Magnetic cloud models with bent and oblate cross-section boundaries

Astronomy and Astrophysics

Volumn 507, Issue 2, 2009, Pages 969-980

  Demoulin P ^a   Dasso, S ^b,c  

^a OBSERVATOIRE DE PARIS   (France)

^b INSTITUTO DE ASTRONOMÍA Y FÍSICA DEL ESPACIO   (Argentina)

^c UNIVERSIDAD DE BUENOS AIRES   (Argentina)

Author keywords

Interplanetary medium; Sun: coronal mass ejections (CMEs); Sun: magnetic fields

Indexed keywords

ARBITRARY CROSS SECTION; BOUNDARY SHAPES; CORONAL MASS EJECTION; CYLINDRICAL MODELS; CYLINDRICAL SYMMETRY; DYNAMICAL EVOLUTION; FIELD STRENGTHS; FLUX ROPES; GLOBAL QUANTITIES; HELICITIES; IN-SITU DATA; IN-SITU OBSERVATIONS; INTERNAL STRUCTURE; INTERPLANETARY MEDIUM; LARGE ANISOTROPY; MAGNETIC CLOUDS; MAGNETIC CONFIGURATION; MAGNETIC FIELD ORIENTATIONS; MAGNETIC FIELD PROFILE; MAGNETIC FIELD STRENGTHS; MAGNETIC FLUX ROPES; MAGNETIC MODELS; MINIMUM VARIANCE; SOLAR SOURCE; SUN: CORONAL MASS EJECTION; SUN: MAGNETIC FIELD; THEORETICAL MODELS; TIME EVOLUTIONS; TOTAL PRESSURE;

ASPECT RATIO; ASTROPHYSICS; BOUNDARY LAYER FLOW; INTERPLANETARY SPACECRAFT; MAGNETIC FIELDS; MAGNETIC FLUX; MAGNETIC STRUCTURE; PLANETARY SURFACE ANALYSIS; SOLAR WIND; SUN;

SEMICONDUCTOR COUNTERS;

EID: 70450248581     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912645     Document Type: Article

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