Post-receptor IGF1 insensitivity restricted to the MAPK pathway in a Silver-Russell syndrome patient with hypomethylation at the imprinting control region on chromosome 11

Background: Hypomethylation of the paternal imprinting center region 1 (ICR1) is the most frequent molecular cause of Silver-Russell syndrome (SRS). Clinical evidence suggests that patients with this epimutation have mild IGF1 insensitivity. Objective: To assess in vitro IGF1 action in fibroblast culture from a patient with SRS and IGF1 insensitivity. Methods: Fibroblast cultures from one patient with SRS due to ICR1 demethylation and controls were established. The SRS patient has severe growth failure, elevated IGF1 level, and poor growth rate during human recombinant GH treatment. IGF1 action was assessed by cell proliferation, AKT, and p42/44-MAPK phosphorylation. Gene expression was determined by real-time PCR. Results: Despite normal IGF1R sequence and expression, fibroblast proliferation induced by IGF1 was 50% lower in SRS fibroblasts in comparison with controls. IGF1 and insulin promoted a p42/44-MAPK activation in SRS fibroblasts 40 and 36%, respectively, lower than that in control fibroblasts. On the other hand, p42/44-MAPK activation induced by EGF stimulation was only slightly reduced (75% in SRS fibroblasts in comparison with control), suggesting a general impairment in MAPK pathway with a greater impairment of the stimulation induced by insulin and IGF1 than by EGF. A PCR array analysis disclosed a defect in MAPK pathway characterized by an increase in DUSP4 and MEF2C gene expressions in patient fibroblasts. Conclusion: A post-receptor IGF1 insensitivity was characterized in one patient with SRS and ICR1 hypomethylation. Although based on one unique severely affected patient, these results raise an intriguing mechanism to explain the postnatal growth impairment observed in SRS patients that needs confirmation in larger cohorts.

Gamma-ray and neutrino fluxes from Heavy Dark Matter in the Galactic Center

We present a study of the Galactic Center region as a possible source of both secondary gamma-ray and neutrino fluxes from annihilating dark matter. We have studied the gamma-ray flux observed by the High Energy Stereoscopic System (HESS) from the J1745-290 Galactic Center source. The data are well fitted as annihilating dark matter in combination with an astrophysical background. The analysis was performed by means of simulated gamma spectra produced by Monte Carlo event generators packages. We analyze the differences in the spectra obtained by the various Monte Carlo codes developed so far in particle physics. We show that, within some uncertainty, the HESS data can be fitted as a signal from a heavy dark matter density distribution peaked at the Galactic Center, with a power-law for the background with a spectral index which is compatible with the Fermi-Large Area Telescope (LAT) data from the same region. If this kind of dark matter distribution generates the gamma-ray flux observed by HESS, we also expect to observe a neutrino flux. We show prospective results for the observation of secondary neutrinos with the Astronomy with a Neutrino Telescope and Abyss environmental RESearch project (ANTARES), Ice Cube Neutrino Observatory (Ice Cube) and the Cubic Kilometer Neutrino Telescope (KM3NeT). Prospects solely depend on the device resolution angle when its effective area and the minimum energy threshold are fixed.

Near-infrared polarimetry in the galactic center. On properties of Sagittarius A* and a dusty S-cluster object

