Seed fields for galactic dynamos by the magnetorotational instability

Astronomy and Astrophysics

Volumn 424, Issue 2, 2004, Pages 565-570

  Kitchatinov, L L ^a,b   Rudiger G ^a  

^a ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

^b INSTITUTE OF SOLAR TERRESTRIAL PHYSICS   (Russian Federation)

Author keywords

Galaxies: evolution; Galaxies: magnetic fields; Magnetohydrodynamics (MHD)

Indexed keywords

AMPLIFICATION; ASTROPHYSICS; GALAXIES; MAGNETIC FIELDS; MAGNETISM; MAGNETOHYDRODYNAMICS; MATHEMATICAL MODELS; PRANDTL NUMBER; ROTATION; TURBULENCE;

COUETTE FLOWS; GALAXIES: EVOLUTION; GALAXIES: MAGNETIC FIELDS; MAGNETOROTATIONAL INSTABILITY (MRI);

DC GENERATORS;

EID: 4544259350     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20040431     Document Type: Article

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