509 research outputs found
On the formation of cyclones and anticyclones in a rotating fluid
It is commonly observed that the columnar vortices that dominate the large scales in homogeneous, rapidly rotating turbulence are predominantly cyclonic. This has prompted us to ask how this asymmetry arises. To provide a partial answer to this we look at the process of columnar vortex formation in a rotating fluid and, in particular, we examine how a localized region of swirl (an eddy) can convert itself into a columnar structure by inertial wave propagation. We show that, when the Rossby number (Ro) is small, the vortices evolve into columnar eddies through the radiation of linear inertial waves. When the Rossby number is large, on the other hand, no such column is formed. Rather, the eddy bursts radially outward under the action of the centrifugal force. There is no asymmetry between cyclonic and anticyclonic eddies for these two regimes. However, cyclones and anticyclones behave differently in the intermediate regime of Ro~1. Here we find that the transition from columnar vortex formation to radial bursting occurs at lower values of Ro for anticyclones, with the transition for anticyclones occurring at Ro~0.5, and that for cyclones at Ro~2. Thus, in a homogeneous turbulence experiment conducted at, say, Ro=1, we would expect to see more cyclones than anticyclones. The reason for this asymmetry at Ro~1 is explained
The decay of Batchelor and Saffman rotating turbulence
The decay rate of isotropic and homogeneous turbulence is known to be
affected by the large-scale spectrum of the initial perturbations, associated
with at least two cannonical self-preserving solutions of the von
K\'arm\'an-Howarth equation: the so-called Batchelor and Saffman spectra. The
effect of long-range correlations in the decay of anisotropic flows is less
clear, and recently it has been proposed that the decay rate of rotating
turbulence may be independent of the large-scale spectrum of the initial
perturbations. We analyze numerical simulations of freely decaying rotating
turbulence with initial energy spectra (Batchelor turbulence) and
(Saffman turbulence) and show that, while a self-similar decay
cannot be identified for the total energy, the decay is indeed affected by
long-range correlations. The decay of two-dimensional and three-dimensional
modes follows distinct power laws in each case, which are consistent with
predictions derived from the anisotropic von K\'arm\'an-Howarth equation, and
with conservation of anisotropic integral quantities by the flow evolution
The decay of turbulence in rotating flows
We present a parametric space study of the decay of turbulence in rotating
flows combining direct numerical simulations, large eddy simulations, and
phenomenological theory. Several cases are considered: (1) the effect of
varying the characteristic scale of the initial conditions when compared with
the size of the box, to mimic "bounded" and "unbounded" flows; (2) the effect
of helicity (correlation between the velocity and vorticity); (3) the effect of
Rossby and Reynolds numbers; and (4) the effect of anisotropy in the initial
conditions. Initial conditions include the Taylor-Green vortex, the
Arn'old-Beltrami-Childress flow, and random flows with large-scale energy
spectrum proportional to . The decay laws obtained in the simulations for
the energy, helicity, and enstrophy in each case can be explained with
phenomenological arguments that separate the decay of two-dimensional from
three-dimensional modes, and that take into account the role of helicity and
rotation in slowing down the energy decay. The time evolution of the energy
spectrum and development of anisotropies in the simulations are also discussed.
