How skeletons turn into quasi-separatrix layers in source models

Astronomy and Astrophysics

Volumn 508, Issue 1, 2009, Pages 433-443

  Restante, A L ^a,b   Aulanier, G ^a   Parnell, C E ^b  

^a UNIVERSITÉ PARIS DIDEROT   (France)

^b UNIVERSITY OF ST ANDREWS   (United Kingdom)

Author keywords

Sun: magnetic fields

Indexed keywords

CONTINUOUS DISTRIBUTION; CURRENT SHEETS; FIELD LINES; FLUX CONCENTRATION; MAGNETIC CONFIGURATION; MAGNETIC NULL POINTS; MAGNETIC SOURCES; NULL POINTS; PHOTOSPHERIC MAGNETIC FIELD; SEPARATRIX; SOURCE MODELS; STANDARD POTENTIAL; SUN: MAGNETIC FIELD;

MAGNETIC FIELDS; PLASMAS;

MAGNETIC MATERIALS;

EID: 71849110688     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912664     Document Type: Article

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