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Propagation of Coronal Mass Ejections Observed During the Rising Phase of Solar Cycle 24
Description: In this study, we investigate the interplanetary consequences and travel time details of 58 coronal mass ejections (CMEs) in the Sun-Earth distance. The CMEs considered are halo and partial halo events of width >120°. These CMEs occurred during 2009 - 2013, in the ascending phase of the Solar Cycle 24. Moreover, they are Earth-directed events that originated close to the centre of the solar disk (within about ±30° from the Sun's centre) and propagated approximately along the Sun-Earth line. [Source: Solar Physics]
URL: https://link.springer.com/article/10.1007/s11207-017-1151-y
Availability: Full Text
Source: Solar Physics
Publish Date: 10/5/2017
Reading Level: Basic
Page Length:  

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