Propagation of Coronal Mass Ejections in the Inner Heliosphere

Abstract

Solar Coronal mass ejections (CMEs) are large-scale ejections of plasma and magnetic field from the corona, which propagate through interplanetary space. CMEs are the most significant drivers of adverse space weather on Earth, but the physics governing their propagation through the Heliosphere is not well understood. This is mainly due to the limited fields-of-view and plane-of-sky projected nature of previous observations. The Solar Terrestrial Relations Observatory (STEREO) mission launched in October 2006, was designed to overcome these limitations. In this thesis, a method for the full three dimensional (3D) reconstruction of the trajectories of CMEs using STEREO was developed. Using the 3D trajectories, the true kinematics were derived, which were free from projection effects. Evidence for solar wind (SW) drag forces acting in interplanetary space were found, with a fast CME decelerated and a slow CME accelerated toward typical SW velocities. It was also found that the fast CME showed a linear dependence on the velocity difference between the CME and the SW, while the slow CME showed a quadratic dependence. The differing forms of drag for the two CMEs indicated the forces responsible for their acceleration may have been different. CMEs are known to generate bow shocks as they propagate through the corona and SW. Although CME-driven shocks have previously been detected indirectly via their emission at radio frequencies, direct imaging has remained elusive due to their low contrast at optical wavelengths. Using STEREO observations, the first images of a CME-driven shock as it propagates through interplanetary space from 8 R_Sun to 120 R_Sun (0.5 AU) were captured. These observations were compared to empirically derived relation and in general showed good agreement.

PhD Thesis completed in Trinity College Dublin, Astrophysics Research Group (http://www.physics.tcd.ie/Astrophysics/). Supervisor: Dr. Peter T. Gallagher. Figure resolution has been reduced and layout has been altered to for arXiv submission, for full resolution figures and layout as submitted see (http://www.tcd.ie/Physics/Astrophysics/theses/shane_maloney.pdf). 222 pages, 107 figures

References in corpus (10)

• Torus instability
• Ideal kink instability of a magnetic loop equilibrium
• Formation of current sheets and sigmoidal structure by the kink instability of a magnetic loop
• Propagation of an Earth-directed coronal mass ejection in three dimensions
• Observations and modeling of the early acceleration phase of erupting filaments involved in coronal mass ejections
• The Depiction of Coronal Structure in White Light Images
• The kinematics of coronal mass ejections using multiscale methods
• Solar Wind Drag and the Kinematics of Interplanetary Coronal Mass Ejections
• Coronal Mass Ejection Detection using Wavelets, Curvelets and Ridgelets: Applications for Space Weather Monitoring
• The Kinematics and Morphology of Solar Coronal Mass Ejections