1,541 research outputs found

    Nonlinear parity mixtures controlling the propagation of interchange modes

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    The propagation velocity of a resistive interchange mode is numerically investigated based on a two-fluid model. It is newly found that the nonlinearity mixes the interchange parity and the tearing parity to produce magnetic islands and controls the propagation velocity of the instability in the poloidal direction. The parity of the interchange mode is conserved during the linear growing evolution. However, when the amplitude of the mode becomes large and nonlinear effects are dominant, the pure interchange mode does not satisfy the nonlinear two-fluid equation. Thus, the nonlinear energy transfer occurs from the interchange parity mode to the tearing parity mode, which is called the nonlinear parity mixtures, and the magnetic islands are produced by the interchange mode. The nonlinear magnetic island formation by the interchange mode plays a central role in controlling the interchange mode's propagation velocity, which is equal to the electron fluid velocity. This nonlinear process is essential in quantitatively reproducing the propagation velocity of the interchange mode, which is the same as the electron fluid velocity observed in the large helical device experiment. It is also found that one of the mechanisms of parity mixtures is a modulational instability

    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

    Starbursts in multiple galaxy mergers

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    We numerically investigate stellar and gaseous dynamical evolution of mergers between five identical late-type disk galaxies with the special emphasis on star formation history and chemical evolution of multiple galaxy mergers. We found that multiple encounter and merging can trigger repetitive massive starbursts (typically \sim 100 MM_{\odot} yr1{\rm yr}^{-1}) owing to the strong tidal disturbance and the resultant gaseous dissipation during merging. The magnitude of the starburst is found to depend on initial virial ratio (i.e., the ratio of total kinematical energy to total potential energy) such that the maximum star formation rate is larger for the merger with smaller virial ratio. Furthermore we found that the time interval between the epochs of the triggered starbursts is longer for the merger with the larger virial ratio. The remnant of a multiple galaxy merger with massive starbursts is found to have metal-poor gaseous halo that is formed by tidal stripping during the merging. We accordingly suggest that metal-poor gaseous halo in a field elliptical galaxy is a fossil record of the past multiple merging events for the galaxy.Comment: 23 pages 16 figures,2000,ApJ,545 in press. For all ps figures, see http://newt.phys.unsw.edu.au/~bekki/res.dir/paper.dir/mul.dir/fig.tar.g

    Indocyanine green fluorescence imaging in colorectal surgery: overview, applications, and future directions

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    Indocyanine green fluorescence imaging is a surgical tool with increasing applications in colorectal surgery. This tool has received acceptance in various surgical disciplines as a potential method to enhance surgical field visualisation, improve lymph node retrieval, and decrease the incidence of anastomotic leaks. In colorectal surgery specifically, small studies have shown that intraoperative fluorescence imaging is a safe and feasible method to assess anastomotic perfusion, and its use might affect the incidence of anastomotic leaks. Controlled trials are ongoing to validate these conclusions. The number of new indications for indocyanine green continues to increase, including innovative options for detecting and guiding management of colorectal metastasis to the liver. These advances could offer great value for surgeons and patients, by improving the accuracy and outcomes of oncological resections

    Multi-Scale Interactions of Microtearing Turbulence in the Tokamak Pedestal

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    Microtearing turbulence in an idealized pedestal scenario is found to saturate via zonal fields, while also exciting strong zonal flows; a concurrent upshift of the non-linear critical gradient is observed. The zonal flows cause electron-temperature-gradient-driven turbulence to be ameliorated. When applying resonant magnetic perturbations, the prompt charge loss off the flux surface erodes the zonal flow, leading to higher electron-scale fluxes, while leaving microtearing saturation physics unaffected.</p

    Influence of transport and ocean ice extent on biogenic aerosol sulfur in the Arctic atmosphere

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    The recent decline in sea ice cover in the Arctic Ocean could affect the regional radiative forcing via changes in sea ice-atmosphere exchange of dimethyl sulfide (DMS) and biogenic aerosols formed from its atmospheric oxidation, such as methanesulfonic acid (MSA). This study examines relationships between changes in total sea ice extent north of 70 degrees N and atmospheric MSA measurement at Alert, Nunavut, during 1980-2009; at Barrow, Alaska, during 1997-2008; and at Ny-Alesund, Svalbard, for 1991-2004. During the 1980-1989 and 1990-1997 periods, summer (July-August) and June MSA concentrations at Alert decreased. In general, MSA concentrations increased at all locations since 2000 with respect to 1990 values, specifically during June and summer at Alert and in summer at Barrow and Ny-Alesund. Our results show variability in MSA at all sites is related to changes in the source strengths of DMS, possibly linked to changes in sea ice extent as well as to changes in atmospheric transport patterns. Since 2000, a late spring increase in atmospheric MSA at the three sites coincides with the northward migration of the marginal ice edge zone where high DMS emissions from ocean to atmosphere have previously been reported. Significant negative correlations are found between sea ice extent and MSA concentrations at the three sites during the spring and June. These results suggest that a decrease in seasonal ice cover influencing other mechanisms of DMS production could lead to higher atmospheric MSA concentrations

    Effect of the curvature and the {\beta} parameter on the nonlinear dynamics of a drift tearing magnetic island

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    We present numerical simulation studies of 2D reduced MHD equations investigating the impact of the electronic \beta parameter and of curvature effects on the nonlinear evolution of drift tearing islands. We observe a bifurcation phenomenon that leads to an amplification of the pressure energy, the generation of E \times B poloidal flow and a nonlinear diamagnetic drift that affects the rotation of the magnetic island. These dynamical modifications arise due to quasilinear effects that generate a zonal flow at the onset point of the bifurcation. Our simulations show that the transition point is influenced by the \beta parameter such that the pressure gradient through a curvature effect strongly stabilizes the transition. Regarding the modified rotation of the island, a model for the frequency is derived in order to study its origin and the effect of the \beta parameter. It appears that after the transition, an E \times B poloidal flow as well as a nonlinear diamagnetic drift are generated due to an amplification of the stresses by pressure effects
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