Abstract: A correct image reflecting monocular/telescope, with apparent straight through the device seeing, well suited for telescope, binocular, or goggle applications, including low profile single-wave and multi-wave night vision devices; comprised of at least one flat mirror, one of which having a central aperture, a concave primary mirror, and an image correcting system with offset angle viewing. The flat mirror with central aperture reflects the incoming light from the monocular aperture into other flat mirrors or directly into the concave primary mirror. The converging reflected light from the primary mirror passes back through the small central opening in the flat aperture mirror and into an image correcting system. The image correcting system upright corrects and deflects the focal image of the primary mirror by an offset angle behind the flat aperture mirror for observation with an eyepiece or other means, making it useful in both terrestrial as well as celestial applications.

Abstract: A correct image reflecting monocular/telescope, with apparent straight through the device seeing, well suited for telescope, binocular, or goggle applications, including low profile single-wave and multi-wave night vision devices; comprised of at least one flat mirror, one of which having a central aperture, a concave primary mirror, and an image correcting system with offset angle viewing. The flat mirror with central aperture reflects the incoming light from the monocular aperture into other flat mirrors or directly into the concave primary mirror. The converging reflected light from the primary mirror passes back through the small central opening in the flat aperture mirror and into an image correcting system. The image correcting system upright corrects and deflects the focal image of the primary mirror by an offset angle behind the flat aperture mirror for observation with an eyepiece or other means, making it useful in both terrestrial as well as celestial applications.

Abstract: A glove made from narrow strap material. Glove advantages when used with a striking tool: improved control, improved striking force, improved tool head acceleration, improved energy transfer, reduced hand fatigue, improved grip, and reduced vibration shock. It can be configured for 1, 2, 3 or 4 fingers plus the thumb. The glove forms a web between the thumb and fingers. The width of the web and the tightness of fit on the thumb and fingers is controlled by a single pull-tab type of adjustment. The adjustment is secured by a contact friction loop which increases in friction during impact force use. The glove can be worn on a bare hand or over the top of a more conventional type of glove while still providing the same advantages.

Abstract: A glove made from narrow strap material. Glove advantages when used with a striking tool: improved control, improved striking force, improved tool head acceleration, improved energy transfer, reduced hand fatigue, improved grip, and reduced vibration shock. It can be configured for 1, 2, 3 or 4 fingers plus the thumb. The glove forms a web between the thumb and fingers. The width of the web and the tightness of fit on the thumb and fingers is controlled by a single pull-tab type of adjustment. The adjustment is secured by a contact friction loop which increases in friction during impact force use. The glove can be worn on a bare hand or over the top of a more conventional type of glove while still providing the same advantages.

Abstract: A telescope mount with a fixed vertical axis of rotation, a fixed horizontal axis of rotation, and a variable axis of rotation. The mount allows a side aperture telescope to simultaneously rotate horizontally and vertically while also allowing the telescope to be tilted up and down.

Abstract: A glove made from a narrow strap of material, which at a minimum loops around the thumb and one finger. The glove forms a “web” between the thumb and the fingers. The web width can be fixed or adjustable and the strap-glove can be worn over a bare hand or over the top of a conventional glove.

Abstract: A correct image reflecting telescope with zoom capability comprised of a flat mirror, a parabolic primary mirror, and an image correcting system. The flat mirror reflects the incoming light from the telescope aperture into the parabolic primary mirror. The reflected light from the primary mirror passes back through a small centrally located opening in the flat aperture mirror and into an image correcting lens system. The image correcting system repositions the focal point of the primary mirror from a point in front of the flat aperture mirror to a point behind this mirror for observation with an eyepiece. The image correcting system makes the telescope useful in terrestrial as well as celestial applications and it can be moved with respect to the primary mirror such that a zoom feature results. This intrinsic zoom of the telescope allows an observer to use a single eyepiece in place of many, eliminates the need for an additional finder scope, and also makes the telescope useful in spotting scope applications.

Abstract: A correct image reflecting telescope with zoom capability comprised of a flat mirror, a parabolic primary mirror, and an image correcting system. The flat mirror reflects the incoming light from the telescope aperture into the parabolic primary mirror. The reflected light from the primary mirror passes back through a small centrally located opening in the flat aperture mirror and into an image correcting lens system. The image correcting system repositions the focal point of the primary mirror from a point in front of the flat aperture mirror to a point behind this mirror for observation with and eyepiece. The image correcting system makes the telescope useful in terrestrial as well as celestial applications and it can be moved with respect to the primary mirror such that a zoom feature results.