The Tornado Flow Configuration—An Effective Method for Screening of a Solar Reactor Window

Author:

Kogan Abraham1,Kogan Meir1

Affiliation:

1. Solar Research Facilities Unit, Weizmann Institute of Science, P.O. Box 26, Rehovot 76100, Israel

Abstract

The working fluid in solar receivers, utilized for effecting chemical reactions, is usually flown through a sealed enclosure provided with a quartz window. When one of the reactants or products of reaction is a powder, care must be taken to prevent contact of the incandescent powder particles with the window, in order to obviate its destruction by overheating. Attempts made in the past to screen the window against particle deposition by a “curtain” of an auxiliary gas stream showed that very substantial flow rates of auxiliary gas (30—80% of the main stream flow rate) were necessary for perfect window screening. The heat absorbed by the auxiliary gas stream represented a major loss of energy. In an effort to reduce the auxiliary stream flow rate to a minimum, a certain flow pattern akin to the natural tornado phenomenon has recently been developed in our laboratory. It enabled effective reactor window screening by an auxiliary gas flow rate less than 5% of the main gas flow rate. The tornado effect is discussed and demonstrated by a smoke flow visualization technique.

Publisher

ASME International

Subject

Energy Engineering and Power Technology,Renewable Energy, Sustainability and the Environment

Reference5 articles.

1. Litterst, T., 1992, “Investigation of Window Damage by Hot Particles in Solar Heated Circulating Fluidized Beds,” Proc. of 6th International Symposium on Solar Thermal Concentrating Technologies, CIEMAT, Moja´car, Spain, 1, pp. 359–369.

2. Steinfeld, A., Brack, M., Meier, A., Weidenkaff, A., and Wuillemin, D., 1998, “A Solar Chemical Reactor for Co-production of Zinc and Synthesis Gas,” Energy (Oxford), 23, pp. 803–814.

3. Batchelor, G. C., 1967, Introduction to Fluid Flow Mechanics, Cambridge University Press, Cambridge, p. 315.

4. Greenspan, H. P., 1968, Theory of Rotating Fluids, Cambridge University Press, Cambridge, p. 3.

5. Encyclopœdia Britannica, 1968, 14th Edition, Vol. 22, pp. 88–89.

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