Structure of interplanetary magnetic cloud on April 16, 1999 and its origin estimated by fitting the torus-shaped flux rope model

Geophysical Research Letters

Volumn 31, Issue 21, 2004, Pages

  Ishibashi, Hiromitsu ^a   Marubashi, Katsuhide ^a  

^a NATIONAL INSTITUTE OF INFORMATION AND COMMUNICATIONS TECHNOLOGY   (Japan)

Author keywords

2134 Interplanetary Physics: Interplanetary magnetic fields; 2164 Interplanetary Physics: Solar wind plasma; 2784 Magnetospheric Physics: Solar wind magnetosphere interactions; 7513 Solar Physics, Astrophysics, and Astronomy: Coronal mass ejections; 7531 Solar Physics, Astrophysics, and Astronomy: Prominence eruptions

Indexed keywords

GEOMETRY; MAGNETIC FLUX; SATELLITES; SOLAR SYSTEM; SURFACE PHENOMENA; PLANETARY SURFACE ANALYSIS; ROPE;

CORONAL MASS EJECTION (CME); GEOMETRICAL FLEXIBILITY; MAGNETIC CLOUD; SOLAR SURFACE PHENOMENA;

SPACE RESEARCH; MAGNETISM;

ASTROPHYSICS;

CORONAL MASS EJECTION; CYLINDRICAL FLUX ROPES; CYLINDRICAL MODELS; FILAMENT ERUPTIONS; GEOMETRICAL FLEXIBILITY; INTERPLANETARY SPACE; PLANAR STRUCTURE; SOLAR SURFACE PHENOMENA;

EID: 13244257094     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/2004GL020702     Document Type: Article

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