A scatterhyphen;hole xhyphen;ray camera has been designed and flown in a rocket to measure solar x radiation. Its distinguishing feature is that many single pinhyphen;hole images are allowed to overlapmdash;a multiplexing approach that saves space, gives practical signalhyphen;tohyphen;fog ratio, and requires special object reconstruction techniques. It was possible to reconstruct the appearance of the dominant source of solar emission on the day of rocket flight with better than one arc minute resolution. The coronal xhyphen;ray region had the same general shape and intensity distribution as the associated calcium Khyphen;line region
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