41 research outputs found
A study investigating the comparative effects of an audiation pause in tonal pattern training on fourth and fifth grade children
The purpose of this study is to examine variations of response time in tonal pattern training. The problem of the study is twofold. 1) To determine the comparative effect of fourth and fifth grade students who echoed tonal patterns immediately and students who echoed after a pause, and 2) to examine how the variations in response time in tonal pattern training effects the performance of high and low aptitude students.
The sample for this study consisted of approximately 140 fourth and fifth grade students who attended an elementary school located in a Southern New Jersey suburban community. The sample included six intact classes, each class randomly assigned to the treatment group and the control group. All six classes received music instruction once a week for 40 minutes from the investigator.
The Intermediate Measures of Music Audiation (IMMA) was administered to all students during regularly scheduled music classes prior to the beginning of the tonal pattern instruction to determine each student\u27s level of musical aptitude. During the ten weeks of instruction, the subjects participated in tonal pattern training during their regularly scheduled music class singing tonic and dominant tonal patterns in major and minor, first at the aural/oral level and then at the verbal association level.
At the end of the period, students were tested individually on their singing achievement of tonal patterns. Within two weeks of the completion of the tonal training, students were tape-recorded singing familiar and unfamiliar tonal patterns on the neutral syllable bum in major and minor. Two judges were trained to evaluate the student performances using a criterion-referenced tonal rating scale.
The interjudge reliability between judges was calculated at .915. No statistically significant differences were found for either the interaction or main effect for the treatment. As expected, however, a main effect for aptitude was confirmed through statistical analysis. Based on the evidence acquired from this study, it cannot be concluded that variations of response time in tonal pattern training is a necessary component for learning theory pedagogy
Mode-coupling and nonlinear Landau damping effects in auroral Farley-Buneman turbulence
The fundamental problem of Farley-Buneman turbulence in the auroral
-region has been discussed and debated extensively in the past two decades.
In the present paper we intend to clarify the different steps that the auroral
-region plasma has to undergo before reaching a steady state. The
mode-coupling calculation, for Farley-Buneman turbulence, is developed in order
to place it in perspective and to estimate its magnitude relative to the
anomalous effects which arise through the nonlinear wave-particle interaction.
This nonlinear effect, known as nonlinear ``Landau damping'' is due to the
coupling of waves which produces other waves which in turn lose energy to the
