Varying the forcing scale in low Prandtl number dynamos

Small-scale dynamos are expected to operate in all astrophysical fluids that are turbulent and electrically conducting, for example the interstellar medium, stellar interiors, and accretion discs, ...

• Publication year

  2018

• Venue

  Monthly notices of the Royal Astronomical Society

• Publication date

  2018-05-03

• Fields of study

  Physics

• Identifiers
  DOI 10.1093/mnras/sty1570arXiv 1805.01249
• External record

  Open on Semantic Scholar

• Source metadata

  Semantic Scholar

• No claims are published for this paper.

• No concepts are published for this paper.

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• Mach number dependence of turbulent magnetic field amplification: solenoidal versus compressive flows.

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• NONLINEAR SMALL-SCALE DYNAMOS AT LOW MAGNETIC PRANDTL NUMBERS

  2011influential reference
• Growth rate of small-scale dynamo at low magnetic Prandtl numbers

  2011cited by this paper
• The bottleneck effect and the Kolmogorov constant in isotropic turbulence

  2010influential reference
• Test-field method for mean-field coefficients with MHD background

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  2010cited by this paper
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  2008cited by this paper
• Numerical demonstration of fluctuation dynamo at low magnetic Prandtl numbers.

  2007influential reference
• Fluctuation dynamo and turbulent induction at low magnetic Prandtl numbers

  2007cited by this paper
• Magnetic-field generation in helical turbulence.

  2005cited by this paper
• Astrophysical magnetic fields and nonlinear dynamo theory

  2004cited by this paper
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  1999cited by this paper
• On the Origin of Magnetic Fields in the Quiet Photosphere

  1999cited by this paper
• Intermittency and anomalous scaling for magnetic fluctuations

  1997cited by this paper
• Universal scaling laws in fully developed turbulence.

  1994influential reference
• Bottleneck phenomenon in developed turbulence

  1994cited by this paper
• On the universal form of energy spectra in fully developed turbulence

  1993cited by this paper
• The spectrum of random magnetic fields in the mean field dynamo theory of the galactic magnetic field

  1992cited by this paper
• Helical and Nonhelical Turbulent Dynamos

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• Magnetic Field Generation in Electrically Conducting Fluids

  1978cited by this paper

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• Saturation mechanism of the fluctuation dynamo in supersonic turbulent plasmas

  2021cites this paper
• Saturation mechanism of the fluctuation dynamo at PrM ≥ 1

  2020cites this paper
• MHD turbulence: a biased review

  2020cites this paper
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  2020cites this paper
• Seed magnetic fields in turbulent small-scale dynamos

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  2019cites this paper
• Ambipolar diffusion in large Prandtl number turbulence

  2019influential citation
• The timestep constraint in solving the gravitational wave equations sourced by hydromagnetic turbulence

  2018cites this paper
• Fully resolved array of simulations investigating the influence of the magnetic Prandtl number on magnetohydrodynamic turbulence.

  2018cites this paper