Efeito da sedação do midazolam, quetamina e butorfanol nos valores do ultrassom com Doppler espectral na artéria femoral e grandes artérias abdominais de gatos

Real time information about direction and type of blood flow can be obtained with Doppler ultrasound. In the literature it was not found data obtained with this method from celiac and cranial mesenteric artery in cats. Moreover, sedation of the animal is occasionally necessary to obtain more information on any blood vessel using this method. The purpose of this study was to evaluate the quantitative aspects of spectral waves formed from blood flow of the celiac, cranial mesenteric, renal, external iliac, femoral, and aortic arteries in healthy cats, and to compare them with the same animals when subjected to midazolam, ketamine, and butorphanol sedation. We also measured the heart rate. Twenty healthy adult cats were evaluated. The values obtained for resistivity index and pulsatility index from the celiac artery were 0.62 ± 0.10 and 1.29 ± 0.55, and those from the mesenteric artery were 0.68 ± 0.09 and 1.37 ± 0.39, respectively. Although heart rate was higher in sedated animals, no significant statistical difference was found in case of other parameters, except celiac artery end diastolic velocity and time averaged mean velocity and iliac artery resistivity and pulsatility index. Thus, we provide the Doppler velocimetry parameter from celiac and mesenteric arteries and conclude that this protocol does not alter the values of Doppler ultrasound in the selected vessels, except the celiac and iliac arteries.Informações em tempo real da direção e tipo de fluxo sanguíneo podem ser obtidas com ultrassonografia com Doppler. Existe na literatura dados relativos a esses parâmetros, em gatos não sedados, obtidos das artérias: aorta, renal, ilíaca e femoral; no entanto não foram encontrados na literatura dados relativos às artérias celíaca e mesentérica cranial. Além disso, ocasionalmente há necessidade de sedar animais inquietos ou agressivos, para que seja possível a realização deste exame. O objetivo do trabalho foi avaliar os aspectos quantitativos da onda espectral formada pelo fluxo sanguíneo das artérias: celíaca, mesentérica cranial, renal, ilíaca externa, femoral e aorta abdominal de gatos hígidos e compará-los aos obtidos dos mesmos animais submetidos à sedação com midazolam, cetamina e butorfanol. A frequência cardíaca também foi mensurada. Foram avaliados 20 gatos SRD adultos e saudáveis. Os valores encontrados em animais não sedados na artéria celíaca de índice de resistividade foi 0,62 ± 0,10 e índice de pulsatilidade 1,29 ± 0,55, enquanto da artéria mesentérica cranial, 0,68 ± 0,11 e 1,37 ± 0,39, respectivamente. Apesar da frequência cardíaca mais elevada nos animais sedados, não foram encontradas diferenças estatisticamente significativas dentre os demais parâmetros avaliados, exceto na velocidade diastólica final e velocidade média da artéria celíaca, e índice de resistividade e de pulsatilidade da artéria ilíaca. Dessa forma, foram fornecidos parâmetros dopplervelocimétricos da artéria celíaca e mesentérica cranial e conclui-se que o protocolo utilizado não alterou os valores encontrados por ultrassonografia Doppler nos vasos selecionados, exceto da artéria celíaca e da ilíaca

Position statement of the Brazilian Academy of Rhinology on the use of antihistamines, antileukotrienes, and oral corticosteroids in the treatment of inflammatory sinonasal diseases

Introduction: Inflammatory conditions of the nose and paranasal sinuses are very prevalent in the general population, resulting in marked loss of quality of life in affected patients, as well as significant work, leisure, and social activity losses. These patients require specific and specialized treatment. A wide range of oral medications are available. Objective: The present document is aimed to clarify, for professionals treating patients with inflammatory sinonasal diseases, both specialists and general practitioners, specific oral therapies in noninfectious nasal inflammatory conditions. Methods: The methodology used to create this article included the search for the key words: oral corticosteroids, antihistamines, antileukotrienes, rhinitis, rhinosinusitis in the MEDLINE and EMBASE databases in the last 5 years. Since no relevant article was found for the text on the subject of interest in the last 5 years, the search was extended for another 5 years, and so on, according to the authors' needs. Results: Relevant literature was found regarding the use of antihistamines, antileukotrienes and oral corticosteroids in these conditions. The Brazilian Academy of Rhinology emphasizes, after extensive discussion by the collegiate, key points in the treatment with these drugs. Conclusion: There is support in the literature for the use of these drugshowever, final considerations about the role of each of them have been made. (C) 2017 Published by Elsevier Editora Ltda. on behalf of Associacao Brasileira de Otorrino-laringologia e Cirurgia Cervico-Facial.Univ Sao Paulo, Disciplina Otorrinolaringol, Sao Paulo, SP, BrazilUniv Sao Paulo, Fac Med, Sao Paulo, SP, BrazilUniv Sao Paulo, Fac Med, Dept Otorrinolaringol, Sao Paulo, SP, BrazilUniv Sao Paulo, Fac Med Ribeirao Preto, Dept Otorrinolaringol, Ribeirao Preto, SP, BrazilUniv Fed Sao Paulo, Ciencias Saude, Sao Paulo, SP, BrazilUniv Fed Sao Paulo, Otorrinolaringol, Sao Paulo, SP, BrazilUniv Fed Minas Gerais, Fac Med, Belo Horizonte, MG, BrazilUniv Sao Paulo, Fac Med Ribeirao Preto, Ribeirao Preto, SP, BrazilUniv Fed Bahia, Fac Med, Disciplina Otorrinolaringol, Salvador, BA, BrazilHosp Inst Paranaense Otorrinolaringol, Centro Rinite & Alergia, Curitiba, PR, BrazilUniv Estado Rio De Janeiro, Rio De Janeiro, RJ, BrazilUniv Brasilia, Fac Med, Brasilia, DF, BrazilUniv Fed Sao Paulo, Dept Otorrinolaringol & Cabeca & Pescoco, Sao Paulo, SP, BrazilUniv Luterana Brasil, Fac Med, Otorrinolaringol, Canoas, RS, BrazilMt Sinai Hosp, Dept Othorhinolaryngol, Toronto, ON, CanadaUniv Sao Paulo, Fac Med, Ciencias, Sao Paulo, SP, BrazilUniv Sao Paulo, Fac Med Ribeirao Preto, Dept Oftalmol Otorrinolaringol & Cirurgia Cabeca, Ribeirao Preto, SP, BrazilUniv Fed Sao Paulo, Ciencias Saude, Sao Paulo, SP, BrazilUniv Fed Sao Paulo, Otorrinolaringol, Sao Paulo, SP, BrazilUniv Fed Sao Paulo, Dept Otorrinolaringol & Cabeca & Pescoco, Sao Paulo, SP, BrazilWeb of Scienc

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

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

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