2.2.1 Observations with HXT


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2.2.1 Observations with HXT

Unlike SXT, HXT is operated in a single observation mode (except for calibration). When the Sun is quiet (i.e. in the quiet-high or quiet-medium mode), only hard X-ray count rate data in the lowest energy band (L band; see section 2-2) are telemetered once in every major frame (e.g. 2-s data accumulation in high-bit rate). When the flare-high mode is (automatically) triggered by the occurrence of a flare, then count rate data in the four energy bands, with a 0.5-s data accumulation, are telemetered to the ground. In this case, four sets of data ((64 SC's 4 energy bands) 4) have their telemetry allocation in one major frame.

When the spacecraft is in South Atlantic Anomaly (SAA) or in spacecraft night, high voltage supplies for the detector photomultipliers are reduced and no solar observations are made with HXT.


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