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- W1519258545 abstract "In terms of a 2.5-D, time-dependent ideal MHD model in Cartesian coordinates, numerical studies are carried out to find equilibrium solutions associated with a magnetic flux rope embedded in a partially open ambient field, which is equivalent to that produced by a two-patch magnetic source on the photospheric surface. The coronal magnetic flux rope is characterized by its annular and axial magnetic fluxes. A catastrophe is demonstrated to exist for the whole system in response to either the variation of the two fluxes of the rope or the change of the ambient field caused by photospheric motions: decreasing of the disitance between the two sources, shrinking of the size of each source, and increasing the shear in the closed component of the ambient field." @default.
- W1519258545 created "2016-06-24" @default.
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- W1519258545 date "2002-01-01" @default.
- W1519258545 modified "2023-10-16" @default.
- W1519258545 title "Catastrophic Behavior of Coronal Magnetic Flux Ropes in Partially Open Magnetic Fields" @default.
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- W1519258545 doi "https://doi.org/10.1016/s0964-2749(02)80142-1" @default.
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