Atmospheric effects on extensive air showers observed with the surface detector of the Pierre Auger observatory

Atmospheric parameters, Such as pressure (P), temperature (T) and density (rho proportional to P/T), affect the development of extensive air showers initiated by energetic cosmic rays. We have Studied the impact of atmospheric variations on extensive air showers by means of the surface detector of the Pierre Auger Observatory. The rate of events shows a similar to 10% seasonal modulation and similar to 2% diurnal one. We find that the observed behaviour is explained by a model including the effects associated with the variations of P and rho. The former affects the longitudinal development of air showers while the latter influences the Moliere radius and hence the lateral distribution of the shower particles. The model is validated with full simulations of extensive air showers using atmospheric profiles measured at the site of the Pierre Auger Observatory. (C) 2009 Elsevier B.V. All rights reserved.

Upper limit on the cosmic-ray photon fraction at EeV energies from the Pierre Auger Observatory

From direct observations of the longitudinal development of ultra-high energy air showers performed with the Pierre Auger Observatory, upper limits of 3.8%, 2.4%, 3.5% and 11.7% (at 95% c.l.) are obtained on the fraction of cosmic-ray photons above 2, 3, 5 and 10 EeV (1 EeV equivalent to 10(18) eV), respectively. These are the first experimental limits on ultra-high energy photons at energies below 10 EeV. The results complement previous constraints on top-down models from array data and they reduce systematic uncertainties in the interpretation of shower data in terms of primary flux, nuclear composition and proton-air cross-section. (C) 2009 Elsevier B.V. All rights reserved.

Anisotropy and chemical composition of ultra-high energy cosmic rays using arrival directions measured by the Pierre Auger Observatory

The Pierre Auger Collaboration has reported. evidence for anisotropy in the distribution of arrival directions of the cosmic rays with energies E > E(th) = 5.5 x 10(19) eV. These show a correlation with the distribution of nearby extragalactic objects, including an apparent excess around the direction of Centaurus A. If the particles responsible for these excesses at E > E(th) are heavy nuclei with charge Z, the proton component of the sources should lead to excesses in the same regions at energies E/Z. We here report the lack of anisotropies in these directions at energies above E(th)/Z (for illustrative values of Z = 6, 13, 26). If the anisotropies above E(th) are due to nuclei with charge Z, and under reasonable assumptions about the acceleration process, these observations imply stringent constraints on the allowed proton fraction at the lower energies.

Search for first harmonic modulation in the right ascension distribution of cosmic rays detected at the Pierre Auger Observatory

We present the results of searches for dipolar-type anisotropies in different energy ranges above 2.5 x 10(17) eV with the surface detector array of the Pierre Auger Observatory, reporting on both the phase and the amplitude measurements of the first harmonic modulation in the right-ascension distribution. Upper limits on the amplitudes are obtained, which provide the most stringent bounds at present, being below 2% at 99% C.L. for EeV energies. We also compare our results to those of previous experiments as well as with some theoretical expectations. (C) 2011 Elsevier B.V. All rights reserved.

The Pierre Auger Observatory scaler mode for the study of solar activity modulation of galactic cosmic rays

Since data-taking began in January 2004, the Pierre Auger Observatory has been recording the count rates of low energy secondary cosmic ray particles for the self-calibration of the ground detectors of its surface detector array. After correcting for atmospheric effects, modulations of galactic cosmic rays due to solar activity and transient events are observed. Temporal variations related with the activity of the heliosphere can be determined with high accuracy due to the high total count rates. In this study, the available data are presented together with an analysis focused on the observation of Forbush decreases, where a strong correlation with neutron monitor data is found.

The exposure of the hybrid detector of the Pierre Auger Observatory

The Pierre Auger Observatory is a detector for ultra-high energy cosmic rays. It consists of a surface array to measure secondary particles at ground level and a fluorescence detector to measure the development of air showers in the atmosphere above the array. The ""hybrid"" detection mode combines the information from the two subsystems. We describe the determination of the hybrid exposure for events observed by the fluorescence telescopes in coincidence with at least one water-Cherenkov detector of the surface array. A detailed knowledge of the time dependence of the detection operations is crucial for an accurate evaluation of the exposure. We discuss the relevance of monitoring data collected during operations, such as the status of the fluorescence detector, background light and atmospheric conditions, that are used in both simulation and reconstruction. (C) 2010 Elsevier B.V. All rights reserved.

