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- W1674789898 abstract "On the basis of a three-dimensional MHD simulation we discuss the magnetic topology of a plasmoid that forms by a localized reconnection process in a magnetotail configuration including a net dawn-dusk magnetic field component ByN . As a consequence of ByN ≠ 0 the plasmoid assumes a helical flux rope structure rather than an isolated island or bubble structure. Initially all field lines of the plasmoid flux rope remain connected with the Earth, while at later times a gradually increasing amount of flux tubes becomes separated, connecting to either the distant boundary or to the flank boundaries. In this stage topologically different flux tubes become tangled and wrapped around each other, consistent with predictions on the basis of an ad-hoc plasmoid model." @default.
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- W1674789898 date "1990-01-01" @default.
- W1674789898 modified "2023-09-23" @default.
- W1674789898 title "The magnetic topology of the plasmoid flux rope in a MHD-simulation of magnetotail reconnection" @default.
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- W1674789898 doi "https://doi.org/10.1029/gm058p0655" @default.
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