Suspensão da irrigação durante a maturação de uvas 'Niágara Rosada'.

Na região noroeste de São Paulo, a videira Niágara Rosada (Vitis labrusca) tem sido uma das principais cultivares adotadas pelos produtores locais. Todas as áreas vitícolas, nessa região, são irrigadas devido ao déficit hídrico que ocorre durante o período de produção da cultura. Diversas técnicas podem ser empregadas com o propósito de aumentar a eficiência do uso da água, sendo que a irrigação com déficit hídrico tem sido uma das mais adotadas para a cultura da videira. No presente trabalho, avaliou-se o efeito de diferentes épocas de suspensão da irrigação durante a fase de maturação de uvas da cultivar ?Niágara Rosada? (Vitis labrusca), sob as condições do noroeste paulista. O experimento foi conduzido em área da Estação Experimental de Viticultura Tropical da Embrapa Uva e Vinho, localizada no município de Jales, noroeste do estado de São Paulo. As plantas de ?Niágara Rosada? sobre porta-enxertos ?IAC 572? foram conduzidas no sistema latada e irrigadas por microaspersão. O delineamento estatístico foi em blocos ao acaso com quatro tratamentos e cinco repetições. Os tratamentos avaliados foram: suspensão da irrigação aos 21 dias (T1), 15 dias (T2) e 9 dias (T3) antes da colheita, e irrigação até o final do ciclo da cultura (T4). Foram avaliadas variáveis relacionadas à qualidade dos frutos, como teor de sólidos solúveis, pH, tamanho de bagas e massa de cachos e bagas. Durante o período de avaliação, não ocorreram precipitações pluviais no local do experimento. Não foram encontradas diferenças significativas pelo teste de Tukey, ao nível de 5% de probabilidade, para as variáveis avaliadas. A suspensão da irrigação aos 21 dias (T1) apresentou uma economia de água de 21% em relação ao total aplicado no tratamento sem suspensão da irrigação (T4)

Efeito da suspensão da irrigação sobre a incidência de requeima na cultivar de videira Niágara Rosada.

O objetivo deste trabalho é avaliar o efeito da suspensão da irrigação, em diferentes épocas da maturação dos frutos, sobre a ocorrência da requeima das folhas da videira 'Niágara Rosada'

A CST simulation and performance analysis for a passive façade integratable metamaterials structure

In the case of stone relics with cultural heritage value that are exposed to the adverse effects of direct exposure to weathering, we present a metamaterial with a composite structure that can passively control the transmittance of infrared and visible light. This periodic multi-layer structure consist of metal and dielectric layers, these have the function of low transmittance at infrared wavelengths and high transmittance in visible light. Its spectrally-selective behavior offers the possibility of both temperature regulation and natural daylighting of cultural relics. In addition, it can be discretely integrated with an existing architectural façade to provide weathering protection against rain and snow. Results show the composite structure can not only obtain a band gap width of 109 THz in the near infrared wave-band but also ensure that most of the visible light's transmittance is higher than τ=0.4. Furthermore, since the transmission spectrum is independent of polarization angle, the cultural relics benefit from its spectral-selective properties regardless of the polarization angle due to the sun's position

Frequência de aplicação de fungicidas para o controle de míldio na cultivar de uva sem semente BRS Vitória.

XV Congresso Latino-Americano de Viticultura e Enologia E XIII Congresso Brasileiro de Viticultura e Enologia. Bento Gonçalves-RS, 3 a 7 de Novembro de 2015

Planck pre-launch status: HFI beam expectations from the optical optimisation of the focal plane

Planck is a European Space Agency (ESA) satellite, launched in May 2009, which will map the cosmic microwave background anisotropies in intensity and polarisation with unprecedented detail and sensitivity. It will also provide full-sky maps of astrophysical foregrounds. An accurate knowledge of the telescope beam patterns is an essential element for a correct analysis of the acquired astrophysical data. We present a detailed description of the optical design of the High Frequency Instrument (HFI) together with some of the optical performances measured during the calibration campaigns. We report on the evolution of the knowledge of the pre-launch HFI beam patterns when coupled to ideal telescope elements, and on their significance for the HFI data analysis procedure

Black hole accretion and star formation as drivers of gas excitation and chemistry in Mrk231

We present a full high resolution SPIRE FTS spectrum of the nearby ultraluminous infrared galaxy Mrk231. In total 25 lines are detected, including CO J=5-4 through J=13-12, 7 rotational lines of H2O, 3 of OH+ and one line each of H2O+, CH+, and HF. We find that the excitation of the CO rotational levels up to J=8 can be accounted for by UV radiation from star formation. However, the approximately flat luminosity distribution of the CO lines over the rotational ladder above J=8 requires the presence of a separate source of excitation for the highest CO lines. We explore X-ray heating by the accreting supermassive black hole in Mrk231 as a source of excitation for these lines, and find that it can reproduce the observed luminosities. We also consider a model with dense gas in a strong UV radiation field to produce the highest CO lines, but find that this model strongly overpredicts the hot dust mass in Mrk231. Our favoured model consists of a star forming disk of radius 560 pc, containing clumps of dense gas exposed to strong UV radiation, dominating the emission of CO lines up to J=8. X-rays from the accreting supermassive black hole in Mrk231 dominate the excitation and chemistry of the inner disk out to a radius of 160 pc, consistent with the X-ray power of the AGN in Mrk231. The extraordinary luminosity of the OH+ and H2O+ lines reveals the signature of X-ray driven excitation and chemistry in this region.Comment: 5 pages, 2 figures, accepted for publication in Astronomy & Astrophysics Special Issue on Herschel first result

Herschel observations of water vapour in Markarian 231

The Ultra Luminous InfraRed Galaxy Mrk 231 reveals up to seven rotational lines of water (H2O) in emission, including a very high-lying (E_{upper}=640 K) line detected at a 4sigma level, within the Herschel/SPIRE wavelength range, whereas PACS observations show one H2O line at 78 microns in absorption, as found for other H2O lines previously detected by ISO. The absorption/emission dichotomy is caused by the pumping of the rotational levels by far-infrared radiation emitted by dust, and subsequent relaxation through lines at longer wavelengths, which allows us to estimate both the column density of H2O and the general characteristics of the underlying far-infrared continuum source. Radiative transfer models including excitation through both absorption of far-infrared radiation emitted by dust and collisions are used to calculate the equilibrium level populations of H2O and the corresponding line fluxes. The highest-lying H2O lines detected in emission, with levels at 300-640 K above the ground state, indicate that the source of far-infrared radiation responsible for the pumping is compact (radius=110-180 pc) and warm (T_{dust}=85-95 K), accounting for at least 45% of the bolometric luminosity. The high column density, N(H2O)~5x10^{17} cm^{-2}, found in this nuclear component, is most probably the consequence of shocks/cosmic rays, an XDR chemistry, and/or an "undepleted chemistry" where grain mantles are evaporated. A more extended region, presumably the inner region of the 1-kpc disk observed in other molecular species, could contribute to the flux observed in low-lying H2O lines through dense hot cores, and/or shocks. The H2O 78 micron line observed with PACS shows hints of a blue-shifted wing seen in absorption, possibly indicating the occurrence of H2O in the prominent outflow detected in OH (Fischer et al., this volume).Comment: 5 pages, 3 figure