Method and system for evaluating on-orbit measurement precision of multi-probe star sensor
A star sensor and measurement accuracy technology, which is applied in the field of on-orbit measurement accuracy evaluation of multi-head star sensors, can solve problems such as time asynchronous error, inability to truly reflect star sensitivity measurement accuracy, uncorrected stellar aberration, etc.
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[0070] The attitude data output by the star sensor is the attitude quaternion of the star sensor measurement coordinate system relative to the inertial coordinate system. Among them, the origin of the star sensor measurement coordinate system is the center of the detector, the X-axis points to the row direction of the detector, the Y-axis points to the row direction of the detector, and the Z-axis is the optical axis direction of the star sensor; the inertial coordinate system is J2000 geocentric Equatorial coordinate system, the origin of the coordinate system is located at the center of the earth, with reference to the flat equatorial plane and the flat vernal equinox at 12:00 on January 1, 2000 in the standard epoch, the X-axis is in the flat equatorial plane, pointing to the flat vernal equinox, and the Z-axis is perpendicular to the flat equator The plane is consistent with the direction of the earth's rotation angular velocity vector, and the Y axis and the X and Z axes s...
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