Scanning wide field telescope and method
A scanning wide-field telescope includes a primary reflecting mirror and a corrector assembly. The corrector assembly corrects light beams for spherical aberration imposed on the light beams by the primary reflecting mirror. The corrector assembly is located between the primary reflecting mirror and a viewing end of the telescope, and is configured to move to multiple optical focal points of the primary reflecting mirror.
1. A scanning wide-field telescope comprising:
a primary reflecting mirror and a corrector assembly,
wherein the corrector assembly is configured between the primary reflecting mirror and a viewing end of the telescope, and is configured to move within a first trajectory,
wherein the first trajectory comprises movement from an axis that is substantially parallel to a center line of sight of the scanning wide-field telescope to an axis that is substantially parallel to a peripheral line of sight of the scanning wide-field telescope, and
wherein the center line of sight and the peripheral line of sight are not parallel.
2. The scanning wide-field telescope of claim 1 , further comprising a selector mirror located at an output of the corrector assembly.
3. The scanning wide-field telescope of claim 2 , wherein the selector mirror is configured to control jitter.
4. The scanning wide-field telescope of claim 1 , wherein the primary reflecting mirror is a spherical mirror.
5. The scanning wide-field telescope of claim 1 , wherein the corrector assembly is configured to process multiple optical bands.
6. The scanning wide-field telescope of claim 5 , wherein the multiple optical bands comprises at least visible light and infrared light.
7. The scanning wide-field telescope of claim 6 , further comprising a switching mirror configured to switch between individual ones of the multiple optical bands.
8. The scanning wide-field telescope of claim 1 , wherein the corrector assembly is configured to correct for spherical aberration.
9. The scanning wide-field telescope of claim 1 , further comprising a steering mirror configured to provide a steering light beam to the primary reflecting mirror.
10. A method for a scanning wide-field telescope, the scanning wide-field telescope including a primary reflecting mirror and a corrector assembly, wherein the corrector assembly is configured between the primary reflecting mirror and a viewing end of the telescope, the method comprising:
receiving light from an object to be viewed at the primary reflecting mirror;
reflecting the light from the primary reflecting mirror;
moving the corrector assembly in a first trajectory to a focal point of the reflected light; and
moving from an axis that is substantially parallel to a center line of sight of the scanning wide-field telescope to an axis that is substantially parallel to a peripheral line of sight of the scanning wide-field telescope,
wherein the center line of sight and the peripheral line of sight are not parallel.
11. The method of claim 10 , further comprising correcting for jitter with a de-jitter mirror.
12. The method of claim 11 , wherein the corrector is configured to move to any of multiple optical focal points of the primary reflecting mirror.
13. The method of claim 10 , further comprising processing multiple optical bands with the corrector assembly.
14. The method of claim 13 , wherein the multiple optical bands comprises at least visible light and infrared light.
15. The method of claim 13 , further comprising switching between individual ones of the multiple optical hands with a switching mirror.
16. The method of claim 10 , further comprising correcting for spherical aberration with the corrector assembly.