Inverse Cascade in Hydrodynamic Turbulence and its Role in Solar Granulation

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3520

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DC Field	Value	Language
dc.contributor.author	Krishan, V	-
dc.date.accessioned	2008-09-10T12:03:30Z	-
dc.date.available	2008-09-10T12:03:30Z	-
dc.date.issued	1990	-
dc.identifier.citation	IAU Symposium, No. 138, pp. 329 - 332	en
dc.identifier.issn	0074-1809	-
dc.identifier.uri	http://hdl.handle.net/2248/3520	-
dc.description.abstract	Self-organization i.e the formation of large ordered structures in a turbulent medium is a consequence of inverse cascade where energy preferentially transfers towards large spatial scales. It is envisaged that this may be one way of explaining solar granulation at various scales.	en
dc.language.iso	en	en
dc.publisher	International Astronomical Union	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1990IAUS..138..329K	en
dc.subject	Inverse Cascade	en
dc.subject	Hydrodynamic Turbulence	en
dc.subject	Solar Granulation	en
dc.title	Inverse Cascade in Hydrodynamic Turbulence and its Role in Solar Granulation	en
dc.type	Article	en
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