G. Michalek

TL;DR: In this paper, the authors present a summary of the statistical properties of the CMEs, including the apparent central position angle, the angular width in the sky plane, and the height (heliocentric distance) as a function of time.

TL;DR: The SOHO/LASCO CME catalog as mentioned in this paper is a data base for the analysis of coronal mass ejections (CMEs) in the solar corona.

TL;DR: In this article, the association between solar energetic particle (SEP) events and coronal mass ejections (CMEs) was studied and it was shown that CME interaction is an important aspect of SEP production.

TL;DR: In this article, the authors compare the statistical properties of these CMEs with those of the general population of CME observed during cycle 23 and find that the 2003 October-November CME were fast and wide on the average and hence were very energetic, nearly 20 percent of the ultrafast CME events of cycle 23 occurred during the October−November interval, including the fastest CME of the study period (∼2700 km s−1 on 4 November 2003 at 1954 UT).

TL;DR: In this article, the visibility of coronal mass ejections (CMEs) of the Large Angle Spectrometric Coronagraph (LASCO) on board the Solar and Heliospheric Observatory (SOHO) was examined using the longitudinal variation of CME association of X-ray flares.