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Visibility of coronal mass ejections as a function of flare location and intensity

✍ Scribed by Yashiro, S.


Book ID
119667445
Publisher
American Geophysical Union
Year
2005
Tongue
English
Weight
470 KB
Volume
110
Category
Article
ISSN
0148-0227

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Visibility and rate of coronal mass ejec
✍ C. Sawyer πŸ“‚ Article πŸ“… 1985 πŸ› Springer 🌐 English βš– 551 KB

Two thirds of the Ha flares associated in time and position with coronal mass ejections (CME) observed by the Coronagraph/Polarimeter (C/P) or by the coronagraph on Skylab lie within 30 ~ of the solar limb. Among type II flares (those with type II radio spectral bursts) with C/P observations, 10 are