dc.contributor.author |
Paniveni, U |
|
dc.contributor.author |
Krishan, V |
|
dc.contributor.author |
Singh, J |
|
dc.contributor.author |
Srikanth, R |
|
dc.date.accessioned |
2012-02-24T14:43:19Z |
|
dc.date.available |
2012-02-24T14:43:19Z |
|
dc.date.issued |
2011-08 |
|
dc.identifier.citation |
Astrophysical Dynamics: From Stars to Galaxies, Proceedings of the International Astronomical Union, IAU Symposium, Vol. 271, pp. 391-392 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/5706 |
|
dc.description |
Open Access |
en |
dc.description.abstract |
We study the complexity of supergranular cells using the intensity patterns obtained at the Kodaikanal solar observatory during the solar maximum. Our data consists of visually identified supergranular cells, from which a fractal dimension D is obtained according to the relation P ∝ AD/2 where A is the area and P is the perimeter of the cells. We find a difference in the fractal dimension between the active and the quiet region cells which is conjectured to be due to the magnetic activity level. |
en |
dc.language.iso |
en |
en |
dc.publisher |
Cambridge University Press |
en |
dc.relation.ispartofseries |
International Astronomical Union Symposium; No. 271 |
|
dc.relation.uri |
http://dx.doi.org/10.1017/S1743921311017947 |
en |
dc.rights |
© International Astronomical Union |
en |
dc.subject |
Sun: granulation —-turbulence |
en |
dc.title |
Supergranulation and its Activity Dependence |
en |
dc.type |
Article |
en |