An optical device such as a telescope may be oriented to view a subject. In one embodiment, an image capture device may be coupled to the optical device, and used to generate image data of a reference subject. The image data may be used to ascertain a first orientation of the optical device. A second orientation of the optical device, at which the subject is viewable using the optical device, may be ascertained. A rotation of the optical device needed to reorient the optical device from the first orientation to the second orientation may be calculated. Instructions may be outputted to the user, indicating how the user can apply the rotation to the optical device.

A digital counting and display system and methods for use with a laser rangefinder that counts backscattered laser beams and displays a distance between a laser and a target. The laser rangefinder includes a laser configured to emit a pulsed laser beam, an afocal Gallilean telescope configured to receive backscattered laser pulses and generate a series of focused backscattered laser pulses, a silicon avalanche photodetector connected to the afocal Gallilean telescope, configured to generate a series of currents signal proportional to the series of focused backscattered laser pulses, a low noise, multistage amplifier connected to the silicon avalanche photodetector, configured to generate a series of linearly changing amplified voltage signals from the series of current signals, an analog-to-digital converter configured to convert the series of linearly changing amplified voltage signals to a series of digital voltage signals, and a digital counting and display circuit connected to the analog-digital converter.

A digital counting and display system and methods for use with a laser rangefinder that counts backscattered laser beams and displays a distance between a laser and a target. The laser rangefinder includes a laser configured to emit a pulsed laser beam, an afocal Gallilean telescope configured to receive backscattered laser pulses and generate a series of focused backscattered laser pulses, a silicon avalanche photodetector connected to the afocal Gallilean telescope, configured to generate a series of currents signal proportional to the series of focused backscattered laser pulses, a low noise, multistage amplifier connected to the silicon avalanche photodetector, configured to generate a series of linearly changing amplified voltage signals from the series of current signals, an analog-to-digital converter configured to convert the series of linearly changing amplified voltage signals to a series of digital voltage signals, and a digital counting and display circuit connected to the analog-digital converter.

The invention relates to an optical system (7) comprising a display unit (5) for displaying an image and comprising an eyepiece (6) for observing the image. The eyepiece (6) comprises a first lens group (LG1) and a second lens group (LG2). An intermediate pupil (ZP) is arranged between the first lens group (LG1) and the second lens group (LG2). The second lens group (LG2) is designed to image the image displayed by the display unit (5) into the intermediate pupil (ZP). The first lens group (LG1) is designed to image the image arranged in the intermediate pupil (ZP) into a spatial region (B). The intermediate pupil (ZP) and the spatial region (B) are conjugate to one another. A filter unit (E, FE) and/or a wavefront manipulator (E, WM) is/are arranged at the intermediate pupil (ZP).

A telescope system includes a telescope and a selective shielding unit including at least one member including a passage allowable region for an observation target electromagnetic wave and a passage blocking region for the observation target electromagnetic wave. The telescope includes a position detectable detector that detects the observation target electromagnetic wave on a surface different from a focal plane of the telescope. The selective shielding unit is disposed on a front side of the detector. Patterns of the passage allowable region and the passage blocking region of the at least one member and disposition of the at least one member are set to allow for reconstruction of an observation image based on an image detected in the detector.

A telescope system includes a telescope and a selective shielding unit including at least one member including a passage allowable region for an observation target electromagnetic wave and a passage blocking region for the observation target electromagnetic wave. The telescope includes a position detectable detector that detects the observation target electromagnetic wave on a surface different from a focal plane of the telescope. The selective shielding unit is disposed on a front side of the detector. Patterns of the passage allowable region and the passage blocking region of the at least one member and disposition of the at least one member are set to allow for reconstruction of an observation image based on an image detected in the detector.

A telescope system (100) comprises a steering minor (M5) arranged in a part of its optical path (L5-L6) between a first telescope stage (10) and a second telescope stage (20). The steering mirror (M5) is configured to controllably rotate over a rotation angle (θm) for controlling a view angle (θv) of the telescope system (100) from the entrance aperture (A1). The steering mirror (M5) is disposed at an intermediate pupil (Pi) of the telescope system (100), at which position an image of the aperture stop (As) is formed by one or more of the optical components (M7, M6) there between.

The disclosure is directed to a reticle for an optical sight of a projectile launching device including, but not limited to a firearm. The reticle provides one or more target acquisition features for a target object of a predetermined width and height including horizontal auto range estimation, vertical auto range estimation, bullet drop compensation, wind adjustment information, moving target lead information, target guidance information, and fire correction information. The reticle includes indicia graduated in angular measurement for horizontal ranging and vertical ranging target objects of known dimensions.

The disclosure is directed to a reticle for an optical sight of a projectile launching device including, but not limited to a firearm. The reticle provides one or more target acquisition features for a target object of a predetermined width and height including horizontal auto range estimation, vertical auto range estimation, bullet drop compensation, wind adjustment information, moving target lead information, target guidance information, and fire correction information. The reticle includes indicia graduated in angular measurement for horizontal ranging and vertical ranging target objects of known dimensions.

A relay optical system (RL) of this telescope has arranged therein, in the following order from the object side: a first lens group (G1) having positive refractive power; a second lens group (G2) having positive refractive power; a third lens group (G3) having positive refractive power; a fourth lens group (G4) having negative refractive power; and a fifth lens group (G5) having positive refractive power, wherein the magnification of the telescope can be changed by causing an image formed on a first image plane (IM1) to be re-formed on a second image plane (IM2) and further causing the second lens group (G2) and the third lens group (G3) to move along the optical axis, and thereby varying the image-forming magnification of the relay optical system (RL).