Indium tin oxide thin films have been deposited on glass substrates using rf magnetron sputtering at different power densities (0.27–0.80 W/cm 2 ) and at different substrate temperatures (RT-250) °C. Film structure, crystallite size and orientation, optical absorption and bandgap have been studied to characterize the films. Carrier concentration and Hall mobility have been determined by Hall effect. X-ray diffraction (XRD) analysis of room temperature (RT) deposited samples reveals a structural change from amorphous to mixed amorphous/polycrystalline structure with <100> preferred orientation with increasing rf power density. The increase in substrate temperature results in a similar structural evolution from amorphous to a mixed phase followed, at temperatures higher than 200°C, by a polycrystalline phase with <111> orientation. The study clearly indicates that ITO films dominated by oxygen vacancies prefer to grow with <100> oriented crystallites whereas the <111> oriented films are characterized by a more effective doping by tin.
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Terzini et al. (1999) studied this question.
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