Visibility and rate of coronal mass ejec
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C. Sawyer
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Article
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1985
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Springer
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English
β 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