção, o SAF T1 apresentou uma probabilidade de 15% de os valores do Valor Presente Líquido (VPL) se concentrarem em torno de R$35.000 ha-1.ano-1

Levantamento alternativas agroflorestais para o Estado de Rondônia.

Tema Central: Sistemas Agroflorestais no Desenvolvimento Sustentável. v.2 Trabalhos voluntarios. Editores Luciano J. Montoya e Moacir J.S. Medrado

Cenário socioeconômico da produção de bracatinga na área norte da região metropolitana de Curitiba.

Palestra

CAFE: Calar Alto Fiber-fed Echelle spectrograph

We present here CAFE, the Calar Alto Fiber-fed Echelle spectrograph, a new instrument built at the Centro Astronomico Hispano Alem\'an (CAHA). CAFE is a single fiber, high-resolution ($R\sim$70000) spectrograph, covering the wavelength range between 3650-9800\AA. It was built on the basis of the common design for Echelle spectrographs. Its main aim is to measure radial velocities of stellar objects up to $V\sim$13-14 mag with a precision as good as a few tens of $m s^{-1}$. To achieve this goal the design was simplified at maximum, removing all possible movable components, the central wavelength is fixed, so the wavelentgth coverage; no filter wheel, one slit and so on, with a particular care taken in the thermal and mechanical stability. The instrument is fully operational and publically accessible at the 2.2m telescope of the Calar Alto Observatory. In this article we describe (i) the design, summarizing its manufacturing phase; (ii) characterize the main properties of the instrument; (iii) describe the reduction pipeline; and (iv) show the results from the first light and commissioning runs. The preliminar results indicate that the instrument fulfill the specifications and it can achieve the foreseen goals. In particular, they show that the instrument is more efficient than anticipated, reaching a $S/N\sim$20 for a stellar object as faint as $V\sim$14.5 mag in $\sim$2700s integration time. The instrument is a wonderful machine for exoplanetary research (by studying large samples of possible systems cotaining massive planets), galactic dynamics (high precise radial velocities in moving groups or stellar associations) or astrochemistry.Comment: 12 pages, 23 figures; Acepted for publishing in A&A, 201