X-ray coronal changes during halo CMEs

Geophysical Research Letters

Volumn 25, Issue 14, 1998, Pages 2481-2484

  Hudson, H S ^a,f   Lemen, J R ^b   St Cyr, O C ^c   Sterling, A C ^d,f,g   Webb, D F ^e,h  

^a Also Solar Physics Research Corporation   (United States)

^b Lockheed Martin Palo Alto Research Lab   (United States)

^c NASA GODDARD SPACE FLIGHT CENTER   (United States)

^d Computational Physics Inc ^*  (United States)

^e BOSTON COLLEGE   (United States)

^f JAPAN AEROSPACE EXPLORATION AGENCY   (Japan)

^g NAVAL RESEARCH LABORATORY   (United States)

^h AIR FORCE RESEARCH LABORATORY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

X RAY ANALYSIS; IMAGING TECHNIQUES; MONITORING; SUN; TELESCOPES; X RAYS;

CORONAL HOLE; CORONAL MASS EJECTION; CORONAL STRUCTURE; FLARE STRUCTURES; SOFT X-RAY; SURFACE FEATURE; TIME RANGE; X-RAY IMAGE;

SUN; ASTROPHYSICS;

CORONAL HOLE; DIMMING; HALO CORONAL MASS EJECTION; SIGMOID TO ARCADE DEVELOPMENT PATTERN; SOLAR DISK CENTER; SOLAR FLARE;

EID: 0032115614     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/98GL01303     Document Type: Article

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