Energy Resolution
14 keV first channel
∼28 keV in other 8 channels
The central crystal was 0.635 cm thick, had a sensitive area of 70 cm2, and was viewed from behind by a pair of photomultiplier tubes. The shield crystal had a wall thickness of 4.4 cm and was viewed by 4 photomultipliers. There were 9 energy channels: the first covering 14–28 keV and the others equally spaced from 28–254 keV. In-flight calibration was done with an 241Am source. The instrument was designed primarily for observation of solar X-ray bursts. A secondary interest was the measurement of the intensity, spectrum, and spatial distribution of the diffuse cosmic background.