Figure 5
From: Major solar eruptions and high-energy particle events during solar cycle 24
Heliographic locations of 16 fast (>1,500 km/s) CMEs from traditional GLE longitudes (W20 to W90). The flux rope locations obtained from the graduated cylindrical shell model has been corrected for solar B0 angles (see text). The CMEs are further distinguished based on their speeds (≥2,000 km/s in blue and 1,500 km/s < speed <2,000 km/s in red) and latitudinal distance from the ecliptic (filled circle within 13° and open circles at or above 13°).