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Physics of a Porous Solar Pond
A solar pond is a useful system for storing solar energy only if convection is strictly prevented. The temperature difference of 50°C between the bottom and the top is obtained with a pond of 1 m depth in one week (radiative heating time), if conduction loss to the ground is neglected. It takes two...
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Published in: | Japanese Journal of Applied Physics 1993, Vol.32 (3A), p.1329-1333, Article 1329 |
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Main Authors: | , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | A solar pond is a useful system for storing solar energy only if convection is strictly prevented. The temperature difference of 50°C between the bottom and the top is obtained with a pond of 1 m depth in one week (radiative heating time), if conduction loss to the ground is neglected. It takes two and a half months (conduction time), however, for the pond to settle in a quasi-stationary state. Then, 90% of the solar energy flux can be utilized. The variation principle is generalized to prove that length scales of thermal conduction and viscous forces acting in a porous pond are reduced so much that the Rayleigh number may be lowered below the critical value for the onset of convection. Piles of coarse sheets of transparent artificial lawn or vertical strings or rods, one in each 4-mm-square area, will be sufficient to prevent convection. The conduction equation is solved, giving the daily variation of temperature as less than 1°C at the bottom and negligible at the top. |
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ISSN: | 1347-4065 0021-4922 1347-4065 |
DOI: | 10.1143/JJAP.32.1329 |