Near-infrared polarimetry observation is a powerful tool to study the central sources at the center of the Milky Way. My aim of this thesis is to analyze the polarized emission present in the central few light years of the Galactic Center region, in particular the non-thermal polarized emission of Sagittarius~A* (Sgr~A*), the electromagnetic manifestation of the super-massive black hole, and the polarized emission of an infrared-excess source in the literature referred to as DSO/G2. This source is in orbit about Sgr~A*. In this thesis I focus onto the Galactic Center observations at $\lambda=2.2~\mu m$ ($K_\mathrm{s}$-band) in polarimetry mode during several epochs from 2004 to 2012. The near-infrared polarized observations have been carried out using the adaptive optics instrument NAOS/CONICA and Wollaston prism at the Very Large Telescope of ESO (European Southern Observatory). Linear polarization at 2.2 $\mu m$, its flux statistics and time variation, can be used to constrain the physical conditions of the accretion process onto the central super-massive black hole. I present a statistical analysis of polarized $K_\mathrm{s}$-band emission from Sgr~A* and investigate the most comprehensive sample of near-infrared polarimetric light curves of this source up to now. I find several polarized flux excursions during the years and obtain an exponent of about 4 for the power-law fitted to polarized flux density distribution of fluxes above 5~mJy. Therefore, this distribution is closely linked to the single state power-law distribution of the total $K_\mathrm{s}$-band flux densities reported earlier by us. I find polarization degrees of the order of 20\%$\pm$10\% and a preferred polarization angle of $13^o\pm15^o$. Based on simulations of polarimetric measurements given the observed flux density and its uncertainty in orthogonal polarimetry channels, I find that the uncertainties of polarization parameters under a total flux density of $\sim 2\,{\mathrm{mJy}}$ are probably dominated by observational uncertainties. At higher flux densities there are intrinsic variations of polarization degree and angle within rather well constrained ranges. Since the emission is most likely due to optically thin synchrotron radiation, the obtained preferred polarization angle is very likely reflecting the intrinsic orientation of the Sgr~A* system i.e. an accretion disk or jet/wind scenario coupled to the super-massive black hole. Our polarization statistics show that Sgr~A* must be a stable system, both in terms of geometry, and the accretion process. I also investigate an infrared-excess source called G2 or Dusty S-cluster Object (DSO) moving on a highly eccentric orbit around the Galaxy's central black hole, Sgr~A*. I use for the first time the near-infrared polarimetric imaging data to determine the nature and the properties of DSO and obtain an improved $K_\mathrm{s}$-band identification of this source in median polarimetry images of different observing years. The source starts to deviate from the stellar confusion in 2008 data and it does not show a flux density variability based on our data set. Furthermore, I measure the polarization degree and angle of this source and conclude based on the simulations on polarization parameters that it is an intrinsically polarized source with a varying polarization angle as it approaches Sgr~A* position. I use the interpretation of the DSO polarimetry measurements to assess its possible properties.

Multiwavelength observations of the black hole candidate 1E 1740.7-2942

Observations of the Galactic center region black hole candidate 1E 1740.7-2942 have been carried out using the Caltech Gamma-Ray Imaging Payload (GRIP), the Röntgensatellit (ROSAT) and the Very Large Array (VLA). These multiwavelength observations have helped to establish the association between a bright emitter of hard X-rays and soft γ-rays, the compact core of a double radio jet source, and the X-ray source, 1E 1740.7-2942. They have also provided information on the X-ray and hard X-ray spectrum.

The Galactic center region was observed by GRIP during balloon flights from Alice Springs, NT, Australia on 1988 April 12 and 1989 April 3. These observations revealed that 1E 1740.7-2942 was the strongest source of hard X-rays within ~10° of the Galactic center. The source spectrum from each flight is well fit by a single power law in the energy range 35-200 keV. The best-fit photon indices and 100 keV normalizations are: γ = (2.05 ± 0.15) and K_(100) = (8.5 ± 0.5) x 10^(-5) cm^(-2) s^(-1) keV^(-1) and γ = (2.2 ± 0.3) and K_(100) = (7.0 ± 0.7) x 10^(-5) cm^(-2) s^(-1) keV^(-1) for the 1988 and 1989 observations respectively. No flux above 200 keV was detected during either observation. These values are consistent with a constant spectrum and indicate that 1E 1740.7-2942 was in its normal hard X-ray emission state. A search on one hour time scales showed no evidence for variability.

The ROSAT HRI observed 1E 1740.7-2942 during the period 1991 March 20-24. An improved source location has been derived from this observation. The best fit coordinates (J2000) are: Right Ascension = 17^h43^m54^s.9, Declination = -29°44'45".3, with a 90% confidence error circle of radius 8".5. The PSPC observation was split between periods from 1992 September 28- October 4 and 1993 March 23-28. A thermal bremsstrahlung model fit to the data yields a column density of N_H = 1.12^(+1.51)_(0.18) x cm^(-2) , consistent with earlier X- ray measurements.

We observed the region of the Einstein IPC error circle for 1E 1740.7-2942 with the VLA at 1.5 and 4.9 GHz on 1989 March 2. The 4.9 GHz observation revealed two sources. Source 'A', which is the core of a double aligned radio jet source (Mirabel et al. 1992), lies within our ROSAT error circle, further strengthening its identification with 1E 1740.7-2942.

