Relationships between supergranular horizontal flow velocity, cell size and cell lifetime

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4136

Full metadata record

DC Field	Value	Language
dc.contributor.author	Paniveni, U.	-
dc.contributor.author	Krishan, Vinod	-
dc.contributor.author	Singh, Jagdev	-
dc.contributor.author	Srikanth, R.	-
dc.date.accessioned	2011-08-23T10:36:25Z	-
dc.date.available	2011-08-23T10:36:25Z	-
dc.date.issued	2006	-
dc.identifier.citation	Proceedings IAU Symposium: Solar Activity and its Magnetic Origin, 2006, Vol. 233, p85	en
dc.identifier.uri	http://hdl.handle.net/2289/4136	-
dc.description	Restricted Access.	en
dc.description.abstract	Supergranules are observed in the high photosphere as large convection eddies with horizontal diverging flows from the cell centre and subsiding flows at the cell borders.	en
dc.language.iso	en	en
dc.publisher	Cambridge University Press	en
dc.relation.uri	http://dx.doi.org/ 10.1017/S1743921306001542	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2006IAUS..233...85P	en
dc.rights	2006, International Astronomical Union	en
dc.subject	Sun: granulation – turbulence	en
dc.title	Relationships between supergranular horizontal flow velocity, cell size and cell lifetime	en
dc.type	Article	en
Appears in Collections:	Research Papers (LAMP)

Files in This Item:

File	Description	Size	Format
2006 IAUS_vol.233, p85.pdf Restricted Access	Restricted access	83.66 kB	Adobe PDF	View/Open Request a copy