关于磁流体力学激波稳定性理论的几个问题

本文讨论一类特殊的MHD激波的稳定性问题(或进化性问题),即此激波与二维斜入射小扰动波的相互作用问题。相当于推广气动力学激波的结果,过去的稳定性理论,即一维小扰动波与MHD激波相互作用的结果是,只有快激波与慢激波是稳定的,中间激波不稳定。本文的结果是:当小扰动波为Alfvén波时,得到与激波前后参数有关的新的稳定条件。当小扰动波为熵波与快、慢磁声波时,则稳定条件还与小扰动波的频率有关。并且作为一种极限情形,取垂直入射(反射、折射)时,快激波与慢激波都不稳定。本文计算还表明,一文的结论不能应用于激波稳定性理论。

The mechanism of energy storage by shearing the solar magnetic field

In this paper, a complete set of MHD equations have been solved by numerical calculations in an attempt to study the dynamical evolutionary processes of the initial equilibrium configuration and to discuss the energy storage mechanism of the solar atmosphere by shearing the magnetic field. The initial equilibrium configuration with an arch bipolar potential field obtained from the numerical solution is similar to the configuration in the vicinity of typical solar flare before its eruption. From the magnetic induction equation in the set of MHD equations and dealing with the non-linear coupling effects between the flow field and magnetic field, the quantitative relationship has been derived for their dynamical evolution. Results show that plasma shear motion at the bottom of the solar atmosphere causes the magnetic field to shear; meanwhile the magnetic field energy is stored in local regions. With the increase of time the local magnetic energy increases and it may reach an order of 4×10^25 J during a day. Thus the local storage of magnetic energy is large enough to trigger a big solar flare and can be considered as the energy source of solar flares. The energy storage mechanism by shearing the magnetic field can well explain the slow changes in solar active regions.

A hall dynamo model for the reversed field pinch

A mechanism for the reversed field pinch (RFP) dynamo is proposed, based on the nonlinear Hall effect of a saturated helical MHD instability. The sign and magnitude of the effect are shown to be those required for the RFP dynamo. Predictions of the model are in accord with RFP fluctuation measurements.

太阳风动量涨落激发磁层亚暴的机制

本文将太阳风涨落传输能量产生磁层亚暴的机制推广到无碰撞等离子体过程。太阳风的涨落在磁层顶激发压缩阿尔文波,并在磁尾的无碰撞等离子体中传播。尾瓣中满足条件β<<1,而等离子体片中β≥1,其中β为等离子体压力与磁压之比。这样,快磁声波在尾瓣中几乎不衰减,而在等离子体片中很快衰减,将波动能量耗散在等离子体片中使等离子体加热或者粒子加速。这种机制还表明,磁尾等离子体片中的高能粒子可以由太阳风涨落动能耗散而被加速,不一定是直接源于太阳。

Effects of Thermocapillary Convection on the Growth Process in Industrial 8-inch Silicon Czochralski Growth

Czochralski (CZ) crystal growth process is a widely used technique in manufacturing of silicon crystals and other semiconductor materials. The ultimate goal of the IC industry is to have the highest quality substrates, which are free of point defect, impurities and micro defect clusters. The scale up of silicon wafer size from 200 mm to 300 mm requires large crucible size and more heat power. Transport phenomena in crystal growth processes are quite complex due to melt and gas flows that may be oscillatory and/or turbulent, coupled convection and radiation, impurities and dopant distributions, unsteady kinetics of the growth process, melt crystal interface dynamics, free surface and meniscus, stoichiometry in the case of compound materials. A global model has been developed to simulate the temperature distribution and melt flow in an 8-inch system. The present program features the fluid convection, magnetohydrodynamics, and radiation models. A multi-zone method is used to divide the Cz system into different zones, e.g., the melt, the crystal and the hot zone. For calculation of temperature distribution, the whole system inside the stainless chamber is considered. For the convective flow, only the melt is considered. The widely used zonal method divides the surface of the radiation enclosure into a number of zones, which has a uniform distribution of temperature, radiative properties and composition. The integro-differential equations for the radiative heat transfer are solved using the matrix inversion technique. The zonal method for radiative heat transfer is used in the growth chamber, which is confined by crystal surface, melt surface, heat shield, and pull chamber. Free surface and crystal/melt interface are tracked using adaptive grid generation. The competition between the thermocapillary convection induced by non-uniform temperature distributions on the free surface and the forced convection by the rotation of the crystal determines the interface shape, dopant distribution, and striation pattern. The temperature gradients on the free surface are influenced by the effects of the thermocapillary force on the free surface and the rotation of the crystal and the crucible.

