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dc.contributor.authorVerhees, Frank
dc.contributor.authorLakhina, G.S.
dc.date.accessioned2017-03-07T11:15:02Z
dc.date.accessioned2021-02-12T09:50:53Z-
dc.date.available2017-03-07T11:15:02Z
dc.date.available2021-02-12T09:50:53Z-
dc.date.issued1996
dc.identifier.citationAstrophysics and Space Science, v.240/2, p.215-224, 1996, doi: 10.1007/BF00639586en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/955-
dc.description.abstractIn electron-positron plasmas the charge-to-mass ratio is the same for both species. This leads for different waves to the vanishing of certain coefficients in the dispersion laws and nonlinear evolution equations, and also to the decoupling of some of the plasma modes. In particular, there is a low-frequency mode which exists at all angles of propagation with respect to the static magnetic field, corresponding at parallel propagation to a degenerate case of circularly polarized waves, and at perpendicular propagation to part of the extraordinary mode. The nonlinear evolution of this generalizedX-mode is governed by a Korteweg-de Vries equation, valid at all angles of propagation except strictly parallel propagation, for which a different approach had been given already. The nonlinearity is strongest at perpendicular propagation.en_US
dc.language.isoenen_US
dc.subjectSolitary Alfvén modesen_US
dc.subjectRelativistic plasmasen_US
dc.titleOblique solitary Alfvén modes in relativistic electron-positron plasmasen_US
dc.typeArticleen_US
dc.identifier.accession091279
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