The role of small versus large scale magnetic topologies in global waves

Astronomy and Astrophysics

Volumn 495, Issue 2, 2009, Pages 571-575

  Delannee C ^a,b  

^a ROYAL OBSERVATORY OF BELGIUM   (Belgium)

^b CNRS   (France)

Author keywords

Sun: activity; Sun: coronal mass ejections (CMEs); Sun: magnetic fields

Indexed keywords

APPROXIMATION THEORY; BOUNDARY LAYER FLOW; MAGNETIC FIELDS; MAGNETIC FLUX; MAGNETIC STRUCTURE; SUN; TOKAMAK DEVICES; TOPOLOGY;

ACTIVE REGIONS; CORONAL HOLES; CORONAL MASS EJECTIONS; CORONAL WAVES; DIFFERENCE IMAGES; LARGE-SCALE STRUCTURES; MAGNETIC FIELD LINES; MAGNETIC FIELD TOPOLOGIES; MAGNETIC FLUX TUBES; MAGNETIC TOPOLOGIES; QUIET SUNS; SUN: ACTIVITY; SUN: CORONAL MASS EJECTIONS (CMES); SUN: MAGNETIC FIELDS; WAVE FRONTS;

MAGNETIC DOMAINS;

EID: 61349124843     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200809451     Document Type: Article

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