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Volumn 392, Issue 2, 2002, Pages 713-727
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The importance of physical structure in solar dynamo models
a a a |
Author keywords
Magnetic fields; MHD; Sun: magnetic fields
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Indexed keywords
APPROXIMATION THEORY;
BIFURCATION (MATHEMATICS);
GEOMETRY;
MAGNETIC FIELDS;
MATHEMATICAL MODELS;
OSCILLATIONS;
SUN;
CARTESIAN GEOMETRY;
MALKUS-PROCTOR FEEDBACK MECHANISM;
SOLAR CONVECTION ZONE;
SOLAR DYNAMO MODELS;
ASTROPHYSICS;
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EID: 0036735799
PISSN: 00046361
EISSN: None
Source Type: Journal
DOI: 10.1051/0004-6361:20020868 Document Type: Article |
Times cited : (18)
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References (82)
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