A Review: Solar Thermal Reactors for Materials Production

"Concentrated solar collectors including solar simulators have been studied to concentrate solar radiation to flux levels capable of reaching temperatures of 3000K. Currently, there are no industrial scale solar reactors used for material processing and only small research units have been tried. Various laboratory scale solar reactor designs are reviewed including their operating temperature and heat transfer efficiency. Solar reactor designs can be classed into directly or indirectly irradiated and single or double cavity construction. Thermal efficiencies of up to 40% have been achieved in experimental units while operating at 1500K. Problems are encountered that relate to the transfer of high heat flux. Hybrid reactor system should be considered in the future to overcome some of the practical issues associated with solar thermal reactors.I. INTRODUCTIONIn the high temperature processing of materials, such as the production of metals, cement, refractory or glass, the reactions are typically performed in the range of 500° to 2000°C. Metals are produced from minerals, which maybe oxides, sulphides, chlorides or silicates, and to recover the metals, these compounds have to undergo chemical reaction to liberate the metal. The thermodynamic stability of these compounds found in minerals necessitates the use of high temperatures to break down the bonds between the metals and other elements. Normally, the raw metals produced from smelting require refining, which is often carried out in the molten state. As new energy sources have been established, new furnace designs have evolved to incorporate the latest technology. Although solar energy has existed longer than all the current energy sources, it has not yet been incorporated into any industrial smelting; refining or melting processes. The solar radiation reaching the earth’s atmosphere, called the “Solar Constant” (SC), is defined as the rate at which solar energy is incident on a surface normal to the sun’s rays at the outer edge of the atmosphere when the earth is at its mean distance from the sun. The currently accepted value is 1367 W/m2 [1]. The earth intercepts only a small amount of this and 30% is reflected back into space, 47% is converted to low-temperature heat and reradiated into space and 23% powers the evaporative and precipitation cycle of the biosphere [2]. As a result, the solar energy reaching the earth’s surface is weakened considerably to about 1000 W/m2 or one sun, on a clear day and much lower on cloudy or smoggy days [3]. The thermodynamic limit for solar concentration is determined from the inverse square law [4] by the factor sin2? = 46,764 sun’s [5] where ? is the angular size of the sun and equals 0.0093 radians [7]. This would produce a steady state temperature equal to that of the sun’s surface of approximately 5800oC. In practice however much lower concentrations are achieved due to geometrical and optical imperfections, shading effects and tracking inaccuracies. Optical configurations based on parabolic-shaped mirrors are commercially available for large-scale collection and concentration of solar energy for the generation of electrical power. The most common configurations used for concentration of the sun’s energy in solar thermal applications are parabolic troughs, solar towers and parabolic dishes [8,9]."