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1A phenomenological treatment of rotating turbulence

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“A phenomenological treatment of rotating turbulence” Metadata:

  • Title: ➤  A phenomenological treatment of rotating turbulence
  • Author:
  • Language: English
  • Publisher: ➤  National Technical Information Service, distributor - Institute for Computer Applications in Science and Engineering, NASA Langley Research Center
  • Publish Date:
  • Publish Location: [Springfield, Va - Hampton, VA

“A phenomenological treatment of rotating turbulence” Subjects and Themes:

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Access and General Info:

  • First Year Published: 1995
  • Is Full Text Available: No
  • Is The Book Public: No
  • Access Status: No_ebook

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    Magnetohydrodynamic turbulence

    Magnetohydrodynamic turbulence concerns the chaotic regimes of magnetofluid flow at high Reynolds number. Magnetohydrodynamics (MHD) deals with what is

    Magnetohydrodynamic generator

    A magnetohydrodynamic generator (MHD generator) is a magnetohydrodynamic converter that transforms thermal energy and kinetic energy directly into electricity

    Magnetohydrodynamics

    meter Magnetohydrodynamic generator Magnetohydrodynamic turbulence Molten salt Plasma stability Shocks and discontinuities (magnetohydrodynamics) List

    List of textbooks in electromagnetism

    University, 1963. Biskamp D, Magnetohydrodynamic Turbulence, Cambridge University, 2003. Biskamp D, Nonlinear Magnetohydrodynamics, Cambridge University, 1993

    Computational magnetohydrodynamics

    physics and microwave heating of liquids. USim MACH2 STAR-CCM+ Magnetohydrodynamic turbulence Magnetic flow meter Plasma modeling Teyssier, R (2002). "Cosmological

    Blakesley Burkhart

    Maria Goeppert-Mayer Award. The awards both cited her work on magnetohydrodynamic turbulence, and for developing innovative techniques for comparing observable

    Magnetic helicity

    "Possibility of an inverse cascade of magnetic helicity in magnetohydrodynamic turbulence". Journal of Fluid Mechanics. 68 (4): 769–778. Bibcode:1975JFM

    Solar wind turbulence

    throughout the heliosphere. Solar wind turbulence displays both magnetohydrodynamic (MHD) and kinetic plasma behaviors. It exhibits Kolmogorov-like power

    Hannes Alfvén

    physicist and winner of the 1970 Nobel Prize in Physics for his work on magnetohydrodynamics (MHD). He described the class of MHD waves now known as Alfvén waves

    Magnetic reconnection

    component arising because of turbulence. For the turbulent flow in the reconnection region, a model for magnetohydrodynamic turbulence should be used such as