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

By S. Yashiro, Nat Gopalswamy, S. Akiyama, G. Michałek, R. Howard. 2005

157 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/1e23e771703ee5c9ec2045c9d521770c9074a9a5

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In Astronomy and Astrophysics

1. Nat Gopalswamy
2. S. Yashiro
3. R. Howard
4. D. Webb
5. M. Temmer
6. A. Vourlidas
7. S. Akiyama
8. Yuming Wang

Citations in the corpus

• NEW SOLAR EXTREME-ULTRAVIOLET IRRADIANCE OBSERVATIONS DURING FLARES (2011, background): “Earlier studies revealed what appeared to be a steady increase in the fraction of CME-related events as a function of flare magnitude, ranging from ∼20% for C flares to ∼50% for M flares, and reaching close to 100% for X flares (Andrews 2003; Wang & Zhang 2007; Yashiro et al. 2005; Hudson 2011).”
• Driving major solar flares and eruptions: A review (2008, background): “For example, Wang and Zhang (2007) find that 90% of 104 studied X-class flares are associated with eruptions, and Yashiro et al. (2005) find that the fraction of flares associated with CMEs increases from 20% for C3-9 flares to 100% for flares above X3.”
• Different Power-Law Indices in the Frequency Distributions of Flares with and without Coronal Mass Ejections (2006, background): “Examining the CME visibility (detection efficiency) of the LASCO coronagraphs, Yashiro et al. (2005) found that about half of disk CMEs associated with C-class flares and ∼16% of disk CMEs associated with M-class flares were invisible to LASCO, while all CMEs associated with X-class flares were…”
• A Comparative Study between Eruptive X-Class Flares Associated with Coronal Mass Ejections and Confined X-Class Flares (2007, background): “Among the 11 confined X-class flares from 1996 to 2004, the first four events have been reported earlier by Yashiro et al. (2005).”
• STEREO IMPACT Investigation Goals, Measurements, and Data Products Overview (2008, unknown): “A few events observed by SOHO LASCO appeared to be traveling at speeds ∼2500 km/s (Yashiro et al. 2005).”
• The SOHO/LASCO CME Catalog (2009, background): “Yashiro et al. (2005) estimated that *20% of CMEs may not have been detected by LASCO because they are either masked by the occulting disk or they are back-sided.”