dc.contributor.author |
Krishan, V |
|
dc.date.accessioned |
2009-12-02T09:46:32Z |
|
dc.date.available |
2009-12-02T09:46:32Z |
|
dc.date.issued |
1995 |
|
dc.identifier.citation |
Kuhn, J. R. and Penn, M. J. eds., Infrared tools for solar astrophysics: What's Next?., 15th National Solar Observatory/Sacramente PeaK Summer Workshop., Sunspot, New Mexico, USA , 19 - 22 Sep, 1994, pp. 327 - 340 |
en |
dc.identifier.isbn |
981-02-2188-6 |
|
dc.identifier.uri |
http://hdl.handle.net/2248/4924 |
|
dc.description |
Restricted Access |
|
dc.description.abstract |
The turbulent nature of the motions on the solar photosphere is being emphasized
more and more by the high resolution quality observations. The processes of inverse
cascade of energy in a turbulent medium are being explored for modeling the
hierarchal flow patterns on the solar surface. Here, the development of large scale
flows is studied using the Kolmogorovic arguments for a statistically stationary turbulent
fluid as well as through the solution of the Navier-Stokes equations including
the Reynold's stresses generated by the small scale flows, in a manner akin to the
dynamo problem. Some of the testable predictions of the model are also listed. |
en |
dc.language.iso |
en |
en |
dc.publisher |
World Scientific Publishing Company |
en |
dc.rights |
© World Scientific Publishing Company |
en |
dc.subject |
Infrared Tools |
en |
dc.subject |
Solar Astrophysics |
en |
dc.subject |
Extragalactic Astrophysics |
en |
dc.subject |
Planetary Astrophysics |
en |
dc.subject |
Infrared Observations |
en |
dc.subject |
Coronagraphy |
en |
dc.subject |
Solar Instruments |
en |
dc.subject |
Turbulent Model |
en |
dc.subject |
Solar Granulation |
en |
dc.title |
A Turbulent model of the solar granulation |
en |
dc.type |
Article |
en |