The basic characteristics of EUV post-eruptive arcades and their role as tracers of coronal mass ejection source regions

Astronomy and Astrophysics

Volumn 422, Issue 1, 2004, Pages 337-349

  Tripathi, D ^a   Bothmer, V ^a   Cremades, H ^a  

^a MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

Author keywords

Sun: Corona; Sun: Coronal mass ejections (CMEs); Sun: Filaments; Sun: Flares; Sun: Photosphere sun: Solar; Terrestrial relations

Indexed keywords

DATA REDUCTION; GEOMAGNETISM; IMAGE ANALYSIS; IMAGING SYSTEMS; MAGNETIC FIELDS; SOLAR RADIATION; SPACE TELESCOPES; SPACECRAFT OBSERVATORIES; ULTRAVIOLET RADIATION; X RAYS;

SUN: CORONA; SUN: CORONAL MASS EJECTIONS (CME); SUN: FILAMENTS; SUN: FLARES; SUN: PHOTOSPHERE; SUN: SOLAR-TERRESTRIAL RELATIONS;

SUN;

EID: 3142731325     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20035815     Document Type: Article

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