Finally, the effect of rotation and helicity in the skewness and kurtosis of
the flow is considered.Comment: Sections reordered to address comments by referee
Тоталітарні режими: ідеологічне обґрунтування цілей, форм і методів володарювання
Розглянуто теоретичні аспекти взаємовпливу ідеології та конкретно-історичних форм володарювання на прикладі фашизму і націонал-соціалізму. Проаналізована сутність праворадикальної ідеології, причини її виникнення, форми впливу та можливі загрози у контексті демократичного розвитку.The article researches the theoretical aspects of the mutual influence of an ideology and particular-historical forms of reigning on the Fascism's and the National-Socialism's example. The author analyzes the essence of right- radical ideology, the reasons of its appearance, forms of its influence as well as probable threats in the context of democratic development
Scale interactions and scaling laws in rotating flows at moderate Rossby numbers and large Reynolds numbers
The effect of rotation is considered to become important when the Rossby
number is sufficiently small, as is the case in many geophysical and
astrophysical flows. Here we present direct numerical simulations to study the
effect of rotation in flows with moderate Rossby numbers (down to Ro~0.1) but
at Reynolds numbers large enough to observe the beginning of a turbulent
scaling at scales smaller than the energy injection scale. We use coherent
forcing at intermediate scales, leaving enough room in the spectral space for
an inverse cascade of energy to also develop. We analyze the spectral behavior
of the simulations, the shell-to-shell energy transfer, scaling laws, and
intermittency, as well as the geometry of the structures in the flow. At late
times, the direct transfer of energy at small scales is mediated by
interactions with the largest scale in the system, the energy containing eddies
with k_perp~1, where "perp" refers to wavevectors perpendicular the axis of
rotation. The transfer between modes with wavevector parallel to the rotation
is strongly quenched. The inverse cascade of energy at scales larger than the
energy injection scale is non-local, and energy is transferred directly from
small scales to the largest available scale. Also, as time evolves and the
energy piles up at the large scales, the intermittency of the direct cascade of
energy is preserved while corrections due to intermittency are found to be the
same (within error bars) as in homogeneous turbulence.Comment: 12 pages, 16 figure
Identification of signaling pathways in early mammary gland development by mouse genetics
The mammary gland develops as an appendage of the ectoderm. The prenatal stage of mammary development is hormone independent and is regulated by sequential and reciprocal signaling between the epithelium and the mesenchyme. A number of recent studies using human and mouse genetics, in particular targeted gene deletion and transgenic expression, have identified some of the signals that control specific steps in development. This process involves cell specification and proliferation, reciprocal tissue interactions and cell migration. Since some of these events are recapitulated during tumorigenesis, an understanding of these signaling pathways may contribute to the development of targeted therapies and novel drugs
The interplay between helicity and rotation in turbulence: implications for scaling laws and small-scale dynamics
Invariance properties of physical systems govern their behavior: energy
conservation in turbulence drives a wide distribution of energy among modes,
observed in geophysical or astrophysical flows. In ideal hydrodynamics, the
role of helicity conservation (correlation between velocity and its curl,
measuring departures from mirror symmetry) remains unclear since it does not
alter the energy spectrum. However, with solid body rotation, significant
differences emerge between helical and non-helical flows. We first outline
several results, like the energy and helicity spectral distribution and the
breaking of strict universality for the individual spectra. Using massive
numerical simulations, we then show that small-scale structures and their
intermittency properties differ according to whether helicity is present or
not, in particular with respect to the emergence of Beltrami-core vortices
(BCV) that are laminar helical vertical updrafts. These results point to the
discovery of a small parameter besides the Rossby number; this could relate the
problem of rotating helical turbulence to that of critical phenomena, through
renormalization group and weak turbulence theory. This parameter can be
associated with the adimensionalized ratio of the energy to helicity flux to
small scales, the three-dimensional energy cascade being weak and self-similar
POMT2 mutations cause alpha-dystroglycan hypoglycosylation and Walker-Warburg syndrome
Background: Walker-Warburg syndrome (WWS) is an autosomal recessive condition characterised by congenital muscular dystrophy, structural brain defects, and eye malformations. Typical brain abnormalities are hydrocephalus, lissencephaly, agenesis of the corpus callosum, fusion of the hemispheres, cerebellar hypoplasia, and neuronal overmigration, which causes a cobblestone cortex. Ocular abnormalities include cataract, microphthalmia, buphthalmos, and Peters anomaly. WWS patients show defective O-glycosylation of α-dystroglycan (α-DG), which plays a key role in bridging the cytoskeleton of muscle and CNS cells with extracellular matrix proteins, important for muscle integrity and neuronal migration. In 20% of the WWS patients, hypoglycosylation results from mutations in either the protein O-mannosyltransferase 1 (POMT1), fukutin, or fukutin related protein (FKRP) genes. The other genes for this highly heterogeneous disorder remain to be identified. Objective: To look for mutations in POMT2 as a cause of WWS, as both POMT1 and POMT2 are required to achieve protein O-mannosyltransferase activity. Methods: A candidate gene approach combined with homozygosity mapping. Results: Homozygosity was found for the POMT2 locus at 14q24.3 in four of 11 consanguineous WWS families. Homozygous POMT2 mutations were present in two of these families as well as in one patient from another cohort of six WWS families. Immunohistochemistry in muscle showed severely reduced levels of glycosylated α-DG, which is consistent with the postulated role for POMT2 in the O-mannosylation pathway. Conclusions: A fourth causative gene for WWS was uncovered. These genes account for approximately one third of the WWS cases. Several more genes are anticipated, which are likely to play a role in glycosylation of α-DG
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