Oblique solitary Alfvén modes in relativistic electron-positron plasmas

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dc.contributor.author Verhees, Frank
dc.contributor.author Lakhina, G.S.
dc.date.accessioned 2017-03-07T11:15:02Z
dc.date.accessioned 2021-02-12T09:50:53Z
dc.date.available 2017-03-07T11:15:02Z
dc.date.available 2021-02-12T09:50:53Z
dc.date.issued 1996
dc.identifier.citation Astrophysics and Space Science, v.240/2, p.215-224, 1996, doi: 10.1007/BF00639586 en_US
dc.identifier.uri http://localhost:8080/xmlui/handle/123456789/955
dc.description.abstract In 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.iso en en_US
dc.subject Solitary Alfvén modes en_US
dc.subject Relativistic plasmas en_US
dc.title Oblique solitary Alfvén modes in relativistic electron-positron plasmas en_US
dc.type Article en_US
dc.identifier.accession 091279


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