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Volumn 484, Issue 3, 2008, Pages 847-850
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Influence of the Hall effect on the reconnection rate at line-tied magnetic X-points
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Author keywords
Magnetohydrodynamics (MHD); Sun: flares; Sun: magnetic fields
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Indexed keywords
ASTROPHYSICS;
COMPUTER NETWORKS;
DECAY (ORGANIC);
ELECTRIC CURRENTS;
FLUID DYNAMICS;
FLUID MECHANICS;
FUNCTION EVALUATION;
GALVANOMAGNETIC EFFECTS;
GYRATORS;
HALL EFFECT;
LINEAR EQUATIONS;
MAGNETIC FIELDS;
MAGNETIC MATERIALS;
MAGNETISM;
MAGNETOHYDRODYNAMICS;
NUMERICAL METHODS;
PHOTOACOUSTIC EFFECT;
SCALES (WEIGHING INSTRUMENTS);
SCALING LAWS;
SOLAR ENERGY;
ASTROPHYSICAL PLASMAS;
DECAY RATES;
ENERGY RELEASES;
EVOLUTION (CO);
HALL MAGNETOHYDRODYNAMICS (H-MHD);
HALL MHD;
IN LINE;
LARGE-SCALE SYSTEMS;
MAGNETIC (CE);
MAGNETIC RECONNECTION (MR);
RECONNECTION RATE;
SOLAR FLARES;
SYSTEM SIZES;
MAGNETIC FIELD EFFECTS;
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EID: 44849136785
PISSN: 00046361
EISSN: 14320746
Source Type: Journal
DOI: 10.1051/0004-6361:200809569 Document Type: Article |
Times cited : (9)
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References (26)
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