High-resistivity (84 and 1250 Ω cm) n+pp+ silicon solar cells, with thickness ranging from 56 to 250 μm, were irradiated by 1-MeV electrons and their performance evaluated using a specially developed analytical model. It was found experimentally that, contrary to expectations based on previous performance data for lower resistivity cells, the greatest cell degradation occurred for the present higher-resistivity cell. In addition, the degradation was found to be much greater than that observed for cells with base resistivities typical of those currently used in space. Relevant details of the analytical model are presented. Computer calculations of optically injected minority carrier distributions, and all voltage components at the maximum power point, are used to interpret the experimental results. The analytical model is valid for both low and high injection and includes the effects of band-gap narrowing in the cell’s heavily doped regions. It was concluded that, for the thicker higher-resistivity cell, lack of conductivity modulation, leading to a large ohmic drop in the cell base, was the predominant cause of cell degradation. Although still a significant factor, the magnitude of the ohmic component is less important in the thinner 1250 Ω cm cell. In the thicker 84 Ω cm cell, absence of conductivity modulation becomes comparable to loss in collection efficiency as a loss mechanism while in the 84 Ω cm thinner cell loss in collection efficiency begins to emerge as a dominant loss mechanism. Our results indicate that lack of conductivity modulation is a fundamental roadblock toward achieving increased radiation resistance simply by indefinitely increasing the base resistivity of silicon solar cells.
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