bulk of the particles by Landau damping. This leads to a decay of the wave
energy and consequently a heating of the plasma. An equation governing the
evolution of the field spectrum is derived and a physical interpration for each
of its terms is provided
Zonal flow and zonal magnetic field generation by finite Ξ² drift waves: a theory for low to high transitions in tokamaks
The understanding of low to high (L-H) transition in tokamaks has been an important area of investigation for more than a decade. Recent 3D finite Ξ² simulations of drift-resistive ballooning modes in a flux tube geometry by Rogers et al. [Phys. Rev. Lett. 81, 4396 (1998)] have provided a unique parametrization of the transition in a two-dimensional phase space. Comparison of the threshold curve in this phase space with data from ASDEX and C-MOD has shown very good agreement. In this Letter we provide a simple theory, based on the generation of zonal flow and zonal magnetic field in a finite-beta plasma, which explains this threshold curve for L-H transition in tokamaks
ΠΡΠΎΠ±Π΅Π½Π½ΠΎΡΡΠΈ ΡΠ°ΡΡΠ΅ΡΠ° ΡΠΊΠΎΠ½ΠΎΠΌΠΈΡΠ΅ΡΠΊΠΈΡ ΠΏΠΎΠΊΠ°Π·Π°ΡΠ΅Π»Π΅ΠΉ Π²ΡΡΠΎΠΊΠΎΡΠΊΠΎΡΠΎΡΡΠ½ΡΡ Π»ΠΎΡΠΌΠ°Π½ΡΠΊΠΈΡ ΠΊΠ°ΡΠ΅ΡΠΎΠ² Π½Π° ΡΡΠ°ΠΏΠ΅ ΠΊΠΎΠ½ΡΠ΅ΠΏΡΡΠ°Π»ΡΠ½ΠΎΠ³ΠΎ ΠΏΡΠΎΠ΅ΠΊΡΠΈΡΠΎΠ²Π°Π½ΠΈΡ
ΠΠ»Π΅Π²Π°, Π―. Π. ΠΡΠΎΠ±Π΅Π½Π½ΠΎΡΡΠΈ ΡΠ°ΡΡΠ΅ΡΠ° ΡΠΊΠΎΠ½ΠΎΠΌΠΈΡΠ΅ΡΠΊΠΈΡ
ΠΏΠΎΠΊΠ°Π·Π°ΡΠ΅Π»Π΅ΠΉ Π²ΡΡΠΎΠΊΠΎΡΠΊΠΎΡΠΎΡΡΠ½ΡΡ
Π»ΠΎΡΠΌΠ°Π½ΡΠΊΠΈΡ
ΠΊΠ°ΡΠ΅ΡΠΎΠ² Π½Π° ΡΡΠ°ΠΏΠ΅ ΠΊΠΎΠ½ΡΠ΅ΠΏΡΡΠ°Π»ΡΠ½ΠΎΠ³ΠΎ ΠΏΡΠΎΠ΅ΠΊΡΠΈΡΠΎΠ²Π°Π½ΠΈΡ = Features of economic indicators calculation for high speed pilot boat on stage of conceptual design / Π―. Π. ΠΠ»Π΅Π²Π° // ΠΠ±. Π½Π°ΡΠΊ. ΠΏΡ. ΠΠ£Π. β ΠΠΈΠΊΠΎΠ»Π°ΡΠ² : ΠΠ£Π, 2016. β β 4 (466). β Π‘. 22β27.ΠΠ°Π»Π΅ΠΆΠ½ΠΎΡΡΡ Π΄Π»Ρ ΡΠΎΠ·ΡΠ°Ρ
ΡΠ½ΠΊΡ ΠΎΡΠ½ΠΎΠ²Π½ΠΈΡ
Π΅ΠΊΠΎΠ½ΠΎΠΌΡΡΠ½ΠΈΡ
ΠΏΠΎΠΊΠ°Π·Π½ΠΈΠΊΡΠ² ΡΠΎΠ·Π³Π»ΡΠ½ΡΡΡ Π· Π²ΡΠ°Ρ
ΡΠ²Π°Π½Π½ΡΠΌ ΡΠΏΠ΅ΡΠΈΡΡΠΊΠΈ Π΅ΠΊΡΠΏΠ»ΡΠ°ΡΠ°ΡΡΡ ΡΠ²ΠΈΠ΄ΠΊΡΡΠ½ΠΈΡ
Π»ΠΎΡΠΌΠ°Π½ΡΡΠΊΠΈΡ
ΠΊΠ°ΡΠ΅ΡΡΠ². Π€ΠΎΡΠΌΡΠ»ΠΈ, ΡΠΎ ΠΏΡΠΎΠΏΠΎΠ½ΡΡΡΡΡΡ, ΠΌΠΎΠΆΡΡΡ Π²ΠΈΠΊΠΎΡΠΈΡΡΠΎΠ²ΡΠ²Π°ΡΠΈΡΡ Π΄Π»Ρ Π²ΠΈΡΡΡΠ΅Π½Π½Ρ Π·Π°Π΄Π°Ρ Π²ΠΈΠ±ΠΎΡΡ ΠΎΠΏΡΠΈΠΌΠ°Π»ΡΠ½ΠΈΡ
Ρ
Π°ΡΠ°ΠΊΡΠ΅ΡΠΈΡΡΠΈΠΊ Π»ΠΎΡΠΌΠ°Π½ΡΡΠΊΠΎΠ³ΠΎ ΠΊΠ°ΡΠ΅ΡΠ°.During the last decades a vast amount of research has been focused on the issues of design, operations, and development of more optimized structures of high-speed craft. The right choice of the criterion function is crucial. Fundamentally, efficiency can be increased with the reduction of production costs, operational costs, and environmental impact, while maintaining or improving craft performance, reliability, and safety. The estimation of economic performances of pilot boats in conceptual design phase should account for many features, such as, different building materials, development of the hull design, choice of the propeller, conditions of operations, and others. The majority of estimation techniques are developed specifically for large ships and, therefore, do not take into account the essential features of design and function of small high-speed craft, namely, pilot boats. Πn this paper we present formulas for estimation of building cost of the conventional pilot boat (a monohull). The author recommends the set of formulas for estimation, which form the mathematical model. These equations can be used in the optimization task.ΠΡΠ΅Π΄ΡΡΠ°Π²Π»Π΅Π½Ρ Π·Π°Π²ΠΈΡΠΈΠΌΠΎΡΡΠΈ Π΄Π»Ρ ΡΠ°ΡΡΠ΅ΡΠ° ΠΎΡΠ½ΠΎΠ²Π½ΡΡ
