Analysis and interpretation of a fast limb CME with eruptive prominence, C-flare, and EUV dimming

Astronomy and Astrophysics

Volumn 483, Issue 2, 2008, Pages 599-608

  Koutchmy, S ^a   Slemzin, V ^b   Filippov, B ^c   Noens, J C ^d   Romeuf, D ^e   Golub, L ^f  

^a INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

^b LEBEDEV PHYSICAL INSTITUTE   (Russian Federation)

^c PUSHKOV INSTITUTE OF TERRESTRIAL MAGNETISM   (Russian Federation)

^d OBSERVATOIRE MIDI PYRÉNÉES   (France)

^e UNIVERSITÉ LYON 1   (France)

^f HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

Author keywords

Sun: activity; Sun: coronal mass ejections (CMEs); Sun: filaments; Sun: flares; Sun: prominences

Indexed keywords

IMAGING SYSTEMS; MAGNETIC FIELD EFFECTS; MAGNETIC STRUCTURE; UNCERTAINTY ANALYSIS; WAVELENGTH;

CORONAL MASS EJECTIONS (CME); ERUPTIVE PROMINENCE; MASS BALANCE; SPACEBORNE OBSERVATIONS;

SPACE RESEARCH;

EID: 43249098169     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20078311     Document Type: Article

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