Update on the correlation of the highest energy cosmic rays with nearby extragalactic matter

Data collected by the Pierre Auger Observatory through 31 August 2007 showed evidence for anisotropy in the arrival directions of cosmic rays above the Greisen-Zatsepin-Kuz`min energy threshold, 6 x 10(19) eV. The anisotropy was measured by the fraction of arrival directions that are less than 3.1 degrees from the position of an active galactic nucleus within 75 Mpc (using the Veron-Cetty and Veron 12th catalog). An updated measurement of this fraction is reported here using the arrival directions of cosmic rays recorded above the same energy threshold through 31 December 2009. The number of arrival directions has increased from 27 to 69, allowing a more precise measurement. The correlating fraction is (38(-6)(+7))%, compared with 21% expected for isotropic cosmic rays. This is down from the early estimate of (69-(+11)(13))%. The enlarged set of arrival directions is examined also in relation to other populations of nearby extragalactic objects: galaxies in the 2 Microns All Sky Survey and active galactic nuclei detected in hard X-rays by the Swift Burst Alert Telescope. A celestial region around the position of the radiogalaxy Cen A has the largest excess of arrival directions relative to isotropic expectations. The 2-point autocorrelation function is shown for the enlarged set of arrival directions and compared to the isotropic expectation. (C) 2010 Elsevier B.V. All rights reserved.

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

A study of the effect of molecular and aerosol conditions in the atmosphere on air fluorescence measurements at the Pierre Auger Observatory

The air fluorescence detector of the Pierre Auger Observatory is designed to perforin calorimetric measurements of extensive air showers created by Cosmic rays of above 10(18) eV. To correct these measurements for the effects introduced by atmospheric fluctuations, the Observatory contains a group Of monitoring instruments to record atmospheric conditions across the detector site, ail area exceeding 3000 km(2). The atmospheric data are used extensively in the reconstruction of air showers, and are particularly important for the correct determination of shower energies and the depths of shower maxima. This paper contains a summary of the molecular and aerosol conditions measured at the Pierre Auger Observatory since the start of regular operations in 2004, and includes a discussion of the impact of these measurements oil air shower reconstructions. Between 10(18) and 10(20) eV, the systematic Uncertainties due to all atmospheric effects increase from 4% to 8% in measurements of shower energy, and 4 g cm(-2) to 8 g cm(-2) in measurements of the shower maximum. (C) 2010 Elsevier B.V. All rights reserved.

TiO(2)-PHOTOCATALYZED DEGRADATION OF PHENOL IN SALINE MEDIA IN AN ANNULAR REACTOR: HYDRODYNAMICS, LUMPED KINETICS, INTERMEDIATES, AND ACUTE TOXICITY

The photocatalytic degradation of phenol in aqueous suspensions of TiO(2) under different salt concentrations in an annular reactor has been investigated. In all cases, complete removal of phenol and mineralization degrees above 90% were achieved. The reactor operational parameters were optimized and its hydrodynamics characterized in order to couple mass balance equations with kinetic ones. The photodegradation of the organics followed a Langmuir-Hinshelwood-Hougen- Watson lumped kinetics. From GC/MS analyses, several intermediates formed during oxidation have been identified. The main ones were catechol, hydroquinone, and 3-phenyl-2-propenal, in this order. The formation of negligible concentrations of 4-chlorophenol was observed only in high salinity medium. Acute toxicity was determined by using Artemia sp. as the test organism, which indicated that intermediate products were all less toxic than phenol and a significant abatement of the overall toxicity was accomplished, regardless of the salt concentration.

Formation Mechanism via a Heterocoagulation Approach of FePt Nanoparticles Using the Modified Polyol Process

Herein, we report a new approach of an FePt nanoparticle formation mechanism studying the evolution of particle size and composition during the synthesis using the modified polyol process. One of the factors limiting their application in ultra-high-density magnetic storage media is the particle-to-particle composition, which affects the A1-to-L1(0) transformation as well as their magnetic properties. There are many controversies in the literature concerning the mechanism of the FePt formation, which seems to be the key to understanding the compositional chemical distribution. Our results convincingly show that, initially, Pt nuclei are formed due to reduction of Pt(acac)(2) by the diol, followed by heterocoagulation of Fe cluster species formed from Fe(acac)(3) thermal decomposition onto the Pt nuclei. Complete reduction of heterocoagulated iron species seems to involve a CO-spillover process, in which the Pt nuclei surface acts as a heterogeneous catalyst, leading to the improvement of the single-particle composition control and allowing a much narrower compositional distribution. Our results show significant decreases in the particle-to-particle composition range, improving the A1-to-L1(0) phase transformation and, consequently, the magnetic properties when compared with other reported methods.

