High-Energy Astrophysics American and Soviet Perspectives/Proceedings from the U.S.-U.S.S.R. Workshop on High-Energy Astrophysics (1991) / Chapter Skim
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ON TWO-DIMENSIONAL RELATIVISTIC STELLAR WINDS
ON TWO-DIMENSIONAL RELATIVISTIC STELLAR WINDS
Pages 108-111
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From page 108... ...
It means in spherical coordinates only b/br = 0 and ~ = ~r/2 In this case, all connections between neighboring field lines are lost and only one is considered. The essentially three-dimensional structure requires a smooth transition from one field line to another, and thus a distortion of the "monopole solution" arises so that the last can be only an approximation at large distances.
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From page 109... ...
Physically the constraint arises because of the distortion of the field lines due to the interaction with the neighboring ones. It is essential and describes the global features of the wind structure, since it cannot be one-dimensional.
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From page 110... ...
We will not discuss the topological features of the solutions of (3~. The reader is referred lo Kennel et al.
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From page 111... ...
Additional constraint arises from the transverse continuity requirement, which gives life to a global parameter, that is constant for the whole structure. The number of asymptotic solutions is reduced to one.
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