配置环形线电极的单极机中的磁流体力学流动

给出配置了环形线电极的单极机中的磁流体力学解析解.由于问题是线性的,求解可简化为基本解的叠加,可利用单极机在两个区域中的基本解的衔接来求得解析解.讨论了基本解的性质.利用非完全电极可改善Hartmann边界层、增加装置中的质量流量.应用基本解讨论了连续电极的单极机.

Magnetohydrodynamic turbulence

We simulate incompressible, MHD turbulence using a pseudo-spectral code. Our major conclusions are as follows.

1) MHD turbulence is most conveniently described in terms of counter propagating shear Alfvén and slow waves. Shear Alfvén waves control the cascade dynamics. Slow waves play a passive role and adopt the spectrum set by the shear Alfvén waves. Cascades composed entirely of shear Alfvén waves do not generate a significant measure of slow waves.

2) MHD turbulence is anisotropic with energy cascading more rapidly along k_⊥ than along k_∥, where k_⊥ and k_∥ refer to wavevector components perpendicular and parallel to the local magnetic field. Anisotropy increases with increasing k_⊥ such that excited modes are confined inside a cone bounded by k_∥ ∝ k^γ_⊥ where γ less than 1. The opening angle of the cone, θ(k_⊥) ∝ k^-(1-γ)_⊥, defines the scale dependent anisotropy.

3) MHD turbulence is generically strong in the sense that the waves which comprise it suffer order unity distortions on timescales comparable to their periods. Nevertheless, turbulent fluctuations are small deep inside the inertial range. Their energy density is less than that of the background field by a factor θ² (k_⊥)≪1.

4) MHD cascades are best understood geometrically. Wave packets suffer distortions as they move along magnetic field lines perturbed by counter propagating waves. Field lines perturbed by unidirectional waves map planes perpendicular to the local field into each other. Shear Alfvén waves are responsible for the mapping's shear and slow waves for its dilatation. The amplitude of the former exceeds that of the latter by 1/θ(k_⊥) which accounts for dominance of the shear Alfvén waves in controlling the cascade dynamics.

5) Passive scalars mixed by MHD turbulence adopt the same power spectrum as the velocity and magnetic field perturbations.

6) Decaying MHD turbulence is unstable to an increase of the imbalance between the flux of waves propagating in opposite directions along the magnetic field. Forced MHD turbulence displays order unity fluctuations with respect to the balanced state if excited at low k by δ(t) correlated forcing. It appears to be statistically stable to the unlimited growth of imbalance.

7) Gradients of the dynamic variables are focused into sheets aligned with the magnetic field whose thickness is comparable to the dissipation scale. Sheets formed by oppositely directed waves are uncorrelated. We suspect that these are vortex sheets which the mean magnetic field prevents from rolling up.

8) Items (1)-(5) lend support to the model of strong MHD turbulence put forth by Goldreich and Sridhar (1995, 1997). Results from our simulations are also consistent with the GS prediction γ = 2/3. The sole not able discrepancy is that the 1D power law spectra, E(k_⊥) ∝ k^-∝_⊥, determined from our simulations exhibit ∝ ≈ 3/2, whereas the GS model predicts ∝ = 5/3.

Experimental and theoretical studies of the electrothermal instability in a nonequilibrium plasma

Experimental and theoretical studies have been made of the electrothermal waves occurring in a nonequilibrium MHD plasma. These waves are caused by an instability that occurs when a plasma having a dependence of conductivity on current density is subjected to crossed electric and magnetic fields. Theoretically, these waves were studied by developing and solving the equations of a steady, one-dimensional nonuniformity in electron density. From these nonlinear equations, predictions of the maximum amplitude and of the half width of steady waves could be obtained. Experimentally, the waves were studied in a nonequilibrium discharge produced in a potassium-seeded argon plasma at 2000°K and 1 atm. pressure. The behavior of such a discharge with four different configurations of electrodes was determined from photographs, photomultiplier measurements, and voltage probes. These four configurations were chosen to produce steady waves, to check the stability of steady waves, and to observe the manifestation of the waves in a MHD generator or accelerator configuration.

Steady, one-dimensional waves were found to exist in a number of situations, and where they existed, their characteristics agreed with the predictions of the steady theory. Some extensions of this theory were necessary, however, to describe the transient phenomena occurring in the inlet region of a discharge transverse to the gas flow. It was also found that in a discharge away from the stabilizing effect of the electrodes, steady waves became unstable for large Hall parameters. Methods of prediction of the effective electrical conductivity and Hall parameter of a plasma with nonuniformities caused by the electrothermal waves were also studied. Using these methods and the values of amplitude predicted by the steady theory, it was found that the measured decrease in transverse conductivity of a MHD device, 50 per cent at a Hall parameter of 5, could be accounted for in terms of the electrothermal instability.

