Using an Ellipsoid Model to Track and Predict the Evolution and Propagation of Coronal Mass Ejections

Abstract

We present a method for tracking and predicting the propagation and evolution of coronal mass ejections (CMEs) using the imagers on the STEREO and SOHO satellites. By empirically modeling the material between the inner core and leading edge of a CME as an expanding, outward propagating ellipsoid, we track its evolution in three-dimensional space. Though more complex empirical CME models have been developed, we examine the accuracy of this relatively simple geometric model, which incorporates relatively few physical assumptions, including i) a constant propagation angle and ii) an azimuthally symmetric structure. Testing our ellipsoid model developed herein on three separate CMEs, we find that it is an effective tool for predicting the arrival of density enhancements and the duration of each event near 1 AU. For each CME studied, the trends in the trajectory, as well as the radial and transverse expansion are studied from 0 to ~.3 AU to create predictions at 1 AU with an average accuracy of 2.9 hours.

18 pages, 11 figures

References in corpus (4)

• Propagation of an Earth-directed coronal mass ejection in three dimensions
• Determining the azimuthal properties of coronal mass ejections from multi-spacecraft remote-sensing observations with stereo secchi
• The kinematics of coronal mass ejections using multiscale methods
• The Brightness of Density Structures at Large Solar Elongation Angles: What is Being Observed by STEREO/SECCHI?