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Moluscos gastrópodes da plataforma continental externa e talude continental ao largo da laguna dos Patos - Rio Grande do Sul, Brasil

Em 1982 o Brasil participa da Convenção das Nações Unidas para o Direito do Mar. Esta convenção dispõe sobre os usos dos espaços marítimos e oceânicos, buscando a utilização racional e a exploração dos recursos do mar. Devido ao escasso conhecimento da região da plataforma externa e talude continental, surge o programa Avaliação do Potencial Sustentável de Recursos Vivos da Zona Econômica Exclusiva – REVIZEE, tanto para a diversificação da exploração pesqueira quanto para a determinação dos limites sustentáveis de captura. Com base em material coletado em abril de 1998, durante campanha de Bentos concernente ao programa REVIZEE, são fornecidos resultados relativos a Gastropoda encontrados na radial 45, estações hidrográficas 6839 (32o55´70´´S - 50o34´60´´W), 6840 (33o01´45´´S - 50o12´75´´W), 6841 (33o00´16´´S - 50o22´84´´W) e 6842 (32o57´81´´S - 50o29´18´´W), localizadas ao largo de Rio Grande, Rio Grande do Sul, Brasil. Para a avaliação da diversidade bêntica foram utilizados três tipos de amostradores de fundo; Draga de arrasto, Box Corer e Van Veen. Molluscos foram separados dos demais grupos taxonômicos pela equipe do REVIZEE e recebidos pelo laboratório de malacologia da Universidade Federal do Rio Grande do Sul. O material foi triado sob lupa Zeiss Stemi 2000- C ou Wild M-38. O material foi identificado por comparação com os dados da bibliografia e/ou por comparação com exemplares depositados nas coleções do Museu Oceanográfico Eliézer de Carvalho Rios (MORG) e/ou com a coleção particular do Dr. José Carlos Tarasconi São identificados e caracterizados quanto a tamanho, esculturação e área de ocorrência 6.020 exemplares distribuídos em 36 famílias - 80 táxons em nível de espécie, 19 em nível de gênero e 2 em nível de família. A família Turridae é a que apresenta o maior número de táxons com 16 espécies. Turritella hookeri Reeve, 1849 é a espécie mais abundante, com 684 exemplares. Registra-se pela primeira vez para o Rio Grande do Sul as seguintes espécies: Brookula conica (Watson, 1886), Calliostoma echinatum Dall, 1881, Solariela carvalhoi Lopes & Cardoso, 1958, Caecum massambabensis Absalão, 1994, Turritella hookeri Reeve, 1849, Crepidula plana Say, 1822, Natica pusilla Say, 1822, Polinices lacteus (Guilding, 1833), Eulima mulata Rios & Absalão, 1990, Melanella aff. hypsela (Verrill & Bush, 1900), Trachipollia turricula (von Maltzan, 1884), Anachis sparsa Reeve, 1859, Dentimargo janeiroensis (E. A. Smith, 1915), Axelella brasiliensis Verhecken, 1991, Drilliola loprestiana (Calcara, 1841), Mitrolumna biplicata (Dall, 1889), Nannodiella vespuciana (Orbigny, 1842), Stenodrillia goundlachi (Dall & Simpson, 1901), Terebra brasiliensis E. A. Smith, 1873 e Mathilda aff. scitula Dall, 1889. Novos limites de profundidade são registrados para 29 espécies. Com base na lista de espécies encontradas, se discute sobre o limite das Províncias Caribenha e Patagônica e sobre a influência da Laguna dos Patos no Talude Continental ao largo de Rio Grande.

Análise dos impactos da tecnologia da informação nas organizações - um ensaio à luz da teoria da agência e da teoria dos custos de transação

À medida que as Organizações desenvolveram a sua habilidade em implementar sistemas de Tecnologia da Informação o foco da análise de sua implementação mudou da Tecnologia da Informação voltada para otimização da produção para a compreensão dos efeitos desta nos indivíduos, Organizações e sistemas econômicos. Através deste estudo busca-se uma nova análise dos efeitos da Tecnologia da Informação nos indivíduos, no ambiente, nas relações internas e externas às Organizações através da análise, à luz da Teoria dos Custos de Transação e Teoria da Agência, aborda-se como esses efeitos resultam em modificações em diversos atributos da Firma. Este trabalho traz como contribuição à área apresentar o estudo do impacto na Tecnologia da Informação nas Organizações utilizando a Teoria da Agência aplicada à modelagem de Galbraith (1977) para análise dos impactos internos a Firma e Teoria dos Custos de Transação aplicada à modelagem de Straub e Watson (2000) para análise dos impactos externos a mesma. A análise dos impactos de TI sob a ótica deste dois modelos constitui trabalho inédito na literatura científica especializada ao tema.