Variation in trawl geometry due to unequal warp length

Survey standardization procedures can reduce the variability in trawl catch efficiency thus producing more precise estimates of biomass. One such procedure, towing with equal amounts of trawl warp on both sides of the net, was experimentally investigated for its importance in determining optimal trawl geometry and for evaluating the effectiveness of the recent National Oceanic and Atmospheric Administration (NOAA) national protocol on accurate measurement of trawl warps. This recent standard for measuring warp length requires that the difference between warp lengths can be no more than 4% of the distance between the otter doors measured along the bridles and footrope. Trawl performance data from repetitive towing with warp differentials of 0, 3, 5, 7, 9, 11, and 20 m were analyzed for their effect on three determinants of flatfish catch efficiency: footrope distance off-bottom, bridle length in contact with the bottom, and area swept by the net. Our results indicated that the distortion of the trawl caused by asymmetry in trawl warp length could have a negative inf luence on flatfish catch efficiency. At a difference of 7 m in warp length, the NOAA 4% threshold value for the 83112 Eastern survey trawl used in our study, we found no effect on the acous-tic-based measures of door spread, wing spread, and headrope height off-bottom. However, the sensitivity of the trawl to 7 m of warp offset could be seen as footrope distances off-bottom increased slightly (particularly in the center region of the net where flatfish escapement is highest), and as the width of the bridle path responsible for flatfish herding, together with the effective net width, was reduced. For this survey trawl, a NOAA threshold value of 4% should be considered a maximum. A more conservative value (less than 4%) would likely reduce potential bias in estimates of relative abundance caused by large differences in warp length approaching 7 m.

Symmetry analysis and numerical simulation of mode characteristics for equilateral-polygonal optical microresonators

Mode characteristics for two-dimensional equilateral-polygonal microresonators are investigated based on symmetry analysis and finite-difference time-domain numerical simulation. The symmetries of the resonators can be described by the point group C-Nv, accordingly, the confined modes in these resonators can be classified into irreducible representations of the point group C-Nv. Compared with circular resonators, the modes in equilateral-polygonal resonators have different characteristics due to the break of symmetries, such as the split of double-degenerate modes, high field intensity in the center region, and anomalous traveling-wave modes, which should be considered in the designs of the polygonal resonator microlasers or optical add-drop filters.

GIANT LOBES OF CENTAURUS A RADIO GALAXY OBSERVED WITH THE SUZAKU X-RAY SATELLITE

We report on Suzaku observations of selected regions within the southern giant lobe of the radio galaxy Centaurus A. In our analysis we focus on distinct X-ray features detected with the X-ray Imaging Spectrometer within the range 0.5-10 keV, some of which are likely associated with fine structure of the lobe revealed by recent high-quality radio intensity and polarization maps. With the available photon statistics, we find that the spectral properties of the detected X-ray features are equally consistent with thermal emission from hot gas with temperatures kT > 1 keV, or with a power-law radiation continuum characterized by photon indices Gamma similar to 2.0 +/- 0.5. However, the plasma parameters implied by these different models favor a synchrotron origin for the analyzed X-ray spots, indicating that a very efficient acceleration of electrons up to greater than or similar to 10 TeV energies is taking place within the giant structure of Centaurus A, albeit only in isolated and compact regions associated with extended and highly polarized radio filaments. We also present a detailed analysis of the diffuse X-ray emission filling the whole field of view of the instrument, resulting in a tentative detection of a soft excess component best fitted by a thermal model with a temperature of kT similar to 0.5 keV. The exact origin of the observed excess remains uncertain, although energetic considerations point to thermal gas filling the bulk of the volume of the lobe and mixed with the non-thermal plasma, rather than to the alternative scenario involving a condensation of the hot intergalactic medium around the edges of the expanding radio structure. If correct, this would be the first detection of the thermal content of the extended lobes of a radio galaxy in X-rays. The corresponding number density of the thermal gas in such a case is n(g) similar to 10(-4) cm(-3), while its pressure appears to be in almost exact equipartition with the volume-averaged non-thermal pressure provided by the radio-emitting electrons and the lobes' magnetic field. A prominent large-scale fluctuation of the Galactic foreground emission, resulting in excess foreground X-ray emission aligned with the lobe, cannot be ruled out. Although tentative, our findings potentially imply that the structure of the extended lobes in active galaxies is likely to be highly inhomogeneous and non-uniform, with magnetic reconnection and turbulent acceleration processes continuously converting magnetic energy to internal energy of the plasma particles, leading to possibly significant spatial and temporal variations in the plasma beta parameter around the volume-averaged equilibrium condition beta similar to 1.

