From solar min to max: half a solar cycle with SOHO

By Alyson G. Wilson. 2002

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Automatic Detection and Tracking of Coronal Mass Ejections in Coronagraph Time Series (2008, methodology): “The first of its kind, the Computer Aided CME Tracking (CACTus) software package was introduced in 2002 (Berghmans, Foing, and Fleck, 2002; Robbrecht and Berghmans, 2004).”
On the nature of EIT waves, EUV dimmings and their link to CMEs (2004, methodology): “The area of TCHs can be determined using brightness segmentation method (see e. g. Veselovsky et al. 2001; Zhukov et al. 2002).”
Coronal Mass Ejections: Observations (2012, background): “The source regions of frontside halo CMEs are likely to be located within a few tens of degrees of Sun center from the perspective of the observer (Cane et al., 2000; Webb, 2002; Gopalswamy, 2004; Gopalswamy et al., 2010b).”
The association of coronal mass ejections with their effects near the Earth (2005, background): “2 we give some useful background information on the status of our current understanding of the whole scenario (for more detailed general reviews see, e.g. Webb, 2000, 2002, and the discussion in Cliver and Hudson, 2002).”