Evidence from the Extreme-ultraviolet Imaging Spectrometer for axial filament rotation before a large flare

Publications of the Astronomical Society of Japan

Volumn 61, Issue 3, 2009, Pages 493-497

  Williams, David R ^a,e   Harra, Louise K ^a   Brooks, David H ^b,e   Imada, Shinsuke ^c   Hansteen, Viggo H ^d  

^a UNIVERSITY COLLEGE LONDON   (United Kingdom)

^b NAVAL RESEARCH LABORATORY   (United States)

^c NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^d UNIVERSITY OF OSLO   (Norway)

^e JAPAN AEROSPACE EXPLORATION AGENCY   (Japan)

Author keywords

Sun: activity; Sun: filaments; Sun: transition region

Indexed keywords

ACTIVE REGIONS; ANTI-SYMMETRIC; APPARENT VELOCITY; AXIAL FILAMENTS; EMISSION LINES; EXTREME ULTRAVIOLET IMAGING SPECTROMETERS; SUN: ACTIVITY; SUN: FILAMENTS; SUN:TRANSITION REGION; X-CLASS FLARES;

SPECTROMETERS;

EID: 68949119964     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/61.3.493     Document Type: Article

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