Evolution of an eruptive flare loop system

Astronomy and Astrophysics

Volumn 498, Issue 3, 2009, Pages 901-907

  Romano, P ^a   Zuccarello, F ^b   Fletcher, L ^c   Rubio Da Costa, F ^b,c   Bain, H M ^c   Contarino, L ^b  

^a INAF OSSERVATORIO ASTROFISICO DI CATANIA   (Italy)

^b UNIVERSITY OF CATANIA   (Italy)

^c UNIVERSITY OF GLASGOW   (United Kingdom)

Author keywords

Sun: activity; Sun: flares; Sun: magnetic fields

Indexed keywords

ACTIVE REGIONS; COLUMN DENSITY; CORONAL MASS EJECTION; CURRENT SHEETS; HARD X-RAY SOURCES; HEATING SOURCE; HIGH ENERGY; HIGH ENERGY X-RAYS; LINEAR BEHAVIOR; LOOP SYSTEMS; LOW ENERGY X RAYS; LOWER LIMITS; MAGNETIC RECONNECTIONS; NONTHERMAL; RADIO EMISSION; SUN: ACTIVITY; SUN: FLARES; SUN: MAGNETIC FIELDS; X-RAY SOURCES;

CHROMOPHORES; ELECTRON SOURCES; EMISSION SPECTROSCOPY; MAGNETIC FIELDS; X RAY APPARATUS; X RAY OPTICS;

SUN;

EID: 66149146271     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200811309     Document Type: Article

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