Dispersão de sementes por aves na galeria ripícola e matriz envolvente

As galerias ripícolas são habitats com uma grande disponibilidade de recursos alimentares e abrigo para a fauna, estando entre os habitats mais importantes e vulneráveis do mundo. São uma fonte de produção de frutos, o que atrai muitos animais, como as aves frugívoras, que são os principais dispersores de sementes na bacia do Mediterrâneo. O objetivo principal deste estudo foi estudar os padrões de dispersão de sementes por aves na interface galeria ripícola-matriz florestal envolvente (Montado). Foram marcadas com fluorescência plantas-mãe produtoras de frutos, e utilizadas armadilhas para sementes e transectos, para a recolha dos dejetos de aves onde, posteriormente, se detetaram as sementes dispersadas. Constatou-se que a dispersão de sementes e a abundância de plantas-mãe foi superior a distâncias mais próximas da ribeira, diminuindo à medida que esta distância aumenta. A espécie mais dispersada foi Smilax aspera e as espécies com sementes de menor dimensão, foram dispersadas a uma maior distância da planta-mãe, provavelmente devido a este tipo de sementes permanecerem mais tempo no trato intestinal das aves. Os resultados deste estudo apresentam algumas implicações para a colonização da matriz adjacente por plantas produtoras de frutos; ABSTRACT: Riparian galleries are habitats with a large availability food resources and shelter for animals, being among the most important and vulnerable habitats in the world. These zones are a great source of fruits attracting many animals, such as frugivorous birds, which are the main seed dispersers in the Mediterranean basin. The objective of this thesis is the study of seed dispersal patterns by birds, in the riparian gallery and in the surrounding forest matrix (Montado). Fruits of several plant species were used to collect bird droppings and detect fluorescent seeds in those droppings. Fruit abundance and seed dispersal were higher close to the stream, and decreased rapidly with an increase in distance from the stream. From all species, the most dispersed was Smilax aspera and species with smaller seed were found at a significantly larger distance from parents plants than species with large seeds. This can be explained by the fact that smaller seed stay longer in the intestinal tract of the birds. The results of this study present some implications for the colonization of freshly fruit plants from the riparian gallery into the adjacent matrix.

Measurement of the energy spectrum of cosmic rays above 10(18) eV using the Pierre Auger Observatory

We report a measurement of the flux of cosmic rays with unprecedented precision and Statistics using the Pierre Auger Observatory Based on fluorescence observations in coincidence with at least one Surface detector we derive a spectrum for energies above 10(18) eV We also update the previously published energy spectrum obtained with the surface detector array The two spectra are combined addressing the systematic uncertainties and, in particular. the influence of the energy resolution on the spectral shape The spectrum can be described by a broken power law E-gamma with index gamma = 3 3 below the ankle which is measured at log(10)(E-ankle/eV) = 18 6 Above the ankle the spectrum is described by a power law with index 2 6 followed by a flux suppression, above about log(10)(E/eV) = 19 5, detected with high statistical significance (C) 2010 Elsevier B V All rights reserved

Effects of the spermatozoa: oocyte ratio, water volume and water temperature on artificial fertilization and sperm activation of cascudo-preto

The objective of this study was to evaluate the effects of water volume and water temperature on the sperm motility duration and the number of spermatozoa, and the water volume on the fertilization rates of oocytes of Rhinelepis aspera. Experiments were carried out to evaluate the effect of semen dilutions (1.74×10-5, 1.74×10-4, 1.74×10-3, 1.74×10-2, 1.74×10-1 and 1.00 mL of sperm.mL-1 of water) and water temperature (5, 10, 15, 20, 25, 30, 35, 40, 45, and 50 ºC) on spermatozoa motility duration. In addition, the effects of insemination dose (7×10³, 7×10(4), 7×10(5), 7×10(6) and 7×10(7) spermatozoa.oocyte-1) and water volume (1.0, 30.0, 60.0, 90.0 and 120.0 mL water.2.0 mL-1 oocytes) on the artificial fertilization rates of oocytes were evaluated. The longest sperm motility duration were observed for the semen dilution of 1.74×10-5 mL semen.mL-1 water and in water at 5 ºC. The highest fertilization rates were obtained for insemination doses between 7.00×10³ and 1.23×10(7) spermatozoa. oocyte-1 and water volume of 28.11 mL water.2.0 mL-1 oocytes.

Nanosecond-level time synchronization of autonomous radio detector stations for extensive air showers

To exploit the full potential of radio measurements of cosmic-ray air showers at MHz frequencies, a detector timing synchronization within 1 ns is needed. Large distributed radio detector arrays such as the Auger Engineering Radio Array (AERA) rely on timing via the Global Positioning System (GPS) for the synchronization of individual detector station clocks. Unfortunately, GPS timing is expected to have an accuracy no better than about 5 ns. In practice, in particular in AERA, the GPS clocks exhibit drifts on the order of tens of ns. We developed a technique to correct for the GPS drifts, and an independent method is used to cross-check that indeed we reach a nanosecond-scale timing accuracy by this correction. First, we operate a "beacon transmitter" which emits defined sine waves detected by AERA antennas recorded within the physics data. The relative phasing of these sine waves can be used to correct for GPS clock drifts. In addition to this, we observe radio pulses emitted by commercial airplanes, the position of which we determine in real time from Automatic Dependent Surveillance Broadcasts intercepted with a software-defined radio. From the known source location and the measured arrival times of the pulses we determine relative timing offsets between radio detector stations. We demonstrate with a combined analysis that the two methods give a consistent timing calibration with an accuracy of 2 ns or better. Consequently, the beacon method alone can be used in the future to continuously determine and correct for GPS clock drifts in each individual event measured by AERA.

Search for ultrarelativistic magnetic monopoles with the Pierre Auger observatory

We present a search for ultrarelativistic magnetic monopoles with the Pierre Auger observatory. Such particles, possibly a relic of phase transitions in the early Universe, would deposit a large amount of energy along their path through the atmosphere, comparable to that of ultrahigh-energy cosmic rays (UHECRs). The air-shower profile of a magnetic monopole can be effectively distinguished by the fluorescence detector from that of standard UHECRs. No candidate was found in the data collected between 2004 and 2012, with an expected background of less than 0.1 event from UHECRs. The corresponding 90% confidence level (C.L.) upper limits on the flux of ultrarelativistic magnetic monopoles range from 10(-1)9 (cm(2) sr s)(-1) for a Lorentz factor gamma = 10(9) to 2.5 x 10(-21) (cm(2) sr s)(-1) for gamma = 10(12). These results-the first obtained with a UHECR detector-improve previously published limits by up to an order of magnitude.