4,179 research outputs found

    Energy transfer in two-dimensional magnetohydrodynamic turbulence: formalism and numerical results

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    The basic entity of nonlinear interaction in Navier-Stokes and the Magnetohydrodynamic (MHD) equations is a wavenumber triad ({\bf k,p,q}) satisfying k+p+q=0{\bf k+p+q=0}. The expression for the combined energy transfer from two of these wavenumbers to the third wavenumber is known. In this paper we introduce the idea of an effective energy transfer between a pair of modes by the mediation of the third mode, and find an expression for it. Then we apply this formalism to compute the energy transfer in the quasi-steady-state of two-dimensional MHD turbulence with large-scale kinetic forcing. The computation of energy fluxes and the energy transfer between different wavenumber shells is done using the data generated by the pseudo-spectral direct numerical simulation. The picture of energy flux that emerges is quite complex---there is a forward cascade of magnetic energy, an inverse cascade of kinetic energy, a flux of energy from the kinetic to the magnetic field, and a reverse flux which transfers the energy back to the kinetic from the magnetic. The energy transfer between different wavenumber shells is also complex---local and nonlocal transfers often possess opposing features, i.e., energy transfer between some wavenumber shells occurs from kinetic to magnetic, and between other wavenumber shells this transfer is reversed. The net transfer of energy is from kinetic to magnetic. The results obtained from the studies of flux and shell-to-shell energy transfer are consistent with each other.Comment: 27 pages REVTEX; 14 ps figure

    Emission-line Intensities of the Hydrogen Atom

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    Hydrodynamical Gravity

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    Groups of Galaxies in Local Filamentary Structures

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    The Oscillations of an Incompressible Viscous Cylinder

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    巨大衝突により生じた周惑星円盤からの天王星の衛星形成

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    京都大学新制・課程博士博士(理学)甲第23007号理博第4684号新制||理||1672(附属図書館)京都大学大学院理学研究科物理学・宇宙物理学専攻(主査)教授 嶺重 慎, 准教授 前田 啓一, 教授 太田 耕司学位規則第4条第1項該当Doctor of ScienceKyoto UniversityDFA

    Calculation of renormalized viscosity and resistivity in magnetohydrodynamic turbulence

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    A self-consistent renormalization (RG) scheme has been applied to nonhelical magnetohydrodynamic turbulence with normalized cross helicity σc=0\sigma_c =0 and σc1\sigma_c \to 1. Kolmogorov's 5/3 powerlaw is assumed in order to compute the renormalized parameters. It has been shown that the RG fixed point is stable for ddc2.2d \ge d_c \approx 2.2. The renormalized viscosity ν\nu^* and resistivity η\eta^* have been calculated, and they are found to be positive for all parameter regimes. For σc=0\sigma_c=0 and large Alfv\'{e}n ratio (ratio of kinetic and magnetic energies) rAr_A, ν=0.36\nu^*=0.36 and η=0.85\eta^*=0.85. As rAr_A is decreased, ν\nu^* increases and η\eta^* decreases, untill rA0.25r_A \approx 0.25 where both ν\nu^* and η\eta^* are approximately zero. For large dd, both ν\nu^* and η\eta^* vary as d1/2d^{-1/2}. The renormalized parameters for the case σc1\sigma_c \to 1 are also reported.Comment: 19 pages REVTEX, 3 ps files (Phys. Plasmas, v8, 3945, 2001
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