ΡΠΊΠΎΠ½ΠΎΠΌΠΈΡΠ΅ΡΠΊΠΈΡ
ΠΏΠΎΠΊΠ°Π·Π°ΡΠ΅Π»Π΅ΠΉ Ρ ΡΡΠ΅ΡΠΎΠΌ ΡΠΏΠ΅ΡΠΈΡΠΈΠΊΠΈ ΠΏΡΠΎΠ΅ΠΊΡΠΈΡΠΎΠ²Π°Π½ΠΈΡ ΠΈ ΡΠΊΡΠΏΠ»ΡΠ°ΡΠ°ΡΠΈΠΈ Π²ΡΡΠΎΠΊΠΎΡΠΊΠΎΡΠΎΡΡΠ½ΡΡ
Π»ΠΎΡΠΌΠ°Π½ΡΠΊΠΈΡ
ΠΊΠ°ΡΠ΅ΡΠΎΠ². ΠΠΎΠ»ΡΡΠ΅Π½Π½ΡΠ΅ ΡΠΎΡΠΌΡΠ»Ρ ΠΌΠΎΠ³ΡΡ Π±ΡΡΡ ΠΈΡΠΏΠΎΠ»ΡΠ·ΠΎΠ²Π°Π½Ρ ΠΏΡΠΈ ΡΠ΅ΡΠ΅Π½ΠΈΠΈ Π·Π°Π΄Π°ΡΠΈ Π²ΡΠ±ΠΎΡΠ° ΠΎΠΏΡΠΈΠΌΠ°Π»ΡΠ½ΡΡ
Ρ
Π°ΡΠ°ΠΊΡΠ΅ΡΠΈΡΡΠΈΠΊ Π»ΠΎΡΠΌΠ°Π½ΡΠΊΠΎΠ³ΠΎ ΠΊΠ°ΡΠ΅ΡΠ°
Statistical properties of driven Magnetohydrodynamic turbulence in three dimensions: Novel universality
We analyse the universal properties of nonequilibrium steady states of driven
Magnetohydrodynamic (MHD) turbulence in three dimensions (3d). We elucidate the
dependence of various phenomenologically important dimensionless constants on
the symmetries of the two-point correlation functions. We, for the first time,
also suggest the intriguing possibility of multiscaling universality class
varying continuously with certain dimensionless parameters. The experimental
and theoretical implications of our results are discussed.Comment: To appear in Europhys. Lett. (2004
High resolution temperature and density profiles during the energy quench of density limit disruptions in Rijnhuizen tokamak project
Measurements of the electron temperature, Te, and density, ne, during the energy quench of a major disruption showed that the onset of Te erosion in the neighborhood of the m/n = 2/1 O point at the low field side (LFS) accelerates the well-known m/n = 1/1 erosion of the core temperature. During this phase Te(r) is only partially flat in the region between the q = 2 and the q = 1 surfaces and ne(r) decreases in the core and increases inside the m/n = 2/1 island. Immediately after the flattening of Te(r) a large peak in Te and to a lesser extent in ne has been observed. This peak is radially localized at the q = 2 radius at the LFS, is very short lived and is poloidally asymmetric. Te profiles measured by the heterodyne radiometer and the Thomson scattering agree very well up to the time Te(r) flattens but afterwards can be a factor of two different
Diamagnetic Suppression of Component Magnetic Reconnection at the Magnetopause
We present particle-in-cell simulations of collisionless magnetic
reconnection in a system (like the magnetopause) with a large density asymmetry
across the current layer. In the presence of an ambient component of the
magnetic field perpendicular to the reconnection plane the gradient creates a
diamagnetic drift that advects the X-line with the electron diamagnetic
velocity. When the relative drift between the ions and electrons is of the
order the Alfven speed the large scale outflows from the X-line necessary for
fast reconnection cannot develop and the reconnection is suppressed. We discuss
how these effects vary with both the plasma beta and the shear angle of the
