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We present a major update to the 3D coronal rope ejection (3DCORE) technique for modeling coronal mass ejection flux ropes in conjunction with an approximate Bayesian computation (ABC) algorithm that is used for fitting the model to in situ magnetic field measurements. The model assumes an empirically motivated torus-like flux rope structure that expands self-similarly within the heliosphere, is influenced by a simplified interaction with the solar wind environment, and carries along an embedded analytical magnetic field. Th ...
Published by: ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES Published on: 01/2021
YEAR: 2021   DOI: 10.3847/1538-4365/abc9bd