摘要:
High precision spacecraft (108) attitude determination is produced by specially positioning (100) the spacecraft's star trackers (112) and then filtering (102) out measurement errors produced from star tracker electronics (216). In addition to the conventional azimuth and elevation controls used for star tracker pointing, the star tracker detector array (400) is rotationally positioned about its boresight (900) so that its pixels (401) are traversed by the imaged star path (404) at an angle within 20° of diagonal. This forces both vertical and horizontal spatial error components (700, 702) in the detector plane to a high frequency range at which they can easily be filtered out (102) in common
摘要:
A lightweight missile terminal guidance system 14 is disclosed which includes a seeker 16 for providing a first signal indicative of a first angle ε between a line-of-sight 15 from the missile 10 to a target 12 and a longitudinal axis 9 extending through the missile 10. The seeker 16 also provides a second signal indicative of a second angle δ between the longitudinal axis 9 extending through the missile 10 and a line-of-sight 11 between the missile 10 and a celestial body 13. A processor 18 is included for computing the line-of-sight angle σ between the line-of-sight 15 from the missile 10 to the target 12 and the line-of-sight 11 from the missile 10 to the celestial body 13 from the first and second angles ε and δ. A terminal guidance subsystem 24 computes acceleration commands from the line-of-sight σ angle which are used by a propulsion system 26 to change the velocity vector of the missile 10 in response thereto.
摘要:
A method and system for celestial navigation are provided. The method comprises requesting access to a light source on a low earth orbit (LEO) satellite; and sending an uplink message to the LEO satellite to power on the light source, in response to the access request. The method further comprises determining whether the LEO satellite is in view of a camera; capturing a light image, from the light source, on a focal plane location of the camera when the LEO satellite is in view of the camera; and comparing the focal plane location to a predicted location of the LEO satellite. The method updates position information of a user based on an observation error from comparing the focal plane location to the predicted location.
摘要:
Described are systems and methods for direct sun imaging by a star tracker. Disclosed in a certain example is a direct sun imaging star tracker that includes an imaging sensor and a baffle. The baffle includes a star port, a sun port, and a beam splitter. The star port is configured to image first viewing environment while the sun port is configured to image a second viewing environment that includes the sun. The beam splitter is configured to combine electromagnetic radiation from the star port and the sun port into a combined image. In various examples, the systems and techniques described herein allow a star tracker to simultaneously view both the sun and the stars.