Conductivity of an ion-acoustically turbulent plasma

dc.contributor.author	Krishan, V
dc.date.accessioned	2008-12-16T14:24:36Z
dc.date.available	2008-12-16T14:24:36Z
dc.date.issued	1978-09
dc.identifier.citation	Solar Physics, Vol. 59, pp. 29 - 42	en
dc.identifier.issn	0038-0938 (Print)1573-093X (Online)
dc.identifier.uri	http://hdl.handle.net/2248/4076
dc.description	Open Access
dc.description.abstract	Three 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.iso	en	en
dc.publisher	D.Reidel Publishing Co.,	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1978SoPh...59...29K	en
dc.relation.uri	http://dx.doi.org/10.1007/BF00154929	en
dc.rights	©D.Reidel Publishing Co.,
dc.subject	Ion Acoustic Waves	en
dc.subject	Plasma Conductivity	en
dc.subject	Plasma Turbulence	en
dc.subject	Solar Physics	en
dc.subject	Acoustic Scattering	en
dc.subject	Damping	en
dc.subject	Density Wave Model	en
dc.subject	Magnetohydrodynamic Stability	en
dc.subject	Plasma-Particle Interactions	en
dc.subject	Saturation	en
dc.subject	Skylab Program	en
dc.subject	Solar Flares	en
dc.subject	Wave Interaction	en
dc.title	Conductivity of an ion-acoustically turbulent plasma	en
dc.type	Article	en