Relativistic Jet Stability and Structure from the Alfven Point Outwards

dc.creatorHardee, P. E.
dc.creatorRosen, A.
dc.creatorHughes, P. A.
dc.creatorDuncan, G. C.
dc.date1999-06-30
dc.date.accessioned2026-07-07T02:32:14Z
dc.date.available2026-07-07T02:32:14Z
dc.descriptionThe amplitude of jet distortions and accompanying pressure and velocity fluctuations resulting from Kelvin-Helmholtz instability of three dimensional relativistic jets are explored. The effect of instability on jets as they accelerate from sub- to super-Alfvénic speeds is explored and a relativistic stabilization mechanism for trans-Alfvénic jets is proposed. The level to which asymmetric instabilities on supermagnetosonic relativistic jets will grow is predicted theoretically and a Doppler boosted ``apparent'' emissivity is computed. Effects due to helically twisted filamentary structure produced by asymmetric modes of instability should be readily observable on relativistic jets.
dc.description10 pages, 3 figures, uses texas.sty file, to appear in the Proceedings of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology (CD-ROM)
dc.identifierhttps://arxiv.org/abs/astro-ph/9906491
dc.identifierhttp://arxiv.org/abs/astro-ph/9906491
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14438
dc.subjectAstrophysics
dc.titleRelativistic Jet Stability and Structure from the Alfven Point Outwards
dc.typetext

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