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Solar heating of a rotating spherical space vehicle

✍ Scribed by W.E. Olmstead; S. Raynor

Publisher
Elsevier Science
Year
1962
Tongue
English
Weight
819 KB
Volume
5
Category
Article
ISSN
0017-9310

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In this communication, a mathematical model is presented to predict the thermal performance of a spherical solar still. The analysis is based on the heat and mass transfer relationships by Dunkle (1961) which have been modified empirically so as to validate the experimental results of Menguy et al.