Matérias-primas da plataforma do Mondego para cerâmica

O presente trabalho divulga os resultados dos estudos levados a efeito nas matérias-primas argilosas que se integram tipologicamente na argila comum, ocorrentes na designada Plataforma do Mondego, Centro de Portugal, na região entre Miranda do Corvo, a SW, e Tábua, a NE. Para tal realizou-se a cartografia superficial dos sedimentos continentais do Cretácico e do Terciário, aí preservados, estabeleceram-se as colunas sedimentares, a nível regional e a nível local, nas áreas de maior potencial reconhecido e, caracterizaram-se as matérias-primas argilosas amostradas, em termos de composição, textura e aptidão cerâmica, objectivando a definição das zonas das jazidas com maior interesse industrial. A informação obtida e compilada, relativa ao caulino e ao feldspato é também apresentada, com vista a uma percepção da potencialidade destas matériasprimas cerâmicas ocorrentes na área. O estudo de caracterização dos materiais argilosos investigados teve como base 53 amostras obtidas em seis regiões da Plataforma do Mondego aqui definidas por motivo de organização do trabalho, segundo os critérios geográfico e geotectónico. As formações de Côja e de Campelo, do Terciário, constituem as unidades onde ocorrem litótipos produtivos, em termos de matéria-prima para a Cerâmica de Barro Vermelho ou Cerâmica de Construção. Relativamente às características texturais e composicionais, em síntese, apresentam-se os factos relevantes seguintes: A matéria-prima argilosa existente na área estudada materializa, granulometricamente, na maioria das amostras, silte, caindo os níveis amostrados com maior percentagem de argila, no domínio do silte argiloso. O défice em fracção argila implica limitações quanto à possibilidade de diversificação de produtos cerâmicos fabricados com estas matérias-primas tal-qual. Os diferentes métodos analíticos utilizados na caracterização mineralógica dos materiais amostrados confirmaram uma composição em termos dos minerais argilosos, consistindo de ilite/mica (em geral, o mais abundante), caulinite e esmectite, interestratificados e clorite. Os minerais não argilosos são quartzo (predominante), feldspato (sobretudo potássico) e hematite, com uma representação baixa. A mineralogia da fracção inferior a 2μm das amostras, não difere das amostras totais, salvo no teor mais elevado dos minerais argilosos e acentuada redução dos minerais não argilosos. Os resultados da análise química por fluorescência de raios X das amostras integrais correlacionam-se com as características mineralógicas observadas através das técnicas analíticas utilizadas. No respeitante às propriedades e comportamento cerâmico verifica-se: Os parâmetros relacionados com a plasticidade indicam que parte das pastas elaboradas com estes materiais argilosos têm uma trabalhabilidade aceitável, mas existem problemas de conformação e acentuada retracção num número significativo de amostras, devido à elevada plasticidade da maioria das amostras. A extrusão é satisfatória a óptima. A RMF e a retracção em seco assumem valores, respectivamente, moderados a baixos e moderados, embora seja necessário ter em conta o procedimento de extrusão dos provetes, sem dispositivo de vácuo. Todas as amostras foram sujeitas a cozedura a 900ºC, e um conjunto seleccionado foi cozido a 1000ºC e a 1100ºC. As fases mineralógicas ocorrentes após cozeduras a 900ºC e 1100ºC foram identificadas num conjunto de amostras, tendo-se evidenciado a coerência dessas fases, com a mineralogia das amostras em seco. Após cozedura a 900ºC, os valores de RMF das amostras satisfazem geralmente os valores mínimos, exigidos para o fabrico de tijolo, abobadilha e, com alguma frequência, de telha, como já se verificava com os valores daquela propriedade em seco. Os valores de retracção seco-cozido são em geral, modestos. A capacidade de absorção de água é maioritariamente elevada. A formação de vidro, sobretudo, condiciona o comportamento destas propriedades por cozedura dos provetes a 1000ºC e a 1100ºC. A coloração predominante em cru das matérias-primas argilosas amostradas é amarelo acastanhado