초록 ▼

An optical relay system for bringing a Cassegrain-type or other type telescope infrared (IR) image through a mount elevation axis, yoke and azimuth axis for focusing at an image plane on the mount which is stationary relative to compound motion of the telescope. The relay system is made up or of def

An optical relay system for bringing a Cassegrain-type or other type telescope infrared (IR) image through a mount elevation axis, yoke and azimuth axis for focusing at an image plane on the mount which is stationary relative to compound motion of the telescope. The relay system is made up or of deflecting or folding mirrors, apertured flat mirrors and concave spherical and elliptical mirrors arranged for minizing field degradation of off-axis objects.

대표청구항 ▼

An optical system for relaying a telescope image from a movable telescope by folding the bundle through a movable telescope mount to a fixed focal plane remote therefrom with improved imaging for off axis focusing comprising: means folding the bundle out of the telescope optical axis and converging

An optical system for relaying a telescope image from a movable telescope by folding the bundle through a movable telescope mount to a fixed focal plane remote therefrom with improved imaging for off axis focusing comprising: means folding the bundle out of the telescope optical axis and converging it to a focal point outside the telescope; a first apertured flat mirror disposed around the bundle axis with its plane at an oblique angle thereto and containing the focal point; a spherical concave mirror downbeam of an facing the first apertured flat mirror for folding the bundle back to the apertured flat mirror from which it is folded to a second apertured flat mirror; said second aperatured flat mirror disposed around the bundle axis with its plane at an oblique angle thereto and folding the bundle to an ellipsoidal concave mirror; said ellipsoidal concave mirror disposed downbeam of an facing the second apertured flat mirror for folding the bundle back to the second apertured flat mirror and converging it to focal points in the aperature thereof in the plane of the second aperture flat mirror; whereby aberrations caused by off-axis focusing of objects by the telescope are minimized in the periphery of the field at the focal plane.