Magnetohydrodynamic turbulence in solar wind

dc.contributor.author	Verma, M. K
dc.date.accessioned	2008-09-08T14:22:35Z
dc.date.available	2008-09-08T14:22:35Z
dc.date.issued	1998
dc.identifier.citation	BASI, Vol. 26, pp. 231 - 232	en
dc.identifier.uri	http://hdl.handle.net/2248/3471
dc.description.abstract	Alfvenic fluctuations in the solar wind is known to exhibit turbulent behaviour. In this paper we state the existing phenomenologies. After this we show the numerical results from pseudo-spectral method. The numerical results appear to favour the Kolmogorov-like MHD turbulence phenomenology over the Kraichnan phenomenology atleast in some regime.	en
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1998BASI...26..231V	en
dc.subject	Solar wind	en
dc.subject	Turbulence	en
dc.subject	Dissipation	en
dc.title	Magnetohydrodynamic turbulence in solar wind	en
dc.type	Article	en