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http://hdl.handle.net/2248/4924| Title: | A Turbulent model of the solar granulation |
| Authors: | Krishan, V |
| Keywords: | Infrared Tools Solar Astrophysics Extragalactic Astrophysics Planetary Astrophysics Infrared Observations Coronagraphy Solar Instruments Turbulent Model Solar Granulation |
| Issue Date: | 1995 |
| Publisher: | World Scientific Publishing Company |
| 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 |
| 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. |
| Description: | Restricted Access |
| URI: | http://hdl.handle.net/2248/4924 |
| ISBN: | 981-02-2188-6 |
| Appears in Collections: | IIAP Publications |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| A Turbulent Model of the Solar Granulation Restricted Access | Restricted Access | 293.33 kB | Adobe PDF | View/Open Request a copy |
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