a castanho avermelhado. Após cozedura a 900ºC, há um acentuado escurecimento e incremento no grau de vermelho. As cozeduras a 1000ºC e 1100ºC promovem escurecimento gradual, com ligeira influência na cor. O comportamento dos provetes após as cozeduras cerâmicas revelou-se homogéneo a cada uma das respectivas temperaturas, não se registando também defeitos significativos, nem eflorescências. A análise das amostras em termos composicionais e tecnológicos permitiu destacar as principais características e aspectos distintivos das matériasprimas, nas diferentes regiões definidas objectivando as diferentes potencialidades cerâmicas. Nesta abordagem comparativa foram consideradas só as amostras dos campos silte e silte arenoso, por serem aquelas com maior interesse para a Cerâmica de Construção. Nas colunas sedimentares das regiões de Tábua e Santa Quitéria constata-se a ocorrência de dois ritmos de sedimentação, que embora assumam características específicas em cada região, têm aspectos composicionais e tecnológicos em comum, traduzindo melhor aptidão cerâmica os ritmos inferiores. A conjugação da cartografia realizada com os estudos laboratoriais permite concluir que as regiões de Tábua e de Santa Quitéria serão as que têm maior potencial por explorar, em matéria-prima para Cerâmica de Construção, apesar da primeira já ser intensamente explorada. Na região de Tábua, as amostras têm como fases mineralógicas principais ilite e quartzo na mesma proporção média (35%) e caulinite (média=19%) que regista enriquecimento significativo na fracção argila (média=38%). As argilas desta região registam a cor em cru mais vermelha e pH mais ácido observados. O ritmo de sedimentação inferior, com esmectite e interestratificados e ligeiramente menos quartzoso, apresenta melhores propriedades cerâmicas. A composição mineralógica média das amostras da região de Santa Quitéria é próxima daquela da região de Tábua, mas menos caulinítica, em especial na sequência inferior, na qual o teor médio de caulinite na fracção argila (7%) é o mais baixo observado. Na região de Côja – Arganil, a actividade extractiva é significativa na bacia de Côja. Aqui, a exploração de novas áreas potenciais é condicionada pela cobertura conglomerática e por estruturas tectónicas e não tectónicas relacionadas com comportamento plástico. Na restante área desta região, os recursos argilosos são penalizados por material areno-conglomerático. As amostras desta região distinguem-se das restantes a nível textural pela maior fracção areia e mineralogicamente pela presença de clorite, teor reduzido de caulinite e elevado de feldspato. As potencialidades em barro vermelho na região de Sanguinheda não serão significativas, pois a Formação de Côja é predominantemente arcósica e a Formação de Campelo pouco espessa e conglomerática. As argilas com melhor aptidão cerâmica foram amostradas na região de Miranda do Corvo – Lousã. Na composição, estas amostras são as que contêm maior fracção de argila, maior teor de ilite e caulinite e menor de argilas expansivas. Registam os melhores valores nas características tecnológicas, nomeadamente a RMF e absorção de água. A consistência dos grupos amostrais e ritmos definidos em termos composicionais e tecnológicos é corroborada pelas técnicas de análise estatística multivariada aplicadas, que os identificam. As condições de amostragem na região de Tábua, permitiram a elaboração de uma coluna tipológica, na qual, a partir de uma caracterização expedita de amostras é possível identificar a sua afinidade com os ritmos argilosos definidos e, consequentemente, a sua situação na coluna sedimentar regional e aptidão cerâmica. A cartografia dos recursos argilosos potenciais, elaborada à escala 1:25.000, constitui um dos objectivos principais deste trabalho e nela constam unidades litológicas, nas quais são diferenciadas unidades argilosas tendo também em consideração a tipologia e guias mineralógicos resultantes da caracterização das amostras. As características composicionais destas unidades denotam diferente aptidão cerâmica e, portanto, permitem salientar as zonas com maior interesse económico.

