Two-dimensional relativistic stellar wind

Details Two-dimensional relativistic stellar wind Two-dimensional relativistic stellar wind

Jan 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.175..291g&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 175, no. 2, Jan. 1991, p. 291-310.

Statistics

Computation

2

Computational Astrophysics, Relativistic Effects, Stellar Winds, Anisotropy, Asymptotic Properties, Magnetohydrodynamic Flow, Stellar Magnetic Fields

Scientific paper

The anisotropic structure of the relativistic stellar wind is investigated. Both relativistic fluid velocity and relativistic temperature are taken into account. General analysis is carried out in the curvilinear coordinates, and the generalization of the 'dispersion equation' is obtained. The topological structure of the individual field lines is the same as in the spherically-symmetric case, except the fact that the magnetic field dependence on distance cannot be established a priori. The interaction between neighboring field lines brings the dependence on the 'transverse' coordinate, numbering the field lines. This dependence leads to a new constraint on the global flow topology. The two-dimensional wind structure is analyzed, with the constraint taken into account.

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