APTIDÃO FÍSICA RELACIONADA À SAÚDE DE ADOLESCENTES RESIDENTES NA ÁREA URBANA E RURAL

Nos últimos anos percebe-se uma inadequação na aptidão física relacionada à saúde e no estilo de vida dos indivíduos, entre eles os adolescentes. Os problemas gerados por essa inadequação podem comprometer à saúde. O objetivo deste estudo foi investigar a aptidão física relacionada à saúde dos adolescentes residentes na área urbana e rural de um município do meio-oeste catarinense. Tratou-se de um estudo realizado com 80 adolescentes, de ambos os sexos, matriculados no ensino médio de uma escola pública, sendo 40 residentes na área urbana e 40 na área rural. Para a seleção da amostra foi adotada a intencionalidade. Foram coletadas informações da capacidade cardiorrespiratória, com a corrida vai e vem (LEGER et al., 1988) e aptidão muscular (CSEF, 1998). Na avaliação da aptidão muscular constatou-se que 8 (20%) dos adolescentes da área rural apresentaram inadequação para critérios de saúde, enquanto que na região urbana foram encontrados 14 (35%) adolescentes com inadequação. Na capacidade cardiorrespiratória os adolescentes da área urbana apresentaram 21 (52,5%) adolescentes com adequação para critérios de saúde enquanto os adolescentes da área rural somente 15 (37,5%) adolescentes. O nível de aptidão muscular e de capacidade cardiorrespiratória dos adolescentes deste município é preocupante, porque apresentam um grande número de adolescentes com critérios inadequados da aptidão física para a saúde. É necessária uma intervenção a fim de que a prática da atividade física seja realizada com maior frequência pelos adolescentes

Comparison of different prognostic scores for patients with cirrhosis hospitalized with SARS-CoV-2 infection

