181 research outputs found
Current status of turbulent dynamo theory: From large-scale to small-scale dynamos
Several recent advances in turbulent dynamo theory are reviewed. High
resolution simulations of small-scale and large-scale dynamo action in periodic
domains are compared with each other and contrasted with similar results at low
magnetic Prandtl numbers. It is argued that all the different cases show
similarities at intermediate length scales. On the other hand, in the presence
of helicity of the turbulence, power develops on large scales, which is not
present in non-helical small-scale turbulent dynamos. At small length scales,
differences occur in connection with the dissipation cutoff scales associated
with the respective value of the magnetic Prandtl number. These differences are
found to be independent of whether or not there is large-scale dynamo action.
However, large-scale dynamos in homogeneous systems are shown to suffer from
resistive slow-down even at intermediate length scales. The results from
simulations are connected to mean field theory and its applications. Recent
work on helicity fluxes to alleviate large-scale dynamo quenching, shear
dynamos, nonlocal effects and magnetic structures from strong density
stratification are highlighted. Several insights which arise from analytic
considerations of small-scale dynamos are discussed.Comment: 36 pages, 11 figures, Spa. Sci. Rev., submitted to the special issue
"Magnetism in the Universe" (ed. A. Balogh
Physiological and behavioural parameters of broiler chicks grown under different heating systems
Received: December 1st, 2022 ; Accepted: March 29th, 2023 ; Published: April 24th
, 2023 ; Correspondence: [email protected] study aimed to compare the internal environment, physiological variables, and
behavioural responses of chicks under two different heating systems. The experiment was
performed in two commercial broiler houses located in Brazil, where 28,000 male Cobb chicks
were housed during the first three weeks of life. One of the broiler houses was heated by an
industrial indirect-fired biomass furnace (S1). In addition, another heating system consisting of
two furnaces for indirect heating of the air using biomass (wood) as fuel, built by hand with
bricks, mud, and dung on an iron structure (S2), was tested. Measurements of the dry bulb
temperature (tdb), dew point temperature (tdp), and relative air humidity (RH) were performed.
Subsequently, the temperature-humidity index (THI) was calculated. In addition, the
physiological variables of the respiratory rate (RR) and cloacal temperature (tcloacal) were
measured three times a day (8:00 am, 2:00 pm, and 6:00 pm) in four chicks. The behaviours were
grouped by dendrograms, in which the similarity of these data was qualified. During the second
and third weeks of life, the THI values were below the recommended range. The RR and tcloacal
data were below the recommended comfort values, which may be an indicator that the chicks
were subjected to cold conditions. Regarding their behaviour, the chicks exhibited calm, feeding,
and sleepy behaviours most of the time. Problems in the heating system inside the broiler house
could be observed, possibly affecting the chicks’ thermal comfort and welfare, which
consequently can result in productive and economic losses
Determinação da razão ótima de espermatozóides por ovócitos de piabanha Brycon insignis (pisces - characidae)
Avaliação de pirogênios em produtos de uso veterinário pelos testes da hipertermia em coelhos e do lisado de amebócitos do Limulus
Desempenho, balanço e retenção de nutrientes e biometria dos órgãos digestivos de frangos de corte alimentados com diferentes níveis de proteína na ração pré-inicial
Modelagem matemática e difusividade efetiva das sementes de pinhão-manso (Jatropha curcas L.) durante a secagem
Open data from the third observing run of LIGO, Virgo, KAGRA, and GEO
The global network of gravitational-wave observatories now includes five detectors, namely LIGO Hanford, LIGO Livingston, Virgo, KAGRA, and GEO 600. These detectors collected data during their third observing run, O3, composed of three phases: O3a starting in 2019 April and lasting six months, O3b starting in 2019 November and lasting five months, and O3GK starting in 2020 April and lasting two weeks. In this paper we describe these data and various other science products that can be freely accessed through the Gravitational Wave Open Science Center at https://gwosc.org. The main data set, consisting of the gravitational-wave strain time series that contains the astrophysical signals, is released together with supporting data useful for their analysis and documentation, tutorials, as well as analysis software packages
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