Advanced optics for irst sensor
US-2016223394-A1 · Aug 4, 2016 · US
US12436378B2 · US · B2
| Field | Value |
|---|---|
| Publication number | US-12436378-B2 |
| Application number | US-202217989546-A |
| Country | US |
| Kind code | B2 |
| Filing date | Nov 17, 2022 |
| Priority date | Nov 17, 2022 |
| Publication date | Oct 7, 2025 |
| Grant date | Oct 7, 2025 |
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An on-gimbal telescope pointing assembly can include a head mirror operable to rotate to adjust an elevation angle of the pointing assembly and an all-reflective telescope operable to rotate to adjust an azimuth angle of the pointing assembly. The all-reflective telescope can include a fold mirror defining an output coude path of the all-reflective telescope. The pointing assembly can be operable to rotate about the coude path such that receiving optics can remain fixed while the pointing assembly rotates.
Opening claim text (preview).
What is claimed is: 1. An on-gimbal telescope pointing assembly comprising: a head mirror operable to rotate to adjust an elevation angle of the pointing assembly; and an all-reflective telescope operable to rotate to adjust an azimuth angle of the pointing assembly, wherein the all-reflective telescope comprises: a fold mirror defining an output coude path of the all-reflective telescope, wherein the pointing assembly is operable to rotate about the coude path; and a plurality of mirrors, wherein at least one mirror of the plurality of mirrors is disposed off of an axis defined by the coude path, the at least one mirror balancing the all-reflective telescope during rotation. 2. The assembly of claim 1 , wherein the plurality of mirrors and the fold mirror are positioned to be centered on a single plane. 3. The assembly of claim 1 , wherein the at least one mirror is positioned off-plane from remaining mirrors of the plurality of mirrors and the fold mirror. 4. The assembly of claim 3 , wherein the at least one mirror comprises a freeform mirror surface. 5. The assembly of claim 1 , wherein the on-gimbal telescope pointing assembly comprises a pointing acceleration of at least one thousand radians per second squared. 6. The assembly of claim 1 , wherein the all-reflective telescope comprises a dual band telescope operable to detect long wave infrared light and short wave infrared light. 7. An on-gimbal telescope pointing assembly comprising: a head mirror operable to rotate to adjust an elevation angle of the pointing assembly; and an all-reflective telescope operable to rotate to adjust an azimuth angle of the pointing assembly; wherein the on-gimbal telescope pointing assembly comprises a field of view of at least two by four degrees. 8. The assembly of claim 1 , wherein the on-gimbal telescope pointing assembly comprises a field of regard of at least 360 by 90 degrees. 9. A method for configuring an on-gimbal telescope pointing assembly, the method comprising: configuring a head mirror that is operable to adjust an elevation angle of the pointing assembly; and configuring an all-reflective telescope that is operable to adjust an azimuth angle of the pointing assembly, wherein the all-reflective telescope comprises: a fold mirror defining an output coude path of the pointing assembly, wherein the pointing assembly is operable to rotate about the coude path; and a plurality of mirrors, wherein at least one mirror of the plurality of mirrors is disposed off of an axis defined by the coude path, the at least one mirror balancing the all-reflective telescope during rotation. 10. The method of claim 9 , wherein the plurality of mirrors and the fold mirror are positioned to be centered on a single plane. 11. The method of claim 9 , wherein the at least one mirror is disposed off-plane from remaining mirrors of the plurality of mirrors and the fold mirror. 12. The method of claim 11 , wherein the at least one mirror comprises a freeform mirror surface. 13. The method of claim 9 , wherein the pointing assembly comprises a pointing acceleration of at least one thousand radians per second squared. 14. The method of claim 9 , wherein the all-reflective telescope comprises a dual band telescope operable to detect long wave infrared light and short wave infrared light. 15. The method of claim 9 , wherein the pointing assembly comprises a field of view of at least two by four degrees and a field of regard of at least 360 by 90 degrees. 16. An on-gimbal telescope pointing assembly comprising: a head mirror operable to rotate to adjust an elevation angle of the pointing assembly; and a telescope comprising a plurality of mirrors, wherein two or more mirrors of the plurality of mirrors are oriented and centered along a first plane; wherein one of the two or more mirrors comprises a fold mirror defining an output coude path of the telescope; wherein the pointing assembly is operable to rotate about the coude path; and wherein at least one mirror of the plurality of mirrors is positioned and centered off of the first plane and is disposed off of an axis defined by the coude path, the at least one mirror balancing the telescope during rotation. 17. The assembly of claim 16 , wherein the at least one mirror comprises a freeform mirror surface. 18. The assembly of claim 16 , wherein the pointing assembly comprises a pointing acceleration of at least one thousand radians per second squared. 19. The assembly of claim 16 , wherein the telescope comprises a dual band telescope operable to detect long wave infrared light and short wave infrared light. 20. The assembly of claim 16 , wherein the pointing assembly comprises a field of view of at least two by four degrees and a field of regard of at least 360 by 90 degrees.
Equatorial mounts · CPC title
involving prisms or mirrors (G02B23/14 takes precedence) · CPC title
Housings; Caps; Mountings; Supports, e.g. with counterweight · CPC title
having a focussing action, e.g. parabolic mirror · CPC title
off-axis or unobscured systems in which not all of the mirrors share a common axis of rotational symmetry, e.g. at least one of the mirrors is warped, tilted or decentered with respect to the other elements · CPC title
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