Understanding the Evolution and Propagation of Coronal Mass Ejections and Associated Plasma Sheaths in Interplanetary Space
Date
2015
Authors
Hess, Phillip
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Abstract
A Coronal Mass Ejection (CME) is an eruption of magnetized plasma from the Coronaof the Sun. Understanding the physical process of CMEs is a fundamental challenge in solarphysics, and is also of increasing importance for our technological society. CMEs are knownthe main driver of space weather that has adverse effects on satellites, power grids, com-munication and navigation systems and astronauts. Understanding and predicting CMEs is still in the early stage of research. In this dissertation, improved observational methods and advanced theoretical analysis are used to study CMEs.
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Keywords
Astronomy, Physics, Astrophysics, Coronal Mass Ejection, Solar Physics, Solar Wind, Space Weather, Sun