Characteristics of coronal mass ejections in the near Sun interplanetary space

Abstract

Based on the observations from the Large Angle and Spectrometric Coronagraph (LASCO) on board the Solar and Heliospheric Observatory (SOHO) spacecraft we studied coronal mass ejections (CME) parameters between 6 and 10 solar radii from the Sun. We have developed a new method to obtain the duration, brightness enhancement (above the background) and speed of the leading part of the CMEs. These properties are important in order to understand the dynamics of the CMEs near the Sun and their evolution in the interplanetary space using numerical models. We present the method of analysis and the results of the application of this method to a set of 9 halo CMEs observed during 1997. We found that i) the CME speeds obtained with this method are in good agreement with measurements of other observers, ii) the average time duration of the CME leading part is 8 hrs. and iii) the brightness maxima decrease with distance as a power law with a mean index of -3.6.