RRI Banner

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

Simple item page
dc.contributor.authorPaniveni, U.
dc.contributor.authorKrishan, Vinod
dc.contributor.authorSingh, Jagdev
dc.contributor.authorSrikanth, R.
dc.date.accessioned2011-08-23T10:36:25Z
dc.date.available2011-08-23T10:36:25Z
dc.date.issued2006
dc.descriptionRestricted Access.en
dc.description.abstractSupergranules 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.identifier.citationProceedings IAU Symposium: Solar Activity and its Magnetic Origin, 2006, Vol. 233, p85en
dc.identifier.urihttp://hdl.handle.net/2289/4136
dc.language.isoenen
dc.publisherCambridge University Pressen
dc.relation.urihttp://dx.doi.org/ 10.1017/S1743921306001542en
dc.relation.urihttp://adsabs.harvard.edu/abs/2006IAUS..233...85Pen
dc.rights2006, International Astronomical Unionen
dc.subjectSun: granulation – turbulenceen
dc.titleRelationships between supergranular horizontal flow velocity, cell size and cell lifetimeen
dc.typeArticleen

Files

Collections

Research Papers (LAMP)