Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4076
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dc.contributor.authorKrishan, V-
dc.date.accessioned2008-12-16T14:24:36Z-
dc.date.available2008-12-16T14:24:36Z-
dc.date.issued1978-09-
dc.identifier.citationSolar Physics, Vol. 59, pp. 29 - 42en
dc.identifier.issn0038-0938 (Print)1573-093X (Online)-
dc.identifier.urihttp://hdl.handle.net/2248/4076-
dc.descriptionOpen Access-
dc.description.abstractThree different mechanisms are suggested for the non-linear saturation of the ion-acoustic instability. These include the indirect wave-particle interaction, the scattering on density fluctuations and the effects of energy renormalization of the particles. A comparison with the earlier theoretical investigations and the recent observations of Skylab has been made.en
dc.language.isoenen
dc.publisherD.Reidel Publishing Co.,en
dc.relation.urihttp://adsabs.harvard.edu/abs/1978SoPh...59...29Ken
dc.relation.urihttp://dx.doi.org/10.1007/BF00154929en
dc.rights©D.Reidel Publishing Co.,-
dc.subjectIon Acoustic Wavesen
dc.subjectPlasma Conductivityen
dc.subjectPlasma Turbulenceen
dc.subjectSolar Physicsen
dc.subjectAcoustic Scatteringen
dc.subjectDampingen
dc.subjectDensity Wave Modelen
dc.subjectMagnetohydrodynamic Stabilityen
dc.subjectPlasma-Particle Interactionsen
dc.subjectSaturationen
dc.subjectSkylab Programen
dc.subjectSolar Flaresen
dc.subjectWave Interactionen
dc.titleConductivity of an ion-acoustically turbulent plasmaen
dc.typeArticleen
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