Study of CME properties using high resolution data
V. G. Fainshtein, Ya. I. Egorov

TL;DR
This study analyzes the early stages of six limb CMEs using high-resolution satellite data, identifying two distinct velocity profiles and observing significant angular size increases during initial propagation.
Contribution
It introduces a detailed analysis of CME initiation and propagation using combined high-resolution data, revealing two velocity profile types and size evolution during early stages.
Findings
Two CME velocity profile types identified
CME angular size increases up to threefold initially
Broadening exceeds longitudinal extension in early propagation
Abstract
The joint use of high-resolution data from PROBA2 and SDO satellites and LASCO/SOHO coronographs enabled us to examine early stages of initiation and propagation of six limb CMEs registered in June 2010 - June 2011. For five events under consideration, the CME initiation is marked by filament (prominence) eruption or by a loop-like structure having another nature. Subsequently, several loop-like structures having higher brightness and following each other at different velocities appear in the region of the CME initiation. The CME frontal structure is formed by these loop-like structures. The time-dependent velocities and acceleration of the ejection front have been obtained for all CMEs under consideration. We have drawn a conclusion about the possible existence of two CME types dependent on the time profile of their velocity. The first CME type comprises the ejections whose velocity…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Geomagnetism and Paleomagnetism Studies