Introduction and Objectives: Viral infections have been described to increase the risk of decompensation in patients with cirrhosis. We aimed to determine the effect of SARS-CoV-2 infection on outcome of hospitalized patients with cirrhosis and to compare the performance of different prognostic models for predicting mortality. Patients: We performed a prospective cohort study including 2211 hospitalized patients with confirmed SARS-CoV-2 infection from April 15, 2020 through October 1, 2020 in 38 Hospitals from 11 Latin American countries. We registered clinical and laboratory parameters of patients with and without cirrhosis. All patients were followed until discharge or death. We evaluated the prognostic performance of different scoring systems to predict mortality in patients with cirrhosis using ROC curves. Results: Overall, 4.6% (CI 3.7–5.6) subjects had cirrhosis (n = 96). Baseline Child-Turcotte-Pugh (CTP) class was assessed: CTP-A (23%), CTP-B (45%) and CTP-C (32%); median MELD-Na score was 19 (IQR 14−25). Mortality was 47% in patients with cirrhosis and 16% in patients without cirrhosis (P 30. The areas under the ROC curves for performance evaluation in predicting 28-days mortality for Chronic Liver Failure Consortium (CLIF-C), North American Consortium for the Study of End-Stage Liver Disease (NACSELD), CTP score and MELD-Na were 0.85, 0.75, 0.69, 0.67; respectively (P < .0001). Conclusions: SARS-CoV-2 infection is associated with elevated mortality in patients with cirrhosis. CLIFC had better performance in predicting mortality than NACSELD, CTP and MELD-Na in patients with cirrhosis and SARS-CoV-2 infection. Clinicaltrials.gov:NCT04358380.Fil: Mendizabal, Manuel. Universidad Austral; Argentina. Red Latinoamericana de Concientización y Educación en Investigación del Hígado; ArgentinaFil: Ridruejo, Ezequiel. Red Latinoamericana de Concientización y Educación en Investigación del Hígado; Argentina. Centro de Educación Médica e Investigaciones Clínicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Piñero, Federico. Universidad Austral; Argentina. Red Latinoamericana de Concientización y Educación en Investigación del Hígado; ArgentinaFil: Anders, Margarita. Hospital Alemán; Argentina. Red Latinoamericana de Concientización y Educación en Investigación del Hígado; ArgentinaFil: Padilla, Martín Jesus. Hospital Nacional Guillermo Almenara Irigoyen; PerúFil: Toro, Luis G.. Fundación de Medellín y Rionegro; ColombiaFil: Torre, Aldo. Instituto Nacional de Ciencias Médicas y Nutrición; MéxicoFil: Montes, Pedro. Hospital Nacional Daniel A. Carrión; ArgentinaFil: Urzúa, Alvaro. Universidad de Chile; ChileFil: Gonzalez Ballerga, Esteban. Universidad de Buenos Aires. Facultad de Medicina. Hospital de Clínicas General San Martín; ArgentinaFil: Silveyra, María Dolores. Sanatorio Anchorena; ArgentinaFil: Michelato, Douglas. Hospital Especializado en Enfermedades Infecciosas Instituto Couto Maia; BrasilFil: Díaz, Javier. Hospital Nacional Edgardo Rebagliati Martins; PerúFil: Peralta, Mirta. Red Latinoamericana de Concientización y Educación en Investigación del Hígado; Argentina. Gobierno de la Ciudad de Buenos Aires. Hospital de Infecciosas "Dr. Francisco Javier Muñiz"; ArgentinaFil: Pages, Josefina. Universidad Austral; Argentina. Red Latinoamericana de Concientización y Educación en Investigación del Hígado; ArgentinaFil: García, Sandro Ruiz. Hospital de Víctor Lazarte Echegaray; PerúFil: Gutierrez Lozano, Isabel. Centro Médico ABC; MéxicoFil: Macias, Yuridia. IMSS Hospital General Regional No. 1 “Dr. Carlos Mc Gregor Sánchez”; MéxicoFil: Cocozzella, Daniel. Red Latinoamericana de Concientización y Educación en Investigación del Hígado; Argentina. Hospital Italiano de La Plata; ArgentinaFil: Chavez Tapia, Norberto. Medica Sur Clinic & Foundation; MéxicoFil: Tagle, Martín. Clínica Anglo-Americana; PerúFil: Dominguez, Alejandra. Hospital Padre Hurtado; ChileFil: Varón, Adriana. Red Latinoamericana de Concientización y Educación en Investigación del Hígado; Argentina. Fundación Cardio Infantil; ColombiaFil: Vera Pozo, Emilia. Hospital Regional Dr. Teodoro Maldonado Carbo del IESS; EcuadorFil: Higuera de la Tijera, Fátima. Hospital General de México “Dr. Eduardo Liceaga”; MéxicoFil: Bustios, Carla. Fundación Cardio Infantil; ColombiaFil: Conte, Damián. Hospital Privado de Córdoba; ArgentinaFil: Escajadillo, Nataly. Universidad Austral; ArgentinaFil: Rubinstein, Fernando Adrian. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Hospital Especializado en Enfermedades Infecciosas Instituto Couto Maia; BrasilFil: Tenorio, Laura. Hospital Nacional Edgardo Rebagliati Martins; Per

Combined fit to the spectrum and composition data measured by the Pierre Auger Observatory including magnetic horizon effects

The measurements by the Pierre Auger Observatory of the energy spectrum and mass composition of cosmic rays can be interpreted assuming the presence of two extragalactic source populations, one dominating the flux at energies above a few EeV and the other below. To fit the data ignoring magnetic field effects, the high-energy population needs to accelerate a mixture of nuclei with very hard spectra, at odds with the approximate E$^{-2}$ shape expected from diffusive shock acceleration. The presence of turbulent extragalactic magnetic fields in the region between the closest sources and the Earth can significantly modify the observed CR spectrum with respect to that emitted by the sources, reducing the flux of low-rigidity particles that reach the Earth. We here take into account this magnetic horizon effect in the combined fit of the spectrum and shower depth distributions, exploring the possibility that a spectrum for the high-energy population sources with a shape closer to E$^{-2}$ be able to explain the observations

Studies of the mass composition of cosmic rays and proton-proton interaction cross-sections at ultra-high energies with the Pierre Auger Observatory

