Turbulent magnetic field amplification from the smallest to the largest magnetic Prandtl numbers
The small-scale dynamo provides a highly efficient mechanism for the conversion of turbulent into magnetic energy. In astrophysical environments, such turbulence often occurs at high Mach numbers, implying steep slopes in the turbulent spectra. It is thus a central question whether the small-scale d...
| Hoofdauteurs: | , , |
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| Formaat: | Artikel |
| Taal: | English |
| Gepubliceerd in: |
IOP Publishing
2013-01-01
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| Reeks: | New Journal of Physics |
| Online toegang: | https://doi.org/10.1088/1367-2630/15/1/013055 |