Large-scale structure of the magnetic field in the outer heliosphere.

Details Large-scale structure of the magnetic field in the outer heliosphere. Large-scale structure of the magnetic field in the outer heliosphere.

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992stgg...36...60v&link_type=abstract

Stud. Geophys. Geod., Vol. 36, No. 1, p. 60 - 66

Physics

1

Scientific paper

Magnetic field structures at great distances from the Sun have been analyzed qualitatively for a simple vacuum reconnection model of the interplanetary and interstellar magnetic field. In dependence on the mutual orientation of the main solar dipole μs and the local interstellar field B0, either an open or closed configuration of the large-scale field is formed. For (μsB0) > 0, the field lines are represented by a system of magnetic lines open towards interstellar space. In the case of (μsB0) < 0 there exist two zero-points and a separating surface below the heliopause separating the open lines of the interstellar field from the closed lines of the interplanetary field. The magnetic field configuration is characterized by a certain asymmetry, which is considered for (μsB0) = 0.

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