Understanding helical magnetic dynamo spectra with a non-linear four-scale theory

Monthly Notices of the Royal Astronomical Society

Volumn 344, Issue 3, 2003, Pages 707-714

  Blackman, Eric G ^a  

^a UNIVERSITY OF ROCHESTER   (United States)

Author keywords

Galaxies: magnetic fields; ISM: magnetic fields; Methods: numerical; MHD; Stars: magnetic fields; Turbulence

Indexed keywords

INTERACTIVE DEVICES; MAGNETOHYDRODYNAMICS; NUMERICAL METHODS; PRANDTL NUMBER; REYNOLDS NUMBER;

FORCINGS; GALAXIES: MAGNETIC FIELDS; ISM: MAGNETIC FIELDS; MAGNETIC ENERGIES; METHOD: NUMERICAL; NON LINEAR; SCALE THEORY; SMALL SCALE; SPECTRA'S; STARS: MAGNETIC FIELD;

TURBULENCE;

EID: 0142167967     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06812.x     Document Type: Article

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