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Showing 1 to 7 of 7 for “"dynamo theory"”.

  1. Cio-cio-san no yuutsu: memoirs of magnetogenesis and turbulent dynamo theory

    … and density. The dependence of the onset of dynamo action on various values of the magnetic Reynolds- and Prandtl numbers for the cases of the Roberts Flow kinematic dynamo and a flow that, in turn, incorporates both a non-helical and helical forcing function that introduces turbulence into …

    cape-town Repository record for Cio-cio-san no yuutsu: memoirs of magnetogenesis and turbulent dynamo theory (opens in a new tab)

  2. Cio-cio-san no Yūutsu: memoirs of magnetogenesis and Turbulent Dynamo Theory

    … and density. The dependence of the onset of dynamo action on various values of the magnetic Reynolds- and Prandtl numbers for the cases of the Roberts Flow kinematic dynamo and a flow that, in turn, incorporates both a non-helical and helical forcing function that introduces turbulence into …

    cape-town Repository record for Cio-cio-san no Yūutsu: memoirs of magnetogenesis and Turbulent Dynamo Theory (opens in a new tab)

  3. Magnetic Field Evolution in Black Hole Accretion Disks and Relativistic Jets

    … I additionally perform a minor study of the disk dynamo, covered in Chapter 3. Using mean-field dynamo theory, I calculate the diagonal, symmetric α_ij components under both a global azimuthal average and a local Gaussian filter average, finding that local averaging returns more robust numerical …

    cambridge Repository record for Magnetic Field Evolution in Black Hole Accretion Disks and Relativistic Jets (opens in a new tab)

  4. Interstellar turbulence driven by magneto-rotational instability

    … using massive parallelization. The alpha-Omega dynamo is known to be one of the most efficient mechanisms to reproduce the observed global galactic fields. The presence of strong turbulence is a pre-requisite for the alpha-Omega dynamo generation of the regular magnetic fields. The observed …

    potsdam-diss Repository record for Interstellar turbulence driven by magneto-rotational instability (opens in a new tab)

  5. Scale selection in hydromagnetic dynamos

    … turbulent convection that ultimately powers the dynamo. Motivated by the scale separation considerations, in this thesis we study the parametric scale selection of dynamo action. Although helioseismology has made a lot of progress in the study of the solar interior, the precise motions of plasma …

    cambridge Repository record for Scale selection in hydromagnetic dynamos (opens in a new tab)

  6. Dynamics of the rise of magnetic flux tubes in stellar interiors

    In sonnenähnlichen Sternen erhält ein Dynamo-Mechanismus die Magnetfelder. Der Babcock-Leighton-Dynamo beruht auf einem solchen Mechanismus und erfordert insbesondere die Existenz von magnetischen Flussröhren. Man nimmt an, dass magnetische Flussröhren am Boden der Konvetionszone entstehen und …

    potsdam-diss Repository record for Dynamics of the rise of magnetic flux tubes in stellar interiors (opens in a new tab)

  7. Shearing waves and the MRI dynamo in stratified accretion discs

    … local simulations of the MRI have shown that the dynamo changes character on addition of vertical stratification. We investigate numerically 3D hydrodynamic shearing waves with a conserved Hermitian form in an isothermal disc with vertical gravity, and describe the associated symplectic structure. …

    cambridge Repository record for Shearing waves and the MRI dynamo in stratified accretion discs (opens in a new tab)