Testing magnetofrictional extrapolation with the Titov-Démoulin model of solar active regions

Astronomy and Astrophysics

Volumn 519, Issue 3, 2010, Pages

  Valori, G ^a   Kliem, B ^b,c,d   Torok T ^a   Titov, V S ^e  

^a UNIVERSITÉ PARIS DIDEROT   (France)

^b UNIVERSITY OF POTSDAM   (Germany)

^c UNIVERSITY COLLEGE LONDON   (United Kingdom)

^d NAVAL RESEARCH LABORATORY   (United States)

^e PREDICTIVE SCIENCE INC   (United States)

Author keywords

magnetic fields; Sun: corona; Sun: surface magnetism

Indexed keywords

ARCHES; EXTRAPOLATION; EXTRATERRESTRIAL ATMOSPHERES; FREE ENERGY; MAGNETIC FIELDS; ROPE; SOLAR ENERGY; VECTOR SPACES;

BEST MATCH; CURRENT DENSITY PROFILES; EVOLUTIONARY PHASIS; EXTERNAL POTENTIAL; EXTRAPOLATION SCHEMES; FLUX DISTRIBUTIONS; FLUX ROPES; FLUX TUBES; FORCE FREE FIELDS; HELICITIES; INITIAL CONDITIONS; PARAMETER SPACES; POTENTIAL FIELD; SEPARATRIX; SOLAR ACTIVE REGIONS; STRUCTURAL ELEMENTS; STRUCTURAL FEATURE; SUN: CORONA; TEST FIELDS; VECTOR FIELDS;

SUN;

EID: 77956535874     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201014416     Document Type: Article

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