Sarcopenia em pacientes idosos com doença renal crônica em hemodiálise

Os pacientes idosos em hemodiálise (HD) são altamente suscetíveis ao desenvolvimento de sarcopenia, devido ao processo natural de envelhecimento e ao catabolismo induzido pelo procedimento de HD. O objetivo deste estudo foi primeiro, avaliar a prevalência de sarcopenia, dinapenia e atrofia muscular em um grupo de pacientes idosos em HD; o segundo, avaliar se os critérios aplicados para o diagnóstico de sarcopenia, propostos por sociedades internacionais, são capazes de distinguir os pacientes com pior condição clínica, estado nutricional e qualidade de vida. Este estudo multicêntrico e transversal incluiu 94 pacientes idosos em HD (> 60 anos) de cinco centros de diálise. Todos os participantes foram submetidos à avaliação antropométrica, de composição corporal, força de preensão manual (FPM), laboratorial e avaliação da condição nutricional através da avaliação subjetiva global de 7 pontos (AGS-7p). Adicionalmente, os participantes responderam um questionário de qualidade de vida. Para o diagnóstico de sarcopenia, foram adotados os critérios propostos por sociedades internacionais, que englobam os parâmetros indicativos de baixa massa muscular e baixa função muscular. Para a massa muscular adotou-se o índice de massa magra (IMM) < percentil 20 para o gênero e faixa etária de uma população de referência, avaliado a partir da massa magra obtida pelo somatório de dobras cutâneas. Para o critério de baixa função muscular, adotou-se a FPM < percentil 10 para o gênero, faixa etária e o braço utilizado de uma população de referência. Os pacientes foram classificados como Sarcopênicos (baixo IMM associado à baixa FPM); Dinapênicos (baixa FPM) e Atrofia muscular (baixo IMM). A sarcopenia estava presente em 13.8% dos pacientes, enquanto a dinapenia foi observada em 37.2% e a atrofia muscular em 35.1%. A sarcopenia foi capaz de distinguir os pacientes que possuíam maior comprometimento do estado nutricional e da composição corporal. O critério de função muscular (isoladamente ou em combinação com a massa muscular) também identificou os pacientes com pior qualidade de vida. Em conclusão, a prevalência de sarcopenia foi observada em 13,8% do grupo. Entretanto, ao usar apenas critérios que indicam redução da força ou massa muscular, esta prevalência aumentou para 30%. A condição de sarcopenia distinguiu pacientes com pior estado nutricional e qualidade de vida.

Do outro lado da linha do trem, havia uma pedra no meio do caminho: um estudo sobre crack no Rio de Janeiro na perspectiva da Teoria Ator-rede

O objetivo dessa pesquisa é discutir o cenário de uso de crack no município do Rio de Janeiro contextualizado com a condição de vulnerabilidade e risco social, através do mapeamento das controvérsias entre os atores dessa rede. As percepções e experiências relatadas neste trabalho dizem respeito aos diferentes espaços profissionais voltados ao atendimento e prestação de serviço a este público. Inicialmente, é trazida a trajetória teórica e prática que levaram a construção desta dissertação. Foram relatadas experiências vividas nas ações conjuntas de abordagem com a SMDS (Secretaria Municipal de Desenvolvimento Social) e a prática como entrevistadora de usuários de crack na Pesquisa Nacional do Crack pela FIOCRUZ. No segundo momento, é feito um breve histórico da origem do crack e suas marcas pelo mundo. São trazidos também, dados sobre a droga no Brasil, em particular sua história no Rio de Janeiro. Ainda nesta sequência, é apresentada a política de Redução de Danos, mostrando de que maneira o sujeito é significado a partir dessa perspectiva, e suas principais contribuições pelo mundo e também no país. A dissertação é construída pela perspectiva das práticas profissionais do psicólogo SMDS pensada através da Teoria Ator-rede. Foi importante destacar as principais ações de política pública voltadas para essa temática, considerando os avanços na discussão da temática. Foram mapeadas e exploradas as relações entre os atores envolvidos nesta temática (usuários de crack, SMDS, SMS Secretaria Municipal de Saúde, Segurança Pública, Mídia, Sociedade), colocando em evidencia as controvérsias existentes nessas relações, como recolhimento compulsório. De maneira conclusiva, são trazidas as impressões tiradas ao final deste percurso, problematizando os papéis do poder público e daqueles que atuam para garantir a população que faz uso abusivo de crack e outras drogas o direito de acessar e exercia sua cidadania.