reconnecting field and discuss observational evidence for diamagnetic
stabilization at the magnetopause.Comment: 10 pages, 10 figures; accepted by JGR; agu2001.cls and agu.bst
include
Magnetic Reconnection in Extreme Astrophysical Environments
Magnetic reconnection is a basic plasma process of dramatic rearrangement of
magnetic topology, often leading to a violent release of magnetic energy. It is
important in magnetic fusion and in space and solar physics --- areas that have
so far provided the context for most of reconnection research. Importantly,
these environments consist just of electrons and ions and the dissipated energy
always stays with the plasma. In contrast, in this paper I introduce a new
direction of research, motivated by several important problems in high-energy
astrophysics --- reconnection in high energy density (HED) radiative plasmas,
where radiation pressure and radiative cooling become dominant factors in the
pressure and energy balance. I identify the key processes distinguishing HED
reconnection: special-relativistic effects; radiative effects (radiative
cooling, radiation pressure, and Compton resistivity); and, at the most extreme
end, QED effects, including pair creation. I then discuss the main
astrophysical applications --- situations with magnetar-strength fields
(exceeding the quantum critical field of about 4 x 10^13 G): giant SGR flares
and magnetically-powered central engines and jets of GRBs. Here, magnetic
energy density is so high that its dissipation heats the plasma to MeV
temperatures. Electron-positron pairs are then copiously produced, making the
reconnection layer highly collisional and dressing it in a thick pair coat that
traps radiation. The pressure is dominated by radiation and pairs. Yet,
radiation diffusion across the layer may be faster than the global Alfv\'en
transit time; then, radiative cooling governs the thermodynamics and
reconnection becomes a radiative transfer problem, greatly affected by the
ultra-strong magnetic field. This overall picture is very different from our
traditional picture of reconnection and thus represents a new frontier in
reconnection research.Comment: Accepted to Space Science Reviews (special issue on magnetic
reconnection). Article is based on an invited review talk at the
Yosemite-2010 Workshop on Magnetic Reconnection (Yosemite NP, CA, USA;
February 8-12, 2010). 30 pages, no figure
Natural Killer Cells from Patients with Recombinase-Activating Gene and Non-Homologous End Joining Gene Defects Comprise a Higher Frequency of CD56bright NKG2A+++ Cells, and Yet Display Increased Degranulation and Higher Perforin Content.
