Initial-Condition Influences on CME Expansion and Propagation |
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Authors: | G L Siscoe N U Crooker H A Elliott |
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Institution: | (1) Center for Space Physics, Boston University, 725 Commonwealth Avenue, Boston, MA 02215, USA;(2) Southwest Research Institute, San Antonio, TX, USA |
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Abstract: | A general-purpose melon-seed-overpressure-expansion (MSOE) model is used to examine the dependence of the expansion and propagation
of fast CMEs on average initial values of the magnetic field inside the CME, the magnetic field outside the CME, and the CME
mass. The MSOE model extracts from the real situation only features that are essential in determining the expansion and propagation
processes and idealizes them to obtain an adaptable “minimalist” set of equations that governs these processes yet retains
enough relevant physics to give useful results. This minimalist set is used to carry out a systematic comparison of solutions
against four sets of observed correlations between CME and ICME parameters in which the input parameters to the MSOE model
are varied to achieve simultaneous fits to all four correlations. The fits impose relations between the three independent
input variables: initial internal field strength, initial external field strength, and initial density. For example, light
CMEs (e.g., those with no prominences) require the external field strength to nearly equal the internal field strength. However, heavy
CMEs (e.g., those with prominences) require the external field strength to be much weaker than the internal field strength. |
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