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TOWARD MORE REALISTIC ANALYTIC MODELS OF THE HELIOTAIL: INCORPORATING MAGNETIC FLATTENING VIA DISTORTION FLOWS

Kleimann, Jens ; Röken, Christian ; Fichtner, Horst ; Heerikhuisen, Jacob



Abstract

Both physical arguments and simulations of the global heliosphere indicate that the tailward heliopause is flattened considerably in the direction perpendicular to both the incoming flow and the large-scale interstellar magnetic field. Despite this fact, all of the existing global analytical models of the outer heliosheath' s magnetic field assume a circular cross section of the heliotail. To ...

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