In this work, we present an estimate of the cosmic-ray mass composition from the distributions of the depth of the shower maximum (Xmax) measured by the fluorescence detector of the Pierre Auger Observatory. We discuss the sensitivity of the mass composition measurements to the uncertainties in the properties of the hadronic interactions, particularly in the predictions of the particle interaction cross-sections. For this purpose, we adjust the fractions of cosmic-ray mass groups to fit the data with Xmax distributions from air shower simulations. We modify the proton-proton cross-sections at ultra-high energies, and the corresponding air shower simulations with rescaled nucleus-air cross-sections are obtained via Glauber theory. We compare the energy-dependent composition of ultra-high-energy cosmic rays obtained for the different extrapolations of the proton-proton cross-sections from low-energy accelerator data

Study of downward Terrestrial Gamma-ray Flashes with the surface detector of the Pierre Auger Observatory

The surface detector (SD) of the Pierre Auger Observatory, consisting of 1660 water-Cherenkov detectors (WCDs), covers 3000 km2 in the Argentinian pampa. Thanks to the high efficiency of WCDs in detecting gamma rays, it represents a unique instrument for studying downward Terrestrial Gamma-ray Flashes (TGFs) over a large area. Peculiar events, likely related to downward TGFs, were detected at the Auger Observatory. Their experimental signature and time evolution are very different from those of a shower produced by an ultrahigh-energy cosmic ray. They happen in coincidence with low thunderclouds and lightning, and their large deposited energy at the ground is compatible with that of a standard downward TGF with the source a few kilometers above the ground. A new trigger algorithm to increase the TGF-like event statistics was installed in the whole array. The study of the performance of the new trigger system during the lightning season is ongoing and will provide a handle to develop improved algorithms to implement in the Auger upgraded electronic boards. The available data sample, even if small, can give important clues about the TGF production models, in particular, the shape of WCD signals. Moreover, the SD allows us to observe more than one point in the TGF beam, providing information on the emission angle

The dynamic range of the upgraded surface-detector stations of AugerPrime

The detection of ultra-high-energy cosmic rays by means of giant detector arrays is often limited by the saturation of the recorded signals near the impact point of the shower core at the ground, where the particle density dramatically increases. The saturation affects in particular the highest energy events, worsening the systematic uncertainties in the reconstruction of the shower characteristics. The upgrade of the Pierre Auger Observatory, called AugerPrime, includes the installation of an 1-inch Small PhotoMultiplier Tube (SPMT) inside each water-Cherenkov station (WCD) of the surface detector array. The SPMT allows an unambiguous measurement of signals down to about 250m from the shower core, thus reducing the number of events featuring a saturated station to a negligible level. In addition, a 3.8m2 plastic scintillator (Scintillator Surface Detector, SSD) is installed on top of each WCD. The SSD is designed to match the WCD (with SPMT) dynamic range, providing a complementary measurement of the shower components up to the highest energies. In this work, the design and performances of the upgraded AugerPrime surface-detector stations in the extended dynamic range are described, highlighting the accuracy of the measurements. A first analysis employing the unsaturated signals in the event reconstruction is also presented

Investigating multiple elves and halos above strong lightning with the fluorescence detectors of the Pierre Auger Observatory

ELVES are being studied since 2013 with the twenty-four FD Telescopes of the Pierre Auger Observatory, in the province of Mendoza (Argentina), the world’s largest facility for the study of ultra-high energy cosmic rays. This study exploits a dedicated trigger and extended readout. Since December 2020, this trigger has been extended to the three High levation Auger Telescopes (HEAT), which observe the night sky at elevation angles between 30 and 60 degrees, allowing a study of ELVES from closer lightning. The high time resolution of the Auger telescopes allows us to upgrade reconstruction algorithms and to do detailed studies on multiple ELVES. The origin of multiple elves can be studied by analyzing the time difference and the amplitude ratio between flashes and comparing them with the properties of radio signals detected by the ENTLN lightning network since 2018. A fraction of multi-ELVES can also be interpreted as halos following ELVES. Halos are disc-shaped light transients emitted at 70-80 km altitudes, appearing at the center of the ELVES rings, due to the rearrangement of electric charges at the base of the ionosphere after a strong lightning event