Efeito do uso do traje de neoprene sobre variáveis técnicas, fisiológicas e perceptivas de nadadores

Ao contrário do que ocorre em provas de piscina, competições em águas abertas estão sujeitas as condições ambientais, sendo uma delas as baixas temperaturas. Em determinadas circunstâncias é permitido o uso de roupas especiais para evitar hipotermia. O objetivo do estudo foi verificar os efeitos do uso da roupa de neoprene em um grupo composto por triatletas e nadadores, comparado ao uso de vestimentas convencionais (sunga) sobre variáveis cinemáticas e psicofisiológicas do nado. Participaram 20 homens (12 triatletas e oito nadadores) de idade 22,0 ± 6,6 anos com desempenhos que correspondem a 75 ± 7,7% do melhor tempo brasileiro na prova de 400 m. Os atletas realizaram duas repetições máximas e duas submáximas de 400 m em nado "crawl", com e sem o uso da roupa de neoprene. Foram comparadas a velocidade média (VM), comprimento de braçada (CB), frequência de braçada (FB), índice de nado (IN), percepção subjetiva de esforço (PSE), frequência cardíaca (FC), e concentração de lactato sanguíneo (LAC). Um conjunto de ANOVAs com medidas repetidas do tipo "two-way" foi aplicado. Quando diferenças foram encontradas o teste de Tukey foi empregado. Com o traje de neoprene, em máxima intensidade, o tempo para nadar a distância foi 6,4% menor, com manutenção da FB e aumento da CB, as variáveis psicofisiológicas não diferiram estatisticamente. Em esforço submáximo, o uso do traje de neoprene resultou em menor FB, maior CB, maior IN e em menores valores de FC, LAC e PSE (p In open water swimming competitions, athletes are prone to environmental conditions and are frequently exposed to low temperatures, in contrast to what occurs in indoor competitions. In some circumstances the use of special swimming suits is allowed to avoid hypothermia. The aim of this study was to verify the effects of the use of a neoprene swimming suit in comparison to a conventional swimming suit on a number of cinematic and psychophysiological variables. Twenty athletes experienced in swimming competitions (12 triathletes and 8 swimmers; 22.0± 6.6 yearsold), whose the performance was 75 ± 7.7% of the National record. Athletes performed two maximal and two submaximal 400m crawl simulated competition with a whole body neoprene swimming suit and with a conventional swimming suit. Mean speed (VM) stroke length (CB), stroke frequency (FB), swimming index (IN), rate of perceived effort (PSE), heart rate, and blood lactate concentration (LAC) were compared between conditions. The time to perform maximal trials with the use of the neoprene swimming suit was 6.4% shorter than when wearing the traditional swimming suit. FB and the psychophysiological variables remained unchanged, while CB increased in response to the use of the neoprene swimming suit. The use of the neoprene swimming suit in submaximal trials provided smaller FB, FC, LAC and PSE and larger CB and IN in comparison to the use of the traditional swimming suit. The results indicated that the neoprene swimming suit increases performance in biomechanical, physiological and perceptive aspects. The VM increase in maximal efforts does not depend exclusively on changes in FB and CB. Possibly, increments of the parameters related to the swimming may have improved the mechanical efficiency of the movement, which may have provided a movement economy that resulted in a better performance

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, \nobreak{$6\times 10^{19}$eV}. The anisotropy was measured by the fraction of arrival directions that are less than $3.1^\circ$ from the position of an active galactic nucleus within 75 Mpc (using the V\'eron-Cetty and V\'eron $12^{\rm th}$ 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 $(38^{+7}_{-6})$, 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.Comment: Accepted for publication in Astroparticle Physics on 31 August 201

The Fluorescence Detector of the Pierre Auger Observatory

The Pierre Auger Observatory is a hybrid detector for ultra-high energy cosmic rays. It combines a surface array to measure secondary particles at ground level together with a fluorescence detector to measure the development of air showers in the atmosphere above the array. The fluorescence detector comprises 24 large telescopes specialized for measuring the nitrogen fluorescence caused by charged particles of cosmic ray air showers. In this paper we describe the components of the fluorescence detector including its optical system, the design of the camera, the electronics, and the systems for relative and absolute calibration. We also discuss the operation and the monitoring of the detector. Finally, we evaluate the detector performance and precision of shower reconstructions.Comment: 53 pages. Submitted to Nuclear Instruments and Methods in Physics Research Section

Advanced functionality for radio analysis in the Offline software framework of the Pierre Auger Observatory

The advent of the Auger Engineering Radio Array (AERA) necessitates the development of a powerful framework for the analysis of radio measurements of cosmic ray air showers. As AERA performs "radio-hybrid" measurements of air shower radio emission in coincidence with the surface particle detectors and fluorescence telescopes of the Pierre Auger Observatory, the radio analysis functionality had to be incorporated in the existing hybrid analysis solutions for fluoresence and surface detector data. This goal has been achieved in a natural way by extending the existing Auger Offline software framework with radio functionality. In this article, we lay out the design, highlights and features of the radio extension implemented in the Auger Offline framework. Its functionality has achieved a high degree of sophistication and offers advanced features such as vectorial reconstruction of the electric field, advanced signal processing algorithms, a transparent and efficient handling of FFTs, a very detailed simulation of detector effects, and the read-in of multiple data formats including data from various radio simulation codes. The source code of this radio functionality can be made available to interested parties on request.Comment: accepted for publication in NIM A, 13 pages, minor corrections to author list and references in v

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 $2.5\times 10^{17}$ 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.Comment: 28 pages, 11 figure

Propagação de abacateiro via estacas estioladas

Este trabalho objetivou testar um método de propagação de abacateiro a partir de estacas estioladas cultivadas em recipientes de diferentes alturas. O experimento foi desenvolvido em câmara de nebulização intermitente. O delineamento experimental foi em blocos ao acaso, em esquema fatorial 3x4, com três repetições, testando-se dois métodos de obstrução de seiva (anelamento da casca, estrangulamento da casca) e quatro alturas de recipientes para o substrato (10, 15, 20 e 25 cm). Decorridos 250 dias, não se observou efeito da altura do recipiente na sobrevivência, no número de folhas desenvolvidas, na altura e no diâmetro das mudas formadas a partir de estacas estioladas. Houve maior sobrevivência e emissão de folhas nas estacas de casca anelada em relação à testemunha; as estacas de casca estrangulada situaram-se em posição intermediária. O prévio anelamento ou estrangulamento da casca de ramos estiolados aumentaram a sobrevivência e o crescimento de mudas na propagação de abacateiro da seleção Viamão, por estaquia