It is shown that the magnetic‐pressure effect in the azimuthal direction in the heliosheath region results in the formation of a global V‐shaped channel structure in both the heliopause and the termination shock surfaces. The physical processes involved in the formation of the V‐shaped heliosphere is closely related with that of a bipolar‐flow type Planetary Nebulae.

Topics
Heliosphere, Nebulae, Termination shock
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© 2005 American Institute of Physics.
2005
American Institute of Physics
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