MRT letter: Extended depth from focus reconstruction method for stretch zone measurement in 15-5PH steel

The stretch zone width (SZW) data for 15-5PH steel CTOD specimens fractured at -150 degrees C to + 23 degrees C temperature were measured based on focused images and 3D maps obtained by extended depth-of-field reconstruction from light microscopy (LM) image stacks. This LM-based method, with a larger lateral resolution, seems to be as effective for quantitative analysis of SZW as scanning electron microscopy (SEM) or confocal scanning laser microscopy (CSLM), permitting to clearly identify stretch zone boundaries. Despite the worst sharpness of focused images, a robust linear correlation was established to fracture toughness (KC) and SZW data for the 15-5PH steel tested specimens, measured at their center region. The method is an alternative to evaluate the boundaries of stretched zones, at a lower cost of implementation and training, since topographic data from elevation maps can be associated with reconstructed image, which summarizes the original contrast and brightness information. Finally, the extended depth-of-field method is presented here as a valuable tool for failure analysis, as a cheaper alternative to investigate rough surfaces or fracture, compared to scanning electron or confocal light microscopes. Microsc. Res. Tech. 75:11551158, 2012. (C) 2012 Wiley Periodicals, Inc.

Vulnerabilidade natural à poluição dos recursos hídricos subterrâneos da área de Araraquara (SP)

Pós-graduação em Geociências e Meio Ambiente - IGCE

Estudo hidrogeológico do aqüífero Tubarão na área de afloramento da porção central do Estado de São Paulo

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Avaliação da estabilidade de tensão do sistema brasileiro: um caso de estudo

Este artigo apresenta resultados de um estudo da atual condição de operação do sistema interligado brasileiro com relação à estabilidade de tensão. As análises são realizadas a partir de dados reais do planejamento e da operação. O sistema é dividido em 4 regiões: Norte, Nordeste, Sul e Sudeste/Centro-Oeste. A margem de estabilidade é obtida para cada uma destas regiões. Os resultados mostram que o sistema interligado brasileiro apresenta margem de estabilidade muito abaixo da sugerida pelos critérios existentes, a qual é limitada pela região Sudeste/Centro-Oeste. Uma análise detalhada para esta área crítica do sistema é realizada. Além de uma avaliação do comportamento da margem de estabilidade de tensão durante um dia típico de semana, esta trabalho apresenta uma análise de contingências. Utilizando a metodologia de análise modal verifica-se a abrangência das contingências, mensurando o impacto de cada contingência como local, de área ou sistêmico.

Integração de informações geológicas para o geoturismo na Bacia do Rio Corumbataí e sua divulgação na Web através do Mapserver

A bacia hidrográfica do Rio Corumbataí, no setor centro oriental do Estado de São Paulo, está inteiramente contida no domínio morfológico da Depressão Periférica Paulista. Nos limites norte, noroeste e oeste, as escarpas arenito-basálticas, as cuestas de derrames basálticos e o Planalto Ocidental Paulista contribuem para a existência de diversas paisagens de beleza cênica. A diversidade geológica da região condiciona parcialmente o seu relevo e guarda registros litológicos e paleontológicos que constituem atrativos geoturísticos. O avanço do conhecimento geocientífico obtido principalmente nas universidades pouco alcança o público em geral devido à especialização dos termos utilizados. Aproveitando a aptidão turística e a diversidade geológica da região propõe-se utilizar o geoturismo como um meio de difusão de conhecimento científico e aumentar o interesse da população para suas riquezas naturais. Para tanto, foram selecionados 16 locais representativos da geologia da área que podem ser utilizados para a prática do geoturismo, sobre os quais foram elaborados textos explicativos em linguagem simplificada. Os textos foram associados a fotografias de afloramentos, figuras e mapas geológicos em um ambiente SIG. Para permitir o amplo e fácil acesso ao público, inclusive de estudantes, órgãos públicos e empresas ligadas ao ramo do turismo, todo este material foi disponibilizado na Internet através da ferramenta Mapserver e Maplab.

Effects of irrigation and time of application on the yield and quality of cv. Cabernet sauvignon in a warm climate

