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Owens, M. J., Merkin, V. G. & Riley, P. A kinematically distorted flux rope model for magnetic clouds.
To perform a realistic lifting simulation, a wire rope model that takes interference into consideration is adopted in this study.
Composition and braiding angle are adjusted to produce a non-linear tensile behavior within the range of the native ligament that can be predicted by a simple rope model.
This cloud was unusual since it had at least two internal structures and the profile of the magnetic field strength did not conform to a simple force-free flux rope model, though the field direction fitted well.
However, if the lifting simulation is performed with the traditional wire rope model modeled by an incompressible spring, it is difficult to check whether the block and the wire ropes interfere with each other, and to calculate the contact forces exerted, if any.
This paper reviews our recent progress in the numerical study of coronal mass ejections (CMEs) based on flux rope model, which shows that when the reconnection-favored emerging flux appears either within or on the outer edge of the filament channel, the flux rope would lose its equilibrium, and be ejected, while a current sheet is formed below the flux rope.
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Such a feature can be interpreted only by flux rope models with the curved shape.
The models are force-free flux rope models including the effect of self-similar expansion.
From the viewpoint of MC modeling by flux rope models, it seems that the selections (i) and (iv) are inappropriate.
For toroidal flux rope models, cases of the right-handed and left-handed are shown by red and blue arrows.
Fig. 6 Orientation in the YZ plane of the axial field estimated for each of the flux rope models.
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