Ion-sound turbulence due to shock gradients in collisionless plasmas

dc.contributor.author	Gopalswamy, N
dc.contributor.author	Thejappa, G
dc.date.accessioned	2009-10-16T11:10:25Z
dc.date.available	2009-10-16T11:10:25Z
dc.date.issued	1985-11
dc.identifier.citation	Pramana, Vol. 25, No. 5, pp. 575 - 585	en
dc.identifier.issn	0304-4289
dc.identifier.uri	http://hdl.handle.net/2248/4867
dc.description.abstract	The dispersion relation for ion sound waves generated in a perpendicular shock is derived and the energy density of ion-sound turbulence is obtained using quasilinear theory. The result is compared with the lower hybrid turbulence generated under similar conditions. It is shown that ion-sound turbulence is a better candidate for the generation of type-I radio bursts in the solar corona.	en
dc.language.iso	en	en
dc.publisher	Indian Academy of Sciences	en
dc.relation.uri	http://www.ias.ac.in/j_archive/pramana/25/vol25contents.html	en
dc.rights	© Indian Academy of Sciences	en
dc.subject	Ion-Sound Turbulence	en
dc.subject	Quasilinear Effects	en
dc.subject	Lower Hybrid Turbulence	en
dc.subject	Type-I Radio Bursts	en
dc.title	Ion-sound turbulence due to shock gradients in collisionless plasmas	en
dc.type	Article	en