Mediterranean climate is characterized by hot summer, high evapotranspiration rates, and scarce precipitations (400 mm per year) during grapevine cycle. These extremely dry conditions affect vineyard productivity and sustainability. Supplementary irrigation is a needed practice in order to maintain yield and quality. Almost all Spanish grape growing regions are characterized by these within this context, especially in the center region, where this study was performed. The main objective of this work was to study the influence of irrigation on yield and quality. For this aim, we applied different levels of irrigation (mm of water applied) during different stages of growth and berry maturity. Four experimental treatments were applied considering the amount of water and the moment of the application: T1: Water irrigation (420 mm) applied from bloom to maturity. T2: Corresponded to the traditional irrigation scheduling, from preveraison to maturity (154 mm). T3: Water irrigation from bloom to preveraison, and water deficit from veraison to maturity (312 mm). T4: Irrigation applied from preveraison to maturity (230 mm) Experimental vineyard, cv. Cabernet Sauvignon, was located in a commercial vineyard (Bodegas Licinia S.L.) in the hot region of Morata de Tajuña (Madrid). The trial was performed during 2010 and 2011 seasons. Our results showed that yield increased from 2010 to 2011 in the treatments with a higher amount of water appli ed, T1 and T3 (24 and 10 % of yield increase respectively). This was mainly due to an increase in bud fertility (nº of bunches per shoot). Furthermore, sugar content was higher in T3 (27.3 ºBrix), followed by T2 (27 ºBrix). By contrast, T4 (irrigation from veraison) presented the lowest solid soluble concentration and the highest acidity. These results suggest that grapevine has an intrinsic capacity to adapt to its environment. However, this adaptation capacity should be evaluated considering the sensibility of quality parameters during the maturity period (acidity, pH, aroma, color...) and its impact on yield. Here, we demonstrated that a higher amount of water irrigation applied was no linked to a negative effect on quality.

Estudio de los efectos en el viñedo de la modificación del déficit hídrico continuo en los periodos anterior y posterior al envero (cv. Cabernet Sauvignon; Vitis vinifera L.)

