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Relevant bibliographies by topics / Magneto-hydro-dynamic turbulence

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Academic literature on the topic 'Magneto-hydro-dynamic turbulence'

Author: Grafiati

Published: 14 March 2023

Last updated: 31 July 2025

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Journal articles on the topic "Magneto-hydro-dynamic turbulence"

1

Materassi, M., and G. Consolini. "Turning the resistive MHD into a stochastic field theory." Nonlinear Processes in Geophysics 15, no. 4 (2008): 701–9. http://dx.doi.org/10.5194/npg-15-701-2008.

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Abstract. Classical systems stirred by random forces of given statistics may be described via a path integral formulation in which their degrees of freedom are stochastic variables themselves, undergoing a multiple-history probabilistic evolution. This framework seems to be easily applicable to resistive Magneto-Hydro-Dynamics (MHD). Indeed, MHD equations form a dynamic system of classical variables in which the terms representing the density, the pressure and the conductivity of the plasma are irregular functions of space and time when turbulence occurs. By treating those irregular terms as r

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2

Becoulet, M., G. T. A. Huijsmans, C. Passeron, et al. "Non-linear MHD modelling of edge localized modes suppression by resonant magnetic perturbations in ITER." Nuclear Fusion 62, no. 6 (2022): 066022. http://dx.doi.org/10.1088/1741-4326/ac47af.

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Abstract Edge localized modes (ELMs) suppression by resonant magnetic perturbations (RMPs) was studied with the non-linear magneto-hydro-dynamic (MHD) code JOREK for the ITER H-mode scenarios at 15 MA, 12.5 MA, 10 MA/5.3 T. The main aim of this work was to demonstrate that ELMs can be suppressed by RMPs while the divertor 3D footprints of heat and particle fluxes remain within divertor material limits. The unstable peeling–ballooning modes responsible for ELMs without RMPs were modelled first for each scenario using numerically accessible parameters for ITER. Then the stabilization of ELMs by

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Park, Hyeon K., Minjun J. Choi, Minho Kim, et al. "Advances in physics of the magneto-hydro-dynamic and turbulence-based instabilities in toroidal plasmas via 2-D/3-D visualization." Reviews of Modern Plasma Physics 6, no. 1 (2022). http://dx.doi.org/10.1007/s41614-022-00076-2.

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4

Zhang, Boya, Junwei Deng, Sunsiqin Wang, et al. "Thermodynamic, transport, and radiation properties of HFO-1336mzz(E) mixtures as eco-friendly SF6 alternatives." Journal of Physics D: Applied Physics, July 19, 2023. http://dx.doi.org/10.1088/1361-6463/ace8a5.

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Abstract HFO-1336mzz(E) is proposed as a novel alternative to SF6 due to its low greenhouse effect and high insulation strength. Typically, it is mixed with CO2 or Air to lower its boiling point to meet the minimum operating temperature. To better understand the thermophysical properties of the gases’ arcing plasma, the composition, thermodynamic properties, transport properties, and net emission coefficient of 30% molar fraction of HFO-1336mzz(E) mixed with CO2 or Air at temperatures from 300 K to 30000 K at 0.12 MPa are calculated. It is found that HFO-1336mzz(E) mixtures have similar turbul

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Dissertations / Theses on the topic "Magneto-hydro-dynamic turbulence"

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Fornieri, Ottavio. "Cosmic-ray transport in the Milky Way and related phenomenology." Doctoral thesis, Università di Siena, 2021. http://hdl.handle.net/11365/1143115.

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In this thesis, we aim at studying some of the open questions regarding the origin of the "Cosmic Rays" (CRs), as well as their transport properties. The exceptional quality of the experimentally measured cosmic-ray observables, especially at the recently-achieved energies in the range ~O(100 GeV - 1 TeV), started to question the standard picture, based on a "Supernova Remnant"-(SNR)-only origin of the CRs and a diffusive propagation inspired by the "Quasi-Linear Theory" (QLT) of pitch-angle interaction against alfvénic turbulence. First, we reproduce the most relevant cosmic-ray obser

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