Mutations of the recombinase Activating Genes 1 and 2 (RAG1, RAG2) in humans are associated with a broad range of phenotypes. For patients with severe clinical presentation, hematopoietic stem cell transplantation (HSCT) represents the only curative treatment, however high rates of graft failure and incomplete immune reconstitution have been observed, especially after unconditioned haploidentical transplantation. Studies in mice have shown that Rag-/- NK cells have a mature phenotype, reduced fitness and increased cytotoxicity. We aimed to analyze NK cell phenotype and function in patients with mutations in RAG and in non-homologous end joining (NHEJ) genes. Here we provide evidence that NK cells from these patients have an immature phenotype, with significant expansion of CD56bright CD16-/int CD57- cells, yet increased degranulation and high perforin content. Correlation was observed between in vitro recombinase activity of the mutant proteins, NK cell abnormalities, and in vivo clinical phenotype. Addition of serotherapy in the conditioning regimen, with the aim of depleting the autologous NK cell compartment, may be important to facilitate engraftment and immune reconstitution in patients with RAG and NHEJ defects treated by HSCT
ΠΡΠΎΠ±Π»ΠΈΠ²ΠΎΡΡΡ ΡΠΎΠ·ΡΠ°Ρ ΡΠ½ΠΊΡ Π΅ΠΊΠΎΠ½ΠΎΠΌΡΡΠ½ΠΈΡ ΠΏΠΎΠΊΠ°Π·Π½ΠΈΠΊΡΠ² Π²ΠΈΡΠΎΠΊΠΎΡΠ²ΠΈΠ΄ΠΊΡΡΠ½ΠΈΡ Π»ΠΎΡΠΌΠ°Π½ΡΡΠΊΠΈΡ ΠΊΠ°ΡΠ΅ΡΡΠ² Π½Π° Π΅ΡΠ°ΠΏΡ ΠΊΠΎΠ½ΡΠ΅ΠΏΡΡΠ°Π»ΡΠ½ΠΎΠ³ΠΎ ΠΏΡΠΎΠ΅ΠΊΡΡΠ²Π°Π½Π½Ρ
During the last decades a vast amount of research has been focused on the issues of design, operations, and development of more optimized structures of high-speed craft. The right choice of the criterion function is crucial. Fundamentally, efficiency can be increased with the reduction of production costs, operational costs, and environmental impact, while maintaining or improving craft performance, reliability, and safety. The estimation of economic performances of pilot boats in conceptual design phase should account for many features, such as, different building materials, development of the hull design, choice of the propeller, conditions of operations, and others. The majority of estimation techniques are developed specifically for large ships and, therefore, do not take into account the essential features of design and function of small high-speed craft, namely, pilot boats. Πn this paper we present formulas for estimation of building cost of the conventional pilot boat (a monohull). The author recommends the set of formulas for estimation, which form the mathematical model. These equations can be used in the optimizationtask.ΠΡΠ΅Π΄ΡΡΠ°Π²Π»Π΅Π½Ρ Π·Π°Π²ΠΈΡΠΈΠΌΠΎΡΡΠΈ Π΄Π»Ρ ΡΠ°ΡΡΠ΅ΡΠ° ΠΎΡΠ½ΠΎΠ²Π½ΡΡ
ΡΠΊΠΎΠ½ΠΎΠΌΠΈΡΠ΅ΡΠΊΠΈΡ
ΠΏΠΎΠΊΠ°Π·Π°ΡΠ΅Π»Π΅ΠΉ Ρ ΡΡΠ΅ΡΠΎΠΌ ΡΠΏΠ΅ΡΠΈΡΠΈΠΊΠΈ ΠΏΡΠΎΠ΅ΠΊΡΠΈΡΠΎΠ²Π°Π½ΠΈΡ ΠΈ ΡΠΊΡΠΏΠ»ΡΠ°ΡΠ°ΡΠΈΠΈ Π²ΡΡΠΎΠΊΠΎΡΠΊΠΎΡΠΎΡΡΠ½ΡΡ
Π»ΠΎΡΠΌΠ°Π½ΡΠΊΠΈΡ
ΠΊΠ°ΡΠ΅ΡΠΎΠ². ΠΠΎΠ»ΡΡΠ΅Π½Π½ΡΠ΅ ΡΠΎΡΠΌΡΠ»Ρ ΠΌΠΎΠ³ΡΡ Π±ΡΡΡ ΠΈΡΠΏΠΎΠ»ΡΠ·ΠΎΠ²Π°Π½Ρ ΠΏΡΠΈ ΡΠ΅ΡΠ΅Π½ΠΈΠΈ Π·Π°Π΄Π°ΡΠΈ Π²ΡΠ±ΠΎΡΠ° ΠΎΠΏΡΠΈΠΌΠ°Π»ΡΠ½ΡΡ
Ρ
Π°ΡΠ°ΠΊΡΠ΅ΡΠΈΡΡΠΈΠΊ Π»ΠΎΡΠΌΠ°Π½ΡΠΊΠΎΠ³ΠΎ ΠΊΠ°ΡΠ΅ΡΠ°.ΠΠ°Π»Π΅ΠΆΠ½ΠΎΡΡΡ Π΄Π»Ρ ΡΠΎΠ·ΡΠ°Ρ
ΡΠ½ΠΊΡ ΠΎΡΠ½ΠΎΠ²Π½ΠΈΡ
Π΅ΠΊΠΎΠ½ΠΎΠΌΡΡΠ½ΠΈΡ
ΠΏΠΎΠΊΠ°Π·Π½ΠΈΠΊΡΠ² ΡΠΎΠ·Π³Π»ΡΠ½ΡΡΡ Π· Π²ΡΠ°Ρ
ΡΠ²Π°Π½Π½ΡΠΌ ΡΠΏΠ΅ΡΠΈΡΡΠΊΠΈ Π΅ΠΊΡΠΏΠ»ΡΠ°ΡΠ°ΡΡΡ ΡΠ²ΠΈΠ΄ΠΊΡΡΠ½ΠΈΡ
Π»ΠΎΡΠΌΠ°Π½ΡΡΠΊΠΈΡ
ΠΊΠ°ΡΠ΅ΡΡΠ². Π€ΠΎΡΠΌΡΠ»ΠΈ, ΡΠΎ ΠΏΡΠΎΠΏΠΎΠ½ΡΡΡΡΡΡ, ΠΌΠΎΠΆΡΡΡ Π²ΠΈΠΊΠΎΡΠΈΡΡΠΎΠ²ΡΠ²Π°ΡΠΈΡΡ Π΄Π»Ρ Π²ΠΈΡΡΡΠ΅Π½Π½Ρ Π·Π°Π΄Π°Ρ Π²ΠΈΠ±ΠΎΡΡ ΠΎΠΏΡΠΈΠΌΠ°Π»ΡΠ½ΠΈΡ
Ρ
Π°ΡΠ°ΠΊΡΠ΅ΡΠΈΡΡΠΈΠΊ Π»ΠΎΡΠΌΠ°Π½ΡΡΠΊΠΎΠ³ΠΎ ΠΊΠ°ΡΠ΅ΡΠ°