User satisfaction on the use of hypermedia in a health-education mobile device application

O uso da tecnologia na área da saúde tem crescido cada vez mais. Os dispositivos móveis possibilitam que as pessoas aprendam em qualquer lugar e a qualquer tempo. OBJETIVO: investigar a satisfação do usuário quanto ao uso de hipermídias para a aprendizagem de educação em saúde por meio de dispositivo móvel. MÉTODO: contou com 4 partes. Na primeira, foi aplicado um questionário pré-teste, em seguida houve a interação com as hipermídias, posteriormente aplicou-se o questionário pós-teste. Por fim, os participantes avaliaram a satisfação quanto ao uso das hipermídias. RESULTADOS: os resultados obtidos demonstraram que os participantes consideraram as hipermídias atraentes, desejadas, que elas promovem o sentimento de integração e aproximação, bem como tem um enorme valor em sua aplicação. CONCLUSÕES: a pesquisa demonstrou que o uso das hipermídias em dispositivos móveis para o aprendizado em cuidados em saúde é uma solução criativa, atrativa e eficaz e aprimora o processo ensino-aprendizagem.The use of technology in healthcare has been growing more each day. Mobile devices make it possible for anyone to learn anywhere, anytime. OBJECTIVE: to investigate user satisfaction regarding the use of hypermedia for learning health education through mobile devices. METHODS: It consisted of 4 parts. At first, a pre-test questionnaire was applied, then there was the interaction with the hypermedia, later the post-test questionnaire was conducted. Finally, participants rated their satisfaction in regard to the use of hypermedia. RESULTS: findings showed that the participants considered the hypermedia appealing, desirable, promoted a feeling of integration and closeness, and had an enormous value in their application. CONCLUSIONS: this study demonstrated that the use of hypermedia on mobile devices for learning in healthcare is a creative, appealing, and effective solution. Also, it improves the teaching-learning process

Measurement of the cosmic ray spectrum above 4×10184{\times}10^{18} eV using inclined events detected with the Pierre Auger Observatory

A measurement of the cosmic-ray spectrum for energies exceeding $4{\times}10^{18}$ eV is presented, which is based on the analysis of showers with zenith angles greater than $60^{\circ}$ detected with the Pierre Auger Observatory between 1 January 2004 and 31 December 2013. The measured spectrum confirms a flux suppression at the highest energies. Above $5.3{\times}10^{18}$ eV, the "ankle", the flux can be described by a power law $E^{-\gamma}$ with index $\gamma=2.70 \pm 0.02 \,\text{(stat)} \pm 0.1\,\text{(sys)}$ followed by a smooth suppression region. For the energy ($E_\text{s}$) at which the spectral flux has fallen to one-half of its extrapolated value in the absence of suppression, we find $E_\text{s}=(5.12\pm0.25\,\text{(stat)}^{+1.0}_{-1.2}\,\text{(sys)}){\times}10^{19}$ eV.Comment: Replaced with published version. Added journal reference and DO

An estimate of the number of tropical tree species

The high species richness of tropical forests has long been recognized, yet there remains substantial uncertainty regarding the actual number of tropical tree species. Using a pantropical tree inventory database from closed canopy forests, consisting of 657,630 trees belonging to 11,371 species, we use a fitted value of Fisher’s alpha and an approximate pantropical stem total to estimate the minimum number of tropical forest tree species to fall between ∼40,000 and ∼53,000, i.e. at the high end of previous estimates. Contrary to common assumption, the Indo-Pacific region was found to be as species-rich as the Neotropics, with both regions having a minimum of ∼19,000–25,000 tree species. Continental Africa is relatively depauperate with a minimum of ∼4,500–6,000 tree species. Very few species are shared among the African, American, and the Indo-Pacific regions. We provide a methodological framework for estimating species richness in trees that may help refine species richness estimates of tree-dependent taxa

A search for ultra-high-energy photons at the Pierre Auger Observatory exploiting air-shower universality

The Pierre Auger Observatory is the most sensitive detector to primary photons with energies above ∼0.2 EeV. It measures extensive air showers using a hybrid technique that combines a fluorescence detector (FD) with a ground array of particle detectors (SD). The signatures of a photon-induced air shower are a larger atmospheric depth at the shower maximum (X$_{max}$) and a steeper lateral distribution function, along with a lower number of muons with respect to the bulk of hadron-induced background. Using observables measured by the FD and SD, three photon searches in different energy bands are performed. In particular, between threshold energies of 1-10 EeV, a new analysis technique has been developed by combining the FD-based measurement of X$_{max}$ with the SD signal through a parameter related to its muon content, derived from the universality of the air showers. This technique has led to a better photon/hadron separation and, consequently, to a higher search sensitivity, resulting in a tighter upper limit than before. The outcome of this new analysis is presented here, along with previous results in the energy ranges below 1 EeV and above 10 EeV. From the data collected by the Pierre Auger Observatory in about 15 years of operation, the most stringent constraints on the fraction of photons in the cosmic flux are set over almost three decades in energy

Study on multi-ELVES in the Pierre Auger Observatory

Since 2013, the four sites of the Fluorescence Detector (FD) of the Pierre Auger Observatory record ELVES with a dedicated trigger. These UV light emissions are correlated to distant lightning strikes. The length of recorded traces has been increased from 100 μs (2013), to 300 μs (2014-16), to 900 μs (2017-present), to progressively extend the observation of the light emission towards the vertical of the causative lightning and beyond. A large fraction of the observed events shows double ELVES within the time window, and, in some cases, even more complex structures are observed. The nature of the multi-ELVES is not completely understood but may be related to the different types of lightning in which they are originated. For example, it is known that Narrow Bipolar Events can produce double ELVES, and Energetic In-cloud Pulses, occurring between the main negative and upper positive charge layer of clouds, can induce double and even quadruple ELVES in the ionosphere. This report shows the seasonal and daily dependence of the time gap, amplitude ratio, and correlation between the pulse widths of the peaks in a sample of 1000+ multi-ELVES events recorded during the period 2014-20. The events have been compared with data from other satellite and ground-based sensing devices to study the correlation of their properties with lightning observables such as altitude and polarity