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Low-Intensity High-Temperature (LIHT) Solar Cells for Venus Atmosphere

Giulia Tagliabue
2018
Journal paper
Abstract

Low-intensity high-temperature solar cells that operate effectively in the atmosphere of Venus at various altitudes and also survive on the 465 °C surface of Venus are being developed. Thermal stability, high-temperature current-voltage (I-V), and external quantum efficiency measurements on GaInP/GaAs double-junction solar cells are presented. Solar-cell modeling under the atmospheric conditions of Venus is used to design the optimum solar-cell structure.

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