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   <subfield code="a">Large-scale structure of the magnetic field in the outer heliosphere</subfield>
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   <subfield code="c">[Igor Veselovskij, L. Třísková]</subfield>
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   <subfield code="a">Summary: 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 fieldB 0 , either an open or closed configuration of the large-scale field is formed. For(μs B 0 )&gt;0, the field lines are represented by a system of magnetic lines open towards interstellar space. In the case of(μs B 0 )&lt;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(μs B 0 )=0.</subfield>
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