En regiones semiáridas, con veranos cálidos, evapotranspiraciones elevadas, humedades relativas bajas, además de precipitaciones intermitentes y escasas (400 mm al año) que reducen la recarga del perfil en invierno, se puede ver afectada la productividad y sostenibilidad de los viñedos. Por eso en estas zonas puede ser necesario utilizar el riego suplementario para mantener la calidad y aumentar la productividad. En este marco de circunstancias es en el que se desarrolla la mayoría de la viticultura española, y en concreto en la zona centro donde se realizó el estudio. Con este trabajo se pretende estudiar la influencia del agua del riego, con distintas dosis y aplicada en diferentes fases de crecimiento y maduración de la baya, en la producción y calidad de la uva. Se estudió la influencia del déficit moderado continuo aplicado antes y después de envero, en el aprovechamiento de los recursos ambientales y en la respuesta del cv. Cabernet Sauvignon. El ensayo se desarrolló en 2010 y 2011 en la finca “La Alcoholera”, perteneciente a bodegas LICINIA S.L., ubicada en la localidad de Chinchón, Comunidad de Madrid, España. Durante 2010 y 2011 se realizaron estudios en cepas del cv. Cabernet Sauvignon (clon 15), injertadas sobre 41B y plantadas en 2005. Con poda corta en Cordón Royat unilateral de 80 cm de altura, y cuya vegetación alcanzó una altura de 97 cm. Las cepas del ensayo fueron conducidas verticalmente en espaldera (VSP), con 10 yemas por metro lineal. Las plantas dentro de la fila fueron separadas 1 m y la distancia de la calle fue de 3 m. La orientación de las filas norte – sur. Se plantearon cuatro tratamientos experimentales con diferentes dosis y momento de aplicación del riego. - T: Testigo. Déficit ligero, con un aporte continuado de agua desde floración (420 mm). - DMc: Déficit moderado continuo. Manejo del riego convencional, empezando en pre-envero (154 mm) - DM1: Déficit moderado a partir de pre-envero. Aporte de riego continuado desde floración reduciéndose la dosis de riego en pre-envero (312 mm). - DM2: Déficit moderado hasta pre-envero. Se empezó a regar a partir de preenvero (230 mm). Se observó que bajo condiciones de estrés hídrico leve, el crecimiento se reduce disminuyendo la migración de fotoasimilados hacia los órganos vegetativos. Generando menor área foliar en las plantas sometidas a déficit hídrico moderado entre floración y cuajado. Disminuyendo su consumo. En maduración la humedad del suelo dependió principalmente del riego aplicado y del consumo de la planta; dicho consumo dependió a la vez del desarrollo foliar del canopy y de la necesidad hídrica de la vid. El aumento del déficit hídrico disminuyó el contenido de agua en el suelo, lo que provocó diferencias en el estado hídrico y en el intercambio gaseoso de las hojas. En condiciones de déficit moderado, la fotosíntesis se encontró altamente correlacionada con el potencial hídrico foliar medido a mediodía solar. Además en condiciones de déficit moderado continuo la disponibilidad hídrica, la demanda atmosférica y el nivel de hidratación de las hojas, interaccionaron de forma compleja en la regulación estomática de las hojas, condicionando el intercambio gaseoso y la eficiencia en el uso del agua. Al aumentar el volumen de agua aplicado el peso de madera de poda por metro de fila fue superior. Las diferencias encontradas en el rendimiento fueron debidas a las diferencias en el peso de baya. El cual estuvo condicionado por la estrategia de riego, ya que, el déficit hídrico moderado antes de envero fue más crítico para el rendimiento que el déficit impuesto durante la madurez. Por otro lado, la biomasa dependió de la actividad fisiológica de la planta, la cual fue altamente dependiente de la disponibilidad hídrica. Déficit hídrico moderado aplicado de cuajado a envero, generó bayas más pequeñas y aumentó la relación hollejo:pulpa. El déficit moderado aplicado después de envero favoreció la acumulación de IPT y antocianos extraíbles, mejorando la calidad de la uva, pero disminuyó la acidez de la baya. El riego aplicado de envero a vendimia desaceleró la concentración de azúcares en bayas que fueron sometidas a déficit antes de pre-envero. ABSTRACT Mediterranean climate is characterized by hot summers, high evapotranspiration rates, and scarce precipitations (400 mm per year) during grapevine cycle. These extremely dry conditions affect vineyard productivity and sustainability. Supplementary irrigation is needed practice in order to maintain yield and quality. Almost all Spanish grape growing regions are characterized by these conditions, especially in the center region, where this trial was performed. The main objective of this work is to study the influence of water irrigation on yield and quality. For this aim, different levels of irrigation (mm of water applied) were applied during different stages of growth and berry maturity of Caberent Sauvignon grapevines. The work was conducted from 2010 to 2011 and located in Licinia (40º 12´ N, 3º 28´ W), Madrid, Spain. The cultivar utilized was Cabernet Sauvignon, clone 15 grafted onto rootstock 41B, planted in 2005. The vineyard was oriented north-south, with spacing on 3 meters between rows and 1 meter between plants. Vines were spurpruned to 10 buds per meter and trained in unilateral cordon with a height of 80 cm. Shoots were positioned vertically (VSP). Considering the amount of water and the moment of the application, four experimental treatments were applied: - T: Control sample. Slight deficit (420 mm) applied from bloom to maturity. - DMc: Continuous moderate deficit. Traditional irrigation: application of 154 mm of water from pre-veraison to maturity. - DM1: Deficit moderate from pre-veraison. Irrigation of 312 mm of water from bloom to pre-veraison. - DM2: Deficit moderate to pre-veraison. Irrigation of 230 mm of water from preveraison to maturity Under moderated water stress conditions it was seen than leaf growth decreases due to the reduction of migration of photo-assimilates to vegetative organs. Vines with moderate water deficit between flowering and ripening develop less leaf area and decrease its water consumption. During maturation of berries, soil moisture depends on irrigation and plant consumption. This consumption further depends on vegetation development and on the vine needs for water. By increasing water deficit, the water content in the soil decreases. This causes differences in leaf water status and in the gases exchange. Under moderate deficit conditions, photosynthesis was found highly correlated with midday leaf water potential. Further, atmospheric demand and the level of leaves hydration interact in complex ways in the stomatal regulation, which affects leaf gas exchange and the efficiency of water use. The amount of water applied is directly proportional to pruning weight. Changes in berry weight cause differences in yield ratios. The differences in berry weights are conditioned by the irrigation strategy, the moderate water deficit before veraison influences more than the deficit applied from veraison. Biomass generated for the plant depends on its physiological activity, which is highly related to the water availability. Moderate water deficit applied from fruit set to ripening generates smaller berries, increasing the pulp/skin ratio. Moderate deficit applied after veraison promotes the accumulation of extractables anthocyans and TPI. Despite this treatment improves color parameters of the grapes, it decreases its total acidity. Irrigation applied from veraison to harvest slows down sugar accumulation in berries compared to those under deficit before veraison conditions.