The purpose of this work is to measure the overall heat transfer coefficient from water to cover in shallow solar stills using yield measurements. The geometry under analysis represents a real solar still operating with laboratory-controlled temperatures and induced heat flows in steady-state. Tempe
Effect of forced convection inside the solar still on heat and mass transfer coefficients
✍ Scribed by H.M. Ali
- Book ID
- 113295337
- Publisher
- Elsevier Science
- Year
- 1993
- Tongue
- English
- Weight
- 361 KB
- Volume
- 34
- Category
- Article
- ISSN
- 0196-8904
No coin nor oath required. For personal study only.
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