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- W2034016729 abstract "The Crab Nebula is powered by the central pulsar. The appearance of lumpy and patchy structures within the nebula results from inhomogeneous distributions of magnetic field and of relativistic electron density. In this paper, we focus on the primary origin of inhomogeneous magnetic field structures. For that purpose, we develop a theoretical model for a two-dimensional propagation of Alfvenic perturbations within the equatorial plane of an axisymmetric relativistic magnetohydrodynamic (RMHD) wind embedded with a spiral magnetic field caused by the rotation of a central source. We obtain analytical solutions within the entire frequency range for asymptotic Alfvenic perturbations at a large radial distance r" @default.
- W2034016729 created "2016-06-24" @default.
- W2034016729 creator A5011230183 @default.
- W2034016729 date "1993-09-01" @default.
- W2034016729 modified "2023-09-25" @default.
- W2034016729 title "Alfvenic fluctuations in a relativistic wind with a spiral magnetic field and random magnetic field structures in the Crab Nebula" @default.
- W2034016729 doi "https://doi.org/10.1086/173111" @default.
- W2034016729 hasPublicationYear "1993" @default.
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